83 results on '"Ariga Akitaka"'
Search Results
2. The Forward Physics Facility: Sites, experiments, and physics potential
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Anchordoqui, Luis A., Ariga, Akitaka, Ariga, Tomoko, Bai, Weidong, Balazs, Kincso, Batell, Brian, Boyd, Jamie, Bramante, Joseph, Campanelli, Mario, Carmona, Adrian, Celiberto, Francesco G., Chachamis, Grigorios, Citron, Matthew, De Lellis, Giovanni, De Roeck, Albert, Dembinski, Hans, Denton, Peter B., Di Crecsenzo, Antonia, Diwan, Milind V., Dougherty, Liam, Dreiner, Herbi K., Du, Yong, Enberg, Rikard, Farzan, Yasaman, Feng, Jonathan L., Fieg, Max, Foldenauer, Patrick, Foroughi-Abari, Saeid, Friedland, Alexander, Fucilla, Michael, Gall, Jonathan, Garzelli, Maria Vittoria, Giuli, Francesco, Goncalves, Victor P., Guzzi, Marco, Halzen, Francis, Helo, Juan Carlos, Hill, Christopher S., Ismail, Ahmed, Ismail, Ameen, Jacobsson, Richard, Jana, Sudip, Jeong, Yu Seon, Jodłowski, Krzysztof, Kelly, Kevin J., Kling, Felix, Kumar, Fnu Karan, Liu, Zhen, Maciuła, Rafał, Abraham, Roshan Mammen, Manshanden, Julien, McFayden, Josh, Mohammed, Mohammed M.A., Nadolsky, Pavel M., Okada, Nobuchika, Osborne, John, Otono, Hidetoshi, Pandey, Vishvas, Papa, Alessandro, Raut, Digesh, Reno, Mary Hall, Resnati, Filippo, Ritz, Adam, Rojo, Juan, Sarcevic, Ina, Scherb, Christiane, Schulz, Holger, Schwaller, Pedro, Sengupta, Dipan, Sjöstrand, Torbjörn, Smith, Tyler B., Soldin, Dennis, Stasto, Anna, Szczurek, Antoni, Tabrizi, Zahra, Trojanowski, Sebastian, Tsai, Yu-Dai, Tuckler, Douglas, Winkler, Martin W., Xie, Keping, and Zhang, Yue
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- 2022
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3. The tracking detector of the FASER experiment
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Abreu, Henso, Antel, Claire, Ariga, Akitaka, Ariga, Tomoko, Bernlochner, Florian, Boeckh, Tobias, Boyd, Jamie, Brenner, Lydia, Cadoux, Franck, Casper, David W., Cavanagh, Charlotte, Chen, Xin, Coccaro, Andrea, Crespo-Lopez, Olivier, Dmitrievsky, Sergey, D’Onofrio, Monica, Dozen, Candan, Ezzat, Abdallah, Favre, Yannick, Fellers, Deion, Feng, Jonathan L., Ferrere, Didier, Gibson, Stephen, Gonzalez-Sevilla, Sergio, Gornushkin, Yuri, Gwilliam, Carl, Hsu, Shih-Chieh, Hu, Zhen, Iacobucci, Giuseppe, Inada, Tomohiro, Jakobsen, Sune, Kajomovitz, Enrique, Kling, Felix, Kose, Umut, Kuehn, Susanne, Lefebvre, Helena, Levinson, Lorne, Li, Ke, Liu, Jinfeng, Magliocca, Chiara, McFayden, Josh, Milanesio, Matteo, Meehan, Sam, Mladenov, Dimitar, Moretti, Théo, Munker, Magdalena, Nakamura, Mitsuhiro, Nakano, Toshiyuki, Nessi, Marzio, Neuhaus, Friedemann, Nevay, Laurie, Otono, Hidetoshi, Pandini, Carlo, Pang, Hao, Paolozzi, Lorenzo, Petersen, Brian, Pietropaolo, Francesco, Prim, Markus, Queitsch-Maitland, Michaela, Resnati, Filippo, Rizzi, Chiara, Rokujo, Hiroki, Ruiz-Choliz, Elisa, Salfeld-Nebgen, Jakob, Sato, Osamu, Scampoli, Paola, Schmieden, Kristof, Schott, Matthias, Sfyrla, Anna, Shively, Savannah, Spencer, John, Takubo, Yosuke, Tarannum, Noshin, Theiner, Ondrej, Torrence, Eric, Tufanli, Serhan, Vasina, Svetlana, Vormwald, Benedikt, and Wang, Di
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- 2022
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4. Muon tomography in geoscientific research – A guide to best practice
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Lechmann, Alessandro, Mair, David, Ariga, Akitaka, Ariga, Tomoko, Ereditato, Antonio, Nishiyama, Ryuichi, Pistillo, Ciro, Scampoli, Paola, Schlunegger, Fritz, and Vladymyrov, Mykhailo
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- 2021
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5. Detecting and studying high-energy collider neutrinos with FASER at the LHC: FASER Collaboration
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Abreu, Henso, Antel, Claire, Ariga, Akitaka, Ariga, Tomoko, Boyd, Jamie, Cadoux, Franck, Casper, David W., Chen, Xin, Coccaro, Andrea, Dozen, Candan, Denton, Peter B., Favre, Yannick, Feng, Jonathan L., Ferrere, Didier, Galon, Iftah, Gibson, Stephen, Gonzalez-Sevilla, Sergio, Hsu, Shih-Chieh, Hu, Zhen, Iacobucci, Giuseppe, Jakobsen, Sune, Jansky, Roland, Kajomovitz, Enrique, Kling, Felix, Kuehn, Susanne, Levinson, Lorne, Li, Congqiao, McFayden, Josh, Meehan, Sam, Neuhaus, Friedemann, Otono, Hidetoshi, Petersen, Brian, Pikhartova, Helena, Queitsch-Maitland, Michaela, Sato, Osamu, Schmieden, Kristof, Schott, Matthias, Sfyrla, Anna, Shively, Savannah, Smolinsky, Jordan, Soffa, Aaron M., Takubo, Yosuke, Torrence, Eric, Trojanowski, Sebastian, Wilkinson, Callum, Zhang, Dengfeng, and Zhang, Gang
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- 2020
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6. Search for dark photons with the FASER detector at the LHC
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Abreu, Henso, Anders, John, Antel, Claire, Ariga, Akitaka, Ariga, Tomoko, Atkinson, Jeremy, Bernlochner, Florian U., Boeckh, Tobias, Boyd, Jamie, Brenner, Lydia, Cadoux, Franck, Casper, David W., Cavanagh, Charlotte, Chen, Xin, Coccaro, Andrea, D'Onofrio, Monica, Desai, Ansh, Dmitrievsky, Sergey, Dozen, Candan, Favre, Yannick, Fellers, Deion, Feng, Jonathan L., Fenoglio, Carlo Alberto, Ferrere, Didier, Galon, Iftah, Gibson, Stephen, Gonzalez-Sevilla, Sergio, Gornushkin, Yuri, Gwilliam, Carl, Hayakawa, Daiki, Hsu, Shih-Chieh, Hu, Zhen, Iacobucci, Giuseppe, Inada, Tomohiro, Jakobsen, Sune, Joos, Hans, Kajomovitz, Enrique, Kawahara, Hiroaki, Keyken, Alex, Kling, Felix, Köck, Daniela, Kose, Umut, Kotitsa, Rafaella, Kuehn, Susanne, Lefebvre, Helena, Levinson, Lorne, Li, Ke, Liu, Jinfeng, MacDonald, Jack, Magliocca, Chiara, Martinelli, Fulvio, McFayden, Josh, Meehan, Sam, Milanesio, Matteo, Moretti, Théo, Munker, Magdalena, Nakamura, Mitsuhiro, Nakano, Toshiyuki, Neuhaus, Friedemann, Nevay, Laurie, Ohashi, Ken, Otono, Hidetoshi, Pang, Hao, Paolozzi, Lorenzo, Petersen, Brian, Prim, Markus, Queitsch-Maitland, Michaela, Rokujo, Hiroki, Ruiz-Choliz, Elisa, Sabater-Iglesias, Jorge, Salfeld-Nebgen, Jakob, Sato, Osamu, Scampoli, Paola, Schmieden, Kristof, Schott, Matthias, Sfyrla, Anna, Shively, Savannah, Takubo, Yosuke, Tarannum, Noshin, Theiner, Ondrej, Torrence, Eric, Trojanowski, Sebastian, Vasina, Svetlana, Vormwald, Benedikt, Wang, Di, Welch, Eli, Zahorec, Samuel, and Zambito, Stefano
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- 2024
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7. Hunting muonic forces at emulsion detectors
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Ariga, Akitaka, Balkin, Reuven, Galon, Iftah, Kajomovitz, Enrique, and Soreq, Yotam
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High Energy Physics - Phenomenology ,High Energy Physics - Phenomenology (hep-ph) ,FOS: Physical sciences - Abstract
Only two types of Standard Model particles are able to propagate the $480\,$meters separating the ATLAS interaction point and FASER: neutrinos and muons. Furthermore, muons are copiously produced in proton collisions. We propose to use FASER$\nu$ as a muon fixed target experiment in order to search for new bosonic degrees of freedom coupled predominantly to muons. These muon force carriers are particularly interesting in light of the recent measurement of the muon anomalous magnetic moment. Using a novel analysis technique, we show that even in the current LHC run, FASER$\nu$ could potentially probe previously unexplored parts of the parameter space. In the high-luminosity phase of the LHC, we find that the improved sensitivity of FASER$\nu2$ will probe unexplored parameter space and may be competitive with dedicated search proposals., Comment: 13 pages + appendices, 11 figures
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- 2023
8. SMAUG v1.0 – a user-friendly muon simulator for the imaging of geological objects in 3-D
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Lechmann, Alessandro, Mair, David, Ariga, Akitaka, Ariga, Tomoko, Ereditato, Antonio, Nishiyama, Ryuichi, Pistillo, Ciro, Scampoli, Paola, Vladymyrov, Mykhailo, Schlunegger, Fritz, Lechmann, Alessandro, Mair, David, Ariga, Akitaka, Ariga, Tomoko, Ereditato, Antonio, Nishiyama, Ryuichi, Pistillo, Ciro, Scampoli, Paola, Vladymyrov, Mykhailo, and Schlunegger, Fritz
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530 Physics ,550 Earth sciences & geology - Abstract
Knowledge about muon tomography has spread in recent years in the geoscientific community and several collaborations between geologists and physicists have been founded. As the data analysis is still mostly done by particle physicists, much of the know-how is concentrated in particle physics and specialised geophysics institutes. SMAUG (Sim- ulation for Muons and their Applications UnderGround), a toolbox consisting of several modules that cover the various aspects of data analysis in a muon tomographic experiment, aims at providing access to a structured data analysis frame- work. The goal of this contribution is to make muon tomog- raphy more accessible to a broader geoscientific audience. In this study, we show how a comprehensive geophysical model can be built from basic physics equations. The emerging un- certainties are dealt with by a probabilistic formulation of the inverse problem, which is finally solved by a Monte Carlo Markov chain algorithm. Finally, we benchmark the SMAUG results against those of a recent study, which, however, have been established with an approach that is not easily accessi- ble to the geoscientific community. We show that they reach identical results with the same level of accuracy and preci- sion.
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- 2022
9. First neutrino interaction candidates at the LHC
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FASER Collaboration, Abreu, Henso, Afik, Yoav, Antel, Claire, Arakawa, Jason, Ariga, Akitaka, Ariga, Tomoko, Bernlochner, Florian, Boeckh, Tobias, Boyd, Jamie, Brenner, Lydia, Cadoux, Franck, Casper, David W., Cavanagh, Charlotte, Cerutti, Francesco, Chen, Xin, Coccaro, Andrea, D'Onofrio, Monica, Dozen, Candan, Favre, Yannick, Fellers, Deion, Feng, Jonathan L., Ferrere, Didier, Gibson, Stephen, Gonzalez-Sevilla, Sergio, Gwilliam, Carl, Hsu, Shih-Chieh, Hu, Zhen, Iacobucci, Giuseppe, Inada, Tomohiro, Ismail, Ahmed, Jakobsen, Sune, Kajomovitz, Enrique, Kling, Felix, Kose, Umut, Kuehn, Susanne, Lefebvre, Helena, Levinson, Lorne, Li, Ke, Liu, Jinfeng, Magliocca, Chiara, McFayden, Josh, Meehan, Sam, Mladenov, Dimitar, Nakamura, Mitsuhiro, Nakano, Toshiyuki, Nessi, Marzio, Neuhaus, Friedemann, Nevay, Laurie, Otono, Hidetoshi, Pandini, Carlo, Pang, Hao, Paolozzi, Lorenzo, Petersen, Brian, Pietropaolo, Francesco, Prim, Markus, Queitsch-Maitland, Michaela, Resnati, Filippo, Rokujo, Hiroki, Sabaté-Gilarte, Marta, Salfeld-Nebgen, Jakob, Sato, Osamu, Scampoli, Paola, Schmieden, Kristof, Schott, Matthias, Sfyrla, Anna, Shively, Savannah, Spencer, John, Takubo, Yosuke, Theiner, Ondrej, Torrence, Eric, Trojanowski, Sebastian, Tufanli, Serhan, Vormwald, Benedikt, Wang, Di, Zhang, Gang, Abreu, Henso, Afik, Yoav, Antel, Claire, Arakawa, Jason, Ariga, Akitaka, Ariga, Tomoko, Bernlochner, Florian, Boeckh, Tobia, Boyd, Jamie, Brenner, Lydia, Cadoux, Franck, Casper, David W., Cavanagh, Charlotte, Cerutti, Francesco, Chen, Xin, Coccaro, Andrea, D???onofrio, Monica, Dozen, Candan, Favre, Yannick, Fellers, Deion, Feng, Jonathan L., Ferrere, Didier, Gibson, Stephen, Gonzalez-Sevilla, Sergio, Gwilliam, Carl, Hsu, Shih-Chieh, Hu, Zhen, Iacobucci, Giuseppe, Inada, Tomohiro, Ismail, Ahmed, Jakobsen, Sune, Kajomovitz, Enrique, Kling, Felix, Kose, Umut, Kuehn, Susanne, Lefebvre, Helena, Levinson, Lorne, Li, Ke, Liu, Jinfeng, Magliocca, Chiara, Mcfayden, Josh, Meehan, Sam, Mladenov, Dimitar, Nakamura, Mitsuhiro, Nakano, Toshiyuki, Nessi, Marzio, Neuhaus, Friedemann, Nevay, Laurie, Otono, Hidetoshi, Pandini, Carlo, Pang, Hao, Paolozzi, Lorenzo, Petersen, Brian, Pietropaolo, Francesco, Prim, Marku, Queitsch-Maitland, Michaela, Resnati, Filippo, Rokujo, Hiroki, Sabat??-Gilarte, Marta, Salfeld-Nebgen, Jakob, Sato, Osamu, Scampoli, Paola, Schmieden, Kristof, Schott, Matthia, Sfyrla, Anna, Shively, Savannah, Spencer, John, Takubo, Yosuke, Theiner, Ondrej, Torrence, Eric, Trojanowski, Sebastian, Tufanli, Serhan, Vormwald, Benedikt, Wang, Di, and Zhang, Gang
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Particle physics ,Physics - Instrumentation and Detectors ,Physics::Instrumentation and Detectors ,FOS: Physical sciences ,law.invention ,High Energy Physics - Experiment ,High Energy Physics - Experiment (hep-ex) ,High Energy Physics - Phenomenology (hep-ph) ,Atlas (anatomy) ,law ,medicine ,Detectors and Experimental Techniques ,Collider ,Nuclear Experiment ,Particle Physics - Phenomenology ,Physics ,Large Hadron Collider ,Interaction point ,Detector ,High Energy Physics::Phenomenology ,Instrumentation and Detectors (physics.ins-det) ,High Energy Physics - Phenomenology ,medicine.anatomical_structure ,Physics::Accelerator Physics ,High Energy Physics::Experiment ,Neutrino ,Particle Physics - Experiment - Abstract
FASER$\nu$ at the CERN Large Hadron Collider (LHC) is designed to directly detect collider neutrinos for the first time and study their cross sections at TeV energies, where no such measurements currently exist. In 2018, a pilot detector employing emulsion films was installed in the far-forward region of ATLAS, 480 m from the interaction point, and collected 12.2 fb$^{-1}$ of proton-proton collision data at a center-of-mass energy of 13 TeV. We describe the analysis of this pilot run data and the observation of the first neutrino interaction candidates at the LHC. This milestone paves the way for high-energy neutrino measurements at current and future colliders., Comment: Auxiliary materials are available at https://faser.web.cern.ch/fasernu-first-neutrino-interaction-candidates
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- 2021
10. The Forward Physics Facility at the High-Luminosity LHC.
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Feng, Jonathan L, Kling, Felix, Reno, Mary Hall, Rojo, Juan, Soldin, Dennis, Anchordoqui, Luis A, Boyd, Jamie, Ismail, Ahmed, Harland-Lang, Lucian, Kelly, Kevin J, Pandey, Vishvas, Trojanowski, Sebastian, Tsai, Yu-Dai, Alameddine, Jean-Marco, Araki, Takeshi, Ariga, Akitaka, Ariga, Tomoko, Asai, Kento, Bacchetta, Alessandro, and Balazs, Kincso
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LARGE Hadron Collider ,SCATTERING (Physics) ,PHYSICS ,CONDITIONAL expectations ,PARTICLE decays ,NEUTRINOS - Abstract
High energy collisions at the High-Luminosity Large Hadron Collider (LHC) produce a large number of particles along the beam collision axis, outside of the acceptance of existing LHC experiments. The proposed Forward Physics Facility (FPF), to be located several hundred meters from the ATLAS interaction point and shielded by concrete and rock, will host a suite of experiments to probe standard model (SM) processes and search for physics beyond the standard model (BSM). In this report, we review the status of the civil engineering plans and the experiments to explore the diverse physics signals that can be uniquely probed in the forward region. FPF experiments will be sensitive to a broad range of BSM physics through searches for new particle scattering or decay signatures and deviations from SM expectations in high statistics analyses with TeV neutrinos in this low-background environment. High statistics neutrino detection will also provide valuable data for fundamental topics in perturbative and non-perturbative QCD and in weak interactions. Experiments at the FPF will enable synergies between forward particle production at the LHC and astroparticle physics to be exploited. We report here on these physics topics, on infrastructure, detector, and simulation studies, and on future directions to realize the FPF's physics potential. [ABSTRACT FROM AUTHOR]
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- 2023
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11. Detecting and studying high-energy collider neutrinos with FASER at the LHC
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FASER Collaboration, Abreu, Henso, Antel, Claire, Ariga, Akitaka, Ariga, Tomoko, Boyd, Jamie, Cadoux, Franck, Casper, David W., Chen, Xin, Coccaro, Andrea, Dozen, Candan, Denton, Peter B., Favre, Yannick, Feng, Jonathan L., Ferrere, Didier, Galon, Iftah, Gibson, Stephen, Gonzalez-Sevilla, Sergio, Hsu, Shih-Chieh, Hu, Zhen, Iacobucci, Giuseppe, Jakobsen, Sune, Jansky, Roland, Kajomovitz, Enrique, Kling, Felix, Kuehn, Susanne, Levinson, Lorne, Li, Congqiao, McFayden, 1 Josh, Meehan, Sam, Neuhaus, Friedemann, Otono, Hidetoshi, Petersen, Brian, Pikhartova, Helena, Queitsch-Maitland, Michaela, Sato, Osamu, Schmieden, Kristof, Schott, Matthias, Sfyrla, Anna, Shively, Savannah, Smolinsky, Jordan, Soffa, Aaron M., Takubo, Yosuke, Torrence, Eric, Trojanowski, Sebastian, Wilkinson, Callum, Zhang, Dengfeng, and Zhang, Gang
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Physics - Instrumentation and Detectors ,hep-ex ,Physics::Instrumentation and Detectors ,Astrophysics::High Energy Astrophysical Phenomena ,High Energy Physics::Phenomenology ,FOS: Physical sciences ,hep-ph ,lcsh:Astrophysics ,Instrumentation and Detectors (physics.ins-det) ,High Energy Physics - Experiment ,High Energy Physics - Phenomenology ,High Energy Physics - Experiment (hep-ex) ,High Energy Physics - Phenomenology (hep-ph) ,lcsh:QB460-466 ,Physics::Accelerator Physics ,lcsh:QC770-798 ,High Energy Physics::Experiment ,lcsh:Nuclear and particle physics. Atomic energy. Radioactivity ,Detectors and Experimental Techniques ,physics.ins-det ,Particle Physics - Experiment ,Particle Physics - Phenomenology - Abstract
Neutrinos are copiously produced at particle colliders, but no collider neutrino has ever been detected. Colliders, and particularly hadron colliders, produce both neutrinos and anti-neutrinos of all flavors at very high energies, and they are therefore highly complementary to those from other sources. FASER, the recently approved Forward Search Experiment at the Large Hadron Collider, is ideally located to provide the first detection and study of collider neutrinos. We investigate the prospects for neutrino studies of a proposed component of FASER, FASER$\nu$, a 25cm x 25cm x 1.35m emulsion detector to be placed directly in front of the FASER spectrometer in tunnel TI12. FASER$\nu$ consists of 1000 layers of emulsion films interleaved with 1-mm-thick tungsten plates, with a total tungsten target mass of 1.2 tons. We estimate the neutrino fluxes and interaction rates at FASER$\nu$, describe the FASER$\nu$ detector, and analyze the characteristics of the signals and primary backgrounds. For an integrated luminosity of 150 fb$^{-1}$ to be collected during Run 3 of the 14 TeV Large Hadron Collider from 2021-23, and assuming standard model cross sections, approximately 1300 electron neutrinos, 20,000 muon neutrinos, and 20 tau neutrinos will interact in FASER$\nu$, with mean energies of 600 GeV to 1 TeV, depending on the flavor. With such rates and energies, FASER will measure neutrino cross sections at energies where they are currently unconstrained, will bound models of forward particle production, and could open a new window on physics beyond the standard model., Comment: Version published in EPJ C
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- 2020
12. Experiments and Facilities for Accelerator-Based Dark Sector Searches
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Ilten, Philip, Tran, Nhan, Patrick Achenbach, Ariga, Akitaka, Ariga, Tomoko, Battaglieri, Marco, Bian, Jianming, Bisio, Pietro, Celentano, Andrea, Citron, Matthew, Crivelli, Paolo, Lellis, Giovanni, Di Crescenzo, Antonia, Diwan, Milind, Feng, Jonathan L., Gatto, Corrado, Gori, Stefania, Kling, Felix, Marsicano, Luca, Mazza, Simone M., Mcfayden, Josh, Molina-Bueno, Laura, Spreafico, Marco, Toro, Natalia, Toups, Matthew, Trojanowski, Sebastian, Tsai, Yu-Dai, Williams, Mike, Zettlemoyer, Jacob, and Zhong, Yiming
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Physics - Instrumentation and Detectors ,flavor ,hep-ex ,FOS: Physical sciences ,Instrumentation and Detectors (physics.ins-det) ,Astrophysics::Cosmology and Extragalactic Astrophysics ,dark matter ,High Energy Physics - Experiment ,thermal ,High Energy Physics - Experiment (hep-ex) ,Physics::Accelerator Physics ,Detectors and Experimental Techniques ,physics.ins-det ,Particle Physics - Experiment - Abstract
This paper provides an overview of experiments and facilities for accelerator-based dark matter searches as part of the US Community Study on the Future of Particle Physics (Snowmass 2021). Companion white papers to this paper present the physics drivers: thermal dark matter, visible dark portals, and new flavors and rich dark sectors., Comment: contribution to Snowmass 2021
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- 2022
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13. AEgIS experiment: Towards antihydrogen beam production for antimatter gravity measurements
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Mariazzi, Sebastiano, Aghion, Stefano, Amsler, Claude, Ariga, Akitaka, Ariga, Tomoko, Belov, Alexandre S., Bonomi, Germano, Bräunig, Philippe, Brusa, Roberto S., Bremer, Johan, Cabaret, Louis, Canali, Carlo, Caravita, Ruggero, Castelli, Fabrizio, Cerchiari, Giovanni, Cialdi, Simone, Comparat, Daniel, Consolati, Giovanni, Dassa, Luca, Derking, Jan Hendrik, Di Domizio, Sergio, Di Noto, Lea, Doser, Michael, Dudarev, Alexey, Ereditato, Antonio, Ferragut, Rafael, Fontana, Andrea, Genova, Pablo, Giammarchi, Marco, Gligorova, Angela, Gninenko, Sergei N., Hogan, Stephen D., Haider, Stefan, Jordan, Elena, Jørgensen, Lars V., Kaltenbacher, Thomas, Kawada, Jiro, Kellerbauer, Alban, Kimura, Mitsuhiro, Knecht, Andreas, Krasnický, Daniel, Lagomarsino, Vittorio, Lehner, Sebastian, Malbrunot, Chloe, Matveev, Viktor A., Merkt, Frederic, Moia, Fabio, Nebbia, Giancarlo, Nédélec, Patrick, Oberthaler, Markus K., Pacifico, Nicola, Petráček, Vojtech, Pistillo, Ciro, Prelz, Francesco, Prevedelli, Marco, Regenfus, Christian, Riccardi, Cristina, Røhne, Ole, Rotondi, Alberto, Sandaker, Heidi, Scampoli, Paola, Storey, James, Subieta Vasquez, Martin A., Špaček, Michal, Testera, Gemma, Vaccarone, Renzo, Villa, Fabio, Widmann, Eberhard, Zavatarelli, Sandra, and Zmeskal, Johann
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- 2014
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14. The trigger and data acquisition system of the FASER experiment
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Abreu, Henso, Mansour, Elham Amin, Casper, David, Cavanagh, Charlotte, Chen, Xin, Coccaro, Andrea, Debieux, Stephane, Dmitrievsky, Sergey, D'Onofrio, Monica, Dozen, Candan, Favre, Yannick, Fellers, Deion, Antel, Claire, Feng, Jonathan L., Ferrere, Didier, Gamberini, Enrico, Galantay, Edward Karl, Gibson, Stephen, Gonzalez-Sevilla, Sergio, Gornushkin, Yuri, Gwilliam, Carl, Hsu, Shih-Chieh, Hu, Zhen, Ariga, Akitaka, Iacobucci, Giuseppe, Inada, Tomohiro, Jakobsen, Sune, Johnson, Eliott, Kajomovitz, Enrique, Kling, Felix, Kose, Umut, Kuehn, Susanne, Lefebvre, Helena, Levinson, Lorne, Ariga, Tomoko, Li, Ke, Liu, Jinfeng, Magliocca, Chiara, McFayden, Josh, Milanesio, Matteo, Meehan, Sam, Mladenov, Dimitar, Moretti, Theo, Munker, Magdalena, Nakamura, Mitsuhiro, Bernlochner, Florian, Nakano, Toshiyuki, Nessi, Marzio, Neuhaus, Friedemann, Nevay, Laurie, Otono, Hidetoshi, Pandini, Carlo, Pang, Hao, Paolozzi, Lorenzo, Petersen, Brian, Pietropaolo, Francesco, Boeckh, Tobias, Prim, Markus, Queitsch-Maitland, Michaela, Resnati, Filippo, Rizzi, Chiara, Rokujo, Hiroki, Ruiz-Choliz, Elisa, Salfeld-Nebgen, Jakob, Sato, Osamu, Scampoli, Paola, Schmieden, Kristof, Boyd, Jamie, Schott, Matthias, Sfyrla, Anna, Shively, Savannah, Sipos, Roland, Spencer, John, Takubo, Yosuke, Tarannum, Noshin, Theiner, Ondrej, Torrence, Eric, Tufanli, Serhan, Brenner, Lydia, Vasina, Svetlana, Vormwald, Benedikt, Wang, Di, FASER Collaboration, Cadoux, Franck, Abreu, H., Amin Mansour, E., Antel, C., Ariga, A., Ariga, T., Bernlochner, F., Boeckh, T., Boyd, J., Brenner, L., Cadoux, F., Casper, D. W., Cavanagh, C., Chen, X., Coccaro, A., Débieux, S., Dmitrievsky, S., D'Onofrio, M., Dozen, C., Favre, Y., Fellers, D., Feng, J. L., Ferrere, D., Gamberini, E., Galantay, E. K., Gibson, S., Gonzalez-Sevilla, S., Gornushkin, Y., Gwilliam, C., Hsu, S. -C., Hu, Z., Iacobucci, G., Inada, T., Jakobsen, S., Johnson, E., Kajomovitz, E., Kling, F., Kose, U., Kuehn, S., Lefebvre, H., Levinson, L., Li, K., Liu, J., Magliocca, C., Mcfayden, J., Milanesio, M., Meehan, S., Mladenov, D., Moretti, T., Munker, M., Nakamura, M., Nakano, T., Nessi, M., Neuhaus, F., Nevay, L., Otono, H., Pandini, C., Pang, H., Paolozzi, L., Petersen, B., Pietropaolo, F., Prim, M., Queitsch-Maitland, M., Resnati, F., Rizzi, C., Rokujo, H., Ruiz-Cholis, E., Salfeld-Nebgen, J., Sato, O., Scampoli, P., Schmieden, K., Schott, M., Sfyrla, A., Shively, S., Sipos, R., Spencer, J., Takubo, Y., Tarannum, N., Theiner, O., Torrence, E., Tufanli, S., Vasina, S., Vormwald, B., and Wang, D.
