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51. Neutrinos below 100 TeV from the southern sky employing refined veto techniques to IceCube data

Author: A. O'Murchadha, D. J. Koskinen, Timothyblake Watson, Timo Karg, A. Kyriacou, E. Bourbeau, R. Maunu, C. Pérez de los Heros, T. Menne, Matthias Vraeghe, Maria Tselengidou, E. O’Sullivan, B. Relethford, J. Auffenberg, Raffaela Busse, D. Soldin, K. Rawlins, Claudio Kopper, J. Becker Tjus, Konstancja Satalecka, Subir Sarkar, Z. Griffith, Theo Glauch, R. Hellauer, K. Mallot, B. J. P. Jones, U. Katz, Minjin Jeong, James W. Wood, James Madsen, Thomas Meures, K. Hoshina, M. E. Huber, P. B. Price, Benjamin Hokanson-Fasig, N. L. Strotjohann, Segev BenZvi, Felix Henningsen, Glenn Spiczak, G. Momenté, M. Rameez, Lu Lu, Marcos Santander, R. Ström, Won Nam Kang, A. R. Fazely, H. Bagherpour, E. Pinat, P. Backes, X. Bai, D. van Eijk, Simona Toscano, D. F. Cowen, U. Naumann, K. D. de Vries, Spencer Klein, Andres Medina, Olga Botner, S. Tilav, E. Unger, L. Gerhardt, G. Neer, T. Kintscher, Francesco Lucarelli, Frederik Hermann Lauber, S. Hickford, A. Olivas, J. J. Beatty, Daniel Bindig, J. P. Yanez, N. Kulacz, G. H. Collin, Azadeh Keivani, T. Glüsenkamp, T. O. B. Schmidt, V. Baum, Teresa Montaruli, K. Jero, Tianlu Yuan, Sebastian Böser, C. Chen, Kara Hoffman, Kendall Mahn, K. Wiebe, J. Stettner, Hermann Kolanoski, A. Terliuk, S. Westerhoff, T. R. Wood, Justin Lanfranchi, R. Turcotte, K. Helbing, Yiqian Xu, Karl J. Clark, Matt Dunkman, Hrvoje Dujmovic, Sander Vanheule, Javier Gonzalez, L. Rauch, Anastasia Maria Barbano, Kurt Woschnagg, T. Kittler, G. W. Sullivan, Giorgio Maggi, James E. Braun, Alexander Sandrock, Thomas Ehrhardt, E. Cheung, Thomas Stuttard, H.-P. Bretz, Qinrui Liu, Martina Karl, M. Song, T. L. Carver, Mike Richman, Jochen M. Schneider, Paul Evenson, Hershal Pandya, C. De Clercq, Mirco Hunnefeld, Wolfgang Rhode, Dirk Ryckbosch, Nahee Park, K. Hultqvist, Stephan Meighen-Berger, Chunfai Tung, S. Yoshida, Elisa Bernardini, David A. Williams, Robert Stein, Lenka Tomankova, D. Hebecker, Karim Ghorbani, Spencer Axani, Simone Garrappa, Darren Grant, L. Wills, Markus Ackermann, S. W. Barwick, M. Stamatikos, D. Rysewyk, M. Silva, Kayla Leonard, M. J. Larson, M. A. Unland Elorrieta, Dmitry Chirkin, Sarah Mancina, Sarah Nowicki, Alexander Kappes, N. Kurahashi, Jenni Adams, I. Taboada, P. Peiffer, Joshua Hignight, Todor Stanev, C. Wendt, Paul Coppin, Michael O. Wolf, P. Nakarmi, Carlos Arguelles, J. P. A. M. de André, N. van Eijndhoven, C. Haack, Delia Tosi, Anna Franckowiak, Tobias Hoinka, Andrea Turcati, Jessie Micallef, A. Goldschmidt, Jung-Hyun Kim, Ibrahim Safa, Francis Halzen, P. Schlunder, G. de Wasseige, M. Wallraff, F. Huang, J. van Santen, A. Stößl, M. Börner, Steve Sclafani, Damian Pieloth, Ali Kheirandish, W. Van Driessche, J. Kiryluk, Alex Pizzuto, Daria Pankova, R. Hoffmann, E. Friedman, George Japaridze, Roger Moore, Gary Binder, Christian Spiering, D. R. Nygren, Reina H. Maruyama, I. Ansseau, K. Becker, Jan Soedingrekso, C. Walck, Marek Kowalski, Steven Robertson, Elisa Lohfink, K. Andeen, Jannes Brostean-Kaiser, Summer Blot, Thomas K. Gaisser, G. B. Yodh, J. Bourbeau, E. Jacobi, R. G. Stokstad, R. Nahnhauer, Gisela Anton, A. Stasik, Justin Vandenbroucke, Juliana Stachurska, H. Dembinski, Emily Dvorak, L. Köpke, Alexander Fritz, D. Z. Besson, Chad Finley, G. Krückl, L. Schumacher, Carsten Rott, Tim Ruhe, Colin Turley, C. Alispach, Seongjin In, Gerald Przybylski, Elisa Resconi, T. Anderson, M. G. Aartsen, Janet Conrad, Federica Bradascio, Alexander Burgman, Pablo Correa, H. Niederhausen, K. Mase, Yuya Makino, R. Cross, Xianwu Xu, Christoph Tönnis, J. Sandroos, Mehmet Gunduz, Johannes Werthebach, M. S. Sutherland, A. Ishihara, R. C. Bay, M. J. Weiss, Kirill Filimonov, Austin Schneider, J. C. Gallagher, Juan Carlos Diaz-Velez, M. Usner, S. Kopper, M. Leuermann, Gerrit Wrede, Kael Hanson, René Reimann, William Luszczak, Allan Hallgren, M. Kauer, Martin Rongen, Pranav Dave, Samridha Kunwar, D. Altmann, K. Meagher, David Kappesser, L. Wille, S. E. Sanchez Herrera, Maximilian Meier, T. Palczewski, Paolo Desiati, M. Günder, D. Heereman, T. Stezelberger, A. Steuer, B. Eberhardt, Raamis Hussain, J. Lünemann, Amirreza Raissi, Chris Weaver, Stephanie Bron, C. J. Lozano Mariscal, G. Merino, N. Wandkowsky, Surujhdeo Seunarine, R. Snihur, Juanan Aguilar, B. J. Whelan, Immacolata Carmen Rea, K. Krings, Jan Weldert, L. Halve, Philipp Eller, M. Plum, Ramesh Koirala, E. Blaufuss, J. Felde, Merlin Schaufel, L. Classen, A. Obertacke Pollmann, A. Wallace, J. L. Kelley, Da Xu, Markus Ahlers, James DeLaunay, Marjon Moulai, S. De Ridder, Christopher Wiebusch, Kunal Deoskar, M. Labare, A. Karle, Erik Ganster, Ioana Codrina Maris, Christian Bohm, Samvel Ter-Antonyan, Christoph Raab, Nadège Iovine, D. Berley, G. C. Hill, Bunheng Ty, Maryon Ahrens, Giovanni Renzi, D. Seckel, Frederik Tenholt, S. Fahey, R. Nagai, M. Medici, S. Miarecki, Tyce DeYoung, Nathan Whitehorn, Jeffrey Lazar, Physics, Faculty of Sciences and Bioengineering Sciences, Vriendenkring VUB, and Elementary Particle Physics
Subjects: background [atmosphere], Physics::Instrumentation and Detectors, media_common.quotation_subject, Astrophysics::High Energy Astrophysical Phenomena, pole, FOS: Physical sciences, 01 natural sciences, High Energy Physics - Experiment, IceCube Neutrino Observatory, IceCube, charged current, High Energy Physics - Experiment (hep-ex), Neutrinos, Point sources, Veto techniques, SEARCH, TRACK RECONSTRUCTION, 0103 physical sciences, supernova, Muon neutrino, atmosphere [muon], 010303 astronomy & astrophysics, Astrophysics::Galaxy Astrophysics, media_common, High Energy Astrophysical Phenomena (astro-ph.HE), Physics, neutrino muon, Muon, 010308 nuclear & particles physics, ICE, Galactic Center, High Energy Physics::Phenomenology, Astronomy, Astronomy and Astrophysics, flux [neutrino], Galactic plane, observatory, Supernova, Physics and Astronomy, Sky, energy [neutrino], gamma ray, ddc:540, spectral, High Energy Physics::Experiment, galaxy, Neutrino, Astrophysics - High Energy Astrophysical Phenomena
Abstract: Many Galactic sources of gamma rays, such as supernova remnants, are expected to produce neutrinos with a typical energy cutoff well below 100 TeV. For the IceCube Neutrino Observatory located at the South Pole, the southern sky, containing the inner part of the Galactic plane and the Galactic Center, is a particularly challenging region at these energies, because of the large background of atmospheric muons. In this paper, we present recent advancements in data selection strategies for track-like muon neutrino events with energies below 100 TeV from the southern sky. The strategies utilize the outer detector regions as veto and features of the signal pattern to reduce the background of atmospheric muons to a level which, for the first time, allows IceCube searching for point-like sources of neutrinos in the southern sky at energies between 100 GeV and several TeV in the muon neutrino charged current channel. No significant clustering of neutrinos above background expectation was observed in four years of data recorded with the completed IceCube detector. Upper limits on the neutrino flux for a number of spectral hypotheses are reported for a list of astrophysical objects in the southern hemisphere., 19 pages, 17 figures, 2 tables
Published: 2020
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52. Status and results from the CUORE experiment

Author: C. Bucci, T. D. Gutierrez, Silvia Capelli, Massimiliano Nastasi, C. Pira, L. Gironi, F. T. Avignone, X. G. Cao, S. Di Domizio, V. Dompè, L. Taffarello, Danielle Speller, L. Cappelli, Laura Cardani, H. Z. Huang, M. Pavan, M. A. Franceschi, B. K. Fujikawa, Stefano Pozzi, Carlo Ligi, C. Pagliarone, Y. Mei, Massimiliano Clemenza, Carlo Cosmelli, Stefano Dell'Oro, A. D’Addabbo, M. Vignati, Lindley Winslow, A. Campani, S. Zucchelli, G. Keppel, K. Wilson, Davide Chiesa, Claudio Gotti, R. G. Huang, M. Faverzani, Jonathan Ouellet, G. Bari, A. Branca, C. Brofferio, L. Ma, Deqing Fang, S. Pirro, C. Rusconi, N. Casali, A. Caminata, Ezio Previtali, S. Zimmermann, S. L. Wagaarachchi, S. Morganti, T. O'Donnell, B. Welliver, K. M. Heeger, G. Fantini, C. Nones, A. Puiu, V. Pettinacci, V. Sharma, D. D'Aguanno, J. Nikkel, N. Chott, Oliviero Cremonesi, Marco Pallavicini, G. Pessina, A. Giuliani, Yu. G. Kolomensky, Ke Han, Reina H. Maruyama, C. Rosenfeld, Stuart J. Freedman, P. Gorla, F. Ferroni, C. Tomei, C. J. Davis, L. Zanotti, Irene Nutini, Evelyn Ferri, Yu-Gang Ma, F. Terranova, N. Moggi, Samuele Sangiorgio, P. T. Surukuchi, A. Nucciotti, L. Pagnanini, C. Alduino, S. Copello, Paolo Carniti, Ettore Fiorini, V. Novati, Andrea Giachero, D. Q. Adams, K. Alfonso, L. Pattavina, N. D. Scielzo, L. Canonica, L. Marini, Vasundhara Singh, J. Johnston, B. Schmidt, B. S. Wang, O. Azzolini, I. Dafinei, M. Sakai, James R. Wilson, F. Bellini, Monica Sisti, R. J. Creswick, Giovanni Benato, Eric B. Norman, T. Napolitano, M. Biassoni, Campani, A, Adams, D, Alduino, C, Alfonso, K, Avignone, F, Azzolini, O, Bari, G, Bellini, F, Benato, G, Biassoni, M, Branca, A, Brofferio, C, Bucci, C, Caminata, A, Canonica, L, Cao, X, Capelli, S, Cappelli, L, Cardani, L, Carniti, P, Casali, N, Chiesa, D, Chott, N, Clemenza, M, Copello, S, Cosmelli, C, Cremonesi, O, Creswick, R, D'Addabbo, A, D'Aguanno, D, Dafinei, I, Davis, C, Dell'Oro, S, Di Domizio, S, Dompe, V, Fang, D, Fantini, G, Faverzani, M, Ferri, E, Ferroni, F, Fiorini, E, Franceschi, M, Freedman, S, Fujikawa, B, Giachero, A, Gironi, L, Giuliani, A, Gorla, P, Gotti, C, Gutierrez, T, Han, K, Heeger, K, Huang, R, Huang, H, Johnston, J, Keppel, G, Kolomensky, Y, Ligi, C, Ma, Y, Ma, L, Marini, L, Maruyama, R, Mei, Y, Moggi, N, Morganti, S, Napolitano, T, Nastasi, M, Nikkel, J, Nones, C, Norman, E, Novati, V, Nucciotti, A, Nutini, I, O'Donnell, T, Ouellet, J, Pagliarone, C, Pagnanini, L, Pallavicini, M, Pattavina, L, Pavan, M, Pessina, G, Pettinacci, V, Pira, C, Pirro, S, Pozzi, S, Previtali, E, Puiu, A, Rosenfeld, C, Rusconi, C, Sakai, M, Sangiorgio, S, Schmidt, B, Scielzo, N, Sharma, V, Singh, V, Sisti, M, Speller, D, Surukuchi, P, Taffarello, L, Terranova, F, Tomei, C, Vignati, M, Wagaarachchi, S, Wang, B, Welliver, B, Wilson, J, Wilson, K, Winslow, L, Zanotti, L, Zimmermann, S, Zucchelli, S, Centre de Sciences Nucléaires et de Sciences de la Matière (CSNSM), 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), Département de Physique des Particules (ex SPP) (DPhP), Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, CUORE, and Département de Physique des Particules (ex SPP) (DPP)
Subjects: Nuclear and High Energy Physics, data analysis method, background: model, [PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex], 01 natural sciences, Combinatorics, CUORE, double-beta decay: (0neutrino), bolometer, 0103 physical sciences, [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], Neutrinoless double beta decay, 010306 general physics, activity report, Physics, 010308 nuclear & particles physics, 29.90.+r, Astronomy and Astrophysics, Background model, Atomic and Molecular Physics, and Optics, tellurium: nuclide, data management, Two-neutrino double beta decay, background model, two-neutrino double beta decay, experimental results
Abstract: Author(s): Campani, A; Adams, DQ; Alduino, C; Alfonso, K; Avignone, FT; Azzolini, O; Bari, G; Bellini, F; Benato, G; Biassoni, M; Branca, A; Brofferio, C; Bucci, C; Caminata, A; Canonica, L; Cao, XG; Capelli, S; Cappelli, L; Cardani, L; Carniti, P; Casali, N; Chiesa, D; Chott, N; Clemenza, M; Copello, S; Cosmelli, C; Cremonesi, O; Creswick, RJ; D'Addabbo, A; D'Aguanno, D; Dafinei, I; Davis, CJ; Dell'oro, S; Di Domizio, S; Dompe, V; Fang, DQ; Fantini, G; Faverzani, M; Ferri, E; Ferroni, F; Fiorini, E; Franceschi, MA; Freedman, SJ; Fujikawa, BK; Giachero, A; Gironi, L; Giuliani, A; Gorla, P; Gotti, C; Gutierrez, TD; Han, K; Heeger, KM; Huang, RG; Huang, HZ; Johnston, J; Keppel, G; Kolomensky, YG; Ligi, C; Ma, YG; Ma, L; Marini, L; Maruyama, RH; Mei, Y; Moggi, N; Morganti, S; Napolitano, T; Nastasi, M; Nikkel, J; Nones, C; Norman, EB; Novati, V; Nucciotti, A; Nutini, I; O'Donnell, T; Ouellet, JL; Pagliarone, CE; Pagnanini, L; Pallavicini, M; Pattavina, L; Pavan, M; Pessina, G; Pettinacci, V; Pira, C; Pirro, S; Pozzi, S | Abstract: The Cryogenic Underground Observatory for Rare Events (CUORE) is a tonne-scale cryogenic experiment located at the Laboratori Nazionali del Gran Sasso that exploits bolometric technique to search for neutrinoless double beta decay (0νββ) of 130Te. The detector consists of a segmented array of 988 natural TeO2 cubic crystals arranged in a cylindrical compact structure of 19 towers. The detector construction was completed in August 2016 and data taking started in Spring 2017. In this work, we present a brief description of the bolometric technique for rare events search and the CUORE detector, then we concentrate on the data analysis results. In this respect, we focus on the procedure for data processing and on the first 0νββ results we obtained from a total TeO2 exposure of 86.3kg yr. Next, we illustrate the main background sources and the CUORE background model, from which we obtain the most precise measurement of 130Te 2νββ half-life to date. Finally, we discuss the improvements achieved with 2018 and 2019 detector optimization campaigns and the current perspectives of our experiment.
Published: 2020
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53. A search for solar axion induced signals with COSINE-100

Author: K. W. Kim, David Leonard, B. J. Park, Eunju Jeon, Hyun Su Lee, F. Mouton, E. Barbosa de Souza, Mitra Djamal, Hyangkyu Park, Moo Hyun Lee, J.H. Lee, Nam Young Kim, Liang Yang, W. A. Lynch, M. Kauer, Reina H. Maruyama, A. C. Ezeribe, H. W. Joo, G. H. Yu, R. L. C. Pitta, Sun-Whe Kim, J. H. Jo, H. Kim, Govinda Adhikari, K. A. Shin, Stephen L. Olsen, Joo Young Lee, Kangsoon Park, S. Choi, Hansoo Park, Carsten Rott, V. A. Kudryavtsev, Y.D. Kim, S. J. Ra, Woosik Kang, Insik Hahn, A. Scarff, Won Nam Kang, Yong Hamb Kim, H. J. Kim, Y. J. Ko, N. Carlin, C. Ha, G. S. Kim, W. G. Thompson, N. J. C. Spooner, P. Adhikari, and H. Prihtiadi
Subjects: Physics, Quantum chromodynamics, Coupling, Particle physics, COLISÕES DE ÍONS PESADOS RELATIVÍSTICOS, 010308 nuclear & particles physics, Dark matter, FOS: Physical sciences, Astronomy and Astrophysics, 01 natural sciences, High Energy Physics - Experiment, High Energy Physics - Experiment (hep-ex), 0103 physical sciences, Trigonometric functions, Limit (mathematics), Nuclear Experiment (nucl-ex), Astrophysics - Instrumentation and Methods for Astrophysics, Instrumentation and Methods for Astrophysics (astro-ph.IM), 010303 astronomy & astrophysics, Axion, Nuclear Experiment
Abstract: We present results from a search for solar axions with the COSINE-100 experiment. We find no evidence of solar axion events from a data-set of 6,303.9 kg$\cdot$days exposure and set a 90\,\% confidence level upper limit on the axion-electron coupling, $g_{ae}$, at 1.70~$\times$~$10^{-11}$ for an axion mass less than 1\,keV/c$^2$. This limit excludes QCD axions heavier than 0.59\,eV/c$^2$ in the DFSZ model and 168.1\,eV/c$^2$ in the KSVZ model., 7 pages, 8 figures
Published: 2020

54. P6012Active selexipag metabolite MRE-269 increases endothelin receptors in pulmonary artery smooth muscle cells

Author: Shunsuke Sakai, Masaki Ieda, and H Maruyama
Subjects: business.industry, Metabolite, Selexipag, Pharmacology, chemistry.chemical_compound, Smooth muscle, chemistry, medicine.artery, Pulmonary artery, cardiovascular system, medicine, Cardiology and Cardiovascular Medicine, business, Endothelin receptor
Abstract: Background The pathology of pulmonary arterial hypertension (PAH) indicates the abnormal outgrowth of pulmonary artery smooth muscle cells (PASMCs) of the media. Abundant expression of endothelin 1 (ET-1) is observed in vessels of PAH, and has been considered to play a pathogenic role. There are several endothelin receptors including ETA, ETB. Compared to ETA, ETB mRNA is less expressed in PASMCs from control individuals, and is reported to be increased in those from PAH patients. However, how ETB is involved in PAH remains unclear. Selexipag, a non-prostanoid IP receptor agonist, was recently authorized for treating PAH. Compared to selexipag, the active metabolite MRE-269 has a higher affinity for the IP receptor. Initial combination therapy come to be accepted as a standard strategy for this disease, although the interaction of each drug has not been discussed enough. Purpose To assess the effect of selexipag on ET-1 receptors in PASMCs. Methods We stimulated purchased human PASMCs and endothelial cells by MRE-269 (300 nM), ET-1 (100 nM) or combination of them in vitro. Quantitative PCR was performed to quantify mRNA expressions. Cell proliferation was assessed by CCK8 cell proliferation assay kit. BQ123, A192621, bosentan was used as blocker against ETA, ETB, or both, respectively. Results In PASMCs, MRE-269 increased ETA and ETB expressions 2- and 7-fold, respectively. On the other hand, it increased ETB 1.2-fold in pulmonary artery endothelial cells; ETA was not detected in those cells. After pretreatment by MRE-269, ET-1 accelerated the proliferation of PASMCs. A192621 and bosentan abrogated this proliferation. In contrast, BQ123 did not abrogate it. Conclusions In PASMCs, active selexipag metabolite MRE-269 increases ETB more strongly than ETA, resulting in accelerated cell proliferation by ET-1 predominantly via ETB. These data call for further study focused on the choice of ET-1 receptor antagonists in the case of combination therapy with selexipag.
Published: 2019
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55. The CUORE Detector and Results

