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107 results on '"Instituto de Física Teórica (IFT)"'

1. Memoria de Actividades 2017

Author: CSIC-UAM - Instituto de Física Teórica (IFT) and CSIC-UAM - Instituto de Física Teórica (IFT)
Published: 2018

2. Memoria de Actividades 2016

Author: CSIC-UAM - Instituto de Física Teórica (IFT) and CSIC-UAM - Instituto de Física Teórica (IFT)
Published: 2017

3. Weyl Invariance in the gravitational sector

Author: Herrero Valea, Mario, Instituto de Física Teórica (IFT), Álvarez Vázquez, Enrique, and UAM. Departamento de Física Teórica
Subjects: Gravedad - Tesis doctorales, Física
Abstract: Tesis doctoral inédita leída en la Universidad Autónoma de Madrid, Facultad de Ciencias, Departamento de Física Teórica. Fecha de lectura: 09-06-2015, It is been known since long ago that eld theories enjoying scale invariance have an improved behaviour in the Ultraviolet. Here we explore the consequences of this symmetry in the presence of dynamical gravitation, where it is described in terms ofWeyl invariance, local rescalings of the metric and the elds involved in the lagrangian. After thoroughly introducing some techniques of common use in the eld theory approach to Quantum Gravity, we address two main questions. First, we study the equivalence premise between the Einstein and Jordan frame in a theory we dub Conformal Dilaton Gravity, where we nd that equivalence is broken in the presence of a Weyl anomaly. Although a regularization that solves this issue exists, it is not clear that it can be implemented in a consistent framework. Later, we move our attention to Unimodular Gravity, where Weyl invariance appears as a way to relax the problem of the cosmological constant, which is here given in terms of an integration constant, its value determined solely by initial conditions. By constructing a gauge xing and ghost sector, we quantize the theory and we compute its one loop e ective action. Our results suggest that the protection of the cosmological constant is preserved by the quantization process provided no anomaly arises in the Weyl symmetry, Es sabido desde hace décadas que aquellas teorías de campos que poseen una invariancia de escala se comportan mejor en el ultravioleta. En este trabajo exploramos las consecuencias que implica esta simetría en presencia de gravedad dinámica, donde viene descrita en términos de invariancia de Weyl, rescaleos locales de la métrica y de los campos que aparecen en el lagrangiano. Tras describir extensivamente algunas técnicas de uso común en el tratamiento de Gravedad Cuántica como una teoría de campos, tratamos de responder dos cuestiones principales. Primero, estudiamos la supuesta equivalencia entre el referencial de Einstein y el de Jordan en una teoría que denominamos Gravedad Dilatónica Conforme, en la que descubrimos que la equivalencia está rota por la presencia de una anomalía Weyl. Pese a que existe una regularización que resuelve este problema, no está claro que pueda ser implementada en un marco teórico consistente. Más tarde, centramos nuestra atención en Gravedad Unimodular, donde la invariancia de Weyl se presenta como una forma de relajar el problema de la constante cosmológica, que pasa a estar definida en términos de una constante de integración cuyo valor está determinado por las condiciones iniciales del sistema. Gracias a la construcción de un sector de fantasmas adecuado, cuantizamos la teoría y calculamos las correcciones a un lazo a la acción efectiva. Nuestro resultado sugiere que la protección de la constante cosmológica se preserva en la presencia de correcciones cuánticas supuesto que no encontremos una anomalía Weyl
Published: 2016

4. Física Teórica: explorando los secretos del Universo

Author: CSIC-UAM - Instituto de Física Teórica (IFT)
Abstract: Fecha de consulta: 2016-05-04, El Instituto de Física Teórica (IFT) UAM-CSIC fue creado oficialmente en 2003 como un centro mixto perteneciente al Consejo Superior de Investigaciones Científicas(CSIC) y a la Universidad Autónoma de Madrid (UAM). Es el único centro Español dedicado íntegramente a la investigación en Física Teórica. En el IFT se trabaja en la frontera de la Física de Partículas Elementales, Astropartículas y Cosmología, con el objetivo de entender las claves fundamentales de la Naturaleza y del Universo. Sus investigadores lideran numerosos proyectos de investigación en el ámbito tanto nacional como internacional. El IFT forma parte de la línea estratégica `Física Teórica y Matemáticas´ del Campus de Excelencia Internacional (CEI) UAM+CSIC establecido en 2009. Desde 2012, está acreditado como Centro de Excelencia Severo Ochoa. Además de la actividad puramente científica, en el IFT se realiza una intensa tarea de formación de jóvenes investigadores y profesionales a través del programa de postgrado en Física Teórica con Mención de Excelencia del CEI y del Ministerio de Educación. También se lleva a cabo una importante labor de transferencia de conocimiento a la sociedad a través de diversos programas de divulgación.
Published: 2015

5. Memoria Severo Ochoa 2013-2015

Author: CSIC-UAM - Instituto de Física Teórica (IFT) and CSIC-UAM - Instituto de Física Teórica (IFT)
Published: 2016

6. Memoria de Actividades 2015

Author: CSIC-UAM - Instituto de Física Teórica (IFT) and CSIC-UAM - Instituto de Física Teórica (IFT)
Published: 2016

7. Memoria de Actividades 2013-2014

Author: CSIC-UAM - Instituto de Física Teórica (IFT) and CSIC-UAM - Instituto de Física Teórica (IFT)
Published: 2015

8. Memoria de Actividades 2011-2012

Author: CSIC-UAM - Instituto de Física Teórica (IFT) and CSIC-UAM - Instituto de Física Teórica (IFT)
Published: 2013

9. Memoria de Actividades 2006-2007

Author: CSIC-UAM - Instituto de Física Teórica (IFT) and CSIC-UAM - Instituto de Física Teórica (IFT)
Published: 2008

10. The hunt for dark matter in gamma-rays with fermi-lat and cta: modelling, predictions and analysis in a variety of astrophysical objects

Author: Pérez Romero, Judit, Sánchez Conde, Miguel Ángel, UAM. Departamento de Física Teórica, and Instituto de Física Teórica (IFT)
Subjects: Materia oscura (Astronomía), Física, Galaxias-Estructura, Rayos gamma-Análisis
Abstract: Tesis Doctoral inédita leída en la Universidad Autónoma de Madrid, Facultad de Ciencias, Departamento de Física Teórica. Fecha de Lectura: 25-11-2022, Gravitational evidences at diferent cosmological scales hint towards the existence of a dark component of the Universe, which amounts up to the 85% of its matter density. Despite all the eforts, the dark matter (DM) has eluded any clear detection and its ultimate nature remains still unknown. The current knowledge suggests that the DM cannot be identifed with the particles comprised in the Standard Model (SM). In this context, the Weakly Interacting Massive Particles (WIMPs) provide a framework that naturally yields the measured DM relic density, while at the same time they are expected to interact with SM particles. From these interactions, one of the most promising channels are γ-rays, which travel the Universe without defection, pointing back towards its original source. This Thesis has been devoted to unveil the unknown properties of the dark matter focusing on the so-called γ-ray indirect DM searches. We have conducted an exhaustive study of the DM contents and distribution in diferent interesting astrophysical objects and computed the state-of-the-art predictions for their annihilation and decay DM fuxes. Then, we have used these models to both, perform searches in existing F ermi-LAT data and obtain the prospects for the future Cherenkov Telescope Array (CTA). In the absence of detection, we proceed to a systematic search starting with galaxy clusters, known to be very good candidates to search DM emission. We compute the sensitivity to difuse γ-ray emission from Perseus, one of the most massive local galaxy clusters, of the future CTA, including in the analysis the CR-induced γ-rays as a background in a template ftting analysis. Staying with galaxy clusters, we then use 12 years of Fermi-LAT data from nearly 50 local galaxy clusters, searching for a DM-induced γ-ray signal, modelled including the expected substructures. We also explore introducing new targets in the quest of DM. For this, we perform the frst DM γ-ray search in dwarf irregular galaxies (dIrrs) using Fermi-LAT data. Finally, we collect the results of the previous studies to model the DM content of a subsample of objects that we have already investigated (dIrrs and clusters) and also of representative dark subhalos of the Milky Way
Published: 2022

11. Primordial black holes from inflation and their gravitational wave signals

Author: Rey Idler, Julián Leonardo, Ballesteros Martínez, Guillermo, UAM. Departamento de Física Teórica, and Instituto de Física Teórica (IFT)
Subjects: Ondas de gravedad, Gravitación, Física, Agujeros negros (Astronomía)
Abstract: Tesis Doctoral inédita leída en la Universidad Autónoma de Madrid, Facultad de Ciencias, Departamento de Física Teórica. Fecha de Lectura: 27-10-2022, We consider the possibility that the majority of dark matter in the Universe consists of black holes of primordial origin, and study the prospects of generating them in single-field models of inflation. Three different scenarios are presented. The first two rely on the presence of an ultra-slow-roll phase in inflation due to an inflection point in the potential. One of these scenarios is characterized by a quartic polynomial potential and is (arguably) the simplest model of inflation able to produce a large population of primordial black holes. The second scenario is aimed at ameliorating the tuning problems present in inflection-point models, and involves a setup that employs the advantages of gravitational collapse in a long epoch of early matter domination, as well as a potential based on a string-inspired class of models in which the inflaton is identified with a non-compact axion field. The third scenario we consider is fundamentally different from the inflection-point models, and consists on obtaining the large peak in the power spectrum of curvature perturbations necessary for black hole formation from a transient dissipative phase during inflation. In this case the enhancement of the power spectrum occurs due to the presence of a stochastic thermal noise source in the equation of motion for the fluctuations. We consider the impact of quantum diffusion on the inflationary dynamics during an ultra-slow-roll phase and show, by means of a fully analytical approach, that the power spectrum of comoving curvature perturbations computed in stochastic inflation matches precisely, at the linear level, the result obtained by solving the Mukhanov-Sasaki equation. Finally, we compute the stochastic background of gravitational waves generated in each scenario. In particular, we study the gravitational waves induced during an early matter-dominated era and determine how much of the parameter space remains available after taking into account the bounds on the gravitational wave energy density arising from the abundance of light elements produced during Big-Bang nucleosynthesis and cosmic microwave background experiments. We examine the gauge dependence of the resulting signal and, by using a heuristic argument based on symmetry properties and dimensional analysis, determine the full gaugeinvariant expression for the energy density of gravitational waves at next-to-leading order in perturbations. We discuss the prospects of detecting the resulting signal with the LISA experiment
Published: 2022

12. Holographic complexity and space time locality

Author: Sasieta Arana, Martín, Fernández Barbón, José Luís, UAM. Departamento de Física Teórica, and Instituto de Física Teórica (IFT)
Subjects: Agujeros negros (Astronomía), Ondas de gravedad, Física
Abstract: Tesis Doctoral inédita leída en la Universidad Autónoma de Madrid, Facultad de Ciencias, Departamento de Física Teórica. Fecha de Lectura: 15-09-2022
Published: 2022

13. Classical and Stringy Properties of Black Holes

Author: Pereñíguez Rodríguez, David, Ortín Miguel, Tomás, Cano Molina-Niñirola, Pablo Antonio, UAM. Departamento de Física Teórica, and Instituto de Física Teórica (IFT)
Subjects: Agujeros negros, Cuerdas, Teoría de las, Termodinámica, Física
Abstract: Tesis Doctoral inédita leída en la Universidad Autónoma de Madrid, Facultad de Ciencias, Departamento de Física Teórica. Fecha de Lectura: 14-09-2022, This thesis is devoted to the study of dynamical and thermodynamical properties of black holes. It has two parts. Part I considers black holes in the context of the low energy effective actions of string theory. The first few higher-derivative corrections induced by finite-size effects in √ the string length ` s ∼ α0 , where α0 is the Regge slope parameter, are well understood for the heterotic superstring (HST). α0-corrected black hole solutions are available and computing their entropy is crucial given its relation to string microstates. However, the Iyer–Wald entropy formula gives a result that is not gauge invariant. This is due to the fact that the original computation assumes that all fields are tensors with no internal gauge freedom. In this thesis, Wald’s derivation is revisited using a formalism that accommodates gauge symmetry conveniently. The main result is a gauge-and Lorentz-invariant entropy formula that includes the first order corrections in α0 . It is also shown, in some particular theories, how magnetic-type terms can be included in the generic proofs of the laws of black hole thermodynamics, even though magnetic charges are not directly associated to gauge symmetry. Part II focuses on dynamical aspects of black holes in different contexts. Rotating black holes in higher-derivative theories are poorly understood due to the complexity of the equations of motion. The problem can be simplified by considering the near horizon geometry of an extremal, charged and rotating black hole. A non-perturbative solution of such a class is presented in a cubic theory called Einsteinian Cubic Gravity. It is the first example in which the entropy of a rotating black hole of higher-order gravity has been exactly computed. In the context of the AdS/CFT correspondence, NUT-charged AdS black holes describe equilibrium states of neutral fluids subject to non-trivial flows at the boundary. Physical transport properties, however, remain largely unexplored. The master equations governing gravitational fluctuations on a class of NUT-charged AdS black holes are derived in this thesis. These exhibit an intriguing relation to Landau quantisation. The gravitational quasinormal mode spectrum of a NUT-charged black hole is computed for the first time, and the spacetime appears to be robustly stable despite the existence of closed causal curves (“time machines”). There is an interesting class of quasi-hydrodynamic modes for which analytic dispersion relations are constructed as a definite holographic prediction for the dual fluid. The last chapter of this thesis deals with the tidal deformability of black holes. Tidal interactions, encoded linearly in the so-called tidal Love numbers, become significant in the last stages of the inspiral phase of a merger. In the case of vacuum, four-dimensional black holes, the tidal Love numbers are zero. The robustness of such a property is investigated by studying the static deformability of charged black holes. It is shown that tidal response coefficients keep on vanishing, in a very non-trivial way, from neutrality all the way down to extremality. This is true not only for gravity (spin-2), but also for spin-0 and spin-1 deformations. In higher dimensions, however, the tidal response is non-trivial and charging up the hole can excite new polarisation modes. One exception is the static response of spin-0 perturbations, which happens to vanish at extremality in any dimension. These results call for further investigation of the tidal deformability properties of black holes
Published: 2022

14. Dark Matter's secret liaisons: phenomenology of a dark U(1) sector with bound states

Author: Taoso, Marco [Instituto de Física Teórica (IFT) UAM/CSIC, calle Nicolás Cabrera 13-15, 28049 Cantoblanco, Madrid (Spain)]
Published: 2017
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15. Measurements of differential cross-sections in four-lepton events in 13 TeV proton-proton collisions with the ATLAS detector