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Physics - Instrumentation and Detectors ,Detector control systems (detector and experiment monitoring and slow-control systems, architecture, hardware, algorithms, databases) ,Physics::Instrumentation and Detectors ,data acquisition ,FOS: Physical sciences ,programming ,High Energy Physics - Experiment ,High Energy Physics - Experiment (hep-ex) ,long-lived [particle] ,tracking detector ,ddc:610 ,Detectors and Experimental Techniques ,signal processing ,Instrumentation ,physics.ins-det ,Mathematical Physics ,hep-ex ,Control and monitor systems online ,Data acquisition concepts ,Instrumentation and Detectors (physics.ins-det) ,efficiency [trigger] ,trigger: design ,monitoring ,CERN LHC Coll ,Trigger concepts and systems (hardware and software) ,trigger: efficiency ,electronics: readout ,design [electronics] ,particle: long-lived ,readout [electronics] ,Particle Physics - Experiment ,performance ,electronics: design ,design [trigger] - Abstract
Journal of Instrumentation 16(12), P12028 (2021). doi:10.1088/1748-0221/16/12/P12028, The FASER experiment is a new small and inexpensive experiment that is placed 480 meters downstream of the ATLAS experiment at the CERN LHC. FASER is designed to capture decays of new long-lived particles, produced outside of the ATLAS detector acceptance. These rare particles can decay in the FASER detector together with about 500–1000 Hz of other particles originating from the ATLAS interaction point. A very high efficiency trigger and data acquisition system is required to ensure that the physics events of interest will be recorded. This paper describes the trigger and data acquisition system of the FASER experiment and presents performance results of the system acquired during initial commissioning., Published by Inst. of Physics, London
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- 2021
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15. Deep Underground Neutrino Experiment (DUNE) Near Detector Conceptual Design Report
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Hewes, V., Abed Abud, Adam, Abi, Babak, Acciarri, Roberto, Acero, Mario, Adamov, Giorge, Adams, David, Adinolfi, Marco, Aduszkiewicz, Antoni, Ahmad, Zubayer, Ahmed, Jhanzeb, Alion, Tyler, Alonso Monsalve, Saul, Alrashed, Munerah, Alt, Christoph, Alton, Andrew, Amedo, Pablo, Anderson, John, Andreopoulos, Costas, Andrews, Michael P, Andrianala, Fenompanirina, Andringa, Sofia, Anfimov, Nikolay, Ankowski, Artur, Antonova, Maria, Antusch, Stefan, Aranda-Fernandez, Alfredo, Ariga, Akitaka, Arnold, Lukas, Arroyave, Manuel, Asaadi, Jonathan, Aurisano, Adam, Aushev, Vladimir, Autiero, Dario, Ayala-Torres, Marco Alberto, Azfar, Farrukh, Back, A., Back, Henning, Back, John, Backhouse, Chris, Baesso, Paolo, Bagaturia, Iuri, Bagby, Linda, Balasubramanian, Supraja, Baldi, Pierre, Baller, Bruce, Bambah, Bindu, Barao, Fernando, Barenboim, Gabriela, Barker, Gary J, Barkhouse, Wayne, Barnes, Christopher, Barr, Giles, Barranco Monarca, Juan, Barros, Nuno, Barrow, Joshua, Basharina-Freshville, Anastasia, Bashyal, Amit, Basque, Vincent, Batista das Chagas, Ewerton, Belchior, E., Battat, J.B. R., Battisti, Federico, Bay, Fatih, Bazo Alba, José Luis, Beacom, John, Bechetoille, Edouard, Behera, Biswaranjan, Bellantoni, Leo, Bellettini, Giorgio, Bellini, Vincenzo, Beltramello, Olga, Belver, Daniel, Benekos, Nektarios, Bento Neves, Francisco, Berkman, Sophie, Bernardini, Paolo, Berner, Roman, Berns, Hans-Gerd, Bertolucci, Sergio, Betancourt, Minerba, Betancur Rodríguez, Amalia, Bhattacharjee, Maharnab, Bhuller, Shyam, Bhuyan, Bipul, Biagi, Simone, Bian, Jianming, Biassoni, Matteo, Biery, Kurt, Bilki, Burak, Bishai, Mary, Bitadze, Alexander, Blake, Andrew, Blaszczyk, Flor de Maria, Blazey, Gerald C, Blucher, Edward, Boissevain, Jan, Bolognesi, Sara, Bolton, Timothy, Bomben, Luca, Bonesini, Maurizio, Bongrand, Mathieu, Bonini, Filiberto, Booth, Alexander, Booth, Chris, Bordoni, Stefania, Borkum, Aran, Boschi, Tommaso, Bostan, Nilay, Bour, Petr, Bourgeois, Christian, Boyd, Steve B, Boyden, Daniel, Bracinik, Juraj, Braga, Davide, Brailsford, Dominic, Brandt, Andrew, Bremer, Johan, Brew, Christopher, Brianne, Eldwan, Brice, Stephen, Brizzolari, Claudia, Bromberg, Carl, Brooijmans, Gustaaf, Brooke, Jim, Bross, Alan, Brunetti, Giulia, Brunetti, Maria, Buchanan, Norman, Budd, Howard, Cagnoli, I., Caiulo, Davide, Calafiura, Paolo, Calcutt, Jacob, Calin, Marius, Calvez, Steven, Calvo, Enrique, Caminata, Alessio, Campanelli, Mario, Cankocak, Kerem, Caratelli, David, Carini, Gabriella, Carlus, Bruno, Carniti, Paolo, Caro Terrazas, Ivan, Carranza, Hector, Carroll, Thomas, Castaño Forero, Javier, Castillo, Andrés, Castromonte, Cesar, Catano-Mur, Erika, Cattadori, Carla, Cavalier, Fabien, Cavanna, Flavio, Centro, Sandro, Cerati, Giuseppe, Cervelli, Alberto, Cervera Villanueva, Anselmo, Chalifour, Michel, Chappell, Andrew, Chardonnet, Etienne, Charitonidis, Nikolas, Chatterjee, Animesh, Chattopadhyay, Subhasish, Chen, Hucheng, Chen, Mu-Chun, Chen, Yifan, Chen, Zheyang, Cherdack, Daniel, Chi, Cheng-Yi, Childress, Sam, Chiriacescu, Ana, Chisnall, Georgia, Cho, Kihyeon, Choate, Sarah, Chokheli, David, Choubey, Sandhya, Christensen, Anne, Christian, David, Christodoulou, Georgios, Chukanov, Artem, Church, Eric, Cicero, V., Clarke, Peter, Coan, Thomas, Cocco, Alfredo, Coelho, J.A. B., Conley, Erin, Conley, Robert, Conrad, Janet M, Convery, Mark, Copello, Simone, Corwin, Luke, Cremaldi, Lucien, Cremonesi, Linda, Crespo-Anadón, José, Cristaldo, Esteban, Cross, Ryan, Cudd, Andrew, Cuesta, Clara, Cui, Yanou, Cussans, David, Dabrowski, Mieczyslaw, Dalager, Olivia, da Motta, Helio, da Silva Peres, Leonardo, David, Claire, David, Quentin, Davies, Gavin, Davini, Stefano, Dawson, Jaime, De, Kaushik, de Almeida, Rogerio, Debbins, Paul, De Bonis, Isabelle, Decowski, M Patrick, de Gouvea, Andre, de Holanda, Pedro, de Icaza Astiz, Iker, Deisting, Alexander, De Jong, Paul, Delbart, Alain, Delepine, David, Delgado, Maritza, Dell'Acqua, Andrea, De Lurgio, Patrick, de Mello Neto, J.R. T., DeMuth, David, Dennis, Steve, Densham, Chris, Deptuch, Grzegorz, De Roeck, Albert, De Romeri, Valentina, de Souza, Greg, Dharmapalan, Ranjan, Diaz, Felix, Diaz, Jorge S, Di Domizio, Sergio, Di Giulio, Letizia, Ding, Pengfei, Di Noto, Lea, Distefano, Carla, Diurba, Richard, Diwan, Milind, Djurcic, Zelimir, Dokania, Neha, Dolan, Stephen, Dolinski, Michelle J, Domine, Laura, Douglas, Daniel, Douillet, Denis, Drake, Gary, Drielsma, Francois, Duchesneau, Dominique, Duffy, Kirsty, Dunne, Patrick, Durkin, Tim, Duyang, Hongyue, Dvornikov, Olexiy, Dwyer, Daniel A, Dyshkant, Alexandre S, Eads, Michael, Earle, Antony, Edmunds, Daniel, Eisch, Jonathan, Emberger, Lorenz, Emery, Sandrine, Ereditato, Antonio, Escobar, Carlos O, Eurin, Guillaume, Evans, Justin, Ewart, Erin, Ezeribe, Anthony, Fahey, Kevin, Falcone, Andrea, Farnese, Christian, Farzan, Yasaman, Felix, Julian, Fernandes Carneiro da Silva, Mateus, Fernandez-Martinez, Enrique, Fernandez Menendez, Pablo, Ferraro, Federico, Fields, Laura, Filthaut, Frank, Fiorentini, Arturo, Fitzpatrick, Rory, Flanagan, Will, Fleming, Bonnie, Flight, Robert, Forero, David, Fowler, Jack, Fox, Walt, Franc, Jiri, Francis, Kurt, Franco, Domenico, Freeman, John, Freestone, Julian, Fried, Jack, Friedland, Alex, Fuess, Stu, Furic, Ivan, Furmanski, Andrew, Gabrielli, A., Gago, AM, Gallagher, Hugh, Gallas, Alexandre, Gallego-Ros, Ana, Gallice, Niccolo, Galymov, Vyacheslav, Gamberini, Enrico, Gamble, Trevor, Gandhi, Raj, Gandrajula, Reddy, Gao, Fan, Gao, Shanshan, Garcia-Gamez, Diego, García-Peris, Miguel, Gardiner, Steven, Gastler, Dan, Ge, Guanqun, Gelli, Bruno, Gendotti, Adamo, Gent, Stephen, Ghorbani-Moghaddam, Zahra, Gibin, Daniele, Gil-Botella, Ines, Gilligan, Sean, Girerd, Claude, Giri, Anjan Kumar, Gnani, Dario, Gogota, Olga, Gold, Michael, Gollapinni, Sowjanya, Gollwitzer, Keith, Gomes, Ricardo, Gomez Bermeo, Laura Vanessa, Fajardo, L.S. 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L.S., Warburton, Karl, Warner, David, Wascko, Morgan, Waters, David, Watson, Alan, Weatherly, Pierce, Weber, Alfons, Weber, Michele, Wei, Hanyu, Weinstein, Amanda, Wenman, Dan, Wetstein, Matthew, White, Andy, Whitehead, Leigh, Whittington, Denver, Wilking, Michael, Wilkinson, Callum, Williams, Zachary, Wilson, Fergus, Wilson, Robert, Wolcott, Jeremy, Wongjirad, Taritree, Wood, Anthony, Wood, Kevin, Worcester, Elizabeth, Worcester, Matthew, Wret, Clarence, Wu, Wanwei, Wu, Wenjie, Xiao, Yiwen, Yandel, Erin, Yang, Guang, Yang, Kang, Yang, Shaokai, Yang, Tingjun, Yankelevich, Alejandro, Yershov, Nikolai, Yonehara, Katsuya, Young, Tim, Yu, Bo, Yu, Haiwang, Yu, Jae, Yuan, Wenlong, Zaki, Rowan, Zalesak, Jaroslav, Zambelli, Laura, Zamorano, Bruno, Zani, Andrea, Zazueta, Luis, Zeit, Grace, Zeller, Geralyn, Zeller, G.P., Zennamo, Joseph, Zeug, Kyle, Zhang, Chao, Zhao, Manhong, Zhivun, Elena, Zhu, Guanying, Zilberman, Perri, Zimmerman, Eric, Zito, Marco, Zucchelli, Stefano, Zuklin, Josef, Zutshi, Vishnu, Zwaska, Robert, Science and Technology Facilities Council (STFC), Commission of the European Communities, Abud, A. A., Abi, B., Acciarri, R., Acero, M. A., Adamov, G., Adams, D., Adinolfi, M., Aduszkiewicz, A., Ahmad, Z., Ahmed, J., Alion, T., Monsalve, S. A., Alrashed, M., Alt, C., Alton, A., Amedo, P., Anderson, J., Andreopoulos, C., Andrews, M. P., Andrianala, F., Andringa, S., Anfimov, N., Ankowski, A., Antonova, M., Antusch, S., Aranda-Fernandez, A., Ariga, A., Arnold, L. O., Arroyave, M. A., Asaadi, J., Aurisano, A., Aushev, V., Autiero, D., Ayala-Torres, M., Azfar, F., Back, A., Back, H., Back, J. J., Backhouse, C., Baesso, P., Bagaturia, I., Bagby, L., Balasubramanian, S., Baldi, P., Baller, B., Bambah, B., Barao, F., Barenboim, G., Barker, G. J., Barkhouse, W., Barnes, C., Barr, G., Monarca, J. B., Barros, N., Barrow, J. L., Basharina-Freshville, A., Bashyal, A., Basque, V., Belchior, E., Battat, J. B. R., Battisti, F., Bay, F., Alba, J. L. B., Beacom, J. F., Bechetoille, E., Behera, B., Bellantoni, L., Bellettini, G., Bellini, V., Beltramello, O., Belver, D., Benekos, N., Neves, F. B., Berkman, S., Bernardini, P., Berner, R. M., Berns, H., Bertolucci, S., Betancourt, M., Rodriguez, A. B., Bhattacharjee, M., Bhuller, S., Bhuyan, B., Biagi, S., Bian, J., Biassoni, M., Biery, K., Bilki, B., Bishai, M., Bitadze, A., Blake, A., Blaszczyk, F. D. M., Blazey, G. C., Blucher, E., Boissevain, J., Bolognesi, S., Bolton, T., Bomben, L., Bonesini, M., Bongrand, M., Bonini, F., Booth, A., Booth, C., Bordoni, S., Borkum, A., Boschi, T., Bostan, N., Bour, P., Bourgeois, C., Boyd, S. B., Boyden, D., Bracinik, J., Braga, D., Brailsford, D., Brandt, A., Bremer, J., Brew, C., Brianne, E., Brice, S. J., Brizzolari, C., Bromberg, C., Brooijmans, G., Brooke, J., Bross, A., Brunetti, G., Brunetti, M., Buchanan, N., Budd, H., Cagnoli, I., Caiulo, D., Calafiura, P., Calcutt, J., Calin, M., Calvez, S., Calvo, E., Caminata, A., Campanelli, M., Cankocak, K., Caratelli, D., Carini, G., Carlus, B., Carniti, P., Terrazas, I. C., Carranza, H., Carroll, T., Castano Forero, J. F., Castillo, A., Castromonte, C., Catano-Mur, E., Cattadori, C., Cavalier, F., Cavanna, F., Centro, S., Cerati, G., Cervelli, A., Villanueva, A. C., Chalifour, M., Chappell, A., Chardonnet, E., Charitonidis, N., Chatterjee, A., Chattopadhyay, S., Chen, H., Chen, M., Chen, Y., Chen, Z., Cherdack, D., Chi, C., Childress, S., Chiriacescu, A., Chisnall, G., Cho, K., Choate, S., Chokheli, D., Choubey, S., Christensen, A., Christian, D., Christodoulou, G., Chukanov, A., Church, E., Cicero, V., Clarke, P., Coan, T. E., Cocco, A. G., Coelho, J. A. B., Conley, E., Conley, R., Conrad, J. M., Convery, M., Copello, S., Corwin, L., Cremaldi, L., Cremonesi, L., Crespo-Anadon, J. I., Cristaldo, E., Cross, R., Cudd, A., Cuesta, C., Cui, Y., Cussans, D., Dabrowski, M., Dalager, O., Da Motta, H., Da Silva Peres, L., David, C., David, Q., Davies, G. S., Davini, S., Dawson, J., De, K., De Almeida, R. M., Debbins, P., De Bonis, I., Decowski, M. P., De Gouvea, A., De Holanda, P. C., De Icaza Astiz, I. L., Deisting, A., De Jong, P., Delbart, A., Delepine, D., Delgado, M., Dell'Acqua, A., De Lurgio, P., De Mello Neto, J. R. T., De Muth, D. M., Dennis, S., Densham, C., Deptuch, G. W., De Roeck, A., De Romeri, V., De Souza, G., Dharmapalan, R., Diaz, F., Diaz, J. S., Di Domizio, S., Di Giulio, L., Ding, P., Di Noto, L., Distefano, C., Diurba, R., Diwan, M., Djurcic, Z., Dokania, N., Dolan, S., Dolinski, M. J., Domine, L., Douglas, D., Douillet, D., Drake, G., Drielsma, F., Duchesneau, D., Duffy, K., Dunne, P., Durkin, T., Duyang, H., Dvornikov, O., Dwyer, D. A., Dyshkant, A. S., Eads, M., Earle, A., Edmunds, D., Eisch, J., Emberger, L., Emery, S., Ereditato, A., Escobar, C. O., Eurin, G., Evans, J. J., Ewart, E., Ezeribe, A. C., Fahey, K., Falcone, A., Farnese, C., Farzan, Y., Felix, J., Carneiro Da Silva, M. F., Fernandez-Martinez, E., Fernandez Menendez, P., Ferraro, F., Fields, L., Filthaut, F., Fiorentini, A., Fitzpatrick, R. S., Flanagan, W., Fleming, B., Flight, R., Forero, D. V., Fowler, J., Fox, W., Franc, J., Francis, K., Franco, D., Freeman, J., Freestone, J., Fried, J., Friedland, A., Fuess, S., Furic, I., Furmanski, A. P., Gabrielli, A., Gago, A., Gallagher, H., Gallas, A., Gallego-Ros, A., Gallice, N., Galymov, V., Gamberini, E., Gamble, T., Gandhi, R., Gandrajula, R., Gao, F., Gao, S., Garcia-Gamez, D., Garcia-Peris, M. A., Gardiner, S., Gastler, D., Ge, G., Gelli, B., Gendotti, A., Gent, S., Ghorbani-Moghaddam, Z., Gibin, D., Gil-Botella, I., Gilligan, S., Girerd, C., Giri, A. K., Gnani, D., Gogota, O., Gold, M., Gollapinni, S., Gollwitzer, K., Gomes, R. A., Gomez Bermeo, L. V., Gomez Fajardo, L. S., Gonnella, F., Gonzalez-Cuevas, J. A., Gonzalez-Diaz, D., Gonzalez-Lopez, M., Goodman, M. C., Goodwin, O., Goswami, S., Gotti, C., Goudzovski, E., Grace, C., Graham, M., Gran, R., Granados, E., Granger, P., Grant, A., Grant, C., Gratieri, D., Green, P., Greenler, L., Greer, J., Griffith, W. C., Groh, M., Grudzinski, J., Grzelak, K., Gu, W., Guarino, V., Guenette, R., Guerard, E., Guerzoni, M., Guglielmi, A., Guo, B., Guthikonda, K. K., Gutierrez, R., Guzowski, P., Guzzo, M. M., Gwon, S., Habig, A., Hadavand, H., Haenni, R., Hahn, A., Haiston, J., Hamacher-Baumann, P., Hamernik, T., Hamilton, P., Han, J., Harris, D. A., Hartnell, J., Harton, J., Hasegawa, T., Hasnip, C., Hatcher, R., Hatfield, K. W., Hatzikoutelis, A., Hayes, C., Hazen, E., Heavey, A., Heeger, K. M., Heise, J., Hennessy, K., Henry, S., Hernandez Morquecho, M. A., Herner, K., Hertel, L., Hewes, J., Higuera, A., Hill, T., Hillier, S. J., Himmel, A., Hoff, J., Hohl, C., Holin, A., Hoppe, E., Horton-Smith, G. A., Hostert, M., Hourlier, A., Howard, B., Howell, R., Huang, J., Hugon, J., Iles, G., Ilic, N., Iliescu, A. M., Illingworth, R., Ingratta, G., Ioannisian, A., Isenhower, L., Itay, R., Izmaylov, A., Jackson, S., Jain, V., James, E., Jargowsky, B., Jediny, F., Jena, D., Jeong, Y. S., Jesus-Valls, C., Ji, X., Jiang, L., Jimenez, S., Jipa, A., Johnson, R., Johnston, N., Jones, B., Jones, S. B., Judah, M., Jung, C. K., Junk, T., Jwa, Y., Kabirnezhad, M., Kaboth, A., Kadenko, I., Kakorin, I., Kamiya, F., Kaneshige, N., Karagiorgi, G., Karaman, G., Karcher, A., Karolak, M., Karyotakis, Y., Kasai, S., Kasetti, S. P., Kashur, L., Kazaryan, N., Kearns, E., Keener, P., Kelly, K. J., Kemp, E., Kemularia, O., Ketchum, W., Kettell, S. H., Khabibullin, M., Khotjantsev, A., Khvedelidze, A., Kim, D., King, B., Kirby, B., Kirby, M., Klein, J., Koehler, K., Koerner, L. W., Kohn, S., Koller, P. P., Kolupaeva, L., Kordosky, M., Kosc, T., Kose, U., Kostelecky, V. A., Kothekar, K., Krennrich, F., Kreslo, I., Kudenko, Y., Kudryavtsev, V. A., Kulagin, S., Kumar, J., Kumar, P., Kumar, R., Kunze, P., Kurita, N., Kuruppu, C., Kus, V., Kutter, T., Lambert, A., Land, B., Lande, K., Lane, C. 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A., Mokhov, N., Molina, J., Molina Bueno, L., Montanari, A., Montanari, C., Montanari, D., Montagna, E., Montano Zetina, L. M., Moon, J., Mooney, M., Moor, A. F., Moreno, D., Morris, C., Mossey, C., Motuk, E., Moura, C. A., Mousseau, J., Mu, W., Mualem, L., Mueller, J., Muether, M., Mufson, S., Muheim, F., Muir, A., Mulhearn, M., Munford, D., Muramatsu, H., Murphy, S., Musser, J., Nachtman, J., Nagu, S., Nalbandyan, M., Nandakumar, R., Naples, D., Narita, S., Navas-Nicolas, D., Navrer-Agasson, A., Nayak, N., Nebot-Guinot, M., Negishi, K., Nelson, J. K., Nesbit, J., Nessi, M., Newbold, D., Newcomer, M., Newhart, D., Newton, H., Niccolo, M., Nichol, R., Nicolas-Arnaldos, F., Nicoletta, M., Niner, E., Nishimura, K., Norman, A., Norrick, A., Northrop, R., Novella, P., Nowak, J. A., Oberling, M., Ochoa-Ricoux, J. P., Olivares Del Campo, A., Olivier, A., Olshevskiy, A., Onel, Y., Onishchuk, Y., Ott, J., Pagani, L., Pakvasa, S., Palacio, G., Palamara, O., Palestini, S., Paley, J. 