Author: James R. Wilson, C. Rosenfeld, S. Morganti, N. D. Scielzo, Carlo Ligi, V. Dompè, A. D'Addabbo, A. Campani, P. Gorla, F. Ferroni, C. Tomei, Monica Sisti, S. Copello, S. L. Wagaarachchi, J. Nikkel, L. Zanotti, Paolo Carniti, C. Pira, M. Faverzani, N. Casali, N. Chott, Simone Capelli, C. J. Davis, Giovanni Benato, H. Z. Huang, G. Keppel, L. Gironi, Ettore Fiorini, F. Terranova, G. Fantini, C. Nones, A. Puiu, S. Zucchelli, V. Novati, Andrea Giachero, Massimiliano Clemenza, Carlo Cosmelli, F. T. Avignone, Irene Nutini, Yu. G. Kolomensky, Massimiliano Nastasi, L. Canonica, L. Marini, V. Pettinacci, K. Wilson, Eric B. Norman, T. O'Donnell, D. Q. Adams, Vasundhara Singh, Jonathan Ouellet, K. Alfonso, S. Di Domizio, J. Johnston, Claudio Gotti, G. Bari, Y. Mei, D. D'Aguanno, T. Napolitano, Evelyn Ferri, Laura Cardani, L. Taffarello, Stefano Dell'Oro, B. K. Fujikawa, Stefano Pozzi, F. Bellini, B. Schmidt, Y. G. Ma, Oliviero Cremonesi, M. Biassoni, Danielle Speller, B. S. Wang, Xi-Guang Cao, C. Brofferio, M. Vignati, M. Pavan, L. Pagnanini, K. M. Heeger, Davide Chiesa, O. Azzolini, N. Moggi, Marco Pallavicini, C. Rusconi, C. Bucci, T. D. Gutierrez, R. J. Creswick, Samuele Sangiorgio, Lindley Winslow, A. Giuliani, Ke Han, Reina H. Maruyama, I. Dafinei, M. Sakai, G. Pessina, Stuart J. Freedman, L. Pattavina, A. Nucciotti, C. Alduino, S. Zimmermann, S. Pirro, L. Ma, D. Q. Fang, A. Branca, M. A. Franceschi, R. G. Huang, L. Cappelli, C. Pagliarone, A. Caminata, Ezio Previtali, B. Welliver, Centre de Sciences Nucléaires et de Sciences de la Matière (CSNSM), 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), Département de Physique des Particules (ex SPP) (DPP), Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Nutini, I, Adams, D, Alduino, C, Alfonso, K, Avignone, F, Azzolini, O, Bari, G, Bellini, F, Benato, G, Biassoni, M, Branca, A, Brofferio, C, Bucci, C, Caminata, A, Campani, A, Canonica, L, Cao, X, Capelli, S, Cappelli, L, Cardani, L, Carniti, P, Casali, N, Chiesa, D, Chott, N, Clemenza, M, Copello, S, Cosmelli, C, Cremonesi, O, Creswick, R, D’Addabbo, A, D’Aguanno, D, Dafinei, I, Davis, C, Dell’Oro, S, Domizio, S, Dompè, V, Fang, D, Fantini, G, Faverzani, M, Ferri, E, Ferroni, F, Fiorini, E, Franceschi, M, Freedman, S, Fujikawa, B, Giachero, A, Gironi, L, Giuliani, A, Gorla, P, Gotti, C, Gutierrez, T, Han, K, Heeger, K, Huang, R, Huang, H, Johnston, J, Keppel, G, Kolomensky, Y, Ligi, C, Ma, Y, Ma, L, Marini, L, Maruyama, R, Mei, Y, Moggi, N, Morganti, S, Napolitano, T, Nastasi, M, Nikkel, J, Nones, C, Norman, E, Novati, V, Nucciotti, A, O’Donnell, T, Ouellet, J, Pagliarone, C, Pagnanini, L, Pallavicini, M, Pattavina, L, Pavan, M, Pessina, G, Pettinacci, V, Pira, C, Pirro, S, Pozzi, S, Previtali, E, Puiu, A, Rosenfeld, C, Rusconi, C, Sakai, M, Sangiorgio, S, Schmidt, B, Scielzo, N, Singh, V, Sisti, M, Speller, D, Taffarello, L, Terranova, F, Tomei, C, Vignati, M, Wagaarachchi, S, Wang, B, Welliver, B, Wilson, J, Wilson, K, Winslow, L, Zanotti, L, Zimmermann, S, Zucchelli, S, Nutini I., Adams D.Q., Alduino C., Alfonso K., Avignone F.T., Azzolini O., Bari G., Bellini F., Benato G., Biassoni M., Branca A., Brofferio C., Bucci C., Caminata A., Campani A., Canonica L., Cao X.G., Capelli S., Cappelli L., Cardani L., Carniti P., Casali N., Chiesa D., Chott N., Clemenza M., Copello S., Cosmelli C., Cremonesi O., Creswick R.J., D'Addabbo A., D'Aguanno D., Dafinei I., Davis C.J., Dell'Oro S., Domizio S.D., Dompe V., Fang D.Q., Fantini G., Faverzani M., Ferri E., Ferroni F., Fiorini E., Franceschi M.A., Freedman S.J., Fujikawa B.K., Giachero A., Gironi L., Giuliani A., Gorla P., Gotti C., Gutierrez T.D., Han K., Heeger K.M., Huang R.G., Huang H.Z., Johnston J., Keppel G., Kolomensky Y.G., Ligi C., Ma Y.G., Ma L., Marini L., Maruyama R.H., Mei Y., Moggi N., Morganti S., Napolitano T., Nastasi M., Nikkel J., Nones C., Norman E.B., Novati V., Nucciotti A., O'Donnell T., Ouellet J.L., Pagliarone C.E., Pagnanini L., Pallavicini M., Pattavina L., Pavan M., Pessina G., Pettinacci V., Pira C., Pirro S., Pozzi S., Previtali E., Puiu A., Rosenfeld C., Rusconi C., Sakai M., Sangiorgio S., Schmidt B., Scielzo N.D., Singh V., Sisti M., Speller D., Taffarello L., Terranova F., Tomei C., Vignati M., Wagaarachchi S.L., Wang B.S., Welliver B., Wilson J., Wilson K., Winslow L.A., Zanotti L., Zimmermann S., Zucchelli S., and Département de Physique des Particules (ex SPP) (DPhP)
Subjects: Particle physics, 0 νββ, Cryogenics, CUORE, Macro-calorimeters, Neutrinos, Physics::Instrumentation and Detectors, Cryogenic, 01 natural sciences, tellurium: oxygen, 010305 fluids & plasmas, crystal, double-beta decay: (0neutrino), Double beta decay, 0103 physical sciences, Neutrino, [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex], General Materials Science, Beta (velocity), [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], 010306 general physics, activity report, detector: design, Physics, 0νββ, 0 nu beta beta, Detector, Astrophysics::Instrumentation and Methods for Astrophysics, Condensed Matter Physics, Atomic and Molecular Physics, and Optics, High Energy Physics::Experiment, tellurium: nuclide, Macro-calorimeter, experimental results
Abstract: The cryogenic underground observatory for rare events (CUORE) is a cryogenic experiment searching for neutrinoless double beta decay ($$0\nu \beta \beta$$0νββ) of $${^{130}\hbox {Te}}$$130Te. The detector consists of an array of $$988\,{\hbox {TeO}_{2}}$$988TeO2 crystals arranged in a compact cylindrical structure of 19 towers. We report the CUORE initial operations and optimization campaigns. We then present the CUORE results on $$0\nu \beta \beta$$0νββ and $$2\nu \beta \beta$$2νββ decay of $${^{130}\hbox {Te}}$$130Te obtained from the analysis of the physics data acquired in 2017.
Published: 2019
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56. Comparison between DAMA/LIBRA and COSINE-100 in the light of Quenching Factors

Author: H. Prihtiadi, S. J. Ra, B. B. Manzato, C. Ha, Y. J. Ko, Carsten Rott, N. J. C. Spooner, K. A. Shin, Stephen L. Olsen, S. Choi, R. L. C. Pitta, P. Adhikari, S. K. Kim, Y.D. Kim, Hansoo Park, K. W. Kim, M. Kauer, R. J. Neal, N. Carlin, A. C. Ezeribe, J. H. Jo, Hyun Su Lee, E. Barbosa de Souza, W. G. Thompson, Mitra Djamal, Woosik Kang, J.J. Choi, Insik Hahn, Kangsoon Park, David Leonard, G. H. Yu, J.H. Lee, G. S. Kim, H. Kim, Hyangkyu Park, Moo Hyun Lee, E.K. Lee, Govinda Adhikari, B. J. Park, Eunju Jeon, Nam Young Kim, W. A. Lynch, Joo Young Lee, Liang Yang, S.H. Lee, Reina H. Maruyama, A. Scarff, Yong Hamb Kim, and H. J. Kim
Subjects: DAMA/LIBRA, Physics - Instrumentation and Detectors, Physics::Instrumentation and Detectors, Dark matter, FOS: Physical sciences, Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, 01 natural sciences, High Energy Physics - Experiment, Galactic halo, High Energy Physics - Experiment (hep-ex), High Energy Physics - Phenomenology (hep-ph), WIMP, 0103 physical sciences, 010306 general physics, Instrumentation and Methods for Astrophysics (astro-ph.IM), Physics, 010308 nuclear & particles physics, Scattering, Astrophysics::Instrumentation and Methods for Astrophysics, Astronomy and Astrophysics, Instrumentation and Detectors (physics.ins-det), Galaxy, Dark matter halo, High Energy Physics - Phenomenology, Weakly interacting massive particles, Astrophysics - Instrumentation and Methods for Astrophysics
Abstract: There is a long standing debate about whether or not the annual modulation signal reported by the DAMA/LIBRA collaboration is induced by Weakly Interacting Massive Particles~(WIMP) in the galaxy's dark matter halo scattering from nuclides in their NaI(Tl) crystal target/detector. This is because regions of WIMP-mass vs. WIMP-nucleon cross-section parameter space that can accommodate the DAMA/LIBRA-phase1 modulation signal in the context of the standard WIMP dark matter galactic halo and isospin-conserving~(canonical), spin-independent~(SI) WIMP-nucleon interactions have been excluded by many of other dark matter search experiments including COSINE-100, which uses the same NaI(Tl) target/detector material. Moreover, the recently released DAMA/LIBRA-phase2 results are inconsistent with an interpretation as WIMP-nuclide scattering via the canonical SI interaction and prefer, instead, isospin-violating or spin-dependent interactions. Dark matter interpretations of the DAMA/LIBRA signal are sensitive to the NaI(Tl) scintillation efficiency for nuclear recoils, which is characterized by so-called quenching factors~(QF), and the QF values used in previous studies differ significantly from recently reported measurements, which may have led to incorrect interpretations of the DAMA/LIBRA signal. In this article, the compatibility of the DAMA/LIBRA and COSINE-100 results, in light of the new QF measurements is examined for different possible types of WIMP-nucleon interactions. The resulting allowed parameter space regions associated with the DAMA/LIBRA signal are explicitly compared with 90\% confidence level upper limits from the initial 59.5~day COSINE-100 exposure. With the newly measured QF values, the allowed 3$\sigma$ regions from the DAMA/LIBRA data are still generally excluded by the COSINE-100 data., Comment: Accepted in JCAP
Published: 2019

57. An experiment to search for dark matter interactions using sodium iodide detectors

Author: Moo Hyun Lee, Y. J. Ko, Carsten Rott, J.S. Park, Sun Kee Kim, Walter C. Pettus, N. Carlin, S. J. Ra, Woosik Kang, K. A. Shin, Stephen L. Olsen, V. A. Kudryavtsev, S.H. Yong, W. G. Thompson, B. C. Kim, Hyang Kyu Park, M. Kauer, F. Mouton, H. Prihtiadi, Woon Gu Kang, Yeongduk Kim, Yong-Hamb Kim, C. Ha, N. J. C. Spooner, Insik Hahn, B. J. Park, H. W. Joo, Seonho Choi, P. Adhikari, Estella Barbosa de Souza, Eunju Jeon, A. C. Ezeribe, Liang Yang, H. Kim, A. J. F. Hubbard, Govinda Adhikari, Joo Young Lee, Nam Young Kim, Hyeonseo Park, Reina H. Maruyama, W. A. Lynch, A. Scarff, D. S. Leonard, J. H. Jo, K. W. Kim, Jongmin Lee, Hongjoo Kim, Hyun Su Lee, Kangsoon Park, and Mitra Djamal
Subjects: Cosmology and Nongalactic Astrophysics (astro-ph.CO), Multidisciplinary, 010308 nuclear & particles physics, Dark matter, FOS: Physical sciences, Elementary particle, Astrophysics, 01 natural sciences, Galaxy, 3. Good health, High Energy Physics - Experiment, Dark matter halo, High Energy Physics - Experiment (hep-ex), Recoil, Weakly interacting massive particles, 0103 physical sciences, Orbital motion, Halo, 010306 general physics, Astrophysics - Instrumentation and Methods for Astrophysics, Instrumentation and Methods for Astrophysics (astro-ph.IM), Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: Observations of galaxies and primordial radiation suggest that the Universe is made mostly of non-luminous dark matter. Several types of new fundamental particles have been proposed as candidates for dark matter such as weakly interacting massive particles (WIMPs) but no definitive signal has been seen despite concerted efforts by many collaborations. One exception is the much-debated claim by the DAMA collaboration of a statistically significant annual modulation in the event rate of their experiment with a period and phase consistent with that expected from WIMP dark matter. Several groups have been working to develop experiments with the aim of reproducing DAMA's results using the same target medium. Here we report results from the initial operation of the COSINE-100 experiment. COSINE-100 uses sodium iodide as the target medium-the same medium as DAMA-and is designed to carry out a model-independent test of DAMA's claim. Initial data based on the first 59.5 days indicate that there is no excess of events over the expected background, confirming that DAMA's annual modulation signal is in severe tension with results from other experiments under the assumption of dark matter having spin independent interactions and the Standard Halo Model. COSINE-100 is now taking data to study the presence of dark matter-induced annual modulation in the event rate of the sodium iodide detectors., 26 pages, 9 figures
Published: 2019

58. Measurement of the cosmic ray energy spectrum with IceTop-73

Author: J. Blumenthal, D. L. Xu, J. Kiryluk, K. Clark, N. Van Eijndhoven, Rasha Abbasi, C. Finley, T. Fuchs, D. Soldin, T. Schmidt, M. Zoll, Stephanie Hickford, K. Jero, M. Labare, Sofia Vallecorsa, K. Hoshina, Segev BenZvi, G. Tešić, S. Schöneberg, E. Unger, D. Heinen, S. Ter-Antonyan, J. P. Rodrigues, M. Wallraff, X. W. Xu, J. Daughhetee, B. Ruzybayev, A. Tamburro, Hermann Kolanoski, Subir Sarkar, Olga Botner, Y. Sestayo, M. Ribordy, Markus Ahlers, D. Heereman, M. Wolf, J. Feintzeig, O. Schulz, G. S. Japaridze, Chun Xu, C. Pfendner, A. Haj Ismail, C. De Clercq, L. Rädel, A. Groß, A. Schukraft, D. J. Boersma, S. Cohen, A. Schönwald, M. Vehring, G. C. Hill, K. Wiebe, J. Van Santen, G. Golup, L. Paul, P. O. Hulth, Kael Hanson, L. Köpke, M. Krasberg, K. D. de Vries, A. Obertacke, K. D. Hoffman, H. Taavola, S. Hussain, D. Bose, S. R. Klein, G. M. Spiczak, H. Landsman, M. Rameez, K. H. Becker, C. Sheremata, Steven W. Barwick, M. G. Aartsen, J. Leute, M. L. Benabderrahmane, P. A. Evenson, K. Rawlins, J. Miller, A. M. Brown, K. Hultqvist, A. Christov, S. Böser, C. Walck, A. Fedynitch, K. Jagielski, L. Gerhardt, D. Grant, C. Wendt, S. Zierke, M. Usner, R. G. Stokstad, K. Krings, J. L. Kelley, L. Gladstone, J. A. Goodman, Tyce DeYoung, T. Feusels, R. Eagan, A. H. Cruz Silva, Carsten Rott, H. Wissing, S. Flis, B. Kaminsky, C. Bohm, M. Wellons, Dariusz Gora, Juanan Aguilar, P. Redl, J. Becker Tjus, T. Stezelberger, P. B. Price, B. Riedel, R. Bruijn, L. Brayeur, H. Niederhausen, G. W. Sullivan, C. Pérez De Los Heros, A. Goldschmidt, J. G. Gonzalez, E. Pinat, P. Zarzhitsky, Thomas Meures, Teresa Montaruli, G. Kroll, T. Salameh, D. F. Cowen, J. Lünemann, Marcos Santander, X. Bai, G. T. Przybylski, D. R. Nygren, J. Auffenberg, K. Mase, Wolfgang Rhode, S. Kopper, W. Huelsnitz, U. Naumann, R. Hellauer, H. S. Matis, S. Yoshida, D. Bindig, J. Kläs, P. Berghaus, Elisa Bernardini, M. Lesiak-Bzdak, T. Fischer-Wasels, R. Reimann, A. Karle, D. J. Koskinen, S. C. Nowicki, T. Kuwabara, A. Stasik, Francis Halzen, Jenni Adams, R. W. Ellsworth, M. Baker, T. Glüsenkamp, M. Vraeghe, E. Blaufuss, N. Kurahashi, R. C. Bay, J. Casey, I. Taboada, D. R. Williams, M. Dunkman, C. Kopper, J. Jacobsen, G. Binder, D. Chirkin, Rezo Shanidze, J. J. Beatty, S. Coenders, D. Pieloth, Alexander Kappes, L. Schulte, K. Schatto, A. Homeier, M. Bissok, D. Ryckbosch, H. P. Bretz, M. W.E. Smith, A. Stößl, J. Madsen, S. Bechet, Reina H. Maruyama, P. A. Toale, K. Woschnagg, F. Clevermann, D. Z. Besson, G. Yodh, T. Ruhe, S. De Ridder, J. H. Köhne, O. Fadiran, B. Eberhardt, B. Christy, J. Ziemann, M. J. Larson, R. Nahnhauer, M. J. Carson, A. R. Fazely, T. Waldenmaier, N. Whitehorn, S. Toscano, A. Olivas, S. Schoenen, M. Richman, Y. Abdou, M. Casier, D. Seckel, D. Bertrand, J. Eisch, S. Odrowski, K. Helbing, O. Jlelati, A. Bernhard, A. Tepe, J. Kunnen, M. Leuermann, F. McNally, R. Ström, V. Baum, J. S. Gallagher, M. Merck, E. Jacobi, Jürgen Brunner, L. Mohrmann, T. Karg, C. H. Wiebusch, Allan Hallgren, A. Ishihara, G. Kohnen, R. Hoffmann, Christian Spiering, S. Tilav, D. Berley, S. M. Saba, J. Posselt, Elisa Resconi, J. C. Davis, T. R. Wood, A. Omairat, P. Hallen, M. Voge, M. Danninger, M. Stamatikos, D. Altmann, E. A. Strahler, J. P. Yanez, P. Desiati, S. Westerhoff, C. Ha, E. Middell, Todor Stanev, J. A. Pepper, O. Macíias, H. G. Sander, Thomas K. Gaisser, S. Euler, S. Seunarine, Giorgio Maggi, Ch Weaver, M. Kowalski, A. Franckowiak, Markus Ackermann, S. Bohaichuk, K. Meagher, K. Filimonov, A. O'Murchadha, N. Milke, R. Morse, A. Van Overloop, K. Frantzen, F. Scheriau, M. Schmitz, S. Miarecki, J. C. Díaz-Vélez, D. T. Grandmont, Physics, Elementary Particle Physics, Aguilar Sanchez, Juan, Christov, Asen, Montaruli, Teresa, Rameez, Mohamed, and Vallecorsa, Sofia
Subjects: High Energy Astrophysical Phenomena (astro-ph.HE), Physics, Nuclear and High Energy Physics, 010308 nuclear & particles physics, FOS: Physical sciences, Astronomy, Cosmic ray, ddc:500.2, Astrophysics, 01 natural sciences, Power law, ICECUBE, IceCube, IceCube Neutrino Observatory, Air shower, Physics and Astronomy, Observatory, 0103 physical sciences, Energy spectrum, ARRAY, ddc:530, Astrophysics - High Energy Astrophysical Phenomena, 010306 general physics, physics
Abstract: Physical review / D 88(4), 042004 (2013). doi:10.1103/PhysRevD.88.042004, We report on the measurement of the all-particle cosmic ray energy spectrum with the IceTop air shower array in the energy range from 1.58 PeV to 1.26 EeV. The IceTop air shower array is the surface component of the IceCube Neutrino Observatory at the geographical South Pole. The analysis was performed using only information from IceTop. The data used in this work were taken from June 1, 2010 to May 13, 2011. During that period the IceTop array consisted of 73 stations, compared to 81 in its final configuration. The measured spectrum exhibits a clear deviation from a single power law above the knee around 4 PeV and below 1 EeV. We observe spectral hardening around 18 PeV and steepening around 130 PeV., Published by Soc., [S.l.]
Published: 2019
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59. COSINE-100 and DAMA/LIBRA-phase2 in WIMP effective models

Author: N. J. C. Spooner, H. W. Joo, P. Adhikari, Woon Gu Kang, F. Mouton, K. W. Kim, N. Carlin, Jongmin Lee, M. Kauer, David Leonard, B. J. Park, Insik Hahn, H. Prihtiadi, Gaurav Tomar, Carsten Rott, Liang Yang, E. Barbosa de Souza, Won Nam Kang, G. S. Kim, A. C. Ezeribe, Stefano Scopel, A. Scarff, Y.D. Kim, K. A. Shin, V. A. Kudryavtsev, Stephen L. Olsen, R. L. C. Pitta, Yong Hamb Kim, W. G. Thompson, H. J. Kim, N.Y. Kim, W. A. Lynch, G. H. Yu, Govinda Adhikari, H. Kim, Reina H. Maruyama, Sunghyun Kang, Hansoo Park, Y. J. Ko, C. Ha, Hyangkyu Park, Moo Hyun Lee, S. K. Kim, Eunju Jeon, Joo Young Lee, Kangsoon Park, S. Choi, J. H. Jo, Jong-Hyun Yoon, S. J. Ra, Hyun Su Lee, Mitra Djamal, Veterinary Biosciences, and Department of Physics
Subjects: DAMA/LIBRA, Particle physics, Cosmology and Nongalactic Astrophysics (astro-ph.CO), Physics beyond the Standard Model, Dark matter, FOS: Physical sciences, Elementary particle, 01 natural sciences, Upper and lower bounds, High Energy Physics - Experiment, High Energy Physics - Experiment (hep-ex), High Energy Physics - Phenomenology (hep-ph), WIMP, 0103 physical sciences, Effective field theory, MODULATION, Instrumentation and Methods for Astrophysics (astro-ph.IM), Physics, dark matter theory, 010308 nuclear & particles physics, dark matter experiments, Astrophysics::Instrumentation and Methods for Astrophysics, Astronomy and Astrophysics, 115 Astronomy, Space science, 3. Good health, Mathematical Operators, High Energy Physics - Phenomenology, Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: Assuming a standard Maxwellian for the WIMP velocity distribution, we obtain the bounds from null WIMP search results of 59.5 days of COSINE-100 data on the DAMA/LIBRA-phase2 modulation effect within the context of the non-relativistic effective theory of WIMP-nucleus scattering. Here, we systematically assume that one of the effective operators allowed by Galilean invariance dominates in the effective Hamiltonian of a spin-1/2 dark matter (DM) particle. We find that, although DAMA/LIBRA and COSINE-100 use the same sodium-iodide target, the comparison of the two results still depends on the particle-physics model. This is mainly due to two reasons: i) the WIMP signal spectral shape; ii) the expected modulation fractions, when the upper bound on the time-averaged rate in COSINE-100 is converted into a constraint on the annual modulation component in DAMA/LIBRA. We find that the latter effect is the dominant one. For several effective operators the expected modulation fractions are larger than in the standard spin-independent or spin-dependent interaction cases. As a consequence, compatibility between the modulation effect observed in DAMA/LIBRA and the null result from COSINE-100 is still possible for several non-relativistic operators. At low WIMP masses such relatively high values of the modulation fractions arise because COSINE-100 is mainly sensitive to WIMP-sodium scattering events, due to the higher threshold compared to DAMA/LIBRA. A next COSINE analysis is expected to have a full sensitivity for the 5$\sigma$ region of DAMA/LIBRA., Comment: 22 pages, 6 figures, 5 tables. Updated to published version
Published: 2019