Author: Aad, Georges, Abbott, Braden Keim, Abraham, Nicola Louise, Araujo Ferraz, Victor, Grancagnolo, Sergio, Grandi, Mario, Grachev, Vadim, Gravila, Paul, Gravili, Francesco Giuseppe, Gray, Chloe, Gray, Heather, Grefe, Christian, Gregersen, Kristian Damlund, Gregor, Ingrid, Pereira, Rodrigo, Grenier, Philippe, Grevtsov, Kirill, Grieco, Chiara, Grieser, Nathan Allen, Grillo, Alex, Grillo, Alexander, Grimm, Kathryn, Grinstein, Sebastian, Grivaz, Jean-francois, Groh, Sabrina, Arcangeletti, Chiara, Gross, Eilam, Grosse-knetter, Joern, Grout, Zara Jane, Grud, Christopher Ryan, Grummer, Aidan, Grundy, James Cameron, Guan, Liang, Guan, Wen, Gubbels, Chris, Gubbels, Christopher, Arce, Ayana Tamu, Guenther, Jaroslav, Guerguichon, Antinea, Guerrero Rojas, J. G. R., Guescini, Francesco, Hance, Michael, Guest, Dan, Guest, Daniel, Gugel, Ralf, Guida, Alessandro, Guillemin, Thibault, Arguin, Jean-francois, Guindon, Stefan, Guo, Jun, Guo, Wen, Guo, Yicheng, Guo, Ziyu, Gupta, Ruchi, Gurbuz, Saime, Gustavino, Giuliano, Guth, Manuel, Gutierrez, Phillip, Argyropoulos, Spyros, Gutschow, Christian, Guyot, Claude, Gwenlan, Claire, Gwilliam, Carl, Haaland, Even Simonsen, Hawkes, Christopher, Haas, Andrew, Haas, Andy, Haber, Carl, Hadavand, Haleh, Argyropoulos, Spyridon, Hadef, Asma, Haleem, Mahsana, Haley, Joseph, Hall, Jack Joseph, Halladjian, Garabed, Hallewell, Gregory, Hamano, Kenji, Hamdaoui, Hassane, Hamer, Matthias, Hamity, Guillermo Nicolas, Arling, Jan-hendrik, Han, Kunlin, Han, Liangliang, Han, Liang, Han, Shuo, Han, Yi Fei, Hanagaki, Kazunori, Hance, Mike, Handl, David Michael, Hank, Michael Donald, Hankache, Robert, Armbruster, Aaron James, Hansen, Eva Brottmann, Hansen, Jorgen Beck, Hansen, Dines, Hansen, Maike Christina, Hansen, Peter, Hanson, Emily Claire, Hara, Kazuhiko, Harenberg, Torsten, Harkusha, Siarhei, Harrison, Paul Fraser, Armstrong, Alexander, Hartman, Nicole Michelle, Hartmann, Nikolai, Hasegawa, Yoji, Hasib, Ahmed, Hassani, Samira, Haug, Sigve, Hauser, Reiner, Havranek, Miroslav, Hawkes, Chris, Hawkings, Richard, Abramowicz, Halina, Arnaez, Olivier, Hayashida, Shota, Hayden, Daniel, Hayes, Christopher Robyn, Hayes, Robin, Hays, Chris, Hays, Jonathan, Hayward, Helen, Haywood, Stephen, He, Fudong, He, Yunjian, Arnold, Hannah, Heath, Matthew Peter, Hedberg, Vincent, Heggelund, Andreas Lokken, Hehir, Natasha, Heidegger, Constantin, Heidegger, Kim Katrin, Heidorn, William Dale, Heilman, Jesse Alan, Heim, Sarah, Heim, Timon, Arrubarrena Tame, Zulit Paola, Heinemann, Beate, Heinlein, James Geddy, Heinrich, Jochen Jens, Heinrich, Lukas Alexander, Hejbal, Jiri, Helary, Louis, Held, Alexander, Hellesund, Simen, Helling, Cole Michael, Hellman, Sten, Artoni, Giacomo, Helsens, Clement, Henderson, R. C. W., Henkelmann, Lars, Henriques Correia, Ana Maria, Herde, Hannah Elizabeth, Hernandez Jimenez, Yesenia, Herr, Holger Arnold, Herrmann, Maximilian Georg, Herrmann, Tim, Herten, Gregor, Asada, Haruka, Hertenberger, Ralf, Hervas, Luis, Hesketh, Gavin, Hessey, Nigel, Hibi, Hiroaki, Higashino, Satoshi, Higon-rodriguez, Emilio, Hildebrand, Kevin, Hill, John, Hill, Kurt Keys, Asai, Kanae, Hiller, Karl Heinz, Hiller, Karlheinz, Hillier, Stephen, Hils, Maximilian, Hinchliffe, Ian, Hinterkeuser, Florian, Hirose, Minoru, Hirose, Shigeki, Hirschbuehl, Dominic, Hiti, Bojan, Asai, Shoji, Hladik, Ondrej, Hobbs, John David, Hobincu, Radu, Tal Hod, Noam, Hodgkinson, Mark, Hoecker, Andreas, Hohn, David, Hohov, Dmytro, Holm, Tanja, Holmes, Tova, Asawatavonvanich, Thanawat, Holzbock, Michael, Hommels, L. B. A. H., Hong, Tae Min, Honig, Jan Cedric, Honle, Andreas, Hooberman, Benjamin Henry, Hopkins, Walter, Horii, Yasuyuki, Horn, Philipp, Horyn, Lesya Anna, Asbah, Nedaa Alexandra, Hou, Suen, Hoummada, Abdeslam, Howarth, James William, Hoya, Joaquin, Hrabovsky, Miroslav, Hrivnac, Julius, Hrynevich, Aliaksei, Hrynova, Tetiana, Hsu, Pai-hsien, Hsu, Shih-chieh, Asimakopoulou, Eleni Myrto, Hu, Qipeng, Hu, Shuyang, Hu, Yi Fan, Huang, Dan Ping, Hu, Yifan, Huang, Danping, Huang, Xiaozhong, Huang, Yicong, Huang, Yanping, Hubacek, Zdenek, Abreu, Henso, Asquith, Lily, Hubaut, Fabrice, Hubner, Michael, Huegging, Fabian, Huffman, Todd Brian, Huhtinen, Mika, Hulsken, Raphael, Hunter, Robert Francis, Huseynov, Nazim, Huston, Joey, Huth, John, Assahsah, Jihad, Hyneman, Rachel Jordan, Hyrych, Sofiia, Iacobucci, Giuseppe, Iakovidis, Georgios, Iakovidis, George, Ibragimov, Iskander, Iconomidou-fayard, Lydia, Iengo, Paolo, Ignazzi, Rosanna, Iguchi, Ryunosuke, Assamagan, Ketevi Adikle, Iizawa, Tomoya, Ikegami, Yoichi, Ikeno, Masahiro, Ilic, Nikolina, Iltzsche, Franziska, Imam, Hajar, Introzzi, Gianluca, Iodice, Mauro, Iordanidou, Kalliopi, Ippolito, Valerio, Astalos, Robert, Isacson, Max Fredrik, Ishino, Masaya, Islam, Wasikul, Issever, Cigdem, Istin, Serhat, Iturbe, Julia, Iuppa, Roberto, Ivina, Anna, Izen, Joseph Michael, Izzo, Vincenzo, Atkin, Ryan Justin, Jacka, Petr, Jackson, Paul, Jacobs, Ruth Magdalena, Jaeger, Benjamin Paul, Jain, Vivek, Jakel, Gunnar, Jakobi, Katharina Bianca, Jakobs, Karl, Jakoubek, Tomas, Jamieson, Jonathan, Atkinson, Markus Julian, Janas, Krzysztof, Jansky, Roland, Janus, Michel, Janus, Piotr Andrzej, Jarlskog, Goran, Jaspan, Adam Elliott, Javadov, Namig, Javurek, Tomas, Javurkova, Martina, Jeanneau, Fabien, Atlay, Naim Bora, Jeanty, Laura, Jejelava, Juansher, Jenni, Peter, Jeong, Namgyun, Jezequel, Stephane, Jia, Jiangyong, Jia, Zihang, Jiang, Hai, Jiang, Yi, Jiang, Zihao, Atmani, Hicham, Jiggins, Stephen, Jimenez Morales, Fabricio Andres, Jimenez Pena, Javier, Jin, Shan, Jinaru, Adam, Jinnouchi, Osamu, Jivan, Harshna, Johansson, Per Daniel Conny, Johns, Kenneth, Johnson, Christian, Atmasiddha, Prachi, Jones, Eleanor, Jones, R. W. L., Jones, Samuel David, Jones, T. J., Jovicevic, Jelena, Ju, Xiangyang, Junggeburth, Johannes Josef, Juste Rozas, Aurelio, Kaczmarska, Anna, Kado, Marumi, Augsten, Kamil, Kagan, Harris, Kagan, Michael Aaron, Kahn, Alan Mathew, Kahra, Christian, Kaji, Toshiaki, Kajomovitz Must, Enrique, Kalderon, Charles William, Kartvelishvili, Vakhtang, Kalderon, Will, Kaluza, Adam, Abulaiti, Yiming, Austrup, Volker Andreas, Kamenshchikov, Andrey, Kaneda, Michiru, Kang, Nathan Jihoon, Kang, Shuaiyan, Kano, Yuya, Kanzaki, Junichi, Kaplan, Laser Seymour, Kar, Deepak, Karava, Kla, Kareem, Mohammad, Avolio, Giuseppe, Karkanias, Ioannis, Karpov, Sergey, Karpova, Zoya, Kaya, Fikriye Idil, Kartvelishvili, Vato, Karyukhin, Andrei, Kasimi, Eirini, Kastanas, Alex, Kato, Chikuma, Katzy, Judith, Ayoub, Mohamad Kassem, Kawade, Kentaro, Kawagoe, Kiyotomo, Kawaguchi, Tomomi, Kawamoto, Tatsuo, Kawamura, Gen, Kay, Ellis, Kaya, Colette, Kazakos, Stergios, Kazanin, Vassili, Keaveney, James Michael, Azuelos, Georges, Keeler, Richard, Keller, John Stakely, Kellermann, Edgar, Kelsey, Daniel Christopher, Kempster, Jacob Julian, Kendrick, James Andrew, Kennedy, Kiley Elizabeth, Kepka, Oldrich, Kersten, Susanne, Kersevan, Borut Paul, Babal, Dominik, Ketabchi, Sana, Khalil-zada, Farhad, Khandoga, Mykola, Khanov, Alexander, Kharlamov, Alexey, Kharlamova, Tatyana, Khoda, Elham E, Khoo, Teng Jian, Khoriauli, Gia, Khramov, Evgeny, Bachacou, Henri, Khubua, Djemal, Kido, Shogo, Kiehn, Moritz, Kim, Eunchong, Kim, Young-kee, Kimura, Naoki, Kirchhoff, Andreas, Kirchmeier, David, Kirk, Julie, Kiryunin, Andrei, Bachas, Dinos, Kishimoto, Tomoe, Kisliuk, Dylan Perry, Kitali, Vincent, Kitsaki, Chara, Kivernyk, Oleh, Klapdor-kleingrothaus, Thorwald, Klassen, Martin, Klein, Christoph Thomas, Klein, Matthew Henry, Klein, Max, Bachas, Konstantinos, Klein, Uta, Kleinknecht, Konrad, Klimek, Pawel Jan, Klimentov, Alexei, Klimpel, Fabian, Klingl, Tobias, Klioutchnikova, Tatiana, Klitzner, Felix Fidelio, Kluit, Peter, Kluth, Stefan, Backman, Karl Filip, Kneringer, Emmerich, Knoops, Edith, Knue, Andrea Helen, Kobayashi, Dai, Kobel, Michael, Kocian, Martin, Kodama, Takafumi, Kodys, Peter, Kock, Daniela, Konig, Philipp, Bagnaia, Paolo, Koffas, Thomas, Koehler, Nicolas, Kolb, Mathis, Koletsou, Iro, Komarek, Tomas, Kondo, Takahiko, Kordas, Konstantinos, Kondo, Taka, Koeneke, Karsten, Kong, Albert, Acharya, Bobby Samir, Bahmani, Marzieh, Konig, Adriaan Clemens, Kono, Takanori, Konstantinides, Vasilis, Konstantinidis, Nikolaos, Konya, Balazs, Kopeliansky, Revital, Koperny, Stefan Zenon, Korcyl, Krzysztof Marian, Kordas, Kostas, Koren, Guy, Bahrasemani, Sina, Korn, Andreas, Korolkov, Ilya, Korolkova, Elena, Korotkova, Natalia, Kortner, Oliver, Kortner, Sandra, Kostyukhin, Vadim, Kotsokechagia, Anastasia, Kotwal, Ashutosh, Koulouris, Aimilianos, Bahrasemani, H., Kourkoumeli-charalampidi, Athina, Kourkoumelis, Christine, Kourlitis, Evangelos, Kouskoura, Vasiliki, Kowalewski, Robert Victor, Kowalewski, Bob, Kozanecki, Witold, Kozhin, Anatoli, Kramarenko, Viktor, Kramberger, Gregor, Bailey, Adam, Krasnopevtsev, Dimitrii, Krasny, Mieczyslaw, Krasznahorkay, Attila, Krauss, Dominik, Kremer, Jakub, Kretzschmar, Jan, Kreul, Ken Matthias, Krieger, Peter, Krieter, Ferdinand, Krishnamurthy, Samyukta, Bailey, Virginia, Krishnan, Anjali, Krivos, Martin, Krizka, Karol, Kroeninger, Kevin Alexander, Kroha, Hubert, Kroll, Jiri, Kroll, Joe, Kroll, Joseph Ira, Krowpman, Kyle Stuart, Kruchonak, Uladzimir, Baines, John, Krueger, Hans, Krumnack, Nils Erik, Kruse, Mark, Krzysiak, Janina Anna, Kubota, Arisa, Kuchinskaia, Olesia, Kuday, Sinan, Kuchler, Daniela, Kuechler, Jan, Kuehn, Susanne, Bakalis, Christos, Kuhl, Thorsten, Kukhtin, Victor, Kulchitsky, Yuri, Kuleshov, Sergey, Koultchitski, Yuri, Kuleshov, Serguei, Kulinich, Yakov Petrovich, Kuna, Marine, Kupco, Alexander, Kupfer, Tobias, Baker, Keith, Kuprash, Oleg, Kurashige, Hisaya, Kurchaninov, Leonid, Kurochkin, Yurii, Kurova, Anastasia, Kurth, Matthew Glenn, Kuwertz, Emma Sian, Kuze, Masahiro, Kvam, Audrey Katherine, Kvita, Jiri, Bakker, Pepijn Johannes, Kwan, Tony, Lacasta Llacer, Carlos, Lacava, Francesco, Lack, David Philip John, Lacker, Heiko Markus, Lacour, Didier, Ladygin, Evgueni, Lafaye, Remi, Laforge, Bertrand, Lagouri, Theodota, Bakos, Evelin, Lai, Stanley, Lai, Stan, Lakomiec, Inga Katarzyna, Lambert, Joseph Earl, Lammers, Sabine Wedam, Lampl, Walter, Lampoudis, Christos, Lancon, Eric Christian, Landgraf, Ulrich, Landon, Murrough, Achkar, Baida, Bakshi Gupta, Debottam, Lang, Valerie, Lange, Joern, Langenberg, Robert Johannes, Lankford, Andrew James, Lanni, Francesco, Lantzsch, Kerstin, Lanza, Agostino, Lapertosa, Alessandro, Laporte, Jean-francois, Lari, Tommaso, Balaji, Shyam, Lasagni Manghi, Federico, Lassnig, Mario, Latonova, Vera, Lau, Tak Shun, Laudrain, Antoine, Laurier, Alexandre, Lavorgna, Marco, Lawlor, Sean Dean, Lazzaroni, Massimo, Le, Brian, Balasubramanian, Rahul, Le Guirriec, Emmanuel, Lebedev, Alexandre, Leblanc, Matthew Edgar, LeCompte, Thomas, Leblanc, Matt, Le Compte, Tom, Ledroit, Fabienne, Lee, Ava Chloe Audrey, Lee, Claire, Lee, Graham Richard, Baldin, Evgenii, Lee Jr, Lawrence, Lee, Shih-chang, Lee, Songkyo, Lefebvre, Benoit, Lefebvre, Helena, Lefebvre, Michel, Leggett, Charles, Lehmann, Konstantin, Lehmann, Niklaus, Lehmann Miotto, Giovanna, Balek, Petr, Leight, William Axel, Leisos, Antonios, Lisboa Leite, Marco, Leitgeb, Clara Elisabeth, Leitner, Rupert, Leney, Katharine, Lenz, Tatjana, Leone, Sandra, Leonidopoulos, Christos, Leopold, Alexander, Balli, Fabrice, Leroy, Claude, Les, Robert, Lester, Christopher, Levchenko, Mikhail, Leveque, Jessica, Lloyd, Stephen, Levin, Dan, Levin, Daniel, Levinson, Lorne, Lewis, Daniel James, Balunas, William Keaton, Li, Boyang, Li, Bing, Li, Changqiao, Li, Fan, Li, Heng, Li, Haifeng, Li, Jing, Li, Ke, Li, Liang, Li, Mengran, Balz, Johannes, Li, Quanyin, Li, Shu, Li, Xingguo, Li, Yichen, Li, Zhi, Li, Zhiying, Li, Zhelun, Li, Zhiyuan, Liang, Zhijun, Liberatore, Marianna, Banas, Elzbieta, Liberti, Barbara, Lie, Ki, Lim, Sanghoon, Lin, Chiao-ying, Lin, Kuan-yu, Linck, Rebecca, Lindley, Rachel Elizabeth, Lindon, Jack, Linss, Arthur, Lionti, Anthony, Bandieramonte, Marilena, Lionti, A. L., Lipeles, Elliot, Lipniacka, Anna, Liss, Anthony Michael, Liss, Tony, Lister, Alison, Little, Jared, Liu, Bo, Liu, Bingxuan, Liu, Hongbin, Adam, Lennart, Bandyopadhyay, Anjishnu, Liu, Jianbei, Liu, Jesse, Liu, Kun, Liu, Minghui, Liu, Mingyi, Liu, Peilian, Liu, Xiaotian, Liu, Yi, Liu, Yang, Liu, Yanlin, Banerjee, Sw., Liu, Yanwen, Livan, Michele, Lleres, Annick, Llorente Merino, Javier, Lloyd, Steve, Lo, Cheuk Yee, Lobodzinska, Ewelina Maria, Loch, Peter, Loffredo, Salvatore, Lohse, Thomas, Banerjee, Swagato, Lohwasser, Kristin, Lokajicek, Milos, Long, Jonathan, Long, Robin Eamonn, Longarini, Iacopo, Longo, Luigi, Lopez Paz, Ivan, Lopez Solis, Alvaro, Lorenz, Jeanette Miriam, Lorenzo Martinez, Narei, Barak, Liron, Lory, Alexander, Loesle, Alena, Lou, Xuanhong, Lou, Xinchou, Lounis, Abdenour, Love, Jeremy Robert, Love, Peter, Lozano Bahilo, Julio, Lu, Miaoran, Lu, Yun-ju, Barbe, William Mickael, Lubatti, Henry, Luci, Claudio, Lucio Alves, Fabio Lucio, Lucotte, Arnaud, Luehring, Fred, Luise, Ilaria, Luminari, Lamberto, Lund-jensen, Bengt, Luongo, Nicholas, Lutz, Margaret Susan, Barberio, Elisabetta, Lynn, David, Lyons, Harry John, Lysak, Roman, Lytken, Else, Lyu, Feng, Lyubushkin, Vladimir, Lyubushkina, Tatiana, Ma, Hong, Ma, Lianliang, Ma, Yanhui, Barberis, Dario, Macdonell, Danika Marina, Maccarrone, Giovanni, Macdonald, Calum Michael, Macdonald, Jack, Machado Miguens, Joana, Madar, Romain, Mader, Wolfgang, Madugoda Ralalage Don, Madhuranga, Madysa, Nico, Maeda, Junpei, Barbero, Marlon Benoit, Maeno, Tadashi, Maerker, Max, Magerl, Veronika, Magini, Nicolo, Magro, Jacopo, Mahon, Devin, Maidantchik, Carmen, Maio, Amelia, Maj, Klaudia, Majersky, Oliver, Barbour, Gregory, Majewski, Stephanie, Makida, Yasuhiro, Makovec, Nikola, Malaescu, Bogdan, Malecki, Pawel, Malecki, Pa., Maleev, Victor, Malek, Fairouz, Malito, Davide, Mallik, Usha, Barillari, Teresa, Malone, Claire, Maltezos, Stavros, Malyukov, Sergey, Mamuzic, Judita, Mancini, Giada, Mandalia, Jesal, Mandic, Igor, Manhaes De Andrade Filho, Luciano, Maniatis, Ioannis Michail, Manjarres, Joany, Adam Bourdarios, Claire, Barisits, Martin, Mankinen, Katja Hannele, Mann, Alexander, Manousos, Athanasios, Manousos, Thanos, Mansoulie, Bruno, Manthos, Ioannis, Manzoni, Stefano, Marantis, Alexandros, Marceca, Gino, Marchese, Luigi, Barkeloo, Jason Tyler Colt, Marchiori, Giovanni, Marcisovsky, Michal, Marcoccia, Lorenzo, Marcon, Caterina, Marjanovic, Marija, Marshall, Zach, Martensson, Mikael, Marti I Garcia, Salvador, Martin, Christopher Blake, Martin, T. A., Barklow, Tim, Martin, Victoria, Martin Dit Latour, Bertrand, Martinelli, Luca, Martinez-perez, Mario, Martinez Agullo, Pablo, Martinez Outschoorn, Verena Ingrid, Martin-haugh, Stewart, Martoiu, Sorin, Martyniuk, Alex Christopher, Marzin, Antoine, Barklow, Timothy, Maschek, Stefan Raimund, Masetti, Lucia, Mashimo, Tetsuro, Mashinistov, Ruslan, Masik, Jiri, Maslennikov, Alexei, Massa, Lorenzo, Massarotti, Paolo, Mastrandrea, Paolo, Mastroberardino, Anna, Barnea, Rotem, Masubuchi, Tatsuya, Matakias, Dimitrios, Matic, Andrea, Matsuzawa, Nobuo, Mattig, Peter, Maurer, Julien, Macek, Bostjan, Maximov, Dmitriy, Mazini, Rachid, Maznas, Ioannis, Barnett, Bruce M, Mazza, Simone Michele, Mc Gowan, John Patrick, Mc Kee, Shawn, Mccarthy, Thomas, Mccormack, William Patrick, McDonald, Emily, Mcfayden, Joshua Angus, McKay, Madalyn Ann, McMahon, Steve, McPherson, Robert, Barnett, Michael, Mcdonald, Millie, Mcdougall, Ashley Ellen, Mcfayden, Josh, Mchedlidze, Gvantsa, Mikenberg, Giora, Mc Kay, Maddie, Mclean, Kayla, Mcmahon, Stephen, Mcnamara, Peter Charles, Mcnicol, Christopher John, Barnovska-Blenessy, Z., Milke, Christopher Don, Mcpherson, Rob, Mdhluli, Joyful Elma, Meadows, Zachary Alden, Meehan, Samuel Ross, Megy, Theo, Mehlhase, Sascha, Mehta, Andrew, Meirose, Bernhard, Melini, Davide, Baroncelli, Toni, Mellado Garcia, Bruce, Mellenthin, Johannes, Melo, Matej, Meloni, Federico, Melzer, Alexander, Gouveia, Emanuel, Mendes Jacques Da Costa, Antonio Manuel, Meng, Huan Yu, Meng, Lingxin, Meng, Xiangting, Baroncelli, Antonio, Menke, Sven, Meoni, Evelin, Mergelmeyer, Sebastian, Merkt, Sebastian Andreas, Merlassino, Claudia, Mermod, Philippe, Merola, Leonardo, Meroni, Chiara, Merz, Garrett William, Meshkov, Oleg, Adamczyk, Leszek, Barone, Gaetano, Meshreki, John Kamal Rizk, Metcalfe, Jessica, Mete, Alaettin Serhan, Meyer, Christopher John, Meyer, Jean-pierre, Michetti, Michele, Middleton, Robin, Mijovic, Liza, Mikenberg, George, Mikestikova, Marcela, Barr, Alan, Mikuz, Marko, Mildner, Hannes, Milic, Adriana, Milke, Chris, Miller, David, Miller, Laura Stephanie, Milov, Alexander, Milstead, David Anthony, Minaenko, Andrei, Minashvili, Irakli, Barranco Navarro, Laura, Mince, Laurynas, Mincer, Allen Irving, Mindur, Bartosz, Mineev, Mikhail, Minegishi, Yuji, Mino, Yuya, Mir Martinez, Lluisa Maria, Mironova, Maria, Mitani, Takashi, Mitrevski, Jovan, Barreiro Alonso, Fernando, Mitsou, Vasiliki, Mittal, Monika, Miu, Ovidiu, Miucci, Antonio, Miyagawa, Paul, Mizukami, Atsushi, Mjoernmark, Jan-ulf, Mkrtchyan, Tigran, Mlynarikova, Michaela, Moa, Torbjorn, Barreiro Guimaraes Da Costa, Joao, Mobius, Silke, Mochizuki, Kazuya, Moder, Paul, Mogg, Philipp, Mohapatra, Soumya, Moles Valls, Regina, Monig, Klaus, Monnier, Emmanuel, Montalbano, Alyssa Rae, Montejo Berlingen, Javier, Barron, Uriel, Montella, Marco, Monticelli, Fernando, Monzani, Simone, Morange, Nicolas, Moreira De Carvalho, Ana Luisa, Moreno Lopez, Deywis, Moreno Llacer, Maria, Moreno Martinez, Carlos, Morettini, Paolo, Morgenstern, Marcus Matthias, Barsov, Sergey, Morgenstern, Stefanie, Mori, Daniel, Morii, Masahiro, Morinaga, Masahiro, Morisbak, Vanja, Morley, Anthony, Mornacchi, Giuseppe, Morris, Alice, Morvaj, Ljiljana, Moschovakos, Paraschos, Bartels, Falk, Moss, Josh, Murray, W. J., Nachman, Benjamin Philip, Moschovakos, Paris, Moser, Brian, Mosidze, Maia, Moskalets, Tetiana, Moskvitina, Polina, Moss, Joshua, Moyse, E. J. W., Bartoldus, Rainer, Muanza, Steve, Mueller, James Alfred, Muller, Ralph, Muenstermann, Daniel, Mullier, Geoffrey, Mungo, Davide Pietro, Munoz Martinez, Jose Luis, Munoz Sanchez, Francisca, Murin, Pavel, Murray, Bill, Bartolini, Giovanni, Murrone, Alessia, Muse, Joseph M, Muskinja, Miha, Mwewa, Chilufya, Myagkov, Alexei, Myers, Ava Anne, Myers, Greg, Myers, John, Myska, Miroslav, Naryshkin, Iouri, Adamek, Lukas, Barton, Adam Edward, Neep, Thomas James, Nachman, Ben, Nackenhorst, Olaf, Nag, Abhishek, Nagai, Koichi, Nagano, Kunihiro, Nagasaka, Yasushi, Nagle, James Lawrence, Nagy, Elemer, Nairz, Armin, Bartos, Pavol, Higuchi, Yu Nakahama, Nakamura, Koji, Nakamura, Tomoaki, Nanjo, Hajime, Napolitano, Fabrizio, Naranjo, Roger, Narayan, Rohin Thampilali, Ng, Yan Wing, Naryshkin, Iurii, Naseri, Mohsen, Basalaev, Artem, Naumann, Thomas, Navarro, Gabriela Alejandra, Nechaeva, Polina, Nechansky, Filip, Neep, Tom, Negri, Andrea, Negrini, Matteo, Nellist, Clara, Nelson, Christina, Nelson, Michael Edward, Basan, Alexander, Nemecek, Stanislav, Nessi, Marzio, Neubauer, Mark, Neuhaus, Friedemann, Neumann, Manuel, Newhouse, Robin, Newman, Paul Richard, Ng, Chi Wing, Ng, Sam Yanwing, Ng, Ying Wun Yvonne, Bassalat, Ahmed, Ngair, Badr-eddine, Nguyen, Hoang Dai Nghia, Nguyen Manh, Tuan, Nibigira, Emery, Nickerson, Richard, Nikolaidou, Rosy, Nielsen, Daniel, Nielsen, Jason, Niemeyer, Marcel, Nikiforou, Nikiforos, Basso, Matthew Joseph, Nikolaenko, Vladimir, Nikolic, Irena, Nikolopoulos, Konstantinos, Nilsson, Paul, Nindhito, Herjuno Rah, Nisati, Aleandro, Nishu, Nishu, Nisius, Richard, Nitsche, Isabel, Nitta, Tatsumi, Bates, Richard, Nobe, Takuya, Noel, Daniel Louis, Noguchi, Yohei, Nomidis, Ioannis, Nomura, Marcelo Ayumu, Nordberg, Markus, Novak, Jakob, Novak, Tadej, Novgorodova, Olga, Novotny, Radek, Batlamous, Souad, Nozka, Libor, Ntekas, Konstantinos, Ntekas, Kostas, Nurse, Emily Laura, Oakham, Gerald, Ocariz, Jose Humberto, Ochi, Atsuhiko, Ochoa, Ines, Ochoa, Jean-pierre, O'connor, Kelsey Shea, Batley, Richard, Oda, Susumu, Odaka, Shigeru, Ordek, Serhat, Ogrodnik, Agnieszka Ewa, Oh, Alexander, Ohm, Christian, Oide, Hideyuki, Oishi, Reiyo, Ojeda, Martina Laura, Okawa, Hideki, Batool, Binish, Okazaki, Yuta, O'keefe, Michael William, Okumura, Yasuyuki, Olariu, Albert, Seabra, Luis, Olivares, Sebastian, Oliveira Damazio, Denis, Oliver, Jason, Olsson, Mats Joakim Robert, Olszewski, Andrzej, Abbott, Brad, Adelman, Jahred, Battaglia, Marco, Olszowska, Jolanta, Oncel, Omer Ogul, O'neil, Dugan, O'neill, Aaron Paul, Onofre, Antonio, Onyisi, P. U. E., Oppen, Henrik, Oreamuno Madriz, Rafael Guillermo, Oreglia, Mark, Orellana, Gonzalo Enrique, Bauce, Matteo, Orestano, Domizia, Orlando, Nicola, Orr, Robert, O'shea, Val, Ospanov, Rustem, Otero Y Garzon, Gustavo, Otono, Hidetoshi, Ott, Philipp Sebastian, Ottino, Gregory James, Ouchrif, Mohamed, Bauer, Florian, Ouellette, Jeff, Ould-saada, Farid, Ouraou, Ahmimed, Ouyang, Qun, Owen, Mark Andrew, Owen, Rhys, Ozcan, Erkcan, Ozturk, Nurcan, Pacalt, Josef, Pacey, Holly, Bauer, Patrick, Pachal, Katherine, Pacheco Pages, Andreu, Padilla Aranda, Cristobal, Pagan Griso, Simone, Palacino, Gabriel, Palazzo, Serena, Palestini, Sandro, Palka, Marek, Palni, Prabhakar, Pandini, Carlo Enrico, Bawa, Harinder Singh, Panduro Vazquez, Jose Guillermo, Panduro Vazquez, William, Pani, Priscilla, Panizzo, Giancarlo, Paolozzi, Lorenzo, Papadatos, Constantine, Papageorgiou, Konstantinos, Parajuli, Santosh, Paramonov, Alexander, Paraskevopoulos, Christos, Bayirli, Arif, Paredes Hernandez, Daniela Katherinne, Paredes Saenz, Santiago Rafael, Parida, Bibhuti, Park, Tae Hyoun, Parker, Adam Jackson, Parker, Andy, Parodi, Fabrizio, Parrish, Elliot, Parsons, John, Parzefall, Ulrich, Beacham, James, Pascual Dominguez, Luis, Pascuzzi, Vincent, Pasner, Jacob Martin, Pasquali, Federica, Pasqualucci, Enrico, Passaggio, Stefano, Pastore, Francesca, Pasuwan, Patrawan, Pataraia, Sophio, Pater, Joleen, Beau, Tristan, Pilcher, James, Pollard, Christopher Samuel, Pater, Jo, Pathak, Atanu, Patton, Joseph, Pauly, Thilo, Pearkes, Jannicke Andree, Pedersen, Maiken, Pedraza Diaz, Lucia, Costa Batalha Pedro, Rute, Beauchemin, Pierre-hugues, Peiffer, Thomas, Peleganchuk, Sergey, Penc, Ondrej, Peng, Chen, Peng, Haiping, Sotto-maior Peralva, Bernardo, Perego, Marta Maria, Peixoto, Ana, Pereira Sanchez, Laura, Perepelitsa, Dennis, Becherer, Fabian, Perez Codina, Estel, Perini, Laura, Pernegger, Heinz, Perrella, Sabrina, Perrevoort, Ann-kathrin, Peters, Krisztian, Peters, Reinhild, Petersen, Brian, Petersen, Troels, Petit, Elisabeth, Adiguzel, Aytul, Bechtle, Philip, Petousis, Vlasios, Petridou, Chariclia, Petrucci, Fabrizio, Pettee, Mariel, Pettersson, Nora Emilia, Potter, Christina, Poveda, Joaquin, Qin, Yang, Mihule, Kristina, Petukhova, Krystsina, Beck, Helge Christoph, Peyaud, Alan, Pezoa Rivera, Raquel, Pezzotti, Lorenzo, Raine, John Andrew, Pham, Joni, Pham, Thu, Phillips, Peter, Phipps, Michael William, Piacquadio, Giacinto, Pianori, Elisabetta, Beck, Hans Peter, Picazio, Attilio, Pickles, Rebecca Hayley, Piegaia, Ricardo, Pietreanu, Dorel, Rajagopalan, Srinivasan, Pilcher, Jim, Pilkington, Andrew, Pinamonti, Michele, Pinfold, James, Pitman Donaldson, Charlie Bruno, Becker, Kathrin, Pitt, Michael, Pizzimento, Luca, Pizzini, Alessio, Pleier, Marc-andre, Plesanovs, Vladislavs, Pleskot, Vojtech, Plotnikova, Elena, Podberezko, Pavel, Pottgen, Ruth, Poggi, Riccardo, Becot, Cyril Pascal, Poggioli, Luc, Pogrebnyak, Ivan, Pohl, David-leon, Pokharel, Ishan, Polesello, Giacomo, Poley, Anne-luise, Policicchio, Antonio, Polifka, Richard, Polini, Alessandro, Pollard, Chris, Beddall, Ayda, Polychronakos, Venetios, Ponomarenko, Daniil, Pontecorvo, Ludovico, Popa, Stefan, Popeneciu, Gabriel, Portales, Louis, Portillo Quintero, Dilia Maria, Pospisil, Stanislav, Potamianos, Karolos, Potrap, Igor, Beddall, Andrew, Potter, Tina, Potti, Harish, Poulsen, Trine, Poveda Torres, Ximo, Powell, Thomas Dennis, Pownall, Gavin, Pozo Astigarraga, Eukeni, Prades Ibanez, Alberto, Pralavorio, Pascal, Prapa, Maria Myrto, Bednyakov, Vadim, Prell, Soeren Andre, Price, Darren, Primavera, Margherita, Proffitt, Mason, Proklova, Nadezda, Prokofiev, Kirill, Prokoshin, Fedor, Protopopescu, Serbanp, Proudfoot, James, Przybycien, Mariusz, Bedognetti, Matteo, Pudzha, Dennis, Puri, Akshat, Puzo, Patrick Michel, Pyatiizbyantseva, Diana, Qian, Jianming, Qin, Quake, Quadt, Arnulf, Queitsch-maitland, Michaela, Rabanal Bolanos, Gabriel, Racko, Michal, Bee, Chris, Ragusa, Francesco, Rahal, Ghita, Raine, Johnny, Rajagopalan, Srini, Ramirez Morales, Andres, Ran, Kunlin, Rassloff, Damir Fabrice, Rauch, Daniel, Rauscher, Felix, Rave, Stefan, Adorni Braccesi Chiassi, Sofia, Bee, Christopher, Ravina, Baptiste, Ravinovich, Ilia, Rawling, Jacob Henry, Raymond, Michel, Read, Alexander Lincoln, Readioff, Nathan Peter, Reale, Marilea, Rebuzzi, Daniela, Redlinger, George, Reeves, Kendall, Beermann, Thomas, Reikher, David, Reiss, Andreas Dominik, Rej, Amartya, Rembser, Christoph, Renardi, Alessia, Renda, Michele, Rendel, Marian Benedikt, Rennie, Adam, Resconi, Silvia, Resseguie, Elodie Deborah, Begalli, Marcia, Rettie, Sebastien, Reynolds, Bryan, Reynolds, Elliot, Rezanova, Olga, Reznicek, Pavel, Ricci, Ester, Richter, Robert, Richter, Stefan, Richter-was, Elzbieta, Ridel, Melissa, Begel, Michael, Rieck, Patrick, Rifki, Othmane, Rijssenbeek, Michael, Rimoldi, Adele, Rimoldi, Marco, Rinaldi, Lorenzo, Rinn, Timothy Thomas, Ripellino, Giulia, Riu, Imma, Rivadeneira Bracho, Pablo Andres, Behera, Arabinda, Rivera Vergara, Juan Cristobal, Rizatdinova, Flera, Rizvi, Eram Syed, Rizzi, Chiara, Robertson, Steven, Robin, Matthieu, Robinson, Dave, Robles Gajardo, Carolina Michel, Robles Manzano, Maria, Robson, Aidan, Behr, Janna Katharina, Rocchi, Alessandro, Roda, Chiara, Rodriguez Bosca, Sergi, Rodriguez Rodriguez, Arturo, Rodriguez Vera, Ana Maria, Roe, Shaun, Roggel, Jens, Rohne, Ole, Rohrig, Rainer, Rojas Caballero, Rimsky Alejandro, Beisiegel, Florian, Roland, Benoit, Roland, Christophe Pol A, Roloff, Jennifer Kathryn, Romaniouk, Anatoli, Romano, Marino, Rompotis, Nikolaos, Ronzani, Manfredi, Roos, Lydia, Rosati, Stefano, Rosin, Guy, Belfkir, Mohamed, Rosser, Benjamin John, Rossi, Edoardo, Rossi, Eleonora, Rossi, Elvira, Rossi, Leonardo, Rossini, Lorenzo, Rosten, Rachel Christine, Rotaru, Marina, Rottler, Benjamin, Rousseau, David, Bell, Andrew Stuart, Rovelli, Giulia, Roy, Avik, Roy, Debarati, Rozanov, Alexandre, Rozen, Yoram, Ruan, Xifeng, Rühr, F., Ruiz-Martinez, Aranzazu, Salnikov, Andrei, Sampsonidis, Dimitrios, Bella, Gideon, Ruan, Ruanxf, Ruggeri, Tristan Andrew, Ruehr, Frederik, Ruiz Martinez, Arantxa, Rummler, Andre, Rurikova, Zuzana, Rusakovich, Nikolai, Russell, Heather, Rustige, Lennart, Rutherfoord, John P, Adye, Tim, Bellagamba, Lorenzo, Ruttinger, Elias, Rybar, Martin, Rybkin, Grigori, Rye, Eli Baverfjord, Ryzhov, Andrey, Sabater Iglesias, Jorge Andres, Sabatini, Paolo, Sabetta, Luigi, Sacerdoti, Sabrina, Sadrozinski, Hartmut, Bellerive, Alain, Sadykov, Renat, Safai Tehrani, Francesco, Safarzadeh Samani, Batool, Safdari, Murtaza, Saha, Puja, Saha, Shreya, Sahinsoy, Merve, Sahu, Arunika, Saimpert, Matthias, Saito, Masahiko, Bellos, Panagiotis, Saito, Tomoyuki, Sakamoto, Hiroshi, Salamani, Dalila, Salamanna, Giuseppe, Schaffer, Arthur, Schune, Ph., Salnikov, Andy, Salt, Jose, Salvador Salas, Adrian, Salvatore, Daniela, Beloborodov, Konstantin, Salvatore, Fabrizio, Salvucci, Antonio, Salzburger, Andreas, Samarati, Jerome, Sammel, Dirk, Sampsonidis, Dimos, Sampsonidou, Despoina, Sanchez Martinez, Francisco Javier, Sanchez Pineda, Arturos, Sandaker, Heidi, Belotskiy, Konstantin, Sander, Christian, Sanderswood, Izaac, Sandhoff, Marisa, Sandoval Usme, Carlos, Sankey, D. P. C., Sannino, Mario, Sano, Yuta, Sansoni, Andrea, Santoni, Claudio, Santos, Helena, Belyaev, Nikita, Santpur, Sai Neha, Santra, Arka, Saoucha, Kamal, Sapronov, Andrey, Mendes Saraiva, Joao Gentil, Sasaki, Osamu, Sato, Koji, Sauerburger, Frank, Sauvan, Emmanuel, Savard, Pierre, Benchekroun, Driss, Sawada, Ryu, Sawyer, Craig Anthony, Sawyer, Lee, Sayago Galvan, Ivan, Sbarra, Carla, Sbrizzi, Antonio, Scanlon, Timothy Paul, Schaarschmidt, Jana, Schacht, Peter, Schaefer, Douglas Michael, Benekos, Nectarios, Schaefer, Leigh Catherine, Schaefer, Uli, Schegelsky, Valery, Schwemling, Ph., Schaffer, R. D., Schaile, Dorothee, Schamberger Jr, Robert Dean, Schanet, Eric, Scharf, Christian, Scharmberg, Nicolas, Benhammou, Yan, Chtcheguelski, Valery, Scheirich, Daniel, Schenck, Ferdinand, Schernau, Michael, Schiavi, Carlo, Schildgen, Lara Katharina, Schillaci, Zachary Michael, Schioppa, Enrico Junior, Schioppa, Marco, Schleicher, Katharina, Benjamin, Doug, Schlenker, Stefan, Schmidt-sommerfeld, Korbinian Ralf, Schmieden, Kristof, Schmitt, Christian, Schmitt, Stefan, Schoeffel, Laurent Olivier, Schoening, Andre, Scholer, Patrick, Schopf, Elisabeth, Schott, Matthias, Affolder, A. A., Benjamin, Douglas, Schouwenberg, J. F. P., Schovancova, Jaroslava, Schramm, Steven, Schroeder, Frederic, Schulte, Alexandra, Schultz-coulon, Hans-christian, Schumacher, Markus, Schumm, Bruce Andrew, Schune, Philippe, Schwartzman, Ariel Gustavo, Benoit, Mathieu, Schwarz, Thomas Andrew, Schwemling, Philippe, Schwienhorst, Reinhard, Sciandra, Andrea, Sciolla, Gabriella, Scuri, Fabrizio, Scutti, Federico, Scyboz, Ludovic Michel, Sebastiani, Cristiano, Sedlaczek, Kevin, Bensinger, Jim, Seema, Pienpen, Seidel, Sally, Seiden, Abraham, Seidlitz, Blair Daniel, Seiss, Todd Michael, Seitz, Claudia, Seixas, Jose, Sekhniaidze, Givi, Sekula, Stephen Jacob, Semprini Cesari, Nicola, Bensinger, James, Sen, Sourav, Serfon, Cedric, Serin, Laurent, Serkin, Leonid, Sessa, Marco, Severini, Horst, Sevova, Stanislava, Sforza, Federico, Sfyrla, Anna, Shabalina, Elizaveta, Bentvelsen, Stan, Shahinian, Jeffrey David, Shaikh, Nabila Wahab, Shatalov, Pavel, Shojaii, Jafar, Shahinian, Jeff, Ahlgren, Nabila Wahab, Shaked Renous, Dan, Shan, Lianyou, Shapiro, Marjorie, Sharma, Abhishek, Beresford, Lydia Audrey, Shatalov, Sppavel, Shaw, Kate, Shaw, Savanna, Shehade, Mahran, Shen, Yu-ting, Sherman, Alexander David, Sherwood, Peter, Shi, Liaoshan, Shimmin, Chase Owen, Beretta, Matteo Mario, Shimogama, Yoshihiro, Shimojima, Makoto, Shinner, James David, Shipsey, Ian, Shirabe, Shohei, Shiyakova, Mariya, Shlomi, Jonathan, Shmeleva, Alevtina, Shochet, M. J., Sijacki, Djordje, Berge, David, Sijacki, Dj., Shojaii, Seyed Ruhollah, Shope, David Richard, Shrestha, Suyog, Shrif, Esra Mohammed, Shroff, Maheyer Jamshed, Shulga, Evgeny, Sicho, Petr, Sickles, Anne Marie, Sideras Haddad, Elias, Bergeaas Kuutmann, Elin, Sidiropoulou, Ourania, Sidoti, Antonio, Siegert, Frank, Solodkov, Alexander, Sijacki, Dorde, Silva, Manuel, Silva Oliveira, Marcos Vinicius, Silverstein, Samuel, Simion, Stefan, Simoniello, Rosa, Berger, Nicolas, Simpson-allsop, Cameron James, Simsek, Sinem, Sinervo, Pekka, Sinetckii, Viktor, Singh, Sundeep, Sinha, Sukanya, Sioli, Maximiliano, Siral, Ismet, Sivoklokov, Serguei, Sjoelin, Joergen, Affolder, Tony, Bergmann, Benedikt Ludwig, Skaf, Ali, Skorda, Eleni, Skubic, Patrick, Slawinska, Magdalena, Sliwa, Krzysztof Jan, Smakhtin, Vladimir, Smart, Ben Harry, Smiesko, Juraj, Smirnov, Nikita, Smirnov, Serge, Bergsten, Laura Jean, Smirnov, Yury, Smirnova, Lidia, Smirnova, Oxana, Smith, Emily Ann, Smith, Hayden Alexander, Smizanska, Maria, Smolek, Karel, Smykiewicz, Andrzej, Snesarev, Andrei, Snoek, Hella, Beringer, Juerg, Snyder, Ian Michael, Snyder, Scott, Sobie, Randall, Soffer, Abner, Soloshenko, Alexei, Soukharev, Andrey, Strauss, Michael, Sobie, Randy, Soffer, Abi, Sogaard, Andreas, Berlendis, Simon, Sohns, Fabian, Solans Sanchez, Carlos, Soldatov, Evgeny, Soldevila Serrano, Urmila, Sopio, Alexander Linus, Solodkov, Sanya, Soloshenko, Aleksey, Solovyanov, Oleg, Solovyev, Victor, Sommer, Philip, Bernardi, Gregorio, Son, Hyungsuk, Sonay, Anil, Song, Weimin, Song, Wen Yi, Sopczak, Andre, Sopio, Alex, Sopkova, Filomena, Sottocornola, Simone, Soualah, Rachik, Sukharev, Andrei, Bernius, Catrin, South, David, Spagnolo, Stefania, Spalla, Margherita, Spangenberg, Martin, Spano, Francesco, Sperlich, Dennis, Spieker, Thomas Malte, Spigo, Giancarlo, Spina, Mario, Spiteri, Dwayne Patrick, Bernlochner, Florian Urs, Spousta, Martin, Stabile, Alberto, Stamas, Brianna, Stamen, Rainer, Stamenkovic, Marko, Stampekis, Alexios, Stanecka, Ewa, Stanislaus, Beojan, Stanitzki, Marcel, Stankaityte, Migle, Berry, Tracey, Stapf, Birgit Sylvia, Starchenko, Evgeny, Stavropoulos, Georgios, Starchenko, Jenya, Stark, Giordon Holtsberg, Stark, Jan, Staroba, Pavel, Starovoitov, Pavel, Staerz, Steffen, Staszewski, Rafal, Berta, Peter, Tikhonov, Yury, Tikhonov, Yu. A., Stavropoulos, George, Stegler, Martin, Steinberg, Peter Alan, Steinhebel, Amanda, Stelzer, Bernd, Stelzer, Joerg, Stelzer-chilton, Oliver, Stenzel, Hasko, Berthold, Anne-sophie, Stevenson, Thomas James, Stewart, Graeme A, Stockton, Mark, Stoicea, Gabriel, Stolarski, Marcin, Stonjek, Stefan, Straessner, Arno, Strandberg, Jonas, Strandberg, Sara, Strauss, Mike, Afik, Yoav, Bertram, Iain, Strebler, Thomas, Strizenec, Pavol, Strohmer, Raimund, Strom, David, Stroynowski, Ryszard, Strubig, Antonia, Stucci, Stefania Antonia, Stugu, Bjarne, Stupak, John, Styles, Nicholas, Bessidskaia Bylund, Olga, Su, Dong, Su, Wanyun, Su, Xiaowen, Suarez, Nicholas Bruno, Sulin, Vladimir, Sullivan, Matthew James, Sultan, D. M. S., Sultanov, Salekh, Sultansoy, S., Sumida, Toshi, Besson, Nathalie, Sun, Siyuan, Sun, Xiaohu, Suster, Carl Joseph Edmund, Sutton, Mark, Suzuki, Shota, Svatos, Michal, Swiatlowski, Maximilian J, Swift, Stewart Patrick, Swirski, Thorben, Sydorenko, Alexander, Bethke, Siegfried, Sykora, Ivan, Sykora, Martin, Sykora, Tomas, Ta, Duc Bao, Tackmann, Kerstin, Kinghorn-taenzer, Joseph Peter, Taffard, Anyes, Tafirout, Reda, Tagiev, Emin, Taibah, Reem Hani M, Betti, Alessandra, Takashima, Ryuichi, Takeda, Kosuke, Takeshita, Toru, Takeva, Emily Petrova, Takubo, Yosuke, Talby, Mossadek, Talyshev, Alexei, Tam, Kai Chung, Tamir, Nadav Michael, Tanaka, Junichi, Bevan, Adrian, Tanaka, Reisaburo, Tokar, Stanislav, Tsukerman, Ilya, Tsybychev, Dmitri, Tanaka, Rei, Tapia Araya, Sebastian, Tapprogge, Stefan, Tarek, Ahmed, Tarem, Shlomit, Tariq, Khuram, Beyer, Julien-christopher, Tarna, Grigore, Tartarelli, Francesco, Tas, Petr, Tasevsky, Marek, Tassi, Enrico, Tateno, Gen, Tavares Delgado, Ademar, Tayalati, Yahya, Taylor, Alan James, Taylor, Geoffrey Norman, Bhatta, Somadutta, Taylor, Wendy Jane, Teagle, Hamish Edward, Tee, Amy, Teixeira De Lima, Rafael, Teixeira-dias, Pedro, Ten Kate, Herman, Teoh, Jia Jian, Terashi, Koji, Terron Cuadrado, Juan, Terzo, Stefano, Bhattacharya, Deb Sankar, Testa, Marianna, Teuscher, Richard, Themistokleous, Neofytos, Theveneaux-pelzer, Timothee, Thomas, David William, Thomas, Juergen, Thompson, Emily Anne, Thompson, Paul, Thomson, Evelyn Jean, Thorpe, Edward James, Bhattarai, Prajita, Tikhomirov, Vladimiro, Tuts, Michael, Vacek, Vaclav, Tikhonov, Iouri, Timoshenko, Sergei, Tipton, Paul Louis, Tisserant, Sylvain, Todome, Kazuki, Todorova, Sarka, Todt, Stefanie, Agapopoulou, Christina, Bhopatkar, Vallary Shashikant, Tojo, Junji, Vandewall, Evan Richard, Tokar, Stano, Tokushuku, Katsuo, Tolley, Emma Elizabeth, Tombs, Rupert, Tomiwa, Kehinde Gbenga, Tomoto, Makoto, Tompkins, Lauren Alexandra, Tornambe, Peter, Bi, Runyu, Torrence, Eric, Torres, Heberth, Torro Pastor, Emma, Toscani, Mariana, Tosciri, Cecilia, Toth, Jozsef, Tovey, Daniel, Traeet, Are Sivertsen, Treado, Colleen Jennifer, Trefzger, Thomas, Bianchi, Riccardo Maria, Tresoldi, Fabio, Tricoli, Alessandro, Trigger, Isabel, Trincaz-duvoid, Sophie, Trischuk, Dominique Anderson, Trischuk, William, Trocme, Benjamin, Trofymov, Artur, Troncon, Clara, Trovato, Fabrizio, Biebel, Otmar, Truong, Thi Ngoc Loan, Trzebinski, Maciej, Trzupek, Adam, Tsai, Fang-ying, Tsiareshka, Pavel, Tsirigotis, Apostolos, Tsiskaridze, Vakhtang, Tskhadadze, Edisher, Tsopoulou, Maria-evanthia, Tsukerman, Ilia, Biedermann, Dustin, Tsulaia, Vakhtang, Tsuno, Soshi, Tsybyshev, Dmitry, Tu, Yanjun, Tudorache, Alexandra, Tudorache, Valentina, Tuna, Alexander Naip, Turchikhin, Semen, Turgeman, Daniel, Turk Cakir, Ilkay, Bielski, Rafal, Turner, Russell James, Turra, Ruggero, Tuts, Mike, Tzamarias, Spyros, Tzovara, Eftychia, Uchida, Kenta, Ukegawa, Fumihiko, Unal, Guillaume, Unal, Mesut, Undrus, Alexander, Bierwagen, Katharina, Unel, Gokhan, Ungaro, Francesca, Unno, Yoshinobu, Uno, Kenta, Urban, Josef, Urquijo, Phillip, Usai, Giulio, Uysal, Zekeriya, Vacek, Vic, Vachon, Brigitte, Biesuz, Nicolo Vladi, Vadla, Knut Oddvar Hoie, Vafeiadis, Theodoros, Vaidya, Amal, Valderanis, Chrysostomos, Valdes Santurio, Eduardo, Valente, Marco, Valentinetti, Sara, Valero Biot, Alberto, Valery, Loic, Vallance, Robert Adam, Biglietti, Michela, Vallier, Alexis, Valls Ferrer, Juan, Van Daalen, Tal Roelof, Van Gemmeren, Peter, Van Stroud, Samuel, Van Vulpen, Ivo, Vanadia, Marco, Vandelli, Wainer, Vandenbroucke, Maxence, Van De Wall, Evan Richard, Billoud, T. R. V., Vannicola, Damiano, Vari, Riccardo, Varnes, Erich Ward, Varni, Carlo, Mete, Tulin, Varouchas, Dimitris, Varvell, Kevin, Vasile, Matei, Vasquez, Gerardo, Vazeille, Francois, Agaras, Merve Nazlim, Bindi, Marcello, Vazquez Furelos, David, Vazquez Schroeder, Tamara, Veatch, Jason Robert, Vecchio, Valentina, Veen, Michiel Jan, Veloce, Laurelle Maria, Veloso, Filipe, Veneziano, Stefano, Ventura, Andrea, Verbytskyi, Andrii, Bingul, Ahmet, Vercesi, Valerio, Verducci, Monica, Vergel Infante, Carlos Miguel, Vergis, Christos, Verkerke, Wouter, Vermeulen, Ambrosius Thomas, Vermeulen, Joseph, Vernieri, Caterina, Verschuuren, Pim Jordi, Vetterli, Michel Joseph, Bini, Cesare, Viaux Maira, Nicolas, Vickey, Trevor, Vickey Boeriu, Oana, Viehhauser, G. H. 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Victoria, Castro, Nuno, Catinaccio, Andrea, Catmore, James, Cattai, Ariella, Alderweireldt, Sara, Cavaliere, Viviana, Cavasinni, Vincenzo, Celebi, Emre, Celli, Federico, Cerny, Karel, Santiago Cerqueira, Augusto, Cerri, Alex, Cerri, Alessandro, Cerrito, Lucio, Cerutti, Fabio, Aleksa, Martin, Cervelli, Alberto, Cetin, Serkant, Chadi, Zakaria, Chakraborty, Dhiman, Chan, Jay, Chan, Terry Ws, Chan, Wing Sheung, Chan, Wai Yuen, Chapman, John Derek, Chargeishvili, Bakar, Alexandrov, Igor, Charlton, Dave, Charman, Thomas Paul, Chatterjee, Meghranjana, Chau, Chav Chhiv, Che, Siinn, Chekanov, Sergei, Chekulaev, Sergey, Shelkov, G., Chen, Boping, Chen, Cheng, Alexa, Calin, Chen, Chunhui, Chen, Huirun, Chen, Hucheng, Chen, Jing, Chen, Jue, Chen, Jiayi, Chen, Shion, Chen, Shenjian, Chen, Xin, Chen, Ye, Abeling, Kira, Alexopoulos, Theodoros, Chen, Yu-heng, Cheng, Hok Chuen, Cheng, Huajie, Cheplakov, Alexander, Cheremushkina, Evgeniya, Cherkaoui El Moursli, Rajaa, Cheu, Elliott, Cheung, Kingman, Chevalerias, Thibault, Chevalier, Laurent, Alfonsi, Alice, Chiarella, Vitaliano, Chiarelli, Giorgio, Chiodini, Gabriele, Chisholm, Andrew Stephen, Chitan, Adrian, Chiu, I-huan, Chiu, Justin, Chizhov, Mihail, Choi, Kyungeon, Chomont, Arthur, Alfonsi, Fabrizio, Chou, Yuan-tang, Chow, Edwin, Chow, Yun Sang, Christopher, Lawrence Davou, Chu, Ming Chung, Chu, Xiaotong, Chudoba, Jiri, Chwastowski, Janusz, Chytka, Ladislav, Cieri, Davide, Alhroob, Muhammad, Ciesla, Krzysztof, Cindro, Vladimir, Cioara, Irina Antonela, Ciocio, Alessandra, Cirotto, Francesco, Citron, Zvi, Citterio, Mauro, Ciubotaru, Dan Andrei, Ciungu, Bianca Monica, Clark, Allan, Ali, Babar, Clark, Philip, Clawson, Savannah, Clement, Christophe, Clissa, Luca, Coadou, Yann, Cobal, Marina, Coccaro, Andrea, Cochran Jr, James Herbert, Coelho Lopes De Sa, Rafael, Cohen, Hadar, Ali, Shahzad, Coimbra, Artur, Cole, Brian, Colijn, Auke-pieter, Collot, Johann, Conde Muino, Patricia, Connell, Simon, Connelly, Ian Allan, Constantinescu, Serban, Conventi, Francesco, Sarkar, Amanda, Aliev, Malik, Cormier, Felix, Cormier, Kyle James Read, Corpe, Louie Dartmoor, Corradi, Massimo, Corrigan, Eric Edward, Corriveau, Francois, Costa Mezquita, Maria Jose, Costanza, Francesco, Costanzo, Davide, Cowan, Glen, Alimonti, Gianluca, Cowley, James William, Crane, Jonathan, Cranmer, Kyle Stuart, Creager, Rachael Ann, Crepe-renaudin, Sabine, Crescioli, Francesco, Cristinziani, Markus, Croft, Vincent Alexander, Crosetti, Giovanni, Cunningham, William Reilly, Allaire, Corentin, Crosetti, Nanni, Cueto Gomez, Ana Rosario, Cuhadar Donszelmann, Tulay, Cui, Han, Cukierman, Aviv Ruben, Dandoy, Jeffrey Rogers, Cunningham, Liam, Czekierda, Sabina Anna, Czodrowski, Patrick Karl, Czurylo, Marta, Allbrooke, Benedict, Sousa, Mario Jose, Da Fonseca Pinto, Joao Victor, Da Via, Cinzia, Dabrowski, Wladyslaw, Dachs, Florian, Dado, Tomas, Dahbi, Salah-eddine, Dai, Tiesheng, Dallapiccola, Carlo, Dam, Mogens, Abhayasinghe, Deshan Kavishka, Allen, Benjamin William, D'amen, Gabriele, D'amico, Valerio, Damp, Johannes Frederic, Darbo, Giovanni, Dandoy, Jeff, Daneri, Maria Florencia, Danninger, Matthias, Dao, Valerio, Darbo, Nanni, Dartsi, Olympia, Allport, Philip Patrick, Dattagupta, Aparajita, Daubney, Thomas, D'auria, Saverio, David, Claire, Davidek, Tomas, Davis, Douglas Raymond, Dawson, Ian, De, Kaushik, De Asmundis, Riccardo, De Beurs, Marcus, Aloisio, Alberto, De Castro, Stefano, De Groot, Nicolo, De Jong, Paul, De La Torre Perez, Hector, De Maria, Antonio, De Pedis, Daniele, De Salvo, Alessandro, De Sanctis, Umberto, De Santis, Maurizio, De Santo, Antonella, Alonso, Francisco, De Vivie De Regie, Jean-baptiste, Dedovich, Dmitri, Deiana, Allison Mccarn, Del Peso, Jose, Delabat Diaz, Yasiel, Delgove, David, Deliot, Frederic, Delitzsch, Chris Malena, Della Pietra, Massimo, Della Volpe, Domenico, Alpigiani, Cristiano, Dell'acqua, Andrea, Dell'asta, Lidia, Delmastro, Marco, Delporte, Charles Eliaz, Delsart, Pierre Antoine, Demers Konezny, Sarah Marie, Demichev, Mikhail, Demontigny, Gabriel, Denisov, Sergey, Denisov, Serguei, Alunno Camelia, Elio, D'eramo, Louis, Derendarz, Dominik Karol, Derkaoui, Jamal, Derue, Frederic, Dervan, Paul, Desch, Klaus, Dette, Karola, Deutsch, Christopher, Devesa, Maria Roberta, Deviveiros, Pier-olivier, Alvarez Estevez, Manuel, Di Bello, Francesco Armando, Di Ciaccio, Anna, Di Ciaccio, Lucia, Di Donato, Camilla, Di Girolamo, Alessandro, Di Gregorio, Giulia, Di Luca, Andrea, Di Micco, Biagio, Di Nardo, Roberto, Di Petrillo, Karri Folan, Alviggi, Mariagrazia, Di Sipio, Riccardo, Diaconu, Cristinel, De Almeida Dias, Flavia, Vale, Tiago, Diaz Gutierrez, Marco Aurelio, Diaz Capriles, Federico Guillermo, Dickinson, Jennet Elizabeth, Didenko, Mariia, Diehl, Edward, Dietrich, Janet, Do Amaral Coutinho, Yara, Diez Cornell, Sergio, Diez Pardos, Carmen, Dimitrievska, Aleksandra, Ding, Wei, Dingfelder, Jochen Christian, Dittmeier, Sebastian, Dittus, Fido, Djama, Fares, Djobava, Tamar, Djuvsland, Julia Isabell, Ambler, Alessandro, Barros do Vale, Maria Aline, Dobre, Monica, Dodsworth, David Michael, Doglioni, Caterina, Dolejsi, Jiri, Dolezal, Zdenek, Donadelli, Marisilvia, Dong, Binbin, Donini, Julien Noce, D'onofrio, Adelina, Abidi, Haider, Ambroz, Luca, D'onofrio, Monica, Dopke, Jens, Doria, Alessandra, Dova, Maria Teresa, Doyle, Tony, Drechsler, Eric, Dreyer, Etienne, Dreyer, Timo, Drobac, Alec Swenson, Du, Dongshuo, Amelung, Christoph, Du Pree, Tristan Arnoldus, Duan, Yanyun, Dubinin, Filipp, Dubovsky, Michal, Dubreuil, Arnaud, Duchovni, Ehud, Duckeck, Guenter, Ducu, Otilia Anamaria, Duda, Dominik, Dudarev, Alexey, Amidei, Dante, Dudder, Andreas Christian, Duffield, Emily Marie, D'uffizi, Matteo, Duflot, Laurent, Duehrssen-debling, Michael, Dulsen, Carsten, Dumancic, Mirta, Dumitriu, Ana Elena, Dunford, Monica, Dungs, Sascha, Amor Dos Santos, Susana Patricia, Duperrin, Arnaud, Yildiz, Duran, Dueren, Michael Johannes, Durglishvili, Archil, Duschinger, Dirk Uwe, Dutta, Baishali, Duvnjak, Damir, Dyckes, George, Dyckes, Ian, Dyndal, Mateusz, Amoroso, Simone, Dysch, Samuel Dezso, Dziedzic, Bartosz Sebastian, Eggleston, Michael Glenn, Eifert, Till, Eigen, Gerald, Einsweiler, Kevin Frank, Ekelof, Tord Johan Carl, El Jarrari, Hassnae, Ellajosyula, Venugopal, Ellert, Mattias, Amrouche, Cherifa Sabrina, Ellinghaus, Frank, Elliot, Alison, Ellis, Nicolas, Emerman, Alexander, Ellis, Nick, Elmsheuser, Johannes, Elsing, Markus, Emeliyanov, Dmitry, Emerman, Alex, Enari, Yuji, An, Fenfen, Epland, Matthew, Erdmann, Johannes, Ereditato, Antonio, Erland, Paula Agnieszka, Errenst, Martin, Escalier, Marc, Escobar Ibanez, Carlos, Estrada Pastor, Oscar, Etzion, Erez, Gaspar De Andrade Evans, Guiomar, Anastopoulos, Christos, Evans, Hal, Evans, Meirin Oan, Ezhilov, Alexey, Ezhilov, Aleksei, Fabbri, Federica, Fabbri, Laura, Fabiani, Veronica, Facini, Gabriel, Fakhrutdinov, Rinat, Falciano, Speranza, Andari, Nansi, Falke, Peter Johannes, Falke, Saskia, Faltova, Jana, Fang, Yi, Fang, Yaquan, Fanourakis, Georgios, Fanti, Marcello, Faraj, Mohammed, Farbin, Amir, Farilla, Addolorata, Andeen, Timothy Robert, Farilla, Ada, Farina, Edoardo Maria, Farooque, Trisha, Farrington, Sinead, Farthouat, Philippe, Fassi, Farida, Fassnacht, Patrick, Fassouliotis, Dimitris, Faucci Giannelli, Michele, Fawcett, William James, Abouzeid, Hass, Anders, John Kenneth, Fayard, Louis, Fedin, Oleg, Fedorko, Woiciech, Fell, Alexandra, Fedorko, Wojtek, Fehr, Armin, Feickert, Matthew Carl, Feligioni, Lorenzo, Fell, Alix, Feng, Cunfeng, Andrean, Stefio Yosse, Feng, Minyu, Fenton, Michael James, Fenyuk, Alexandre, Ferguson, Sarah Whitney, Ferrando, James Edward, Ferrari, Arnaud, Ferrari, Pamela, Ferrari, Roberto, Ferreira De Lima, Danilo Enoque, Ferrer Soria, Antonio, Andreazza, Attilio, Ferrere, Didier, Ferretti, Claudio, Fiedler, Frank, Filipcic, Andrej, Filthaut, Frank, Finelli, Kevin Daniel, Castro Nunes Fiolhais, Miguel, Fiorini, Luca, Fischer, Florian, Fischer, Julian, Andrei, Victor, Fisher, Wade Cameron, Fitschen, Tobias, Fleck, Ivor, Fleischmann, Philipp, Flick, Tobias, Flierl, Bernhard Matthias, Flores, Lucas Macrorie, Flores Castillo, Luis Roberto, Follega, Francesco Maria, Fomin, Nikolai, Anelli, Christopher Ryan, Foo, Joel Hengwei, Forcolin, Giulio Tiziano, Forland, Blake Christopher, Formica, Andrea, Forster, Fabian Alexander, Forti, Alessandra, Fortin, Etienne Marie, Foti, Maria Giovanna, Fournier, Daniel, Fox, Harald, Angelidakis, Stylianos, Francavilla, Paolo, Francescato, Simone, Franchini, Matteo, Franchino, Silvia, Francis, David, Franco, Luca, Franconi, Laura, Franklin, Melissa, Frattari, Guglielmo, Fray, Antony, Angerami, Aaron, Freeman, Patrick Moriishi, Freund, Benjamin, Spolidoro Freund, Werner, Freundlich, Elena Murielle, Frizzell, Dylan Cooper, Froidevaux, Daniel, Frost, James, Fujimoto, Minori, Fukunaga, Chikara, Fullana Torregrosa, Esteban, Anisenkov, Alexey, Fusayasu, Takahiro, Fuster Verdu, Juan, Gabrielli, Alessandro, Gabrielli, Andrea, Gadatsch, Stefan, Gadow, Paul Philipp, Gagliardi, Guido, Gagnon, Louis-guillaume, Gallardo, Gabriel, Gallas, Elizabeth, Annovi, Alberto, Gallop, Bruce Joseph, Gamboa Goni, Rodrigo, Gan, Kock Kiam, Ganguly, Sanmay, Gao, Jun, Gao, Yanyan, Gao, Yongsheng, Garay Walls, Francisca, Garcia, Carmen, Garcia Navarro, Jose Enrique, Antel, Claire, Garcia Pascual, Juan Antonio, Garcia, Juanan, Garcia Argos, Carlos, Garcia-sciveres, Maurice, Gardner Jr, Robert William, Garelli, Nicoletta, Gargiulo, Simona, Garner, Christopher Andrew, Garonne, Vincent, Gasiorowski, Sean Joseph, Abouzeid, Ossama, Anthony, Matthew Thomas, Do Nascimento Gaspar, Philipp, Gaudiello, Andrea, Gaudio, Gabriella, Gauzzi, Paolo, Gavrilenko, Igor, Gavrilyuk, Alexander, Gavriliuk, Aleksandr, Gay, Colin Warren, Gaycken, Goetz, Gazis, Evangelos, Antipov, Egor, Geanta, Andrei Alexandru, Gee, Carolyn, Gee, C. N. P., Geisen, Jannik, Geisen, Marc, Gemme, Claudia, Genest, Marie-helene, Geng, Cong, Gentile, Simonetta, George, Simon, Antonelli, Mario, Geralis, Theodoros, Gerlach, Lino Oscar, Gessinger-befurt, Paul, Gessner, Gregor, Ghasemi Bostanabad, Meisam, Ghneimat, Mazuza, Ghosh, Aishik, Ghosh, Anindya, Giacobbe, Benedetto, Giagu, Stefano, Antrim, Daniel Joseph, Giangiacomi, Nico, Giannetti, Paola, Giannini, Antonio, Giannini, Giulia, Gibson, Stephen, Gignac, Matthew, Gil, Damian Tomasz, Gilbert, Benjamin Jacob, Gillberg, Dag, Gilles, Geoffrey, Anulli, Fabio, Gillwald, Nils, Gingrich, Douglas, Giordani, MarioPaolo, Gingrich, Doug, Giordani, Mapo, Giraud, Pierre-francois, Giugliarelli, Gilberto, Giugni, Danilo, Giuli, Francesco, Gkaitatzis, Stamatios, Aoki, Masato, Gkialas, Ioannis, Gkougkousis, Evangelos, Gkougkousis, Vagelis, Gkountoumis, Panagiotis, Gladilin, Leonid, Glasman, Claudia, Glatzer, Julian, Glaysher, P. C. F., Glazov, Alexander, Gledhill, Galen Rhodes, Aparisi Pozo, Javier Alberto, Gnesi, Ivan, Goblirsch-kolb, Maximilian Emanuel, Godin, Dominique, Goldfarb, Steven, Golling, Tobias, Golubkov, Dmitry, Da Silva Gomes, Agostinho, Goncalves Gama, Rafael, Morais Silva Goncalo, Ricardo Jose, Gonella, Giulia, Aparo, Marco, Gonella, Laura, Gongadze, Alexi, Gonnella, Francesco, Gonski, Julia Lynne, Gonzalez De La Hoz, Santiago, Gonzalez Fernandez, Sergio, Gonzalez Lopez, Ricardo, Gonzalez Renteria, Cesar, Gonzalez Suarez, Rebeca, Gonzalez Sevilla, Sergio, Aperio Bella, Ludovica, Gonzalvo Rodriguez, Galo Rafael, Goossens, Luc, Gorasia, Nandish Arjan, Gorbounov, Petr, Gordon, Howard, Gorini, Benedetto, Gorini, Edoardo, Gorisek, Andrej, Goshaw, Al, Goshaw, Alfred, Aranzabal Barrio, Nordin, Gostkin, Mikhail, Gottardo, Carlo Alberto, Gouighri, Mohamed, Goussiou, Anna, Govender, Nicolin, Goy, Corinne, Grabowska-bold, Iwona, Graham, Emily Charlotte, Gramling, Johanna, Gramstad, Eirik, Aad, G., Abbott, B., Abbott, D. C., Abed Abud, A., Abeling, K., Abhayasinghe, D. K., Abidi, S. H., Abouzeid, O. S., Abraham, N. L., Abramowicz, H., Abreu, H., Abulaiti, Y., Acharya, B. S., Achkar, B., Adam, L., Adam Bourdarios, C., Adamczyk, L., Adamek, L., Adelman, J., Adiguzel, A., Adorni, S., Adye, T., Affolder, A. A., Afik, Y., Agapopoulou, C., Agaras, M. N., Aggarwal, A., Agheorghiesei, C., Aguilar-Saavedra, J. A., Ahmad, A., Ahmadov, F., Ahmed, W. S., Ai, X., Aielli, G., Akatsuka, S., Akbiyik, M., Akesson, T. P. A., Akilli, E., Akimov, A. V., Al Khoury, K., Alberghi, G. L., Albert, J., Alconada Verzini, M. J., Alderweireldt, S., Aleksa, M., Aleksandrov, I. N., Alexa, C., Alexopoulos, T., Alfonsi, A., Alfonsi, F., Alhroob, M., Ali, B., Ali, S., Aliev, M., Alimonti, G., Allaire, C., Allbrooke, B. M. M., Allen, B. W., Allport, P. P., Aloisio, A., Alonso, F., Alpigiani, C., Alunno Camelia, E., Alvarez Estevez, M., Alviggi, M. G., Amaral Coutinho, Y., Ambler, A., Ambroz, L., Amelung, C., Amidei, D., Amor Dos Santos, S. P., Amoroso, S., Amrouche, C. S., An, F., Anastopoulos, C., Andari, N., Andeen, T., Anders, J. K., Andrean, S. Y., Andreazza, A., Andrei, V., Anelli, C. R., Angelidakis, S., Angerami, A., Anisenkov, A. V., Annovi, A., Antel, C., Anthony, M. T., Antipov, E., Antonelli, M., Antrim, D. J. A., Anulli, F., Aoki, M., Aparisi Pozo, J. A., Aparo, M. A., Aperio Bella, L., Aranzabal, N., Araujo Ferraz, V., Araujo Pereira, R., Arcangeletti, C., Arce, A. T. H., Arguin, J. -F., Argyropoulos, S., Arling, J. -H., Armbruster, A. J., Armstrong, A., Arnaez, O., Arnold, H., Arrubarrena Tame, Z. P., Artoni, G., Asada, H., Asai, K., Asai, S., Asawatavonvanich, T., Asbah, N., Asimakopoulou, E. M., Asquith, L., Assahsah, J., Assamagan, K., Astalos, R., Atkin, R. J., Atkinson, M., Atlay, N. B., Atmani, H., Atmasiddha, P. A., Augsten, K., Austrup, V. A., Avolio, G., Ayoub, M. 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[0000-0002-3360-4965], Zheng, Z. [0000-0002-8323-7753], Zhong, D. [0000-0001-9377-650X], Zhou, C. [0000-0001-5904-7258], Zhou, H. [0000-0002-7986-9045], Zhou, M. [0000-0001-7223-8403], Zhou, N. [0000-0002-1775-2511], Zhu, C. G. [0000-0001-8015-3901], Zhu, C. [0000-0002-5918-9050], Zhu, H. L. [0000-0001-8479-1345], Zhu, H. [0000-0001-8066-7048], Zhu, J. [0000-0002-5278-2855], Zhu, Y. [0000-0002-7306-1053], Zhuang, X. [0000-0003-0996-3279], Zhukov, K. [0000-0003-2468-9634], Zhulanov, V. [0000-0002-0306-9199], Zieminska, D. [0000-0002-6311-7420], Zimine, N. I. [0000-0003-0277-4870], Zimmermann, S. [0000-0002-1529-8925], Živković, L. [0000-0003-4236-8930], Zobernig, G. [0000-0001-8113-1499], Zoccoli, A. [0000-0002-0993-6185], Zoch, K. [0000-0003-2138-6187], Zorbas, T. G. [0000-0003-2073-4901], Zou, R. [0000-0002-0542-1264], Zwalinski, L. [0000-0002-9397-2313], Apollo - University of Cambridge Repository, ATLAS (IHEF, IoP, FNWI), XENON (IHEF, IoP, FNWI), Other Research IHEF (IoP, FNWI), Centre de Physique des Particules de Marseille (CPPM), Aix Marseille Université (AMU)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Laboratoire d'Annecy de Physique des Particules (LAPP), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Physique des 2 Infinis Irène Joliot-Curie (IJCLab), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Physique de Clermont (LPC), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Clermont Auvergne (UCA), Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE (UMR_7585)), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP ), Université Grenoble Alpes (UGA), Centre de Calcul de l'IN2P3 (CC-IN2P3), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), ATLAS, De Castro , S., Fabbri , L., Gabrielli , A., Rinaldi , L., Semprini Cesari , N., Sioli , M., Villa , M., Zoccoli , A., Bellagamba , L., Boscherini , D., Bruni , A., Bruni , G., Giacobbe , B., Polini , A., Sbarra , C., Sidoti , A., Franchini , M., Romano , M., Valentinetti , S., Alberghi , G. L., Lasagni Manghi , F, Massa , L., Vittori , C., Alfonsi , F, Cabras , G., Cervelli , A., Negrini , M., Todome , K., Carratta , G., Cavalli , N., Clissa , L., ATLAS collaboration, Współautorami artykułu są członkowie ATLAS Collaboration w liczbie 2933, Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Aad, G, Bachas, K, Chiodini, G, Gorini, E, Gravili, F, Longo, L, Primavera, M, Reale, M, Schioppa, E, Spagnolo, S, Ventura, A, and ATLAS Collaboration, And
Subjects: 13000 GeV-cms, QC770-798, 01 natural sciences, 7. Clean energy, lepton: flavor, proton-proton scattering, Subatomär fysik, Higgs particle: hadroproduction, effective field theory, Hadron-Hadron scattering (experiments), scattering [p p], Z0: pair production, Invariant (mathematics), Leading order qcd, Settore FIS/01, Large Hadron Collider, 3. Good health, pair production [Z0], muon: pair production, CERN LHC Coll, kinematics, Strahlung, Higgs boson, Branching fraction, colliding beams [p p], Z0: branching ratio: measured, p p: scattering, mass spectrum: (4lepton), gauge [symmetry], branching ratio: measured [Z0], Standard Model, TeV, ddc:530, pair production [electron], High Energy Physics, 010306 general physics, Fusion, Particle Physics, Muon, 010308 nuclear & particles physics, Parton Distributions, Computer Science::Information Retrieval, (4lepton) [mass spectrum], +4lepton%22">Z0 --> 4lepton, Beyond Standard Model, p p: colliding beams, Kjerne- og elementærpartikkelfysikk: 431 [VDP], dilepton: mass spectrum, Physics beyond the Standard Model, measured [channel cross section], transverse momentum [dilepton], mass spectrum [dilepton], High Energy Physics - Experiment, electron: pair production, High Energy Physics - Experiment (hep-ex), Subatomic Physics, [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex], Invariant mass, Z0: single production, Physics, angular correlation, new physics: search for, ZZ production, ATLAS, Lepton production, Nuclear and elementary particle physics: 431 [VDP], category, LHC, single production [Z0], channel cross section: measured, Particle Physics - Experiment, Higgs production, Nuclear and High Energy Physics, Particle physics, 530 Physics, Regular Article - Experimental Physics, interference, FOS: Physical sciences, differential cross section: measured, search for [new physics], measured [differential cross section], Nuclear and particle physics. Atomic energy. Radioactivity, 0103 physical sciences, flavor [lepton], pair production [muon], hep-ex, High Energy Physics::Phenomenology, symmetry: gauge, spontaneous symmetry breaking, Física, Higgs Boson, leptonic decay [Z0], Z0: leptonic decay, hadroproduction [Higgs particle], High Energy Physics::Experiment, dilepton: transverse momentum, Hadron-hadron collisions, experimental results, Lepton
Abstract: We thank CERN for the very successful operation of the LHC, as well as the support staff from our institutions without whom ATLAS could not be operated efficiently. We acknowledge the support of ANPCyT, Argentina; YerPhI, Armenia; ARC, Australia; BMWFW and FWF, Austria; ANAS, Azerbaijan; SSTC, Belarus; CNPq and FAPESP, Brazil; NSERC, NRC and CFI, Canada; CERN; ANID, Chile; CAS, MOST and NSFC, China; COLCIENCIAS, Colombia; MSMT CR, MPO CR and VSC CR, Czech Republic; DNRF and DNSRC, Denmark; IN2P3-CNRS and CEA-DRF/IRFU, France; SRNSFG, Georgia; BMBF, HGF and MPG, Germany; GSRT, Greece; RGC and Hong Kong SAR, China; ISF and Benoziyo Center, Israel; INFN, Italy; MEXT and JSPS, Japan; CNRST, Morocco; NWO, Netherlands; RCN, Norway; MNiSW and NCN, Poland; FCT, Portugal; MNE/IFA, Romania; JINR; MES of Russia and NRC KI, Russian Federation; MESTD, Serbia; MSSR, Slovakia; ARRS and MIZŠ, Slovenia; DST/NRF, South Africa; MICINN, Spain; SRC and Wallenberg Foundation, Sweden; SERI, SNSF and Cantons of Bern and Geneva, Switzerland; MOST, Taiwan; TAEK, Turkey; STFC, United Kingdom; DOE and NSF, United States of America. In addition, individual groups and members have received support from BCKDF, CANARIE, Compute Canada, CRC and IVADO, Canada; Beijing Municipal Science & Technology Commission, China; COST, ERC, ERDF, Horizon 2020 and Marie Skłodowska-Curie Actions, European Union; Investissements d’Avenir Labex, Investissements d’Avenir Idex and ANR, France; DFG and AvH Foundation, Germany; Herakleitos, Thales and Aristeia programmes co-financed by EU-ESF and the Greek NSRF, Greece; BSF-NSF and GIF, Israel; La Caixa Banking Foundation, CERCA Programme Generalitat de Catalunya and PROMETEO and GenT Programmes Generalitat Valenciana, Spain; Göran Gustafssons Stiftelse, Sweden; The Royal Society and Leverhulme Trust, United Kingdom. The crucial computing support from all WLCG partners is acknowledged gratefully, in particular from CERN, the ATLAS Tier-1 facilities at TRIUMF (Canada), NDGF (Denmark, Norway, Sweden), CC-IN2P3 (France), KIT/GridKA (Germany), INFN-CNAF (Italy), NL-T1 (Netherlands), PIC (Spain), ASGC (Taiwan), RAL (UK) and BNL (USA), the Tier-2 facilities worldwide and large non-WLCG resource providers. Major contributors of computing resources are listed in ref. [109]., Measurements of four-lepton differential and integrated fiducial cross-sections in events with two same-flavour, opposite-charge electron or muon pairs are presented. The data correspond to 139 fb(-1) of root s = 13 TeV proton-proton collisions, collected by the ATLAS detector during Run 2 of the Large Hadron Collider (2015-2018). The final state has contributions from a number of interesting Standard Model processes that dominate in different four-lepton invariant mass regions, including single Z boson production, Higgs boson production and on-shell ZZ production, with a complex mix of interference terms, and possible contributions from physics beyond the Standard Model. The differential cross-sections include the four-lepton invariant mass inclusively, in slices of other kinematic variables, and in different lepton flavour categories. Also measured are dilepton invariant masses, transverse momenta, and angular correlation variables, in four regions of four-lepton invariant mass, each dominated by different processes. The measurements are corrected for detector effects and are compared with state-of-the-art Standard Model calculations, which are found to be consistent with the data. The Z -> 4l branching fraction is extracted, giving a value of (4.41 +/- 0.30) x 10(-6). Constraints on effective field theory parameters and a model based on a spontaneously broken B - L gauge symmetry are also evaluated. Further reinterpretations can be performed with the provided information., ANPCyT, Argentina, YerPhI, Armenia, ARC, Australia, BMWFW and FWF, Austria, ANAS, Azerbaijan, SSTC, Belarus, CNPq and FAPESP, Brazil, NSERC, NRC and CFI, Canada, CERN, ANID, Chile, CAS, MOST and NSFC, China, COLCIENCIAS, Colombia, MSMT CR, MPO CR and VSC CR, Czech Republic, DNRF and DNSRC, Denmark, IN2P3-CNRS and CEA-DRF/IRFU, France, SRNSFG, Georgia, BMBF, HGF and MPG, Germany, GSRT, Greece, RGC and Hong Kong SAR, China, ISF and Benoziyo Center, Israel, INFN, Italy, MEXT and JSPS, Japan, CNRST, Morocco, NWO, Netherlands, RCN, Norway, MNiSW and NCN, Poland, FCT, Portugal, MNE/IFA, Romania, JINR, MES of Russia and NRC KI, Russian Federation, MESTD, Serbia, MSSR, Slovakia, ARRS and MIZŠ, Slovenia, DST/NRF, South Africa, MICINN, Spain, SRC and Wallenberg Foundation, Sweden, SERI, SNSF and Cantons of Bern and Geneva, Switzerland, MOST, Taiwan, TAEK, Turkey, STFC, United Kingdom, DOE and NSF, United States of America, BCKDF, CANARIE, Compute Canada, CRC and IVADO, Canada, Beijing Municipal Science & Technology Commission, China, COST, ERC, ERDF, Horizon 2020 and Marie Skłodowska-Curie Actions, European Union, Investissements d’Avenir Labex, Investissements d’Avenir Idex and ANR, France, DFG and AvH Foundation, Germany, Herakleitos, Thales and Aristeia programmes co-financed by EU-ESF and the Greek NSRF, Greece, BSF-NSF and GIF, Israel, La Caixa Banking Foundation, CERCA Programme Generalitat de Catalunya and PROMETEO and GenT Programmes Generalitat Valenciana, Spain, Göran Gustafssons Stiftelse, Sweden, The Royal Society and Leverhulme Trust, United Kingdom.
Published: 2021
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16. Updated galactic radio constraints on Dark Matter