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D., Zito, M., Zucchelli, S., Zuklin, J., Zutshi, V., Zwaska, R., Institut de Physique des 2 Infinis de Lyon (IP2I Lyon), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Centre National de la Recherche Scientifique (CNRS), 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 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), AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres 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IoP, FNWI), Other Research IHEF (IoP, FNWI), ATLAS (IHEF, IoP, FNWI), IHEF (IoP, FNWI), Abud A.A., Abi B., Acciarri R., Acero M.A., Adamov G., Adams D., Adinolfi M., Aduszkiewicz A., Ahmad Z., Ahmed J., Alion T., Monsalve S.A., Alrashed M., Alt C., Alton A., Amedo P., Anderson J., Andreopoulos C., Andrews M.P., Andrianala F., Andringa S., Anfimov N., Ankowski A., Antonova M., Antusch S., Aranda-Fernandez A., Ariga A., Arnold L.O., Arroyave M.A., Asaadi J., Aurisano A., Aushev V., Autiero D., Ayala-Torres M., Azfar F., Back A., Back H., Back J.J., Backhouse C., Baesso P., Bagaturia I., Bagby L., Balasubramanian S., Baldi P., Baller B., Bambah B., Barao F., Barenboim G., Barker G.J., Barkhouse W., Barnes C., Barr G., Monarca J.B., Barros N., Barrow J.L., Basharina-Freshville A., Bashyal A., Basque V., Belchior E., Battat J.B.R., Battisti F., Bay F., Alba J.L.B., Beacom J.F., Bechetoille E., Behera B., Bellantoni L., Bellettini G., Bellini V., Beltramello O., Belver D., Benekos N., Neves F.B., Berkman S., Bernardini P., Berner R.M., Berns H., Bertolucci S., Betancourt M., Rodriguez A.B., Bhattacharjee M., Bhuller S., Bhuyan B., Biagi S., Bian J., Biassoni M., Biery K., Bilki B., Bishai M., Bitadze A., Blake A., Blaszczyk F.D.M., Blazey G.C., Blucher E., Boissevain J., Bolognesi S., Bolton T., Bomben L., Bonesini M., Bongrand M., Bonini F., Booth A., Booth C., Bordoni S., Borkum A., Boschi T., Bostan N., Bour P., Bourgeois C., Boyd S.B., Boyden D., Bracinik J., Braga D., Brailsford D., Brandt A., Bremer J., Brew C., Brianne E., Brice S.J., Brizzolari C., Bromberg C., Brooijmans G., Brooke J., Bross A., Brunetti G., Brunetti M., Buchanan N., Budd H., Cagnoli I., Caiulo D., Calafiura P., Calcutt J., Calin M., Calvez S., Calvo E., Caminata A., Campanelli M., Cankocak K., Caratelli D., Carini G., Carlus B., Carniti P., Terrazas I.C., Carranza H., Carroll T., Castano Forero J.F., Castillo A., Castromonte C., Catano-Mur E., Cattadori C., Cavalier F., Cavanna F., Centro S., Cerati G., Cervelli A., Villanueva A.C., Chalifour M., Chappell A., Chardonnet E., Charitonidis N., Chatterjee A., Chattopadhyay S., Chen H., Chen M., Chen Y., Chen Z., Cherdack D., Chi C., Childress S., Chiriacescu A., Chisnall G., Cho K., Choate S., Chokheli D., Choubey S., Christensen A., Christian D., Christodoulou G., Chukanov A., Church E., Cicero V., Clarke P., Coan T.E., Cocco A.G., Coelho J.A.B., Conley E., Conley R., Conrad J.M., Convery M., Copello S., Corwin L., Cremaldi L., Cremonesi L., Crespo-Anadon J.I., Cristaldo E., Cross R., Cudd A., Cuesta C., Cui Y., Cussans D., Dabrowski M., Dalager O., Da Motta H., Da Silva Peres L., David C., David Q., Davies G.S., Davini S., Dawson J., De K., De Almeida R.M., Debbins P., De Bonis I., Decowski M.P., De Gouvea A., De Holanda P.C., De Icaza Astiz I.L., Deisting A., De Jong P., Delbart A., Delepine D., Delgado M., Dell'Acqua A., De Lurgio P., De Mello Neto J.R.T., De Muth D.M., Dennis S., Densham C., Deptuch G.W., De Roeck A., De Romeri V., De Souza G., Dharmapalan R., Diaz F., Diaz J.S., Di Domizio S., Di Giulio L., Ding P., Di Noto L., Distefano C., Diurba R., Diwan M., Djurcic Z., Dokania N., Dolan S., Dolinski M.J., Domine L., Douglas D., Douillet D., Drake G., Drielsma F., Duchesneau D., Duffy K., Dunne P., Durkin T., Duyang H., Dvornikov O., Dwyer D.A., Dyshkant A.S., Eads M., Earle A., Edmunds D., Eisch J., Emberger L., Emery S., Ereditato A., Escobar C.O., Eurin G., Evans J.J., Ewart E., Ezeribe A.C., Fahey K., Falcone A., Farnese C., Farzan Y., Felix J., Carneiro Da Silva M.F., Fernandez-Martinez E., Fernandez Menendez P., Ferraro F., Fields L., Filthaut F., Fiorentini A., Fitzpatrick R.S., Flanagan W., Fleming B., Flight R., Forero D.V., Fowler J., Fox W., Franc J., Francis K., Franco D., Freeman J., Freestone J., Fried J., Friedland A., Fuess S., Furic I., Furmanski A.P., Gabrielli A., Gago A., Gallagher H., Gallas A., Gallego-Ros A., Gallice N., Galymov V., Gamberini E., Gamble T., Gandhi R., Gandrajula R., Gao F., Gao S., Garcia-Gamez D., Garcia-Peris M.A., Gardiner S., Gastler D., Ge G., Gelli B., Gendotti A., Gent S., Ghorbani-Moghaddam Z., Gibin D., Gil-Botella I., Gilligan S., Girerd C., Giri A.K., Gnani D., Gogota O., Gold M., Gollapinni S., Gollwitzer K., Gomes R.A., Gomez Bermeo L.V., Gomez Fajardo L.S., Gonnella F., Gonzalez-Cuevas J.A., Gonzalez-Diaz D., Gonzalez-Lopez M., Goodman M.C., Goodwin O., Goswami S., Gotti C., Goudzovski E., Grace C., Graham M., Gran R., Granados E., Granger P., Grant A., Grant C., Gratieri D., Green P., Greenler L., Greer J., Griffith W.C., Groh M., Grudzinski J., Grzelak K., Gu W., Guarino V., Guenette R., Guerard E., Guerzoni M., Guglielmi A., Guo B., Guthikonda K.K., Gutierrez R., Guzowski P., Guzzo M.M., Gwon S., Habig A., Hadavand H., Haenni R., Hahn A., Haiston J., Hamacher-Baumann P., Hamernik T., Hamilton P., Han J., Harris D.A., Hartnell J., Harton J., Hasegawa T., Hasnip C., Hatcher R., Hatfield K.W., Hatzikoutelis A., Hayes C., Hazen E., Heavey A., Heeger K.M., Heise J., Hennessy K., Henry S., Hernandez Morquecho M.A., Herner K., Hertel L., Hewes J., Higuera A., Hill T., Hillier S.J., Himmel A., Hoff J., Hohl C., Holin A., Hoppe E., Horton-Smith G.A., Hostert M., Hourlier A., Howard B., Howell R., Huang J., Hugon J., Iles G., Ilic N., Iliescu A.M., Illingworth R., Ingratta G., Ioannisian A., Isenhower L., Itay R., Izmaylov A., Jackson S., Jain V., James E., Jargowsky B., Jediny F., Jena D., Jeong Y.S., Jesus-Valls C., Ji X., Jiang L., Jimenez S., Jipa A., Johnson R., Johnston N., Jones B., Jones S.B., Judah M., Jung C.K., Junk T., Jwa Y., Kabirnezhad M., Kaboth A., Kadenko I., Kakorin I., Kamiya F., Kaneshige N., Karagiorgi G., Karaman G., Karcher A., Karolak M., Karyotakis Y., Kasai S., Kasetti S.P., Kashur L., Kazaryan N., Kearns E., Keener P., Kelly K.J., Kemp E., Kemularia O., Ketchum W., Kettell S.H., Khabibullin M., Khotjantsev A., Khvedelidze A., Kim D., King B., Kirby B., Kirby M., Klein J., Koehler K., Koerner L.W., Kohn S., Koller P.P., Kolupaeva L., Kordosky M., Kosc T., Kose U., Kostelecky V.A., Kothekar K., Krennrich F., Kreslo I., Kudenko Y., Kudryavtsev V.A., Kulagin S., Kumar J., Kumar P., Kumar R., Kunze P., Kurita N., Kuruppu C., Kus V., Kutter T., Lambert A., Land B., Lande K., Lane C.E., Lang K., Langford T., Larkin J., Lasorak P., Last D., Lastoria C., Laundrie A., Laurenti G., Lawrence A., Lazanu I., Lazur R., Le T., Leardini S., Learned J., Lebrun P., Lecompte T., Lehmann Miotto G., Lehnert R., Leigui De Oliveira M.A., Leitner M., Li L., Li S.W., Li T., Li Y., Liao H., Lin C.S., Lin Q., Lin S., Lister A., Littlejohn B.R., Liu J., Lockwitz S., Loew T., Lokajicek M., Lomidze I., Long K., Loo K., Lorca D., Lord T., Losecco J.M., Louis W.C., Lu X.-G., Luk K.B., Luo X., Lurkin N., Lux T., Luzio V.P., Macfarlane D., Machado A.A., Machado P., Macias C.T., Macier J.R., Maddalena A., Madera A., Madigan P., Magill S., Mahn K., Maio A., Major A., Maloney J.A., Mandrioli G., Mandujano R.C., Maneira J., Manenti L., Manly S., Mann A., Manolopoulos K., Manrique Plata M., Manyam V.N., Manzanillas L., Marchan M., Marchionni A., Marciano W., Marfatia D., Mariani C., Maricic J., Marie R., Marinho F., Marino A.D., Marsden D., Marshak M., Marshall C.M., Marshall J., Marteau J., Martin-Albo J., Martinez N., Martinez Caicedo D.A., Martynenko S., Mason K., Mastbaum A., Masud M., Matsuno S., Matthews J., Mauger C., Mauri N., Mavrokoridis K., Mawby I., Mazza R., Mazzacane A., Mazzucato E., McAskill T., McCluskey E., McConkey N., McFarland K.S., McGrew C., McNab A., Mefodiev A., Mehta P., Melas P., Mena O., Menary S., Mendez H., Mendez D.P., Menegolli A., Meng G., Messier M.D., Metcalf W., Mettler T., Mewes M., Meyer H., Miao T., Michna G., Miedema T., Migenda J., Mikola V., Milincic R., Miller W., Mills J., Milne C., Mineev O., Miranda O.G., Miryala S., Mishra C.S., Mishra S.R., Mislivec A., Mladenov D., Mocioiu I., Moffat K., Moggi N., Mohanta R., Mohayai 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(IN2P3)-Centre National de la Recherche Scientifique (CNRS), Abud, A, Abi, B, Acciarri, R, Acero, M, Adamov, G, Adams, D, Adinolfi, M, Aduszkiewicz, A, Ahmad, Z, Ahmed, J, Alion, T, Monsalve, S, Alrashed, M, Alt, C, Alton, A, Amedo, P, Anderson, J, Andreopoulos, C, Andrews, M, Andrianala, F, Andringa, S, Anfimov, N, Ankowski, A, Antonova, M, Antusch, S, Aranda-Fernandez, A, Ariga, A, Arnold, L, Arroyave, M, Asaadi, J, Aurisano, A, Aushev, V, Autiero, D, Ayala-Torres, M, Azfar, F, Back, A, Back, H, Back, J, Backhouse, C, Baesso, P, Bagaturia, I, Bagby, L, Balasubramanian, S, Baldi, P, Baller, B, Bambah, B, Barao, F, Barenboim, G, Barker, G, Barkhouse, W, Barnes, C, Barr, G, Monarca, J, Barros, N, Barrow, J, Basharina-Freshville, A, Bashyal, A, Basque, V, Belchior, E, Battat, J, Battisti, F, Bay, F, Alba, J, Beacom, J, Bechetoille, E, Behera, B, Bellantoni, L, Bellettini, G, Bellini, V, Beltramello, O, Belver, D, Benekos, N, Neves, F, Berkman, S, Bernardini, P, Berner, R, Berns, H, Bertolucci, S, Betancourt, M, Rodriguez, A, Bhattacharjee, M, Bhuller, S, Bhuyan, B, Biagi, S, Bian, J, Biassoni, M, Biery, K, Bilki, B, Bishai, M, Bitadze, A, Blake, A, Blaszczyk, F, Blazey, G, Blucher, E, Boissevain, J, Bolognesi, S, Bolton, T, Bomben, L, Bonesini, M, Bongrand, M, Bonini, F, Booth, A, Booth, C, Bordoni, S, Borkum, A, Boschi, T, Bostan, N, Bour, P, Bourgeois, C, Boyd, S, Boyden, D, Bracinik, J, Braga, D, Brailsford, D, Brandt, A, Bremer, J, Brew, C, Brianne, E, Brice, S, Brizzolari, C, Bromberg, C, Brooijmans, G, Brooke, J, Bross, A, Brunetti, G, Brunetti, M, Buchanan, N, Budd, H, Cagnoli, I, Caiulo, D, Calafiura, P, Calcutt, J, Calin, M, Calvez, S, Calvo, E, Caminata, A, Campanelli, M, Cankocak, K, Caratelli, D, Carini, G, Carlus, B, Carniti, P, Terrazas, I, Carranza, H, Carroll, T, Castano Forero, J, Castillo, A, Castromonte, C, Catano-Mur, E, Cattadori, C, Cavalier, F, Cavanna, F, Centro, S, Cerati, G, Cervelli, A, Villanueva, A, Chalifour, M, Chappell, A, Chardonnet, E, Charitonidis, N, Chatterjee, A, Chattopadhyay, S, Chen, H, Chen, M, Chen, Y, Chen, Z, Cherdack, D, Chi, C, Childress, S, Chiriacescu, A, Chisnall, G, Cho, K, Choate, S, Chokheli, D, Choubey, S, Christensen, A, Christian, D, Christodoulou, G, Chukanov, A, Church, E, Cicero, V, Clarke, P, Coan, T, Cocco, A, Coelho, J, Conley, E, Conley, R, Conrad, J, Convery, M, Copello, S, Corwin, L, Cremaldi, L, Cremonesi, L, Crespo-Anadon, J, Cristaldo, E, Cross, R, Cudd, A, Cuesta, C, Cui, Y, Cussans, D, Dabrowski, M, Dalager, O, Da Motta, H, Da Silva Peres, L, David, C, David, Q, Davies, G, Davini, S, Dawson, J, De, K, De Almeida, R, Debbins, P, De Bonis, I, Decowski, M, De Gouvea, A, De Holanda, P, De Icaza Astiz, I, Deisting, A, De Jong, P, Delbart, A, Delepine, D, Delgado, M, Dell'Acqua, A, De Lurgio, P, De Mello Neto, J, De Muth, D, Dennis, S, Densham, C, Deptuch, G, De Roeck, A, De Romeri, V, De Souza, G, Dharmapalan, R, Diaz, F, Diaz, J, Di Domizio, S, Di Giulio, L, Ding, P, Di Noto, L, Distefano, C, Diurba, R, Diwan, M, Djurcic, Z, Dokania, N, Dolan, S, Dolinski, M, Domine, L, Douglas, D, Douillet, D, Drake, G, Drielsma, F, Duchesneau, D, Duffy, K, Dunne, P, Durkin, T, Duyang, H, Dvornikov, O, Dwyer, D, Dyshkant, A, Eads, M, Earle, A, Edmunds, D, Eisch, J, Emberger, L, Emery, S, Ereditato, A, Escobar, C, Eurin, G, Evans, J, Ewart, E, Ezeribe, A, Fahey, K, Falcone, A, Farnese, C, Farzan, Y, Felix, J, Carneiro Da Silva, M, Fernandez-Martinez, E, Fernandez Menendez, P, Ferraro, F, Fields, L, Filthaut, F, Fiorentini, A, Fitzpatrick, R, Flanagan, W, Fleming, B, Flight, R, Forero, D, Fowler, J, Fox, W, Franc, J, Francis, K, Franco, D, Freeman, J, Freestone, J, Fried, J, Friedland, A, Fuess, S, Furic, I, Furmanski, A, Gabrielli, A, Gago, A, Gallagher, H, Gallas, A, Gallego-Ros, A, Gallice, N, Galymov, V, Gamberini, E, Gamble, T, Gandhi, R, Gandrajula, R, Gao, F, Gao, S, Garcia-Gamez, D, Garcia-Peris, M, Gardiner, S, Gastler, D, Ge, G, Gelli, B, Gendotti, A, Gent, S, Ghorbani-Moghaddam, Z, Gibin, D, Gil-Botella, I, Gilligan, S, Girerd, C, Giri, A, Gnani, D, Gogota, O, Gold, M, Gollapinni, S, Gollwitzer, K, Gomes, R, Gomez Bermeo, L, Gomez Fajardo, L, Gonnella, F, Gonzalez-Cuevas, J, Gonzalez-Diaz, D, Gonzalez-Lopez, M, Goodman, M, Goodwin, O, Goswami, S, Gotti, C, Goudzovski, E, Grace, C, Graham, M, Gran, R, Granados, E, Granger, P, Grant, A, Grant, C, Gratieri, D, Green, P, Greenler, L, Greer, J, Griffith, W, Groh, M, Grudzinski, J, Grzelak, K, Gu, W, Guarino, V, Guenette, R, Guerard, E, Guerzoni, M, Guglielmi, A, Guo, B, Guthikonda, K, Gutierrez, R, Guzowski, P, Guzzo, M, Gwon, S, Habig, A, Hadavand, H, Haenni, R, Hahn, A, Haiston, J, Hamacher-Baumann, P, Hamernik, T, Hamilton, P, Han, J, Harris, D, Hartnell, J, Harton, J, Hasegawa, T, Hasnip, C, Hatcher, R, Hatfield, K, Hatzikoutelis, A, Hayes, C, Hazen, E, Heavey, A, Heeger, K, Heise, J, Hennessy, K, Henry, S, Hernandez Morquecho, M, Herner, K, Hertel, L, Hewes, J, Higuera, A, Hill, T, Hillier, S, Himmel, A, Hoff, J, Hohl, C, Holin, A, Hoppe, E, Horton-Smith, G, Hostert, M, Hourlier, A, Howard, B, Howell, R, Huang, J, Hugon, J, Iles, G, Ilic, N, Iliescu, A, Illingworth, R, Ingratta, G, Ioannisian, A, Isenhower, L, Itay, R, Izmaylov, A, Jackson, S, Jain, V, James, E, Jargowsky, B, Jediny, F, Jena, D, Jeong, Y, Jesus-Valls, C, Ji, X, Jiang, L, Jimenez, S, Jipa, A, Johnson, R, Johnston, N, Jones, B, Jones, S, Judah, M, Jung, C, Junk, T, Jwa, Y, Kabirnezhad, M, Kaboth, A, Kadenko, I, Kakorin, I, Kamiya, F, Kaneshige, N, Karagiorgi, G, Karaman, G, Karcher, A, Karolak, M, Karyotakis, Y, Kasai, S, Kasetti, S, Kashur, L, Kazaryan, N, Kearns, E, Keener, P, Kelly, K, Kemp, E, Kemularia, O, Ketchum, W, Kettell, S, Khabibullin, M, Khotjantsev, A, Khvedelidze, A, Kim, D, King, B, Kirby, B, Kirby, M, Klein, J, Koehler, K, Koerner, L, Kohn, S, Koller, P, Kolupaeva, L, Kordosky, M, Kosc, T, Kose, U, Kostelecky, V, Kothekar, K, Krennrich, F, Kreslo, I, Kudenko, Y, Kudryavtsev, V, Kulagin, S, Kumar, J, Kumar, P, Kumar, R, Kunze, P, Kurita, N, Kuruppu, C, Kus, V, Kutter, T, Lambert, A, Land, B, Lande, K, Lane, C, Lang, K, Langford, T, Larkin, J, Lasorak, P, Last, D, Lastoria, C, Laundrie, A, Laurenti, G, Lawrence, A, Lazanu, I, Lazur, R, Le, T, Leardini, S, Learned, J, Lebrun, P, Lecompte, T, Lehmann Miotto, G, Lehnert, R, Leigui De Oliveira, M, Leitner, M, Li, L, Li, S, Li, T, Li, Y, Liao, H, Lin, C, Lin, Q, Lin, S, Lister, A, Littlejohn, B, Liu, J, Lockwitz, S, Loew, T, Lokajicek, M, Lomidze, I, Long, K, Loo, K, Lorca, D, Lord, T, Losecco, J, Louis, W, Lu, X, Luk, K, Luo, X, Lurkin, N, Lux, T, Luzio, V, Macfarlane, D, Machado, A, Machado, P, Macias, C, Macier, J, Maddalena, A, Madera, A, Madigan, P, Magill, S, Mahn, K, Maio, A, Major, A, Maloney, J, Mandrioli, G, Mandujano, R, Maneira, J, Manenti, L, Manly, S, Mann, A, Manolopoulos, K, Manrique Plata, M, Manyam, V, Manzanillas, L, Marchan, M, Marchionni, A, Marciano, W, Marfatia, D, Mariani, C, Maricic, J, Marie, R, Marinho, F, Marino, A, Marsden, D, Marshak, M, Marshall, C, Marshall, J, Marteau, J, Martin-Albo, J, Martinez, N, Martinez Caicedo, D, Martynenko, S, Mason, K, Mastbaum, A, Masud, M, Matsuno, S, Matthews, J, Mauger, C, Mauri, N, Mavrokoridis, K, Mawby, I, Mazza, R, Mazzacane, A, Mazzucato, E, Mcaskill, T, Mccluskey, E, Mcconkey, N, Mcfarland, K, Mcgrew, C, Mcnab, A, Mefodiev, A, Mehta, P, Melas, P, Mena, O, Menary, S, Mendez, H, Mendez, D, Menegolli, A, Meng, G, Messier, M, Metcalf, W, Mettler, T, Mewes, M, Meyer, H, Miao, T, Michna, G, Miedema, T, Migenda, J, Mikola, V, Milincic, R, Miller, W, Mills, J, Milne, C, Mineev, O, Miranda, O, Miryala, S, Mishra, C, Mishra, S, Mislivec, A, Mladenov, D, Mocioiu, I, Moffat, K, Moggi, N, Mohanta, R, Mohayai, T, Mokhov, N, Molina, J, Molina Bueno, L, Montanari, A, Montanari, C, Montanari, D, Montagna, E, Montano Zetina, L, Moon, J, Mooney, M, Moor, A, Moreno, D, Morris, C, Mossey, C, Motuk, E, Moura, C, Mousseau, J, Mu, W, Mualem, L, Mueller, J, Muether, M, Mufson, S, Muheim, F, Muir, A, Mulhearn, M, Munford, D, Muramatsu, H, Murphy, S, Musser, J, Nachtman, J, Nagu, S, Nalbandyan, M, Nandakumar, R, Naples, D, Narita, S, Navas-Nicolas, D, Navrer-Agasson, A, Nayak, N, Nebot-Guinot, M, Negishi, K, Nelson, J, Nesbit, J, Nessi, M, Newbold, D, Newcomer, M, Newhart, D, Newton, H, Niccolo, M, Nichol, R, Nicolas-Arnaldos, F, Nicoletta, M, Niner, E, Nishimura, K, Norman, A, Norrick, A, Northrop, R, Novella, P, Nowak, J, Oberling, M, Ochoa-Ricoux, J, Olivares Del Campo, A, Olivier, A, Olshevskiy, A, Onel, Y, Onishchuk, Y, Ott, J, Pagani, L, Pakvasa, S, Palacio, G, Palamara, O, Palestini, S, Paley, J, Pallavicini, M, Palomares, C, Palomino-Gallo, J, Pantic, E, Paolone, V, Papadimitriou, V, Papaleo, R, Papanestis, A, Paramesvaran, S, Parke, S, Parsa, Z, Parvu, M, Pascoli, S, Pasqualini, L, Pasternak, J, Pater, J, Patrick, C, Patrizii, L, Patterson, R, Patton, S, Patzak, T, Paudel, A, Paulos, B, Paulucci, L, Pavlovic, Z, Pawloski, G, Payne, D, Pec, V, Peeters, S, Pennacchio, E, Penzo, A, Peres, O, Perry, J, Pershey, D, Pessina, G, Petrillo, G, Petta, C, Petti, R, Piastra, F, Pickering, L, Pietropaolo, F, Plunkett, R, Poling, R, Pons, X, Poonthottathil, N, Poppi, F, Pordes, S, Porter, J, Potekhin, M, Potenza, R, Potukuchi, B, Pozimski, J, Pozzato, M, Prakash, S, Prakash, T, Prince, S, Pugnere, D, Qian, X, Queiroga Bazetto, M, Raaf, J, Radeka, V, Rademacker, J, Radics, B, Rafique, A, Raguzin, E, Rai, M, Rajaoalisoa, M, Rakhno, I, Rakotonandrasana, A, Rakotondravohitra, L, Ramachers, Y, Rameika, R, Ramirez Delgado, M, Ramson, B, Rappoldi, A, Raselli, G, Ratoff, P, Raut, S, Razakamiandra, R, Real, J, Rebel, B, Reggiani-Guzzo, M, Rehak, T, Reichenbacher, J, Reitzner, S, Rejeb Sfar, H, Renshaw, A, Rescia, S, Resnati, F, Reynolds, A, Riccio, C, Riccobene, G, Rice, L, Ricol, J, Rigamonti, A, Rigaut, Y, Rivera, D, Rochester, L, Roda, M, Rodrigues, P, Rodriguez Alonso, M, Rodriguez Bonilla, E, Rodriguez Rondon, J, Rosauro-Alcaraz, S, Rosenberg, M, Rosier, P, Roskovec, B, Rossella, M, Rout, J, Roy, P, Roy, S, Rubbia, A, Rubbia, C, Rubio, F, Russell, B, Ruterbories, D, Saakyan, R, Sacerdoti, S, Safford, T, Sahay, R, Sahu, N, Sala, P, Samios, N, Samoylov, O, Sanchez, M, Sanders, D, Sankey, D, Santana, S, Santos-Maldonado, M, Saoulidou, N, Sapienza, P, Sarasty, C, Sarcevic, I, Savage, G, Savinov, V, Scaramelli, A, Scarff, A, Scarpelli, A, Schaffer, T, Schellman, H, Schlabach, P, Schmitz, D, Scholberg, K, Schukraft, A, Segreto, E, Sensenig, J, Seong, I, Sergi, A, Sgalaberna, D, Shaevitz, M, Shafaq, S, Shamma, M, Sharankova, R, Sharma, H, Sharma, R, Shaw, T, Shepherd-Themistocleous, C, Shin, S, Shooltz, D, Shrock, R, Simard, L, Simon, F, Simos, N, Sinclair, J, Sinev, G, Singh, J, Singh, V, Sipos, R, Sippach, F, Sirri, G, Sitraka, A, Siyeon, K, Skarpaas, K, Smith, A, Smith, E, Smith, P, Smolik, J, Smy, M, Snider, E, Snopok, P, Soares Nunes, M, Sobel, H, Soderberg, M, Solano Salinas, C, Soldner-Rembold, S, Soleti, S, Solomey, N, Solovov, V, Sondheim, W, Sorel, M, Soto-Oton, J, Sousa, A, Soustruznik, K, Spagliardi, F, Spanu, M, Spitz, J, Spooner, N, Spurgeon, K, Staley, R, Stancari, M, Stanco, L, Stanley, R, Stein, R, Steiner, H, Stewart, J, Stillwell, B, Stock, J, Stocker, F, Stokes, T, Strait, M, Strauss, T, Striganov, S, Stuart, A, Suarez, J, Sullivan, H, Summers, D, Surdo, A, Susic, V, Suter, L, Sutera, C, Svoboda, R, Szczerbinska, B, Szelc, A, Talaga, R, Tanaka, H, Oregui, B, Tapper, A, Tariq, S, Tatar, E, Tayloe, R, Teklu, A, Tenti, M, Terao, K, Ternes, C, Terranova, F, Testera, G, Thea, A, Thompson, J, Thorn, C, Timm, S, Todd, J, Tonazzo, A, Torbunov, D, Torti, M, Tortola, M, Tortorici, F, Totani, D, Toups, M, Touramanis, C, Tosi, N, Travaglini, R, Trevor, J, Trilov, S, Trzaska, W, Tsai, Y, Tsamalaidze, Z, Tsang, K, Tsverava, N, Tufanli, S, Tull, C, Tyley, E, Tzanov, M, Uchida, M, Urheim, J, Usher, T, Uzunyan, S, Vagins, M, Vahle, P, Valdiviesso, G, Valencia, E, Valerio, P, Vallari, Z, Valle, J, Vallecorsa, S, Van Berg, R, Van De Water, R, Varanini, F, Vargas, D, Varner, G, Vasel, J, Vasina, S, Vasseur, G, Vaughan, N, Vaziri, K, Ventura, S, Verdugo, A, Vergani, S, Vermeulen, M, Verzocchi, M, Vicenzi, M, Vieira De Souza, H, Vignoli, C, Vilela, C, Viren, B, Vrba, T, Wachala, T, Waldron, A, Wallbank, M, Wang, H, Wang, J, Wang, L, Wang, M, Wang, Y, Warburton, K, Warner, D, Wascko, M, Waters, D, Watson, A, Weatherly, P, Weber, A, Weber, M, Wei, H, Weinstein, A, Wenman, D, Wetstein, M, White, A, Whitehead, L, Whittington, D, Wilking, M, Wilkinson, C, Williams, Z, Wilson, F, Wilson, R, Wolcott, J, Wongjirad, T, Wood, A, Wood, K, Worcester, E, Worcester, M, Wret, C, Wu, W, Xiao, Y, Yandel, E, Yang, G, Yang, K, Yang, S, Yang, T, Yankelevich, A, Yershov, N, Yonehara, K, Young, T, Yu, B, Yu, H, Yu, J, Yuan, W, Zaki, R, Zalesak, J, Zambelli, L, Zamorano, B, Zani, A, Zazueta, L, Zeit, G, Zeller, G, Zennamo, J, Zeug, K, Zhang, C, Zhao, M, Zhivun, E, Zhu, G, Zilberman, P, Zimmerman, E, Zito, M, Zucchelli, S, Zuklin, J, Zutshi, V, Zwaska, R, and The DUNE Collaboration