60. Results from the CUORE experiment

Author: Adams, D, Alduino, C, Alfonso, K, Avignone III, F, Azzolini, O, Bari, G, Bellini, F, Benato, G, Biassoni, M, Branca, A, Brofferio, C, Bucci, C, Camilleri, J, Caminata, A, Campani, A, Canonica, L, Cao, X, Capelli, S, Cappelli, L, Cardani, L, Carniti, P, Casali, N, Chiesa, D, Clemenza, M, Copello, S, Cosmelli, C, Cremonesi, O, Creswick, R, D'Addabbo, A, D'Aguanno, D, Dafinei, I, Davis, C, Del Corso, F, Dell'Oro, S, Di Domizio, S, Dompè, V, Fang, D, Fantini, G, Faverzani, M, Ferri, E, Ferroni, F, Fiorini, E, Franceschi, M, Freedman, S, Fujikawa, B, Giachero, A, Gironi, L, Giuliani, A, Gorla, P, Gotti, C, Gutierrez, T, Han, K, Heeger, K, Huang, R, Huang, H, Johnston, J, Keppel, G, Kolomensky, Y, Ligi, C, Ma, L, Ma, Y, Marini, L, Maruyama, R, Mei, Y, Moggi, N, Morganti, S, Napolitano, T, Nastasi, M, Nikkel, J, Nones, C, Norman, E, Novati, V, Nucciotti, A, Nutini, I, O'Donnell, T, Ouellet, J, Pagliarone, C, Pagnanini, L, Pallavicini, M, Pattavina, L, Pavan, M, Pessina, G, Pettinacci, V, Pira, C, Pirro, S, Pozzi, S, Previtali, E, Puiu, A, Rosenfeld, C, Rusconi, C, Sakai, M, Sangiorgio, S, Schmidt, B, Scielzo, N, Singh, V, Sisti, M, Speller, D, Taffarello, L, Terranova, F, Tomei, C, Vignati, M, Wagaarachchi, S, Wang, B, Welliver, B, Wilson, J, Wilson, K, Winslow, L, Zanotti, L, Zimmermann, S, Zucchelli, S, D. Q. Adams, C. Alduino, K. Alfonso, F. T. Avignone III, O. Azzolini, G. Bari, F. Bellini, G. Benato, M. Biassoni, A. Branca, C. Brofferio, C. Bucci, J. Camilleri, A. Caminata, A. Campani, L. Canonica, X. G. Cao, S. Capelli, L. Cappelli, L. Cardani, P. Carniti, N. Casali, D. Chiesa, M. Clemenza, S. Copello, C. Cosmelli, O. Cremonesi, R. J. Creswick, A. D'Addabbo, D. D'Aguanno, I. Dafinei, C. J. Davis, F. Del Corso, S. Dell'Oro, S. Di Domizio, V. Dompè, D. Q. Fang, G. Fantini, M. Faverzani, E. Ferri, F. Ferroni, E. Fiorini, M. A. Franceschi, S. J. Freedman, B. K. Fujikawa, A. Giachero, L. Gironi, A. Giuliani, P. Gorla, C. Gotti, T. D. Gutierrez, K. Han, K. M. Heeger, R. G. Huang, H. Z. Huang, J. Johnston, G. Keppel, Yu. G. Kolomensky, C. Ligi, L. Ma, Y. G. Ma, L. Marini, R. H. Maruyama, Y. Mei, N. Moggi, S. Morganti, T. Napolitano, M. Nastasi, J. Nikkel, C. Nones, E. B. Norman, V. Novati, A. Nucciotti, I. Nutini, T. O'Donnell, J. L. Ouellet, C. E. Pagliarone, L. Pagnanini, M. Pallavicini, L. Pattavina, M. Pavan, G. Pessina, V. Pettinacci, C. Pira, S. Pirro, S. Pozzi, E. Previtali, A. Puiu, C. Rosenfeld, C. Rusconi, M. Sakai, S. Sangiorgio, B. Schmidt, N. D. Scielzo, V. Singh, M. Sisti, D. Speller, L. Taffarello, F. Terranova, C. Tomei, M. Vignati, S. L. Wagaarachchi, B. S. Wang, B. Welliver, J. Wilson, K. Wilson, L. A. Winslow, L. Zanotti, S. Zimmermann, S. Zucchelli, Adams, D, Alduino, C, Alfonso, K, Avignone III, F, Azzolini, O, Bari, G, Bellini, F, Benato, G, Biassoni, M, Branca, A, Brofferio, C, Bucci, C, Camilleri, J, Caminata, A, Campani, A, Canonica, L, Cao, X, Capelli, S, Cappelli, L, Cardani, L, Carniti, P, Casali, N, Chiesa, D, Clemenza, M, Copello, S, Cosmelli, C, Cremonesi, O, Creswick, R, D'Addabbo, A, D'Aguanno, D, Dafinei, I, Davis, C, Del Corso, F, Dell'Oro, S, Di Domizio, S, Dompè, V, Fang, D, Fantini, G, Faverzani, M, Ferri, E, Ferroni, F, Fiorini, E, Franceschi, M, Freedman, S, Fujikawa, B, Giachero, A, Gironi, L, Giuliani, A, Gorla, P, Gotti, C, Gutierrez, T, Han, K, Heeger, K, Huang, R, Huang, H, Johnston, J, Keppel, G, Kolomensky, Y, Ligi, C, Ma, L, Ma, Y, Marini, L, Maruyama, R, Mei, Y, Moggi, N, Morganti, S, Napolitano, T, Nastasi, M, Nikkel, J, Nones, C, Norman, E, Novati, V, Nucciotti, A, Nutini, I, O'Donnell, T, Ouellet, J, Pagliarone, C, Pagnanini, L, Pallavicini, M, Pattavina, L, Pavan, M, Pessina, G, Pettinacci, V, Pira, C, Pirro, S, Pozzi, S, Previtali, E, Puiu, A, Rosenfeld, C, Rusconi, C, Sakai, M, Sangiorgio, S, Schmidt, B, Scielzo, N, Singh, V, Sisti, M, Speller, D, Taffarello, L, Terranova, F, Tomei, C, Vignati, M, Wagaarachchi, S, Wang, B, Welliver, B, Wilson, J, Wilson, K, Winslow, L, Zanotti, L, Zimmermann, S, Zucchelli, S, D. Q. Adams, C. Alduino, K. Alfonso, F. T. Avignone III, O. Azzolini, G. Bari, F. Bellini, G. Benato, M. Biassoni, A. Branca, C. Brofferio, C. Bucci, J. Camilleri, A. Caminata, A. Campani, L. Canonica, X. G. Cao, S. Capelli, L. Cappelli, L. Cardani, P. Carniti, N. Casali, D. Chiesa, M. Clemenza, S. Copello, C. Cosmelli, O. Cremonesi, R. J. Creswick, A. D'Addabbo, D. D'Aguanno, I. Dafinei, C. J. Davis, F. Del Corso, S. Dell'Oro, S. Di Domizio, V. Dompè, D. Q. Fang, G. Fantini, M. Faverzani, E. Ferri, F. Ferroni, E. Fiorini, M. A. Franceschi, S. J. Freedman, B. K. Fujikawa, A. Giachero, L. Gironi, A. Giuliani, P. Gorla, C. Gotti, T. D. Gutierrez, K. Han, K. M. Heeger, R. G. Huang, H. Z. Huang, J. Johnston, G. Keppel, Yu. G. Kolomensky, C. Ligi, L. Ma, Y. G. Ma, L. Marini, R. H. Maruyama, Y. Mei, N. Moggi, S. Morganti, T. Napolitano, M. Nastasi, J. Nikkel, C. Nones, E. B. Norman, V. Novati, A. Nucciotti, I. Nutini, T. O'Donnell, J. L. Ouellet, C. E. Pagliarone, L. Pagnanini, M. Pallavicini, L. Pattavina, M. Pavan, G. Pessina, V. Pettinacci, C. Pira, S. Pirro, S. Pozzi, E. Previtali, A. Puiu, C. Rosenfeld, C. Rusconi, M. Sakai, S. Sangiorgio, B. Schmidt, N. D. Scielzo, V. Singh, M. Sisti, D. Speller, L. Taffarello, F. Terranova, C. Tomei, M. Vignati, S. L. Wagaarachchi, B. S. Wang, B. Welliver, J. Wilson, K. Wilson, L. A. Winslow, L. Zanotti, S. Zimmermann, and S. Zucchelli
Published: 2020

61. Performance of the low threshold Optimum Trigger on CUORE data

Author: Branca, A, Adams, D, Alduino, C, Alfonso, K, Avignone III, F, Azzolini, O, Bari, G, Bellini, F, Benato, G, Biassoni, M, Brofferio, C, Bucci, C, Camilleri, J, Caminata, A, Campani, A, Canonica, L, Cao, X, Capelli, S, Cappelli, L, Cardani, L, Carniti, P, Casali, N, Chiesa, D, Clemenza, M, Copello, S, Cosmelli, C, Cremonesi, O, Creswick, R, D'Addabbo, A, D'Aguanno, D, Dafinei, I, Davis, C, Del Corso, F, Dell'Oro, S, Di Domizio, S, Dompè, V, Fang, D, Fantini, G, Faverzani, M, Ferri, E, Ferroni, F, Fiorini, E, Franceschi, M, Freedman, S, Fujikawa, B, Giachero, A, Gironi, L, Giuliani, A, Gorla, P, Gotti, C, Gutierrez, T, Han, K, Heeger, K, Huang, R, Huang, H, Johnston, J, Keppel, G, Kolomensky, Y, Ligi, C, Ma, L, Ma, Y, Marini, L, Maruyama, R, Mei, Y, Moggi, N, Morganti, S, Napolitano, T, Nastasi, M, Nikkel, J, Nones, C, Norman, E, Novati, V, Nucciotti, A, Nutini, I, O'Donnell, T, Ouellet, J, Pagliarone, C, Pagnanini, L, Pallavicini, M, Pattavina, L, Pavan, M, Pessina, G, Pettinacci, V, Pira, C, Pirro, S, Pozzi, S, Previtali, E, Puiu, A, Rosenfeld, C, Rusconi, C, Sakai, M, Sangiorgio, S, Schmidt, B, Scielzo, N, Sharma, V, Singh, V, Sisti, M, Speller, D, Taffarello, L, Terranova, F, Tomei, C, Vignati, M, Wagaarachchi, S, Wang, B, Welliver, B, Wilson, J, Wilson, K, Winslow, L, Zanotti, L, Zimmermann, S, Zucchelli, S, A. Branca, D. Q. Adams, C. Alduino, K. Alfonso, F. T. Avignone III, O. Azzolini, G. Bari, F. Bellini, G. Benato, M. Biassoni, C. Brofferio, C. Bucci, J. Camilleri, A. Caminata, A. Campani, L. Canonica, X. G. Cao, S. Capelli, L. Cappelli, L. Cardani, P. Carniti, N. Casali, D. Chiesa, M. Clemenza, S. Copello, C. Cosmelli, O. Cremonesi, R. J. Creswick, A. D'Addabbo, D. D'Aguanno, I. Dafinei, C. J. Davis, F. Del Corso, S. Dell'Oro, S. Di Domizio, V. Dompè, D. Q. Fang, G. Fantini, M. Faverzani, E. Ferri, F. Ferroni, E. Fiorini, M. A. Franceschi, S. J. Freedman, B. K. Fujikawa, A. Giachero, L. Gironi, A. Giuliani, P. Gorla, C. Gotti, T. D. Gutierrez, K. Han, K. M. Heeger, R. G. Huang, H. Z. Huang, J. Johnston, G. Keppel, Yu. G. Kolomensky, C. Ligi, L. Ma, Y. G. Ma, L. Marini, R. H. Maruyama, Y. Mei, N. Moggi, S. Morganti, T. Napolitano, M. Nastasi, J. Nikkel, C. Nones, E. B. Norman, V. Novati, A. Nucciotti, I. Nutini, T. O'Donnell, J. L. Ouellet, C. E. Pagliarone, L. Pagnanini, M. Pallavicini, L. Pattavina, M. Pavan, G. Pessina, V. Pettinacci, C. Pira, S. Pirro, S. Pozzi, E. Previtali, A. Puiu, C. Rosenfeld, C. Rusconi, M. Sakai, S. Sangiorgio, B. Schmidt, N. D. Scielzo, V. Sharma, V. Singh, M. Sisti, D. Speller, L. Taffarello, F. Terranova, C. Tomei, M. Vignati, S. L. Wagaarachchi, B. S. Wang, B. Welliver, J. Wilson, K. Wilson, L. A. Winslow, L. Zanotti, S. Zimmermann, S. Zucchelli, Branca, A, Adams, D, Alduino, C, Alfonso, K, Avignone III, F, Azzolini, O, Bari, G, Bellini, F, Benato, G, Biassoni, M, Brofferio, C, Bucci, C, Camilleri, J, Caminata, A, Campani, A, Canonica, L, Cao, X, Capelli, S, Cappelli, L, Cardani, L, Carniti, P, Casali, N, Chiesa, D, Clemenza, M, Copello, S, Cosmelli, C, Cremonesi, O, Creswick, R, D'Addabbo, A, D'Aguanno, D, Dafinei, I, Davis, C, Del Corso, F, Dell'Oro, S, Di Domizio, S, Dompè, V, Fang, D, Fantini, G, Faverzani, M, Ferri, E, Ferroni, F, Fiorini, E, Franceschi, M, Freedman, S, Fujikawa, B, Giachero, A, Gironi, L, Giuliani, A, Gorla, P, Gotti, C, Gutierrez, T, Han, K, Heeger, K, Huang, R, Huang, H, Johnston, J, Keppel, G, Kolomensky, Y, Ligi, C, Ma, L, Ma, Y, Marini, L, Maruyama, R, Mei, Y, Moggi, N, Morganti, S, Napolitano, T, Nastasi, M, Nikkel, J, Nones, C, Norman, E, Novati, V, Nucciotti, A, Nutini, I, O'Donnell, T, Ouellet, J, Pagliarone, C, Pagnanini, L, Pallavicini, M, Pattavina, L, Pavan, M, Pessina, G, Pettinacci, V, Pira, C, Pirro, S, Pozzi, S, Previtali, E, Puiu, A, Rosenfeld, C, Rusconi, C, Sakai, M, Sangiorgio, S, Schmidt, B, Scielzo, N, Sharma, V, Singh, V, Sisti, M, Speller, D, Taffarello, L, Terranova, F, Tomei, C, Vignati, M, Wagaarachchi, S, Wang, B, Welliver, B, Wilson, J, Wilson, K, Winslow, L, Zanotti, L, Zimmermann, S, Zucchelli, S, A. Branca, D. Q. Adams, C. Alduino, K. Alfonso, F. T. Avignone III, O. Azzolini, G. Bari, F. Bellini, G. Benato, M. Biassoni, C. Brofferio, C. Bucci, J. Camilleri, A. Caminata, A. Campani, L. Canonica, X. G. Cao, S. Capelli, L. Cappelli, L. Cardani, P. Carniti, N. Casali, D. Chiesa, M. Clemenza, S. Copello, C. Cosmelli, O. Cremonesi, R. J. Creswick, A. D'Addabbo, D. D'Aguanno, I. Dafinei, C. J. Davis, F. Del Corso, S. Dell'Oro, S. Di Domizio, V. Dompè, D. Q. Fang, G. Fantini, M. Faverzani, E. Ferri, F. Ferroni, E. Fiorini, M. A. Franceschi, S. J. Freedman, B. K. Fujikawa, A. Giachero, L. Gironi, A. Giuliani, P. Gorla, C. Gotti, T. D. Gutierrez, K. Han, K. M. Heeger, R. G. Huang, H. Z. Huang, J. Johnston, G. Keppel, Yu. G. Kolomensky, C. Ligi, L. Ma, Y. G. Ma, L. Marini, R. H. Maruyama, Y. Mei, N. Moggi, S. Morganti, T. Napolitano, M. Nastasi, J. Nikkel, C. Nones, E. B. Norman, V. Novati, A. Nucciotti, I. Nutini, T. O'Donnell, J. L. Ouellet, C. E. Pagliarone, L. Pagnanini, M. Pallavicini, L. Pattavina, M. Pavan, G. Pessina, V. Pettinacci, C. Pira, S. Pirro, S. Pozzi, E. Previtali, A. Puiu, C. Rosenfeld, C. Rusconi, M. Sakai, S. Sangiorgio, B. Schmidt, N. D. Scielzo, V. Sharma, V. Singh, M. Sisti, D. Speller, L. Taffarello, F. Terranova, C. Tomei, M. Vignati, S. L. Wagaarachchi, B. S. Wang, B. Welliver, J. Wilson, K. Wilson, L. A. Winslow, L. Zanotti, S. Zimmermann, and S. Zucchelli
Abstract: The Optimum Trigger (OT) is based on a threshold algorithm applied on waveforms filtered by exploiting the matched filter technique. The OT trigger thresholds improve by 60-90% with respect to the thresholds obtained with the standard trigger, ranging between ∼ 20 and 100 keV . Low trigger thresholds open the way to Dark Matter searches and to improvements in the neutrinoless double beta decay analysis. Nevertheless, running the OT on CUORE data is demanding from the computational resources point of view. For this reason, the algorithm has been revised and adapted to cope with CUORE data. The work done to implement OT in CUORE and its performances will be discussed.
Published: 2020

62. Publisher Correction: Detection of a particle shower at the Glashow resonance with IceCube

Author: Jeffrey Lazar, George Japaridze, Roger Moore, M. Zöcklein, D. B. Fox, Timo Karg, Federica Bradascio, Alexander Burgman, S. Sarkar, J. Bourbeau, J. S. Gallagher, Richard Naab, Jan Soedingrekso, Merlin Schaufel, Seongjin In, J. A. Aguilar, Hermann Kolanoski, Elisa Resconi, M. Kauer, M. E. Huber, Marcos Santander, Le Viet Nguyen, D. Kang, Sarah Mancina, Stef Verpoest, Anna Franckowiak, Tobias Hoinka, Alexander Trettin, Aswathi Balagopal, L. Gerhardt, A. Porcelli, K. Krings, Vedant Basu, A. Schneider, Suyong Choi, G. Krückl, David Kappesser, Steve Sclafani, Alan Coleman, Gerrit Wrede, I. Taboada, Dustin Hebecker, Thomas Huber, B. J. P. Jones, A. Olivas, Frank G. Schröder, Ek Narayan Paudel, Allan Hallgren, Sandro Kopper, R. Maunu, Tim Ruhe, Matti Jansson, Thomas Ehrhardt, S. H. Robertson, Christian Haack, A. Kyriacou, C. S. Hill, B. J. Whelan, David Vannerom, Joanna Kiryluk, J. Auffenberg, K. Hoshina, Glenn Spiczak, Pablo Correa, B. A. Clark, G. Momenté, Shefali Shefali, K. Filimonov, D. F. Cowen, Martin Unland Elorrieta, S. De Ridder, A. Wallace, U. Naumann, A. Goldschmidt, Christoph Tönnis, T. Anderson, John Hardin, Mohamed Rameez, Abdul Rehman, Jan Weldert, E. Unger, L. Halve, Thorsten Glusenkamp, Carsten Rott, R. Hellauer, Y. Popovych, Joonghan Kim, Elisa Bernardini, K. Woschnagg, Z. Griffith, M. Kowalski, Etienne Bourbeau, Maria Prado Rodriguez, K. Rawlins, I. C. Mariş, A. O. Pollmann, Chiara Bellenghi, Daria Pankova, E. Friedman, Timothy W. Schmidt, D. Tosi, Chujie Chen, K. Tollefson, Max Renschler, D. J. Koskinen, Elisa Lohfink, Jenni Adams, Xinyue Kang, H. Schieler, Surujhdeo Seunarine, A. Weindl, Johan Wulff, Timothyblake Watson, J. Felde, K. Helbing, David R. Williams, P. Schlunder, Claudio Kopper, Maryon Ahrens, J. Buscher, Spencer Griswold, James DeLaunay, C. Bohm, C. Alispach, James Madsen, Frederik Tenholt, Raffaela Busse, M. Richman, Roxanne Turcotte, Benjamin Bastian, Anastasia Maria Barbano, Maria Tselengidou, Marjon Moulai, M. Medici, Xu X. W., Anatoli Fedynitch, C. H. Wiebusch, Simeon Reusch, Markus Ahlers, S. Hickford, Lu Lu, Cristina Lagunas Gualda, P. B. Price, Michael DuVernois, K. Meagher, T. Kittler, Paul Coppin, Andrea Turcati, C. Pérez de los Heros, Konstancja Satalecka, Theo Glauch, Francesco Lucarelli, S. Böser, Ramesh Koirala, R. G. Stokstad, Jannis Necker, Robert A. Cross, J. van Santen, K. D. de Vries, J. Stettner, Johannes Werthebach, L. Schumacher, A. Ishihara, C. De Clercq, N. L. Strotjohann, Karen Andeen, N. Kulacz, Gerald Przybylski, Michael J Larson, Teresa Montaruli, Felix Henningsen, T. R. Wood, E. Blaufuss, Alex Pizzuto, Michael Campana, Cristian Jesus Lozano Mariscal, Kendall Mahn, A. Steuer, Erik Ganster, T. Kintscher, Markus Ackermann, S. W. Barwick, Gerrit Roellinghoff, William Luszczak, Hershal Pandya, Alexander Fritz, Pranav Dave, A. R. Fazely, J. L. Kelley, Sebastian Sanchez Herrera, Benjamin Hokanson-Fasig, T. Stanev, Paul Evenson, L. Classen, N. Wandkowsky, Wolfgang Rhode, R. Morse, Jakob Bottcher, Mirco Hunnefeld, Marie Oehler, Julia Becker Tjus, Samvel Ter-Antonyan, Robert Stein, Hrvoje Dujmovic, Frederik Hermann Lauber, Yang Lyu, Stephen L. Hauser, S. Tilav, Grant Parker, G. H. Collin, Saskia Philippen, C. Wendt, Gary Binder, Simona Toscano, P. Heix, S. Y. BenZvi, Raamis Hussain, P. Muth, C. B. Finley, T. Stezelberger, A. Desai, Simone Garrappa, Feifei Huang, Dmitry Chirkin, Gisela Anton, Spencer Axani, Andrew Ludwig, A. Terliuk, G. de Wasseige, K. Wiebe, R. Hoffmann, Kayla Leonard, Alexander Kappes, G. Maggi, C. Walck, J. Lünemann, D. Z. Besson, Carlos Arguelles, Sukeerthi Dharani, Justin Lanfranchi, Francis Halzen, J. Merz, J. G. Gonzalez, Jessie Micallef, Ibrahim Safa, Damian Pieloth, M. U. Nisa, Thomas K. Gaisser, R. Engel, K.-H. Becker, Yiqian Xu, Matt Dunkman, R. Joppe, I. Ansseau, Christian Spiering, Aaron Fienberg, M. Silva, Najia Moureen Binte Amin, Juliana Stachurska, Lenka Tomankova, Amirreza Raissi, Mehmet Gunduz, Chris Weaver, Stephanie Bron, Justin Vandenbroucke, Frank McNally, Chunfai Tung, Colin Turley, Jannes Brostean-Kaiser, E. Cheung, Thomas Stuttard, M. Plum, Sarah Pieper, Maximilian Karl Scharf, A. Kheirandish, Dirk Ryckbosch, M. Stamatikos, Stephan Meighen-Berger, Joakim Sandroos, Y. L. Li, Devyn Rysewyk Cantu, Daniela Mockler, Agnieszka Leszczyńska, Martin Wolf, P. Peiffer, R. C. Bay, Joshua Hignight, Timo Sturwald, R. Halliday, Ben Smithers, Jean Pierre Twagirayezu, L. Köpke, A. Haungs, Nahee Park, K. Hultqvist, Darren Grant, Sarah Nowicki, Ryo Nagai, J. P. Yanez, H. Bagherpour, M. G. Aartsen, K. D. Hoffman, S. Baur, Olga Botner, V. Baum, G. W. Sullivan, James E. Braun, Juan Carlos Diaz-Velez, Erin O'Sullivan, Sreetama Goswami, F. Jonske, Ken'ichi Kin, J. J. Beatty, Tianlu Yuan, H. Dembinski, Reina H. Maruyama, Summer Blot, Naoko Kurahashi, Qinrui Liu, S. R. Klein, Martina Karl, Jochen M. Schneider, Martin Rongen, Zhedong Zhang, Ava Ghadimi, P. Mallik, Hans Niederhausen, K. Mase, Yuya Makino, Karl J. Clark, Alberto Martin Gago Medina, M. J. Weiss, René Reimann, Leander Fischer, D. van Eijk, Christoph Raab, Nadège Iovine, M. Song, D. Berley, G. C. Hill, T. L. Carver, Paras Koundal, Bunheng Ty, Woosik Kang, Kael Hanson, Moritz Kellermann, Giovanni Renzi, D. Seckel, S. Fahey, D. R. Nygren, Tyce DeYoung, Nathan Whitehorn, Immacolata Carmen Rea, Jan Conrad, Ma W. Y., Michael Kovacevich, X. Bai, G. Neer, A. Diaz, Robert Snihur, Philipp Eller, Alexander Sandrock, Kunal Deoskar, A. Karle, Rasha Abbasi, Maximilian Meier, Paolo Desiati, Matthias Vraeghe, Minjin Jeong, L. Rauch, D. Soldin, S. Yoshida, Daniel Bindig, N. van Eijndhoven, Timothée Grégoire, Emily Dvorak, M. Relich, Benedikt Riedel, and U. Katz
Subjects: Physics, Particle physics, Multidisciplinary, Particle shower, Glashow resonance
Published: 2021
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63. FSHD / OPMD / MYOTONIC DYSTROPHY