Author: Taoso, Marco [Instituto de Física Teórica (IFT) UAM/CSIC,calle Nicolás Cabrera 13-15, Cantoblanco, Madrid, 28049 (Spain)]
Published: 2016
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17. Entanglement in inhomogeneous quantum chains

Author: Samos Sáenz de Buruaga, Daniel Nadir, Sierra, Germán, Rodríguez Laguna, Javier, UAM. Departamento de Física Teórica, and Instituto de Física Teórica (IFT)
Subjects: Teoría cuántica-Tesis doctorales, Física
Abstract: Tesis Doctoral inédita leída en la Universidad Autónoma de Madrid, Facultad de Ciencias, Departamento de Física Teórica. Fecha de Lectura: 05-04-2022
Published: 2022

18. Physics and Geometry of Gravity at High Energies

Author: Murcia Gil, Angel Jesús, Ortín Miguel, Tomás, Shahbazi Alonso, Carlos Shahin, UAM. Departamento de Física Teórica, and Instituto de Física Teórica (IFT)
Subjects: Física, Supergravedad, Supercuerdas, Teoría de
Abstract: Tesis Doctoral inédita leída en la Universidad Autónoma de Madrid, Facultad de Ciencias, Departamento de Física Teórica. Fecha de Lectura: 12-09-2022, En esta tesis se estudian aspectos físicos y geométricos de la gravedad a altas energías. Por un lado, se realiza una investigación detallada de la física gravitacional en este régimen con la ayuda de las gravedades de orden superior. Son extensiones de la Relatividad General que incluyen términos en derivadas superiores de la métrica y otros campos que, además de una interpretación como teorías efectivas, también poseen una relevancia intrínseca. En concreto, nos concentramos en gravedades de orden superior de la clase Cuasitopológica (Generalizada). Se definen como aquellas que admiten soluciones estáticas y esféricamente simétricas caracterizadas por una sola función que cumple una ecuación de segundo orden o inferior en derivadas. La motivación para el estudio de dichas teorías es doble: permiten cálculos explícitos y son lo suficientemente genéricas como para capturar efectos de los términos de orden superior, quizá propios de la teoría subyacente de Gravedad Cuántica. Primero, nos restringimos a teorías de gravedad pura y demostramos que todas las gravedades de orden superior se pueden escribir, mediante redefiniciones de campo perturbativas, como Gravedades Cuasitopológicas Generalizadas. En segundo lugar, añadimos un vector gauge U(1) e identificamos familias infinitas de Gravedades Electromagnéticas Cuasitopológicas (Generalizadas) (GEC(G)s). Establecemos diversas propiedades interesantes de estas teorías y exploramos las soluciones estáticas y esféricamente simétricas con carga. En particular, probamos que un subconjunto de las GECs admite agujeros negros con carga eléctrica completamente regulares para cualquier masa y carga no nula. A continuación, analizamos extensiones con derivadas superiores de la teoría de Einstein- Maxwell que son invariantes bajo dualidad. Clasificamos dichas teorías hasta octavo orden en derivadas y observamos que, hasta sexto orden, todas ellas se pueden reformular como una gravedad de orden superior con un vector acoplado mínimamente. Asimismo, somos capaces de clasificar todas las teorías exactamente invariantes bajo dualidad cuadráticas en el campo de Maxwell. Después, volvemos a las GECs y examinamos aspectos holográficos de las mismas. Logramos obtener resultados completamente analíticos y no perturbativos que nos ayudan a descubrir un nuevo resultado universal válido para todas las Teorías Conformes de Campos en dimensiones d 3, que demostramos rigurosamente. Por otro lado, estudiamos propiedades geométricas de la gravedad a altas energías. Elegimos Supergravedad y Teoría de Cuerdas como los escenarios en los que verificar estas propiedades y analizamos varias líneas de investigación, tratando de obtener una panorámica general del tipo de estructuras geométricas que podemos hallar en este contexto. Nos centramos primero en espinores reales paralelos en cuatro-variedades globalmente hiperbólicas, reformulando el problema en términos de un sistema de ecuaciones diferenciales para una familia de funciones y bases ortonormales del espacio cotangente en una superficie de Cauchy que denominamos flujo de espinor paralelo. Observamos que el flujo de Einstein y el de espinor paralelo coinciden en datos iniciales comunes, lo cual nos proporciona una caracterización de los datos iniciales de un espinor real paralelo en una cuatro-variedad globalmente hiperbólica Ricci plana. Luego, reorientamos nuestras pesquisas hacia las cuatro-variedades autoduales Einstein que admiten una acción isométrica y principal del grupo de Heisenberg tres-dimensional con órbitas no-degeneradas, logrando clasificar todas ellas. Finalmente, introducimos las estructuras de " -contacto, que además de englobar las nociones habituales de estructuras riemannianas y lorentzianas de contacto así como las estructuras métricas de para-contacto, incluyen la posibilidad de un vector de Reeb de tipo luz. Concluimos mostrando cómo se pueden emplear estas estructuras para la construcción de soluciones de Supergravedad en seis dimensiones
Published: 2022

19. La Búsqueda de Nueva Física: desde Supersimetría y Modelos de Sabor a los Análisis Basados en Datos con Técnicas de Machine Learning en el LHC

Author: Martín Ramiro, Pablo, Moreno Moreno, Jesús M., García Cerdeño, David, UAM. Departamento de Física Teórica, and Instituto de Física Teórica (IFT)
Subjects: Supersimetría, Modelo estándar, Física, Materia oscura
Abstract: Tesis doctoral inédita leída en la Universidad Autónoma de Madrid, Facultad de Ciencias, Departamento de Física Teórica. Fecha de lectura: 21-01-2022
Published: 2022

20. Pushing the limits of the Swampland distance conjeture

Author: Calderón Infante, José, Uranga Urteaga, Angel M., UAM. Departamento de Física Teórica, and Instituto de Física Teórica (IFT)
Subjects: Cuerdas, Teoría de las, Teoría cuántica-Programas, Gravedad cuántica, Física
Abstract: Tesis Doctoral inédita leída en la Universidad Autónoma de Madrid, Facultad de Ciencias, Departamento de Física Teórica. Fecha de Lectura: 16-09-2022
Published: 2022