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Physics - Instrumentation and Detectors ,Physics::Instrumentation and Detectors ,Physics beyond the Standard Model ,far detector ,QC770-798 ,7. Clean energy ,01 natural sciences ,High Energy Physics - Experiment ,design [detector] ,Near detector ,High Energy Physics - Experiment (hep-ex) ,neutrino ,Conceptual design ,[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex] ,antimatter ,Detectors and Experimental Techniques ,Instrumentation ,physics.ins-det ,QC ,media_common ,QB ,Physics ,new physics ,Neutrino oscillations ,Detector ,Instrumentation and Detectors (physics.ins-det) ,oscillation ,Antimatter ,beam ,Neutrino ,Particle Physics - Experiment ,performance ,Neutrino oscillation ,530 Physics ,Deep Underground Neutrino Experiment ,DUNE ,media_common.quotation_subject ,QC1-999 ,FOS: Physical sciences ,interaction ,near detector ,Nuclear and particle physics. Atomic energy. Radioactivity ,0103 physical sciences ,supernova ,[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det] ,010306 general physics ,detector: design ,activity report ,neutrino oscillations ,010308 nuclear & particles physics ,hep-ex ,Astronomy ,Universe ,High Energy Physics::Experiment - Abstract
FERMILAB-PUB-21-067-E-LBNF-PPD-SCD-T This document was prepared by the DUNE collaboration using the resources of the Fermi National Accelerator Laboratory (Fermilab), a U.S. Department of Energy, Office of Science, HEP User Facility. Fermilab is managed by Fermi Research Alliance, LLC (FRA), acting under Contract No. DE-AC02-07CH11359. This work was supported by CNPq, FAPERJ, FAPEG and FAPESP, Brazil; CFI, IPP and NSERC, Canada; CERN; MŠMT, Czech Republic; ERDF, H2020-EU and MSCA, European Union; CNRS/IN2P3 and CEA, France; INFN, Italy; FCT, Portugal; NRF, South Korea; CAM, Fundación “La Caixa”, MICINN, GVA, Xunta de Galicia and AEI, Spain; SERI and SNSF, Switzerland; TÜBİTAK, Turkey; The Royal Society and UKRI/STFC, United Kingdom; DOE and NSF, United States of America. This research used resources of the National Energy Research Scientific Computing Center (NERSC), a U.S. Department of Energy Office of Science User Facility operated under Contract No. DE-AC02-05CH11231., This work was supported by CNPq, FAPERJ, FAPEG and FAPESP, Brazil; CFI, IPP and NSERC, Canada; CERN; MŠMT, Czech Republic; ERDF, H2020-EU and MSCA, European Union; CNRS/IN2P3 and CEA, France; INFN, Italy; FCT, Portugal; NRF, South Korea; CAM, Fundación “La Caixa”, MICINN, GVA, Xunta de Galicia and AEI, Spain; SERI and SNSF, Switzerland; TÜBİTAK, Turkey; The Royal Society and UKRI/STFC, United Kingdom; DOE and NSF, United States of America., The Deep Underground Neutrino Experiment (DUNE) is an international, world-class experiment aimed at exploring fundamental questions about the universe that are at the forefront of astrophysics and particle physics research. DUNE will study questions pertaining to the preponderance of matter over antimatter in the early universe, the dynamics of supernovae, the subtleties of neutrino interaction physics, and a number of beyond the Standard Model topics accessible in a powerful neutrino beam. A critical component of the DUNE physics program involves the study of changes in a powerful beam of neutrinos, i.e., neutrino oscillations, as the neutrinos propagate a long distance. The experiment consists of a near detector, sited close to the source of the beam, and a far detector, sited along the beam at a large distance. This document, the DUNE Near Detector Conceptual Design Report (CDR), describes the design of the DUNE near detector and the science program that drives the design and technology choices. The goals and requirements underlying the design, along with projected performance are given. It serves as a starting point for a more detailed design that will be described in future documents., Fermi Research Alliance, LLC DE-AC02-07CH11359, H2020-EU, TÜBİTAK, National Science Foundation, U.S. Department of Energy DE-AC02-05CH11231, Multiple Sclerosis Center of Atlanta, CERN, UK Research and Innovation, Natural Sciences and Engineering Research Council of Canada, Science and Technology Facilities Council, Royal Society, European Commission, Singapore Eye Research Institute, Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung, Fundação de Amparo à Pesquisa do Estado de São Paulo, Ministerstvo Školství, Mládeže a Tělovýchovy, Fundação para a Ciência e a Tecnologia, Generalitat Valenciana, Conselho Nacional de Desenvolvimento Científico e Tecnológico, National Research Foundation of Korea, Instituto Nazionale di Fisica Nucleare, Fundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de Janeiro, Centre National de la Recherche Scientifique, Ministerio de Ciencia e Innovación, Fundação de Amparo à Pesquisa do Estado de Goiás, Commissariat à l'Énergie Atomique et aux Énergies Alternatives, European Regional Development Fund, Xunta de Galicia, Agencia Estatal de Investigación, Institut National de Physique Nucléaire et de Physique des Particules
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- 2021
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16. Technical Proposal: FASERnu
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FASER Collaboration, Abreu, Henso, Andreini, Marco, Antel, Claire, Ariga, Akitaka, Ariga, Tomoko, Bertone, Caterina, Boyd, Jamie, Buckley, Andy, Cadoux, Franck, Casper, David W., Cerutti, Francesco, Chen, Xin, Coccaro, Andrea, Danzeca, Salvatore, Dougherty, Liam, Dozen, Candan, Denton, Peter B., Favre, Yannick, Fellers, Deion, Feng, Jonathan L., Ferrere, Didier, Gall, Jonathan, Galon, Iftah, Gibson, Stephen, Gonzalez-Sevilla, Sergio, Hsu, Shih-Chieh, Hu, Zhen, Iacobucci, Giuseppe, Jakobsen, Sune, Jansky, Roland, Kajomovitz, Enrique, Kling, Felix, Kose, Umut, Kuehn, Susanne, Lamont, Mike, Lefebvre, Helena, Levinson, Lorne, Li, Ke, McFayden, Josh, Meehan, Sam, Mladenov, Dimitar, Nakamura, Mitsuhiro, Nakano, Toshiyuki, Nessi, Marzio, Neuhaus, Friedemann, Osborne, John, Otono, Hidetoshi, Pelletier, Serge, Petersen, Brian, Pietropaolo, Francesco, Queitsch-Maitland, Michaela, Resnati, Filippo, Sabate-Gilarte, Marta, Salfeld-Nebgen, Jakob, Galan, Francisco Sanchez, Diaz, Pablo Santos, Sato, Osamu, Scampoli, Paola, Schmieden, Kristof, Schott, Matthias, Schulz, Holger, Sfyrla, Anna, Shively, Savannah, Smolinsky, Jordan, Soffa, Aaron M., Takubo, Yosuke, Torrence, Eric, Trojanowski, Sebastian, Tufanli, Serhan, Zhang, Dengfeng, and Zhang, Gang
- Subjects
High Energy Physics - Experiment (hep-ex) ,High Energy Physics - Phenomenology ,High Energy Physics - Phenomenology (hep-ph) ,Physics - Instrumentation and Detectors ,Physics::Instrumentation and Detectors ,FOS: Physical sciences ,High Energy Physics::Experiment ,Instrumentation and Detectors (physics.ins-det) ,Detectors and Experimental Techniques ,Particle Physics - Experiment ,Particle Physics - Phenomenology ,High Energy Physics - Experiment - Abstract
FASERnu is a proposed small and inexpensive emulsion detector designed to detect collider neutrinos for the first time and study their properties. FASERnu will be located directly in front of FASER, 480 m from the ATLAS interaction point along the beam collision axis in the unused service tunnel TI12. From 2021-23 during Run 3 of the 14 TeV LHC, roughly 1,300 electron neutrinos, 20,000 muon neutrinos, and 20 tau neutrinos will interact in FASERnu with TeV-scale energies. With the ability to observe these interactions, reconstruct their energies, and distinguish flavors, FASERnu will probe the production, propagation, and interactions of neutrinos at the highest human-made energies ever recorded. The FASERnu detector will be composed of 1000 emulsion layers interleaved with tungsten plates. The total volume of the emulsion and tungsten is 25cm x 25cm x 1.35m, and the tungsten target mass is 1.2 tonnes. From 2021-23, 7 sets of emulsion layers will be installed, with replacement roughly every 20-50 1/fb in planned Technical Stops. In this document, we summarize FASERnu's physics goals and discuss the estimates of neutrino flux and interaction rates. We then describe the FASERnu detector in detail, including plans for assembly, transport, installation, and emulsion replacement, and procedures for emulsion readout and analyzing the data. We close with cost estimates for the detector components and infrastructure work and a timeline for the experiment., 49 pages, 25 figures; submitted to the CERN LHCC on 28 October 2019
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- 2020
17. Deep Underground Neutrino Experiment (DUNE), Far Detector Technical Design Report, Volume I Introduction to DUNE
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Abi, Babak, Acciarri, Roberto, Acero, Mario, Adamov, Giorge, Adams, David, Adinolfi, Marco, Ahmad, Zubayer, Ahmed, Jhanzeb, Alion, Tyler, Alonso Monsalve, Saul, Alt, Christoph, Anderson, John, Andreopoulos, Costas, Andrews, Michael P, Andriamirado, Manoa, Andrianala, Fenompanirina, Andringa, Sofia, Ankowski, Artur, Anthony, Jack, Antoniu, Iliescu, Antonova, Maria, Antusch, Stefan, Aranda Fernandez, Alfredo, Ariga, Akitaka, Arnold, Lukas, Arroyave, Manuel, Asaadi, Jonathan, Aurisano, Adam, Aushev, Vladimir, Autiero, Dario, Azfar, Farrukh, Back, Ashley, Back, Henning, Back, John, Backhouse, Chris, Baesso, Paolo, Bagby, Linda, Bajou, Raphael, Balasubramanian, Supraja, Baldi, Pierre, Bambah, Bindu, Barao, Fernando, Barenboim, Gabriela, Barker, Gary J, Barkhouse, Wayne, Barnes, Christopher, Barr, Giles, Barranco Monarca, Juan, Barros, Nuno, Barrow, Joshua, Bashyal, Amit, Basque, Vincent, Bay, Fatih, Bazo Alba, J.L., Beacom, John, Bechetoille, Edouard, Behera, Biswaranjan, Bellantoni, Leo, Bellettini, Giorgio, Bellini, Vincenzo, Beltramello, Olga, Belver, D., Benekos, Nektarios, Bento Neves, Francisco, Berger, Joshua, Berkman, Sophie, Bernardini, Paolo, Berner, Roman, Berns, Hans-Gerd, Bertolucci, Sergio, Betancourt, Minerba, Bezawada, Y., Bhattacharjee, maharnab, Bhuyan, Bipul, Biagi, Simone, Bian, Jianming, Biassoni, Matteo, Biery, Kurt, Bilki, Burak, Bishai, Mary, Bitadze, Alexander, Blake, Andrew, Blanco Siffert, Beatriz, Blaszczyk, Flor de Maria, Blazey, Gerald C, Blucher, Edward, Boissevain, Jan, Bolognesi, Sara, Bolton, Timothy, Bonesini, Maurizio, Bongrand, Mathieu, Bonini, Filiberto, Booth, Alexander, Booth, Chris, Bordoni, Stefania, Borkum, Aran, Boschi, Tommaso, Bostan, Nilay, Bour, Petr, Boyd, Steve B, Boyden, Daniel, Bracinik, Juraj, Braga, Davide, Brailsford, Dominic, Brandt, Andrew, Bremer, Johan, Brew, Chris, Brianne, Eldwan, Brice, Stephen, Brizzolari, Claudia, Bromberg, Carl, Brooijmans, Gustaaf, Brooke, Jim, Bross, Alan, Brunetti, Giulia, Buchanan, Norman, Budd, Howard, Caiulo, Davide, Calafiura, Paolo, Calcutt, Jacob, Calin, Marius, Calvez, Steven, Calvo, Enrique, Camilleri, Leslie, Caminata, Alessio, Campanelli, Mario, Caratelli, David, Carini, Gabriella, Carlus, Bruno, Carniti, Paolo, Caro Terrazas, Ivan, Carranza, Hector, Castillo, Andrés, Castromonte, Cesar, Cattadori, Carla, Cavalier, Fabien, Cavanna, Flavio, Centro, Sandro, Cerati, Giuseppe, Cervelli, Alberto, Cervera Villanueva, Anselmo, Chalifour, Michel, Chang, C., Chardonnet, Etienne, Chatterjee, Animesh, Chattopadhyay, Subhasish, Chaves, Jorge, Chen, Hucheng, Chen, Mu-Chun, Chen, Yifan, Cherdack, Daniel, Chi, Cheng-Yi, Childress, Sam, Chiriacescu, Ana, Cho, Kihyeon, Choubey, Sandhya, Christensen, Anne, Christian, David, Christodoulou, Georgios, Church, Eric, Clarke, Peter, Coan, Thomas, Cocco, Alfredo, Coelho, Joao, Conley, Erin, Conrad, Janet M, Convery, Mark, Corwin, Luke, Cotte, Philippe, Cremaldi, Lucien, Cremonesi, Linda, Crespo-Anadón, Jose I, Cristaldo, Esteban, Cross, Ryan, Cuesta, Clara, Cui, Yanou, Cussans, David, Dabrowski, Mieczyslaw, Da Motta, Helio, Peres, L. Da Silva, David, Quentin, Davies, Gavin, Davini, Stefano, Dawson, Jaime, De, Kaushik, de Almeida, Rogerio, Debbins, Paul, De Bonis, Isabelle, Decowski, M Patrick, de Gouvea, Andre, de Holanda, Pedro, de Icaza Astiz, Iker, Deisting, Alexander, De Jong, Paul, Delbart, Alain, Delepine, David, Delgado, Maritza, Dell'Acqua, Andrea, De Lurgio, Patrick, Ewart, Kevin, Grant, Nick, Hernandez Morquecho, Miguel Angel, Hewes, Jeremy, Huang, Junting, Huang, Junying, Leigui de Oliveira, M A, Li, Shaorui, Li, Shirley W, Ramirez Delgado, Manuel Alejandro, Singh, Jaydip, Singh, Jyotsna, Smith, Adryanna, Smith, Andrew, Todd, Jacob, Torres de Mello Neto, Joao, DeMuth, David, Dennis, Steve, Densham, Chris, Gregor Recalde, Derlis, De Roeck, Albert, De Romeri, Valentina, Jan De Vries, Joris, Dharmapalan, Ranjan, Diaz, Felix, Diaz, Jorge S, Di Domizio, Sergio, Di Giulio, Letizia, Ding, Pengfei, Di Noto, Lea, Distefano, Carla, Diurba, Richard, Diwan, Milind, Djurcic, Zelimir, Dokania, Neha, Dolinski, Michelle 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Kasai, Seiji, Kasetti, Siva, Kashur, Lane, Kazaryan, Narine, Kearns, Edward, Keener, Paul, Kelly, Kevin, Kemp, Ernesto, Ketchum, Wes, Kettell, Steve H, Khabibullin, Marat, Khotjantsev, Alexei, Khvedelidze, Arsen, Kim, D., King, Bonnie, Kirby, Brian, Kirby, Mike, Klein, Joshua, Koehler, Kevin, Koerner, Lisa, Kohn, Sam, Koller, Patrick, Kordosky, Mike, Kosc, Thomas, Kose, Umut, Kostelecky, V Alan, Kothekar, Kunal, Krennrich, Frank, Kreslo, Igor, Kudenko, Yury, Kudryavtsev, Vitaly A, Kulagin, Sergey, Kumar, Jason, KUMAR, Rajeev, Kuruppu, Chatura, Kus, Vaclav, Kutter, Thomas, Lambert, A., Lande, Kenneth, Lane, Charles, Lang, Karol, Langford, Thomas, Lasorak, Pierre, Last, David, Lastoria, Chiara, Laundrie, Andy, Lawrence, A., Lazanu, Ionel, LaZur, Ryan, Le, Trung, Learned, John, LeBrun, Patrice, Lehmann Miotto, Giovanna, Lehnert, Ralf, Leitner, M., Leyton, Michael, Li, Lingge, Li, Teng, Li, Yichen, Liao, Heng-Ye, Lin, Cheng-Ju Stephen, Lin, Shih-Kai, Lister, Adam, Littlejohn, Bryce, Liu, J., Lockwitz, Sarah, Loew, Timothy, Lokajicek, Milos, Lomidze, Irakli, Long, Ken, Loo, Kai, Lorca, David, Lord, Tom, LoSecco, John M, Louis, William, Luk, Kam-Biu, Luo, Xiao, Lurkin, Nicolas, Lux, Thorsten, Luzio, Vitor Prestes, MacFarlane, David, Machado, Ana Amelia, Machado, Pedro, Macias, Christopher Thomas, Macier, Jolie R, Maddalena, Antonello, Madigan, Peter, Magill, Steve, Mahn, Kendall, Maio, Amélia, Maloney, James, Mandrioli, Gianni, Maneira, José, Manenti, Laura, Manly, Steve, Mann, Anthony, Manolopoulos, Konstantinos, Manrique Plata, Maria, Marchionni, Alberto, Marciano, William, Marfatia, Danny, Mariani, Camillo, Maricic, Jelena, Marinho, Franciole, Marino, Alysia, Marshak, Marvin, Marshall, Chris, Marshall, John, Marteau, Jacques, Martin-Albo, Justo, Martinez, Norman, Martinez Caicedo, David, Martynenko, Sergey, Mason, Katie, Mastbaum, Andrew, Masud, Mehedi, Matsuno, Shigenobu, Matthews, James, Mauger, Christopher, Mauri, Nicoletta, Mavrokoridis, Konstantinos, Mazza, Roberto, Mazzacane, Anna, Mazzucato, Edoardo, McCluskey, Elaine, McConkey, Nicola, McFarland, Kevin, McGrew, Clark, McNab, Andrew, Mefodiev, Alexander, Mehta, Poonam, Melas, Pantelis, Mellinato, Michele, Mena, Olga, Menary, Scott, Mendes Santos, Lucas, Mendez, Hector, Menegolli, A, Meng, Guang, Messier, Mark, Metcalf, William, Mewes, Matthew, Meyer, Holger, Miao, Ting, Michna, Gregory, Miedema, Thijs, Migenda, Jost, Milincic, Radovan, Miller, William, Mills, Joshua, Milne, Cody, Mineev, Oleg, Miranda, Omar, Miryala, Sandeep, Mishra, C Shekhar, Mishra, Sanjib R, Mislivec, Aaron, Mladenov, Dimitar, Mocioiu, Irina, Moffat, Kristian, Moggi, Niccolo, Mohanta, Rukmani, Mohayai, Tanaz, Mokhov, Nikolai, Molina, Jorge, Molina Bueno, Laura, Montanari, Alessandro, Montanari, Claudio, Montanari, David, Montano Zetina, Luis, Moon, Jarrett, Mooney, Michael, Moreno, Deywis, Morgan, Ben, Morris, Casandra, Mossey, Chris, Motuk, Erdem, Moura, Célio, Mousseau, Joel, Mu, Wei, Mualem, Leon, Mueller, Justin, Muether, Mathew, Mufson, Stuart, Muheim, Franz, Muir, Alan, Mulhearn, Mike, Muramatsu, Hajime, Murphy, Sebastien, Musser, Jim, Nachtman, Jane, Nagu, S., Nalbandyan, Mikayel, Nandakumar, Raja, Naples, Donna, Narita, Shinya, Navas-Nicolas, D., Nayak, Nitish, Nebot-Guinot, Miquel, Necib, Lina, Negishi, Kentaro, Nelson, Jeff, Nesbit, Jake, Nessi, Marzio, Newbold, David, Newcomer, Mitch, Newhart, Duane, Nichol, Ryan, Niner, Evan, Nishimura, Kurtis, Norman, Andrew, Northrop, Rich, Novella, Pau, Nowak, Jaroslaw, Oberling, Michael, Olivares Del Campo, Andres, Olivier, Andrew, Onel, Yasar, Onishchuk, Yuriy, Ott, Jordan, Pagani, Luca, Pakvasa, Sandip, Palamara, Ornella, Palestini, Sandro, Paley, Jonathan, Pallavicini, Marco, Palomares, Carmen, Pantic, Emilija, Paolone, Vittorio, Papadimitriou, Vaia, Papaleo, Riccardo, Papanestis, Antonis, Paramesvaran, Sudarshan, Parke, Stephen, Parsa, Zohreh, Parvu, Mihaela, Pascoli, Silvia, Pasqualini, Laura, Pasternak, Jaroslaw, Pater, Joleen, Patrick, Cheryl, Patrizii, Laura, Patterson, Ryan, Patton, Simon John, Patzak, Thomas, Paudel, Ajib, Paulos, Bob, Paulucci, Laura, Pavlovic, Zarko, Pawloski, Greg, Payne, David, Pec, Viktor, Peeters, Simon, Penichot, Yves, Pennacchio, Elisabetta, Penzo, Aldo, Peres, Orlando, Perry, James, Pershey, Daniel, Pessina, Gianluigi, Petrillo, Gianluca, Petta, Catia, Petti, Roberto, Piastra, Francesco, Pickering, Luke, Pietropaolo, Francesco, Pillow, James, Plunkett, Robert, Poling, Ronald, Pons, Xavier, Poonthottathil, Navaneeth, Pordes, Stephen, Potekhin, Maxim, Potenza, Renato, Potukuchi, B.V.K.S., Pozimski, Juergen, Pozzato, Michele, Prakash, Suprabh, Prakash, Tarun, Prince, Sebastien, Pugnere, Denis, Qi, K., Qian, Xin, Raaf, Jennifer