Author: T. Kurashige, H. Morino, H. Ueno, T. Murao, T. Watanabe, T. Hinoi, I. Nishino, H. Maruyama, and T. Torii
Subjects: Neurology, Pediatrics, Perinatology and Child Health, Neurology (clinical), Genetics (clinical)
Published: 2020
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64. CUORE: The first bolometric experiment at the ton scale for the search for neutrino-less double beta decay

Author: James R. Wilson, N. Moggi, Monica Sisti, Carlo Cosmelli, Samuele Sangiorgio, Lindley Winslow, Jeremy S. Cushman, C. Rosenfeld, A. Nucciotti, Claudio Gotti, C. Alduino, C. Bucci, T. D. Gutierrez, S. Copello, V. Pettinacci, P. Gorla, F. Ferroni, C. Tomei, C. Brofferio, M. Faverzani, Stefano Pirro, D. D'Aguanno, S. Morganti, Paolo Carniti, A. Giuliani, Davide Chiesa, C. Rusconi, C. J. Davis, I. Dafinei, M. Sakai, M. Pavan, S. Zucchelli, K. Wilson, Y. Mei, N. Chott, S. Di Domizio, L. Cappelli, Eric B. Norman, T. Napolitano, V. Dompè, Oliviero Cremonesi, Jonathan Ouellet, G. Bari, A. D'Addabbo, Stefano Dell'Oro, M. Clemenza, Laura Cardani, T. Wise, D. Q. Fang, B. K. Fujikawa, Vasundhara Singh, Stefano Pozzi, Xi-Guang Cao, H. Z. Huang, K. M. Heeger, G. Keppel, M. Biassoni, L. Taffarello, C. Pagliarone, S. Zimmermann, Marco Pallavicini, T. O'Donnell, A. Caminata, Carlo Ligi, Yu. G. Kolomensky, Ezio Previtali, G. Pessina, B. Schmidt, Danielle Speller, B. S. Wang, B. Welliver, M. Vignati, O. Azzolini, Irene Nutini, Ettore Fiorini, V. Novati, Andrea Giachero, A. Campani, C. Pira, L. Pattavina, A. Drobizhev, Silvia Capelli, C. Nones, A. Puiu, F. Terranova, Yu-Gang Ma, Massimiliano Nastasi, D. Q. Adams, K. Alfonso, N. Casali, Giovanni Benato, M. A. Franceschi, G. Fantini, A. Branca, R. G. Huang, Ke Han, Reina H. Maruyama, Stuart J. Freedman, S. L. Wagaarachchi, L. Gironi, F. T. Avignone, A. Bersani, R. J. Creswick, F. Bellini, A. Leder, N. D. Scielzo, L. Zanotti, L. Canonica, L. Marini, J. Johnston, Evelyn Ferri, Centre de Sciences Nucléaires et de Sciences de la Matière (CSNSM), 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), Département de Physique des Particules (ex SPP) (DPP), Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Adams D.Q., Alduino C., Alfonso K., Avignone F.T., Azzolini O., Bari G., Bellini F., Benato G., Bersani A., Biassoni M., Branca A., Brofferio C., Bucci C., Caminata A., Campani A., Canonica L., Cao X.G., Capelli S., Cappelli L., Cardani L., Carniti P., Casali N., Chiesa D., Chott N., Clemenza M., Copello S., Cosmelli C., Cremonesi O., Creswick R.J., Cushman J.S., D'Addabbo A., D'Aguanno D., Dafinei I., Davis C.J., Dell'Oro S., Di Domizio S., Dompe V., Drobizhev A., Fang D.Q., Fantini G., Faverzani M., Ferri E., Ferroni F., Fiorini E., Franceschi M.A., Freedman S.J., Fujikawa B.K., Giachero A., Gironi L., Giuliani A., Gorla P., Gotti C., Gutierrez T.D., Han K., Heeger K.M., Huang R.G., Huang H.Z., Johnston J., Keppel G., Kolomensky Y.G., Leder A., Ligi C., Ma Y.G., Marini L., Maruyama R.H., Mei Y., Moggi N., Morganti S., Napolitano T., Nastasi M., Nones C., Norman E.B., Novati V., Nucciotti A., Nutini I., O'Donnell T., Ouellet J.L., Pagliarone C.E., Pallavicini M., Pattavina L., Pavan M., Pessina G., Pettinacci V., Pira C., Pirro S., Pozzi S., Previtali E., Puiu A., Rosenfeld C., Rusconi C., Sakai M., Sangiorgio S., Schmidt B., Scielzo N.D., Singh V., Sisti M., Speller D., Taffarello L., Terranova F., Tomei C., Vignati M., Wagaarachchi S.L., Wang B.S., Welliver B., Wilson J., Wilson K., Winslow L.A., Wise T., Zanotti L., Zimmermann S., Zucchelli S., Département de Physique des Particules (ex SPP) (DPhP), Adams, D, Alduino, C, Alfonso, K, Avignone, F, Azzolini, O, Bari, G, Bellini, F, Benato, G, Bersani, A, Biassoni, M, Branca, A, Brofferio, C, Bucci, C, Caminata, A, Campani, A, Canonica, L, Cao, X, Capelli, S, Cappelli, L, Cardani, L, Carniti, P, Casali, N, Chiesa, D, Chott, N, Clemenza, M, Copello, S, Cosmelli, C, Cremonesi, O, Creswick, R, Cushman, J, D'Addabbo, A, D'Aguanno, D, Dafinei, I, Davis, C, Dell'Oro, S, Di Domizio, S, Dompe, V, Drobizhev, A, Fang, D, Fantini, G, Faverzani, M, Ferri, E, Ferroni, F, Fiorini, E, Franceschi, M, Freedman, S, Fujikawa, B, Giachero, A, Gironi, L, Giuliani, A, Gorla, P, Gotti, C, Gutierrez, T, Han, K, Heeger, K, Huang, R, Huang, H, Johnston, J, Keppel, G, Kolomensky, Y, Leder, A, Ligi, C, Ma, Y, Marini, L, Maruyama, R, Mei, Y, Moggi, N, Morganti, S, Napolitano, T, Nastasi, M, Nones, C, Norman, E, Novati, V, Nucciotti, A, Nutini, I, O'Donnell, T, Ouellet, J, Pagliarone, C, Pallavicini, M, Pattavina, L, Pavan, M, Pessina, G, Pettinacci, V, Pira, C, Pirro, S, Pozzi, S, Previtali, E, Puiu, A, Rosenfeld, C, Rusconi, C, Sakai, M, Sangiorgio, S, Schmidt, B, Scielzo, N, Singh, V, Sisti, M, Speller, D, Taffarello, L, Terranova, F, Tomei, C, Vignati, M, Wagaarachchi, S, Wang, B, Welliver, B, Wilson, J, Wilson, K, Winslow, L, Wise, T, Zanotti, L, Zimmermann, S, and Zucchelli, S
Subjects: Cryostat, Nuclear and High Energy Physics, Physics::Instrumentation and Detectors, Dark matter, energy resolution, 01 natural sciences, tellurium: oxygen, law.invention, Nuclear physics, energy: threshold, CUORE, Bolometers, Neutrinoless double beta decay, Ton-scale detector, double-beta decay: (0neutrino), bolometer, law, Observatory, Double beta decay, 0103 physical sciences, [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], 010306 general physics, Instrumentation, activity report, background: suppression, detector: design, Neutrinoless double beta decay, Ton-scale detector, Bolometers, Physics, 010308 nuclear & particles physics, Bolometer, Detector, sensitivity, cryogenics, High Energy Physics::Experiment, Neutrino, performance
Abstract: The Cryogenic Underground Observatory for Rare Events (CUORE) is the most massive bolometric experiment searching for neutrino-less double beta (0 ν β β ) decay. The detector consists of an array of 988 TeO 2 crystals (742 kg) arranged in a compact cylindrical structure of 19 towers. This paper will describe the CUORE experiment, including the cryostat, and present the detector performance during the first year of running. Additional detail will describe the effort made in improving the energy resolution in the 130Te 0 ν β β decay region of interest (ROI) and the suppression of backgrounds. A description of work to lower the energy threshold in order to give CUORE the sensitivity to search for other rare events, such as dark matter, will also be provided.
Published: 2019
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65. Erratum to: Search for non-relativistic magnetic monopoles with IceCube

Author: M. J. Larson, A. Olivas, M. Stamatikos, K. Mase, F. Huang, M. Quinnan, J. Blumenthal, L. Schulte, Olga Botner, V. Baum, L. Classen, A. Goldschmidt, M. W. E. Smith, J. A. Aguilar, K. Rawlins, J. Kiryluk, H. Landsman, James Madsen, L. Brayeur, I. Taboada, Dustin Hebecker, S. Flis, M. N. Tobin, O. Schulz, D. Z. Besson, Ch. Weaver, J. van Santen, A. Franckowiak, René Reimann, R. Nahnhauer, M. L. Benabderrahmane, Teresa Montaruli, P. Gretskov, K. Schatto, G. Kohnen, K. Krings, Oscar Macias, N. van Eijndhoven, C. Haack, J. C. Gallagher, A. O'Murchadha, M. Leuermann, L. Mohrmann, Surujhdeo Seunarine, J. Miller, Gary Binder, Axel Groß, Chad Finley, Nathan Whitehorn, Gerald Przybylski, M. Zoll, Allan Hallgren, S. Hussain, A. Kriesten, D. R. Nygren, J. P. A. M. de André, D. J. Koskinen, Takao Kuwabara, B. Christy, Sandro Kopper, Carlos Arguelles, M. Schmitz, J. Auffenberg, Seth M. Cohen, K. Jero, A. Ishihara, G. Kroll, T. Stanev, D. Berley, Matthias Wolf, G. C. Hill, J. C. Groh, A. Obertacke, Michael J. Baker, Maria Tselengidou, O. Jlelati, J. Feintzeig, L. Gladstone, Dirk Heinen, D. Seckel, S. Miarecki, S. Tilav, L. Rädel, R. Ström, Carsten Rott, M. Richman, A. Tamburro, A. R. Fazely, Tyce DeYoung, P. A. Toale, Javier Gonzalez, E. A. Strahler, M. Krasberg, M. Bissok, M. Vehring, A. Homeier, K.-H. Becker, Giorgio Maggi, N. Milke, C. Ha, R. Hellauer, E. Jacobi, George Japaridze, Timo Karg, Matt Dunkman, Xianwu Xu, T. Feusels, C. De Clercq, C. Bohm, Christopher Wiebusch, C. Kopper, G. Golup, T. Fischer-Wasels, Hermann Kolanoski, J. Daughhetee, A. Schukraft, S. Böser, David A. Williams, M. Casier, J. E. Jacobsen, Marcos Santander, J. Ziemann, S. Yoshida, C. Pérez de los Heros, Markus Ackermann, S. W. Barwick, Dirk Ryckbosch, Sally Robertson, L. Gerhardt, J. Lünemann, J. L. Kelley, Markus Ahlers, S. Euler, Thomas Meures, J. Leute, G. Tešić, Larissa Paul, F. Scheriau, R. C. Bay, Elisa Resconi, E. Unger, P. B. Price, Rezo Shanidze, Juan Carlos Diaz-Velez, B. Ruzybayev, H.-P. Bretz, M. Merck, N. L. Strotjohann, T. O. B. Schmidt, Kael Hanson, T. R. Wood, Frank McNally, Kurt Woschnagg, A. Christov, Albrecht Karle, T. Fuchs, Paul Evenson, C. Wendt, M. Day, A. Schönwald, Anatoli Fedynitch, D. Altmann, K. Wiebe, K. Meagher, Dmitry Chirkin, R. Hoffmann, Alexander Kappes, K. D. de Vries, R. Morse, C. Walck, R. Eagan, Thomas K. Gaisser, G. B. Yodh, Carl Pfendner, Paolo Desiati, E. Pinat, Samvel Ter-Antonyan, D. T. Grandmont, J. Becker Tjus, J. P. Rodrigues, Sofia Vallecorsa, B. J. Whelan, T. Stezelberger, Simona Toscano, K. Hoshina, S. M. Saba, Glenn Spiczak, B. Kaminsky, K. Clark, M. Kowalski, N. A. Stanisha, H. G. Sander, M. Danninger, D. F. Cowen, J. J. Beatty, Donglian Xu, S. Schoenen, U. Naumann, Mohamed Rameez, M. Lesiak-Bzdak, P. Redl, J. Posselt, Thorsten Glusenkamp, W. Huelsnitz, A. Stößl, M. G. Aartsen, Reina H. Maruyama, Xinhua Bai, R. Bruijn, D. Heereman, Kirill Filimonov, K. Helbing, Segev BenZvi, Spencer Klein, Kara Hoffman, A. H. Cruz Silva, Subir Sarkar, Wolfgang Rhode, A. Meli, P. Berghaus, J. Kläs, J. Kunnen, Damian Pieloth, A. M. Brown, L. Köpke, J. A. Goodman, M. Wellons, Dariusz Gora, Joshua Pepper, E. Middell, Elisa Bernardini, M. Ribordy, Jenni Adams, S. Hickford, R. G. Stokstad, Dennis Soldin, H. Taavola, E. Blaufuss, D. J. Boersma, J. C. Davis, K. Jagielski, S. De Ridder, M. Labare, S. Coenders, A. Bernhard, M. Kauer, D. Bose, T. Palczewski, B. Eberhardt, A. Tepe, H. S. Matis, Francis Halzen, P. Zarzhitsky, O. Fadiran, A. Haj Ismail, Matthias Vraeghe, M. Usner, C. Sheremata, P. O. Hulth, J. Eisch, S. Westerhoff, Björn Eichmann, J.-H. Köhne, H. Wissing, Daniel Bindig, T. C. Arlen, Hans Niederhausen, Naoko Kurahashi, Christian Spiering, S. Schöneberg, S. Odrowski, S. Zierke, A. Omairat, P. Hallen, K. Hultqvist, Darren Grant, M. Wallraff, M. Voge, Sarah Nowicki, Rasha Abbasi, J. Casey, Tim Ruhe, Benedikt Riedel, A. Stasik, K. Frantzen, F. Clevermann, Y. Sestayo, J. P. Yanez, and G. W. Sullivan
Subjects: Physics, Particle physics, Physics and Astronomy (miscellaneous), 010308 nuclear & particles physics, Mean free path, Nuclear Theory, 0103 physical sciences, Magnetic monopole, 010306 general physics, Nucleon, 01 natural sciences, Engineering (miscellaneous)
Abstract: In the analyses, published in Ref. [1], the exclusion limits are calculated in dependence of the mean free path of the magnetic monopole - nucleon catalysis interaction.
Published: 2019
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66. Erratum to: Search for annihilating dark matter in the Sun with 3 years of IceCube data

Author: B. Eichmann, H.-P. Bretz, L. Köpke, Christian Bohm, B. Relethford, Aongus O'Murchadha, Christoph Raab, Athina Meli, G. C. Hill, C. Krüger, T. R. Wood, Christopher Wiebusch, S. Fahey, M. Voge, A. R. Fazely, Aya Ishihara, Dennis Soldin, H. Taavola, E. Jacobi, G. Kohnen, L. Gladstone, P. A. Evenson, B. J. P. Jones, S. Euler, C. Pérez de los Heros, Logan Wille, P. Peiffer, M. Day, Matthew Relich, Sally Robertson, G. W. Sullivan, D. J. Koskinen, R. Koirala, J. Braun, D. Seckel, Albrecht Karle, B. Eberhardt, D. Bose, J. P. Dumm, S. Flis, Sebastian Böser, S. Miarecki, D. Z. Besson, P. Schlunder, D. Chirkin, Azadeh Keivani, T. Palczewski, D. V. Pankova, T. Stezelberger, B. Riedel, Matthias Wolf, A. Stasik, Matthew Weiss, Chad Finley, G. Krückl, Hermann Kolanoski, D. R. Nygren, Ö. Penek, S. Schöneberg, E. Vogel, K. Meagher, A. Turcati, T. Kittler, G. H. Collin, Marek Kowalski, J. Kim, E. Hansen, Matthias Huber, V. Baum, Gisela Anton, J. van Santen, C. Kopper, F. Tenholt, A. Stößl, J. A. Pepper, Kurt Becker, Kael Hanson, J. Feintzeig, N. van Eijndhoven, Dirk Ryckbosch, J. P. A. M. de André, Thomas Kintscher, G. Merino, N. Wandkowsky, J. C. Díaz-Vélez, S. Kopper, Janet Conrad, K. Jero, A. Christov, V. di Lorenzo, S. Wickmann, J. Auffenberg, D. Bindig, Jenni Adams, Dirk Lennarz, A. Steuer, Ignacio Taboada, D. Grant, D. Hebecker, H. Dujmovic, G. S. Japaridze, R. Nahnhauer, M. Quinnan, T. Meures, M. Vraeghe, A. Olivas, S. Schoenen, R. Cross, David Berley, M. Rongen, M. J. Larson, S. Bron, J. J. Beatty, C. Walck, G. Yodh, A. Burgman, D. Rysewyk, M. Börner, F. Huang, M. Song, T. L. Carver, Mike Richman, A. Bernhard, Steven W. Barwick, Juanan Aguilar, Stijn Blot, R. Hoffmann, Marjon Moulai, Chris Wendt, J. Becker Tjus, M. Bissok, J. Kunnen, K. Mase, C.-C. Fösig, E. Pinat, M. Labare, L. Gerhardt, R. Reimann, S. Tilav, Ch. Weaver, G. M. Spiczak, S. Hickford, R. Konietz, K. Rawlins, M. Vehring, G. T. Przybylski, M. van Rossem, Joeran Stettner, K. D. de Vries, T. Glüsenkamp, M. Kauer, Frank McNally, S. Westerhoff, Olga Botner, Elisa Resconi, Y. Xu, M. Rameez, Reina H. Maruyama, Joshua Hignight, James Madsen, K. Wiebe, Lu Lu, T. DeYoung, M. Zoll, Maryon Ahrens, K. Helbing, D. Heereman, H. Niederhausen, Francis Halzen, M. Dunkman, E. Unger, M. Medici, S. Coenders, E. Woolsey, G. Binder, Delia Tosi, S. Ter-Antonyan, R. Ström, Won Nam Kang, M. N. Tobin, Konstancja Satalecka, Theo Glauch, I. Ansseau, J. Lünemann, G. Neer, Teresa Montaruli, Elisa Bernardini, Timo Karg, M. Lesiak-Bzdak, Christian Spiering, E. Blaufuss, A. Terliuk, J. C. Gallagher, H. Dembinski, K. Krings, T. O. B. Schmidt, M. G. Aartsen, Klas Hultqvist, J. Kiryluk, S. C. Nowicki, Kendall Mahn, F. Bos, K. Andeen, S. De Ridder, Justin Vandenbroucke, Anna Franckowiak, Allan Hallgren, R. C. Bay, T. Anderson, C. De Clercq, M. Leuermann, Kurt Woschnagg, S. Yoshida, P. A. Toale, L. Brayeur, T. Hansmann, Karim Ghorbani, M. Casier, Spencer Axani, W. Giang, J. L. Lanfranchi, M. Archinger, T. Ehrhardt, C. Haack, Michael Sutherland, J. Tatar, S. Mancina, Carlos Arguelles, X. W. Xu, U. Naumann, M. Meier, N. Kurahashi, Todor Stanev, R. Hellauer, M. Jeong, G. de Wasseige, M. Tselengidou, Thomas K. Gaisser, P. Desiati, M. Mandelartz, F. Lauber, Lisa Johanna Schumacher, Javier Gonzalez, Giorgio Maggi, David A. Williams, Markus Ackermann, Carsten Rott, Alexander Kappes, Kirill Filimonov, Uli Katz, Segev BenZvi, A. Wallace, J. Sandroos, D. Altmann, S. Toscano, Spencer Klein, D. F. Cowen, L. Classen, Kara Hoffman, T. Ruhe, D. Pieloth, M. Kroll, Wolfgang Rhode, B. J. Whelan, S. In, L. Wills, Ali Kheirandish, T. Fuchs, L. Sabbatini, Takao Kuwabara, K. Clark, K. Hoshina, Stijn Vanheule, Philipp Eller, A. Sandrock, J. Felde, J. P. Yanez, H. Pandya, Xinhua Bai, A. Obertacke Pollmann, S. Kunwar, J. L. Kelley, M. Wallraff, Markus Ahlers, L. Rädel, R. G. Stokstad, A. Goldschmidt, S. E. Sanchez Herrera, E. Cheung, M. Usner, Elizabeth Friedman, R. Maunu, N. L. Strotjohann, Z. Griffith, Min Suk Kim, Donglian Xu, P. B. Price, G. Tešić, E. del Pino Rosendo, Subir Sarkar, Tobias Menne, S. Seunarine, Bron, Stéphanie, Carver, Tessa, Christov, Asen, Montaruli, Teresa, and Rameez, Mohamed
Subjects: background [atmosphere], Particle physics, Physics and Astronomy (miscellaneous), Physics::Instrumentation and Detectors, Astrophysics::High Energy Astrophysical Phenomena, Dark matter, lcsh:Astrophysics, ddc:500.2, 01 natural sciences, Signal, horizon, IceCube, Subatomär fysik, 0103 physical sciences, lcsh:QB460-466, Subatomic Physics, lcsh:Nuclear and particle physics. Atomic energy. Radioactivity, ddc:530, atmosphere [muon], 010306 general physics, detector [neutrino], mass [WIMP], Engineering (miscellaneous), Computer Science::Databases, direct detection [dark matter], Physics, Muon, 010308 nuclear & particles physics, scattering, sensitivity, statistics, lcsh:QC770-798, High Energy Physics::Experiment, Neutrino
Abstract: The European physical journal / C Particles and fields C 79(3), 214 (2019). doi:10.1140/epjc/s10052-019-6702-y, Published by Springer24928, Heidelberg
Published: 2019
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67. CUORE: The first bolometric experiment at the ton scale for rare decay searches