21. Sensitivity of the Cherenkov Telescope Array to a dark matter signal from the Galactic centre

Author: Abdalla, H., Abe, H., Abe, S., Abusleme, A., Acero, F., Acharyya, A., Acín Portella, V., Ackley, K., Adam, R., Adams, C., Adhikari, S. S., Aguado-Ruesga, I., Agudo, I., Aguilera, R., Aguirre-Santaella, A., Aharonian, F., Alberdi, A., Alfaro, R., Alfaro, J., Alispach, C., Aloisio, R., Alves Batista, R., Amans, J. -P, Amati, L., Amato, E., Ambrogi, L., Ambrosi, G., Ambrosio, M., Ammendola, R., Anderson, J., Anduze, M., Angüner, E. O., Antonelli, L. A., Antonuccio, V., Antoranz, P., Anutarawiramkul, R., Aragunde Gutierrez, J., Aramo, C., Araudo, A., Araya, M., Arbet-Engels, A., Arcaro, C., Arendt, V., Armand, C., Armstrong, T., Arqueros, F., Arrabito, L., Arsioli, B., Artero, M., Asano, K., Ascasíbar, Y., Aschersleben, J., Ashley, M., Attinà, P., Aubert, P., Singh, C. B., Baack, D., Babic, A., Backes, M., Baena, V., Bajtlik, S., Baktash, A., Balazs, C., Balbo, M., Ballester, O., Ballet, J., Balmaverde, B., Bamba, A., Bandiera, R., Baquero Larriva, A., Barai, P., Barbier, C., Barbosa Martins, V., Barcelo, M., Barkov, M., Barnard, M., Baroncelli, L., Barres Almeida, U., Barrio, J. A., Bastieri, D., Batista, P. I., Batkovic, I., Bauer, C., Bautista-González, R., Baxter, J., Becciani, U., Becerra González, J., Becherini, Y., Beck, G., Becker Tjus, J., Bednarek, W., Belfiore, A., Bellizzi, L., Belmont, R., Benbow, W., Berge, D., Bernardini, E., Bernardos, M. I., Bernlöhr, K., Berti, A., Berton, M., Bertucci, B., Beshley, V., Bhatt, N., Bhattacharyya, S., Bhattacharyya, W., Bi, B., Bicknell, G., Biederbeck, N., Bigongiari, C., Biland, A., Bird, R., Bissaldi, E., Biteau, J., Bitossi, M., Blanch, O., Blank, M., Blazek, J., Bobin, J., Boccato, C., Bocchino, F., Boehm, C., Bohacova, M., Boisson, C., Boix, J., Bolle, J. -P, Bolmont, J., Bonanno, G., Bonavolontà, C., Bonneau Arbeletche, L., Bonnoli, G., Bordas, P., Borkowski, J., Bórquez, S., Bose, R., Bose, D., Bosnjak, Z., Bottacini, E., Böttcher, M., Botticella, M. T., Boutonnet, C., Bouyjou, F., Bozhilov, V., Bozzo, E., Brahimi, L., Braiding, C., Brau-Nogué, S., Breen, S., Bregeon, J., Breuhaus, M., Brill, A., Brisken, W., Brocato, E., Brown, A. M., Brügge, K., Brun, P., Brun, F., Brunetti, L., Brunetti, G., Bruno, P., Bruno, A., Bruzzese, A., Bucciantini, N., Buckley, J., Bühler, R., Bulgarelli, A., Bulik, T., Bünning, M., Bunse, M., Burton, M., Burtovoi, A., Buscemi, M., Buschjäger, S., Busetto, G., Buss, J., Byrum, K., Caccianiga, A., Cadoux, F., Calanducci, A., Calderón, C., Calvo Tovar, J., Cameron, R., Campaña, P., Canestrari, R., Cangemi, F., Cantlay, B., Capalbi, M., Capasso, M., Cappi, M., Caproni, A., Capuzzo-Dolcetta, R., Caraveo, P., Cárdenas, V., Cardiel, L., Cardillo, M., Carlile, C., Caroff, S., Carosi, R., Carosi, A., Carquín, E., Carrère, M., Casandjian, J. -M, Casanova, S., Cascone, E., Cassol, F., Castro-Tirado, A. J., Catalani, F., Catalano, O., Cauz, D., Ceccanti, A., Celestino Silva, C., Celli, S., Cerny, K., Cerruti, M., Chabanne, E., Chadwick, P., Chai, Y., Chambery, P., Champion, C., Chandra, S., Chaty, S., Chen, A., Cheng, K., Chernyakova, M., Chiaro, G., Chiavassa, A., Chikawa, M., Chitnis, V. R., Chudoba, J., Chytka, L., Cikota, S., Circiello, A., Clark, P., Çolak, M., Colombo, E., Colome, J., Colonges, S., Comastri, A., Compagnino, A., Conforti, V., Congiu, E., Coniglione, R., Conrad, J., Conte, F., Contreras, J. L., Coppi, P., Cornat, R., Coronado-Blazquez, J., Cortina, J., Costa, A., Costantini, H., Cotter, G., Courty, B., Covino, S., Crestan, S., Cristofari, P., Crocker, R., Croston, J., Cubuk, K., Cuevas, O., Cui, X., Cusumano, G., Cutini, S., D’aì, A., D’amico, G., D’ammando, F., D’avanzo, P., Da Vela, P., Dadina, M., Dai, S., Dalchenko, M., Dall’ Ora, M., Daniel, M. K., Dauguet, J., Davids, I., Davies, J., Dawson, B., Angelis, A., Araújo Carvalho, A. E., Bony Lavergne, M., Caprio, V., Cesare, G., Frondat, F., Gouveia Dal Pino, E. M., La Calle, I., Lotto, B., Luca, A., Martino, D., Menezes, R. M., Naurois, M., Oña Wilhelmi, E., Palma, F., Persio, F., Simone, N., Souza, V., Del Santo, M., Del Valle, M. V., Delagnes, E., Deleglise, G., Delfino Reznicek, M., Delgado, C., Delgado Giler, A. G., Delgado Mengual, J., Della Ceca, R., Della Valle, M., Della Volpe, D., Depaoli, D., Depouez, D., Devin, J., Di Girolamo, T., Di Giulio, C., Di Piano, A., Di Pierro, F., Di Venere, L., Díaz, C., Díaz-Bahamondes, C., Dib, C., Diebold, S., Digel, S., Dima, R., Djannati-Ataï, A., Djuvsland, J., Dmytriiev, A., Docher, K., Domínguez, A., Dominis Prester, D., Donath, A., Donini, A., Dorner, D., Doro, M., Dos Anjos, R. D. C., Dournaux, J. -L, Downes, T., Drake, G., Drass, H., Dravins, D., Duangchan, C., Duara, A., Dubus, G., Ducci, L., Duffy, C., Dumora, D., Dundas Morå, K., Durkalec, A., Dwarkadas, V. V., Ebr, J., Eckner, C., Eder, J., Ederoclite, A., Edy, E., Egberts, K., Einecke, S., Eisch, J., Eleftheriadis, C., Elsässer, D., Emery, G., Emmanoulopoulos, D., Ernenwein, J. -P, Errando, M., Escarate, P., Escudero, J., Espinoza, C., Ettori, S., Eungwanichayapant, A., Evans, P., Evoli, C., Fairbairn, M., Falceta-Goncalves, D., Falcone, A., Fallah Ramazani, V., Falomo, R., Farakos, K., Fasola, G., Fattorini, A., Favre, Y., Fedora, R., Fedorova, E., Fegan, S., Feijen, K., Feng, Q., Ferrand, G., Ferrara, G., Ferreira, O., Fesquet, M., Fiandrini, E., Fiasson, A., Filipovic, M., Fink, D., Finley, J. P., Fioretti, V., Fiorillo, D. F. G., Fiorini, M., Flis, S., Flores, H., Foffano, L., Föhr, C., Fonseca, M. V., Font, L., Fontaine, G., Fornieri, O., Fortin, P., Fortson, L., Fouque, N., Fournier, A., Fraga, B., Franceschini, A., Franco, F. J., Franco Ordovas, A., Freixas Coromina, L., Fresnillo, L., Fruck, C., Fugazza, D., Fujikawa, Y., Fujita, Y., Fukami, S., Fukazawa, Y., Fukui, Y., Fulla, D., Funk, S., Furniss, A., Gabella, O., Gabici, S., Gaggero, D., Galanti, G., Galaz, G., Galdemard, P., Gallant, Y., Galloway, D., Gallozzi, S., Gammaldi, V., Garcia, R., Garcia, E., García, E., Garcia López, R., Garczarczyk, M., Gargano, F., Gargano, C., Garozzo, S., Gascon, D., Gasparetto, T., Gasparrini, D., Gasparyan, H., Gaug, M., Geffroy, N., Gent, A., Germani, S., Gesa, L., Ghalumyan, A., Ghedina, A., Ghirlanda, G., Gianotti, F., Giarrusso, S., Giarrusso, M., Giavitto, G., Giebels, B., Giglietto, N., Gika, V., Gillardo, F., Gimenes, R., Giordano, F., Giovannini, G., Giro, E., Giroletti, M., Giuliani, A., Giunti, L., Gjaja, M., Glicenstein, J. -F, Gliwny, P., Godinovic, N., Göksu, H., Goldoni, P., Gómez, J. L., Gómez-Vargas, G., González, M. M., González, J. M., Gothe, K. S., Götz, D., Goulart Coelho, J., Gourgouliatos, K., Grabarczyk, T., Graciani, R., Grandi, P., Grasseau, G., Grasso, D., Green, A. J., Green, D., Green, J., Greenshaw, T., Grenier, I., Grespan, P., Grillo, A., Grondin, M. -H, Grube, J., Guarino, V., Guest, B., Gueta, O., Gündüz, M., Gunji, S., Gusdorf, A., Gyuk, G., Hackfeld, J., Hadasch, D., Haga, J., Hagge, L., Hahn, A., Hajlaoui, J. E., Hakobyan, H., Halim, A., Hamal, P., Hanlon, W., Hara, S., Harada, Y., Hardcastle, M. J., Harvey, M., Hashiyama, K., Hassan Collado, T., Haubold, T., Haupt, A., Hautmann, U. A., Havelka, M., Hayashi, K., Hayashida, M., He, H., Heckmann, L., Heller, M., Helo, J. C., Henault, F., Henri, G., Hermann, G., Hermel, R., Hernández Cadena, S., Herrera Llorente, J., Herrero, A., Hervet, O., Hinton, J., Hiramatsu, A., Hiroshima, N., Hirotani, K., Hnatyk, B., Hnatyk, R., Hoang, J. K., Hoffmann, D., Hofmann, W., Hoischen, C., Holder, J., Holler, M., Hona, B., Horan, D., Hörandel, J., Horns, D., Horvath, P., Houles, J., Hovatta, T., Hrabovsky, M., Hrupec, D., Huang, Y., Huet, J. -M, Hughes, G., Hui, D., Hull, G., Humensky, T. B., Hütten, M., Iaria, R., Iarlori, M., Illa, J. M., Imazawa, R., Impiombato, D., Inada, T., Incardona, F., Ingallinera, A., Inome, Y., Inoue, S., Inoue, T., Inoue, Y., Insolia, A., Iocco, F., Ioka, K., Ionica, M., Iori, M., Iovenitti, S., Iriarte, A., Ishio, K., Ishizaki, W., Iwamura, Y., Jablonski, C., Jacquemier, J., Jacquemont, M., Jamrozy, M., Janecek, P., Jankowsky, F., Jardin-Blicq, A., Jarnot, C., Jean, P., Jiménez Martínez, I., Jin, W., Jocou, L., Jordana, N., Josselin, M., Jouvin, L., Jung-Richardt, I., Junqueira, F. J. P. A., Juramy-Gilles, C., Jurysek, J., Kaaret, P., Kadowaki, L. H. S., Kagaya, M., Kalekin, O., Kankanyan, R., Kantzas, D., Karas, V., Karastergiou, A., Karkar, S., Kasai, E., Kasperek, J., Katagiri, H., Kataoka, J., Katarzyński, K., Katsuda, S., Katz, U., Kawanaka, N., Kazanas, D., Kerszberg, D., Khélifi, B., Kherlakian, M. C., Kian, T. P., Kieda, D. B., Kihm, T., Kim, S., Kimeswenger, S., Kisaka, S., Kissmann, R., Kleijwegt, R., Kleiner, T., Kluge, G., Kluźniak, W., Knapp, J., Knödlseder, J., Kobakhidze, A., Kobayashi, Y., Koch, B., Kocot, J., Kohri, K., Kokkotas, K., Komin, N., Kong, A., Kosack, K., Kowal, G., Krack, F., Krause, M., Krennrich, F., Krumholz, M., Kubo, H., Kudryavtsev, V., Kunwar, S., Kuroda, Y., Kushida, J., Kushwaha, P., La Barbera, A., La Palombara, N., La Parola, V., La Rosa, G., Lahmann, R., Lamanna, G., Lamastra, A., Landoni, M., Landriu, D., Lang, R. G., Lapington, J., Laporte, P., Lason, P., Lasuik, J., Lazendic-Galloway, J., Le Flour, T., Le Sidaner, P., Leach, S., Leckngam, A., Lee, S. -H, Lee, W. H., Lee, S., Leigui Oliveira, M. A., Lemière, A., Lemoine-Goumard, M., Lenain, J. -P, Leone, F., Leray, V., Leto, G., Leuschner, F., Levy, C., Lindemann, R., Lindfors, E., Linhoff, L., Liodakis, I., Lipniacka, A., Lloyd, S., Lobo, M., Lohse, T., Lombardi, S., Longo, F., Lopez, A., López, M., López-Coto, R., Loporchio, S., Louis, F., Louys, M., Lucarelli, F., Lucchesi, D., Ludwig Boudi, H., Luque-Escamilla, P. L., Lyard, E., Maccarone, M. C., Maccarone, T., Mach, E., Maciejewski, A. J., Mackey, J., Madejski, G. M., Maeght, P., Maggio, C., Maier, G., Majczyna, A., Majumdar, P., Makariev, M., Mallamaci, M., Malta Nunes Almeida, R., Maltezos, S., Malyshev, D., Mandat, D., Maneva, G., Manganaro, M., Manicò, G., Manigot, P., Mannheim, K., Maragos, N., Marano, D., Marconi, M., Marcowith, A., Marculewicz, M., Marčun, B., Marín, J., Marinello, N., Marinos, P., Mariotti, M., Markoff, S., Marquez, P., Marsella, G., Martí, J., Martin, J. -M, Martin, P., Martinez, O., Martínez, M., Martínez, G., Martínez, O., Martínez-Huerta, H., Marty, C., Marx, R., Masetti, N., Massimino, P., Mastichiadis, A., Matsumoto, H., Matthews, N., Maurin, G., Max-Moerbeck, W., Maxted, N., Mazin, D., Mazziotta, M. N., Mazzola, S. M., Mbarubucyeye, J. D., Mc Comb, L., Mchardy, I., Mckeague, S., Mcmuldroch, S., Medina, E., Medina Miranda, D., Melandri, A., Melioli, C., Melkumyan, D., Menchiari, S., Mender, S., Mereghetti, S., Merino Arévalo, G., Mestre, E., Meunier, J. -L, Meures, T., Meyer, M., Micanovic, S., Miceli, M., Michailidis, M., Michałowski, J., Miener, T., Mievre, I., Miller, J., Minaya, I. A., Mineo, T., Minev, M., Miranda, J. M., Mirzoyan, R., Mitchell, A., Mizuno, T., Mode, B., Moderski, R., Mohrmann, L., Molina, E., Molinari, E., Teresa Montaruli, Monteiro, I., Moore, C., Moralejo, A., Morcuende-Parrilla, D., Moretti, E., Morganti, L., Mori, K., Moriarty, P., Morik, K., Morlino, G., Morris, P., Morselli, A., Mosshammer, K., Moya, P., Mukherjee, R., Muller, J., Mundell, C., Mundet, J., Murach, T., Muraczewski, A., Muraishi, H., Murase, K., Musella, I., Musumarra, A., Nagai, A., Nagar, N., Nagataki, S., Naito, T., Nakamori, T., Nakashima, K., Nakayama, K., Nakhjiri, N., Naletto, G., Naumann, D., Nava, L., Navarro, R., Nawaz, M. A., Ndiyavala, H., Neise, D., Nellen, L., Nemmen, R., Newbold, M., Neyroud, N., Ngernphat, K., Nguyen Trung, T., Nicastro, L., Nickel, L., Niemiec, J., Nieto, D., Nievas, M., Nigro, C., Nikołajuk, M., Ninci, D., Nishijima, K., Noda, K., Nogami, Y., Nolan, S., Nomura, R., Norris, R., Nosek, D., Nöthe, M., Novosyadlyj, B., Novotny, V., Nozaki, S., Nunio, F., O’brien, P., Obara, K., Oger, R., Ohira, Y., Ohishi, M., Ohm, S., Ohtani, Y., Oka, T., Okazaki, N., Okumura, A., Olive, J. -F, Oliver, C., Olivera, G., Olmi, B., Ong, R. A., Orienti, M., Orito, R., Orlandini, M., Orlando, S., Orlando, E., Osborne, J. P., Ostrowski, M., Otte, N., Ovcharov, E., Owen, E., Oya, I., Ozieblo, A., Padovani, M., Pagano, I., Pagliaro, A., Paizis, A., Palatiello, M., Palatka, M., Palazzi, E., Panazol, J. -L, Paneque, D., Panes, B., Panny, S., Pantaleo, F. R., Panter, M., Paoletti, R., Paolillo, M., Papitto, A., Paravac, A., Paredes, J. M., Pareschi, G., Park, N., Parmiggiani, N., Parsons, R. 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B., H??tten, M., Iarlori, M., Inada, T., Inoue, S., Iocco, F., Iori, M., Jamrozy, M., Janecek, P., Jin, W., Jouvin, L., Jurysek, J., Karukes, E., Katarzy??ski, K., Kazanas, D., Kerszberg, D., Kherlakian, M. C., Kissmann, R., Kn??dlseder, J., Kobayashi, Y., Kohri, K., Komin, N., Kubo, H., Kushida, J., Lamanna, G., Lapington, J., Laporte, P., Leigui de Oliveira, M. A., Lenain, J., Leone, F., Leto, G., Lindfors, E., Lohse, T., Lombardi, S., Longo, F., Lopez, A., L??pez, M., L??pez-Coto, R., Loporchio, S., Luque-Escamilla, P. L., Mach, E., Maggio, C., Maier, G., Mallamaci, M., Malta Nunes de Almeida, R., Mandat, D., Manganaro, M., Mangano, S., Manic??, G., Marculewicz, M., Mariotti, M., Markoff, S., Marquez, P., Mart??, J., Martinez, O., Mart??nez, M., Mart??nez, G., Mart??nez-Huerta, H., Maurin, G., Mazin, D., Mbarubucyeye, J. D., Medina Miranda, D., Meyer, M., Miceli, M., Miener, T., Minev, M., Miranda, J. M., Mirzoyan, R., Mizuno, T., Mode, B., Moderski, R., Mohrmann, L., Molina, E., Montaruli, T., Moralejo, A., Morcuende-Parrilla, D., Morselli, A., Mukherjee, R., Mundell, C., Nagai, A., Nakamori, T., Nemmen, R., Niemiec, J., Nieto, D., Niko??ajuk, M., Ninci, D., Noda, K., Nosek, D., Nozaki, S., Ohira, Y., Ohishi, M., Ohtani, Y., Oka, T., Okumura, A., Ong, R. A., Orienti, M., Orito, R., Orlandini, M., Orlando, S., Orlando, E., Ostrowski, M., Oya, I., Pagano, I., Pagliaro, A., Palatiello, M., Pantaleo, F. R., Paredes, J. M., Pareschi, G., Parmiggiani, N., Patricelli, B., Pavleti??, L., Pe'Er, A., Pecimotika, M., P??rez-Romero, J., Persic, M., Petruk, O., Pfrang, K., Piano, G., Piatteli, P., Pietropaolo, E., Pillera, R., Pilszyk, B., Pintore, F., Pohl, M., Poireau, V., Prado, R. R., Prandini, E., Prast, J., Principe, G., Prokoph, H., Prouza, M., Przybilski, H., P??hlhofer, G., Pumo, M. L., Queiroz, F., Quirrenbach, A., Rain??, S., Rando, R., Razzaque, S., Recchia, S., Reimer, O., Reisenegger, A., Renier, Y., Rhode, W., Ribeiro, D., Rib??, M., Richtler, T., Rico, J., Rieger, F., Rinchiuso, L., Rizi, V., Rodriguez, J., Rodriguez Fernandez, G., Rodriguez Ramirez, J. C., Rojas, G., Romano, P., Romeo, G., Rosado, J., Rowell, G., Rudak, B., Russo, F., Sadeh, I., S??ther Hatlen, E., Safi-Harb, S., Salesa Greus, F., Salina, G., Sanchez, D., S??nchez-Conde, M., Sangiorgi, P., Sano, H., Santander, M., Santos, E. M., Santos-Lima, R., Sanuy, A., Sarkar, S., Saturni, F. G., Sawangwit, U., Schussler, F., Schwanke, U., Sciacca, E., Scuderi, S., Seglar-Arroyo, M., Sergijenko, O., Servillat, M., Seweryn, K., Shalchi, A., Sharma, P., Shellard, R. C., Siejkowski, H., Silk, J., Siqueira, C., Sliusar, V., S??owikowska, A., Sokolenko, A., Sol, H., Spencer, S., Stamerra, A., Stani??, S., Starling, R., Stolarczyk, T., Straumann, U., Stri??kovi??, J., Suda, Y., Suomijarvi, T., wierk, P., Tavecchio, F., Taylor, L., Tejedor, L. A., Teshima, M., Testa, V., Tibaldo, L., Todero Peixoto, C. J., Tokanai, F., Tonev, D., Tosti, G., Tosti, L., Tothill, N., Truzzi, S., Travnicek, P., Vagelli, V., Vallage, B., Vallania, P., van Eldik, C., Vandenbroucke, J., Varner, G. S., Vassiliev, V., V??zquez Acosta, M., Vecchi, M., Ventura, S., Vercellone, S., Vergani, S., Verna, G., Viana, A., Vigorito, C. F., Vink, J., Vitale, V., Vorobiov, S., Vovk, I., Vuillaume, T., Wagner, S. J., Walter, R., Watson, J., Weniger, C., White, R., White, M., Wiemann, R., Wierzcholska, A., Will, M., Williams, D. A., Wischnewski, R., Yanagita, S., Yang, L., Yoshikoshi, T., Zacharias, M., Zaharijas, G., Zakaria, A. A., Zampieri, L., Zanin, R., Zaric, D., Zavrtanik, M., Zavrtanik, D., Zdziarski, A. A., Zech, A., Zechlin, H., Zhdanov, V. I., ivec, M., ITA, USA, GBR, FRA, DEU, ESP, AUT, BEL, BRA, HRV, DNK, JPN, IRL, NLD, POL, SVN, CHE, High Energy Astrophys. & Astropart. Phys (API, FNWI), GRAPPA (ITFA, IoP, FNWI), Centre National de la Recherche Scientifique (CNRS)-École polytechnique (X)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Diderot - Paris 7 (UPD7), Université Montpellier 2 - Sciences et Techniques (UM2)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université de Montpellier (UM)-Centre National de la Recherche Scientifique (CNRS), Astrophysique Interprétation Modélisation (AIM (UMR_7158 / UMR_E_9005 / UM_112)), Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Institut national des sciences de l'Univers (INSU - CNRS)-Université Toulouse III - Paul Sabatier (UT3), Université Fédérale Toulouse Midi-Pyrénées-Université Fédérale Toulouse Midi-Pyrénées-Observatoire Midi-Pyrénées (OMP), Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Centre National de la Recherche Scientifique (CNRS), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Iocco, Fabio, Anguner, E. O., Ascasibar, Y., Bernlohr, K., Colak, M., D'Ai, A., de Angelis, A., de Caprio, V., de Cassia dos Anjos, R., de Lotto, B., de Martino, D., de Ona Wilhelmi, E., de Palma, F., Dominguez, A., Elsasser, D., Gonzalez, M. M., Hernandez Cadena, S., Horandel, J., Hutten, M., Katarzynski, K., Knodlseder, J., Lopez, M., Lopez-Coto, R., Manico, G., Marti, J., Martinez, M., Martinez, G., Martinez-Huerta, H., Nikolajuk, M., Pavletic, L., Perez-Romero, J., Puhlhofer, G., Raino, S., Ribo, M., Saether Hatlen, E., Sanchez-Conde, M., Slowikowska, A., Stanic, S., Striskovic, J., Swierk, P., Vazquez Acosta, M., Zivec, M., Consortium, The CTA, Acharyya A., Adam R., Adams C., Agudo I., Aguirre-Santaella A., Alfaro R., Alfaro J., Alispach C., Aloisio R., Alves Batista R., Amati L., Ambrosi G., Anguner E.O., Antonelli L.A., Aramo C., Araudo A., Armstrong T., Arqueros F., Asano K., Ascasibar Y., Ashley M., Balazs C., Ballester O., Baquero Larriva A., Barbosa Martins V., Barkov M., Barres de Almeida U., Barrio J.A., Bastieri D., Becerra J., Beck G., Becker Tjus J., Benbow W., Benito M., Berge D., Bernardini E., Bernlohr K., Berti A., Bertucci B., Beshley V., Biasuzzi B., Biland A., Bissaldi E., Biteau J., Blanch O., Blazek J., Bocchino F., Boisson C., Bonneau Arbeletche L., Bordas P., Bosnjak Z., Bottacini E., Bozhilov V., Bregeon J., Brill A., Bringmann T., Brown A.M., Brun P., Brun F., Bruno P., Bulgarelli A., Burton M., Burtovoi A., Buscemi M., Cameron R., Capasso M., Caproni A., Capuzzo-Dolcetta R., Caraveo P., Carosi R., Carosi A., Casanova S., Cascone E., Cassol F., Catalani F., Cauz D., Cerruti M., Chadwick P., Chaty S., Chen A., Chernyakova M., Chiaro G., Chiavassa A., Chikawa M., Chudoba J., Colak M., Conforti V., Coniglione R., Conte F., Contreras J.L., Coronado-Blazquez J., Costa A., Costantini H., Cotter G., Cristofari P., D'Ai A., D'Ammando F., Damone L.A., Daniel M.K., Dazzi F., de Angelis A., de Caprio V., de Cassia dos Anjos R., de Gouveia Dal Pino E.M., de Lotto B., de Martino D., de Ona Wilhelmi E., de Palma F., de Souza V., Delgado C., Delgado Giler A.G., della Volpe D., Depaoli D., Di Girolamo T., Di Pierro F., Di Venere L., Diebold S., Dmytriiev A., Dominguez A., Donini A., Doro M., Ebr J., Eckner C., Edwards T.D.P., Ekoume T.R.N., Elsasser D., Evoli C., Falceta-Goncalves D., Fedorova E., Fegan S., Feng Q., Ferrand G., Ferrara G., Fiandrini E., Fiasson A., Filipovic M., Fioretti V., Fiori M., Foffano L., Fontaine G., Fornieri O., Franco F.J., Fukami S., Fukui Y., Gaggero D., Galaz G., Gammaldi V., Garcia E., Garczarczyk M., Gascon D., Gent A., Ghalumyan A., Gianotti F., Giarrusso M., Giavitto G., Giglietto N., Giordano F., Giuliani A., Glicenstein J., Gnatyk R., Goldoni P., Gonzalez M.M., Gourgouliatos K., Granot J., Grasso D., Green J., Grillo A., Gueta O., Gunji S., Halim A., Hassan T., Heller M., Hernandez Cadena S., Hiroshima N., Hnatyk B., Hofmann W., Holder J., Horan D., Horandel J., Horvath P., Hovatta T., Hrabovsky M., Hrupec D., Hughes G., Humensky T.B., Hutten M., Iarlori M., Inada T., Inoue S., Iocco F., Iori M., Jamrozy M., Janecek P., Jin W., Jouvin L., Jurysek J., Karukes E., Katarzynski K., Kazanas D., Kerszberg D., Kherlakian M.C., Kissmann R., Knodlseder J., Kobayashi Y., Kohri K., Komin N., Kubo H., Kushida J., Lamanna G., Lapington J., Laporte P., Leigui de Oliveira M.A., Lenain J., Leone F., Leto G., Lindfors E., Lohse T., Lombardi S., Longo F., Lopez A., Lopez M., Lopez-Coto R., Loporchio S., Luque-Escamilla P.L., Mach E., Maggio C., Maier G., Mallamaci M., Malta Nunes de Almeida R., Mandat D., Manganaro M., Mangano S., Manico G., Marculewicz M., Mariotti M., Markoff S., Marquez P., Marti J., Martinez O., Martinez M., Martinez G., Martinez-Huerta H., Maurin G., Mazin D., Mbarubucyeye J.D., Medina Miranda D., Meyer M., Miceli M., Miener T., Minev M., Miranda J.M., Mirzoyan R., Mizuno T., Mode B., Moderski R., Mohrmann L., Molina E., Montaruli T., Moralejo A., Morcuende-Parrilla D., Morselli A., Mukherjee R., Mundell C., Nagai A., Nakamori T., Nemmen R., Niemiec J., Nieto D., Nikolajuk M., Ninci D., Noda K., Nosek D., Nozaki S., Ohira Y., Ohishi M., Ohtani Y., Oka T., Okumura A., Ong R.A., Orienti M., Orito R., Orlandini M., Orlando S., Orlando E., Ostrowski M., Oya I., Pagano I., Pagliaro A., Palatiello M., Pantaleo F.R., Paredes J.M., Pareschi G., Parmiggiani N., Patricelli B., Pavletic L., Pe'Er A., Pecimotika M., Perez-Romero J., Persic M., Petruk O., Pfrang K., Piano G., Piatteli P., Pietropaolo E., Pillera R., Pilszyk B., Pintore F., Pohl M., Poireau V., Prado R.R., Prandini E., Prast J., Principe G., Prokoph H., Prouza M., Przybilski H., Puhlhofer G., Pumo M.L., Queiroz F., Quirrenbach A., Raino S., Rando R., Razzaque S., Recchia S., Reimer O., Reisenegger A., Renier Y., Rhode W., Ribeiro D., Ribo M., Richtler T., Rico J., Rieger F., Rinchiuso L., Rizi V., Rodriguez J., Rodriguez Fernandez G., Rodriguez Ramirez J.C., Rojas G., Romano P., Romeo G., Rosado J., Rowell G., Rudak B., Russo F., Sadeh I., Saether Hatlen E., Safi-Harb S., Salesa Greus F., Salina G., Sanchez D., Sanchez-Conde M., Sangiorgi P., Sano H., Santander M., Santos E.M., Santos-Lima R., Sanuy A., Sarkar S., Saturni F.G., Sawangwit U., Schussler F., Schwanke U., Sciacca E., Scuderi S., Seglar-Arroyo M., Sergijenko O., Servillat M., Seweryn K., Shalchi A., Sharma P., Shellard R.C., Siejkowski H., Silk J., Siqueira C., Sliusar V., Slowikowska A., Sokolenko A., Sol H., Spencer S., Stamerra A., Stanic S., Starling R., Stolarczyk T., Straumann U., Striskovic J., Suda Y., Suomijarvi T., Swierk P., Tavecchio F., Taylor L., Tejedor L.A., Teshima M., Testa V., Tibaldo L., Todero Peixoto C.J., Tokanai F., Tonev D., Tosti G., Tosti L., Tothill N., Truzzi S., Travnicek P., Vagelli V., Vallage B., Vallania P., van Eldik C., Vandenbroucke J., Varner G.S., Vassiliev V., Vazquez Acosta M., Vecchi M., Ventura S., Vercellone S., Vergani S., Verna G., Viana A., Vigorito C.F., Vink J., Vitale V., Vorobiov S., Vovk I., Vuillaume T., Wagner S.J., Walter R., Watson J., Weniger C., White R., White M., Wiemann R., Wierzcholska A., Will M., Williams D.A., Wischnewski R., Yanagita S., Yang L., Yoshikoshi T., Zacharias M., Zaharijas G., Zakaria A.A., Zampieri L., Zanin R., Zaric D., Zavrtanik M., Zavrtanik D., Zdziarski A.A., Zech A., Zechlin H., Zhdanov V.I., and Zivec M.
Subjects: Cherenkov Telescope Array, MATÉRIA ESCURA, scale: TeV, Astronomy, atmosphere [Cherenkov counter], dark matter experiment, Dark matter theory, energy resolution, Gamma ray experiments, Particle, Astrophysics, cosmic background radiation, 01 natural sciences, 7. Clean energy, High Energy Physics - Phenomenology (hep-ph), benchmark, WIMP, HESS, energy: flux, TeV [scale], relativistic [charged particle], gamma ray experiment, MAGIC (telescope), Monte Carlo, Event reconstruction, Physics, High Energy Astrophysical Phenomena (astro-ph.HE), Contraction, spatial distribution, track data analysis, density [dark matter], Clumpy, Astrophysics::Instrumentation and Methods for Astrophysics, imaging, High Energy Physics - Phenomenology, dark matter experiments, dark matter theory, gamma ray experiments, galaxy morphology, Dark matter experiments, Física nuclear, VERITAS, Astrophysics - High Energy Astrophysical Phenomena, Simulations, noise, Astrophysics::High Energy Astrophysical Phenomena, Dark matter, satellite, Cosmic background radiation, FOS: Physical sciences, Annihilation, dark matter: density, Astrophysics::Cosmology and Extragalactic Astrophysics, Cherenkov counter: atmosphere, heavy [dark matter], annihilation [dark matter], GLAST, Galaxy morphology, cosmic radiation [p], 0103 physical sciences, Cherenkov [radiation], Candidates, ddc:530, AGN, Cherenkov radiation, Radiative Processes, thermal [cross section], 010308 nuclear & particles physics, Física, dark matter: annihilation, Gamma-Ray Signals, dark matter, Galactic Center, TeV gamma-ray astronomy, Astronomy and Astrophysics, Mass, radiation: Cherenkov, sensitivity, MAGIC, Galaxy, Astronomía, dark matter: heavy, gamma ray, p: cosmic radiation, [PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph], correlation, charged particle: relativistic, flux [energy], galaxy, supersymmetry, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], cross section: thermal
Abstract: Full list of authors: Acharyya, A.; Adam, R.; Adams, C.; Agudo, I.; Aguirre-Santaella, A.; Alfaro, R.; Alfaro, J.; Alispach, C.; Aloisio, R.; Alves Batista, R.; Amati, L.; Ambrosi, G.; Angüner, E. O.; Antonelli, L. A.; Aramo, C.; Araudo, A.; Armstrong, T.; Arqueros, F.; Asano, K.; Ascasíbar, Y. Ashley, M.; Balazs, C.; Ballester, O.; Baquero Larriva, A.; Barbosa Martins, V.; Barkov, M.; Barres de Almeida, U.; Barrio, J. A.; Bastieri, D.; Becerra, J.; Beck, G.; Becker Tjus, J.; Benbow, W.; Benito, M.; Berge, D.; Bernardini, E.; Bernlöhr, K.; Berti, A.; Bertucci, B.; Beshley, V.; Biasuzzi, B.; Biland, A.; Bissaldi, E.; Biteau, J.; Blanch, O.; Blazek, J.; Bocchino, F.; Boisson, C.; Bonneau Arbeletche, L.; Bordas, P.; Bosnjak, Z.; Bottacini, E.; Bozhilov, V.; Bregeon, J.; Brill, A.; Bringmann, T.; Brown, A. M.; Brun, P.; Brun, F.; Bruno, P.; Bulgarelli, A.; Burton, M.; Burtovoi, A.; Buscemi, M.; Cameron, R.; Capasso, M.; Caproni, A.; Capuzzo-Dolcetta, R.; Caraveo, P.; Carosi, R.; Carosi, A.; Casanova, S.; Cascone, E.; Cassol, F.; Catalani, F.; Cauz, D.; Cerruti, M.; Chadwick, P.; Chaty, S.; Chen, A.; Chernyakova, M.; Chiaro, G.; Chiavassa, A.; Chikawa, M.; Chudoba, J.; Çolak, M.; Conforti, V.; Coniglione, R.; Conte, F.; Contreras, J. L.; Coronado-Blazquez, J.; Costa, A.; Costantini, H.; Cotter, G.; Cristofari, P.; D'Aimath, A.; D'Ammando, F.; Damone, L. A.; Daniel, M. K.; Dazzi, F.; De Angelis, A.; De Caprio, V.; de Cássia dos Anjos, R.; de Gouveia Dal Pino, E. M.; De Lotto, B.; De Martino, D.; de Oña Wilhelmi, E.; De Palma, F.; de Souza, V.; Delgado, C.; Delgado Giler, A. G.; della Volpe, D.; Depaoli, D.; Di Girolamo, T.; Di Pierro, F.; Di Venere, L.; Diebold, S.; Dmytriiev, A.; Domínguez, A.; Donini, A.; Doro, M.; Ebr, J.; Eckner, C.; Edwards, T. D. P.; Ekoume, T. R. N.; Elsässer, D.; Evoli, C.; Falceta-Goncalves, D.; Fedorova, E.; Fegan, S.; Feng, Q.; Ferrand, G.; Ferrara, G.; Fiandrini, E.; Fiasson, A.; Filipovic, M.; Fioretti, V.; Fiori, M.; Foffano, L.; Fontaine, G.; Fornieri, O.; Franco, F. J.; Fukami, S.; Fukui, Y.; Gaggero, D.; Galaz, G.; Gammaldi, V.; Garcia, E.; Garczarczyk, M.; Gascon, D.; Gent, A.; Ghalumyan, A.; Gianotti, F.; Giarrusso, M.; Giavitto, G.; Giglietto, N.; Giordano, F.; Giuliani, A.; Glicenstein, J.; Gnatyk, R.; Goldoni, P.; González, M. M.; Gourgouliatos, K.; Granot, J.; Grasso, D.; Green, J.; Grillo, A.; Gueta, O.; Gunji, S.; Halim, A.; Hassan, T.; Heller, M.; Hernández Cadena, S.; Hiroshima, N.; Hnatyk, B.; Hofmann, W.; Holder, J.; Horan, D.; Hörandel, J.; Horvath, P.; Hovatta, T.; Hrabovsky, M.; Hrupec, D.; Hughes, G.; Humensky, T. B.; Hütten, M.; Iarlori, M.; Inada, T.; Inoue, S.; Iocco, F.; Iori, M.; Jamrozy, M.; Janecek, P.; Jin, W.; Jouvin, L.; Jurysek, J.; Karukes, E.; Katarzyński, K.; Kazanas, D.; Kerszberg, D.; Kherlakian, M. C.; Kissmann, R.; Knödlseder, J.; Kobayashi, Y.; Kohri, K.; Komin, N.; Kubo, H.; Kushida, J.; Lamanna, G.; Lapington, J.; Laporte, P.; Leigui de Oliveira, M. A.; Lenain, J.; Leone, F.; Leto, G.; Lindfors, E.; Lohse, T.; Lombardi, S.; Longo, F.; Lopez, A.; López, M.; López-Coto, R.; Loporchio, S.; Luque-Escamilla, P. L.; Mach, E.; Maggio, C.; Maier, G.; Mallamaci, M.; Malta Nunes de Almeida, R.; Mandat, D.; Manganaro, M.; Mangano, S.; Manicò, G.; Marculewicz, M.; Mariotti, M.; Markoff, S.; Marquez, P.; Martí, J.; Martinez, O.; Martínez, M.; Martínez, G.; Martínez-Huerta, H.; Maurin, G.; Mazin, D.; Mbarubucyeye, J. D.; Medina Miranda, D.; Meyer, M.; Miceli, M.; Miener, T.; Minev, M.; Miranda, J. M.; Mirzoyan, R.; Mizuno, T.; Mode, B.; Moderski, R.; Mohrmann, L.; Molina, E.; Montaruli, T.; Moralejo, A.; Morcuende-Parrilla, D.; Morselli, A.; Mukherjee, R.; Mundell, C.; Nagai, A.; Nakamori, T.; Nemmen, R.; Niemiec, J.; Nieto, D.; Nikołajuk, M.; Ninci, D.; Noda, K.; Nosek, D.; Nozaki, S.; Ohira, Y.; Ohishi, M.; Ohtani, Y.; Oka, T.; Okumura, A.; Ong, R. A.; Orienti, M.; Orito, R.; Orlandini, M.; Orlando, S.; Orlando, E.; Ostrowski, M.; Oya, I.; Pagano, I.; Pagliaro, A.; Palatiello, M.; Pantaleo, F. R.; Paredes, J. M.; Pareschi, G.; Parmiggiani, N.; Patricelli, B.; Pavletić, L.; Pe'er, A.; Pecimotika, M.; Pérez-Romero, J.; Persic, M.; Petruk, O.; Pfrang, K.; Piano, G.; Piatteli, P.; Pietropaolo, E.; Pillera, R.; Pilszyk, B.; Pintore, F.; Pohl, M.; Poireau, V.; Prado, R. R.; Prandini, E.; Prast, J.; Principe, G.; Prokoph, H.; Prouza, M.; Przybilski, H.; Pühlhofer, G.; Pumo, M. L.; Queiroz, F.; Quirrenbach, A.; Rainò, S.; Rando, R.; Razzaque, S.; Recchia, S.; Reimer, O.; Reisenegger, A.; Renier, Y.; Rhode, W.; Ribeiro, D.; Ribó, M.; Richtler, T.; Rico, J.; Rieger, F.; Rinchiuso, L.; Rizi, V.; Rodriguez, J.; Rodriguez Fernandez, G.; Rodriguez Ramirez, J. C.; Rojas, G.; Romano, P.; Romeo, G.; Rosado, J.; Rowell, G.; Rudak, B.; Russo, F.; Sadeh, I.; Sæther Hatlen, E.; Safi-Harb, S.; Salesa Greus, F.; Salina, G.; Sanchez, D.; Sánchez-Conde, M.; Sangiorgi, P.; Sano, H.; Santander, M.; Santos, E. M.; Santos-Lima, R.; Sanuy, A.; Sarkar, S.; Saturni, F. G.; Sawangwit, U.; Schussler, F.; Schwanke, U.; Sciacca, E.; Scuderi, S.; Seglar-Arroyo, M.; Sergijenko, O.; Servillat, M.; Seweryn, K.; Shalchi, A.; Sharma, P.; Shellard, R. C.; Siejkowski, H.; Silk, J.; Siqueira, C.; Sliusar, V.; Słowikowska, A.; Sokolenko, A.; Sol, H.; Spencer, S.; Stamerra, A.; Stanič, S.; Starling, R.; Stolarczyk, T.; Straumann, U.; Strišković, J.; Suda, Y.; Suomijarvi, T.; Świerk, P.; Tavecchio, F.; Taylor, L.; Tejedor, L. A.; Teshima, M.; Testa, V.; Tibaldo, L.; Todero Peixoto, C. J.; Tokanai, F.; Tonev, D.; Tosti, G.; Tosti, L.; Tothill, N.; Truzzi, S.; Travnicek, P.; Vagelli, V.; Vallage, B.; Vallania, P.; van Eldik, C.; Vandenbroucke, J.; Varner, G. S.; Vassiliev, V.; Vázquez Acosta, M.; Vecchi, M.; Ventura, S.; Vercellone, S.; Vergani, S.; Verna, G.; Viana, A.; Vigorito, C. F.; Vink, J.; Vitale, V.; Vorobiov, S.; Vovk, I.; Vuillaume, T.; Wagner, S. J.; Walter, R.; Watson, J.; Weniger, C.; White, R.; White, M.; Wiemann, R.; Wierzcholska, A.; Will, M.; Williams, D. A.; Wischnewski, R.; Yanagita, S.; Yang, L.; Yoshikoshi, T.; Zacharias, M.; Zaharijas, G.; Zakaria, A. A.; Zampieri, L.; Zanin, R.; Zaric, D.; Zavrtanik, M.; Zavrtanik, D.; Zdziarski, A. A.; Zech, A.; Zechlin, H.; Zhdanov, V. I.; Živec, M.-- This is an open access article published by IOP Publishing Ltd on behalf of Sissa Medialab. Original content from this work may be used under the terms of the Creative Commons Attribution 4.0 licence. Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI., We provide an updated assessment of the power of the Cherenkov Telescope Array (CTA) to search for thermally produced dark matter at the TeV scale, via the associated gamma-ray signal from pair-annihilating dark matter particles in the region around the Galactic centre. We find that CTA will open a new window of discovery potential, significantly extending the range of robustly testable models given a standard cuspy profile of the dark matter density distribution. Importantly, even for a cored profile, the projected sensitivity of CTA will be sufficient to probe various well-motivated models of thermally produced dark matter at the TeV scale. This is due to CTA's unprecedented sensitivity, angular and energy resolutions, and the planned observational strategy. The survey of the inner Galaxy will cover a much larger region than corresponding previous observational campaigns with imaging atmospheric Cherenkov telescopes. CTA will map with unprecedented precision the large-scale diffuse emission in high-energy gamma rays, constituting a background for dark matter searches for which we adopt state-of-the-art models based on current data. Throughout our analysis, we use up-to-date event reconstruction Monte Carlo tools developed by the CTA consortium, and pay special attention to quantifying the level of instrumental systematic uncertainties, as well as background template systematic errors, required to probe thermally produced dark matter at these energies. © 2021 The Author(s)., We gratefully acknowledge financial support from the following agencies and organisations: State Committee of Science of Armenia, Armenia; The Australian Research Council, Astronomy Australia Ltd, The University of Adelaide, Australian National University, Monash University, The University of New South Wales, The University of Sydney, Western Sydney University, Australia; Federal Ministry of Education, Science and Research, and Innsbruck University, Austria; Conselho Nacional de Desenvolvimento Cientifico e Tecnologico (CNPq), Fundacao de Amparo a Pesquisa do Estado do Rio de Janeiro (FAPERJ), Fundacao de Amparo a Pesquisa do Estado de Sao Paulo (FAPESP), Ministry of Science, Technology, Innovations and Communications (MCTIC), and Instituto Serrapilheira, Brasil; Ministry of Education and Science, National RI Roadmap Project DO1-153/28.08.2018, Bulgaria; The Natural Sciences and Engineering Research Council of Canada and the Canadian Space Agency, Canada; CONICYT-Chile grants CATA AFB 170002, ANID PIA/APOYO AFB 180002, ACT 1406, FONDECYT-Chile grants, 1161463, 1170171, 1190886, 1171421, 1170345, 1201582, Gemini-ANID 32180007, Chile; Croatian Science Foundation, Rudjer Boskovic Institute, University of Osijek, University of Rijeka, University of Split, Faculty of Electrical Engineering, Mechanical Engineering and Naval Architecture, University of Zagreb, Faculty of Electrical Engineering and Computing, Croatia; Ministry of Education, Youth and Sports, MEYS LM2015046, LM2018105, LTT17006, EU/MEYS CZ.02.1.01/0.0/0.0/16_013/0001403, CZ.02.1.01/0.0/0.0/18_046/0016007 and CZ.02.1.01/0.0/0.0/16_019/0000754, Czech Republic; Academy of Finland (grant nr.317636, 320045, 317383 and 320085), Finland; Ministry of Higher Education and Research, CNRS-INSU and CNRS-IN2P3, CEA-Irfu, ANR, Regional Council Ile de France, Labex ENIGMASS, OSUG2020, P2IO and OCEVU, France; Max Planck Society, BMBF, DESY, Helmholtz Association, Germany; Department of Atomic Energy, Department of Science and Technology, India; Istituto Nazionale di Astrofisica (INAF), Istituto Nazionale di Fisica Nucleare (INFN), MIUR, Istituto Nazionale di Astrofisica (INAF-OABRERA) Grant Fondazione Cariplo/Regione Lombardia ID 2014-1980/RST_ERC, Italy; ICRR, University of Tokyo, JSPS, MEXT, Japan; Netherlands Research School for Astronomy (NOVA), Netherlands Organization for Scientific Research (NWO), Netherlands; University of Oslo, Norway; Ministry of Science and Higher Education, DIR/WK/2017/12, the National Centre for Research and Development and the National Science Centre, UMO-2016/22/M/ST9/00583, Poland; Slovenian Research Agency, grants P1-0031, P1-0385, I0-0033, J1-9146, J1-1700, N1-0111, and the Young Researcher program, Slovenia; South African Department of Science and Technology and National Research Foundation through the South African Gamma-Ray Astronomy Programme, South Africa; The Spanish Ministry of Science and Innovation and the Spanish Research State Agency (AEI) through grants AYA2016-79724-C4-1-P, AYA2016-80889-P, AYA2016-76012-C3-1-P, BES-2016-076342, ESP2017-87055-C2-1-P, FPA2017-82729-C6-1-R, FPA2017-82729-C6-2-R, FPA2017-82729-C6-3-R, FPA2017-82729-C6-4-R, FPA2017-82729-C6-5-R, FPA2017-82729-C6-6-R, PGC2018-095161-B-I00, PGC2018-095512-B-I00; the \Centro de Excelencia Severo Ochoa"program through grants no. SEV-2015-0548, SEV-2016-0597, SEV-2016-0588, SEV-2017-0709; the "Unidad de Excelencia Maria de Maeztu" program through grant no. MDM-2015-0509; the "Ramon y Cajal" programme through grants RYC-2013-14511, RyC-2013-14660, RYC-2017-22665; and the MultiDark Consolider Network FPA2017-90566-REDC. Atraccion de Talento contract no. 2016-T1/TIC-1542 granted by the Comunidad de Madrid; the "Postdoctoral Junior Leader Fellowship" programme from La Caixa Banking Foundation, grants no. LCF/BQ/LI18/11630014 and LCF/BQ/PI18/11630012; the "Programa Operativo" FEDER2014-2020, Consejeria de Economia y Conocimiento de la Junta de Andalucia (ref. 1257737), PAIDI 2020 (ref. P18-FR-1580), and Universidad de Jaen; the Spanish AEI EQC2018-005094-P FEDER 2014-2020; the European Union's "Horizon 2020" research and innovation programme under Marie Sklodowska-Curie grant agreement no. 665919; and the ESCAPE project with grant no. GA:824064, Spain; Swedish Research Council, Royal Physiographic Society of Lund, Royal Swedish Academy of Sciences, The Swedish National Infrastructure for Computing (SNIC) at Lunarc (Lund), Sweden; State Secretariat for Education, Research and Innovation (SERI) and Swiss National Science Foundation (SNSF), Switzerland; Durham University, Leverhulme Trust, Liverpool University, University of Leicester, University of Oxford, Royal Society, Science and Technology Facilities Council, U.K.; U.S. National Science Foundation, U.S. Department of Energy, Argonne National Laboratory, Barnard College, University of California, University of Chicago, Columbia University, Georgia Institute of Technology, Institute for Nuclear and Particle Astrophysics (INPAC-MRPI program), Iowa State University, the Smithsonian Institution, Washington University McDonnell Center for the Space Sciences, The University of Wisconsin and the Wisconsin Alumni Research Foundation, U.S.A. The research leading to these results has received funding from the European Union's Seventh Framework Programme (FP7/2007-2013) under grant agreements No 262053 and No 317446. This project is receiving funding from the European Union's Horizon 2020 research and innovation programs under agreement No 676134.
Published: 2022