L, Raboanary, R., Radeka, Veljko, Rademacker, Jonas, Radics, Balint, Rafique, Aleena, Raguzin, Eric, Rai, Mousam, Rajaoalisoa, Miriama, Rakhno, Igor, Rakotondramanana, H.T., Rakotondravohitra, Laza, Ramachers, Yorck A, Rameika, Regina, Ramson, Bryan, Rappoldi, A, Raselli, GL, Ratoff, Peter, Ravat, Sylvain, Razafinime, H., Real, Jean-Sebastien, Rebel, Brian, Redondo, David, Reggiani-Guzzo, Marina, Rehak, Tyler, Reichenbacher, Juergen, Reitzner, S, Renshaw, Andrew, Rescia, Sergio, Resnati, Filippo, Reynolds, Aidan, Riccobene, Giorgio, Rice, Logan, Rielage, Keith, Rigaut, Yann-Axel, Rivera, David, Rochester, Leon, Roda, Marco, Rodrigues, Philip, Rodriguez Alonso, Manual Jesus, Rodriguez Rondon, Jairo, Roeth, Alison J, Rogers, Hannah, Rosauro-Alcaraz, Salvador, Rossella, M, Rout, Jogesh, Roy, Samiran, Rubbia, Andre, Rubbia, Carlo, Russell, Brooke, Russell, James, Ruterbories, Daniel, Saakyan, Ruben, Sacerdoti, Sabrina, Safford, Twymun, Sahu, Narendra, Sala, Paola, Samios, Nicholas, Sanchez, Mayly, Sanders, David, Sankey, David, Santana, Samuel, Santos-Maldonado, Marvin, Saoulidou, Niki, Sapienza, Piera, Sarasty, Carlos, Sarcevic, Ina, Savage, Geoffrey, Savinov, Vladimir, Scaramelli, Alberto, Scarff, Andrew, Scarpelli, Andrea, Schaffer, Tom, Schellman, Heidi, Schlabach, Philip, Schmitz, David, Scholberg, Kate, Schukraft, Anne, Segreto, Ettore, Sensenig, Jon, Seong, Ilsoo, Sergi, Antonino, Sergiampietri, F., Sgalaberna, Davide, Shaevitz, Michael H, Shafaq, Sheeba, Shamma, M., Sharma, Hans, Sharma, Rahul, Shaw, Terri, Shepherd-Themistocleous, Claire, Shin, Seodong, Shooltz, Dean, Shrock, Robert, Simard, Laurent, Simos, Nikolaos, Sinclair, James, Sinev, Gleb, Sipos, Roland, Sippach, F W, Sirri, Gabriele, Sitraka, Andriaseta, Siyeon, Kim, Smargianaki, D., Smith, Erica, Smith, Paul, Smolik, Jan, Smy, Michael, Snopok, Pavel, Soares Nunes, Mônica, Sobel, Henry, Soderberg, Mitch, Solano Salinas, Carlos, Söldner-Rembold, Stefan, Solomey, Nicholas, Solovov, Vladimir, Sondheim, Walter, Sorel, Michel, Soto-Oton, Jose, Sousa, Alexandre, Soustruznik, Karel, Spagliardi, Fabio, Spanu, Maura, Spitz, Joshua, Spooner, Neil JC, Spurgeon, Kyle, Staley, Richard, Stancari, Michelle, Stanco, Luca, Steiner, Herbert M, Stewart, James, Stillwell, Ben, Stock, Jason, Stocker, Francesca, Stokes, Tyler, Strait, Matthew, Strauss, Thomas, Striganov, Sergei, Stuart, Alexander, Summers, Don, Surdo, Antonio, Susic, Vasja, Suter, Louise, Sutera, Concetta Maria, Svoboda, Robert, Szczerbinska, Barbara, Szelc, Andrzej, Talaga, Richard, Tanaka, Hirohisa, Tapia Oregui, Beatriz, Tapper, Alexander, Tariq, Salman, Tatar, E., Tayloe, Rex, Teklu, Abraham Meles, Tenti, Matteo, Terao, Kazuhiro, Ternes, Christoph, Terranova, Francesco, Testera, Gemma, Thea, Alessandro, Thompson, Joshua, Thorn, Craig, Timm, Steven C, Tonazzo, Alessandra, Torti, Marta, Tortola, Mariam, Tortorici, Francesco, Totani, Dante, Toups, Matthew, Touramanis, Christos, Trevor, Jason, Trzaska, Wladyslaw, Tsai, Yun-Tse, Tsamalaidze, Zviadi, Tsang, Ka Vang, Tsverava, Nikolozi, Tufanli, Serhan, Tull, Craig, Tyley, E., Tzanov, Martin, Uchida, Melissa, Urheim, Jon, Usher, Tracy, Vagins, Mark R, Vahle, Patricia, Valdiviesso, Gustavo, Valencia, E., Vallari, Zoya, Valle, Jose, Vallecorsa, Sofia, Van Berg, Rick, Van de Water, Richard, Vanegas Forero, David, Varanini, Filippo, Vargas, Danaisis, Varner, Gary, Vasel, Justin, Vasseur, Georges, Vaziri, Kamran, Ventura, Sandro, Verdugo, Antonio, Vergani, Stefano, Vermeulen, Milo, Verzocchi, Marco, Vieira de Souza, Henrique, Vignoli, Chiara, Vilela, Cristovao, Viren, Brett, Vrba, Tomas, Wachala, Tomasz, Waldron, Abigail, Wallbank, Michael, Wang, Hanguo, Wang, Jingbo, Wang, Yi, Wang, Yue, Warburton, Karl, Warner, David, Wascko, Morgan, Waters, David, Watson, Alan, Weatherly, Pierce, Weber, Alfons, Weber, Michele, Wei, Hanyu, Weinstein, Amanda, Wenman, Dan, Wetstein, Matthew, Yang, Shaokai, Zeller, Geralyn (Sam), While, M.R., White, Andy, Whitehead, Leigh, Whittington, Denver, Wilking, Michael, Wilkinson, Callum, Williams, Zachary, Wilson, Fergus, Wilson, Robert, Wolcott, Jeremy, Wongjirad, Taritree, Wood, Kevin, Wood, Lynn, Worcester, Elizabeth, Worcester, Matthew, Wret, Clarence, Wu, Wanwei, Xiao, Y., Yang, Guang, Yang, Tingjun, Yershov, Nikolai, Yonehara, Katsuya, Young, Tim, Yu, Bo, Yu, Jae, Zalesak, Jaroslav, Zambelli, Laura, Zamorano, Bruno, Zani, Andrea, Zazueta, Luis, Zeller, G.P., Zennamo, Joseph, Zeug, Kyle, Zhang, Chao, Zhao, Manhong, Zhivun, Elena, Zhu, Guanying, Zimmerman, Eric, Zito, Marco, Zucchelli, Stefano, Zuklin, Josef, Zutshi, Vishnu, Zwaska, Robert, Institut de Physique des 2 Infinis de Lyon (IP2I Lyon), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Centre National de la Recherche Scientifique (CNRS), AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), 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 l'Accélérateur Linéaire (LAL), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), 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 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), DUNE, 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), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), and Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)
- Subjects
detector: technology ,Physics - Instrumentation and Detectors ,hep-ex ,Physics::Instrumentation and Detectors ,far detector ,FOS: Physical sciences ,Instrumentation and Detectors (physics.ins-det) ,time projection chamber: liquid argon ,High Energy Physics - Experiment ,High Energy Physics - Experiment (hep-ex) ,neutrino: deep underground detector ,near detector ,[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex] ,High Energy Physics::Experiment ,data management ,[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det] ,Detectors and Experimental Techniques ,physics.ins-det ,Particle Physics - Experiment ,activity report ,detector: design - Abstract
The preponderance of matter over antimatter in the early universe, the dynamics of the supernovae that produced the heavy elements necessary for life, and whether protons eventually decay -- these mysteries at the forefront of particle physics and astrophysics are key to understanding the early evolution of our universe, its current state, and its eventual fate. The Deep Underground Neutrino Experiment (DUNE) is an international world-class experiment dedicated to addressing these questions as it searches for leptonic charge-parity symmetry violation, stands ready to capture supernova neutrino bursts, and seeks to observe nucleon decay as a signature of a grand unified theory underlying the standard model. The DUNE far detector technical design report (TDR) describes the DUNE physics program and the technical designs of the single- and dual-phase DUNE liquid argon TPC far detector modules. This TDR is intended to justify the technical choices for the far detector that flow down from the high-level physics goals through requirements at all levels of the Project. Volume I contains an executive summary that introduces the DUNE science program, the far detector and the strategy for its modular designs, and the organization and management of the Project. The remainder of Volume I provides more detail on the science program that drives the choice of detector technologies and on the technologies themselves. It also introduces the designs for the DUNE near detector and the DUNE computing model, for which DUNE is planning design reports. Volume II of this TDR describes DUNE's physics program in detail. Volume III describes the technical coordination required for the far detector design, construction, installation, and integration, and its organizational structure. Volume IV describes the single-phase far detector technology. A planned Volume V will describe the dual-phase technology., Comment: Minor corrections made for JINST submission; 244 pages, 114 figures
- Published
- 2020
18. Deep Underground Neutrino Experiment (DUNE), Far Detector Technical Design Report, Volume III: DUNE Far Detector Technical Coordination
- Author
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Abi, Babak, Acciarri, Roberto, Acero, Mario, Adamov, Giorge, Adams, David, Adinolfi, Marco, Ahmad, Zubayer, Ahmed, Jhanzeb, Alion, Tyler, Alonso Monsalve, Saul, Alt, Christoph, Anderson, John, Andreopoulos, Costas, Andrews, Michael P, Andriamirado, Manoa, Andrianala, Fenompanirina, Andringa, Sofia, Ankowski, Artur, Anthony, Jack, Antoniu, Iliescu, Antonova, Maria, Antusch, Stefan, Aranda Fernandez, Alfredo, Ariga, Akitaka, Arnold, Lukas, Arroyave, Manuel, Asaadi, Jonathan, Aurisano, Adam, Aushev, Vladimir, Autiero, Dario, Azfar, Farrukh, Back, Ashley, Back, Henning, Back, John, Backhouse, Chris, Baesso, Paolo, Bagby, Linda, Bajou, Raphael, Balasubramanian, Supraja, Baldi, Pierre, Bambah, Bindu, Barao, Fernando, Barenboim, Gabriela, Barker, Gary J, Barkhouse, Wayne, Barnes, Christopher, Barr, Giles, Barranco Monarca, Juan, Barros, Nuno, Barrow, Joshua, Bashyal, Amit, Basque, Vincent, Bay, Fatih, Bazo Alba, J.L., Beacom, John, Bechetoille, Edouard, Behera, Biswaranjan, Bellantoni, Leo, Bellettini, Giorgio, Bellini, Vincenzo, Beltramello, Olga, Belver, D., Benekos, Nektarios, Bento Neves, Francisco, Berger, Joshua, Berkman, Sophie, Bernardini, Paolo, Berner, Roman, Berns, Hans-Gerd, Bertolucci, Sergio, Betancourt, Minerba, Bezawada, Y., Bhattacharjee, maharnab, Bhuyan, Bipul, Biagi, Simone, Bian, Jianming, Biassoni, Matteo, Biery, Kurt, Bilki, Burak, Bishai, Mary, Bitadze, Alexander, Blake, Andrew, Blanco Siffert, Beatriz, Blaszczyk, Flor de Maria, Blazey, Gerald C, Blucher, Edward, Boissevain, Jan, Bolognesi, Sara, Bolton, Timothy, Bonesini, Maurizio, Bongrand, Mathieu, Bonini, Filiberto, Booth, Alexander, Booth, Chris, Bordoni, Stefania, Borkum, Aran, Boschi, Tommaso, Bostan, Nilay, Bour, Petr, Boyd, Steve B, Boyden, Daniel, Bracinik, Juraj, Braga, Davide, Brailsford, Dominic, Brandt, Andrew, Bremer, Johan, Brew, Chris, Brianne, Eldwan, Brice, Stephen, Brizzolari, Claudia, Bromberg, Carl, Brooijmans, Gustaaf, Brooke, Jim, Bross, Alan, Brunetti, Giulia, Buchanan, Norman, Budd, Howard, Caiulo, Davide, Calafiura, Paolo, Calcutt, Jacob, Calin, Marius, Calvez, Steven, Calvo, Enrique, Camilleri, Leslie, Caminata, Alessio, Campanelli, Mario, Caratelli, David, Carini, Gabriella, Carlus, Bruno, Carniti, Paolo, Caro Terrazas, Ivan, Carranza, Hector, Castillo, Andrés, Castromonte, Cesar, Cattadori, Carla, Cavalier, Fabien, Cavanna, Flavio, Centro, Sandro, Cerati, Giuseppe, Cervelli, Alberto, Cervera Villanueva, Anselmo, Chalifour, Michel, Chang, C., Chardonnet, Etienne, Chatterjee, Animesh, Chattopadhyay, Subhasish, Chaves, Jorge, Chen, Hucheng, Chen, Mu-Chun, Chen, Yifan, Cherdack, Daniel, Chi, Cheng-Yi, Childress, Sam, Chiriacescu, Ana, Cho, Kihyeon, Choubey, Sandhya, Christensen, Anne, Christian, David, Christodoulou, Georgios, Church, Eric, Clarke, Peter, Coan, Thomas, Cocco, Alfredo, Coelho, Joao, Conley, Erin, Conrad, Janet M, Convery, Mark, Corwin, Luke, Cotte, Philippe, Cremaldi, Lucien, Cremonesi, Linda, Crespo-Anadón, Jose I, Cristaldo, Esteban, Cross, Ryan, Cuesta, Clara, Cui, Yanou, Cussans, David, Dabrowski, Mieczyslaw, Da Motta, Helio, Peres, L. Da Silva, David, Quentin, Davies, Gavin, Davini, Stefano, Dawson, Jaime, De, Kaushik, de Almeida, Rogerio, Debbins, Paul, De Bonis, Isabelle, Decowski, M Patrick, de Gouvea, Andre, de Holanda, Pedro, de Icaza Astiz, Iker, Deisting, Alexander, De Jong, Paul, Delbart, Alain, Delepine, David, Delgado, Maritza, Dell'Acqua, Andrea, De Lurgio, Patrick, Ewart, Kevin, Grant, Nick, Hernandez Morquecho, Miguel Angel, Hewes, Jeremy, Huang, Junting, Huang, Junying, Leigui de Oliveira, M A, Li, Shaorui, Li, Shirley W, Ramirez Delgado, Manuel Alejandro, Singh, Jaydip, Singh, Jyotsna, Smith, Adryanna, Smith, Andrew, Todd, Jacob, Torres de Mello Neto, Joao, DeMuth, David, Dennis, Steve, Densham, Chris, Gregor Recalde, Derlis, De Roeck, Albert, De Romeri, Valentina, Jan De Vries, Joris, Dharmapalan, Ranjan, Diaz, Felix, Diaz, Jorge S, Di Domizio, Sergio, Di Giulio, Letizia, Ding, Pengfei, Di Noto, Lea, Distefano, Carla, Diurba, Richard, Diwan, Milind, Djurcic, Zelimir, Dokania, Neha, Dolinski, Michelle J, Domine, Laura, Douglas, Daniel, Drielsma, Francois, Duchesneau, Dominique, Duffy, Kirsty, Dunne, Patrick, Durkin, Tim, Duyang, Hongyue, Dvornikov, Olexiy, Dwyer, Daniel A, Dyshkant, Alexandre S, Eads, Michael, Edmunds, Daniel, Eisch, Jonathan, Emery, Sandrine, Ereditato, Antonio, Escobar, Carlos O, Escudero Sanchez, Lorena, Evans, Justin, Ewart, E., Ezeribe, Anthony, Fahey, Kevin, Falcone, Andrea, Farnese, Christian, Farzan, Yasaman, Felix, Julian, Fernandez-Martinez, Enrique, Fernandez Menendez, Pablo, Ferraro, Federico, Fields, Laura, Filkins, A., Filthaut, Frank, Fitzpatrick, Rory, Flanagan, Will, Fleming, Bonnie, Flight, Robert, Fowler, Jack, Fox, Walt, Franc, Jiri, Francis, Kurt, Franco, Domenico, Freeman, John, Freestone, Julian, Fried, Jack, Friedland, Alex, Fuess, Stu, Furic, Ivan, Furmanski, Andrew, Gago, A., Gallagher, Hugh, Gallego-Ros, Ana, Gallice, Niccolo, Galymov, Vyacheslav, Gamberini, Enrico, Gamble, Trevor, Gandhi, Raj, Gandrajula, Reddy, Gao, Shanshan, Garcia-Gamez, Diego, García-Peris, Miguel, Gardiner, Steven, Gastler, Dan, Ge, Guanqun, Gelli, Bruno, Gendotti, Adamo, Gent, Stephen, Ghorbani-Moghaddam, Zahra, Gibin, Daniele, Gil-Botella, Ines, Girerd, Claude, Giri, Anjan Kumar, Gnani, D., Gogota, Olga, Gold, Michael, Gollapinni, Sowjanya, Gollwitzer, Keith, Gomes, Ricardo, Gomez Bermeo, Laura Vanessa, Gomez Fajardo, Luz, Gonnella, Francesco, Gonzalez-Cuevas, Juan Alberto, Goodman, Maury, Goodwin, Owen, Goswami, Srubabati, Gotti, Claudio, Goudzovski, Evgueni, Grace, Carl, Graham, Mathew, Gramellini, E., Gran, Rik, Granados, Everardo, Grant, Alan, Grant, Christopher, Gratieri, Diego, Green, Patrick, Green, Steven, Greenler, Leland, Greenwood, M., Greer, Joel, Griffith, Clark, Groh, Micah, Grudzinski, James, Grzelak, Katarzyna, Gu, Wenqiang, Guarino, Victor, Guenette, Roxanne, Guglielmi, Alberto, Guo, Bing, Guthikonda, K K, Gutierrez, Rafael, Guzowski, Pawel, Guzzo, Marcelo, Gwon, Sunwoo, Habig, Alec, Hackenburg, A., Hadavand, Haleh, Haenni, Roger, Hahn, Alan, Haigh, Jennifer, Haiston, James, Hamernik, Thomas, Hamilton, Philip, Han, Jiyeon, Harder, Kristian, Harris, Debbie, Hartnell, Jeffrey, Hasegawa, Takyua, Hatcher, Robert, Hazen, Eric, Heavey, Anne, Heeger, Karsten, Hennessy, Karol, Henry, Sarah, Herner, Kenneth, Hertel, Lars, Hewes, V., Higuera Pichardo, Aaron, Hill, Tony, Hillier, Stephen, Himmel, Alexander, Hoff, James, Hohl, Christian, Holin, Anna, Hoppe, Eric, Horton-Smith, Glenn, Hostert, Matheus, Hourlier, Adrien, Howard, Bruce, Howell, Ryan, Hugon, Justin, Iles, Gregory, Illingworth, Robert, Ioannisian, Ara, Itay, Ran, Izmaylov, Alexander, James, Eric, Jargowsky, B., Jediny, Filip, Jesús-Valls, César, Ji, Xiangpan, Jiang, L., Jiménez, Sergio, Jipa, Alexandru, Johnson, Connor, Johnson, Randy, Jones, Benjamin, Jones, Sebastian, Jung, Chang Kee, Junk, Thomas, Jwa, Yeon-jae, Kabirnezhad, Monireh, Kaboth, Asher, Kadenko, I, Kamiya, Felipe, Karagiorgi, Georgia, Karcher, A., Karolak, Mark, Karyotakis, Yannis, Kasai, Seiji, Kasetti, Siva, Kashur, Lane, Kazaryan, Narine, Kearns, Edward, Keener, Paul, Kelly, Kevin, Kemp, Ernesto, Ketchum, Wes, Kettell, Steve H, Khabibullin, Marat, Khotjantsev, Alexei, Khvedelidze, Arsen, Kim, D., King, Bonnie, Kirby, Brian, Kirby, Mike, Klein, Joshua, Koehler, Kevin, Koerner, Lisa, Kohn, Sam, Koller, Patrick, Kordosky, Mike, Kosc, Thomas, Kose, Umut, Kostelecky, V Alan, Kothekar, Kunal, Krennrich, Frank, Kreslo, Igor, Kudenko, Yury, Kudryavtsev, Vitaly A, Kulagin, Sergey, Kumar, Jason, KUMAR, Rajeev, Kuruppu, Chatura, Kus, Vaclav, Kutter, Thomas, Lambert, A., Lande, Kenneth, Lane, Charles, Lang, Karol, Langford, Thomas, Lasorak, Pierre, Last, David, Lastoria, Chiara, Laundrie, Andy, Lawrence, A., Lazanu, Ionel, LaZur, Ryan, Le, Trung, Learned, John, LeBrun, Patrice, Lehmann Miotto, Giovanna, Lehnert, Ralf, Leitner, M., Leyton, Michael, Li, Lingge, Li, Teng, Li, Yichen, Liao, Heng-Ye, Lin, Cheng-Ju Stephen, Lin, Shih-Kai, Lister, Adam, Littlejohn, Bryce, Liu, J., Lockwitz, Sarah, Loew, Timothy, Lokajicek, Milos, Lomidze, Irakli, Long, Ken, Loo, Kai, Lorca, David, Lord, Tom, LoSecco, John M, Louis, William, Luk, Kam-Biu, Luo, Xiao, Lurkin, Nicolas, Lux, Thorsten, Luzio, Vitor Prestes, MacFarlane, David, Machado, Ana Amelia, Machado, Pedro, Macias, Christopher Thomas, Macier, Jolie R, Maddalena, Antonello, Madigan, Peter, Magill, Steve, Mahn, Kendall, Maio, Amélia, Maloney, James, Mandrioli, Gianni, Maneira, José, Manenti, Laura, Manly, Steve, Mann, Anthony, Manolopoulos, Konstantinos, Manrique Plata, Maria, Marchionni, Alberto, Marciano, William, Marfatia, Danny, Mariani, Camillo, Maricic, Jelena, Marinho, Franciole, Marino, Alysia, Marshak, Marvin, Marshall, Chris, Marshall, John, Marteau, Jacques, Martin-Albo, Justo, Martinez, Norman, Martinez Caicedo, David, Martynenko, Sergey, Mason, Katie, Mastbaum, Andrew, Masud, Mehedi, Matsuno, Shigenobu, Matthews, James, Mauger, Christopher, Mauri, Nicoletta, Mavrokoridis, Konstantinos, Mazza, Roberto, Mazzacane, Anna, Mazzucato, Edoardo, McCluskey, Elaine, McConkey, Nicola, McFarland, Kevin, McGrew, Clark, McNab, Andrew, Mefodiev, Alexander, Mehta, Poonam, Melas, Pantelis, Mellinato, Michele, Mena, Olga, Menary, Scott, Mendes Santos, Lucas, Mendez, Hector, Menegolli, A, Meng, Guang, Messier, Mark, Metcalf, William, Mewes, Matthew, Meyer, Holger, Miao, Ting, Michna, Gregory, Miedema, Thijs, Migenda, Jost, Milincic, Radovan, Miller, William, Mills, Joshua, Milne, Cody, Mineev, Oleg, Miranda, Omar, Miryala, Sandeep, Mishra, C Shekhar, Mishra, Sanjib R, Mislivec, Aaron, Mladenov, Dimitar, Mocioiu, Irina, Moffat, Kristian, Moggi, Niccolo, Mohanta, Rukmani, Mohayai, Tanaz, Mokhov, Nikolai, Molina, Jorge, Molina Bueno, Laura, Montanari, Alessandro, Montanari, Claudio, Montanari, David, Montano Zetina, Luis, Moon, Jarrett, Mooney, Michael, Moreno, Deywis, Morgan, Ben, Morris, Casandra, Mossey, Chris, Motuk, Erdem, Moura, Célio, Mousseau, Joel, Mu, Wei, Mualem, Leon, Mueller, Justin, Muether, Mathew, Mufson, Stuart, Muheim, Franz, Muir, Alan, Mulhearn, Mike, Muramatsu, Hajime, Murphy, Sebastien, Musser, Jim, Nachtman, Jane, Nagu, S., Nalbandyan, Mikayel, Nandakumar, Raja, Naples, Donna, Narita, Shinya, Navas-Nicolas, D., Nayak, Nitish, Nebot-Guinot, Miquel, Necib, Lina, Negishi, Kentaro, Nelson, Jeff, Nesbit, Jake, Nessi, Marzio, Newbold, David, Newcomer, Mitch, Newhart, Duane, Nichol, Ryan, Niner, Evan, Nishimura, Kurtis, Norman, Andrew, Northrop, Rich, Novella, Pau, Nowak, Jaroslaw, Oberling, Michael, Olivares