Author: A. Bersani, L. Pattavina, Oliviero Cremonesi, Massimiliano Clemenza, Carlo Cosmelli, C. Pagliarone, C. Rosenfeld, P. Gorla, H. Z. Huang, G. Keppel, F. Ferroni, C. Tomei, K. Wilson, V. Palmieri, C. Nones, Eric B. Norman, A. Puiu, Jonathan Ouellet, G. Bari, Claudio Gotti, T. Napolitano, C. Brofferio, L. Gironi, F. T. Avignone, C. J. Davis, A. Caminata, Ezio Previtali, B. Welliver, S. Copello, Guoqiang Zhang, Lorenzo Cassina, Evelyn Ferri, Paolo Carniti, L. Canonica, A. Giuliani, S. Di Domizio, M. M. Deninno, Davide Chiesa, L. Marini, C. Rusconi, Ettore Fiorini, M. Biassoni, N. Moggi, V. Novati, Andrea Giachero, F. Bellini, S. Zimmermann, Laura Cardani, J. Johnston, Ke Han, A. Branca, B. K. Fujikawa, Stefano Pozzi, L. Gladstone, D. Q. Adams, K. Alfonso, M. L. Di Vacri, Reina H. Maruyama, Samuele Sangiorgio, Stuart J. Freedman, C. Bucci, S. L. Wagaarachchi, T. D. Gutierrez, Miriam Lucio Martinez, Stefano Dell'Oro, R. Hennings-Yeomans, A. Nucciotti, R. J. Creswick, Stefano Pirro, N. Chott, D. D'Aguanno, C. Alduino, M. Vignati, M. Faverzani, S. Zucchelli, L. Cappelli, Giovanni Benato, N. Casali, Marco Pallavicini, Irene Nutini, Yu. G. Kolomensky, G. Pessina, S. Morganti, F. Terranova, Yu-Gang Ma, F. Reindl, H. W. Wang, T. O'Donnell, S. S. Nagorny, Y. Mei, Lindley Winslow, V. Dompè, M. Sakai, Xi-Guang Cao, A. D'Addabbo, K. M. Heeger, Carlo Ligi, N. D. Scielzo, A. Campani, T. Wise, L. Taffarello, Danielle Speller, L. Zanotti, I. Dafinei, C. Pira, A. Leder, D. Santone, Vasundhara Singh, B. Schmidt, B. S. Wang, D. Q. Fang, O. Azzolini, A. Drobizhev, Jeremy S. Cushman, M. A. Franceschi, R. G. Huang, Silvia Capelli, Massimiliano Nastasi, M. Pavan, James R. Wilson, Monica Sisti, Adams D.Q., Alduino C., Alfonso K., Avignone F.T., Azzolini O., Bari G., Bellini F., Benato G., Bersani A., Biassoni M., Branca A., Brofferio C., Bucci C., Caminata A., Campani A., Canonica L., Cao X.G., Capelli S., Cappelli L., Cardani L., Carniti P., Casali N., Cassina L., Chiesa D., Chott N., Clemenza M., Copello S., Cosmelli C., Cremonesi O., Creswick R.J., Cushman J.S., D'Addabbo A., D'Aguanno D., Dafinei I., Davis C.J., Dell'Oro S., Deninno M.M., Domizio S.D., Vacri M.L.D., Dompe V., Drobizhev A., Fang D.Q., Faverzani M., Ferri E., Ferroni F., Fiorini E., Franceschi M.A., Freedman S.J., Fujikawa B.K., Giachero A., Gironi L., Giuliani A., Gladstone L., Gorla P., Gotti C., Gutierrez T.D., Han K., Heeger K.M., Hennings-Yeomans R., Huang R.G., Huang H.Z., Johnston J., Keppel G., Kolomensky Y.G., Leder A., Ligi C., Ma Y.G., Marini L., Martinez M., Maruyama R.H., Mei Y., Moggi N., Morganti S., Nagorny S.S., Napolitano T., Nastasi M., Nones C., Norman E.B., Novati V., Nucciotti A., Nutini I., O'Donnell T., Ouellet J.L., Pagliarone C.E., Pallavicini M., Palmieri V., Pattavina L., Pavan M., Pessina G., Pira C., Pirro S., Pozzi S., Previtali E., Puiu A., Reindl F., Rosenfeld C., Rusconi C., Sakai M., Sangiorgio S., Santone D., Schmidt B., Scielzo N.D., Singh V., Sisti M., Speller D., Taffarello L., Terranova F., Tomei C., Vignati M., Wagaarachchi S.L., Wang B.S., Wang H.W., Welliver B., Wilson J., Wilson K., Winslow L.A., Wise T., Zanotti L., Zhang G.Q., Zimmermann S., Zucchelli S., Centre de Sciences Nucléaires et de Sciences de la Matière (CSNSM), 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), Département de Physique des Particules (ex SPP) (DPP), Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Département de Physique des Particules (ex SPP) (DPhP), Adams, D, Alduino, C, Alfonso, K, Avignone, F, Azzolini, O, Bari, G, Bellini, F, Benato, G, Bersani, A, Biassoni, M, Branca, A, Brofferio, C, Bucci, C, Caminata, A, Campani, A, Canonica, L, Cao, X, Capelli, S, Cappelli, L, Cardani, L, Carniti, P, Casali, N, Cassina, L, Chiesa, D, Chott, N, Clemenza, M, Copello, S, Cosmelli, C, Cremonesi, O, Creswick, R, Cushman, J, D’Addabbo, A, D’Aguanno, D, Dafinei, I, Davis, C, Dell’Oro, S, Deninno, M, Domizio, S, Vacri, M, Dompè, V, Drobizhev, A, Fang, D, Faverzani, M, Ferri, E, Ferroni, F, Fiorini, E, Franceschi, M, Freedman, S, Fujikawa, B, Giachero, A, Gironi, L, Giuliani, A, Gladstone, L, Gorla, P, Gotti, C, Gutierrez, T, Han, K, Heeger, K, Hennings-Yeomans, R, Huang, R, Huang, H, Johnston, J, Keppel, G, Kolomensky, Y, Leder, A, Ligi, C, Ma, Y, Marini, L, Martinez, M, Maruyama, R, Mei, Y, Moggi, N, Morganti, S, Nagorny, S, Napolitano, T, Nastasi, M, Nones, C, Norman, E, Novati, V, Nucciotti, A, Nutini, I, O’Donnell, T, Ouellet, J, Pagliarone, C, Pallavicini, M, Palmieri, V, Pattavina, L, Pavan, M, Pessina, G, Pira, C, Pirro, S, Pozzi, S, Previtali, E, Puiu, A, Reindl, F, Rosenfeld, C, Rusconi, C, Sakai, M, Sangiorgio, S, Santone, D, Schmidt, B, Scielzo, N, Singh, V, Sisti, M, Speller, D, Taffarello, L, Terranova, F, Tomei, C, Vignati, M, Wagaarachchi, S, Wang, B, Wang, H, Welliver, B, Wilson, J, Wilson, K, Winslow, L, Wise, T, Zanotti, L, Zhang, G, Zimmermann, S, and Zucchelli, S
Subjects: Nuclear and High Energy Physics, Cryogenic, Superconductive Devices, Physics::Instrumentation and Detectors, Cryogenic, 01 natural sciences, tellurium: oxygen, Combinatorics, CUORE, bolometer, double-beta decay: (0neutrino), Superconductive Devices, 0103 physical sciences, [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], 010306 general physics, Instrumentation, detector: design, activity report, Physics, 010308 nuclear & particles physics, Astrophysics::Instrumentation and Methods for Astrophysics, Superconductive Device, cryogenics, Physics::Accelerator Physics, High Energy Physics::Experiment, performance
Abstract: Author(s): Adams, DQ; Alduino, C; Alfonso, K; Avignone, FT; Azzolini, O; Bari, G; Bellini, F; Benato, G; Bersani, A; Biassoni, M; Branca, A; Brofferio, C; Bucci, C; Caminata, A; Campani, A; Canonica, L; Cao, XG; Capelli, S; Cappelli, L; Cardani, L; Carniti, P; Casali, N; Cassina, L; Chiesa, D; Chott, N; Clemenza, M; Copello, S; Cosmelli, C; Cremonesi, O; Creswick, RJ; Cushman, JS; D'Addabbo, A; D'Aguanno, D; Dafinei, I; Davis, CJ; Dell'Oro, S; Deninno, MM; Domizio, SD; Vacri, MLD; Dompe, V; Drobizhev, A; Fang, DQ; Faverzani, M; Ferri, E; Ferroni, F; Fiorini, E; Franceschi, MA; Freedman, SJ; Fujikawa, BK; Giachero, A; Gironi, L; Giuliani, A; Gladstone, L; Gorla, P; Gotti, C; Gutierrez, TD; Han, K; Heeger, KM; Hennings-Yeomans, R; Huang, RG; Huang, HZ; Johnston, J; Keppel, G; Kolomensky, YG; Leder, A; Ligi, C; Ma, YG; Marini, L; Martinez, M; Maruyama, RH; Mei, Y; Moggi, N; Morganti, S; Nagorny, SS; Napolitano, T; Nastasi, M; Nones, C; Norman, EB; Novati, V; Nucciotti, A; Nutini, I; O'Donnell, T; Ouellet, JL; Pagliarone, CE; Pallavicini, M | Abstract: The Cryogenic Underground Observatory for Rare Events (CUORE) is the first bolometric experiment searching for neutrinoless double beta decay that has been able to reach the 1-ton scale. The detector consists of an array of 988 TeO2 crystals arranged in a cylindrical compact structure of 19 towers. The construction of the experiment and, in particular, the installation of all towers in the cryostat was completed in August 2016 and data taking started in spring 2017. In this contribution the achievement of the commissioning phase and the performance of the detector and the cryostat during the first physics run will be presented.
Published: 2019
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68. Time-integrated Neutrino Source Searches with 10 years of IceCube Data

Author: Federica Bradascio, Alexander Burgman, Merlin Schaufel, Daria Pankova, E. Friedman, Claudio Kopper, Subir Sarkar, Chad Finley, J. J. Beatty, Tianlu Yuan, M. Kauer, D. Kang, Christoph Tönnis, Frank G. Schröder, Alexander Fritz, D. Z. Besson, K. Mase, Yuya Makino, R. Morse, Suyong Choi, I. Taboada, R. Maunu, David Kappesser, Michael O. Wolf, Minjin Jeong, Thomas Meures, N. L. Strotjohann, Felix Henningsen, A. R. Fazely, E. Pinat, Simona Toscano, P. Heix, K. Jero, Sander Vanheule, N. Kurahashi, Karl J. Clark, S. De Ridder, Z. Griffith, Jenni Adams, J. Lünemann, C. Pérez de los Heros, A. Obertacke Pollmann, Aswathi Balagopal, Saskia Philippen, D. Rysewyk, M. Song, T. L. Carver, Mike Richman, J. L. Kelley, Markus Ahlers, K. Meagher, F. McNally, M. J. Weiss, M. Labare, T. Palczewski, C. Wendt, E. O’Sullivan, S. Hickford, Jan Soedingrekso, M. Stamatikos, S. Kopper, René Reimann, A. O'Murchadha, Lenka Tomankova, Chunfai Tung, P. Peiffer, M. J. Larson, Pranav Dave, Timothyblake Watson, Erik Ganster, T. Menne, G. de Wasseige, B. Eberhardt, A. Stößl, L. Rauch, Benjamin Hokanson-Fasig, Yang Lyu, Samvel Ter-Antonyan, M. Silva, R. G. Stokstad, B. Relethford, S. Yoshida, Won Nam Kang, Amirreza Raissi, Chris Weaver, Stephanie Bron, Max Renschler, D. J. Koskinen, Wing Yan Ma, Tim Ruhe, B. J. P. Jones, R. Hoffmann, B. J. Whelan, X. Bai, G. Neer, E. Bourbeau, C. J. Lozano Mariscal, G. Merino, Reina H. Maruyama, James DeLaunay, C. Alispach, G. Krückl, Konstancja Satalecka, N. Wandkowsky, H. Dujmovic, Janet Conrad, K. Wiebe, Marjon Moulai, Summer Blot, Andres Medina, Theo Glauch, Jan Weldert, Thomas Ehrhardt, Spencer Griswold, Steven Robertson, Joshua Hignight, L. Halve, Philipp Eller, Shefali Shefali, D. Mockler, M. Günder, Alejandro Diaz, R. Cross, Timo Sturwald, H. Niederhausen, Kael Hanson, Surujhdeo Seunarine, R. Snihur, A. Weindl, Maria Tselengidou, D. Soldin, Johannes Werthebach, Carsten Rott, Juanan Aguilar, T. Stezelberger, R. Joppe, D. van Eijk, Joshua A. Wood, J. Felde, C. Walck, Jeffrey Lazar, R. Hellauer, J. Buscher, P. Schlunder, Maryon Ahrens, Alan Coleman, William Luszczak, Alexander Sandrock, Frederik Tenholt, R. Nagai, A. Goldschmidt, L. Schumacher, M. Zöcklein, Xianwu Xu, M. Medici, J. Sandroos, Timo Karg, T. Stanev, Maximilian Meier, Thomas K. Gaisser, G. B. Yodh, P. Steinmüller, F. Huang, G. H. Collin, Matthias Vraeghe, J. Stettner, J. Kim, Delia Tosi, U. Katz, Mehmet Gunduz, Agnieszka Leszczyńska, M. E. Huber, Marcos Santander, Paolo Desiati, S. E. Sanchez Herrera, R. C. Bay, K. D. de Vries, Sebastian Baur, Sebastian Böser, P. Backes, Gisela Anton, Elisa Bernardini, G. W. Sullivan, H. S. Matis, D. B. Fox, L. Gerhardt, A. Olivas, Austin Schneider, James E. Braun, N. van Eijndhoven, K. Helbing, C. Haack, Juan Carlos Diaz-Velez, H. Bagherpour, Benjamin Bastian, Anastasia Maria Barbano, T. Kittler, Daniel Bindig, Hermann Kolanoski, K. Becker, Emily Dvorak, N. Kulacz, Olga Botner, Kayla Leonard, D. R. Nygren, Javier Gonzalez, Roxanne Turcotte, Marek Kowalski, D. Hebecker, F. Jonske, Alexander Trettin, Giorgio Maggi, Mirco Hunnefeld, Marie Oehler, V. Baum, Sarah Mancina, Anna Franckowiak, Tobias Hoinka, Francis Halzen, J. Auffenberg, M. Börner, Steve Sclafani, J. Kiryluk, C. De Clercq, S. Tilav, I. Ansseau, Paul Coppin, Andrea Turcati, J. C. Gallagher, M. Leuermann, K. Andeen, Elisa Lohfink, J. P. Yanez, Gerrit Wrede, K. Hoshina, Thomas Huber, David A. Williams, Allan Hallgren, Juliana Stachurska, J. van Santen, H. Dembinski, Alex Pizzuto, Markus Ackermann, Glenn Spiczak, G. Momenté, M. G. Aartsen, Pablo Correa, S. W. Barwick, M. Rameez, D. F. Cowen, Gary Binder, Gerald Przybylski, U. Naumann, R. Halliday, George Japaridze, Roger Moore, E. Unger, A. Kyriacou, J. Bourbeau, K. Krings, Seongjin In, Elisa Resconi, Yiqian Xu, Matt Dunkman, Alessio Porcelli, M. Plum, J. Becker Tjus, E. Cheung, Ramesh Koirala, Thomas Stuttard, Dirk Ryckbosch, Stephan Meighen-Berger, K. Tollefson, E. Blaufuss, Albrecht Karle, Qinrui Liu, T. Glüsenkamp, L. Classen, Martina Karl, Jochen M. Schneider, M. A. Unland Elorrieta, D. Heereman, M. Wallraff, A. Steuer, Raamis Hussain, Colin Turley, T. Anderson, Immacolata Carmen Rea, Andreas Haungs, A. Ishihara, K. Mallot, H. Schieler, Kirill Filimonov, Segev BenZvi, T. Kintscher, M. Usner, Frederik Hermann Lauber, Spencer Klein, A. Terliuk, Justin Lanfranchi, Kara Hoffman, Julia Böttcher, Christian Spiering, Hershal Pandya, Wolfgang Rhode, Robert Stein, Justin Vandenbroucke, L. Wills, P. Muth, Ioana Codrina Maris, S. C. Nowicki, Christian Bohm, Ibrahim Safa, Damian Pieloth, Ali Kheirandish, W. Van Driessche, Nahee Park, K. Hultqvist, Darren Grant, Jannes Brostean-Kaiser, Christoph Raab, Nadège Iovine, M. U. Nisa, L. Köpke, D. Berley, G. C. Hill, Bunheng Ty, Ralph Engel, Giovanni Renzi, K. Rawlins, D. Seckel, S. Fahey, Tyce DeYoung, Nathan Whitehorn, Martin Rongen, R. S. Busse, Christopher Wiebusch, Kunal Deoskar, James Madsen, Lu Lu, L. Wille, Teresa Montaruli, Kendall Mahn, P. B. Price, Francesco Lucarelli, T. O. B. Schmidt, C. Chen, Karim Ghorbani, Spencer Axani, T. R. Wood, Carlos Arguelles, Jessie Micallef, P. Mallik, Kurt Woschnagg, Paul Evenson, Simone Garrappa, Dmitry Chirkin, Alexander Kappes, A. Wallace, Da Xu, Physics, Faculty of Sciences and Bioengineering Sciences, Elementary Particle Physics, and Vriendenkring VUB
Subjects: background [atmosphere], Astrophysics::High Energy Astrophysical Phenomena, media_common.quotation_subject, General Physics and Astronomy, FOS: Physical sciences, Astrophysics::Cosmology and Extragalactic Astrophysics, 01 natural sciences, IceCube, particle source [neutrino], TRACK RECONSTRUCTION, 0103 physical sciences, ddc:530, atmosphere [muon], 010306 general physics, Astrophysics::Galaxy Astrophysics, media_common, astro-ph.HE, Physics, High Energy Astrophysical Phenomena (astro-ph.HE), Muon, Astrophysics::Instrumentation and Methods for Astrophysics, Northern Hemisphere, Astronomy, Galaxy, messenger, Physics and Astronomy, Sky, correlation, time dependence, upgrade, galaxy, Neutrino, Astrophysics - High Energy Astrophysical Phenomena, statistical
Abstract: Physical review letters 124(5), 051103 (1-9) (2020). doi:10.1103/PhysRevLett.124.051103, This paper presents the results from point-like neutrino source searches using ten years of IceCube data collected between April 6, 2008 and July 10, 2018. We evaluate the significance of an astrophysical signal from a point-like source looking for an excess of clustered neutrino events with energies typically above $\sim1\,$TeV among the background of atmospheric muons and neutrinos. We perform a full-sky scan, a search within a selected source catalog, a catalog population study, and three stacked Galactic catalog searches. The most significant point in the Northern hemisphere from scanning the sky is coincident with the Seyfert II galaxy NGC 1068, which was included in the source catalog search. The excess at the coordinates of NGC 1068 is inconsistent with background expectations at the level of $2.9\,\sigma$ after accounting for statistical trials. The combination of this result along with excesses observed at the coordinates of three other sources, including TXS 0506+056, suggests that, collectively, correlations with sources in the Northern catalog are inconsistent with background at 3.3$\,\sigma$ significance. These results, all based on searches for a cumulative neutrino signal integrated over the ten years of available data, motivate further study of these and similar sources, including time-dependent analyses, multimessenger correlations, and the possibility of stronger evidence with coming upgrades to the detector., Published by APS, College Park, Md.
Published: 2019
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69. Double-beta decay of $^{130}\hbox {Te}$ to the first $0^+$ excited state of $^{130}\hbox {Xe}$ with CUORE-0