22. Aspectos de la dinámica de campos escalares y de la energía de vacío en el programa de swampland en teoría de cuerdas

Author: Buratti, Ginevra, Uranga, Angel M., UAM. Departamento de Física Teórica, and Instituto de Física Teórica (IFT)
Subjects: Cuerdas, Teoría de las, Física, Vacío (Física)-Tesis doctorales
Abstract: Tesis Doctoral inédita leída en la Universidad Autónoma de Madrid, Facultad de Ciencias, Departamento de Física Teórica. Fecha de Lectura: 30-05-2022, This thesis, written as a compendium of articles, investigates the properties of scalar dynamics and vacuum energy in the context of string theory compactifications, and their connection with the swampland program. In the first article presented in the thesis, we consider warped throats with locally AdS geometry, and study their stability properties. Motivated by considering the near horizon limit of systems of fractional D-branes at singularities, we propose that such backgrounds cannot be stable in the absence of supersymmetry, and thus generalize the swampland criterion that forbids stable non supersymmetric AdS vacua. This allows us to rule out large classes of warped throats with supersymmetry breaking ingredients, shedding new light on already known instabilities, including the runaway in the dP1 theory, and unveiling novel decay mechanisms such as the one associated to N = 2 fractional branes. In the second article we focus on the asymptotic Klebanov–Tseytlin solution, regarded as a compactification to five dimensions in which an axion runs in the radial direction of the locally AdS spacetime. The model can be reinterpreted as a fully backreacted solution of transplanckian axion monodromy, with the axion traversing arbitrarily large distances in field space, and provides an existence proof of transplanckian field excursions in string theory. In particular, we discuss how the ten-dimensional solution fully encodes the backreaction of the axion dynamics including the impact on the axion kinetic term, and the backreaction on other sectors, such as the compactification moduli and the vacuum energy. In the third article we propose a refinement of certain swampland conjectures in the presence of discrete gauge symmetries. We consider theories with both discrete and continuous gauge symmetries, and relate the gauge coupling of the continuous symmetry with the order of the discrete symmetry. We also study discrete symmetries associated to domain walls, and we use them to justify the presence of separation of scales in an infinite family of AdS4 flux vacua of type IIA string theory. In the last two articles of the thesis, we study running solutions sourced by tadpoles for dynamical fields, and analyse their properties in large classes of string theory models. These solutions can only extend up to a finite distance in spacetime, scaling inversely with the strength of the tadpole, and are capped off by cobordism walls of nothing in a dynamical realization of the cobordism conjecture. We also discuss domain walls interpolating between different (but cobordant) theories. The key criterion to distinguish between the two kinds of walls is related to the distance in field space, and suggests a connection with the distance conjecture
Published: 2022

23. Espectroscopía y truncamientos a partir de holografía y dualidades excepcionales

Author: Larios Plaza, Gabriel, Varela Rizo, Óscar Maigno, UAM. Departamento de Física Teórica, and Instituto de Física Teórica (IFT)
Subjects: Espectroscopía, Física
Abstract: Tesis Doctoral inédita leída en la Universidad Autónoma de Madrid, Facultad de Ciencias, Departamento de Física teórica. Fecha de Lectura: 17-06-2022, This thesis explores the relation between theories in different dimensions, focusing on the physics of string theory compactifications down to D = 4. We consider the limit in which the higher-dimensional theories are described by D = 11 or type II supergravity, and the studied solutions contain an AdS4 factor and are thus relevant for holography. The two main objects of study are Kaluza-Klein (KK) spectroscopy and consistent truncations. The first consists in the study of the features of the infinite towers of modes resulting from the compactification, whose properties are controlled by the choice of fluxes and geometry on the internal space. The latter are situations in which we can reduce these towers to a finite subset of modes whose dynamics is given by a lower-dimensional supergravity which can be consistently embedded into the higher-dimensional counterpart. After discussing the compactifications on tori as an introductory example to present the relevant concepts, we will analyse each topic in separate parts. In the first part, we explain how progress has been made in obtaining consistent truncations based on supersymmetry and G-structures, and on the duality groups governing the lower-dimensional supergravities thanks to the tensor and duality hierarchies and Exceptional Field Theory (ExFT). The second part addresses KK spectroscopy and its importance to holography. Until very recently, on non-homogeneous solutions only tools to study the spin-2 sector were available. These tools are combined with group theory to examine the configuration dual to the IR SCFT of a relevant deformation of the theory in the worldvolume of a stack of M2 branes. Subsequently, we show how these methods can be extended to lower-spin fields within the ExFT framework, and use them to analyse different classes of solutions in D = 10 and D = 11 of holographic interest
Published: 2022

24. The first law and Wald entropy formula of heterotic stringy black holes at first order in α

Author: Elgood, Zachary Alexander Veenhof, Ortín Miguel, Tomás, UAM. Departamento de Física Teórica, and Instituto de Física Teórica (IFT)
Subjects: Física
Abstract: Tesis Doctoral inédita leída en la Universidad Autónoma de Madrid, Facultad de Ciencias, Departamento de Física Teórica. Fecha de Lectura: 29-09-2022, The project that gave rise to these results received the support of a fellowship from ”la Caixa” Foundation (ID 100010434). The fellowship code is LCF/BQ/DI18/11660042. This project has received funding from the European Union´s Horizon 2020 research and innovation programme under the Marie Skłodowska-Curie grant agreement No. 713673
Published: 2022

25. Quantum and thermodynamic windows into the Universe

Author: Espinosa Portales, Llorenç, García-Bellido Capdevila, Juan, UAM. Departamento de Física Teórica, and Instituto de Física Teórica (IFT)
Subjects: Vacío (Física), Campos gravitatorios, Física, Entropía
Abstract: Tesis Doctoral inédita leída en la Universidad Autónoma de Madrid, Facultad de Ciencias, Departamento de Física Teórica. Fecha de Lectura: 14-09-2022, The author received funding from a fellowship from ’la Caixa’ Foundation (ID 100010434) with fellowship code LCF/BQ/IN18/11660041 and from the European Union’s Horizon 2020 research and innovation programme under the Marie Sklodowska-Curie grant agreement No. 713673
Published: 2022

26. Phenomenological Aspects Of The Minimal Linear σ Model And Of Its Extensions

Author: Alonso González, Javier, Merlo, Luca, UAM. Departamento de Física Teórica, and Instituto de Física Teórica (IFT)
Subjects: Modelos matemáticos, High Energy Physics::Phenomenology, Física, Higgs, Bosones de, Simetría
Abstract: Tesis doctoral inédita leída en la Universidad Autónoma de Madrid, Facultad de Ciencias, Departamento de Física Teórica. Fecha de lectura: 14-12-2021, In this Thesis the phenomenology of the Minimal Linear Model and of its possible extensions is analysed. This model is a perturbative renormalisable construction where the Higgs arises as a pseudo-Nambu-Goldstone boson from the linearly realised SO(5)=SO(4) breaking. The radial mode s of the eld that spontaneously breaks the global symmetry is an EW singlet that mixes with the Higgs and plays a crucial role in major part of the discussion. When this scalar mediates the decays of the lightest vector-like quarks of the model, it can lead to novel phenomena di erent to what experimental searches typically considered. Several present LHC searches can be sensitive to these new signatures. In the context of a CP violating version of the Minimal Linear Model, the validity of conclusions based on the E ective Field Theory approach with such a eld s in the spectrum is also examined. To this end, bounds from the electron Electric Dipole Moment on the resulting e ective SM top Yukawa couplings are analysed. Likewise, it is discussed the possibility of a rst order Electroweak Phase Transition compatible with the observed Baryon Asymmetry of the Universe when s is present in the scalar sector. Finally, in the context of the Axion-Minimal Linear Model, axion-like particle realisations are identi ed where the usual ne-tuning problem of axion models is avoided. In addition, a study about the possible signatures of these realisations at avour factories and colliders is performed
Published: 2021

27. Swampland Conjectures: a link between particle physics and String Theory

Author: Gonzalo Badía, Eduardo, Ibañez Santiago, Luis Enrique, UAM. Departamento de Física Teórica, Instituto de Física Teórica (IFT), and Ibáñez Santiago, Luís E.
Subjects: Partículas (Física nuclear), Cosmología, Física, Teoría de cuerdas
Abstract: Tesis Doctoral inédita leída en la Universidad Autónoma de Madrid, Facultad de Ciencias, Departamento de Física Teórica. Fecha de Lectura: 07-10-2021, Esta tesis tiene embargado el acceso al texto completo hasta el 2023-04-07
Published: 2021

28. The quest for quantum gravity: from weyl invariance to transverse theories

Author: Santos García, Raquel, Álvarez Vázquez, Enrique, Uranga Urteaga, Angel, UAM. Departamento de Física Teórica, and Instituto de Física Teórica (IFT)
Subjects: Gravedad cuántica, Física, Hermann Weyl, Relatividad
Abstract: Tesis Doctoral inédita leída en la Universidad Autónoma de Madrid, Facultad de Ciencias, Departamento de Física Teórica. Fecha de Lectura: 16-07-2021, This thesis, written as a compendium of articles, addresses some of the fundamental problems encountered when trying to build a theory of Quantum Gravity. Taking General Relativity (GR) as the starting point, its well-known non-renormalizable character leads to the need for an ultraviolet completion. Besides, the Cosmological Constant (CC) problem is still one of the cornerstones of Theoretical Physics. The following articles explore possible insights into these problems within the context of gravitational Effective Field Theories. The first article is devoted to the study of quadratic (in curvature) theories of gravity when treated in the First Order formalism, where the metric and the connection are considered as independent fields. These renormalizable theories are quadratic in the derivatives of the connection and do not contain quartic propagators, leaving a priori some room for unitarity. Nevertheless, it is not clear whether these theories include a graviton or whether they are free of ghosts, as all the dynamics is now encoded in the connection field. A complete study of the propagating degrees of freedom is then needed. In this work, we analyze the spin content of a generic torsion-free connection by constructing a complete basis of 22 six index spin projectors. We find that these theories generically propagate a spin three piece together with several lower spin components. One of the classical solutions to the CC problem is to consider Weyl invariant theories, as they forbid a CC term in the action. This symmetry is a generalization of the usual conformal invariance to cases where gravity is present. In the second article of the thesis, we carry out an analysis of the (in)equivalence of conformal and Weyl invariant theories for the gravitational field. The most general Lagrangian for spin two particles up to dimension six operators is explored, corresponding to the low-energy expansion of linear and quadratic (in curvature) theories of gravity. We carry out a full classification of the theories invariant under linearized (transverse) diffeomorphism, linearized Weyl transformations, and the usual conformal and scale symmetries. In the last part of the thesis, the theory of Unimodular Gravity (UG) is examined. This theory is an alternative low-energy description of gravity defined as the truncation of GR to unit determinant metrics. In UG the CC does not couple directly to gravity due to the unimodular constraint, and thus, it possesses a completely different nature. In particular, it does not receive radiative corrections, partially solving the CC problem. Apart from the character of the CC, UG is found to be classically equivalent to GR, and the question of the full (in)equivalence of both theories is still an open debate when quantum corrections are considered. The potential differences arising when studying the coupling to matter are investigated, via the introduction of a non-minimally coupled scalar field. We compute all the one-loop divergences in both theories and find a physical combination of couplings whose running differs for intermediate values of the non-minimal coupling
Published: 2021

29. A Systematic Search of Dark Matter Subhalos in Gamma Rays among Unidentifed Sources and Constraints on Dark Matter Properties

Author: Coronado Blázquez, Javier, Sánchez-Conde, Miguel A., Muñoz, Carlos, UAM. Departamento de Física Teórica, and Instituto de Física Teórica (IFT)
Subjects: Materia oscura (Astronomía), Física, Rayos gamma
Abstract: Tesis Doctoral inédita leída en la Universidad Autónoma de Madrid, Facultad de Ciencias, Departamento de Física Teórica. Fecha de Lectura: 01-10-2021, Esta tesis tiene embargado el acceso al texto completo hasta el 01-04-2023
Published: 2021

30. The Clustering Dynamics of Primordial Black Boles in N-Body Simulations

Author: Juan Garcia-Bellido, Manuel Trashorras, Savvas Nesseris, UAM.Departamento de Física Teórica, Instituto de Física Teórica (IFT), Ministerio de Economía y Competitividad (España), and Ministerio de Ciencia, Innovación y Universidades (España)
Subjects: lcsh:QC793-793.5, Cosmology and Nongalactic Astrophysics (astro-ph.CO), Stellar mass, Dark matter, Black Hole Mergers, FOS: Physical sciences, General Physics and Astronomy, Binary number, Primordial black hole, General Relativity and Quantum Cosmology (gr-qc), Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, 01 natural sciences, General Relativity and Quantum Cosmology, dark matter, 0103 physical sciences, Primordial Black Holes, Cluster (physics), Mass segregation, Dark Matter, N-body simulations, 010303 astronomy & astrophysics, Astrophysics::Galaxy Astrophysics, black hole mergers, Physics, 010308 nuclear & particles physics, lcsh:Elementary particle physics, primordial black holes, Física, N-Body Simulations, Astronomía, black hole binaries, Black Hole Binaries, Halo, Phenomenology (particle physics), Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: © 2021 by the authors., We explore the possibility that Dark Matter (DM) may be explained by a nonuniform background of approximately stellar mass clusters of Primordial Black Holes (PBHs) by simulating the evolution from recombination to the present with over 5000 realisations using a Newtonian N-body code. We compute the cluster rate of evaporation and extract the binary and merged sub-populations along with their parent and merger tree histories, lifetimes and formation rates, the dynamical and orbital parameter profiles, the degree of mass segregation and dynamical friction and power spectrum of close encounters. Overall, we find that PBHs can constitute a viable DM candidate, and that their clustering presents a rich phenomenology throughout the history of the Universe. We show that binary systems constitute about 9.5% of all PBHs at present, with mass ratios of q¯B=0.154, and total masses of m¯T,B=303M⊙. Merged PBHs are rare, about 0.0023% of all PBHs at present, with mass ratios of q¯B=0.965 with total and chirp masses of m¯T,B=1670M⊙ and m¯c,M=642M⊙, respectively. We find that cluster puffing up and evaporation leads to bubbles of these PBHs of order 1 kpc containing at present times about 36% of objects and mass, with one-hundred pc-sized cores. We also find that these PBH sub-haloes are distributed in wider PBH haloes of order hundreds of kpc, containing about 63% of objects and mass, coinciding with the sizes of galactic halos. We find at last high rates of close encounters of massive Black Holes (M∼1000M⊙), with ΓS=(1.2+5.9−0.9)×107yr−1Gpc−3 and mergers with ΓM=1337±41yr−1Gpc−3., This research was funded by Research Project PGC2018-094773-B-C32 [MINECO-FEDER]; Centro de Excelencia Severo Ochoa Program SEV-2016-0597; Ramón y Cajal program through Grant No. RYC-2014-15843; Grant No. BES-2016-077817 (MINECO-FPI).
Published: 2021

31. Measurements of top-quark pair single- and double-differential cross-sections in the all-hadronic channel in pp collisions at √s = 13 TeV using the ATLAS detector