Del Campo, Andres, Olivier, Andrew, Onel, Yasar, Onishchuk, Yuriy, Ott, Jordan, Pagani, Luca, Pakvasa, Sandip, Palamara, Ornella, Palestini, Sandro, Paley, Jonathan, Pallavicini, Marco, Palomares, Carmen, Pantic, Emilija, Paolone, Vittorio, Papadimitriou, Vaia, Papaleo, Riccardo, Papanestis, Antonis, Paramesvaran, Sudarshan, Parke, Stephen, Parsa, Zohreh, Parvu, Mihaela, Pascoli, Silvia, Pasqualini, Laura, Pasternak, Jaroslaw, Pater, Joleen, Patrick, Cheryl, Patrizii, Laura, Patterson, Ryan, Patton, Simon John, Patzak, Thomas, Paudel, Ajib, Paulos, Bob, Paulucci, Laura, Pavlovic, Zarko, Pawloski, Greg, Payne, David, Pec, Viktor, Peeters, Simon, Penichot, Yves, Pennacchio, Elisabetta, Penzo, Aldo, Peres, Orlando, Perry, James, Pershey, Daniel, Pessina, Gianluigi, Petrillo, Gianluca, Petta, Catia, Petti, Roberto, Piastra, Francesco, Pickering, Luke, Pietropaolo, Francesco, Pillow, James, Plunkett, Robert, Poling, Ronald, Pons, Xavier, Poonthottathil, Navaneeth, Pordes, Stephen, Potekhin, Maxim, Potenza, Renato, Potukuchi, B.V.K.S., Pozimski, Juergen, Pozzato, Michele, Prakash, Suprabh, Prakash, Tarun, Prince, Sebastien, Pugnere, Denis, Qi, K., Qian, Xin, Raaf, Jennifer L, Raboanary, R., Radeka, Veljko, Rademacker, Jonas, Radics, Balint, Rafique, Aleena, Raguzin, Eric, Rai, Mousam, Rajaoalisoa, Miriama, Rakhno, Igor, Rakotondramanana, H.T., Rakotondravohitra, Laza, Ramachers, Yorck A, Rameika, Regina, Ramson, Bryan, Rappoldi, A, Raselli, GL, Ratoff, Peter, Ravat, Sylvain, Razafinime, H., Real, Jean-Sebastien, Rebel, Brian, Redondo, David, Reggiani-Guzzo, Marina, Rehak, Tyler, Reichenbacher, Juergen, Reitzner, S, Renshaw, Andrew, Rescia, Sergio, Resnati, Filippo, Reynolds, Aidan, Riccobene, Giorgio, Rice, Logan, Rielage, Keith, Rigaut, Yann-Axel, Rivera, David, Rochester, Leon, Roda, Marco, Rodrigues, Philip, Rodriguez Alonso, Manual Jesus, Rodriguez Rondon, Jairo, Roeth, Alison J, Rogers, Hannah, Rosauro-Alcaraz, Salvador, Rossella, M, Rout, Jogesh, Roy, Samiran, Rubbia, Andre, Rubbia, Carlo, Russell, Brooke, Russell, James, Ruterbories, Daniel, Saakyan, Ruben, Sacerdoti, Sabrina, Safford, Twymun, Sahu, Narendra, Sala, Paola, Samios, Nicholas, Sanchez, Mayly, Sanders, David, Sankey, David, Santana, Samuel, Santos-Maldonado, Marvin, Saoulidou, Niki, Sapienza, Piera, Sarasty, Carlos, Sarcevic, Ina, Savage, Geoffrey, Savinov, Vladimir, Scaramelli, Alberto, Scarff, Andrew, Scarpelli, Andrea, Schaffer, Tom, Schellman, Heidi, Schlabach, Philip, Schmitz, David, Scholberg, Kate, Schukraft, Anne, Segreto, Ettore, Sensenig, Jon, Seong, Ilsoo, Sergi, Antonino, Sergiampietri, F., Sgalaberna, Davide, Shaevitz, Michael H, Shafaq, Sheeba, Shamma, M., Sharma, Hans, Sharma, Rahul, Shaw, Terri, Shepherd-Themistocleous, Claire, Shin, Seodong, Shooltz, Dean, Shrock, Robert, Simard, Laurent, Simos, Nikolaos, Sinclair, James, Sinev, Gleb, Sipos, Roland, Sippach, F W, Sirri, Gabriele, Sitraka, Andriaseta, Siyeon, Kim, Smargianaki, D., Smith, Erica, Smith, Paul, Smolik, Jan, Smy, Michael, Snopok, Pavel, Soares Nunes, Mônica, Sobel, Henry, Soderberg, Mitch, Solano Salinas, Carlos, Söldner-Rembold, Stefan, Solomey, Nicholas, Solovov, Vladimir, Sondheim, Walter, Sorel, Michel, Soto-Oton, Jose, Sousa, Alexandre, Soustruznik, Karel, Spagliardi, Fabio, Spanu, Maura, Spitz, Joshua, Spooner, Neil JC, Spurgeon, Kyle, Staley, Richard, Stancari, Michelle, Stanco, Luca, Steiner, Herbert M, Stewart, James, Stillwell, Ben, Stock, Jason, Stocker, Francesca, Stokes, Tyler, Strait, Matthew, Strauss, Thomas, Striganov, Sergei, Stuart, Alexander, Summers, Don, Surdo, Antonio, Susic, Vasja, Suter, Louise, Sutera, Concetta Maria, Svoboda, Robert, Szczerbinska, Barbara, Szelc, Andrzej, Talaga, Richard, Tanaka, Hirohisa, Tapia Oregui, Beatriz, Tapper, Alexander, Tariq, Salman, Tatar, E., Tayloe, Rex, Teklu, Abraham Meles, Tenti, Matteo, Terao, Kazuhiro, Ternes, Christoph, Terranova, Francesco, Testera, Gemma, Thea, Alessandro, Thompson, Joshua, Thorn, Craig, Timm, Steven C, Tonazzo, Alessandra, Torti, Marta, Tortola, Mariam, Tortorici, Francesco, Totani, Dante, Toups, Matthew, Touramanis, Christos, Trevor, Jason, Trzaska, Wladyslaw, Tsai, Yun-Tse, Tsamalaidze, Zviadi, Tsang, Ka Vang, Tsverava, Nikolozi, Tufanli, Serhan, Tull, Craig, Tyley, E., Tzanov, Martin, Uchida, Melissa, Urheim, Jon, Usher, Tracy, Vagins, Mark R, Vahle, Patricia, Valdiviesso, Gustavo, Valencia, E., Vallari, Zoya, Valle, Jose, Vallecorsa, Sofia, Van Berg, Rick, Van de Water, Richard, Vanegas Forero, David, Varanini, Filippo, Vargas, Danaisis, Varner, Gary, Vasel, Justin, Vasseur, Georges, Vaziri, Kamran, Ventura, Sandro, Verdugo, Antonio, Vergani, Stefano, Vermeulen, Milo, Verzocchi, Marco, Vieira de Souza, Henrique, Vignoli, Chiara, Vilela, Cristovao, Viren, Brett, Vrba, Tomas, Wachala, Tomasz, Waldron, Abigail, Wallbank, Michael, Wang, Hanguo, Wang, Jingbo, Wang, Yi, Wang, Yue, Warburton, Karl, Warner, David, Wascko, Morgan, Waters, David, Watson, Alan, Weatherly, Pierce, Weber, Alfons, Weber, Michele, Wei, Hanyu, Weinstein, Amanda, Wenman, Dan, Wetstein, Matthew, Yang, Shaokai, Zeller, Geralyn (Sam), While, M.R., White, Andy, Whitehead, Leigh, Whittington, Denver, Wilking, Michael, Wilkinson, Callum, Williams, Zachary, Wilson, Fergus, Wilson, Robert, Wolcott, Jeremy, Wongjirad, Taritree, Wood, Kevin, Wood, Lynn, Worcester, Elizabeth, Worcester, Matthew, Wret, Clarence, Wu, Wanwei, Xiao, Y., Yang, Guang, Yang, Tingjun, Yershov, Nikolai, Yonehara, Katsuya, Young, Tim, Yu, Bo, Yu, Jae, Zalesak, Jaroslav, Zambelli, Laura, Zamorano, Bruno, Zani, Andrea, Zazueta, Luis, Zeller, G.P., Zennamo, Joseph, Zeug, Kyle, Zhang, Chao, Zhao, Manhong, Zhivun, Elena, Zhu, Guanying, Zimmerman, Eric, Zito, Marco, Zucchelli, Stefano, Zuklin, Josef, Zutshi, Vishnu, Zwaska, Robert, Institut de Physique des 2 Infinis de Lyon (IP2I Lyon), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Centre National de la Recherche Scientifique (CNRS), AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), 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 l'Accélérateur Linéaire (LAL), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), 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 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), DUNE, 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), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), and Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)
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safety ,Neutrino Oscillations. Neutrino detectors ,Physics - Instrumentation and Detectors ,hep-ex ,Physics::Instrumentation and Detectors ,engineering ,far detector ,FOS: Physical sciences ,Instrumentation and Detectors (physics.ins-det) ,fabrication ,time projection chamber: liquid argon ,High Energy Physics - Experiment ,High Energy Physics - Experiment (hep-ex) ,neutrino: deep underground detector ,quality ,[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex] ,High Energy Physics::Experiment ,[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det] ,Detectors and Experimental Techniques ,physics.ins-det ,Particle Physics - Experiment ,activity report - Abstract
The preponderance of matter over antimatter in the early universe, the dynamics of the supernovae that produced the heavy elements necessary for life, and whether protons eventually decay -- these mysteries at the forefront of particle physics and astrophysics are key to understanding the early evolution of our universe, its current state, and its eventual fate. The Deep Underground Neutrino Experiment (DUNE) is an international world-class experiment dedicated to addressing these questions as it searches for leptonic charge-parity symmetry violation, stands ready to capture supernova neutrino bursts, and seeks to observe nucleon decay as a signature of a grand unified theory underlying the standard model. The DUNE far detector technical design report (TDR) describes the DUNE physics program and the technical designs of the single- and dual-phase DUNE liquid argon TPC far detector modules. Volume III of this TDR describes how the activities required to design, construct, fabricate, install, and commission the DUNE far detector modules are organized and managed. This volume details the organizational structures that will carry out and/or oversee the planned far detector activities safely, successfully, on time, and on budget. It presents overviews of the facilities, supporting infrastructure, and detectors for context, and it outlines the project-related functions and methodologies used by the DUNE technical coordination organization, focusing on the areas of integration engineering, technical reviews, quality assurance and control, and safety oversight. Because of its more advanced stage of development, functional examples presented in this volume focus primarily on the single-phase (SP) detector module., Minor corrections made for JINST submission, 209 pages, 55 figures (updated typos in Table A.5; corrected errors in author list)
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- 2020
19. SMAUG v1.0 - a user-friendly muon simulator for transmission tomography of geological objects in 3D.
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Lechmann, Alessandro, Mair, David, Ariga, Akitaka, Ariga, Tomoko, Ereditato, Antonio, Nishiyama, Ryuichi, Pistillo, Ciro, Scampoli, Paola, Vladymyrov, Mykhailo, and Schlunegger, Fritz
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PARTICLE physics ,MARKOV chain Monte Carlo ,TOMOGRAPHY ,INVERSE problems ,MUONS - Abstract
Knowledge about muon tomography has spread in recent years in the geoscientific community and several collaborations between geologists and physicists have been founded. As the data analysis is still mostly done by particle physicists, we address the need of the geoscientific community to participate in the data analysis, while not having to worry too much about the particle physics equations in the background. The result hereof is SMAUG, a toolbox consisting of several modules that cover the various aspects of data analysis in a muon tomographic experiment. In this study we show how a comprehensive geophysical model can be built from basic physics equations. The emerging uncertainties are dealt with by a probabilistic formulation of the inverse problem, which is finally solved by a Monte Carlo Markov Chain algorithm. Finally, we benchmark the SMAUG results against those of a recent study, which however, have been established with an approach that is not easily accessible to the geoscientific community. We show that they reach identical results with the same level of accuracy and precision. [ABSTRACT FROM AUTHOR]
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- 2021
- Full Text
- View/download PDF
20. Summary of the International Conference on Onco-Nephrology: an emerging field in medicine
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Anna Capasso, Ariella Benigni, Umberto Capitanio, Farhad R. Danesh, Vincenzo Di Marzo, Loreto Gesualdo, Giuseppe Grandaliano, Edgar A. Jaimes, Jolanta Malyszko, Mark A. Perazella, Qi Qian, Pierre Ronco, Mitchell H. Rosner, Francesco Trepiccione, Davide Viggiano, Carmine Zoccali, Giovambattista Capasso, Ariga Akitaka, Amit Alahoti, Todd R. Alexander, Lucia Altucci, Hatem Amer, Vincenzo Barone, Ariela Benigni, Luigi Biancone, Joseph V. Bonventre, Giovanni Camussi, Fortunato Ciardiello, Michele Caraglia, Giacomo Cartenì, Andrés Cervantes, Franco Citterio, Laura Cosmai, Bruno Daniele, Antonietta D’Errico, Ferdinando De Vita, Antonio Ereditato, Geppino Falco, Denis Fouque, Renato Franco, Maurizio Gallieni, Giovanni Gambaro, Calvin Kuo, Vincent Launay-Vacher, Evaristo Maiello, Francesca Mallamaci, Jolanta Malysxko, Gennaro Marino, Erica Martinelli, Giuseppe Matarese, Takeshi Matsubara, Piergiorgio Messa, Carlo Messina, Vincenzo Mirone, Floriana Morgillo, Alessandro Nanni Costa, Michele Orditura, Antonello Pani, Mark Anthony Perazella, Alessandra Perna, Claudio Pisano, Todd Pitts, Camillo Porta, Giuseppe Procopio, Giuseppe Remuzzi, Domenico Russo, Lilian L. Siu, Walter Stadler, Teresa Troiani, Alessandro Weisz, Andrzej Więcek, Ding Xiaoqiang, Ortensio Zecchino, Dipartimento di Patologia Generale, Seconda Università degli studi di Napoli, IRCCS - Istituto di Ricerche Farmacologiche 'Mario Negri' [Milan, Italy], University of Turin, Università degli studi di Torino (UNITO), Department of urology, Università Vita-Salute San Raffaele, Department of Biochemistry and Biophysics, University of Naples Federico II, Universitat de València (UV), Department of Surgery , Renal Transplantation, Rome, Catholic University, Rome, Endocannabinoid Research Group, Institute of Biomolecular Chemistry (ENDOCANNABINOID RESEARCH GROUP), Consiglio Nazionale delle Ricerche [Roma] (CNR), Cardiovasculaire, métabolisme, diabétologie et nutrition (CarMeN), Institut National de la Recherche Agronomique (INRA)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National des Sciences Appliquées de Lyon (INSA Lyon), Université de Lyon-Institut National des Sciences Appliquées (INSA)-Institut National des Sciences Appliquées (INSA)-Hospices Civils de Lyon (HCL)-Institut National de la Santé et de la Recherche Médicale (INSERM), Pathologic Anatomy, Istituto Nazionale Tumori Fondazione Pascale, CeRTA, Service information conseil adaptation rénale [CHU Pitié-Salpêtrière] (Icar), Assistance publique - Hôpitaux de Paris (AP-HP) (AP-HP)-CHU Pitié-Salpêtrière [AP-HP], Sorbonne Université (SU)-Assistance publique - Hôpitaux de Paris (AP-HP) (AP-HP)-Sorbonne Université (SU), Azienda Ospedaliera Ospedali Civili Riuniti, 'Federico II' University of Naples Medical School, Division of Nephrology, Maggiore Hospital, IRCCS, Università degli studi di Napoli Federico II, GlaxoSmithKline, Glaxo Smith Kline, Research & Development, Sigma-Tau, Zhejiang University, CHU Tenon [AP-HP], Sorbonne Université (SU)-Assistance publique - Hôpitaux de Paris (AP-HP) (AP-HP), Paris-Centre de Recherche Cardiovasculaire (PARCC - UMR-S U970), Hôpital Européen Georges Pompidou [APHP] (HEGP), Assistance publique - Hôpitaux de Paris (AP-HP) (AP-HP)-Hôpitaux Universitaires Paris Ouest - Hôpitaux Universitaires Île de France Ouest (HUPO)-Assistance publique - Hôpitaux de Paris (AP-HP) (AP-HP)-Hôpitaux Universitaires Paris Ouest - Hôpitaux Universitaires Île de France Ouest (HUPO)-Université Paris Descartes - Paris 5 (UPD5)-Institut National de la Santé et de la Recherche Médicale (INSERM), SCIENZE BIOMOLECOLARI E BIOTECNOLOGIE, Inherited Kidney Diseases Nephrology Department, Barcelona, CNR-IFC Clinical Epidemiology and Pathophysiology of Renal Diseases and Hpertension Unit, Reggio Calabria, Reggio Calabria c/o Ospedali Riuniti, Université de Lyon-Institut National des Sciences Appliquées (INSA)-Institut National des Sciences Appliquées (INSA)-Institut National de la Santé et de la Recherche Médicale (INSERM)-Hospices Civils de Lyon (HCL), Assistance publique - Hôpitaux de Paris (AP-HP) (APHP)-CHU Pitié-Salpêtrière [APHP], CHU Tenon [APHP], Université Paris Descartes - Paris 5 (UPD5)-Institut National de la Santé et de la Recherche Médicale (INSERM)-Hôpital Européen Georges Pompidou [APHP] (HEGP), Assistance publique - Hôpitaux de Paris (AP-HP) (APHP)-Hôpitaux Universitaires Paris Ouest - Hôpitaux Universitaires Île de France Ouest (HUPO)-Assistance publique - Hôpitaux de Paris (AP-HP) (APHP)-Hôpitaux Universitaires Paris Ouest - Hôpitaux Universitaires Île de France Ouest (HUPO), Capasso, A., Benigni, A., Capitanio, U., Danesh, F. R., Di Marzo, V., Gesualdo, L., Grandaliano, G., Jaimes, E. A., Malyszko, J., Perazella, M. A., Qian, Q., Ronco, P., Rosner, M. H., Trepiccione, F., Viggiano, D., Zoccali, C., Capasso, G., Akitaka, A., Alahoti, A., Alexander, T. R., Altucci, L., Amer, H., Barone, V., Eri, K., Biancone, L., Bonventre, J. V., Camussi, G., Ciardiello, F., Caraglia, M., Carteni, G., Cervantes, A., Citterio, F., Cosmai, L., Daniele, B., D'Errico, A., De Vita, F., Ereditato, A., Falco, G., Fouque, D., Franco, R., Gallieni, M., Gambaro, G., Kuo, C., Launay-Vacher, V., Maiello, E., Mallamaci, F., Malysxko, J., Marino, G., Martinelli, E., Matarese, G., Matsubara, T., Messa, P., Messina, C., Mirone, V., Morgillo, F., Costa, A. N., Orditura, M., Pani, A., Perna, A., Pisano, C., Pitts, T., Porta, C., Procopio, G., Remuzzi, G., Russo, D., Siu, L. L., Stadler, W., Troiani, T., Weisz, A., Wiecek, A., Xiaoqiang, D., Zecchino, O., Université Paris Descartes - Paris 5 (UPD5)-Hôpital Européen Georges Pompidou [APHP] (HEGP), and Hôpitaux Universitaires Paris Ouest - Hôpitaux Universitaires Île de France Ouest (HUPO)-Assistance publique - Hôpitaux de Paris (AP-HP) (APHP)-Hôpitaux Universitaires Paris Ouest - Hôpitaux Universitaires Île de France Ouest (HUPO)-Assistance publique - Hôpitaux de Paris (AP-HP) (APHP)-Institut National de la Santé et de la Recherche Médicale (INSERM)
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0301 basic medicine ,renal cell carcinoma ,kidney ,Tumor incidence ,030232 urology & nephrology ,Medical Oncology ,chemotherapy ,Key issues ,Multidisciplinary team ,Kidney transplant ,Nephrologists ,Onco nephrology ,03 medical and health sciences ,0302 clinical medicine ,Neoplasms ,[SDV.BBM.GTP]Life Sciences [q-bio]/Biochemistry, Molecular Biology/Genomics [q-bio.GN] ,Nephrologist ,Settore MED/14 - NEFROLOGIA ,Humans ,cancer ,Medicine ,Cancer biology ,Renal Insufficiency, Chronic ,ComputingMilieux_MISCELLANEOUS ,Oncologists ,Medical education ,acute kidney injury ,chronic kidney disease ,nephrotoxicity ,business.industry ,Cancer ,endocannabinoid ,Congresses as Topic ,medicine.disease ,Faculty ,Kidney Transplantation ,3. Good health ,030104 developmental biology ,Nephrology ,Oncologist ,Neoplasm ,business ,Human - Abstract
Onco-nephrology is an emerging field in medicine. Patients with cancer may suffer from kidney diseases because of the cancer itself and cancer-related therapy. It is critical for nephrologists to be knowledgeable of cancer biology and therapy in order to be fully integrated in the multidisciplinary team and optimally manage patients with cancer and kidney diseases. In a recent international meeting, the key issues in this challenging clinical interface were addressed, including many unresolved basic science questions, such as the high tumor incidence in kidney transplant recipients. To this end, 70 highly qualified faculty members were gathered from all over the world to discuss these issues in 8 plenary sessions, including 5 keynote lectures. In addition, 48 young nephrologists and oncologists were invited to present their original observations that were highlighted in 2 large poster sessions.