Author: Alan R. Smith, Massimiliano Clemenza, Carlo Cosmelli, Oliviero Cremonesi, L. Canonica, L. Marini, Kevin Hickerson, L. Gladstone, M. Faverzani, C. Rosenfeld, R. Hennings-Yeomans, P. Gorla, F. Ferroni, B. X. Zhu, C. Tomei, S. Zucchelli, R. J. Creswick, Emanuele Ferri, Eugene E. Haller, C. Brofferio, James R. Wilson, P. J. Mosteiro, S. Zimmermann, C. Bucci, T. D. Gutierrez, Miriam Lucio Martinez, S. Morganti, D. R. Artusa, Monica Sisti, V. Palmieri, C. J. Davis, L. Carbone, N. Casali, A. Camacho, S. Copello, Eric B. Norman, T. Napolitano, Jeremy S. Cushman, G. Piperno, G. Bari, L. Zanotti, Ke Han, Reina H. Maruyama, Yu. G. Kolomensky, Luigi Cappelli, Davide Chiesa, K. E. Lim, Paolo Carniti, N. D. Scielzo, S. L. Wagaarachchi, Stuart J. Freedman, L. Taffarello, M. Maino, Lorenzo Cassina, Jeffrey W. Beeman, S. Trentalange, M. Biassoni, M. M. Deninno, S. Di Domizio, Y. Mei, I. Dafinei, Guimin Zhang, A. Bersani, A. D'Addabbo, N. Moggi, Simone Capelli, R. W. Kadel, M. Pavan, L. Gironi, F. T. Avignone, Claudio Gotti, H. Z. Huang, B. K. Fujikawa, S. Pirro, Stefano Dell'Oro, Carlo Ligi, Stefano Pozzi, C. Pira, Samuele Sangiorgio, H. W. Wang, G. Keppel, Xi-Guang Cao, A. Leder, F. Bellini, A. Nucciotti, Yu-Gang Ma, T. O'Donnell, A. Caminata, Ezio Previtali, T. I. Banks, K. M. Heeger, M. Vignati, A. Woodcraft, X. Liu, A. Giuliani, G. Fernandes, C. Alduino, F. Orio, Vasundhara Singh, J. Feintzeig, D. Santone, F. Terranova, Ettore Fiorini, E. V. Hansen, N. Chott, M. Tenconi, B. S. Wang, Marco Pallavicini, O. Azzolini, G. Pessina, K. Alfonso, M. L. Di Vacri, C. Nones, C. Rusconi, V. Pettinacci, L. Cardani, Lindley Winslow, L. Pattavina, A. Drobizhev, M. A. Franceschi, A. Giachero, D. Q. Fang, J. L. Ouellet, C. Pagliarone, T. Wise, Centre de Sciences Nucléaires et de Sciences de la Matière (CSNSM), 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), Département de Physique des Particules (ex SPP) (DPP), Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, CUORE, and Département de Physique des Particules (ex SPP) (DPhP)
Subjects: Semileptonic decay, topology, Physics and Astronomy (miscellaneous), energy levels: splitting, data acquisition, detector: mass, [PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex], 01 natural sciences, energy: transition, CUORE, background: low, double-beta decay: (0neutrino), Double beta decay, 0103 physical sciences, [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], 010306 general physics, Engineering (miscellaneous), Physics, S076H0N, 010308 nuclear & particles physics, excited state: energy, particle: Majorana, semileptonic decay, Excited state, xenon: nuclide, tellurium: nuclide, Neutrino, Atomic physics, Radioactive decay
Abstract: We report on a search for double beta decay of $$^{130}\hbox {Te}$$130Te to the first $$0^{+}$$0+ excited state of $$^{130}\hbox {Xe}$$130Xe using a $$9.8\,\hbox {kg}\cdot \hbox {yr}$$9.8kg·yr exposure of $$^{130}\hbox {Te}$$130Te collected with the CUORE-0 experiment. In this work we exploit different topologies of coincident events to search for both the neutrinoless and two-neutrino double beta decay modes. We find no evidence for either mode and place lower bounds on the half-lives: $$T^{0\nu }_{0^+_1}>7.9\cdot 10^{23}\hbox {yr}$$T01+0ν>7.9·1023yr and $$T^{2\nu }_{0^+_1}>2.4\cdot 10^{23}\hbox {yr}$$T01+2ν>2.4·1023yr ($$90\%\,\hbox {CL}$$90%CL). Combining our results with those obtained by the CUORICINO experiment, we achieve the most stringent constraints available for these processes: $$T^{0\nu }_{0^+_1}>1.4\cdot 10^{24}\hbox {yr}$$T01+0ν>1.4·1024yr and $$T^{2\nu }_{0^+_1}>2.5\cdot 10^{23}\hbox {yr}$$T01+2ν>2.5·1023yr ($$90\%\,\hbox {CL}$$90%CL).
Published: 2019
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70. First Direct Search for Inelastic Boosted Dark Matter with COSINE-100

Author: S. Choi, R. L. C. Pitta, H. W. Joo, W. G. Thompson, K. A. Shin, Stephen L. Olsen, Carsten Rott, K. W. Kim, H. Prihtiadi, F. Mouton, A. Scarff, E. Barbosa de Souza, Yong Hamb Kim, V. A. Kudryavtsev, Reina H. Maruyama, Nam Young Kim, H. J. Kim, Govinda Adhikari, J.H. Lee, N. J. C. Spooner, W. A. Lynch, G. S. Kim, David Leonard, M. Kauer, Kangsoon Park, P. Adhikari, Y. D. Kim, J. H. Jo, N. Carlin, Woosik Kang, G. H. Yu, Insik Hahn, Won Nam Kang, H. Kim, Hyun Su Lee, Mitra Djamal, Joo Young Lee, B. J. Park, Eunju Jeon, S. K. Kim, C. Ha, Y. J. Ko, Liang Yang, S. J. Ra, A. C. Ezeribe, Hansoo Park, Hyangkyu Park, and Moo Hyun Lee
Subjects: Physics, Physics - Instrumentation and Detectors, COLISÕES DE ÍONS PESADOS RELATIVÍSTICOS, Dark matter, FOS: Physical sciences, General Physics and Astronomy, Instrumentation and Detectors (physics.ins-det), Electron, Parameter space, Inelastic scattering, 01 natural sciences, Galaxy, Dark photon, Standard Model, High Energy Physics - Experiment, Nuclear physics, High Energy Physics - Experiment (hep-ex), 0103 physical sciences, High Energy Physics::Experiment, Nuclear Experiment (nucl-ex), 010306 general physics, Astrophysics - Instrumentation and Methods for Astrophysics, Instrumentation and Methods for Astrophysics (astro-ph.IM), Event (particle physics), Nuclear Experiment
Abstract: A search for inelastic boosted dark matter (iBDM) using the COSINE-100 detector with 59.5 days of data is presented. This relativistic dark matter is theorized to interact with the target material through inelastic scattering with electrons, creating a heavier state that subsequently produces standard model particles, such as an electron-positron pair. In this study, we search for this electron-positron pair in coincidence with the initially scattered electron as a signature for an iBDM interaction. No excess over the predicted background event rate is observed. Therefore, we present limits on iBDM interactions under various hypotheses, one of which allows us to explore an area of the experimental search for iBDM using a terrestrial detector., 6 pages, 5 figures
Published: 2018

71. Astrophysical neutrinos and cosmic rays observed by IceCube

Author: D. Hebecker, Andrea Turcati, M. Kroll, K. Krings, J. van Santen, K. D. de Vries, G. Merino, N. Wandkowsky, Segev BenZvi, R. Maunu, Spencer Klein, M. Mandelartz, M. Usner, Ramesh Koirala, J. Becker Tjus, Dennis Soldin, G. H. Collin, H. Taavola, Gary Binder, E. Blaufuss, T. Kuwabara, Surujhdeo Seunarine, L. Classen, Kara Hoffman, Juanan Aguilar, S. De Ridder, M. Labare, M. van Rossem, K. Rawlins, Maryon Ahrens, Frederik Tenholt, M. Medici, B. J. Whelan, M. Relich, A. Ishihara, J. Veenkamp, S. Coenders, C. Pérez de los Heros, H.-P. Bretz, Killian Holzapfel, Hershal Pandya, Frank McNally, Martin Rongen, Francis Halzen, Wolfgang Rhode, A. Christov, A. Meli, L. Wille, James Madsen, S. E. Sanchez Herrera, A. Goldschmidt, D. Z. Besson, Lu Lu, Z. Griffith, T. Kintscher, S. Euler, Hans Niederhausen, A. Bernhard, K. Clark, I. Ansseau, H. Dembinski, J. C. Gallagher, Thomas Meures, L. Wills, B. J. P. Jones, Ch. Weaver, M. N. Tobin, A. Stasik, Frederik Hermann Lauber, R. Konietz, M. Leuermann, J. Feintzeig, N. L. Strotjohann, J. Kunnen, Jenni Adams, N. Kurahashi, Todor Stanev, C. Wendt, Chad Finley, A. Wallace, G. de Wasseige, K. Meagher, F. Bos, J. Lünemann, Damian Pieloth, Ali Kheirandish, Tim Ruhe, K.-H. Becker, Janet Conrad, T. Stezelberger, R. Hoffmann, M. Day, B. Riedel, Yiqian Xu, Matt Dunkman, R. G. Stokstad, A. R. Fazely, R. Cross, Joshua Hignight, Da Xu, Allan Hallgren, C. Walck, A. Terliuk, S. Westerhoff, Justin Lanfranchi, Stephanie Bron, Philipp Eller, Sarah Mancina, Albrecht Karle, M. S. Sutherland, Kendall Mahn, C.-C. Fösig, Sandro Kopper, T. Fuchs, E. Pinat, Kael Hanson, K. Wiebe, Thomas K. Gaisser, G. B. Yodh, E. Cheung, Christian Spiering, D. R. Nygren, P. Schlunder, L. Köpke, Simona Toscano, M. Kauer, M. Börner, J. Kiryluk, K. Jero, G. Krückl, Dirk Ryckbosch, Marek Kowalski, K. Andeen, Matthias Wolf, M. Vehring, D. Altmann, Alexander Burgman, T. Anderson, D. Bose, P. B. Price, Justin Vandenbroucke, Javier Gonzalez, J. P. Dumm, Azadeh Keivani, Thomas Ehrhardt, T. Palczewski, J. Felde, S. Schöneberg, Karim Ghorbani, Spencer Axani, M. Song, M. Lesiak-Bzdak, L. Brayeur, L. Sabbatini, T. L. Carver, Mike Richman, Giorgio Maggi, Maximilian Meier, T. O. B. Schmidt, D. Heereman, G. Tešić, Daria Pankova, E. Vogel, M. S. Kim, Dirk Lennarz, S. Wickmann, J. Auffenberg, Paolo Desiati, T. R. Wood, R. Nahnhauer, Gisela Anton, E. Friedman, R. Hellauer, I. Taboada, A. Steuer, E. del Pino Rosendo, A. Obertacke Pollmann, S. Kunwar, Subir Sarkar, Minjin Jeong, Carlos Arguelles, S. Schoenen, W. Giang, S. Flis, S. Tilav, C. De Clercq, K. Mase, B. Eberhardt, Kurt Woschnagg, Paul Evenson, J. P. Yanez, J. L. Kelley, Markus Ahlers, Kirill Filimonov, Sally Robertson, Matthias Vraeghe, Sebastian Böser, G. W. Sullivan, David A. Williams, M. J. Weiss, Carsten Rott, James E. Braun, J. Kim, Christopher Wiebusch, George Japaridze, Dmitry Chirkin, S. Hickford, K. Helbing, Björn Eichmann, T. Kittler, Markus Ackermann, S. W. Barwick, M. Bissok, Alexander Kappes, K. Hultqvist, S. Yoshida, T. Hansmann, E. Woolsey, Darren Grant, T. Montaruli, N. van Eijndhoven, Xianwu Xu, Joshua Pepper, J. Sandroos, René Reimann, E. Jacobi, Samvel Ter-Antonyan, C. Haack, C. Bohm, Delia Tosi, Daniel Bindig, Christoph Raab, Sarah Nowicki, Seongjin In, Elisa Resconi, J. Tatar, Elisa Bernardini, D. Berley, G. C. Hill, R. Ström, J. P. A. M. de André, Won Nam Kang, M. Jurkovic, L. Gladstone, C. Krüger, D. Seckel, S. Fahey, M. G. Aartsen, S. Miarecki, X. Bai, G. Neer, P. Peiffer, T. Menne, Tyce DeYoung, L. Schumacher, P. A. Toale, B. Relethford, Konstancja Satalecka, Theo Glauch, M. Casier, U. Katz, Alexander Sandrock, R. C. Bay, Hermann Kolanoski, J. Stettner, Juan Carlos Diaz-Velez, M. Archinger, A. Olivas, K. Hoshina, F. Huang, Glenn Spiczak, M. Rameez, D. F. Cowen, C. Kopper, U. Naumann, E. Unger, J. J. Beatty, A. O'Murchadha, D. J. Koskinen, D. Rysewyk, A. Stößl, Reina H. Maruyama, Maria Tselengidou, Ö. Penek, Summer Blot, L. Rädel, Timo Karg, E. Hansen, M. E. Huber, L. Gerhardt, M. J. Larson, M. Quinnan, A. Franckowiak, Marjon Moulai, Olga Botner, V. Baum, Gerald Przybylski, M. Zoll, Hrvoje Dujmovic, Sander Vanheule, G. Kohnen, V. di Lorenzo, T. Glüsenkamp, M. Wallraff, M. Voge, Physics, Elementary Particle Physics, Vriendenkring VUB, and Faculty of Sciences and Bioengineering Sciences
Subjects: Atmospheric Science, Astrophysics::High Energy Astrophysical Phenomena, Aerospace Engineering, Cosmic ray, Astrophysics, Physics and Astronomy(all), 7. Clean energy, 01 natural sciences, IceCube Neutrino Observatory, IceCube, cosmic rays, Observatory, 0103 physical sciences, Neutrinos, 010303 astronomy & astrophysics, Cosmic rays, Physics, Muon, 010308 nuclear & particles physics, Gamma ray, Astrophysics::Instrumentation and Methods for Astrophysics, neutrinos, Astronomy, Astronomy and Astrophysics, Geophysics, Space and Planetary Science, Neutrino detector, 13. Climate action, Physique des particules élémentaires, General Earth and Planetary Sciences, Neutrino, Neutrino astronomy
Abstract: The core mission of the IceCube neutrino observatory is to study the origin and propagation of cosmic rays. IceCube, with its surface component IceTop, observes multiple signatures to accomplish this mission. Most important are the astrophysical neutrinos that are produced in interactions of cosmic rays, close to their sources and in interstellar space. IceCube is the first instrument that measures the properties of this astrophysical neutrino flux and constrains its origin. In addition, the spectrum, composition, and anisotropy of the local cosmic-ray flux are obtained from measurements of atmospheric muons and showers. Here we provide an overview of recent findings from the analysis of IceCube data, and their implications to our understanding of cosmic rays., 0, SCOPUS: ar.j, info:eu-repo/semantics/published
Published: 2018

72. Molecular detection of Mycobacterium leprae by Polymerase Chain Reaction in captive and free-ranging wild animals

Author: Valéria Dutra, Thais Oliveira Morgado, Fernanda H. Maruyama, Luciano Nakazato, and Richard de Campos Pacheco
Subjects: 0301 basic medicine, Microbiology (medical), DNA, Bacterial, 030231 tropical medicine, lcsh:QR1-502, Animals, Wild, Biology, Polymerase Chain Reaction, lcsh:Microbiology, law.invention, Microbiology, lcsh:Infectious and parasitic diseases, 03 medical and health sciences, 0302 clinical medicine, law, Leprosy, Animals, Humans, lcsh:RC109-216, Mycobacterium leprae, Polymerase chain reaction, Free ranging, biology.organism_classification, 030104 developmental biology, Infectious Diseases, Brazil
Published: 2018

73. P3561Active selexipag-metabolite MRE-269 induces DUSP1 and inhibits PASMC proliferation

Author: Kazuhiro Aonuma, Shunsuke Sakai, and H Maruyama
Subjects: chemistry.chemical_compound, chemistry, business.industry, Metabolite, Medicine, Selexipag, Pharmacology, Cardiology and Cardiovascular Medicine, business
Published: 2018
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74. Results from the Cuore Experiment

Author: Deqing Fang, Benjamin Schmidt, A. Bersani, A. Caminata, L. Zanotti, S. Copello, N. Casali, Carlo Ligi, V. Dompè, C. Pira, Carlo Cosmelli, A. Campani, C. Bucci, Paolo Carniti, Chris Alduino, A. Leder, K. Wilson, C. Pagliarone, S. Zimmermann, Oliviero Cremonesi, Lindley Winslow, L. Gironi, R. Hennings-Yeomans, F. T. Avignone, Vivek Singh, Irene Nutini, T. Wise, Giovanni Benato, Ke Han, A. Branca, C. Brofferio, N. Moggi, Reina H. Maruyama, Jeremy S. Cushman, Jonathan Ouellet, Yu-Gang Ma, Claudia Tomei, G. Bari, L. Taffarello, L. Pattavina, M. Pavan, Eric B. Norman, Lucia Canonica, N. Chott, Danielle Speller, G. Fantini, Nick Scielzo, V. Novati, V. Pettinacci, Silvio Morganti, F. Bellini, T. Napolitano, Samuele Sangiorgio, T. D. Gutierrez, F. Terranova, Stefano Dell'Oro, M. Clemenza, Stefano Pirro, D. D'Aguanno, A. Nucciotti, O. Azzolini, Barbara Wang, A. Puiu, Sergio Di Domizio, A. D'Addabbo, M. Biassoni, Davide Chiesa, S. J. Freedman, G. Keppel, C. Rosenfeld, Silvia Capelli, M. Faverzani, Y. u. G. Kolomensky, P. Gorla, Massimiliano Nastasi, Claudia Nones, F. Ferroni, Claudio Gotti, Laura Cardani, Emanuele Ferri, Milena Deninno, B. K. Fujikawa, Ettore Fiorini, J. S. Wilson, C. Rusconi, Y. Mei, Stefano Pozzi, L. Marini, C. J. Davis, Andrea Giachero, J. Johnston, Ioan Dafinei, Marco Pallavicini, M. Vignati, A. Giuliani, G. Pessina, H. Z. Huang, D. Q. Adams, Sachinthya Wagaarachchi, K. Alfonso, M. Sakai, T. O'Donnell, Xi-Guang Cao, K. M. Heeger, Luigi Cappelli, M. I. Martínez, S. Zucchelli, Monica Sisti, A. Drobizhev, Richard Creswick, M. A. Franceschi, R. G. Huang, Ezio Previtali, Bradford Welliver, Centre de Sciences Nucléaires et de Sciences de la Matière (CSNSM), 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), Département de Physique des Particules (ex SPP) (DPP), Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Caminata A., Adams D., Alduino C., Alfonso K., Avignone F., Azzolini O., Bari G., Bellini F., Benato G., Bersani A., Biassoni M., Branca A., Brofferio C., Bucci C., Campani A., Canonica L., Cao X.-G., Capelli S., Cappelli L., Cardani L., Carniti P., Casali N., Chiesa D., Chott N., Clemenza M., Copello S., Cosmelli C., Cremonesi O., Creswick R., Cushman J., D'Addabbo A., D'Aguanno D., Dafinei I., Davis C., Dell'Oro S., Deninno M., Di Domizio S., Dompe V., Drobizhev A., Fang D.-Q., Fantini G., Faverzani M., Ferri E., Ferroni F., Fiorini E., Franceschi M.A., Freedman S., Fujikawa B., Giachero A., Gironi L., Giuliani A., Gorla P., Gotti C., Gutierrez T., Han K., Heeger K., Hennings-Yeomans R., Huang R., Huang H.Z., Johnston J., Keppel G., Kolomensky Y., Leder A., Ligi C., Ma Y.-G., Marini L., Martinez M., Maruyama R., Mei Y., Moggi N., Morganti S., Napolitano T., Nastasi M., Nones C., Norman E., Novati V., Nucciotti A., Nutini I., O'Donnell T., Ouellet J., Pagliarone C., Pallavicini M., Pattavina L., Pavan M., Pessina G., Pettinacci V., Pira C., Pirro S., Pozzi S., Previtali E., Puiu A., Rosenfeld C., Rusconi C., Sakai M., Sangiorgio S., Schmidt B., Scielzo N., Singh V., Sisti M., Speller D., Taffarello L., Terranova F., Tomei C., Vignati M., Wagaarachchi S., Wang B., Welliver B., Wilson J., Wilson K., Winslow L., Wise T., Zanotti L., Zimmermann S., Zucchelli S., Caminata, A, Adams, D, Alduino, C, Alfonso, K, Avignone, F, Azzolini, O, Bari, G, Bellini, F, Benato, G, Bersani, A, Biassoni, M, Branca, A, Brofferio, C, Bucci, C, Campani, A, Canonica, L, Cao, X, Capelli, S, Cappelli, L, Cardani, L, Carniti, P, Casali, N, Chiesa, D, Chott, N, Clemenza, M, Copello, S, Cosmelli, C, Cremonesi, O, Creswick, R, Cushman, J, D’Addabbo, A, D’Aguanno, D, Dafinei, I, Davis, C, Dell’Oro, S, Deninno, M, Di Domizio, S, Dompè, V, Drobizhev, A, Fang, D, Fantini, G, Faverzani, M, Ferri, E, Ferroni, F, Fiorini, E, Franceschi, M, Freedman, S, Fujikawa, B, Giachero, A, Gironi, L, Giuliani, A, Gorla, P, Gotti, C, Gutierrez, T, Han, K, Heeger, K, Hennings-Yeomans, R, Huang, R, Huang, H, Johnston, J, Keppel, G, Kolomensky, Y, Leder, A, Ligi, C, Ma, Y, Marini, L, Martinez, M, Maruyama, R, Mei, Y, Moggi, N, Morganti, S, Napolitano, T, Nastasi, M, Nones, C, Norman, E, Novati, V, Nucciotti, A, Nutini, I, O’Donnell, T, Ouellet, J, Pagliarone, C, Pallavicini, M, Pattavina, L, Pavan, M, Pessina, G, Pettinacci, V, Pira, C, Pirro, S, Pozzi, S, Previtali, E, Puiu, A, Rosenfeld, C, Rusconi, C, Sakai, M, Sangiorgio, S, Schmidt, B, Scielzo, N, Singh, V, Sisti, M, Speller, D, Taffarello, L, Terranova, F, Tomei, C, Vignati, M, Wagaarachchi, S, Wang, B, Welliver, B, Wilson, J, Wilson, K, Winslow, L, Wise, T, Zanotti, L, Zimmermann, S, Zucchelli, S, Center for Neutrino Physics, and Département de Physique des Particules (ex SPP) (DPhP)
Subjects: lcsh:QC793-793.5, CUORE, Majorana Neutrino, Neutrinoless double beta decay, lower limit, energy resolution, General Physics and Astronomy, bolometer: crystal, 01 natural sciences, 7. Clean energy, Lower limit, neutrinoless double beta decay, law.invention, Nuclear physics, Effective energy, double-beta decay: (0neutrino), Observatory, law, Double beta decay, 0103 physical sciences, talk: Kolymbari 2018/07/04, [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex], tellurium: lifetime, structure, 010306 general physics, Physics, 010308 nuclear & particles physics, background, lcsh:Elementary particle physics, Bolometer, neutrino: Majorana: mass, observatory, Full width at half maximum, experimental results
Abstract: The Cryogenic Underground Observatory for Rare Events (CUORE) is the first bolometric experiment searching for neutrinoless double beta decay that has been able to reach the 1-ton scale. The detector consists of an array of 988 TeO 2 crystals arranged in a cylindrical compact structure of 19 towers, each of them made of 52 crystals. The construction of the experiment was completed in August 2016 and the data taking started in spring 2017 after a period of commissioning and tests. In this work we present the neutrinoless double beta decay results of CUORE from examining a total TeO 2 exposure of 86.3 kg yr , characterized by an effective energy resolution of 7.7 keV FWHM and a background in the region of interest of 0.014 counts / ( keV kg yr ) . In this physics run, CUORE placed a lower limit on the decay half-life of neutrinoless double beta decay of 130 Te &gt, 1.3 &middot, 10 25 yr (90% C.L.). Moreover, an analysis of the background of the experiment is presented as well as the measurement of the 130 Te 2 &nu, &beta, decay with a resulting half-life of T 1 / 2 2 &nu, = [ 7.9 &plusmn, 0.1 ( stat . ) &plusmn, 0.2 ( syst . ) ] &times, 10 20 yr which is the most precise measurement of the half-life and compatible with previous results.
Published: 2018
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75. Background model for the NaI(Tl) crystals in COSINE-100