Author: Gabriela Navarro, Veronica Fabiani, Akira Yamamoto, Stanislava Sevova, Z. Liang, Edoardo Maria Farina, C. Zhu, Andrzej Olszewski, Claudia Merlassino, Elisabeth Schopf, Balthasar Maria Schachtner, Hannes Mildner, Sebastian Andreas Merkt, Gideon Bella, Allison Mccarn Deiana, Sarah Kate Boutle, H. Ten Kate, D. Fassouliotis, T. Dias Do Vale, Simona Serena Bocchetta, A. Ventura, Jacqueline Batley, Babar Ali, Petr Sicho, R. S. P. Mueller, Auriane Canesse, Xiangyu Xie, Xi Chen, S. Shirabe, Theodoros Alexopoulos, Jianqiao Ye, Marco Lavorgna, Frederic Deliot, Jacob Henry Rawling, C. Di Donato, Xing Long Li, Marco Montella, Steffen Schmitt, Kerstin Tackmann, Olga Novgorodova, D. Su, Francesco Spanò, Cole Michael Helling, James Pinfold, Gregory Barbour, Vincent Hedberg, Giuseppe Salamanna, Ines Ochoa, Sara Caroline Alderweireldt, Zuzana Rurikova, V. Araujo Ferraz, Hadar Yosef Cohen, F. J. Munoz Sanchez, Emma Sian Kuwertz, Raimund Ströhmer, Grigore Tarna, Michele Pinamonti, Sabine Lammers, Volker Büscher, Luca Ambroz, A. T. Goshaw, Hernan Wahlberg, Falk Bartels, D. E. Ferreira de Lima, Andrey Kamenshchikov, S. Prell, Maosen Zhou, Jie Zhang, James H Cochran, Marcela Mikestikova, Matthew Feickert, Emily Anne Thompson, Adam Kaluza, T. Yamazaki, Antony Fray, Janna Katharina Behr, Yury Smirnov, Alexander Cheplakov, Robin Hayes, S. R. Hou, Valerio Vercesi, Kazuki Todome, Mossadek Talby, Lucrezia Stella Bruni, James Baker Beacham, Tomas Dado, W. J. Murray, Nico Madysa, Kevin Thomas Bauer, Florian Dachs, Damiano Vannicola, Konstantin Lehmann, Malik Aliev, John Andrew Raine, Philipp Fleischmann, Tatyana Kharlamova, N. M. Köhler, T. Jakoubek, Paul Gessinger-Befurt, Fernando Barreiro, O. E. Vickey Boeriu, K. K. Gan, Maria Giovanna Foti, Brian Petersen, Namig Javadov, Yang Yang, A. Ferrer, Bengt Lund-Jensen, Susumu Oda, J. S. Keller, Aidan Robson, Joachim Heinrich, Grazia Cabras, Egor Antipov, Arthur Rene Chomont, K. Kordas, James Ferrando, Alexander Fenyuk, Tamar Djobava, Duc Ta, Sinan Kuday, R. Camacho Toro, Ahmet Bingul, Elzbieta Richter-Was, L. F. Oleiro Seabra, Adrian Chitan, Michal Marcisovsky, Adam James Bozson, T. Kawamoto, Benjamin Wynne, Martin Aleksa, A. De Salvo, Radek Novotny, Koji Terashi, Mario Campanelli, Borut Paul Kerševan, Inga Katarzyna Lakomiec, Dongshuo Du, Giovandomenico Carducci, G. A. Chelkov, Andre Schoening, Simon Berlendis, Evgeniy Khramov, Tasneem Rashid, Hiroshi Sakamoto, T. S. Lau, A. G. Clark, Barbara Wosiek, B. Di Micco, Simon George, Gregory James Ottino, Alexander Bogdanchikov, Spyridon Argyropoulos, Mikhail Levchenko, J. Urban, Gabriel Gallardo, Ben William Whitmore, Alexander Linus Sopio, Aaron Foley Webb, Alexi Gongadze, Giovanni Darbo, Marianna Testa, Holly Ann Pacey, Graeme Stewart, Tomoki Saito, Mattias Ellert, P. M. Tuts, J. Geisen, Yuji Enari, T. Javůrek, Maria Roberta Devesa, Igor Potrap, Marta Lidia Rimoldi, Regina Moles-Valls, Binbin Dong, J. K. K. Liu, Jan-Ulf Mjörnmark, Giuliano Gustavino, H. J. Yang, R. F. Naranjo Garcia, Shan Jin, Sandra Leone, Marek Palka, Jay Chan, Ivor Fleck, A. M. Rodríguez Vera, Lorenzo Massa, Adam Trzupek, Emilio Higón-Rodriguez, Y. Delabat Diaz, Martin White, Sahal Yacoob, Oleg Solovyanov, Kristof Schmieden, Margherita Spalla, Marie Christine Lanfermann, Jindong Li, Ulrike Blumenschein, M. J. Costa, Tadashi Maeno, Jamal Eddine Derkaoui, W. R. Cunningham, Florian Bauer, Patrick Czodrowski, Joleen Pater, N. Viaux Maira, Vladimir Tikhomirov, Ioulian Budagov, Makoto Tomoto, Yahya Tayalati, Takuya Tashiro, D. della Volpe, Thomas Peiffer, Stefan Simion, Gianluca Alimonti, Rainer Stamen, Franziska Iltzsche, Sergey Barsov, Jacob Julian Kempster, Christos Anastopoulos, Joseph Haley, Thorben Swirski, F. Wang, Y. Amaral Coutinho, Laurent Schoeffel, Y. W. Liu, C. N. P. Gee, Artem Basalaev, Kamil Augsten, A. 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Lozano Bahilo, Henri Bachacou, Daniel Fournier, Jing Guo, Patrick Scholer, Asma Hadef, Louis Fayard, Thorwald Klapdor-kleingrothaus, Christos Paraskevopoulos, Savanna Marie Shaw, A. Mirto, Mikhail Mineev, Mohamad Kassem Ayoub, Ferdinand Schenck, Alexander Milov, Leonardo Carminati, R. E. Ticse Torres, C. J. E. Suster, Steven Goldfarb, Z. G. Zhao, Clara Elisabeth Leitgeb, Alexander Lincoln Read, Jessica Levêque, M. De Santis, Frank Ellinghaus, Mykola Khandoga, Claire Gwenlan, R. Gamboa Goni, Marina Rotaru, Ishan Pokharel, Baida Achkar, Athanasios Manousos, Ajit S. Puri, C. A. Solans Sanchez, S. Malyukov, Xin Wu, Abdenour Lounis, Yi Fan Hu, S. Passaggio, Luiz Caloba, Henric George Wilkens, F. La Ruffa, G. N. Taylor, Marco Bomben, Konstantinos Papageorgiou, Benjamin Brau, Nazim Huseynov, Francisco Anuar Arduh, Sabina Czekierda, Michael A. Strauss, Jaroslava Schovancova, Wenge Wang, E. Thomson, Matteo Negrini, L. Zhang, S. Rodriguez Bosca, Seppe Kuehn, J. C. 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N., Santra, A., Sapronov, A., Saraiva, J. G., Sasaki, O., Sato, K., Sauerburger, F., Sauvan, E., Savard, P., Sawada, R., Sawyer, C., Sawyer, L., Sayago Galvan, I., Sbarra, C., Sbrizzi, A., Scanlon, T., Schaarschmidt, J., Schacht, P., Schachtner, B. M., Schaefer, D., Schaefer, L., Schaepe, S., Schafer, U., Schaffer, A. C., Schaile, D., Schamberger, R. D., Schanet, E., Scharmberg, N., Schegelsky, V. A., Scheirich, D., Schenck, F., Schernau, M., Schiavi, C., Schildgen, L. K., Schillaci, Z. M., Schioppa, E. J., Schioppa, M., Schleicher, K. E., Schlenker, S., Schmidt-Sommerfeld, K. R., Schmieden, K., Schmitt, C., Schmitt, S., Schmoeckel, J. C., Schoeffel, L., Schoening, A., Scholer, P. G., Schopf, E., Schott, M., Schouwenberg, J. F. P., Schovancova, J., Schramm, S., Schroeder, F., Schulte, A., Schultz-Coulon, H. -C., Schumacher, M., Schumm, B. A., Schune, P., Schwartzman, A., Schwarz, T. 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C., Unno, Y., Uno, K., Urban, J., Urquijo, P., Usai, G., Uysal, Z., Vacek, V., Vachon, B., Vadla, K. O. H., Vafeiadis, T., Vaidya, A., Valderanis, C., Valdes Santurio, E., Valente, M., Valentinetti, S., Valero, A., Valery, L., Vallance, R. A., Vallier, A., Valls Ferrer, J. A., Van Daalen, T. R., Van Gemmeren, P., Van Vulpen, I., Vanadia, M., Vandelli, W., Vandenbroucke, M., Vandewall, E. R., Vaniachine, A., Vannicola, D., Vari, R., Varnes, E. W., Varni, C., Varol, T., Varouchas, D., Varvell, K. E., Vasile, M. E., Vasquez, G. A., Vazeille, F., Vazquez Furelos, D., Vazquez Schroeder, T., Veatch, J., Vecchio, V., Veen, M. J., Veloce, L. M., Veloso, F., Veneziano, S., Ventura, A., Venturi, N., Verbytskyi, A., Vercesi, V., Verducci, M., Vergel Infante, C. M., Vergis, C., Verkerke, W., Vermeulen, A. T., Vermeulen, J. C., Vernieri, C., Vetterli, M. C., Viaux Maira, N., Vickey, T., Vickey Boeriu, O. E., Viehhauser, G. H. A., Vigani, L., Villa, M., Villaplana Perez, M., Villhauer, E. M., Vilucchi, E., Vincter, M. G., Virdee, G. S., Vishwakarma, A., Vittori, C., Vivarelli, I., Vogel, M., Vokac, P., von Buddenbrock, S. E., Von Toerne, E., Vorobel, V., Vorobev, K., Vos, M., Vossebeld, J. H., Vozak, M., Vranjes, N., Vranjes Milosavljevic, M., Vrba, V., Vreeswijk, M., Vuillermet, R., Vukotic, I., Wada, S., Wagner, P., Wagner, W., Wagner-Kuhr, J., Wahdan, S., Wahlberg, H., Wakasa, R., Walbrecht, V. M., Walder, J., Walker, R., Walker, S. D., Walkowiak, W., Wallangen, V., Wang, A. M., Wang, A. Z., Wang, C., Wang, F., Wang, H., Wang, J., Wang, P., Wang, Q., Wang, R. -J., Wang, R., Wang, S. M., Wang, W. T., Wang, W., Wang, W. X., Wang, Y., Wang, Z., Wanotayaroj, C., Warburton, A., Ward, C. P., Wardrope, D. R., Warrack, N., Watson, A. T., Watson, M. F., Watts, G., Waugh, B. M., Webb, A. F., Weber, C., Weber, M. S., Weber, S. A., Weber, S. M., Weidberg, A. R., Weingarten, J., Weirich, M., Weiser, C., Wells, P. S., Wenaus, T., Wengler, T., Wenig, S., Wermes, N., Werner, M. 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I., Zimmermann, S., Zinonos, Z., Ziolkowski, M., Zivkovic, L., Zobernig, G., Zoccoli, A., Zoch, K., Zorbas, T. G., Zou, R., Zwalinski, L., Współautorami artykułu są członkowie ATLAS Collaboration w liczbie 2928, Centre de Physique des Particules de Marseille (CPPM), Aix Marseille Université (AMU)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Laboratoire d'Annecy de Physique des Particules (LAPP), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Physique des 2 Infinis Irène Joliot-Curie (IJCLab), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Physique de Clermont (LPC), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Clermont Auvergne (UCA), Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE (UMR_7585)), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP ), Université Grenoble Alpes (UGA), Centre de Calcul de l'IN2P3 (CC-IN2P3), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), ATLAS, Aloisio, Alberto, Alviggi, Mariagrazia, Canale, Vincenzo, Della Pietra, Massimo, Merola, Leonardo, Massarotti, Paolo, Conventi, Francesco, Rossi, Elvira, Carlino, Giampaolo, de Asmundis, Riccardo, Di Donato, Camilla, Doria, Alessandra, Iengo, Paolo, Izzo, Vincenzo, Perrella, Sabrina, Sekhniaidze, Givi, Cirotto, Francesco, Lavorgna, Marco, Giannini, Antonio, Atlas, Collaboration, Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), ATLAS (IHEF, IoP, FNWI), XENON (IHEF, IoP, FNWI), Carratta , G., De Castro , S., Fabbri , L., Gabrielli , A., Rinaldi , L., Semprini Cesari , N., Sioli , M., Villa , M., Zoccoli , A., Bellagamba , L., Boscherini , D., Bruni , A., Bruni , G., Giacobbe , B., Polini , A., Sbarra , C., Sidoti , A., Franchini , M., Romano , M., Valentinetti , S., Alberghi , G. L., Biondi , S., Lasagni Manghi , F, Massa , L., Vittori , C., Alfonsi , F, Cabras , G., Cervelli , A., Negrini , M., Todome , K., ATLAS collaboration, Apollo - University of Cambridge Repository, Aad, G, Bachas, K, Chiodini, G, Gorini, E, Gravili, F, Longo, L, Primavera, M, Reale, M, Schioppa, E, Spagnolo, S, Ventura, A, and ATLAS Collaboration, And
Subjects: Top quark, Kjerne- og elementærpartikkelfysikk: 431 [VDP], final state: ((n)jet), 13000 GeV-cms, Hadron, Nuclear Theory, Parton, pair production [top], transverse momentum dependence, 01 natural sciences, High Energy Physics - Experiment, rapidity dependence, Subatomär fysik, High Energy Physics - Experiment (hep-ex), Hadron-Hadron scattering (experiments), Subatomic Physics, scattering [p p], [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex], parton, Nuclear Experiment, Physics, Settore FIS/01, ATLAS experiment, Monte Carlo [numerical calculations], multiplicity: dependence, ATLAS, mass dependence, medicine.anatomical_structure, Nuclear and elementary particle physics: 431 [VDP], CERN LHC Coll, Top physics, kinematics, colliding beams [p p], multiplicity [jet], numerical calculations: Monte Carlo, top: pair production, Particle Physics - Experiment, Nuclear and High Energy Physics, p p: scattering, CERN Lab, Regular Article - Experimental Physics, 530 Physics, FOS: Physical sciences, jet: multiplicity, decay modes, Top physics, ATLAS, Nuclear physics, differential cross section: measured, Atlas (anatomy), transverse momentum [top], ((n)jet) [final state], measured [differential cross section], 0103 physical sciences, medicine, ddc:530, lcsh:Nuclear and particle physics. Atomic energy. Radioactivity, High Energy Physics, 010306 general physics, top quark, top: transverse momentum, mass spectrum: (2top), 010308 nuclear & particles physics, High Energy Physics::Phenomenology, Física, Collision, PARTON DISTRIBUTIONS, dependence [multiplicity], Pair production, correlation, lcsh:QC770-798, High Energy Physics::Experiment, Hadron-hadron collisions, p p: colliding beams, Differential (mathematics), (2top) [mass spectrum], experimental results
Abstract: We acknowledge the support of ANPCyT, Argentina; YerPhI, Armenia; ARC, Australia; BMWFW and FWF, Austria; ANAS, Azerbaijan; SSTC, Belarus; CNPq and FAPESP, Brazil; NSERC, NRC and CFI, Canada; CERN; ANID, Chile; CAS, MOST and NSFC, China; COLCIENCIAS, Colombia; MSMT CR, MPO CR and VSC CR, Czech Republic; DNRF and DNSRC, Denmark; IN2P3-CNRS and CEA-DRF/IRFU, France; SRNSFG, Georgia; BMBF, HGF and MPG, Germany; GSRT, Greece; RGC and Hong Kong SAR, China; ISF and Benoziyo Center, Israel; INFN, Italy; MEXT and JSPS, Japan; CNRST, Morocco; NWO, Netherlands; RCN, Norway; MNiSW and NCN, Poland; FCT, Portugal; MNE/IFA, Romania; MES of Russia and NRC KI, Russia Federation; JINR; MESTD, Serbia; MSSR, Slovakia; ARRS and MIZS, Slovenia; DST/NRF, South Africa; MICINN, Spain; SRC and Wallenberg Foundation, Sweden; SERI, SNSF and Cantons of Bern and Geneva, Switzerland; MOST, Taiwan; TAEK, Turkey; STFC, United Kingdom; DOE and NSF, United States of America. In addition, individual groups and members have received support from BCKDF, CANARIE, Compute Canada, CRC and IVADO, Canada; Beijing Municipal Science & Technology Commission, China; COST, ERC, ERDF, Horizon 2020 and Marie Sklodowska-Curie Actions, European Union; Investissements d'Avenir Labex, Investissements d'Avenir Idex and ANR, France; DFG and AvH Foundation, Germany; Herakleitos, Thales and Aristeia programmes co-financed by EU-ESF and the Greek NSRF, Greece; BSF-NSF and GIF, Israel; La Caixa Banking Foundation, CERCA Programme Generalitat de Catalunya and PROMETEO and GenT Programmes Generalitat Valenciana, Spain; Goran Gustafssons Stiftelse, Sweden; The Royal Society and Leverhulme Trust, United Kingdom., Differential cross-sections are measured for top-quark pair production in the all-hadronic decay mode, using proton-proton collision events collected by the ATLAS experiment in which all six decay jets are separately resolved. Absolute and normalised single- and double-differential cross-sections are measured at particle and parton level as a function of various kinematic variables. Emphasis is placed on well-measured observables in fully reconstructed final states, as well as on the study of correlations between the top-quark pair system and additional jet radiation identified in the event. The study is performed using data from proton-proton collisions at s√ = 13 TeV collected by the ATLAS detector at CERN’s Large Hadron Collider in 2015 and 2016, corresponding to an integrated luminosity of 36.1 fb−1. The rapidities of the individual top quarks and of the top-quark pair are well modelled by several independent event generators. Significant mismodelling is observed in the transverse momenta of the leading three jet emissions, while the leading top-quark transverse momentum and top-quark pair transverse momentum are both found to be incompatible with several theoretical predictions., ANPCyT, YerPhI, Armenia, Australian Research Council, BMWFW, Austria, Austrian Science Fund (FWF), Azerbaijan National Academy of Sciences (ANAS), SSTC, Belarus, National Council for Scientific and Technological Development (CNPq), Fundacao de Amparo a Pesquisa do Estado de Sao Paulo (FAPESP), Natural Sciences and Engineering Research Council of Canada (NSERC), NRC, Canada, Canada Foundation for Innovation, CERN, ANID, Chile, Chinese Academy of Sciences, Ministry of Science and Technology, China, National Natural Science Foundation of China (NSFC), Departamento Administrativo de Ciencia, Tecnologia e Innovacion Colciencias, Ministry of Education, Youth & Sports - Czech Republic Czech Republic Government, DNRF, Denmark, Danish Natural Science Research Council, Centre National de la Recherche Scientifique (CNRS), CEA-DRF/IRFU, France, SRNSFG, Georgia, Federal Ministry of Education & Research (BMBF), HGF, Germany, Max Planck Society, Greek Ministry of Development-GSRT, RGC, China, Hong Kong SAR, China, Israel Science Foundation, Benoziyo Center, Israel, Istituto Nazionale di Fisica Nucleare (INFN), Ministry of Education, Culture, Sports, Science and Technology, Japan (MEXT) Japan Society for the Promotion of Science, CNRST, Morocco, Netherlands Organization for Scientific Research (NWO) Netherlands Government, RCN, Norway, Ministry of Science and Higher Education, Poland, NCN, Poland, Portuguese Foundation for Science and Technology, MNE/IFA, Romania, MES of Russia, Russia Federation, NRC KI, Russia Federation, JINR, MESTD, Serbia, MSSR, Slovakia, Slovenian Research Agency - Slovenia, MIZS, Slovenia, DST/NRF, South Africa, Spanish Government, SRC, Sweden, Wallenberg Foundation, Sweden, SERI, Switzerland, Swiss National Science Foundation (SNSF), Canton of Bern, Switzerland, Canton of Geneva, Switzerland, Ministry of Science and Technology, Taiwan, Ministry of Energy & Natural Resources - Turkey, UK Research & Innovation (UKRI) Science & Technology Facilities Council (STFC), United States Department of Energy (DOE), National Science Foundation (NSF), BCKDF, Canada, CANARIE, Canada, Compute Canada, Canada, CRC, Canada, IVADO, Canada, Beijing Municipal Science & Technology Commission, COST, European Union, European Union (EU) European Research Council (ERC), Horizon 2020, European Union, French National Research Agency (ANR), German Research Foundation (DFG), Alexander von Humboldt Foundation, Herakleitos programme - EU-ESF, Thales programme - EU-ESF, Aristeia programme - EU-ESF, Greek NSRF, Greece, BSF-NSF, Israel, German-Israeli Foundation for Scientific Research and Development, La Caixa Banking Foundation, Spain, CERCA Programme Generalitat de Catalunya, Spain, PROMETEO Programme Generalitat Valenciana, Spain, GenT Programme Generalitat Valenciana, Spain, Goran Gustafssons Stiftelse, Sweden, Royal Society of London, Leverhulme Trust
Published: 2021