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- 2019
21. FASER: ForwArd Search ExpeRiment at the LHC
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FASER Collaboration, Ariga, Akitaka, Ariga, Tomoko, Boyd, Jamie, Cadoux, Franck, Casper, David W., Favre, Yannick, Feng, Jonathan L., Ferrere, Didier, Galon, Iftah, Gonzalez-Sevilla, Sergio, Hsu, Shih-Chieh, Iacobucci, Giuseppe, Kajomovitz, Enrique, Kling, Felix, Kuehn, Susanne, Levinson, Lorne, Otono, Hidetoshi, Petersen, Brian, Sato, Osamu, Schott, Matthias, Sfyrla, Anna, Smolinsky, Jordan, Soffa, Aaron M., Takubo, Yosuke, Torrence, Eric, Trojanowski, Sebastian, and Zhang, Gang
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Physics - Instrumentation and Detectors ,Physics::Instrumentation and Detectors ,hep-ex ,FOS: Physical sciences ,hep-ph ,Instrumentation and Detectors (physics.ins-det) ,High Energy Physics - Experiment ,High Energy Physics - Experiment (hep-ex) ,High Energy Physics - Phenomenology ,High Energy Physics - Phenomenology (hep-ph) ,Detectors and Experimental Techniques ,physics.ins-det ,Particle Physics - Experiment ,Particle Physics - Phenomenology - Abstract
FASER, the ForwArd Search ExpeRiment, is a proposed experiment dedicated to searching for light, extremely weakly-interacting particles at the LHC. Such particles may be produced in the LHC's high-energy collisions in large numbers in the far-forward region and then travel long distances through concrete and rock without interacting. They may then decay to visible particles in FASER, which is placed 480 m downstream of the ATLAS interaction point. In this work, we describe the FASER program. In its first stage, FASER is an extremely compact and inexpensive detector, sensitive to decays in a cylindrical region of radius R = 10 cm and length L = 1.5 m. FASER is planned to be constructed and installed in Long Shutdown 2 and will collect data during Run 3 of the 14 TeV LHC from 2021-23. If FASER is successful, FASER 2, a much larger successor with roughly R ~ 1 m and L ~ 5 m, could be constructed in Long Shutdown 3 and collect data during the HL-LHC era from 2026-35. FASER and FASER 2 have the potential to discover dark photons, dark Higgs bosons, heavy neutral leptons, axion-like particles, and many other long-lived particles, as well as provide new information about neutrinos, with potentially far-ranging implications for particle physics and cosmology. We describe the current status, anticipated challenges, and discovery prospects of the FASER program., 13 pages, 4 figures, submitted as Input to the European Particle Physics Strategy Update 2018-2020 and draws on FASER's Letter of Intent, Technical Proposal, and physics case documents (arXiv:1811.10243, arXiv:1812.09139, and arXiv:1811.12522)
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- 2019
22. Measurement of the single π⁰ production rate in neutral current neutrino interactions on water
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Ariga, Akitaka, Ereditato, Antonio, Hierholzer, Martin, Koller, Patrick Pascal, Nirkko, Martti, Pistillo, Ciro, Redij, Asmita Ajit, and Wilkinson, Callum
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Physics::Instrumentation and Detectors ,530 Physics ,Astrophysics::High Energy Astrophysical Phenomena ,High Energy Physics::Experiment ,Nuclear Experiment - Abstract
The single π⁰ production rate in neutral current neutrino interactions on water in a neutrino beam with a peak neutrino energy of 0.6 GeV has been measured using the PØD, one of the subdetectors of the T2K near detector. The production rate was measured for data taking periods when the PØD contained water (2.64×10²⁰ protons-on-target) and also periods without water (3.49×10²⁰ protons-on-target). A measurement of the neutral current single π⁰ production rate on water is made using appropriate subtraction of the production rate with water in from the rate with water out of the target region. The subtraction analysis yields 106±41 (stat.) ± 69 (sys.) signal events where the uncertainties are statistical (stat.) and systematic (sys.) respectively. This is consistent with the prediction of 157 events from the nominal simulation. The measured to expected ratio is 0.68±0.26(stat)±0.44(sys)±0.12(flux). The nominal simulation uses a flux integrated cross section of 7.63×10-39 cm2 per nucleon with an average neutrino interaction energy of 1.3 GeV.
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- 2018
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23. Measurement of ν¯μ and νμ charged current inclusive cross sections and their ratio with the T2K off-axis near detector
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Ariga, Akitaka, Ereditato, Antonio, Koller, Patrick Pascal, Pistillo, Ciro, and Wilkinson, Callum
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530 Physics - Abstract
We report a measurement of cross section σ(νμ+nucleus→μ-+X) and the first measurements of the cross section σ(ν¯μ+nucleus→μ++X) and their ratio R(σ(ν¯)σ(ν)) at (anti) neutrino energies below 1.5 GeV. We determine the single momentum bin cross section measurements, averaged over the T2K ν¯/ν-flux, for the detector target material (mainly carbon, oxygen, hydrogen and copper) with phase space restricted laboratory frame kinematics of θμ500 MeV/c. The results are σ(ν¯)=(0.900±0.029(stat)±0.088(syst))×10-39 and σ(ν)=(2.41±0.022(stat)±0.231(syst))×10-39 in units of cm2/nucleon and R(σ(ν¯)σ(ν))=0.373±0.012(stat)±0.015(syst).
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- 2017
24. Updated T2K measurements of muon neutrino and antineutrino disappearance using 1.5×10²¹ protons on target
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Ariga, Akitaka, Ereditato, Antonio, Nirkko, Martti, Pistillo, Ciro, Redij, Asmita Ajit, and Wilkinson, Callum
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530 Physics - Published
- 2017
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25. Extra-large crystal emulsion detectors for future large-scale experiments
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Ariga, Tomoko, Ariga, Akitaka, Scampoli, Paola, and Vladymyrov, Mykhailo
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Physics::Instrumentation and Detectors ,530 Physics - Abstract
Photographic emulsion is a particle tracking device which features the best spatial resolution among particle detectors. For certain applications, for example muon radiography, large-scale detectors are required. Therefore, a huge surface has to be analyzed by means of automated optical microscopes. An improvement of the readout speed is then a crucial point to make these applications possible and the availability of a new type of photographic emulsions featuring crystals of larger size is a way to pursue this program. This would allow a lower magnification for the microscopes, a consequent larger field of view resulting in a faster data analysis. In this framework, we developed new kinds of emulsion detectors with a crystal size of 600-1000 nm, namely 3-5 times larger than conventional ones, allowing a 25 times faster data readout. The new photographic emulsions have shown a sufficient sensitivity and a good signal to noise ratio. The proposed development opens the way to future large-scale applications of the technology, e.g. 3D imaging of glacier bedrocks or future neutrino experiments.
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- 2016
26. Direct detection of antiprotons with the Timepix3 in a new electrostatic selection beamline
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Ereditato, Antonio, Scampoli, Paola, Ariga, Tomoko, and Ariga, Akitaka
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530 Physics - Published
- 2016
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27. Detection of low energy antimatter with emulsions
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Ariga, Tomoko, Ereditato, Antonio, Scampoli, Paola, Pistillo, Ciro, and Ariga, Akitaka
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Physics::Instrumentation and Detectors ,530 Physics ,High Energy Physics::Experiment - Abstract
Emulsion detectors feature a very high position resolution and consequently represent an ideal device when particle detection is required at the micrometric scale. This is the case of quantum interferometry studies with antimatter, where micrometric fringes have to be measured. In this framework, we designed and realized a new emulsion based detector characterized by a gel enriched in terms of silver bromide crystal contents poured on a glass plate. We tested the sensitivity of such a detector to low energy positrons in the range 10–20 keV . The obtained results prove that nuclear emulsions are highly efficient at detecting positrons at these energies. This achievement paves the way to perform matter-wave interferometry with positrons using this technology.
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- 2016
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28. Discovery of τ Neutrino Appearance in the CNGS Neutrino Beam with the OPERA Experiment
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Tufanli, Serhan, Pistillo, Ciro, Vuilleumier, Jean-Luc, Ereditato, Antonio, Ariga, Tomoko, Ariga, Akitaka, and Kreslo, Igor
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530 Physics - Abstract
The OPERA experiment was designed to search for νµ → ντ oscillations in appearance mode, i.e. by detecting the τ leptons produced in charged current ντ interactions. The experiment took data from 2008 to 2012 in the CERN Neutrinos to Gran Sasso beam. The observation of the νµ → ντ appearance, achieved with four candidate events in a subsample of the data, was previously reported. In this Letter, a fifth ντ candidate event, found in an enlarged data sample, is described. Together with a further reduction of the expected background, the candidate events detected so far allow us to assess the discovery of νµ → ντ oscillations in appearance mode with a significance larger than 5 σ.
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- 2015
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29. Characterization of the dose distribution in the halo region of a clinical proton pencil beam using emulsion film detectors
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Nesteruk, Konrad Pawel, Braccini, Saverio, Ariga, Akitaka, Scampoli, Paola, Pistillo, Ciro, Ariga, Tomoko, Ereditato, Antonio, and Giacoppo, Francesca
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530 Physics ,Quantitative Biology::Tissues and Organs ,Physics::Medical Physics ,Physics::Accelerator Physics - Abstract
Proton therapy is a high precision technique in cancer radiation therapy which allows irradiating the tumor with minimal damage to the surrounding healthy tissues. Pencil beam scanning is the most advanced dose distribution technique and it is based on a variable energy beam of a few millimeters FWHM which is moved to cover the target volume. Due to spurious effects of the accelerator, of dose distribution system and to the unavoidable scattering inside the patient's body, the pencil beam is surrounded by a halo that produces a peripheral dose. To assess this issue, nuclear emulsion films interleaved with tissue equivalent material were used for the first time to characterize the beam in the halo region and to experimentally evaluate the corresponding dose. The high-precision tracking performance of the emulsion films allowed studying the angular distribution of the protons in the halo. Measurements with this technique were performed on the clinical beam of the Gantry1 at the Paul Scherrer Institute. Proton tracks were identified in the emulsion films and the track density was studied at several depths. The corresponding dose was assessed by Monte Carlo simulations and the dose profile was obtained as a function of the distance from the center of the beam spot.
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- 2015
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30. Measurement of the νμ charged current quasielastic cross section on carbon with the T2K on-axis neutrino beam
- Author
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Hierholzer, Martin, Nirkko, Martti, Pistillo, Ciro, Göldi, Damian, Redij, Asmita Ajit, Ariga, Akitaka, and Ereditato, Antonio
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530 Physics ,Astrophysics::High Energy Astrophysical Phenomena ,High Energy Physics::Experiment ,Nuclear Experiment - Abstract
We report a measurement of the νµ charged current quasi-elastic cross-sections on carbon in the T2K on-axis neutrino beam. The measured charged current quasi-elastic cross-sections on carbon at mean neutrino energies of 1.94 GeV and 0.93 GeV are (11.95 ± 0.19(stat.) +1.82−1.47(syst.)) ×10^−39 cm^2/neutron, and (10.64 ± 0.37(stat.)+2.03−1.65(syst.)) × 10^−39 cm^2/neutron, respectively. These results agree well with the predictions of neutrino interaction models. In addition, we investigated the effects of the nuclear model and the multi-nucleon interaction.
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- 2015
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31. Experiments with low-energy antimatter
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Aghion, S., Gerber, S., Mariazzi, S., Malbrunot, C., Eidelman, S., Caravita, R., Demetrio, A., Zavatarelli, S., Di Noto, L., Storey, James William, Giardina, G., Rotondi, A., Petracek, V., Fontana, A., Testera, G., Amsler, Claude, Oberthaler, M., Comparat, D., Rosenberger, S., Brusa, R.S., Bonomi, G., Nedelec, P., Doser, M., Consolati, G., Lehner, S., Prelz, F., Riccardi, C., Cabaret, L., Zmeskal, J., Castelli, F., Derking, H., Chlouba, K., Jordan, E. J., Pacifico, N., Widmann, E., Bremer, J., Sacerdoti, M., Mandaglio, G., Hogan, S., Giammarchi, M., Ariga, Akitaka, Gligorova, A., Scampoli, Paola, Pistillo, Ciro, Strojek, I. M., Gninenko, S., Simon, M., Nebbia, G., Santoro, R., Kimura, Mitsuhiro, Cerchiari, G., Kellerbauer, A., Penasa, L., Kawada, Jiro, Venanzoni, G., Battaglieri, M., Cialdi, S., Dudarev, A., Prevedelli, M., Ariga, Tomoko, Matveev, V., Yzombard, P., Caccia, M., Krasnicky, D., Sandaker, H., Røhne, O.M., Holmestad, H., Bräunig, P., Ereditato, Antonio, Mazzotta, Z., Belov, A., Subieta, M., Ferragut, R., Lagomarsino, V., Ravelli, L., Haider, S., Huse, T., Spacek, M., Institut de Physique Nucléaire de Lyon (IPNL), Centre National de la Recherche Scientifique (CNRS)-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), G., Giardina, G., Consolati, S., Aghion, C., Amsler, A., Ariga, T., Ariga, A., Belov, G., Bonomi, P., Bräunig, J., Bremer, R. S., Brusa, L., Cabaret, M., Caccia, R., Caravita, F., Castelli, G., Cerchiari, K., Chlouba, S., Cialdi, D., Comparat, A., Demetrio, H., Derking, L., Di Noto, M., Doser, A., Dudarev, A., Ereditato, R., Ferragut, A., Fontana, S., Gerber, M., Giammarchi, A., Gligorova, S., Gninenko, S., Haider, S., Hogan, H., Holmestad, T., Huse, E. J., Jordan, J., Kawada, A., Kellerbauer, M., Kimura, D., Krasnicky, V., Lagomarsino, S., Lehner, C., Malbrunot, S., Mariazzi, V., Matveev, Z., Mazzotta, G., Nebbia, P., Nedelec, M., Oberthaler, N., Pacifico, L., Penasa, V., Petracek, C., Pistillo, F., Prelz, M., Prevedelli, L., Ravelli, C., Riccardi, O. M., Røhne, S., Rosenberger, A., Rotondi, M., Sacerdoti, H., Sandaker, R., Santoro, Scampoli, Paola, M., Simon, M., Spacek, J., Storey, I. M., Strojek, M., Subieta, G., Testera, E., Widmann, P., Yzombard, S., Zavatarelli, J., Zmeskal, S., Eidelman, G., Venanzoni, M., Battaglieri, and G., Mandaglio
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Physics ,Large Hadron Collider ,530 Physics ,QC1-999 ,PLASMAS ,ANTIHYDROGEN BEAM ,AEGIS EXPERIMENT ,PENNING TRAP ,GRAVITY ,SILICA ,ATOMS ,Nuclear physics ,Antiproton Decelerator ,Physics and Astronomy (all) ,Low energy ,Antimatter ,Systems engineering ,[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det] ,Antihydrogen ,GeneralLiterature_REFERENCE(e.g.,dictionaries,encyclopedias,glossaries) ,Particle Physics - Experiment ,ComputingMilieux_MISCELLANEOUS - Abstract
Investigations on antimatter allow us to shed light on fundamental issues of contemporary physics. The only antiatom presently available, antihydrogen, is produced making use of the Antiproton Decelerator (AD) facility at CERN. International collaborations currently on the floor (ALPHA, ASACUSA and ATRAP) have succeeded in producing antihydrogen and are now involved in its confinement and manipulation. The AEGIS experiment is currently completing the commissioning of the apparatus which will generate and manipulate antiatoms. The present paper, after a report on the main results achieved with antihydrogen physics, gives an overview of the AEGIS experiment, describes its current status and discusses its first target.
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- 2015
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32. Fast 3D tracking with GPUs for analysis of antiproton annihilations in emulsion detectors
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Ariga, Akitaka
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track data analysis ,nuclear emulsion ,Physics ,annihilation [anti-p p] ,3 [dimension] ,microprocessor ,graphics [multiprocessor] ,performance - Abstract
Contribution to Proceedings, Proc. of GPUHEP 2014, 119 - 124; DESY-PROC-2014-05; ISSN 1435-8077
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- 2015
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33. Measurements of neutrino oscillation in appearance and disappearance channels by the T2K experiment with 6.6×10²⁰ protons on target
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Ariga, Akitaka, Göldi, Damian, Ereditato, Antonio, Hierholzer, Martin, Nirkko, Martti, Pistillo, Ciro, and Redij, Asmita Ajit
- Subjects
530 Physics - Abstract
We report on measurements of neutrino oscillation using data from the T2K long-baseline neutrino experiment collected between 2010 and 2013. In an analysis of muon neutrino disappearance alone, we find the following estimates and 68% confidence intervals for the two possible mass hierarchies: Normal Hierarchy: sin²θ₂₃= 0.514+0.055−0.056 and ∆m²_32 = (2.51 ± 0.10) × 10⁻³ eV²/c⁴ Inverted Hierarchy: sin²θ₂₃= 0.511 ± 0.055 and ∆m²_13 = (2.48 ± 0.10) × 10⁻³ eV²/c⁴ The analysis accounts for multi-nucleon mechanisms in neutrino interactions which were found to introduce negligible bias. We describe our first analyses that combine measurements of muon neutrino disappearance and electron neutrino appearance to estimate four oscillation parameters, |∆m^2|, sin²θ₂₃, sin²θ₁₃, δCP , and the mass hierarchy. Frequentist and Bayesian intervals are presented for combinations of these parameters, with and without including recent reactor measurements. At 90% confidence level and including reactor measurements, we exclude the region δCP = [0.15, 0.83]π for normal hierarchy and δCP = [−0.08, 1.09]π for inverted hierarchy. The T2K and reactor data weakly favor the normal hierarchy with a Bayes Factor of 2.2. The most probable values and 68% 1D credible intervals for the other oscillation parameters, when reactor data are included, are: sin²θ₂₃= 0.528+0.055−0.038 and |∆m²_32| = (2.51 ± 0.11) × 10⁻³ eV²/c⁴.
- Published
- 2015
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34. The effect of rock composition on muon tomography measurements.
- Author
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Lechmann, Alessandro, Mair, David, Ariga, Akitaka, Ariga, Tomoko, Ereditato, Antonio, Nishiyama, Ryuichi, Pistillo, Ciro, Scampoli, Paola, Schlunegger, Fritz, and Vladymyrov, Mykhailo
- Subjects
BASALT ,LIMESTONE ,TOMOGRAPHY ,COSMIC ray muons ,COSMOGENIC nuclides - Abstract
In recent years, the use of radiographic inspection with cosmic-ray muons has spread into multiple research and industrial fields. This technique is based on the high-penetration power of cosmogenic muons. Specifically, it allows the resolution of internal density structures of large-scale geological objects through precise measurements of the muon absorption rate. So far, in many previous works, this muon absorption rate has been considered to depend solely on the density of traversed material (under the assumption of a standard rock) but the variation in chemical composition has not been taken seriously into account. However, from our experience with muon tomography in Alpine environments, we find that this assumption causes a substantial bias in the muon flux calculation, particularly where the target consists of high {Z2/A} rocks (like basalts and limestones) and where the material thickness exceeds 300 m. In this paper, we derive an energy loss equation for different minerals and we additionally derive a related equation for mineral assemblages that can be used for any rock type on which mineralogical data are available. Thus, for muon tomography experiments in which high {Z2/A} rock thicknesses can be expected, it is advisable to plan an accompanying geological field campaign to determine a realistic rock model. [ABSTRACT FROM AUTHOR]
- Published
- 2018
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- View/download PDF
35. The AEgIS Experiment
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Knecht, Andreas, Aghion, Stefano, Ahlén, O., Amsler, Claude, Ariga, Akitaka, Ariga, Tomoko, Belov, Alexander S., Bonomi, Germano, Bräunig, Philippe, Bremer, Johan, Brusa, Roberto S., Cabaret, Louis, Canali, Carlo, Caravita, Ruggero, Castelli, Fabrizio, Cerchiari, Giovanni, Cialdi, Simone, Comparat, Daniel, Consolati, Giovanni, Derking, Jan H., Di Domizio, Sergio, Di Noto, Lea, Doser, Michael, Dudarev, Alexey V., Ereditato, Antonio, Ferragut, Rafael, Fontana, Andrea, Genova, Pablo, Giammarchi, Marco G., Gligorova, Angela, Gninenko, Sergei N., Haider, Stefan, Hogan, Stephen D., Huse, Torkjell, Jordan, Elena J., Jørgensen, Lars V., Kaltenbacher, Thomas, Kawada, Jiro, Kellerbauer, Alban I., Kimura, Mitsuhiro, Krasnický, Daniel, Lagomarsino, Vittorio, Lehner, Sebastian, Malbrunot, Chloé, Mariazzi, Sebastiano, Matveev, Viktor A., Merkt, Frédéric, Moia, Fabio, Nebbia, Giancarlo, Nédélec, Patrick, Oberthaler, Markus K., Pacifico, Nicola, Petráček, Vojtěch, Pistillo, Ciro, Prelz, Francesco, Prevedelli, Marco, Regenfüs, Christian, Riccardi, Cristina, Røhne, Ole M., Rotondi, Alberto, Storey, James W., Subieta Vasquez, Martin A., Špaček, Michal, Testera, Gemma, Trezzi, Davide, Vaccarone, Renzo, Widmann, Eberhard, Zavatarelli, Sandra, and Zmeskal, Johannes
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Antimatter ,Gravity ,Antihydrogen - Abstract
The AEgIS experiment aims at performing the first test of the Weak Equivalence Principle of General Relativity in the antimatter sector by measuring the gravitational acceleration acting on a beam of cold antihydrogen to a precision of 1%. The installation of the apparatus is making good progress and large parts were taken into operation. Parasitic detector tests during the beamtime in December 2012 gave essential input for an optimal moiré deflectometer and the detector layout necessary to perform the gravity measurement., Hyperfine Interactions, 228 (1-3), ISSN:0304-3843, ISSN:0304-3834, ISSN:1572-9540, Proceedings of the 11th International Conference on Low Energy Antiproton Physics (LEAP 2013) held in Uppsala, Sweden, 10–15 June, 2013
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- 2014
36. Precise Measurement of the Neutrino Mixing Parameter θ₂₃ from Muon Neutrino Disappearance in an Off-Axis Beam
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Ariga, Tomoko, Kreslo, Igor, Nirkko, Martti, Göldi, Damian, Redij, Asmita Ajit, Ereditato, Antonio, Pistillo, Ciro, Ariga, Akitaka, and Hierholzer, Martin
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530 Physics - Abstract
New data from the T2K neutrino oscillation experiment produce the most precise measurement of the neutrino mixing parameter θ 23 . Using an off-axis neutrino beam with a peak energy of 0.6 GeV and a data set corresponding to 6.57×10 20 protons on target, T2K has fit the energy-dependent ν μ oscillation probability to determine oscillation parameters. The 68% confidence limit on sin 2 (θ 23 ) is 0.514 +0.055 −0.056 (0.511±0.055 ), assuming normal (inverted) mass hierarchy. The best-fit mass-squared splitting for normal hierarchy is Δm 2 32 =(2.51±0.10)×10 −3 eV 2 /c 4 (inverted hierarchy: Δm 2 13 =(2.48±0.10)×10 −3 eV 2 /c 4 ). Adding a model of multinucleon interactions that affect neutrino energy reconstruction is found to produce only small biases in neutrino oscillation parameter extraction at current levels of statistical uncertainty.