Author: Seonho Choi, J. H. Jo, H. Prihtiadi, E. Barbosa de Souza, A. C. Ezeribe, Stephen L. Olsen, M. Kauer, Ju-Yeol Lee, F. Mouton, B.H. Kim, W.A. Lynch, Hongjoo Kim, Reina H. Maruyama, Carsten Rott, K. W. Kim, W. G. Thompson, Y.D. Kim, C. Ha, Govinda Adhikari, N. Carlin, J. Y. Lee, Eunju Jeon, Nam Young Kim, W. Q. Choi, V. A. Kudryavtsev, Kangsoon Park, J.S. Park, A. Scarff, H. W. Joo, Insik Hahn, Hansoo Park, S.H. Yong, Hyangkyu Park, Moo Hyun Lee, M.C. Kim, S. K. Kim, Woon Gu Kang, N. J. C. Spooner, Hyun Su Lee, Mitra Djamal, P. Adhikari, David Leonard, A.J.F. Hubbard, W. Kang, Yong Hamb Kim, Walter C. Pettus, H. J. Kim, S. J. Ra, and Liang Yang
Subjects: Physics - Instrumentation and Detectors, Physics and Astronomy (miscellaneous), Regular Article - Experimental Physics, Monte Carlo method, Dark matter, FOS: Physical sciences, lcsh:Astrophysics, 01 natural sciences, Particle detector, Nuclear physics, lcsh:QB460-466, 0103 physical sciences, lcsh:Nuclear and particle physics. Atomic energy. Radioactivity, 010306 general physics, Engineering (miscellaneous), Instrumentation and Methods for Astrophysics (astro-ph.IM), Background radiation, Physics, Isotope, 010308 nuclear & particles physics, Instrumentation and Detectors (physics.ins-det), Scintillation counter, Measuring instrument, lcsh:QC770-798, Astrophysics - Instrumentation and Methods for Astrophysics, Radioactive decay
Abstract: The COSINE-100 dark matter search experiment is an array of NaI(Tl) crystal detectors located in the Yangyang Underground Laboratory (Y2L). To understand measured backgrounds in the NaI(Tl) crystals we have performed Monte Carlo simulations using the Geant4 toolkit and developed background models for each crystal that consider contributions from both internal and external sources, including cosmogenic nuclides. The background models are based on comparisons of measurement data with Monte Carlo simulations that are guided by a campaign of material assays and are used to evaluate backgrounds and identify their sources. The average background level for the six crystals (70 kg total mass) that are studied is 3.5 counts/day/keV/kg in the (2–6) keV energy interval. The dominant contributors in this energy region are found to be \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$^{210}$$\end{document}210Pb and \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$^3$$\end{document}3H.
Published: 2018

76. Results from phase 1 of the HAYSTAC microwave cavity axion experiment

Author: William Kindel, Maxime Malnou, Danielle Speller, J. R. Root, L. Zhong, Sidney Cahn, S. Al Kenany, Gianpaolo Carosi, Daniel Palken, K. van Bibber, K. M. Backes, Maria Simanovskaia, S. K. Lamoreaux, I. Urdinaran, Reina H. Maruyama, B. M. Brubaker, Y. V. Gurevich, Nicholas M. Rapidis, Samantha M. Lewis, Konrad Lehnert, and T. M. Shokair
Subjects: Physics, Physics - Instrumentation and Detectors, 010308 nuclear & particles physics, Quantum limit, Dark matter, FOS: Physical sciences, Instrumentation and Detectors (physics.ins-det), Coupling (probability), 01 natural sciences, High Energy Physics - Experiment, High Energy Physics - Experiment (hep-ex), 0103 physical sciences, Sensitivity (control systems), Atomic physics, Parametric oscillator, 010306 general physics, Axion, Order of magnitude, Microwave cavity
Abstract: We report on the results from a search for dark matter axions with the HAYSTAC experiment using a microwave cavity detector at frequencies between 5.6 and 5.8 GHz. We exclude axion models with two photon coupling gaγγ≳2×10−14 GeV−1, a factor of 2.7 above the benchmark KSVZ model over the mass range 23.15
Published: 2018
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77. First Results from CUORE: A Search for Lepton Number Violation via 0νββ Decay of Te130

Author: R. Gaigher, Massimiliano Clemenza, Carlo Cosmelli, Marisa Pedretti, M. M. Deninno, C. Nones, F. Rimondi, R. Cereseto, I. Dafinei, C. Brofferio, G. Pessina, K. Wilson, Davide Chiesa, A. Caminata, Ezio Previtali, Marco Pallavicini, Jonathan Ouellet, Y. G. Ma, G. Bari, B. Welliver, C. Crescentini, H. Z. Huang, Jeffrey W. Beeman, M. Capodiferro, N. D. Scielzo, G. Keppel, K. E. Lim, E. V. Hansen, A. Bersani, Lucia Canonica, Stefano Dell'Oro, J. Schmidt, L. Ioannucci, S. Di Domizio, V. Pettinacci, F. Bellini, X. Liu, N. Casali, D. D'Aguanno, L. Gladstone, F. Bragazzi, D. Schaeffer, A. Giuliani, M. Guerzoni, P. J. Mosteiro, J. Wallig, C. Maiano, C. Zarra, Laura Cardani, I. C. Bandac, S. S. Nagorny, M. Pavan, R. J. Creswick, N. Chott, B. K. Fujikawa, C. Rusconi, R. Hennings-Yeomans, S. L. Wagaarachchi, Eric B. Norman, C. Pagliarone, M. Vignati, B. X. Zhu, C. Martinez Amaya, C. Arnaboldi, Lindley Winslow, R. W. Kadel, Stefano Zucchelli, S. Zimmermann, K. Alfonso, F. Reindl, M. L. Di Vacri, M. Maino, C. Rossi, M. Faverzani, M. Iannone, C. Bucci, T. D. Gutierrez, Miriam Lucio Martinez, Irene Nutini, Vladimir Datskov, B. S. Wang, G. Ventura, L. Tatananni, A. Chiarini, F. Stivanello, S. Copello, T. I. Banks, Paolo Carniti, C. Bulfon, M. Balata, L. Pattavina, C. Salvioni, L. Zanotti, Jeremy S. Cushman, L. Gironi, G. Piperno, M. Tenconi, F. T. Avignone, F. Orio, Claudio Gotti, M. Cariello, L. Taffarello, B. Schmidt, V. Novati, Virendra Singh, Oliviero Cremonesi, J. Goett, Guimin Zhang, Y. Mei, C. Pira, M. Tessaro, E. Andreotti, O. Azzolini, L. Di Paolo, A. D'Addabbo, Larissa M. Ejzak, M. Sakai, Silvia Capelli, S. Pirro, Xi-Guang Cao, Massimiliano Nastasi, Carlo Ligi, M. Barucci, D. Biare, K. M. Heeger, M. Carrettoni, C. Rosenfeld, P. Gorla, F. Ferroni, C. Tomei, A. Bryant, Emanuele Ferri, Eugene E. Haller, G. Ceruti, C. J. Davis, A. Camacho, L. Kogler, S. Morganti, F. Terranova, S. Pozzi, E. Olivieri, James R. Wilson, E. Fiorini, A. Pelosi, Alan R. Smith, Ke Han, A. Branca, Reina H. Maruyama, N. Moggi, H. W. Wang, Stuart J. Freedman, T. O'Donnell, A. Leder, L. Risegari, Samuele Sangiorgio, Stefano Nisi, T. Wise, A. Nucciotti, M. Sisti, C. Alduino, D. Santone, Yu. G. Kolomensky, Luigi Cappelli, F. Alessandria, R. Pedrotta, D. Conventi, L. Marini, Kevin Hickerson, C. Guandalini, E. Sala, V. Palmieri, A. Giachero, T. Napolitano, D. Q. Fang, M. Biassoni, A. Buccheri, M. Olcese, F. Del Corso, R. Faccini, Giovanni Benato, L. Cassina, A. Drobizhev, D. Orlandi, and M. A. Franceschi
Subjects: Physics, Particle physics, 010308 nuclear & particles physics, Bolometer, Statistical sensitivity, General Physics and Astronomy, 01 natural sciences, Lepton number, law.invention, MAJORANA, Full width at half maximum, CUORE, law, Double beta decay, 0103 physical sciences, Neutrino, 010306 general physics
Abstract: The CUORE experiment, a ton-scale cryogenic bolometer array, recently began operation at the Laboratori Nazionali del Gran Sasso in Italy. The array represents a significant advancement in this technology, and in this work we apply it for the first time to a high-sensitivity search for a lepton-number-violating process: ^{130}Te neutrinoless double-beta decay. Examining a total TeO_{2} exposure of 86.3 kg yr, characterized by an effective energy resolution of (7.7±0.5) keV FWHM and a background in the region of interest of (0.014±0.002) counts/(keV kg yr), we find no evidence for neutrinoless double-beta decay. Including systematic uncertainties, we place a lower limit on the decay half-life of T_{1/2}^{0ν}(^{130}Te)>1.3×10^{25} yr (90% C.L.); the median statistical sensitivity of this search is 7.0×10^{24} yr. Combining this result with those of two earlier experiments, Cuoricino and CUORE-0, we find T_{1/2}^{0ν}(^{130}Te)>1.5×10^{25} yr (90% C.L.), which is the most stringent limit to date on this decay. Interpreting this result as a limit on the effective Majorana neutrino mass, we find m_{ββ}
Published: 2018
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78. Cracking Behaviors Caused by the Corrosion of Reinforcing Bars in RC Columns

Author: Y. Gakuhari, Y. Shinohara, and H. Maruyama
Subjects: Cracking, Materials science, Composite material, Rc columns, Corrosion
Published: 2015

79. Measurement of Atmospheric Neutrino Oscillations at 6–56 GeV with IceCube DeepCore

Author: P. Schlunder, R. Hellauer, Sally Robertson, S. De Ridder, F. Bos, Dirk Lennarz, Gisela Anton, M. E. Huber, Allan Hallgren, L. Classen, T. Kittler, S. Flis, M. Labare, J. Werthebach, K. Clark, A. Wallace, Darren Grant, Sarah Nowicki, G. H. Collin, Piotr Kalaczyński, C. Pérez de los Heros, F. D. Wandler, M. Brenzke, J. P. A. M. de André, L. Gerhardt, Minjin Jeong, M. Vehring, D. F. Cowen, J. P. Barron, S. Yoshida, Stijn Vanheule, Maryon Ahrens, Frederik Tenholt, M. Rameez, M. Medici, A. Waza, Philipp Eller, Thomas Meures, E. Woolsey, G. Binder, P. B. Price, T. O. B. Schmidt, Francis Halzen, Joshua Pepper, Karim Ghorbani, S. Coenders, K. Helbing, Christian Spiering, Sarah Mancina, Spencer Axani, K. Jero, Joshua A. Wood, I. Ansseau, T. R. Wood, Kurt Woschnagg, Elisa Bernardini, A. Terliuk, Justin Vandenbroucke, Paul Evenson, S. Schöneberg, H. Dembinski, Frank McNally, Chunfai Tung, Klas Hultqvist, J. Kiryluk, J. Felde, Xinhua Bai, K. Andeen, E. Jacobi, A. Kyriacou, D. Berley, Benjamin Hokanson-Fasig, W. Giang, J. L. Lanfranchi, P. Nakarmi, Carlos Arguelles, Janet Conrad, Dmitry Chirkin, F. Bradascio, A. Obertacke Pollmann, I. Al Samarai, J. L. Kelley, Alexander Kappes, C. Walck, Jessie Micallef, R. Cross, M. Rongen, Joshua Hignight, K. Krings, M. S. Sutherland, M. Börner, Markus Ahlers, S. Tilav, U. Katz, E. Pinat, K. Rawlins, George Japaridze, Roger Moore, Ramesh Koirala, Dennis Soldin, A. Christov, William Luszczak, Frederik Hermann Lauber, Jenni Adams, S. Hickford, D. J. Koskinen, Simona Toscano, M. Kauer, M. Zoll, S. Westerhoff, James Madsen, J. Bourbeau, E. Blaufuss, Lu Lu, Donglian Xu, Yiqian Xu, J. Tatar, Samvel Ter-Antonyan, D. Bose, R. G. Stokstad, M. J. Larson, Seongjin In, Hermann Kolanoski, Elisa Resconi, M. N. Tobin, M. Song, T. L. Carver, Mike Richman, J. Becker Tjus, A. Stasik, J. P. Dumm, Subir Sarkar, E. Cheung, M. Usner, T. Palczewski, Dirk Ryckbosch, M. Day, C. Kopper, Teresa Montaruli, T. Karg, R. Maunu, T. Kuwabara, E. Vogel, M. Stamatikos, J. Braun, T. Stezelberger, Jan Soedingrekso, B. Eberhardt, Kendall Mahn, Jae Yool Kim, J. Stachurska, N. L. Strotjohann, T. Menne, L. Rädel, J. Casey, S. Schoenen, D. Bindig, A. Franckowiak, D. Heereman, B. Relethford, P. Peiffer, Konstancja Satalecka, Theo Glauch, A. Goldschmidt, Gerald Przybylski, Z. Griffith, Marjon Moulai, S. Kunwar, K. Meagher, Jay Gallagher, J. C. Díaz-Vélez, Azadeh Keivani, C. F. Turley, G. Krückl, Matthias Vraeghe, N. Kurahashi, B. J. Whelan, Todor Stanev, G. Tešić, T. Anderson, E. Friedman, A. Olivas, Delia Tosi, Mirco Hunnefeld, C. Wendt, F. Huang, M. Dunkman, G. de Wasseige, J. Stettner, D. R. Nygren, J. Lünemann, C. De Clercq, J. J. Beatty, Tianlu Yuan, K. Hoshina, M. Lesiak-Bzdak, R. Hoffmann, Glenn Spiczak, G. Momenté, M. Tselengidou, M. G. Aartsen, Thomas K. Gaisser, G. B. Yodh, U. Naumann, K. H. Becker, T. Kintscher, Marsha J. Wolf, E. Unger, Javier Gonzalez, D. Rysewyk, Giorgio Maggi, K. Wiebe, Marek Kowalski, David A. Williams, B. J. P. Jones, T. Sälzer, Markus Ackermann, A. Stößl, H. Bagherpour, Olga Botner, Reina H. Maruyama, M. Relich, V. Baum, Chris Weaver, G. Merino, Kirill Filimonov, M. Kroll, N. Wandkowsky, K. D. de Vries, H. Dujmovic, J. P. Koschinsky, R. Nahnhauer, L. Schumacher, Carsten Rott, D. V. Pankova, M. Casier, M. Leuermann, L. Wills, Surujhdeo Seunarine, G. Kohnen, J. P. Yanez, A. Steuer, Juanan Aguilar, N. van Eijndhoven, J. Kunnen, S. Böser, R. C. Bay, A. Ishihara, D. Z. Besson, Xianwu Xu, Damian Pieloth, J. Sandroos, D. Altmann, Austin Schneider, Ali Kheirandish, J. Auffenberg, W. Van Driessche, G. W. Sullivan, Jannes Brostean-Kaiser, T. Fuchs, L. Köpke, Albrecht Karle, L. Brayeur, I. Taboada, Segev BenZvi, Spencer Klein, Kara Hoffman, Won Nam Kang, Hershal Pandya, Wolfgang Rhode, J. J. DeLaunay, G. Neer, Tim Ruhe, J. van Santen, Kael Hanson, M. Plum, S. Bron, Steven W. Barwick, Maximilian Meier, Paolo Desiati, T. Ehrhardt, Alexander Sandrock, D. Hebecker, K. Mase, Andrea Turcati, Stijn Blot, C. Haack, M. J. Weiss, R. Reimann, S. Kopper, Christopher Wiebusch, Christian Bohm, Aongus O'Murchadha, Christoph Raab, G. C. Hill, Bunheng Ty, D. Seckel, S. Fahey, S. Miarecki, A. R. Fazely, Tyce DeYoung, P. A. Toale, Immacolata Carmen Rea, B. Eichmann, H.-P. Bretz, M. Kim, L. Wille, S. E. Sanchez Herrera, Hans Niederhausen, V. di Lorenzo, C. Finley, A. Burgman, Qinrui Liu, T. Glüsenkamp, M. Wallraff, Physics, Elementary Particle Physics, Vriendenkring VUB, Faculty of Sciences and Bioengineering Sciences, Massachusetts Institute of Technology. Department of Physics, Arguelles Delgado, Carlos A, Axani, Spencer Nicholas, Collin, G. H., Conrad, Janet Marie, Moulai, Marjon H., Al Samarai, Imen, Bron, Stéphanie, Carver, Tessa, Christov, Asen, and Montaruli, Teresa
Subjects: interaction [cosmic radiation], Physics::Instrumentation and Detectors, Solar neutrino, General Physics and Astronomy, 01 natural sciences, 7. Clean energy, High Energy Physics - Experiment, IceCube, Subatomär fysik, High Energy Physics - Experiment (hep-ex), Observatory, Subatomic Physics, TOOL, Physics, oscillation [neutrino], Astrophysics::Instrumentation and Methods for Astrophysics, atmosphere [neutrino], threshold [energy], mass difference [neutrino], ddc, observatory, Neutrino detector, Physique des particules élémentaires, Astrophysics::Earth and Planetary Astrophysics, Neutrino, Particle physics, cosmic radiation [neutrino], accelerator, Astrophysics::High Energy Astrophysical Phenomena, FOS: Physical sciences, ddc:500.2, Physics and Astronomy(all), IceCube Neutrino Observatory, Physics and Astronomy (all), 0103 physical sciences, neutrino/mu, ddc:530, energy: high [neutrino], 010306 general physics, Neutrino oscillation, Astroparticle physics, 010308 nuclear & particles physics, ICE, High Energy Physics::Phenomenology, Astronomy, Solar neutrino problem, Physics and Astronomy, 13. Climate action, mass [neutrino], High Energy Physics::Experiment, SYSTEM, mixing angle [neutrino], experimental results
Abstract: We present a measurement of the atmospheric neutrino oscillation parameters using three years of data from the IceCube Neutrino Observatory. The DeepCore infill array in the center of IceCube enables the detection and reconstruction of neutrinos produced by the interaction of cosmic rays in Earth's atmosphere at energies as low as ∼5 GeV. That energy threshold permits measurements of muon neutrino disappearance, over a range of baselines up to the diameter of the Earth, probing the same range of L/Eν as long-baseline experiments but with substantially higher-energy neutrinos. This analysis uses neutrinos from the full sky with reconstructed energies from 5.6 to 56 GeV. We measure Δm322=2.31-0.13+0.11×10-3 eV2 and sin2θ23=0.51-0.09+0.07, assuming normal neutrino mass ordering. These results are consistent with, and of similar precision to, those from accelerator- and reactor-based experiments., 0, SCOPUS: ar.j, info:eu-repo/semantics/published
Published: 2018
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80. Study of Rare Nuclear Processes with CUORE