32. Evidence for Higgs boson decay to a pair of muons

Author: Colin Jessop, Manuel Olmedo Negrete, Ivan Ovtin, Changwoo Joo, Alessandro Calandri, Giorgio Apollinari, Matthias Kasemann, Luca Giommi, Cole Lindsey, Paola Salvini, Ibrahim Soner Zorbakir, Costas Foudas, Devdatta Majumder, Anna Zacharopoulou, Kyeongpil Lee, David Hamilton, Dominique Gigi, Alexandra Carvalho Antunes De Oliveira, Teruki Kamon, James Buchanan, Maxim Pieters, David Vannerom, Catherine Vander Velde, Marcos Fernandez, Shaaban Khalil, Young-Il Choi, J William Gary, Florian Beaudette, Raffaello D'Alessandro, Slawek Tkaczyk, Ulrich Heintz, Bjorn Burkle, Hanwen Wang, Giuseppe Iaselli, Vincenzo Mastrapasqua, Raghunath Pradhan, Andrei Sobol, Gabriella Pasztor, Sebastian Templ, Georgi Sultanov, Armando Bermúdez Martínez, Evan Wolfe, David Cutts, Daniel Arcaro, Christina Wang, Marek Walczak, Federico Siviero, Helena Bialkowska, Marcella Diemoz, Erhan Gülmez, Kaori Maeshima, Aurelijus Rinkevicius, Gian Luca Pinna Angioni, Kevin Stenson, Martin Erdmann, Achim Stahl, Karl Gill, Bora Akgun, Dario Soldi, Gui Nyun Kim, M. Mohammadi Najafabadi, Andrea Gelmi, Andrew Wisecarver, Olena Hlushchenko, Sergey Petrushanko, Matti J Kortelainen, Cheng-Chieh Peng, Hao Qiu, Yacine Haddad, Antonio Ranieri, Marius Teroerde, S. Sanchez Cruz, Lucas Corcodilos, Antonin Kveton, Mauro Menichelli, Patricia McBride, Charles Harrington, Emil Sørensen Bols, Panja-Riina Luukka, Muhammad Imran Malik Awan, Jennifer Ngadiuba, Miguel Medina Jaime, Claudia Pistone, Roberto Salerno, Vladimir Makarenko, Scarlet Norberg, Olga Kodolova, Mariana Araujo, Luca Perniè, Roland Horisberger, Yuan Chao, Michele Arneodo, Garvita Agarwal, Wolfgang Adam, Krzysztof Doroba, Pantelis Kontaxakis, Dylan Rankin, Andrew Brinkerhoff, Thomas Ferguson, Ram Krishna Dewanjee, Bora Isildak, Jennifer Chu, Luigi Guiducci, Gregory R Snow, Pierre Van Hove, Sung Won Lee, Ka Tung Lau, Leonid Didukh, Jose Flix, Saikat Karmakar, Diego Matos Figueiredo, Kenichi Hatakeyama, Viktor Khristenko, Gaël Perrin, Michael Finger Jr, Laurent Pétré, Georgia Karapostoli, Florian Joel J Bury, Marc Dünser, Davide Valsecchi, Brieuc Francois, Paul Edmund Karchin, Thomas Madlener, Christopher Rogan, Janek Bechtel, Umesh Joshi, Jared Sturdy, Doris Eckstein, Achim Geiser, Batoul Diab, Marcos Cerrada, Daniel Winterbottom, Thorben Quast, Igor Volobouev, Matej Roguljic, Hirak Bandyopadhyay, Javier Cuevas, Özlem Özçelik, Yuan Chen, Guillaume Bourgatte, Fanbo Meng, Jhovanny Mejia Guisao, Caroline Collard, Marcello Abbrescia, Akram Khan, Ruslan Chistov, Po-Hsun Chen, Stefano Mersi, Anna Woodard, Marco Costa, Nikolai Golubev, Javier Alberto Murillo Quijada, Jangbae Lee, Didier Contardo, Danila Tlisov, Andrei Gritsan, Jian Wang, Felipe Torres Da Silva De Araujo, Alexander Toropin, Marcel Rieger, Anders Ryd, Gavin Davies, Mykyta Haranko, Arash Jofrehei, Elisabetta Gallo, Vincenzo Ciriolo, Nicolas Chanon, Camelia Mironov, Tongguang Cheng, Valentina Avati, Jeongeun Lee, Jesus Puerta Pelayo, Virgil E Barnes, Andrzej Novak, Efe Yigitbasi, Wing Yan Wong, Nicola Turini, Cristina Mantilla, Georgios Anagnostou, Melody A. Swartz, Maxwell Chertok, Danek Kotlinski, Jordan Martins, Denis Gelé, Chang-Seong Moon, Graham Wilson, Zviad Tsamalaidze, Catherine Schiber, Mauro Emanuele Dinardo, Carmen Albajar, Sven Dildick, Cilicia Uzziel Perez, Samuel Nathan Webb, Alessio Ghezzi, Giovanni Mocellin, Francesco Pandolfi, Tomas Kello, Anton Petrov, Alexander Lanev, Danyer Pérez Adán, Rudy Ceccarelli, Benedikt Vormwald, Ilknur Hos, J. N. Butler, Fabiola Vazquez Valencia, Susan Dittmer, Georgios Daskalakis, Sergei Gninenko, Senka Duric, Benjamin Tannenwald, Abideh Jafari, Johannes Haller, Vadim Oreshkin, Byung Hun Oh, Mateusz Zarucki, Dan Quach, Guler Karapinar, Sandro Fonseca De Souza, Mate Csanad, Junho Choi, M. J. Kim, Geetanjali Chaudhary, Brian L Winer, Mehmet Özgür Sahin, Donato Creanza, Marc Dobson, Catherine Kirsty Mackay, Robin Aggleton, Ferhat Ozok, Prasanna Siddireddy, Jaehyeok Yoo, Antoni Shtipliyski, Paolo Lariccia, Dmitry Sosnov, Rudolf Fruehwirth, Nick Van Remortel, Chad Freer, Stefan Piperov, Alexandre Zabi, Nhan Viet Tran, Mohammad Abrar Wadud, Christof Roland, Yao Yao, David Colling, Amina Zghiche, Emily MacDonald, Danilo Meuser, Andrew Gilbert, Ridhi Chawla, Meenakshi Narain, Ketino Kaadze, Samuel May, Muzamil Ahmad Bhat, Giuseppe Latino, William Tabb, Thong Nguyen, Rylan Conway, Hans Van Haevermaet, Meng Lu, David Overton, Sang Il Pak, Shao Min Tan, Patricia Rebello Teles, Matthew Kilpatrick, Tejinder Virdee, Paolo Dini, Péter Major, Fabio Ravera, Süleyman Durgut, Paul Sheldon, Yuichi Kubota, Gilles De Lentdecker, Andreas Albert, Alexander Titterton, Erich Schmitz, Lutz Feld, Werner Sun, Tommaso Boccali, Mohit Gola, Marino Missiroli, Amandeep Kaur, Andrius Juodagalvis, Inna Makarenko, Shubhanshu Chauhan, Alessandro Giassi, Giacomo Ortona, Evan Ranken, Riccardo Salvatico, Maurizio Pierini, David Cussans, John Paul Chou, Rishabh Uniyal, Brian Paul Padley, Justin Williams, Tobias Pook, Jay Hauser, Andrei Starodumov, Isidro Gonzalez Caballero, P. Klabbers, Maren Tabea Meinhard, Rogelio Reyes-Almanza, Cheng Chen, Nikola Godinovic, Hualin Mei, Altan Cakir, Paolo Meridiani, Aron Soha, Henriette Aarup Petersen, Patrick Asenov, Sudeshna Banerjee, Alexander Dierlamm, Minna Leonora Vesterbacka Olsson, Jonatan Piedra Gomez, Shahram Rahatlou, Vivek Sharma, Alexander Malakhov, Günter Flügge, Danyyl Brzhechko, Santeri Laurila, Christian Dziwok, Emmanuel Olaiya, Alexander Schmidt, Elizabeth Starling, Akshansh Singh, Nan Lu, René Caspart, Wajid Ali Khan, Inna Kucher, Jelena Mijuskovic, Victor Shang, Mirena Ivova Paneva, Thomas Eichhorn, Mar Barrio Luna, Alessandro Thea, Cristina Fernandez Bedoya, Isabel Pedraza, Sunil Somalwar, Saswati Nandan, Nicolò Tosi, Rajarshi Bhattacharya, Elisabetta Manca, Camilla Galloni, Alex Dorsett, Vincenzo Daponte, Michal Szleper, Philippe Gras, Chia-Ming Kuo, Candan Dozen, Nadir Daci, Julia Thom, Finn Rebassoo, Michael Wayne Arenton, Mohsen Khakzad, Siddhesh Sawant, Xuyang Gao, Shalini Thakur, James John Brooke, Cédric Prieels, Christophe Royon, Elizabeth Sexton-Kennedy, Vladimir Andreev, Aruna Nayak, Kerstin Borras, Praveen Chandra Tiwari, Martina Ressegotti, Álvaro Navarro Tobar, Federica Legger, Tuure Tuuva, Oleksii Turkot, Fabrizio Gasparini, Michele Selvaggi, Markus Spanring, Soumya Mukherjee, Michael Krohn, Jeremie Alexandre Merlin, Piotr Zalewski, Andre David Tinoco Mendes, Robert Clare, Cristina Martin Perez, Lucas Torterotot, Patrizia Azzi, Luis Ignacio Estevez Banos, Daniel R Claes, Gulsen Onengut, Xinmei Niu, Viktor Matveev, Bobae Kim, Matthias Wolf, Paolo Ronchese, Badder Marzocchi, Sanjay Kumar Swain, Marc M Baarmand, Daniele Trocino, Silvia Maselli, Rhys Taus, Christoph Grab, Zhaozhong Shi, Henning Kirschenmann, Edouard Boos, Daniele Bonacorsi, Nicholas Haubrich, Emilien Chapon, M. R. Di Domenico, Vittorio Raoul Tavolaro, Clemens Lange, Roberto Dell'Orso, Santiago Folgueras, George Alverson, Roman Kogler, Satoshi Hasegawa, Margaret Zientek, Liam Wezenbeek, Yuta Takahashi, Sioni Summers, Mikko Voutilainen, Sumit Keshri, Sergey Troshin, Gervasio Gomez, Gregory Iles, Donghyun Song, David Stuart, Alice Mignerey, Giacomo Fedi, David D'Enterria, Liliana Teodorescu, Adolf Bornheim, Aaron Bundock, Katerina Lipka, Andrew Wildridge, Unki Yang, Sangeun Lee, Thomas Hebbeker, Paul Lecoq, Ozgun Kara, Ramkrishna Sharma, Daniel Gastler, Alain Givernaud, Seth Moortgat, Alessandro Rossi, Fatma Aydogmus Sen, Archana Sharma, Ravindra Kumar Verma, Stefanos Leontsinis, Chayanit Asawatangtrakuldee, Lucia Silvestris, Neeti Parashar, Klaus Rabbertz, Mark Pesaresi, Claudia Ciocca, Kaitlin Salyer, Dragos Velicanu, Agostino De Iorio, Nuno Leonardo, Markus Seidel, Vaia Papadimitriou, Vineet Kumar, Muhammad Waqas, Izaak Neutelings, Sebastiano Albergo, Hui Wang, Tyler Mitchell, Yasser Mohammed, Ian Laflotte, Winston Ko, Reza Goldouzian, Mohd Nizam Yusli, Vivan Nguyen, Ksenia Shchelina, Albert M. Sirunyan, Steffie Ann Thayil, Gaël Touquet, Jeremi Niedziela, Aleksandr Iuzhakov, Sándor Lökös, Philip Keicher, Vladimir Epshteyn, Helio Nogima, Vinay Hegde, Saptaparna Bhattacharya, David Zou, Finn Feindt, Ashutosh Bhardwaj, Martin Kirakosyan, Oliver Rieger, Georgios Bakas, Andrey Korytov, Nairit Sur, Javier Andres Brochero Cifuentes, P. Chang, Elif Asli Yetkin, James Alexander, Lukasz Kreczko, Alberto Orso Maria Iorio, Sanghyun Ko, Byung-Sik Hong, Mahmod Moussa Abdelkhalek Gadallah, Atul Gurtu, Michael Hildreth, Oscar Gonzalez Lopez, Felice Pantaleo, Chanwook Hwang, Tanmay Sarkar, Matthew Joyce, Simone Giani, Rosamaria Venditti, Anastasia Karavdina, Gian Mario Bilei, Bożena Boimska, Antonio Delgado Peris, Caterina Aruta, Flavia Cetorelli, Kerem Cankocak, Eduardo De Moraes Gregores, Ashfaq Ahmad, Vladimir Korenkov, Harrison Prosper, Benjamin Krikler, Mario Deile, Stephen Robert Wagner, Kak Wong, Georgy Antchev, Ioanna Papavergou, David Sperka, Gaelle Boudoul, Alexis Kalogeropoulos, Apichart Hortiangtham, Dezso Horvath, David Walter, Matthias Schröder, Predrag Milenovic, Peter R Hobson, Kin Ho Lo, Chiara Amendola, Giorgia Rauco, Nancy Marinelli, Renato Potenza, Metin Yalvac, Stephan Lammel, Tagir Aushev, Daniel Noonan, Alexander Nikitenko, Ashim Roy, Vladislav Shalaev, Daniel Diaz, Kyungwook Nam, Sudarshan Paramesvaran, Victor Daniel Elvira, Max Philip Rauch, Frans Meijers, Stephen Trembath-Reichert, Igor Lokhtin, Antonio Di Pilato, Zachary Lesko, Gabriella Pugliese, Rachel Yohay, Hessamoddin Kaveh, Edward Scott, Andre Frankenthal, Timothy Koeth, Jan Krolikowski, Luiz Mundim, Kelci Mohrman, Guenter Eckerlin, Armen Tumasyan, Paula Eerola, Manoj Sharan, Jasvinder A. Singh, Andris Skuja, Jaebeom Park, Jingzhou Zhao, Branislav Ristic, Balashangar Kailasapathy, Ricardo Lopez-Fernandez, Christina Reissel, Ryan Mueller, Illia Babounikau, Torben Dreyer, Alessia Tricomi, Hyunchul Kim, Zhixing Wang, Dipanwita Dutta, Meena Meena, Peter Meiring, Tribeni Mishra, Alexei Safonov, Duccio Abbaneo, Matteo Bonanomi, Isa Dumanoglu, Elizabeth Locci, Sheila Mara Silva Do Amaral, Lata Panwar, Bilal Kiani, Ilaria Vai, Maciej Malawski, Kevin Lannon, Stephane Cooperstein, Barbara Chazin Quero, Nikolay Tyurin, Roumyana Hadjiiska, Pedro Silva, Regina Demina, Olaf Behnke, Reyer Band, Manfred Paulini, Arkadios Manousakis-Katsikakis, Igor Smirnov, Ivica Puljak, Hans Reithler, Xin Chen, Teresa Rodrigo, Tom Cornelis, Shivali Malhotra, Gunter Quast, Jordan Nash, Tanmay Mudholkar, Ennio Monteil, Aldo Penzo, Nicolas Tonon, Artur Gottmann, Peter Raics, Peicho Petkov, Sicheng Wang, Gabriele Benelli, Janos Erö, Michael Revering, Plamen Iaydjiev, Erik Brücken, Achille Petrilli, Jessica Prisciandaro, Pierluigi Bortignon, Kenyi Hurtado Anampa, Younes Otarid, Leszek Grzanka, Robert M Harris, Ben Bylsma, Roberto Tenchini, Meng Xiao, Fan Xia, Dietrich Liko, Mykhailo Dalchenko, Hamed Bakhshiansohi, Guenakh Mitselmakher, Tamás Álmos Vámi, Sungwoong Cho, Zhengyun You, Kristian Harder, Mia Tosi, Andrew Mehta, Somnath Choudhury, Jacobo Konigsberg, Young Do Oh, Zhicai Zhang, Sung Keun Park, Prashant Shukla, John Alison, Shimaa Abu Zeid, Aliakbar Ebrahimi, Vladimir Petrov, Sushil Chauhan, Aimilios Ioannou, Milan Stojanovic, Kajari Mazumdar, Nickolas Mccoll, Evgueni Vlasov, André Rosowsky, Andrew Ivanov, Karl Ehataht, Thomas N. Williams, Julia Velkovska, Qianying Guo, Enrico Robutti, G. Zumerle, Pieter Everaerts, Sourabh Dube, Sam Harper, Kerstin Hoepfner, Eirini Tziaferi, Richard Loveless, Veikko Karimäki, Nicola Cavallo, Sudha Ahuja, Nikolai Gorbounov, Halil Saka, Pietro Govoni, Svenja Schumann, Rui Xiao, Kevin Burkett, Kisoo Lee, Lalit Mohan Pant, Elliot Hughes, Gurpreet Singh Chahal, Andrew Buccilli, Kinga Anna Wozniak, Ruchi Chudasama, Stephen Sanders, Wesley H Smith, Bryan Cardwell, Matteo Cremonesi, Shuichi Kunori, Ilia Zhizhin, Paolo Azzurri, Arun Kumar, Marc Huwiler, Daniele Spiga, Jordan Damgov, Piotr Traczyk, D. 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A., Acosta, G., Oliveros, S., Avdeeva, E., Bloom, K., Claes, D. R., Fangmeier, C., Golf, F., Suarez, R. Gonzalez, Kamalieddin, R., Kravchenko, I., Monroy, J., Siado, J. E., Snow, G. R., Stieger, B., Godshalk, A., Harrington, C., Iashvili, I., Kharchilava, A., Mclean, C., Nguyen, D., Parker, A., Rappoccio, S., Roozbahani, B., Alverson, G., Barberis, E., Freer, C., Hortiangtham, A., Morse, D. M., Orimoto, T., De Lima, R. Teixeira, Wamorkar, T., Wang, B., Wisecarver, A., Wood, D., Charaf, O., Hahn, K. A., Mucia, N., Odell, N., Schmitt, M. H., Sevova, S., Sung, K., Trovato, M., Velasco, M., Bucci, R., Dev, N., Hildreth, M., Anampa, K. Hurtado, Jessop, C., Karmgard, D. J., Kellams, N., Lannon, K., Li, W., Loukas, N., Marinelli, N., Meng, F., Mueller, C., Musienko, Y., Planer, M., Reinsvold, A., Ruchti, R., Siddireddy, P., Smith, G., Taroni, S., Wayne, M., Wightman, A., Wolf, M., Woodard, A., Alimena, J., Antonelli, L., Bylsma, B., Durkin, L. S., Flowers, S., Francis, B., Hart, A., Hill, C., Ji, W., Ling, T. Y., Luo, W., Winer, B. L., Wulsin, H. W., Cooperstein, S., Elmer, P., Hardenbrook, J., Higginbotham, S., Kalogeropoulos, A., Lange, D., Lucchini, M. T., Luo, J., Marlow, D., Mei, K., Ojalvo, I., Olsen, J., Palmer, C., Piroue, P., Salfeld-Nebgen, J., Stickland, D., Tully, C., Norberg, S., Barker, A., Barnes, V. E., Das, S., Gutay, L., Jones, M., Jung, A. W., Khatiwada, A., Mahakud, B., Miller, D. H., Neumeister, N., Peng, C. C., Qiu, H., Schulte, J. F., Sun, J., Wang, F., Xiao, R., Xie, W., Cheng, T., Dolen, J., Parashar, N., Chen, Z., Ecklund, K. M., Freed, S., Geurts, F. J. M., Kilpatrick, M., Michlin, B., Padley, B. P., Roberts, J., Rorie, J., Shi, W., Tu, Z., Zabel, J., Zhang, A., Bodek, A., de Barbaro, P., Demina, R., Duh, Y. t., Dulemba, J. L., Fallon, C., Ferbel, T., Galanti, M., Garcia-Bellido, A., Han, J., Hindrichs, O., Khukhunaishvili, A., Lo, K. H., Tan, P., Taus, R., Verzetti, M., Agapitos, A., Chou, J. P., Gershtein, Y., Espinosa, T. A. Gomez, Halkiadakis, E., Heindl, M., Hughes, E., Kaplan, S., Elayavalli, R. Kunnawalkam, Kyriacou, S., Lath, A., Montalvo, R., Nash, K., Osherson, M., Saka, H., Salur, S., Schnetzer, S., Sheffield, D., Somalwar, S., Stone, R., Thomas, S., Thomassen, P., Walker, M., Delannoy, A. G., Heideman, J., Riley, G., Spanier, S., Thapa, K., Bouhali, O., Celik, A., Dalchenko, M., De Mattia, M., Delgado, A., Dildick, S., Eusebi, R., Gilmore, J., Huang, T., Kamon, T., Luo, S., Mueller, R., Patel, R., Perloff, A., Pernie, L., Rathjens, D., Safonov, A., Akchurin, N., Damgov, J., De Guio, F., Dudero, P. R., Kunori, S., Lamichhane, K., Mengke, T., Muthumuni, S., Peltola, T., Undleeb, S., Volobouev, I., Greene, S., Gurrola, A., Janjam, R., Johns, W., Maguire, C., Melo, A., Ni, H., Padeken, K., Alvarez, J. D. Ruiz, Sheldon, P., Tuo, S., Velkovska, J., Verweij, M., Xu, Q., Arenton, M. W., Barria, P., Cox, B., Hirosky, R., Joyce, M., Ledovskoy, A., Li, H., Neu, C., Sinthuprasith, T., Wolfe, E., Xia, F., Harr, R., Karchin, P. E., Poudyal, N., Sturdy, J., Thapa, P., Zaleski, S., Brodski, M., Buchanan, J., Caillol, C., Carlsmith, D., Dasu, S., Dodd, L., Gomber, B., Grothe, M., Herndon, M., Herve, A., Hussain, U., Klabbers, P., Lanaro, A., Long, K., Loveless, R., Ruggles, T., Savin, A., Smith, N., Smith, W. H., Woods, N., Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Laboratoire Leprince-Ringuet (LLR), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-École polytechnique (X)-Centre National de la Recherche Scientifique (CNRS), Institut Pluridisciplinaire Hubert Curien (IPHC), Université de Strasbourg (UNISTRA)-Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA)), Institut de Physique Nucléaire de Lyon (IPNL), Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Laboratoire d'Annecy de Physique des Particules (LAPP), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS), CMS, Department of Physics, Helsinki Institute of Physics, Damarseçkin, Serdal, Ero, J., Escalante Del Valle, A., Fruhwirth, R., Lechner, L., Schofbeck, R., Templ, S., Litomin, A., Makarenko, V., Suarez Gonzalez, J., Darwish, M. R., Kello, T., Rejeb Sfar, H., Van Putte, S., Bols, E. S., Muller, D., Makarenko, I., Moureaux, L., Petre, L., Wezenbeek, L., Gruchala, M., Bury, F., Donertas, I. S., Prisciandaro, J., Taliercio, A., Teklishyn, M., Wuyckens, S., Alda Junior, W. L., Brandao Malbouisson, H., Martins, J., Medina Jaime, M., Silva Do Amaral, S. M., Lemos, D. S., Padula, S. S., Antchev, G., Atanasov, I., Ivanov, T., Petrov, A., Guo, Q., Yi, K., Javaid, T., Liu, Z. -A., Thomas-wilsker, J., Chen, C., Huang, Q., Lu, M., Lyu, X., Xiao, J., You, Z., Fraga, J., Sarkar, A., Jaramillo, J., Mejia Guisao, J., Ramirez, F., Ruiz Alvarez, J. D., Salazar Gonzalez, C. A., Vanegas Arbelaez, N., Giljanovic, D., Roguljic, M., Erodotou, E., Ioannou, A., Konstantinou, S., Tsiakkouri, D., Kveton, A., Tomsa, J., Carrera Jarrin, E., Salama, E., Mahmoud, M. A., Carvalho Antunes De Oliveira, A., Forthomme, L., Osterberg, K., Brucken, E., Garcia, F., Hamel de Monchenault, G., Lenzi, B., Bonanomi, M., Buchot Perraguin, A., Diab, B., Falmagne, G., Granier de Cassagnac, R., Hakimi, A., Martin Perez, C., Rembser, J., Bourgatte, G., Grimault, C., Camen, C., Carle, A., Jain, S., Lesauvage, A., Shchablo, K., Torterotot, L., Touquet, G., Meuser, D., Pauls, A., Eliseev, D., Fackeldey, P., Fischer, B., Mocellin, G., Mondal, S., Noll, D., Novak, A., Rath, Y., Roemer, J., Schuler, S. C., Wiedenbeck, S., Dziwok, C., Flugge, G., Haj Ahmad, W., Ziemons, T., Aarup Petersen, H., Aldaya Martin, M., Asmuss, P., Baxter, S., Bermudez Martinez, A., Brunner, D., Cardini, A., Consuegra Rodriguez, S., Didukh, L., Dominguez Damiani, D., Eckstein, D., Estevez Banos, L. I., Giraldi, A., Jomhari, N. Z., Kasem, A., Kaveh, H., Krucker, D., Lidrych, J., Metwally, J., Mussgiller, A., Otarid, Y., Perez Adan, D., Saibel, A., Scheurer, V., Sosa Ricardo, R. E., Walter, D., Wuchterl, S., Zlebcik, R., De Leo, K., Ebrahimi, A., Eich, M., Feindt, F., Frohlich, A., Garbers, C., Kramer, T., Lange, T., Malara, A., Niemeyer, C. E. N., Nigamova, A., Pena Rodriguez, K. J., Schwarz, D., Steinbruck, G., Zoi, I., Bechtel, J., Berger, T., Droll, A., Floh, K., Gottmann, A., Heidecker, C., Keicher, P., Koppenhofer, R., Maier, S., Metzler, M., Rauser, J., Savoiu, D., Schafer, D., Schnepf, M., Seith, D., Wassmer, M., Wozniewski, S., Asenov, P., Diamantopoulou, M., Karasavvas, D., Koraka, C. K., Manousakis-katsikakis, A., Vourliotis, E., Bakas, G., Zacharopoulou, A., Manitara, K., Gadallah, M. M. A., Lokos, S., Csorgo, T., Nemes, F., Novak, T., Kumar, D., Panwar, L., Dash, D., Mishra, T., Muraleedharan Nair Bindhu, V. K., Chaudhary, G., Meena, M., Virdi, A. K., Ahmed, A., Kumar, A., Shah, A., Palit, P., Sahu, B., Behera, S. C., Kalbhor, P., Muhammad, A., Pradhan, R., Pujahari, P. R., Sikdar, A. K., Naskar, K., Kumar Verma, R., Sarkar, U., Kansal, B., Rastogi, A., Mohammadi Najafabadi, M., Aly, R., Aruta, C., Di Pilato, A., Elmetenawee, W., Margjeka, I., Mastrapasqua, V., Simone, F. M., Diotalevi, T., Fontanesi, E., Giommi, L., Lo Meo, S., Costa, S., Cassese, A., Ceccarelli, R., Lizzo, M., Seidita, R., Bozzo, M., Mulargia, R., Cetorelli, F., Dini, P., Guzzi, L., Monti, F., Tabarelli de Fatis, T., Valsecchi, D., De Iorio, A., Rossi, B., Bisello, D., De Castro Manzano, P., Layer, L., Presilla, M., Yarar, H., Aime, C., Calzaferri, S., Fiorina, D., Moscatelli, F., Piccinelli, A., Tedeschi, T., Bertacchi, V., Di Domenico, M. R., Roy Chowdhury, S., Scribano, A., Shafiei, N., Turini, N., Di Marco, E., Quaranta, C., Tramontano, R., Bellora, A., Berenguer Antequera, J., Cappati, A., Legger, F., Pinna Angioni, G. L., Salvatico, R., Siviero, F., Tornago, M., Da Rold, A., Dogra, S., Huh, C., Kim, B., Pak, S. I., Park, J., Gurtu, A., Kim, Y., Bhyun, J. H., Choi, J., Jeon, S., Ko, S., Kwon, H., Oh, B. H., Oh, M., Seo, H., Yoon, I., Ko, B., Song, D., Watson, I. J., Jeong, Y., Lee, Y., Maghrbi, Y., Tamulaitis, G., Vaitkevicius, A., Wan Abdullah, W. A. T., Benitez, J. F., Castaneda Hernandez, A., Murillo Quijada, J. A., Valencia Palomo, L., Ayala, G., Mondragon Herrera, C. A., Perez Navarro, D. A., Carrillo Moreno, S., Oropeza Barrera, C., Vazquez Valencia, F., Salazar Ibarguen, H. A., Uribe Estrada, C., Morelos Pineda, A., Mijuskovic, J., Raicevic, N., Awais, A., Awan, M. I. M., Avati, V., Grzanka, L., Malawski, M., Kalinowski, A., Bastos, D., Niknejad, T., Gorbunov, I., Karjavine, V., Korenkov, V., Shalaev, V., Shulha, S., Teryaev, O., Yuldashev, B. S., Zhizhin, I., Gavrilov, G., Golovtcov, V., Volkov, S., Andreev, Y., Pivovarov, G., Oskin, A., Bunichev, V., Ovtin, I., Iuzhakov, A., Sukhikh, L., Borchsh, V., Ivanchenko, V., Tcherniaev, E., Aguilar-Benitez, M., Bedoya, C. F., Leon Holgado, J., Navarro Tobar, A., Sanchez Navas, S., Urda Gomez, L., Willmott, C., Alvarez Gonzalez, B., Ramon Alvarez, C., Ripoll Sau, J., Trapote, A., Jayananda, M., Kailasapathy, B., Sonnadara, D. U. J., Wickramarathna, D., Dharmaratna, W. G. D., Liyanage, K., Perera, N., Wickramage, N., Baechler, J., Bossini, E., Deile, M., Emriskova, N., Giani, S., Kaspar, J., Kratochwil, N., Quast, T., Scarfi, S., Snoeys, W., Wozniak, K. A., Calandri, A., Gadek, T., Gomez Espinosa, T. A., Lyon, A. -M., Niedziela, J., Perovic, V., Ratti, M. G., Reichmann, M., Reissel, C., Reitenspiess, T., Ristic, B., Sanz Becerra, D. A., Stampf, V., Vesterbacka Olsson, M. L., Huwiler, M., Jofrehei, A., Macchiolo, A., Meiring, P., Mikuni, V. M., Molinatti, U., Adloff, C., Ceard, L., Li, Y., Eskut, E., Gurpinar Guler, E., Kayis Topaksu, A., Simsek, A. E., Ocalan, K., Ozcelik, O., Aydogmus Sen, F., Kaynak, B., Sunar Cerci, D., Bhal, E., Bologna, S., Krikler, B., Seif El Nasr-Storey, S., Stylianou, N., Ellis, K. V., Manolopoulos, K., Schuh, T., Bonomally, S., Cepaitis, V., Chahal, G. S., Langford, J., Milosevic, V., Raymond, D. M., Webb, S. N., Zecchinelli, A. G., Caraway, B., Kanuganti, A. R., Sawant, S., Wilson, J., Uniyal, R., Vargas Hernandez, A. M., Perez, C. U., Akpinar, A., Cosby, C., Salyer, K., Yuan, S., Burkle, B., Duh, Y., Lau, K. T., Wong, W. Y., Zhang, W., Calderon De La Barca Sanchez, M., Yao, Y., Hamilton, D., Iqbal, M. A., Lam, T., Nash, W. A., Stone, B., Manganelli, N., Olmedo Negrete, M., Zhang, Y., May, S., Dorsett, A., Marsh, B., Quinnan, M., Cerri, O., Dutta, I., Lu, N., Mao, J., Alison, J., Cranshaw, D. J., Frankenthal, A., Sun, W., Herwig, T. C., Papadimitriou, V., Reinsvold Hall, A., Guerrero, D., Kim, M., Menendez, N., Rosenzweig, D., Yigitbasi, E., Zuo, X., Diaz, D., Habibullah, R., Butalla, S., Elkafrawy, T., Saunders, M., Becerril Gonzalez, H., Viinikainen, J., Ye, Z., Koseyan, O. K., Amram, O., Corcodilos, L., Eminizer, M., Mantilla, C., Baldenegro Barrera, C., Isidori, T., King, J., Lindsey, C., Minafra, N., Royon, C., Tapia Takaki, J. D., Williams, J., Wilson, G., Adams, E., Koeth, T., Nabili, S., Gomez Ceballos, G., Krupa, J., Shi, Z., Hiltbrand, J., Revering, M., Saradhy, R., Schroeder, N., Acosta, J. G., Joo, C., Tabb, W., Yan, F., Agarwal, G., Bandyopadhyay, H., Hay, L., Madigan, G., Nguyen, V., Tishelman-Charny, A., Bueghly, J., Gunter, T., Hurtado Anampa, K., Mcalister, I., Mohrman, K., Zygala, L., Cardwell, B., Lefeld, A., Bonham, B., Dezoort, G., Dropulic, A., Greenberg, B., Haubrich, N., Kopp, G., Kwan, S., Kondratyev, D., Stojanovic, M., Wildridge, A., Redjimi, R., Stahl Leiton, A. G., Ranken, E., Chiarito, B., Gandrakota, A., Laflotte, I., Thayil, S. A., Acharya, H., Overton, D., Appelt, E., Cummings, G., Li, A., Tannenwald, B., Black, K., He, H., Loeliger, A., Madhusudanan Sreekala, J., Mallampalli, A., Shang, V., Teague, D., Trembath-reichert, S., Vetens, W., CMS Collaboration, Sirunyan, A, Tumasyan, A, Adam, W, Bergauer, T, Dragicevic, M, Erö, J, Escalante Del Valle, A, Frühwirth, R, Jeitler, M, Krammer, N, Lechner, L, Liko, D, Mikulec, I, Pitters, F, Rad, N, Schieck, J, Schöfbeck, R, Spanring, M, Templ, S, Waltenberger, W, Wulz, C, Zarucki, M, Chekhovsky, V, Litomin, A, Makarenko, V, Suarez Gonzalez, J, Darwish, M, De Wolf, E, Di Croce, D, Janssen, X, Kello, T, Lelek, A, Pieters, M, Rejeb Sfar, H, Van Haevermaet, H, Van Mechelen, P, Van Putte, S, Van Remortel, N, Blekman, F, Bols, E, Chhibra, S, D’Hondt, J, De Clercq, J, Lontkovskyi, D, Lowette, S, Marchesini, I, Moortgat, S, Morton, A, Müller, D, Python, Q, Tavernier, S, Van Doninck, W, Van Mulders, P, Beghin, D, Bilin, B, Clerbaux, B, De Lentdecker, G, Dorney, B, Favart, L, Grebenyuk, A, Kalsi, A, Makarenko, I, Moureaux, L, Pétré, L, Popov, A, Postiau, N, Starling, E, Thomas, L, Vander Velde, C, Vanlaer, P, Vannerom, D, Wezenbeek, L, Cornelis, T, Dobur, D, Gruchala, M, Khvastunov, I, Niedziela, M, Roskas, C, Skovpen, K, Tytgat, M, Verbeke, W, Vermassen, B, Vit, M, Bruno, G, Bury, F, Caputo, C, David, P, Delaere, C, Delcourt, M, Donertas, I, Giammanco, A, Lemaitre, V, Mondal, K, Prisciandaro, J, Taliercio, A, Teklishyn, M, Vischia, P, Wertz, S, Wuyckens, S, Alves, G, Hensel, C, Moraes, A, Aldá Júnior, W, Belchior Batista Das Chagas, E, BRANDAO MALBOUISSON, H, Carvalho, W, Chinellato, J, Coelho, E, Da Costa, E, Da Silveira, G, De Jesus Damiao, D, Fonseca De Souza, S, Martins, J, Matos Figueiredo, D, Medina Jaime, M, Mora Herrera, C, Mundim, L, Nogima, H, Rebello Teles, P, Sanchez Rosas, L, Santoro, A, Silva Do Amaral, S, Sznajder, A, Thiel, M, Torres Da Silva De Araujo, F, Vilela Pereira, A, Bernardes, C, Calligaris, L, Fernandez Perez Tomei, T, Gregores, E, Lemos, D, Mercadante, P, Novaes, S, Padula, S, Aleksandrov, A, Antchev, G, Atanasov, I, Hadjiiska, R, Iaydjiev, P, Misheva, M, Rodozov, M, Shopova, M, Sultanov, G, Dimitrov, A, Ivanov, T, Litov, L, Pavlov, B, Petkov, P, Petrov, A, Cheng, T, Fang, W, Guo, Q, Wang, H, Yuan, L, Ahmad, M, Bauer, G, Hu, Z, Wang, Y, Yi, K, Chapon, E, Chen, G, Chen, H, Chen, M, Javaid, T, Kapoor, A, Leggat, D, Liao, H, Liu, Z, Sharma, R, Spiezia, A, Tao, J, Thomas-wilsker, J, Wang, J, Zhang, H, Zhang, S, Zhao, J, Agapitos, A, Ban, Y, Chen, C, Huang, Q, Levin, A, Li, Q, Lu, M, Lyu, X, Mao, Y, Qian, S, Wang, D, Wang, Q, Xiao, J, You, Z, Gao, X, Xiao, M, Avila, C, Cabrera, A, Florez, C, Fraga, J, Sarkar, A, Segura Delgado, M, Jaramillo, J, Mejia Guisao, J, Ramirez, F, Ruiz Alvarez, J, Salazar González, C, Vanegas Arbelaez, N, Giljanovic, D, Godinovic, N, Lelas, D, Puljak, I, Antunovic, Z, Kovac, M, Sculac, T, Brigljevic, V, Ferencek, D, Majumder, D, Roguljic, M, Starodumov, A, Susa, T, Ather, M, Attikis, A, 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Gerosa R., Gilbert D., Krutelyov V., Letts J., Masciovecchio M., May S., Padhi S., Pieri M., Sharma V., Tadel M., Wurthwein F., Yagil A., Amin N., Campagnari C., Citron M., Dorsett A., Dutta V., Incandela J., Marsh B., Mei H., Ovcharova A., Qu H., Quinnan M., Richman J., Sarica U., Stuart D., Wang S., Bornheim A., Cerri O., Dutta I., Lawhorn J.M., Lu N., Mao J., Newman H.B., Ngadiuba J., Nguyen T.Q., Pata J., Spiropulu M., Vlimant J.R., Wang C., Xie S., Zhang Z., Zhu R.Y., Alison J., Andrews M.B., Ferguson T., Mudholkar T., Paulini M., Sun M., Vorobiev I., Cumalat J.P., Ford W.T., MacDonald E., Mulholland T., Patel R., Perloff A., Stenson K., Ulmer K.A., Wagner S.R., Alexander J., Cheng Y., Chu J., Cranshaw D.J., Datta A., Frankenthal A., Mcdermott K., Monroy J., Patterson J.R., Quach D., Ryd A., Sun W., Tan S.M., Tao Z., Thom J., Wittich P., Zientek M., Albrow M., Alyari M., Apollinari G., Apresyan A., Apyan A., Bauerdick L.A.T., Beretvas A., Berry D., Berryhill J., Bhat P.C., Burkett K., Butler J.N., Canepa A., Cerati G.B., Cheung H.W.K., Chlebana F., Cremonesi M., Elvira V.D., Freeman J., Gecse Z., Gottschalk E., Gray L., Green D., Grunendahl S., Gutsche O., Harris R.M., Hasegawa S., Heller R., Herwig T.C., Hirschauer J., Jayatilaka B., Jindariani S., Johnson M., Joshi U., Klabbers P., Klijnsma T., Klima B., Kortelainen M.J., Lammel S., Lincoln D., Lipton R., Liu M., Liu T., Lykken J., Maeshima K., Mason D., McBride P., Merkel P., Mrenna S., Nahn S., O'Dell V., Papadimitriou V., Pedro K., Pena C., Prokofyev O., Ravera F., Reinsvold Hall A., Ristori L., Schneider B., Sexton-Kennedy E., Smith N., Soha A., Spalding W.J., Spiegel L., Stoynev S., Strait J., Taylor L., Tkaczyk S., Tran N.V., Uplegger L., Vaandering E.W., Weber H.A., Woodard A., Acosta D., Avery P., Bourilkov D., Cadamuro L., Cherepanov V., Errico F., Field R.D., Guerrero D., Joshi B.M., Kim M., Konigsberg J., Korytov A., Lo K.H., Matchev K., Menendez N., Mitselmakher G., Rosenzweig D., Shi K., Sturdy J., Yigitbasi E., Zuo X., Adams T., Askew A., Diaz D., Habibullah R., Hagopian S., Hagopian V., Johnson K.F., Khurana R., Kolberg T., Martinez G., Prosper H., Schiber C., Yohay R., Zhang J., Baarmand M.M., Butalla S., Elkafrawy T., Hohlmann M., Noonan D., Rahmani M., Saunders M., Yumiceva F., Adams M.R., Apanasevich L., Becerril Gonzalez H., Cavanaugh R., Chen X., Dittmer S., Evdokimov O., Gerber C.E., Hangal D.A., Hofman D.J., Mills C., Oh G., Roy T., Tonjes M.B., Varelas N., Viinikainen J., Wang X., Wu Z., Ye Z., Alhusseini M., Dilsiz K., Durgut S., Gandrajula R.P., Haytmyradov M., Khristenko V., Koseyan O.K., Merlo J.-P., Mestvirishvili A., Moeller A., Nachtman J., Ogul H., Onel Y., Ozok F., Penzo A., Snyder C., Tiras E., Wetzel J., Amram O., Blumenfeld B., Corcodilos L., Eminizer M., Gritsan A.V., Kyriacou S., Maksimovic P., Mantilla C., Roskes J., Swartz M., Vami T.A., Baldenegro Barrera C., Baringer P., Bean A., Bylinkin A., Isidori T., King J., Krintiras G., Kropivnitskaya A., Lindsey C., Minafra N., Murray M., Rogan C., Royon C., Sanders S., Schmitz E., Tapia Takaki J.D., Williams J., Wilson G., Duric S., Ivanov A., Kaadze K., Kim D., Maravin Y., Mitchell T., Modak A., Mohammadi A., Rebassoo F., Wright D., Adams E., Baden A., Baron O., Belloni A., Eno S.C., Feng Y., Hadley N.J., Jabeen S., Jeng G.Y., Kellogg R.G., Koeth T., Mignerey A.C., Nabili S., Seidel M., Skuja A., Tonwar S.C., Wang L., Wong K., Abercrombie D., Allen B., Bi R., Brandt S., Busza W., Cali I.A., D'Alfonso M., Gomez Ceballos G., Goncharov M., Harris P., Hsu D., Hu M., Klute M., Kovalskyi D., Krupa J., Lee Y.-J., Luckey P.D., Maier B., Marini A.C., Mcginn C., Mironov C., Narayanan S., Niu X., Paus C., Rankin D., Roland C., Roland G., Shi Z., Stephans G.S.F., Sumorok K., Tatar K., Velicanu D., Wang T.W., Wang Z., Wyslouch B., Chatterjee R.M., Evans A., Hansen P., Hiltbrand J., Krohn M., Kubota Y., Lesko Z., Mans J., Revering M., Rusack R., Saradhy R., Schroeder N., Strobbe N., Wadud M.A., Acosta J.G., Oliveros S., Bloom K., Claes D.R., Fangmeier C., Finco L., Golf F., Gonzalez Fernandez J.R., Joo C., Kravchenko I., Siado J.E., Snow G.R., Tabb W., Yan F., Agarwal G., Bandyopadhyay H., Harrington C., Hay L., Iashvili I., Kharchilava A., McLean C., Nguyen D., Pekkanen J., Rappoccio S., Roozbahani B., Alverson G., Barberis E., Freer C., Haddad Y., Hortiangtham A., Li J., Madigan G., Marzocchi B., Morse D.M., Nguyen V., Orimoto T., Parker A., Skinnari L., Tishelman-Charny A., Wamorkar T., Wang B., Wisecarver A., Wood D., Bueghly J., Chen Z., Gilbert A., Gunter T., Hahn K.A., Odell N., Schmitt M.H., Sung K., Velasco M., Bucci R., Dev N., Goldouzian R., Hildreth M., Hurtado Anampa K., Jessop C., Karmgard D.J., Lannon K., Loukas N., Marinelli N., Mcalister I., Meng F., Mohrman K., Musienko Y., Ruchti R., Siddireddy P., Taroni S., Wayne M., Wightman A., Wolf M., Zygala L., Alimena J., Bylsma B., Cardwell B., Durkin L.S., Francis B., Hill C., Lefeld A., Winer B.L., Yates B.R., Bonham B., Das P., Dezoort G., Dropulic A., Elmer P., Greenberg B., Haubrich N., Higginbotham S., Kalogeropoulos A., Kopp G., Kwan S., Lange D., Lucchini M.T., Luo J., Marlow D., Mei K., Ojalvo I., Olsen J., Palmer C., Piroue P., Stickland D., Tully C., Norberg S., Barnes V.E., Chawla R., Das S., Gutay L., Jones M., Jung A.W., Kondratyev D., Negro G., Neumeister N., Peng C.C., Piperov S., Purohit A., Qiu H., Schulte J.F., Stojanovic M., Trevisani N., Wang F., Wildridge A., Xiao R., Xie W., Dolen J., Parashar N., Baty A., Dildick S., Ecklund K.M., Freed S., Geurts F.J.M., Kilpatrick M., Li W., Padley B.P., Redjimi R., Roberts J., Rorie J., Shi W., Stahl Leiton A.G., Bodek A., de Barbaro P., Demina R., Dulemba J.L., Fallon C., Ferbel T., Galanti M., Garcia-Bellido A., Hindrichs O., Khukhunaishvili A., Ranken E., Taus R., Chiarito B., Chou J.P., Gandrakota A., Gershtein Y., Halkiadakis E., Hart A., Heindl M., Hughes E., Kaplan S., Karacheban O., Laflotte I., Lath A., Montalvo R., Nash K., Osherson M., Salur S., Schnetzer S., Somalwar S., Stone R., Thayil S.A., Thomas S., Acharya H., Delannoy A.G., Spanier S., Bouhali O., Dalchenko M., Delgado A., Eusebi R., Gilmore J., Huang T., Kamon T., Luo S., Malhotra S., Mueller R., Overton D., Pernie L., Rathjens D., Safonov A., Akchurin N., Damgov J., Hegde V., Kunori S., Lamichhane K., Mengke T., Muthumuni S., Peltola T., Undleeb S., Volobouev I., Whitbeck A., Appelt E., Greene S., Gurrola A., Janjam R., Johns W., Maguire C., Melo A., Ni H., Padeken K., Romeo F., Sheldon P., Tuo S., Velkovska J., Arenton M.W., Cox B., Cummings G., Hakala J., Hirosky R., Joyce M., Ledovskoy A., Li A., Neu C., Tannenwald B., Wolfe E., Xia F., Karchin P.E., Poudyal N., Thapa P., Black K., Bose T., Buchanan J., Caillol C., Dasu S., De Bruyn I., Everaerts P., Galloni C., He H., Herndon M., Herve A., Hussain U., Lanaro A., Loeliger A., Loveless R., Madhusudanan Sreekala J., Mallampalli A., Pinna D., Savin A., Shang V., Smith W.H., Teague D., Trembath-reichert S., Vetens W., Physics, Elementary Particle Physics, Faculty of Sciences and Bioengineering Sciences, and Vriendenkring VUB
Subjects: ComputerSystemsOrganization_COMPUTERSYSTEMIMPLEMENTATION, fusion [gluon gluon], 13000 GeV-cms, High energy physics, Experimental particle physics, LHC, CMS, Hadron-Hadron scattering (experiments), Higgs physics, p p: colliding beams, Higgs particle: pair production, bottom: 2, p p: scattering, Higgs particle: coupling, Higgs particle: hadroproduction, Higgs particle: decay modes, bottom: pair production, photon: pair production, top: pair production, coupling: Yukawa, coupling constant: upper limit, vector boson: fusion, mass spectrum: two-photon, Standard model, 01 natural sciences, Physics, Particles & Fields, High Energy Physics - Experiment, Vector boson, High Energy Physics - Experiment (hep-ex), Lepton production, STANDARD MODEL, PROGRAM, SEARCH, MASS, ComputingMilieux_COMPUTERSANDEDUCATION, scattering [p p], [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex], Physics, (muon+ muon-) [mass spectrum], 0105 Mathematical Physics, Large Hadron Collider, Settore FIS/01 - Fisica Sperimentale, ratio: measured [cross section], Coupling (probability), Nuclear & Particles Physics, muon: pair production, CERN LHC Coll, Higgs particle: production, category, gluon gluon: fusion, Physical Sciences, 0202 Atomic, Molecular, Nuclear, Particle and Plasma Physics, ComputingMethodologies_DOCUMENTANDTEXTPROCESSING, Physique des particules élémentaires, Higgs boson, PARTICLE PHYSICS, Production (computer science), colliding beams [p p], Particle Physics - Experiment, +muon%2B+muon%22">Higgs particle --> muon+ muon, Nuclear and High Energy Physics, Particle physics, coupling [Higgs particle], CERN Lab, FOS: Physical sciences, Higgs particle, fusion [vector boson], 114 Physical sciences, Standard Model, 0103 physical sciences, lcsh:Nuclear and particle physics. Atomic energy. Radioactivity, ddc:530, pair production [muon], Higgs particle: leptonic decay, 010306 general physics, 0206 Quantum Physics, leptonic decay [Higgs particle], Science & Technology, Muon, ComputingMilieux_THECOMPUTINGPROFESSION, LARGE HADRON COLLIDER, hep-ex, 010308 nuclear & particles physics, background, hal-02955746, High Energy Physics::Phenomenology, Física, Higgs physic, Gluon, mass spectrum: (muon+ muon-), production [Higgs particle], cross section: ratio: measured, lcsh:QC770-798, High Energy Physics::Experiment, experimental results
Abstract: CMS collaboration: et al., Evidence for Higgs boson decay to a pair of muons is presented. This result combines searches in four exclusive categories targeting the production of the Higgs boson via gluon fusion, via vector boson fusion, in association with a vector boson, and in association with a top quark-antiquark pair. The analysis is performed using proton-proton collision data at s√ = 13 TeV, corresponding to an integrated luminosity of 137 fb−1, recorded by the CMS experiment at the CERN LHC. An excess of events over the back- ground expectation is observed in data with a significance of 3.0 standard deviations, where the expectation for the standard model (SM) Higgs boson with mass of 125.38 GeV is 2.5. The combination of this result with that from data recorded at s√ = 7 and 8 TeV, corresponding to integrated luminosities of 5.1 and 19.7 fb−1, respectively, increases both the expected and observed significances by 1%. The measured signal strength, relative to the SM prediction, is 1.19+0.40−0.39(stat)+0.15−0.14(syst). This result constitutes the first evidence for the decay of the Higgs boson to second generation fermions and is the most precise measurement of the Higgs boson coupling to muons reported to date., Individuals have received support from the Marie-Curie programme and the European Research Council and Horizon 2020 Grant, contract Nos. 675440, 752730, and 765710 (European Union); the Programa Estatal de Fomento de la Investigación Científica y Técnica de Excelencia María de Maeztu, grant MDM-2015-0509 and the Programa Severo Ochoa del Principado de Asturias.
Published: 2021
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33. Neutrino windows to the origin of matter

Author: Salvador Rosauro Alcaraz, Fernández Martínez, Enrique, UAM. Departamento de Física Teórica, and Instituto de Física Teórica (IFT)
Subjects: High Energy Physics::Phenomenology, Física, High Energy Physics::Experiment, Neutrinos, Modelo estándar (Física nuclear)
Abstract: Tesis doctoral inédita leída en la Universidad Autónoma de Madrid, Facultad de Ciencias, Departamento de Física Teórica. Fecha de lectura: 01-10-2021, The Standard Model of particle Physics (SM) is a quantum eld theory based on the SU(3)c SU(2)L U(1)Y gauge group, which has so far precisely described strong and electroweak interactions between elementary particles. We know, however, that the SM cannot be the end of the story, as it is not able to give a consistent description of gravity. Thus, the SM has to be the low energy version of a more complete theory. Besides, there are other questions, both experimental and theoretical ones, which the SM cannot answer that call for the existence of Physics beyond the Standard Model (BSM). On the experimental side, the observation of non-baryonic particle dark matter (DM) in the Universe through its gravitational e ects call for an extension of the SM to include such new states. Additionally, through Big Bang nucleosynthesis (BBN) and CMB observations, we know that there is an imbalance between matter and antimatter. However, even though the SM has all the necessary ingredients to explain such an asymmetry, it was shown that it cannot generate the observed imbalance between baryons and antibaryons, such that BSM Physics is also necessary to explain this fact. Moreover, we have overwhelming evidence for BSM Physics from the observation of the neutrino oscillation phenomenon. This is arguably the clearest signal for BSM Physics from laboratory experiments. Thus, the neutrino sector seems a particularly green eld area of investigation in order to nd new Physics and to relating di erent open problems of the SM. This thesis focuses on the study of a future neutrino super beam to study neutrino oscillations and probe for the still unknown parameters characterizing the neutrino sector, such as CP violation, and the neutrino mass ordering. Secondly, we study the possibility that the DM is primarily interacting with neutrinos through the neutrino portal, and that therefore large neutrino detectors acting as observatories might be our best probe to explore the dark sector. Later on we will consider the possibility that a keV neutrino arising from the neutrino mass mechanism could be itself the DM. In the third part we will study the possible relation between the neutrino mass mechanism and the matter-antimatter asymmetry
Published: 2021

34. 4-Forms and Membranes: From the Flux Potential to the Swampland

Author: Herráez Escudero, Alvaro, Ibañez Santiago, Luis Enrique, UAM. Departamento de Física Teórica, Instituto de Física Teórica (IFT), and Ibáñez Santiago, Luis Enrique
Subjects: Teoría de flujo potencial, Física, Membranas
Abstract: Tesis doctoral inédita leída en la Universidad Autónoma de Madrid, Facultad de Ciencias, Departamento de Física Teórica. Fecha de lectura: 11-09-2020, Esta tesis tiene embargado el acceso al texto completo hasta el 11-03-2022, This thesis analyzes type II string compactifications, focusing both on the structure of the scalar potential and its relation to 3-forms and membranes and on exploring several Swampland Conjectures in this context. We begin by introducing some basic concepts of type II flux compactifications on Calabi-Yau (orientifolds). The corresponding moduli space is introduced and its structure is examined, giving some remarks on mirror symmetry, too. The flux induced superpotential is also reviewed. The structure of the perturbative flux-induced potential is the object of study of the second part of the thesis. We review its formulation for type IIA Calabi-Yau orientifolds in terms of 4-dimensional 3-forms. It is found that it enjoys a generalized Dvali-Kaloper-Sorbo structure, namely it can be obtained from the couplings between Minkowski 4-forms (with saxion-dependent kinetic terms) and shift invariant axion polynomials, which depend only on fluxes and axions. Moreover, we explain how the whole potential (including the terms coming form localized sources) can be written as a bilinear of the aforementioned polynomials, which can at the same time be further factorized into an axion dependent matrix and a flux vector. This structure is interpreted microscopically in terms of the preclusion of Freed-Witten anomalies (and the Hanany-Witten effect). We obtain a very simple relation between the superpotential and what we call the master axion polynomial. Motivated by this structure of the potential in terms of 3-forms, which couple naturally to (codimension 1) membranes, we propose a correspondence between the 4-dimensional F-term N = 1 scalar potential and a system of parallel BPS membranes. In fact, it is shown how each of the different terms in the formula for the potential is in one-to-one correspondence with the exchange of 3-forms, scalars and gravitons between the membranes. Moreover, this correspondence turns out to be valid not only at the vacua of the potential, but also in the rest of field space. Finding the set of generic conditions that are fulfilled by every Effective Field Theory that can be embedded in QG is the goal of the Swampland program, and exploring this in the context of type II compactifications is the main point of the third part of this thesis. We begin by reviewing some Swampland Conjectures and then turn to the study of the Swampland Distance Conjecture for type II compactifications on a Calabi-Yau (orientifold), focusing on extended objects. We compute the masses and tensions of particles, strings and membranes arising from different Dp and NS5-branes wrapping supersymmetric cycles. The objects becoming massless or tensionless at different infinite distance points are classified, and consistency with mirror symmetry is checked, supporting the known result that further non-geometric objects are needed. Additionally, we construct the infinite monodromy orbits of membranes. Moreover, we investigate toroidal models and relate the previously found tensionless membranes with the Weak Gravity Conjecture and the prevention of higherform symmetries from becoming global at the infinite distance points. The gauge couplings going to zero at such points are identified and verified to correspond exactly to the 3-forms that couple to the tensionless membranes. We finish by examining Scale Separation in a particular class of type II compactifications on twisted tori. Taking into account the full 10-dimensional picture turns out to be crucial. In fact, the backreaction of the internal geometry is seen to modify the results from the naive 4-dimensional EFT, which appeared to violate the relevant conjectures, in the right way for them to be satisfied
Published: 2020

35. Study of mesonic observables from a mixed action lattice QCD formalism

Author: Romero Jurado, José Ángel, Herdoiza Bolaños, Gregorio (dir.), UAM. Departamento de Física Teórica, Instituto de Física Teórica (IFT), and Herdoiza Bolaños, Gregorio
Subjects: High Energy Physics::Lattice, High Energy Physics::Phenomenology, Quarks - Propiedades - Tesis doctorales, Física, High Energy Physics::Experiment, Materia - Composición - Tesis doctorales
Abstract: Tesis doctoral inédita leída en la Universidad Autónoma de Madrid, Facultad de Ciencias, Departamento de Física Teórica. Fecha de lectura: 17-04-2020, Presentamos una acción mixta para QCD en el retículo donde los fermiones del sector del mar son discretizados mediante una acción Nf = 2+1 no perturbativa sin efectos de discretización O(a). Asimismo, los fermiones de valencia son rotados quiralmente a un punto donde la masa de quark tiene únicamente componente quiral y la masa estándar se anula. Se discuten dos alternativas para hacer la correspondencia entre las masas de los quarks del sector del mar y de valencia. Llevamos a cabo un control de la validez de la acción mixta mediante una comparación de la extrapolación al continuo de las masas de quarks y de los factores de decaimiento mesonicos de dicha acción con la acción unitaria Wilson. Se implementa un método para fijar la escala reticular y determinar las masas de quarks del sector ligero y extraño. Se presta particular atención al análisis estadístico de los resultados y a la estimación del error sistemático, We propose a Lattice QCD mixed-action approach in with sea quarks regularize using Nf = 2 + 1 non-perturbatively O(a)-improved Wilson fermions with open boundary conditions in the time direction, while a Wilson twisted mass action at maximal twist is used for valence quarks. In this setup, fermionic observables are free from O(a) lattice artifacts proportional to the valence quark masses. Two alternative procedures for the matching of sea and valence quark masses are discussed. We perform a universality check by comparing continuum limit extrapolations of the quark masses and of the pseudoscalar meson decay constants obtained with two setups: the mixed action and the standard approach where Wilson fermions are used in sea and valence sectors. We use the gradient flow scale t0 and physical input from the pion and kaon decay constants to carry out a scale setting procedure. This is applied to the determination of the light and strange quark masses. A particular attention is given to the statistical analysis of the lattice data and to the assessment of the systematic uncertainties
Published: 2020