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- 2014
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37. Measurement of the neutrino-oxygen neutral-current interaction cross section by observing nuclear deexcitation γ rays
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Kreslo, Igor, Ereditato, Antonio, Hierholzer, Martin, Ariga, Akitaka, Pistillo, Ciro, Redij, Asmita Ajit, Martti, Nirkko, Göldi, Damian, and Ariga, Tomoko
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Physics::Instrumentation and Detectors ,530 Physics ,610 Medicine & health ,360 Social problems & social services - Abstract
We report the first measurement of the neutrino-oxygen neutral-current quasielastic (NCQE) cross section. It is obtained by observing nuclear deexcitation γ rays which follow neutrino-oxygen interactions at the Super-Kamiokande water Cherenkov detector. We use T2K data corresponding to 3.01 × 1020 protons on target. By selecting only events during the T2K beam window and with well-reconstructed vertices in the fiducial volume, the large background rate from natural radioactivity is dramatically reduced. We observe 43 events in the 4–30 MeV reconstructed energy window, compared with an expectation of 51.0, which includes an estimated 16.2 background events. The background is primarily nonquasielastic neutral-current interactions and has only 1.2 events from natural radioactivity. The flux-averaged NCQE cross section we measure is 1.55 × 10−38 cm2 with a 68% confidence interval of ð1.22; 2.20Þ × 10−38 cm2 at a median neutrino energy of 630 MeV, compared with the theoretical prediction of 2.01 × 10−38 cm2.
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- 2014
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38. Measuring gbar with AEgIS, progress and perspectives
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Amsler, Claude, Ariga, Akitaka, Ariga, Tomoko, Ereditato, Antonio, Kawada, Jiro, Kimura, Mitsuhiro, Pistillo, Ciro, Scampoli, Paola, and Storey, James William
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530 Physics - Abstract
AEgIS experiment’s main goal is to measure the local gravitational acceleration of antihydrogen¯g and thus perform a direct test of the weak equivalence principle with antimatter. In the first phase of the experiment the aim is to measure ¯g with 1% relative precision. This paper presents the antihydrogen production method and a description of some components of the experiment, which are necessary for the gravity measurement. Current status of the AE¯gIS experimental apparatus is presented and recent commissioning results with antiprotons are outlined. In conclusion we discuss the short-term goals of the AE¯gIS collaboration that will pave the way for the first gravity measurement in the near future.
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- 2014
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39. Evidence for νμ → ντ appearance in the CNGS neutrino beam with the OPERA experiment
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Ariga, Akitaka, Tufanli, Serhan, Kawada, Jiro, Brunetti, Giulia, Ariga, Tomoko, Pistillo, Ciro, Kreslo, Igor, Ben Dhahbi, Anis, Vuilleumier, Jean-Luc, Kimura, Mitsuhiro, Strauss, Thomas, and Ereditato, Antonio
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530 Physics - Abstract
The OPERA experiment is designed to search for ν μ →ν τ oscillations in appearance mode, i.e., through the direct observation of the τ lepton in ν τ -charged current interactions. The experiment has taken data for five years, since 2008, with the CERN Neutrino to Gran Sasso beam. Previously, two ν τ candidates with a τ decaying into hadrons were observed in a subsample of data of the 2008–2011 runs. Here we report the observation of a third ν τ candidate in the τ − →μ − decay channel coming from the analysis of a subsample of the 2012 run. Taking into account the estimated background, the absence of ν μ →ν τ oscillations is excluded at the 3.4 σ level.
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- 2014
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40. Measurement of the TeV atmospheric muon charge ratio with the complete OPERA data set
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Ereditato, Antonio, Ariga, Akitaka, Ariga, Tomoko, Kawada, Jiro, Kreslo, Igor, Pistillo, Ciro, Tufanli, Serhan, and Vuilleumier, Jean-Luc
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Physics::Instrumentation and Detectors ,530 Physics ,Astrophysics::High Energy Astrophysical Phenomena ,High Energy Physics::Experiment - Abstract
The OPERA detector, designed to search for νμ → ντ oscillations in the CNGS beam, is located in the underground Gran Sasso laboratory, a privileged location to study TeV-scale cosmic rays. For the analysis here presented, the detector was used to measure the atmospheric muon charge ratio in the TeV region. OPERA collected chargeseparated cosmic ray data between 2008 and 2012. More than 3 million atmospheric muon events were detected and reconstructed, among which about 110000 multiple muon bundles. The charge ratio Rμ ≡ Nμ+/Nμ− was measured separately for single and for multiple muon events. The analysis exploited the inversion of the magnet polarity which was performed on purpose during the 2012 Run. The combination of the two data sets with opposite magnet polarities allowedminimizing systematic uncertainties and reaching an accurate determination of the muon charge ratio. Data were fitted to obtain relevant parameters on the composition of primary cosmic rays and the associated kaon production in the forward fragmentation region. In the surface energy range 1–20 TeV investigated by OPERA, Rμ is well described by a parametric model including only pion and kaon contributions to themuon flux, showing no significant contribution of the prompt component. The energy independence supports the validity of Feynman scaling in the fragmentation region up to 200 TeV/nucleon primary energy.
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- 2014
41. AEgIS Experiment: Measuring the acceleration g of the earth gravitational field on antihydrogen beam
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AEgIS, Experiment, Amsler, Claude, Ariga, Akitaka, Ariga, Tomoko, Ereditato, Antonio, Kawada, Jiro, Kimura, Mitsuhiro, Pistillo, Ciro, Scampoli, Paola, and Storey, James William
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530 Physics - Published
- 2014
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42. Development of nuclear emulsions with View the 1µm source spatial resolution for the AEgIS experiment
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Kimura, M., Aghion, Stefano, Ahlén, O., Amsler, Claude, Ariga, Akitaka, Ariga, Tadashi, Belov, A.S., Bonomi, Germano, Bräunig, P., Bremer, J, Brusa, R.S., Burghart, G., Cabaret, L., Canali, Claudia, Caravita, Ruggero, Castelli, Francesco, Cerchiari, Giovanni, Cialdi, S., Comparat, D., Consolati, Giovanni, Di Domizio, Sergio, Nédélec, P., Noto, L. Di, Doser, M., Dudarev, A., Ereditato, A., Ferragut, R., Fontana, A., Genova, P., Giammarchi, M., Gligorova, A., Gninenko, S. N., Haider, S., Hogan, S. D., Huse, T., Jordan, E., Jørgensen, L. V., Kaltenbacher, T., Kawada, J., Kellerbauer, A., Knecht, A., Krasnický, D., Lagomarsino, V., Mariazzi, S., Matveev, V. A., Merkt, F., Moia, F., Nebbia, G., Oberthaler, M. K., Pacifico, N., Petracek, Vojtech, Pistillo, Ciro, Prelz, F., Prevedelli, M., Regenfus, C., Riccardi, C., Røhne, O., Rotondi, A., Sandaker, H., Scampoli, P., Storey, J., Vasquez, M. A. Subieta, Špaček, M., Testera, G., Trezzi, D., Vaccarone, R., Zavatarelli, S., Laboratoire Aimé Cotton (LAC), École normale supérieure - Cachan (ENS Cachan)-Université Paris-Sud - Paris 11 (UP11)-Centre National de la Recherche Scientifique (CNRS), 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), European Organization for Nuclear Research (CERN), Démarche intégrée pour l'obtention d'aliments de qualité (UMR Qualisud), Centre de Coopération Internationale en Recherche Agronomique pour le Développement (Cirad)-Université Montpellier 1 (UM1)-Université Montpellier 2 - Sciences et Techniques (UM2)-Centre international d'études supérieures en sciences agronomiques (Montpellier SupAgro)-Avignon Université (AU)-Université de La Réunion (UR)-Université de Montpellier (UM)-Institut national d’études supérieures agronomiques de Montpellier (Montpellier SupAgro), AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Structure and Dynamics of Nucleic Acids, National Centre for Biological Sciences, Eidgenössische Technische Hochschule - Swiss Federal Institute of Technology [Zürich] (ETH Zürich), Istituto Nazionale di Fisica Nucleare, Sezione di Padova (INFN, Sezione di Padova), Istituto Nazionale di Fisica Nucleare (INFN), Dipartimento di Chimica Fisica e Inorganica [Bologna], Alma Mater Studiorum Università di Bologna [Bologna] (UNIBO), AEGIS, Centre National de la Recherche Scientifique (CNRS)-Université Paris-Sud - Paris 11 (UP11)-École normale supérieure - Cachan (ENS Cachan), Centre National de la Recherche Scientifique (CNRS)-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), Institut national d'enseignement supérieur pour l'agriculture, l'alimentation et l'environnement (Institut Agro)-Institut national d'enseignement supérieur pour l'agriculture, l'alimentation et l'environnement (Institut Agro), Observatoire de Paris, and Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)
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CERN-AD ,Photographic emulsions ,Physics::Instrumentation and Detectors ,AEgIS ,[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det] ,Nuclear Experiment ,Antihydrogen ,Antigravity - Abstract
see paper for full list of authors; International audience; The main goal of the AEgIS experiment at CERN is to test the weak equivalence principle for antimatter. We will measure the Earth's gravitational acceleration with antihydrogen atoms being launched in a horizontal vacuum tube and traversing a moiré deflectometer. We intend to use a position sensitive device made of nuclear emulsions (combined with a time-of-flight detector such as silicon ) to measure precisely their annihilation points at the end of the tube. The goal is to determine with a 1% relative accuracy. In 2012 we tested emulsion films in vacuum and at room temperature with low energy antiprotons from the CERN antiproton decelerator. First results on the expected performance for AEgIS are presented.
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- 2013
43. The T2K Neutrino Flux Prediction
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Ariga, Akitaka, Frank, Eike, Messina, Marcello, Bay, Fatih, Ereditato, Antonio, T2K, Collaboration, Ariga, Tomoko, and Kreslo, Igor
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530 Physics - Published
- 2013
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44. Measurement of the Inclusive NuMu Charged Current Cross Section on Carbon in the Near Detector of the T2K
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Ariga, Tomoko, Ereditato, Antonio, Kreslo, Igor, T2K, Collaboration, Messina, Marcello, Bay, Fatih, Frank, Eike, and Ariga, Akitaka
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Physics::Instrumentation and Detectors ,530 Physics ,High Energy Physics::Experiment ,Nuclear Experiment - Abstract
T2K has performed the first measurement of nu(mu) inclusive charged current interactions on carbon at neutrino energies of similar to 1 GeV where the measurement is reported as a flux-averaged double differential cross section in muon momentum and angle. The flux is predicted by the beam Monte Carlo and external data, including the results from the NA61/SHINE experiment. The data used for this measurement were taken in 2010 and 2011, with a total of 10.8 x 10(19) protons-on-target. The analysis is performed on 4485 inclusive charged current interaction candidates selected in the most upstream fine-grained scintillator detector of the near detector. The flux-averaged total cross section is (phi) = (6.91 +/- 0.13(stat) +/- 0.84(syst)) x 10(-39) cm(2)/nucleon for a mean neutrino energy of 0.85 GeV.
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- 2013
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45. OPERA experiment and its releted emulsion techniques.
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Ariga, Akitaka
- Subjects
- *
NEUTRINOS , *EMULSIONS , *OSCILLATIONS , *SCANNING systems , *NUCLEAR physics - Abstract
The OPERA experiment is designed to clarify neutrino oscillation by detecting appearance of ντ in pure νμ beam through a long baseline method (CNGS beam from cern to the Gran Sasso laboratory). The key technique is the use of emulsion films and their scanning. We developed a new high speed scanning system with speed of 50 cm2/h and it was successfully demonstrated in 2006 CNGS commissioning. The new scanning system is not only meant for the OPERA experiment, but it has large potential of applications. For example, measurement of νe with strong separation power against π0. Or a compact emulsion spectrometer for future neutrino experiments. [ABSTRACT FROM AUTHOR]
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- 2008
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46. An alternative approach to interface detection in muon tomography experiments: Algebraic surfaces.
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Lechmann, Alessandro, Mair, David, Schlunegger, Fritz, Ariga, Akitaka, Ereditato, Antonio, Pistillo, Ciro, Scampoli, Paola, Vladymyrov, Mykhailo, Ariga, Tomoko, and Nishiyama, Ryuichi
- Published
- 2019
47. Testing the Weak Equivalence Principle with an antimatter beam at CERN
- Author
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Ravelli, L, Zmeskal, J., Yzombard, P, Bonomi, G., Ereditato, Antonio, Kellerbauer, A, Cerchiari, G., Riccardi, C, Pagano, D, Lehner, S, Holmestad, H, Spacek, M, Amsler, Claude, Haider, S, Storey, James William, Matveev, V, Kimura, Mitsuhiro, Krasnicky, D, Sorrentino, F, Doser, M, Caravita, R., Belov, A., Ariga, Akitaka, Jordan, E J, Zavatarelli, S, Lagomarsino, V, Cialdi, S, Caccia, M., Røhne, O M, Testera, G, Gerber, S, Chlouba, K., Castelli, F., Rotondi, A, Scampoli, Paola, Santoro, R, Ariga, Tomoko, Malbrunot, C, Comparat, D, Kawada, Jiro, Dudarev, A, Oberthaler, M, Demetrio, A, Bräunig, P., Derking, H, Ferragut, R, Huse, T, Pistillo, Ciro, Mazzotta, Z, Noto, L Di, Cabaret, L., Bremer, J., Pacifico, N, Strojek, I M, Petracek, V, Sandaker, H, Rosenberger, S, Gninenko, S, Widmann, E, Penasa, L, Prevedelli, M, Consolati, G, Fontana, A, Brusa, R. S., Gligorova, A, Prelz, F, Aghion, S., Nedelec, P, Subieta, M, Giammarchi, M, Mariazzi, S, Nebbia, G, and Sacerdoti, M
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Physics::General Physics ,530 Physics ,Physics::Atomic and Molecular Clusters ,Physics::Accelerator Physics ,Physics::Atomic Physics ,7. Clean energy - Abstract
The goal of the AEgIS experiment is to measure the gravitational acceleration of antihydrogen – the simplest atom consisting entirely of antimatter – with the ultimate precision of 1%. We plan to verify the Weak Equivalence Principle (WEP), one of the fundamental laws of nature, with an antimatter beam. The experiment consists of a positron accumulator, an antiproton trap and a Stark accelerator in a solenoidal magnetic field to form and accelerate a pulsed beam of antihydrogen atoms towards a free-fall detector. The antihydrogen beam passes through a moir ́e deflectometer to measure the vertical displacement due to the gravitational force. A position and time sensitive hybrid detector registers the annihilation points of the antihydrogen atoms and their time-of-flight. The detection principle has been successfully tested with antiprotons and a miniature moir ́e deflectometer coupled to a nuclear emulsion detector.
48. Observation of Electron Neutrino Appearance in a Muon Neutrino Beam
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Reinherz-Aronis, E., Drapier, O., Sobczyk, J. T., Marteau, J., Gonin, M., Koch, L., Kudenko, Y., Ziembicki, M., Adam, J., Okusawa, T., Murakami, A., Marzec, J., Emery, S., Zalipska, J., Shustrov, Y., Thompson, L. F., Suzuki, K., Kakuno, H., Kolaceke, A., Laveder, M., Metelko, C., Pickard, L. J., Miura, M., Smith, R. J., Davis, S., Grant, N., Hastings, N. C., Pinzon Guerra, E. S., Oyama, Y., Naples, D., Poplawska, E., Ieva, M., Cartwright, S. L., Kurjata, R., Bronner, C., Perevozchikov, O., Myslik, J., Petrov, Y., Koseki, K., Friend, M., Hara, T., Nakayama, S., Szeglowski, T., Macaire, M., Zaremba, K., Weber, A., Matveev, V., Horikawa, S., Martti, Nirkko, Kearns, E., Ueno, K., Floetotto, L., Tzanov, M., Uchida, Y., Totsuka, Y., Bordoni, S., Catanesi, M. G., McCarthy, M., Plonski, P., Kitching, P., Mazzucato, E., Densham, C., Tomura, T., Göldi, Damian, Duffy, K., Dziewiecki, M., Scholberg, K., Kobayashi, T., Kreslo, Igor, Berardi, V., Cervera, A., Finch, A. J., Oryszczak, W., Hirota, S., Kilinski, A., Ishii, T., Escudero, L., Golan, T., Seiya, Y., Sinclair, P., Lamont, I., Haigh, M. D., Di Lodovico, F., Korzenev, A., Mathie, E. L., Kikawa, T., Nishimura, Y., Khabibullin, M., Tsukamoto, T., Blondel, A., Okumura, K., Takahashi, S., Dumarchez, J., Redij, Asmita Ajit, Suzuki, A., Karlen, D., Iyogi, K., Aihara, H., Ieki, K., Castillo, R., Galymov, V., Akiri, T., Terhorst, D., Yokoyama, M., Robert, A., Wachala, T., Karpikov, I., Toki, W., Brailsford, D., Christodoulou, G., Pistillo, Ciro, Missert, A., Smith, B., Jacob, A., Popov, B., Wilkes, R. J., Perkin, J. D., Mineev, O., Dealtry, T., Hasegawa, T., Jamieson, B., Aoki, S., Suzuki, Y., Lindner, T., Sánchez, F., Lister, C., Bertram, I., Di Luise, S., Giffin, S., Lazos, M., Owen, R. A., Kropp, W., McGrew, C., Zimmerman, E. D., Gilje, K., Ravonel, M., Cremonesi, L., Murdoch, M., Marino, A. D., Nakahata, M., Dytman, S., Rondio, E., Miller, C. A., Giganti, C., Duboyski, T., Takeda, A., Tanaka, H. A., Lawe, M., Nagasaki, T., Oser, S. M., Ariga, Tomoko, Schwehr, J., Mahn, K., Coleman, S. J., Dennis, S. R., Assylbekov, S., Ohta, R., Ishida, T., Rayner, M. A. M., Southwell, L., Mijakowski, P., Autiero, D., Calland, R. G., Kutter, T., Dufour, F., Nakamura, K., Suda, Y., Wilson, R. J., Takeuchi, Y., Insler, J., Vasseur, G., Hierholzer, Martin, Roth, S., Andreopoulos, C., Furmanski, A. P., Steinmann, J., Vagins, M., Ruterbories, D., Palladino, V., Hansen, D., Hayato, Y., Yamamoto, K., Hignight, J., Nishikawa, K., Wilking, M. J., Lee, K. P., Kameda, J., Nakaya, T., Touramanis, C., Danko, I., Fukuda, Y., Abe, K., Bentham, S. W., Sgalaberna, D., Connolly, K., Yershov, N., Waldron, A. V., Yuan, T., Nakayoshi, K., Hadley, D. R., Terri, R., Vacheret, A., Konaka, A., Scantamburlo, E., Irvine, T. J., Bravar, A., Wark, D., Retiere, F., Batkiewicz, M., Fujii, Y., Coleman, J., Maruyama, T., Manly, S., Sacco, R., Huang, K., Himmel, A., Malek, M., Clifton, A., Kormos, L. L., Mine, S., Ives, S. J., Das, R., Ratoff, P. N., Gudin, D., Moriyama, S., Yamada, Y., Hamilton, P., Haesler, A., Wilkinson, C., Caravaca Rodríguez, J., Sobel, H., Żmuda, J., Johnson, R. A., Walter, C. W., Scott, M., Poutissou, J.-M., Helmer, R. L., Sakashita, K., Dabrowska, A., Ikeda, M., Murphy, S., McCauley, N., Nielsen, C., Rubbia, A., Kajita, T., Jonsson, P., Short, S., Przewlocki, P., Berger, B. E., Khotjantsev, A., Radicioni, E., Tobayama, S., Berkman, S., Koshio, Y., Mezzetto, M., Jo, J. H., Kumaratunga, S., Sato, F., Nakai, T., Barr, G., Kim, J., Blaszczyk, F. D. M., Wongjirad, T., Licciardi, C., Reeves, M., Longhin, A., De Perio, P., Yanagisawa, C., Thorley, A., Boyd, S. B., Cherdack, D., Ichikawa, A. K., Martin, J. F., Stamoulis, P., Yen, S., Izmaylov, A., Litchfield, R. P., Hartz, M., Rodrigues, P. A., Zalewska, A., Kanazawa, Y., Collazuol, G., Laihem, K., Zito, M., Nakadaira, T., Wascko, M. O., Smy, M., Hillairet, A., Ereditato, Antonio, Paolone, V., Minamino, A., Quilain, B., Buchanan, N., Holeczek, J., Tanaka, M. M., Mueller, Th. A., Still, B., Lagoda, J., Tada, M., Tanaka, H. K., Sekiya, H., Rojas, P., Jung, C. K., Zambelli, L., Sorel, M., Kisiel, J., Mavrokoridis, K., Gomez-Cadenas, J. J., Ariga, Akitaka, Suzuki, S. Y., Bhadra, S., Pearce, G. F., Monfregola, L., Williamson, Z., Bay, F., Ludovici, L., Bass, M., Kaboth, A. C., Posiadala, M., Gaudin, A., De Rosa, G., O’Keeffe, H. M., McFarland, K. S., Wendell, R., Barbi, M., Hiraki, T., Kielczewska, D., Shiozawa, M., Kubo, H., Bojechko, C., Tacik, R., Magaletti, L., Hearty, C., Imber, J., Payne, D., Sekiguchi, T., Wilson, J. R., Poutissou, R., and Barker, G. J.
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530 Physics ,7. Clean energy - Abstract
The T2K experiment has observed electron neutrino appearance in a muon neutrino beam produced 295 km from the Super-Kamiokande detector with a peak energy of 0.6 GeV. A total of 28 electron neutrino events were detected with an energy distribution consistent with an appearance signal, corresponding to a significance of 7.3σ when compared to 4.92 ± 0.55 expected background events. In the PMNS mixing model, the electron neutrino appearance signal depends on several parameters including three mixing angles θ12, θ23, θ13, a mass difference Δm232 and a CP violating phase δCP. In this neutrino oscillation scenario, assuming |Δm232|=2.4×10−3 eV2, sin2θ23=0.5, δCP=0, and Δm232>0 (Δm232
49. The mass-hierarchy and CP-violation discovery reach of the LBNO long-baseline neutrino experiment
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Ariga, Akitaka, Ariga, Tomoko, Ereditato, Antonio, Haug, Sigve, Hierholzer, Martin, Kawada, Jiro, Kreslo, Igor, Pistillo, Ciro, Strauss, Thomas, and Weber, Michael
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Physics::Instrumentation and Detectors ,13. Climate action ,530 Physics ,7. Clean energy - Abstract
The next generation neutrino observatory proposed by the LBNO collaboration will address fundamental questions in particle and astroparticle physics. The experiment consists of a far detector, in its first stage a 20 kt LAr double phase TPC and a magnetised iron calorimeter, situated at 2300 km from CERN and a near detector based on a highpressure argon gas TPC. The long baseline provides a unique opportunity to study neutrino flavour oscillations over their 1st and 2nd oscillation maxima exploring the L/E behaviour, and distinguishing effects arising from δCP and matter. In this paper we have reevaluated the physics potential of this setup for determining the mass hierarchy (MH) and discovering CP-violation (CPV), using a conventional neutrino beam from the CERN SPS with a power of 750 kW. We use conservative assumptions on the knowledge of oscillation parameter priors and systematic uncertainties. The impact of each systematic error and the precision of oscillation prior is shown. We demonstrate that the first stage of LBNO can determine unambiguously the MH to > 5δ C.L. over the whole phase space. We show that the statistical treatment of the experiment is of very high importance, resulting in the conclusion that LBNO has ~ 100% probability to determine the MH in at most 4-5 years of running. Since the knowledge of MH is indispensable to extract δCP from the data, the first LBNO phase can convincingly give evidence for CPV on the 3δ C.L. using today’s knowledge on oscillation parameters and realistic assumptions on the systematic uncertainties.
50. A moiré deflectometer for antimatter
- Author
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Scampoli, Paola, Pistillo, Ciro, Ereditato, Antonio, Kimura, Mitsuhiro, Amsler, Claude, Ariga, Tomoko, Ariga, Akitaka, Storey, James William, and Kawada, Jiro
- Subjects
Physics::General Physics ,530 Physics ,7. Clean energy - Abstract
The precise measurement of forces is one way to obtain deep insight into the fundamental interactions present in nature. In the context of neutral antimatter, the gravitational interaction is of high interest, potentially revealing new forces that violate the weak equivalence principle. Here we report on a successful extension of a tool from atom optics—the moiré deflectometer—for a measurement of the acceleration of slow antiprotons. The setup consists of two identical transmission gratings and a spatially resolving emulsion detector for antiproton annihilations. Absolute referencing of the observed antimatter pattern with a photon pattern experiencing no deflection allows the direct inference of forces present. The concept is also straightforwardly applicable to antihydrogen measurements as pursued by the AEgIS collaboration. The combination of these very different techniques from high energy and atomic physics opens a very promising route to the direct detection of the gravitational acceleration of neutral antimatter.
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