36. Black holes in string theory with higher-derivative corrections

Author: Ruipérez Vicente, Alejandro, Ortín Miguel, Tomás (dir.), Fernández Ramírez, Pedro (dir.), UAM. Departamento de Física Teórica, Instituto de Física Teórica (IFT), Ortín Miguel, Tomás, and Fernández Ramírez, Pedro
Subjects: General Relativity and Quantum Cosmology, High Energy Physics::Theory, Cuerdas, teoría de las, Física, Agujeros negros (Astronomía)
Abstract: Tesis doctoral inédita leída en la Universidad Autónoma de Madrid, Facultad de Ciencias, Departamento de Física Teórica. Fecha de lectura: 23-09-2020, The low-energy limit of superstring theories admits a description in terms of an effective eld theory for its massless modes. The corresponding action is given by a double perturbative expansion in gs, the string coupling, and in 0, the square of the string length. The leading term of this expansion is given by one of the different ten-dimensional supergravity theories, whereas subleading terms involve terms of higher order in derivatives. The work presented in this thesis is the result of a research program that starts with the study of supersymmetric solutions of gauged supergravity and reaches the summit with the understanding of the effects produced by the 0 corrections to solutions of the heterotic superstring e ective action. This thesis is divided in two parts. The rst one focuses on the supersymmetric solutions of a minimal extension of the STU model of N = 1; d = 5 supergravity whose main interest lies on the fact that it can be obtained as a toroidal compacti cation of ten-dimensional N = 1 supergravity coupled to a triplet of SU(2) gauge elds. Concretely, we construct and study solutions describing black holes and smooth horizonless geometries with non-trivial Yang-Mills elds. The understanding of this type of solutions from the framework of string theory serves as a motivation for the work of the second part of the thesis, which is devoted to the study of solutions of the effective action of the heterotic string at rst order in 0. The latter does not simply coincide with the action of N = 1; d = 10 supergravity coupled to a Yang-Mills vector multiplet as the Green-Schwarz anomaly cancellation mechanism and supersymmetry enforce us to introduce additional terms in the action. These terms are constructed out of the spin connection with torsion given by the eld strength associated to the Kalb-Ramond 2-form and their contributions to the equations of motion are analogous to those of the Yang-Mills elds. This fact is exploited to construct analytic supersymmetric black-hole solutions with 0 corrections. The most important lesson to extract from our results is that the mass and the conserved charges of the black holes do get modi ed by the 0 corrections. This is what one would expect on physical grounds as the corrections act in the string equations of motion as effective sources of energy, momentum and charge. This information is crucial to establish a correspondence between the parameters that characterize the effective or coarse-grained description (the black hole) and those that characterize the microscopic system of string theory that it describes. The effects on the charges introduced by the higher-derivative corrections has a major impact in the understanding of the so-called small black holes, which are an effective description of a fundamental string with winding and momentum charges. Small black holes are singular solutions with vanishing horizon area in the supergravity approximation. It has long been believed that higher-derivative corrections would be able to stretch the horizon, making the solution regular. Our results reveal that this is not the case at rst order in 0, and that previous regularizations of heterotic small black holes actually describe a different microscopic system which is already regular in the supergravity approximation. The last chapter of the thesis contains the computation of the most general correction to the four-dimensional Kerr solution when the Einstein-Hilbert term is supplemented with higher curvature terms up to cubic order, including the possibility of having dynamical couplings. This general set-up includes, as a particular case, the corrections predicted by the heterotic superstring effective action
Published: 2020

37. New Physics Signals of the Electroweak Chiral Lagrangian in Vector Boson Scattering at the LHC

Author: Garcia-Garcia, Claudia, Herrero Solans, María José, UAM. Departamento de Física Teórica, and Instituto de Física Teórica (IFT)
Subjects: High Energy Physics - Phenomenology, High Energy Physics - Phenomenology (hep-ph), High Energy Physics::Phenomenology, Física, FOS: Physical sciences, hep-ph, Partículas (Física nuclear) - Tesis doctorales, Particle Physics - Phenomenology
Abstract: Tesis doctoral inédita leída en la Universidad Autónoma de Madrid, Facultad de Ciencias, Departamento de Física Teórica. Fecha de lectura: 15-10-2019, The Standard Model of fundamental interactions, albeit an incredibly elegant and successful theory, lacks explanations for some experimental and theoretical open questions. Interestingly, many of these problems seem to be related to the electroweak symmetry breaking sector of the theory, whose dynamical generation is still unknown. Important questions such as what is the true nature of the Higgs boson, why is its mass so light and so close to that of the electroweak gauge bosons or whether the properties of this particle are the ones predicted in the Standard Model remain unanswered. The LHC is our tool to unveil these mysteries and vector boson scattering processes are the perfect window to access them, since they are considered as the most sensitive observables to new physics in the electroweak symmetry breaking sector. In this Thesis we employ the effective electroweak chiral Lagrangian with a light Higgs, which assumes a strongly interacting electroweak symmetry breaking sector, to perform a model independent analysis of the phenomenology of vector boson scattering processes at the LHC as well as to present quantitative predictions for the sensitivity to possible beyond the Standard Model physics scenarios., A pesar de que el Modelo Estándar de las interacciones fundamentales es una de las teorías más elegantes y exitosas en el contexto de la física de partículas, existen ciertas cuestiones tanto experimentales como teóricas que no es capaz de explicar. Muchas de ellas parecen estar relacionadas con el sector de ruptura espontánea de la simetría electrodébil, cuyo origen dinámico nos es aún desconocido. Preguntas tales como cuál es la verdadera naturaleza del bosón de Higgs, por qué es éste tan ligero, estando su masa tan próxima a la de los bosones gauge electrodébiles o si sus acoplamientos al resto de partículas del Modelo Estándar son como los predichos por esta teoría todavía deben ser contestadas. El LHC es nuestra herramienta para desvelar estos misterios y los procesos de scattering de bosones vectoriales son la ventana perfecta para acceder a ellos, ya que dichos procesos se consideran como los más sensibles a la posible nueva física relacionada con el sector de ruptura espontánea de la simetría electrodébil. En esta Tesis empleamos el Lagrangiano quiral electrodébil efectivo con un Higgs ligero, que asume un sector de ruptura espontánea de la simetría electrodébil que interacciona fuertemente, para llevar a cabo un análisis exhaustivo de la fenomenología de los procesos de scattering de bosones vectoriales en el LHC, así como para presentar predicciones cuantitativas de la sensibilidad de este experimento a algunos escenarios de física más allá del Modelo Estándar.
Published: 2020
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38. Quantum foundation of infrared physics

Author: Letschka, Raoul Alexander, Gómez López, César, UAM. Departamento de Física Teórica, and Instituto de Física Teórica (IFT)
Subjects: Teoría cuántica de campos - Tesis doctorales, Física, Radiacion infrarroja - Tesis doctorales
Abstract: Tesis doctoral inédita leída Universidad Autónoma de Madrid, Facultad de Ciencias, Departamento de Física Teórica. Fecha de lectura: 13-12-2019, In this thesis we will take a look on the infrared (IR) and collinear limit of QED and perturbative gravity. First we study the infrared regime with its connection to the memory effect and to the decoherence of density matrices. Lastly, we study the consistency of QED with massless electrons. First we investigate the memory effects in scattering processes which are described in terms of the asymptotic retarded fields. These fields are completely determined by the scattering data and the zero mode part is set by the soft photon theorem. The dressed asymptotic states defining an infrared finite S-matrix for charged particles can be defined as quantum coherent states using the corpuscular resolution of the asymptotic retarded fields. Imposing that the net radiated energy in the scattering is zero leads to the new set of conservation laws for the scattering S-matrix which are equivalent to the decoupling of the soft modes. The actual observability of the memory requires a non-vanishing radiated energy and could be described using the infrared part of the differential cross section that only depends on the scattering data and the radiated energy. This is the IR safe cross section with any number of emitted photons carrying total energy equal to the energy involved in the actual memory detection. Secondly, we investigate on possible decoherence of the density matrix in QED or perturbative gravity due to entanglement with soft radiated modes and use thereby the two standard approaches to cancel infrared divergences coming from soft loop contributions. In the inclusive way only rates that include emitted soft radiation are non-vanishing. Independently of detector resolution, finite observables can only be obtained after integrating over the IRcomponent of this radiation. This integration can lead to some loss of quantum coherence. We argue that it should in general not lead to full decoherence. Based on unitarity, we suggest a way to define non-vanishing off-diagonal pieces of the IR-finite density matrix. For this IR-finite density matrix, we estimate the dependence of the loss of quantum coherence i.e. of its purity, on the scattering kinematics. In the coherent state approach we dress the initial and final states with a cloud of infinite many photons to achieve a not fully decoherent density matrix. The inclusive way and the coherent state approach both yield the same IRfinite rates, but we point out that they are not equivalent since they encode different infrared scales. In particular, dressing states are independent of the resolution scale of radiation. Instead, they define radiative vacua in the von Neumann space. We present a combined formalism that can simultaneously describe both dressing and radiation. This unified approach allows us to tackle the problem of quantum decoherence due to tracing over unresolved radiation. We again obtain an IR-finite density matrix with non-vanishing off-diagonal elements and again estimate how its purity depends on scattering kinematics and the resolution scale. Along the way, we comment on collinear divergences as well as the connection of large gauge transformations and dressing. Lastly, we work out in the forward limit and up to order e6 in perturbation theory the collinear divergences. In this kinematical regime we discover new collinear divergences that we argue can be only cancelled using quantum interference with processes contributing to the gauge anomaly. This rules out the possibility of a quantum consistent and anomaly free theory with massless charges and long range interactions. We use the anomalous threshold singularities to derive a gravitational lower bound on the mass of the lightest charged fermion
Published: 2019

39. Sampling the μνSSM in the light of experimental data

Author: Kpatcha, Essodjolo, Muñoz López, Carlos, UAM. Departamento de Física Teórica, and Instituto de Física Teórica (IFT)
Subjects: High Energy Physics::Phenomenology, Supersimetría - Tesis doctorales, Física, High Energy Physics::Experiment, Modelo estándar (Física nuclear) - Tesis doctorales
Abstract: Tesis doctoral inédita leída en la Universidad Autónoma de Madrid. Facultad de Ciencias, Departamento de Física Teórica. Fecha de Lectura: 10-12-2019, The properties and signal rates of the scalar boson discovered by ATLAS and CMS Collaborations at the Large Hadron Collider (LHC) in 2012 indicate that this resonance is compatible with the expectations for the Higgs boson of the Standard Model (SM) of particle physics. Hence, this particle represents the last piece of evidence in favour of the SM in explaining the known elementary particles and their interactions. However, there are relevant questions that cannot be answered in the theoretical framework of the SM, such as for example the origin of the Higgs potential producing the electroweak symmetry breaking (EWSB), the solution of the hierarchy problem, the origin of neutrino masses and mixing angles, the nature of dark matter (DM), the solution to the strong CP problem, the origin of matter anti-matter asymmetry, or how to accommodate the gravitational interaction. From the theoretical viewpoint, many theories have been proposed to address some of these questions. Even though the motivation for each theory might diﬀer, the common point for most of them is that the SM particle content has to be extended and that the new particles are expected to show up at scales not too far from the electroweak (EW) scale. Among a handful of eligible theories beyond the standard model (BSM), EW Supersymmetry (SUSY) has received extensive attention from both theoretical and experimental perspectives over a long period of time. SUSY is a symmetry that provides a connection between fermions and bosons in such a way that for each SM particle there exists a supersymmetric partner (also called sparticle) with the same set of quantum numbers but a half integer spin diﬀerence. Thus, SUSY principle allows every SM boson (fermion) to have a supersymmetric partner that is a fermion (boson). As a consequence, SUSY predicts a large number of new particles that could be discovered at the LHC or at the next generation of colliders. Nevertheless, no sparticle has been detected yet despite numerous searches and tremendous eﬀorts of the experimental collaborations. Therefore, the parameter spaces of SUSY models seem to be shrinking considerably. It appears then crucial to conduct thorough studies of the current situation for the diﬀerent models. In this thesis, we consider the ‘µ from ν’ Supersymmetric Standard Model (µνSSM) as the theoretical model to be analyzed. In addition to the usual advantages of SUSY models, the µνSSM, through the presence of three families of right-handed neutrino superﬁelds can simultaneously solve the µ-problem of the Minimal Supersymmetric Standard Model (MSSM), as well as the ν-problem, being able to reproduce the correct neutrino masses and mixing angles. It can also provide a good candidate for DM, the gravitino. In SUSY models, the presence of baryon- and lepton-number violating terms predicts too fast proton decay, and usually the R-parity symmetry is used to forbid these terms from appearing in the Lagrangian. This strategy gives rise to the so-called R-parity conserving (RPC) models, such as the MSSM. On the contrary, the µνSSM is an R-parity violating (RPV) model due to the presence of new couplings involving right-handed neutrinos, and therefore violating lepton number (harmless for proton decay). Then, since the lightest supersymmetric particle (LSP) is no longer stable in the µνSSM, it leads to novel signatures at colliders, such as the production of displaced vertices, multileptons or new decay chains. The goal of this thesis is to thoroughly study the parameter space of the µνSSM in the light of current experimental data, using a powerful likelihood data-driven method. In particular, we study the viable regions compatible with current neutrino oscillations and Higgs data, as well as a class of ﬂavor observables. On the one hand, we analyze those regions that can be explored at the current and future runs of the LHC via the extended Higgs sector of the µνSSM, which in general consists of two Higgs doublets mixed with the three families of sneutrinos. Then, we apply this strategy to study the compatibility of the left sneutrino as an interesting LSP candidate in the µνSSM, with current displaced dilepton searches. On the other hand, we also analyze the regions that can explain a long standing puzzle of the SM, namely, the deviation of the measurement of the anomalous magnetic moment of the muon with respect to the theoretical prediction
Published: 2019

40. Primordial black holes survive SN lensing constraints

Author: Juan Garcia-Bellido, Sebastien Clesse, Pierre Fleury, UAM. Departamento de Física Teórica, and Instituto de Física Teórica (IFT)
Subjects: Physics, 010308 nuclear & particles physics, Dark matter, Gravitational lensing, Física, Primordial black holes, Astronomy and Astrophysics, Primordial black hole, Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics, 01 natural sciences, LIGO, Supernova, Gravitational lens, Space and Planetary Science, Bounded function, 0103 physical sciences, Log-normal distribution, Degeneracy (mathematics), 010303 astronomy & astrophysics
Abstract: It has been claimed in [arxiv:1712.02240] that massive primordial black holes (PBH) cannot constitute all of the dark matter (DM), because their gravitational-lensing imprint on the Hubble diagram of type Ia supernovae (SN) would be incompatible with present observations. In this note, we critically review those constraints and find several caveats on the analysis. First of all, the constraints on the fraction α of PBH in matter seem to be driven by a very restrictive choice of priors on the cosmological parameters. In particular, the degeneracy between Ωmand α was ignored and thus, by fixing Ωm, transferred the constraining power of SN magnitudes to α. Furthermore, by considering more realistic physical sizes for the type-Ia supernovae, we find an effect on the SN lensing magnification distribution that leads to significantly looser constraints. Moreover, considering a wide mass spectrum of PBH, such as a lognormal distribution, further softens the constraints from SN lensing. Finally, we find that the fraction of PBH that could constitute DM today is bounded by fPBH, JGB thanks the CERN TH-Division for hospitality during his sabbatical, and acknowledges support from the Research Project FPA2015-68048-03-3P [MINECO-FEDER] and the Centro de Excelencia Severo Ochoa Program SEV- 2016-0597. He also acknowledges support from the Salvador de Madariaga Program, Ref. PRX17/00056. The work of SC is supported by a Charg e de Recherche grant of the Belgian Fund for Research FRS/FNRS. PF acknowledges support by the Swiss National Science Foundation
Published: 2018

41. Quasi-local energy and compactification

Author: Enrique Alvarez, Raquel Santos-Garcia, Jesus Anero, Guillermo Milans del Bosch, UAM. Departamento de Física Teórica, and Instituto de Física Teórica (IFT)
Subjects: High Energy Physics - Theory, Nuclear and High Energy Physics, Physics::General Physics, Trace (linear algebra), Compact dimension, FOS: Physical sciences, Field Theories in Higher Dimensions, General Relativity and Quantum Cosmology (gr-qc), Curvature, 01 natural sciences, General Relativity and Quantum Cosmology, 0103 physical sciences, Minkowski space, lcsh:Nuclear and particle physics. Atomic energy. Radioactivity, Compactification (mathematics), 010306 general physics, Mathematical physics, Physics, Spacetime, 010308 nuclear & particles physics, Zero (complex analysis), Física, Hypersurface, High Energy Physics - Theory (hep-th), lcsh:QC770-798, Classical Theories of Gravity
Abstract: Based on the quasi-local energy definition of Brown and York, we compute the integral of the trace of the extrinsic curvature over a codimension-2 hypersurface. In particular, we study the difference between the uncompactified Minkowski spacetime and the toroidal Kaluza-Klein compactification. For the latter, we find that this quantity interpolates between zero and the value for the uncompactified spacetime, as the size of the compact dimension increases. Thus, the quasi-local energy is able to discriminate between the two spacetimes., GMB is supported by the project FPA2015-65480-P and RSG is supported by the Spanish FPU Grant No FPU16/01595. This work has received funding from the Spanish Research Agency (Agencia Estatal de Investigacion) through the grant IFT Centro de Excelencia Severo Ochoa SEV-2016-0597, and the European Unions Horizon 2020 research and innovation programme under the Marie Sklodowska-Curie grants agreement No 674896 and No 690575. We also have been partially supported by FPA2016-78645-P(Spain) and COST actions MP1405 (Quantum Structure of Spacetime)
Published: 2018

42. Supersymmetric solutions of the cosmological, gauged, ℂ magic model

Author: Tomás Ortín, Alejandro Ruipérez, Samuele Chimento, UAM. Departamento de Física Teórica, and Instituto de Física Teórica (IFT)
Subjects: High Energy Physics - Theory, Nuclear and High Energy Physics, Instanton, High Energy Physics::Lattice, FOS: Physical sciences, 01 natural sciences, Minimal model, High Energy Physics::Theory, Gauge group, 0103 physical sciences, Black Holes in String Theory, lcsh:Nuclear and particle physics. Atomic energy. Radioactivity, Abelian group, 010306 general physics, Mathematical physics, Gauge symmetry, Physics, Compactification (physics), 010308 nuclear & particles physics, Supergravity, High Energy Physics::Phenomenology, Superstring theory, Física, Solitons Monopoles and Instantons, High Energy Physics - Theory (hep-th), Gauge Symmetry, lcsh:QC770-798, Supergravity Models
Abstract: We construct supersymmetric solutions of theories of gauged N = 1, d = 5 supergravity coupled to vector multiplets with a U(1)RAbelian (Fayet-Iliopoulos) gauging and an independent SU(2) gauging associated to an SU(2) isometry group of the Real Special scalar manifold. These theories provide minimal supersymmetrizations of 5-dimensional SU(2) Einstein-Yang-Mills theories with negative cosmological constant. We consider a minimal model with these gauge groups and the “magic model” based on the Jordan algebra J3ℂwith gauge group SU(3) × U(1)R, which is a consistent truncation of maximal SO(6)-gauged supergravity in d = 5 and whose solutions can be embedded in Type IIB Superstring Theory. We find several solutions containing selfdual SU(2) instantons, some of which asymptote to AdS5and some of which are very small, supersymmetric, deformations of AdS5. We also show how some of those solutions can be embedded in Romans’ SU(2) × U(1)-gauged half-maximal supergravity, which was obtained by Lu, Pope and Tran by compactification of the Type IIB Superstring effective action. This provides another way of uplifting those solutions to 10 dimensions., The work of AR has been supported by a Campus Internacional de Excelencia UAM-CSIC FPI grant and also by a Residencia de Estudiantes grant. This work has been supported in part by the MINECO/FEDER, UE grant FPA2015-66793-P and by the Spanish Research Agency (Agencia Estatal de Investigación) through the gtrant IFT Centro de Excelencia Severo Ochoa SEV-2016-0597 which has also suppported the work of SC.
Published: 2018

43. Constraints from microlensing experiments on clustered primordial black holes

Author: Juan Garcia-Bellido, Sebastien Clesse, UAM. Departamento de Física Teórica, Instituto de Física Teórica (IFT), and UCL - SST/IRMP - Institut de recherche en mathématique et physique
Subjects: High Energy Physics - Theory, Astrophysics and Astronomy, Cosmology and Nongalactic Astrophysics (astro-ph.CO), gr-qc, astro-ph.GA, Astrophysics::High Energy Astrophysical Phenomena, Dark matter, Microlensing, FOS: Physical sciences, Primordial black holes, Primordial black hole, Astrophysics, General Relativity and Quantum Cosmology (gr-qc), Astrophysics::Cosmology and Extragalactic Astrophysics, Gravitational microlensing, 01 natural sciences, General Relativity and Quantum Cosmology, 0103 physical sciences, Primordial Black Holes, Dark Matter, 010306 general physics, Reionization, Astrophysics::Galaxy Astrophysics, Physics, Solar mass, Mass distribution, General Relativity and Cosmology, 010308 nuclear & particles physics, hep-th, Física, Astronomy and Astrophysics, Astrophysics - Astrophysics of Galaxies, Galaxy, Black hole, High Energy Physics - Theory (hep-th), Space and Planetary Science, Astrophysics of Galaxies (astro-ph.GA), astro-ph.CO, Particle Physics - Theory, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: It has recently been proposed that massive primordial black holes (PBH) could constitute all of the dark matter, providing a novel scenario of structure formation, with early reionization and a rapid growth of the massive black holes at the center of galaxies and dark matter halos. The scenario arises from broad peaks in the primordial power spectrum that give both a spatially clustered and an extended mass distribution of PBH. The constraints from the observed microlensing events on the extended mass function have already been addressed. Here we study the impact of spatial clustering on the microlensing constraints. We find that the bounds can be relaxed significantly for relatively broad mass distributions if the number of primordial black holes within each cluster is typically above one hundred. On the other hand, even if they arise from individual black holes within the cluster, the bounds from CMB anisotropies are less stringent due to the enhanced black hole velocity in such dense clusters. This way, the window between a few and ten solar masses has opened up for PBH to comprise the totality of the dark matter., Comment: 6 pages, 3 figures, comments welcome
Published: 2018

44. Higher-Curvature Gravity, Black Holes and Holography

Author: Cano Molina-Niñirola, Pablo Antonio, Ortín, Tomás, Bueno, Pablo, UAM. Departamento de Física Teórica, and Instituto de Física Teórica (IFT)
Subjects: General Relativity and Quantum Cosmology, Holografía - Tesis doctorales, Física, Agujeros negros (Astronomía) - Tesis doctorales, Gravitación - Tesis doctorales
Abstract: Tesis Doctoral inédita leída en la Universidad Autónoma de Madrid. Facultad de Ciencias, Departamento de Física Teórica. Fecha de Lectura: 19-09-2019, Higher-curvature theories of gravity are extensions of General Relativity (GR) that arise in effective descriptions of quantum gravity theories, such as String Theory. While at low energies the behaviour of the gravitational field in higher-curvature gravities is almost indistinguishable from the one predicted by GR, the differences can be dramatic in extreme gravity scenarios, such as in the case of black holes (BHs). It is therefore an exciting task to study how black hole geometries are modified by higher-curvature corrections, with the hope that some problematic characteristics of BHs observed in GR could be improved, providing hints on the effects of an underlying UV-complete theory of gravity. However, there are some difficulties associated with higher-derivative theories, such as the existence of instabilities, propagation of ghost modes, or simply the extreme complexity of the differential equations governing the dynamics of the gravitational field. In this thesis we identify a new family of higher-curvature gravities that avoid some of these problems. Known as Generalized quasi-topological gravities (GQGs), such theories represent extensions of GR that are free of instabilities and ghosts at the linear level, and whose equations of motion for static, spherically symmetric spaces acquire a sufficiently simple form so as to allow for the non-perturbative study of black hole solutions. The simplest non-trivial member of this family in four dimensions — and also the first one to be discovered — is known as Einsteinian cubic gravity, and it will have a starring role in this thesis. Besides the intrinsic interesting properties of GQGs, we argue that they capture the most general higher-derivative correction to GR when field redefinitions are included into the game. Then, we use these theories to study the non-perturbative corrections to the Schwarzschild black hole in four dimensions and we focus our attention on the modified thermodynamic relations. The most impressive prediction of these theories is that the Hawking temperature of static, neutral black holes vanishes in the zero-mass limit instead of diverging — which is the answer predicted by GR. As a consequence, small black holes become thermodynamically stable and their evaporation process takes an infinite time. In addition, higher-curvature gravities find very rewarding applications in the Anti-de Sitter/ Conformal Field Theory (AdS/CFT) correspondence, a duality that relates a classical theory of gravity in AdS space to a quantum field theory that lives in the boundary of AdS. In this context, holographic higher-curvature gravities are useful toy models that we can use, for instance, to extract general lessons about the dynamics of CFTs or to question the generality of the predictions of holographic Einstein gravity. In this thesis we explore the holographic applications of four-dimensional Einsteinian cubic gravity, which provides a toy model for a non-supersymmetric holographic CFT in three dimensions. In addition, we construct new Euclidean-AdS-Taub-NUT solutions, which are dual to conformal field theories placed on squashed spheres. Using these results, we derive a universal expression for the expansion of the free energy of three-dimensional CFTs on squashed spheres up to cubic order in the deformation parameter., Esta tesis ha sido posible gracias a la financiación que he recibido por parte de la Fundación “la Caixa” a través de una beca “la Caixa - Severo Ochoa” asociada al Instituto de Física Teórica UAM-CSIC
Published: 2019

45. Phenomenology of the Higgs sectors of the uvSSM and the N2HDM

Author: Biekötter, Thomas, Heinemeyer, Sven, Muñoz López, Carlos, UAM. Departamento de Física Teórica, and Instituto de Física Teórica (IFT)
Subjects: Física
Abstract: Tesis Doctoral inédita leída en la Universidad Autónoma de Madrid. Facultad de Ciencias, Departamento de Física Teórica. Fecha de Lectura: 05-09-2019
Published: 2019

46. Neutrino windows to new physics

Author: Gehrlein, Julia, Fernández Martínez, Enrique, Blennow, Mattias, UAM. Departamento de Física Teórica, and Instituto de Física Teórica (IFT)
Subjects: Neutrinos - Tesis doctorales, Física, Modelo estándar (Física nuclear) - Tesis doctorales
Abstract: Tesis Doctoral inédita leída en la Universidad Autónoma de Madrid, Facultad de Ciencias, Departamento de Física Teórica. Fecha de lectura: 25-06-2019
Published: 2019

47. Probing the electroweak sector of the μνSSM at the LHC

Author: Lara Pérez, Iñaki, Muñoz López, Carlos, UAM. Departamento de Física Teórica, and Instituto de Física Teórica (IFT)
Subjects: Aceleradores de partículas.- Tesis doctorales, Física, Partículas (Física nuclear) - Tesis doctorales
Abstract: Tesis Doctoral inédita leída en la Universidad Autónoma de Madrid, Facultad de Ciencias, Departamento de Física Teórica. Fecha de lectura: 22-01-2019
Published: 2019

48. Semi-analytical galaxies in the multidark-universe: A perspective on the evolution of the most luminous and massive galaxies throughout cosmic history

Author: Stoppacher, Doris, Prada Martínez, Francisco, Knebe, Alexander, UAM. Departamento de Física Teórica, and Instituto de Física Teórica (IFT)
Subjects: Galaxias - Tesis doctorales, Física, Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics::Galaxy Astrophysics
Abstract: Tesis doctoral inédita leída en la Universidad Autónoma de Madrid, Facultad de Ciencias, Departamento de Física Teórica. Fecha de lectura: 13-12-2019, Esta tesis tiene embargado el acceso al texto completo hasta el 13-06-2021, Understanding the formation and evolution of galaxies within a self-consistent cosmological context is one of the outstanding and most challenging topics of astrophysics. This dissertation is dedicated to investigating the concepts of galaxy formation with cosmology, in particular, the formation of large-scale structures and the assembly and evolution of their associated galaxies over cosmic time. This forms part of a vibrate and innovative field of research spanning all imaginable scales from The Big Bang to the Milky Way Galaxy with its many satellites. Over the last few decades a lot of effort has been invested into the development of models which can produce statistically significant sets of galaxy properties in a computationally efficient way. These models included the population of dark matter halos using simplified phenomenological treatments of baryonic processes and coarse-graining the properties of galaxies. As a result, relevant equation systems can be solved more efficiently – a semi-analytical model (SAM) was born. The MultiDark-Galaxies was an ambitious project dedicated to the release of galaxy catalogues from three different SAMs: Galacticus, SAG, and SAGE; run on the MultiDark Planck 2 N-body simulation covering a cubic volume of 1h􀀀��1Gpc as part of this thesis work. To this point, the released galaxy catalogues remain one of the largest of their kind based on SAMs. We perform a comparison of the outputs of the three models and their conformity with fundamental galaxy properties derived from observations. Each model of galaxy formation has its unique recipe followed by individual calibration and tuning, therefore we highlight their differences and similarities. We demonstrate further that SAMs are an exceptional resourceful method of studying statistically significant samples of galaxy properties. We identify modelled galaxies from Galacticus, which show similar properties as observational samples and therefore are truly comparable with luminous red galaxies (LRGs) from e.g. SDSS at z 0:1 or BOSS-CMASS at z 0:5. We extract CMASS-mock samples from Galacticus using the original photometric selection as well as alternative methods mimicking such a selection. We study these mock samples in detail and find correlations of properties related to star formation: (specific) star formation rate, gas-phase metallicity ZCold, and cold-gas fraction MCold=M , but also properties such as the halo mass M200c or the black hole mass MBH; with the large-scale structure environment e.g. filaments or knots. We emphasise that, the bimodalities found in the properties of Galacticus’ CMASS-mocks, manifesting themselves as two distinct populations, could provide insights in the galaxy evolution in the context of the origin of the fundamental luminosity/mass-metallicity relation, mergerinduced star formation, or “downsizing”. Our results may further challenge the paradigm that the large-scale environment does not influence the galaxy formation and predictions on the evolution of a galaxy inside its halo can be derived only from the halo mass and the occupation distribution, also know as the galaxy assembly bias. We trace the progenitors of Galacticus’ LRG-samples at low redshift to z 0:5 and identify 20% of them as CMASS. We show further the full mass growth history of the progenitors of the most diverse populations, red and blue, found in the CMASS-mock of Galacticus. We find that those samples have distinct properties, cluster differently, and have been assembled at different cosmic times, most probably throughout different evolutionary paths. We will conduct further analyses in order to confirm the possible detection of a galaxy assembly bias signal in our SAM
Published: 2019

49. Holography in out of equilibrium systems and asymptotic symmetries of black holes

Author: Milans del Bosch de Linos, Guillermo, Lopez Manzanares, Esperanza, UAM. Departamento de Física Teórica, and Instituto de Física Teórica (IFT)
Subjects: Holografía - Tesis doctorales, Teoría cuántica de campos - Tesis doctorales, Física, Relatividad, Teoría de la - Tesis doctorales
Abstract: Tesis Doctoral inédita leída en la Universidad Autónoma de Madrid, Facultad de Ciencias, Departamento de Física Teórica. Fecha de lectura: 26-06-2019, This thesis, presented in the form of a "compilation of articles", touches different areas of Theoretical Physics. The first part, which comprises the first two articles, focuses on using applied holography to study out-of-equilibrium physics. More specifically, in the first article we study quantum processes called quenches and we show, by holographically constructing gravitational dual backgrounds, the way to implement a quantum quench with a real change in the hamiltonian in a Lorentz-invariant manner. The second article is framed under the theory of anomalous transport. The object of study is the gravitational contribution to the chiral anomaly, which through the chiral magnetic effect induces an energy current proportional to the square of the temperature when the system is in equilibrium. In this framework, we implement holographic quantum quenches to bring the system out of equilibrium, where no temperature can be well defined. Our results indicate a strong suppression of this effect when the system is very far from equilibrium. The second part of the thesis lies in the context of exact, non-linear general relativity. In the third article, we characterize generic, non-expanding black hole horizons and study the effect of supertranslations on them. We present a freely specifiable data set which is both necessary and sufficient to reconstruct the full horizon geometry and is composed of objects that are invariant under supertranslations. Therefore we conclude that these transformations do not transform the geometry of the horizon and should be regarded as pure gauge., Esta tesis, presentada en la forma de "compilación de artículos", toca diferentes areas de la Física Teórica. La primera parte, que consta de los dos primeros artículos, se centra en usar holografía aplicada al estudio de la física fuera del equilibrio. Más concretamente, en el primer artículo estudiamos procesos cuánticos llamados quenches y demostramos, construyendo holográficamente los escenarios gravitacionales de la teoría dual, la manera de implementar un quench cuántico con un cambio real en el hamiltoniano de manera invariante Lorentz. El segundo artículo se encuadra bajo la teoría de transporte anómalo. El objeto de estudio es la contribución gravitacional a la anomalía quiral, que a través del efecto magnético quiral induce una corriente de energía que es proporcional al cuadrado de la temperatura cuando el sistema está en equilibrio. En este escenario implementamos quenches holográficos para llevar al sistema fuera del equilibrio, donde la temperatura no está bien definida. Nuestros resultados indican una fuerte supresión de este efecto cuando el sistema está lejos de encontrarse en equilibrio. La segunda parte de esta tesis se encuentra en el contexto de la relatividad general exacta y no-lineal. En el tercer artículo, caracterizamos horizontes genéricos y que no se expanden de agujeros negros, y estudiamos el efecto que tienen las supertraslaciones en ellos. Presentamos un conjunto de datos que pueden especificarse libremente, que son necesarios y suficientes para reconstruir la geometría completa del horizonte y que son invariante bajo supertraslaciones. Por lo tanto concluimos que estas transformaciones no transforman la geometría del horizonte y deben ser consideradas como puro gauge.
Published: 2019

50. Bipartite field theories and D-brane instantons

Author: Angel M. Uranga, Sebastian Franco, Eduardo García-Valdecasas, UAM. Departamento de Física Teórica, and Instituto de Física Teórica (IFT)
Subjects: High Energy Physics - Theory, Nuclear and High Energy Physics, Instanton, Brane Dynamics in Gauge Theories, FOS: Physical sciences, String theory, 01 natural sciences, Supersymmetric Gauge Theory, symbols.namesake, Theoretical physics, High Energy Physics::Theory, 0103 physical sciences, lcsh:Nuclear and particle physics. Atomic energy. Radioactivity, D-brane, 010306 general physics, Physics, 010308 nuclear & particles physics, Riemann surface, S-duality, Física, High Energy Physics - Theory (hep-th), Supersymmetric gauge theory, D-branes, Bipartite graph, symbols, lcsh:QC770-798, Seiberg duality
Abstract: We study D-brane instantons in systems of D3-branes at toric CY 3-fold singularities. The instanton effect can be described as a backreaction modifying the geometry of the mirror configuration, in which the breaking of $U(1)$ symmetries by the instanton translates into the recombination of gauge D-branes, which also directly generates the instanton-induced charged field theory operator. In this paper we describe the D-brane instanton backreaction in terms of a combinatorial operation in the bipartite dimer diagram of the original theory. Interestingly, the resulting theory is a general Bipartite Field Theory (BFT), defined by a bipartite graph tiling a general (possibly higher-genus) Riemann surface. This provides the first string theory realization of such general BFTs. We study the general properties of the resulting theories, including the construction of the higher-dimensional toric diagrams and the interplay between backreaction and Seiberg duality. In cases where the non-perturbative effects relate to complex deformations, we show that the procedure reproduces and explains earlier existing combinatorial recipes. The combinatorial operation and its properties generalize to an operation on the class of general BFTs, even including boundaries, relating BFTs defined on Riemann surfaces of different genus., Comment: 51 pages, 49 figures. Minor corrections
Published: 2018

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