Author: C. Pira, L. Canonica, L. Marini, T. Wise, L. Taffarello, C. Pagliarone, Vasundhara Singh, A. Bersani, B. Schmidt, B. S. Wang, O. Azzolini, Carlo Cosmelli, L. Gladstone, H. Z. Huang, G. Keppel, K. E. Lim, C. Brofferio, Davide Chiesa, C. Rusconi, A. Drobizhev, R. J. Creswick, M. Faverzani, Oliviero Cremonesi, M. M. Deninno, M. A. Franceschi, Marco Pallavicini, L. Pattavina, L. Gironi, F. Bellini, F. T. Avignone, Jeremy S. Cushman, G. Pessina, M. Pavan, C. Rosenfeld, S. Pirro, Nicholas Scielzo, P. Gorla, F. Ferroni, C. Tomei, Emanuele Ferri, C. J. Davis, A. Camacho, James R. Wilson, Giovanni Benato, C. Bucci, T. D. Gutierrez, H. W. Wang, T. O'Donnell, Monica Sisti, V. Palmieri, S. Di Domizio, D. Q. Fang, N. Casali, S. Zucchelli, Eric B. Norman, Laura Cardani, B. K. Fujikawa, Stefano Pozzi, T. Napolitano, N. Moggi, Silvia Capelli, F. Reindl, M. Vignati, Massimiliano Nastasi, V. Novati, M. Biassoni, C. Nones, Samuele Sangiorgio, A. Nucciotti, C. Alduino, K. Wilson, Ettore Fiorini, Jonathan Ouellet, G. Bari, Andrea Giachero, K. Alfonso, M. I. Martínez, M. L. Di Vacri, Lorenzo Cassina, Yu. G. Kolomensky, D. Santone, S. Zimmermann, Ioan Dafinei, S. Copello, L. Zanotti, Paolo Carniti, Claudio Gotti, Stefano Dell'Oro, M. Clemenza, A. Giuliani, N. Chott, S. L. Wagaarachchi, D. D'Aguanno, S. Morganti, S. S. Nagorny, Lindley Winslow, L. Cappelli, A. Leder, Irene Nutini, Y. Mei, V. Dompè, Yu-Gang Ma, A. Caminata, M. Sakai, Ezio Previtali, R. Hennings-Yeomans, Xi-Guang Cao, A. D'Addabbo, B. Welliver, K. M. Heeger, Carlo Ligi, J. Schmidt, Ke Han, A. Branca, Reina H. Maruyama, Stuart J. Freedman, F. Terranova, Guimin Zhang, Centre de Sciences Nucléaires et de Sciences de la Matière (CSNSM), 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), Département de Physique des Particules (ex SPP) (DPP), Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, CUORE, Alduino, C., Alfonso, K., Avignone, F.T., Azzolini, O., Bari, G., Bellini, F., Benato, G., Bersani, A., Biassoni, M., Branca, A., Brofferio, C., Bucci, C., Camacho, A., Caminata, A., Canonica, L., Cao, X.G., Capelli, S., Cappelli, L., Cardani, L., Carniti, P., Casali, N., Cassina, L., Chiesa, D., Chott, N., Clemenza, M., Copello, S., Cosmelli, C., Cremonesi, O., Creswick, R.J., Cushman, J.S., D'Addabbo, A., D'Aguanno, D., Dafinei, I., Davis, C.J., Dell'Oro, S., Deninno, M.M., Di Domizio, S., Di Vacri, M.L., Dompe, V., Drobizhev, A., Fang, D.Q., Faverzani, M., Ferri, E., Ferroni, F., Fiorini, E., Franceschi, M.A., Freedman, S.J., Fujikawa, B.K., Giachero, A., Gironi, L., Giuliani, A., Gladstone, L., Gorla, P., Gotti, C., Gutierrez, T.D., Han, K., Heeger, K.M., Hennings-Yeomans, R., Huang, H.Z., Keppel, G., Kolomensky, Yu.G., Leder, A., Ligi, C., Lim, K.E., Ma, Y.G., Marini, L., Martinez, M., Maruyama, R.H., Mei, Y., Moggi, N., Morganti, S., Nagorny, S.S., Napolitano, T., Nastasi, M., Nones, C., Norman, E.B., Novati, V., Nucciotti, A., Nutini, I., O'Donnell, T., Ouellet, J.L., Pagliarone, C.E., Pallavicini, M., Palmieri, V., Pattavina, L., Pavan, M., Pessina, G., Pira, C., Pirro, S., Pozzi, S., Previtali, E., Reindl, F., Rosenfeld, C., Rusconi, C., Sakai, M., Sangiorgio, S., Santone, D., Schmidt, B., Schmidt, J., Scielzo, N.D., Singh, V., Sisti, M., Taffarello, L., Terranova, F., Tomei, C., Vignati, M., Wagaarachchi, S.L., Wang, B.S., Wang, H.W., Welliver, B., Wilson, J., Wilson, K., Winslow, L.A., Wise, T., Zanotti, L., Zhang, G.Q., Zimmermann, S., Zucchelli, S., Centre de Sciences Nucléaires et de Sciences de la Matière ( CSNSM ), 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 ), Département de Physique des Particules (ex SPP) ( DPP ), Institut de Recherches sur les lois Fondamentales de l'Univers ( IRFU ), Commissariat à l'énergie atomique et aux énergies alternatives ( CEA ) -Université Paris-Saclay-Commissariat à l'énergie atomique et aux énergies alternatives ( CEA ) -Université Paris-Saclay, Alduino, C, Alfonso, K, Avignone, F, Azzolini, O, Bari, G, Bellini, F, Benato, G, Bersani, A, Biassoni, M, Branca, A, Brofferio, C, Bucci, C, Camacho, A, Caminata, A, Canonica, L, Cao, X, Capelli, S, Cappelli, L, Cardani, L, Carniti, P, Casali, N, Cassina, L, Chiesa, D, Chott, N, Clemenza, M, Copello, S, Cosmelli, C, Cremonesi, O, Creswick, R, Cushman, J, D’Addabbo, A, D’Aguanno, D, Dafinei, I, Davis, C, Dell’Oro, S, Deninno, M, Di Domizio, S, Di Vacri, M, Dompè, V, Drobizhev, A, Fang, D, Faverzani, M, Ferri, E, Ferroni, F, Fiorini, E, Franceschi, M, Freedman, S, Fujikawa, B, Giachero, A, Gironi, L, Giuliani, A, Gladstone, L, Gorla, P, Gotti, C, Gutierrez, T, Han, K, Heeger, K, Hennings-Yeomans, R, Huang, H, Keppel, G, Kolomensky, Y, Leder, A, Ligi, C, Lim, K, Ma, Y, Marini, L, Martinez, M, Maruyama, R, Mei, Y, Moggi, N, Morganti, S, Nagorny, S, Napolitano, T, Nastasi, M, Nones, C, Norman, E, Novati, V, Nucciotti, A, Nutini, I, O’Donnell, T, Ouellet, J, Pagliarone, C, Pallavicini, M, Palmieri, V, Pattavina, L, Pavan, M, Pessina, G, Pira, C, Pirro, S, Pozzi, S, Previtali, E, Reindl, F, Rosenfeld, C, Rusconi, C, Sakai, M, Sangiorgio, S, Santone, D, Schmidt, B, Schmidt, J, Scielzo, N, Singh, V, Sisti, M, Taffarello, L, Terranova, F, Tomei, C, Vignati, M, Wagaarachchi, S, Wang, B, Wang, H, Welliver, B, Wilson, J, Wilson, K, Winslow, L, Wise, T, Zanotti, L, Zhang, G, Zimmermann, S, Zucchelli, S, and Département de Physique des Particules (ex SPP) (DPhP)
Subjects: Second-order weak decay, Particle physics, CUORE, Double beta decay, Low-temperature detectors, Rare events searches, Second-order weak decays, Atomic and Molecular Physics, and Optics, Nuclear and High Energy Physics, Astronomy and Astrophysics, Physics - Instrumentation and Detectors, Atomic and Molecular Physics, and Optic, rare events searches, FOS: Physical sciences, double beta decay, [PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex], 7. Clean energy, 01 natural sciences, Low-temperature detector, low-temperature detectors, 23.40.-s, 07.57.Kp, second-order weak decays, Atomic and Molecular Physics, 0103 physical sciences, [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], Nuclear Experiment (nucl-ex), [ PHYS.NEXP ] Physics [physics]/Nuclear Experiment [nucl-ex], Detector array, 010306 general physics, Nuclear Experiment, [ PHYS.PHYS.PHYS-INS-DET ] Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], Nuclear and High Energy Physic, Physics, 010308 nuclear & particles physics, Instrumentation and Detectors (physics.ins-det), Neutrino, and Optics, Rare events searche, Tellurium compounds, FIS/04 - FISICA NUCLEARE E SUBNUCLEARE, Radioactive decay, 07.20.Mc
Abstract: TeO2 bolometers have been used for many years to search for neutrinoless double beta decay in 130-Te. CUORE, a tonne-scale TeO2 detector array, recently published the most sensitive limit on the half-life, $T_{1/2}^{0��} > 1.5 \times 10^{25}\,$yr, which corresponds to an upper bound of $140-400$~meV on the effective Majorana mass of the neutrino. While it makes CUORE a world-leading experiment looking for neutrinoless double beta decay, it is not the only study that CUORE will contribute to in the field of nuclear and particle physics. As already done over the years with many small-scale experiments, CUORE will investigate both rare decays (such as the two-neutrino double beta decay of 130-Te and the hypothesized electron capture in 123-Te), and rare processes (e.g., dark matter and axion interactions). This paper describes some of the achievements of past experiments that used TeO2 bolometers, and perspectives for CUORE., 36 pages, 13 figures, sumbitted to IJMPA Special Issue "Results and Developments in the investigation of rare nuclear decays and processes"
Published: 2018
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81. Searching for Neutrinoless Double-Beta Decay of130Te with CUORE

Author: A. De Biasi, M. Balata, N. Casali, P. Gorla, F. Ferroni, C. Tomei, F. Orio, Carlo Ligi, Alan R. Smith, Emanuele Ferri, Eugene E. Haller, M. Tenconi, B. S. Wang, B. X. Zhu, M. Faverzani, Massimiliano Clemenza, Davide Chiesa, O. Azzolini, M. Carrettoni, Marco Pallavicini, H. A. Farach, V. Pettinacci, A. Giuliani, G. Bari, X. Liu, Simone Capelli, R. W. Kadel, James R. Wilson, L. Cardani, N. Chott, G. Fernandes, N. Moggi, Oliviero Cremonesi, G. Pessina, Stuart Freedman, Ke Han, Reina H. Maruyama, Jeffrey W. Beeman, J. Goett, Yingqi Ma, T. Wise, R. J. Creswick, G. Keppel, D. R. Artusa, Monica Sisti, Y. L. Li, A. Bersani, V. Rampazzo, Marisa Pedretti, Samuele Sangiorgio, Stefano Nisi, H. Z. Huang, A. Nucciotti, G. Piperno, Elena Sala, Y. Mei, V. Palmieri, A. Dally, Yu G. Kolomensky, R. Hennings-Yeomans, Xi-Guang Cao, K. M. Heeger, Eric B. Norman, Ettore Fiorini, Silvio Morganti, L. Gironi, A. Woodcraft, T. I. Banks, C. Maiano, S. Pirro, T. Napolitano, G. Ventura, S. Trentalange, Lindley Winslow, F. T. Avignone, Nicholas Scielzo, Andrea Giachero, X. Z. Cai, F. Terranova, S. Di Domizio, M. Biassoni, C. Zarra, L. Wielgus, W. D. Tian, M. M. Deninno, M. Maino, B. K. Fujikawa, Claudio Gotti, L. Taffarello, C. Nones, J. L. Ouellet, K. Kazkaz, M. L. Di Vacri, H. W. Wang, C. Cosmelli, T. O'Donnell, C. Bucci, T. D. Gutierrez, M. Vignati, C. Rusconi, S. Copello, S. Zucchelli, C. Pira, Larissa M. Ejzak, F. Bellini, D. Orlandi, M. A. Franceschi, C. Brofferio, Alejandro E. Camacho, D. Q. Fang, L. Carbone, Ezio Previtali, L. Pattavina, L. Zanotti, L. Canonica, M. I. Martínez, M. Pavan, Ioan Dafinei, Vladimir Datskov, C. Rosenfeld, Artusa, D.R., Avignone, F.T., Azzolini, O., Balata, M., Banks, T.I., Bari, G., Beeman, J., Bellini, F., Bersani, A., Biassoni, M., Brofferio, C., Bucci, C., Cai, X.Z., Camacho, A., Canonica, L., Cao, X.G., Capelli, S., Carbone, L., Cardani, L., Carrettoni, M., Casali, N., Chiesa, D., Chott, N., Clemenza, M., Copello, S., Cosmelli, C., Cremonesi, O., Creswick, R.J., Dafinei, I., Dally, A., Datskov, V., De Biasi, A., Deninno, M.M., Di Domizio, S., Di Vacri, M.L., Ejzak, L., Fang, D.Q., Farach, H.A., Faverzani, M., Fernandes, G., Ferri, E., Ferroni, F., Fiorini, E., Franceschi, M.A., Freedman, S.J., Fujikawa, B.K., Giachero, A., Gironi, L., Giuliani, A., Goett, J., Gorla, P., Gotti, C., Gutierrez, T.D., Haller, E.E., Han, K., Heeger, K.M., Hennings-Yeomans, R., Huang, H.Z., Kadel, R., Kazkaz, K., Keppel, G., Kolomensky, Yu.G., Li, Y.L., Ligi, C., Liu, X., Ma, Y.G., Maiano, C., Maino, M., Martinez, M., Maruyama, R.H., Mei, Y., Moggi, N., Morganti, S., Napolitano, T., Nisi, S., Nones, C., Norman, E.B., Nucciotti, A., O'Donnell, T., Orio, F., Orlandi, D., Ouellet, J.L., Pallavicini, M., Palmieri, V., Pattavina, L., Pavan, M., Pedretti, M., Pessina, G., Pettinacci, V., Piperno, G., Pira, C., Pirro, S., Previtali, E., Rampazzo, V., Rosenfeld, C., Rusconi, C., Sala, E., Sangiorgio, S., Scielzo, N.D., Sisti, M., Smith, A.R., Taffarello, L., Tenconi, M., Terranova, F., Tian, W.D., Tomei, C., Trentalange, S., Ventura, G., Vignati, M., Wang, B.S., Wang, H.W., Wielgus, L., Wilson, J., Winslow, L.A., Wise, T., Woodcraft, A., Zanotti, L., Zarra, C., Zhu, B.X., Zucchelli, S., Artusa, D, Avignone, F, Azzolini, O, Balata, M, Banks, T, Bari, G, Beeman, J, Bellini, F, Bersani, A, Biassoni, M, Brofferio, C, Bucci, C, Cai, X, Camacho, A, Canonica, L, Cao, X, Capelli, S, Carbone, L, Cardani, L, Carrettoni, M, Casali, N, Chiesa, D, Chott, N, Clemenza, M, Copello, S, Cosmelli, C, Cremonesi, O, Creswick, R, Dafinei, I, Dally, A, Datskov, V, De Biasi, A, Deninno, M, Di Domizio, S, Di Vacri, M, Ejzak, L, Fang, D, Farach, H, Faverzani, M, Fernandes, G, Ferri, E, Ferroni, F, Fiorini, E, Franceschi, M, Freedman, S, Fujikawa, B, Giachero, A, Gironi, L, Giuliani, A, Goett, J, Gorla, P, Gotti, C, Gutierrez, T, Haller, E, Han, K, Heeger, K, Hennings Yeomans, R, Huang, H, Kadel, R, Kazkaz, K, Keppel, G, Kolomensky, Y, Li, Y, Ligi, C, Liu, X, Ma, Y, Maiano, C, Maino, M, Martinez, M, Maruyama, R, Mei, Y, Moggi, N, Morganti, S, Napolitano, T, Nisi, S, Nones, C, Norman, E, Nucciotti, A, O'Donnell, T, Orio, F, Orlandi, D, Ouellet, J, Pallavicini, M, Palmieri, V, Pattavina, L, Pavan, M, Pedretti, M, Pessina, G, Pettinacci, V, Piperno, G, Pira, C, Pirro, S, Previtali, E, Rampazzo, V, Rosenfeld, C, Rusconi, C, Sala, E, Sangiorgio, S, Scielzo, N, Sisti, M, Smith, A, Taffarello, L, Tenconi, M, Terranova, F, Tian, W, Tomei, C, Trentalange, S, Ventura, G, Vignati, M, Wang, B, Wang, H, Wielgus, L, Wilson, J, Winslow, L, Wise, T, Woodcraft, A, Zanotti, L, Zarra, C, Zhu, B, and Zucchelli, S
Subjects: Neutrinoless double-beta, Nuclear and High Energy Physics, Particle physics, Physics - Instrumentation and Detectors, FOS: Physical sciences, RESPONSE STABILIZATION, 7. Clean energy, VALIDATION, Nuclear physics, CUORICINO, CUORE, Double beta decay, DETECTORS, Nuclear Experiment (nucl-ex), Nuclear Experiment, Physics, BOLOMETERS, Half-life, Instrumentation and Detectors (physics.ins-det), Beta decay, lcsh:QC1-999, 3. Good health, MAJORANA, RARE EVENTS, High Energy Physics::Experiment, Nuclear and High Energy Physics. RADIOACTIVE CONTAMINATION, Neutrino, lcsh:Physics, Radioactive decay, Lepton
Abstract: Neutrinoless double-beta ($0\nu\beta\beta$) decay is a hypothesized lepton-number-violating process that offers the only known means of asserting the possible Majorana nature of neutrino mass. The Cryogenic Underground Observatory for Rare Events (CUORE) is an upcoming experiment designed to search for $0\nu\beta\beta$ decay of $^{130}$Te using an array of 988 TeO$_2$ crystal bolometers operated at 10 mK. The detector will contain 206 kg of $^{130}$Te and have an average energy resolution of 5 keV; the projected $0\nu\beta\beta$ decay half-life sensitivity after five years of live time is $1.6\times 10^{26}$ y at $1\sigma$ ($9.5\times10^{25}$ y at the 90% confidence level), which corresponds to an upper limit on the effective Majorana mass in the range 40--100 meV (50--130 meV). In this paper we review the experimental techniques used in CUORE as well as its current status and anticipated physics reach., Comment: 20 pages, 8 figures. Published in Advances in High Energy Physics, Volume 2015 (2015), Article ID 879871
Published: 2015
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82. Searches for small-scale anisotropies from neutrino point sources with three years of IceCube data

Author: H.-P. Bretz, Frank McNally, Jenni Adams, P. B. Price, M. Stamatikos, S. Schoenen, T. O. B. Schmidt, N. Milke, George Japaridze, Thorsten Glusenkamp, T. R. Wood, Kurt Woschnagg, Paul Evenson, K. Hoshina, W. Huelsnitz, S. Hickford, Glenn Spiczak, K. Helbing, R. G. Stokstad, J. C. Groh, C. Pérez de los Heros, Dmitry Chirkin, Matthias Vraeghe, P. O. Hulth, J. Eisch, A. Goldschmidt, Elisa Resconi, M. Schmitz, K. Jero, Matthias Wolf, Alexander Kappes, Björn Eichmann, U. Naumann, Mohamed Rameez, A. Bernhard, E. Unger, B. Ruzybayev, Anatoli Fedynitch, A. Koob, Timo Karg, J.-H. Köhne, H. Wissing, A. O'Murchadha, M. Wellons, Dariusz Gora, L. Schulte, M. Kroll, B. J. Whelan, K. D. de Vries, M. Day, A. Tepe, T. Feusels, R. Maunu, S. Hussain, O. Jlelati, R. Ström, Daniel Bindig, J. C. Gallagher, M. Leuermann, S. Zierke, A. Omairat, F. Bos, Allan Hallgren, M. Relich, D. J. Koskinen, K. Clark, M. Kowalski, Sandro Kopper, T. Kuwabara, J. E. Jacobsen, S. Tilav, P. Hallen, Marcos Santander, Joshua Pepper, A. Tamburro, K. Hultqvist, R. Nahnhauer, E. A. Strahler, M. Danninger, Darren Grant, K. Wiebe, R. Gaior, N. van Eijndhoven, M. Vehring, D. F. Cowen, C. Ha, E. Middell, Elisa Bernardini, Sarah Nowicki, D. Berley, G. C. Hill, L. Gerhardt, L. Mohrmann, J. Felde, Benedikt Riedel, A. Stasik, Maria Tselengidou, Ö. Penek, S. Schöneberg, X. Bai, A. Haj Ismail, Carsten Rott, Hermann Kolanoski, L. Rädel, Thomas Meures, Todor Stanev, Dawn Williams, C. Wendt, K. Rawlins, L. Gladstone, Dirk Heinen, J. L. Kelley, Markus Ahlers, K.-H. Becker, M. Usner, N. L. Strotjohann, D. Seckel, S. Miarecki, E. Middlemas, G. Kroll, M. Bissok, Matt Dunkman, Tyce DeYoung, J. Kiryluk, I. Rees, T. Fischer-Wasels, R. Hoffmann, A. R. Fazely, Gerald Przybylski, P. A. Toale, A. Schukraft, J. Pütz, James Madsen, M. Zoll, Martin Rongen, J. van Santen, J. A. Goodman, E. Pinat, D. T. Larsen, J. J. Beatty, E. Cheung, M. J. Larson, Xianwu Xu, Sofia Vallecorsa, M. Quinnan, C. Walck, R. Eagan, Samvel Ter-Antonyan, A. Kriesten, Dirk Ryckbosch, D. Hellwig, D. R. Nygren, S. Euler, C. Pfendner, Mike Richman, D. Z. Besson, K. Krings, J. P. A. M. de André, A. Homeier, Donglian Xu, A. Terliuk, S. Westerhoff, Ch. Weaver, Christopher Wiebusch, Hans Niederhausen, C. Bohm, Thomas K. Gaisser, G. B. Yodh, M. N. Tobin, Kael Hanson, Nathan Whitehorn, Naoko Kurahashi, O. Schulz, J. Auffenberg, A. Olivas, J. Daughhetee, Gary Binder, Teresa Montaruli, A. Obertacke, A. Franckowiak, Axel Groß, Christian Spiering, K. Frantzen, K. Mase, S. Odrowski, J. Blumenthal, Javier Gonzalez, Subir Sarkar, J. Casey, Chad Finley, J. Posselt, Justin Vandenbroucke, J. Ziemann, P. Gretskov, C. Haack, A. Christov, Giorgio Maggi, C. De Clercq, F. Huang, S. Böser, M. Wallraff, M. Voge, Dennis Soldin, Joakim Sandroos, F. Clevermann, H. Taavola, Paolo Desiati, René Reimann, Y. Sestayo, Olga Botner, Markus Ackermann, S. W. Barwick, L. Classen, Carlos Arguelles, H. G. Sander, E. Blaufuss, D. J. Boersma, J. C. Davis, J. Becker Tjus, V. Baum, J. P. Yanez, G. Tešić, A. Stößl, J. P. Rodrigues, M. W. E. Smith, T. C. Arlen, T. Stezelberger, S. M. Saba, G. W. Sullivan, R. Hellauer, K. Jagielski, Reina H. Maruyama, B. Kaminsky, R. Morse, M. Jurkovic, L. Brayeur, S. Yoshida, Sally Robertson, Tim Ruhe, E. Jacobi, I. Taboada, Dustin Hebecker, S. Flis, M. Casier, J. Lünemann, S. De Ridder, K. Schatto, G. Kohnen, Rezo Shanidze, Juan Carlos Diaz-Velez, M. Labare, J. Feintzeig, Maryon Ahrens, M. Medici, C. Kopper, G. Golup, S. Coenders, Surujhdeo Seunarine, J. Miller, Juanan Aguilar, B. Christy, A. Ishihara, J. Leute, Larissa Paul, F. Scheriau, H. S. Matis, Albrecht Karle, A. Schönwald, Francis Halzen, P. Zarzhitsky, O. Fadiran, D. Altmann, K. Meagher, D. Heereman, M. Kauer, D. Gier, D. Bose, T. Palczewski, C. Wichary, B. Eberhardt, Delia Tosi, M. G. Aartsen, Segev BenZvi, Spencer Klein, Kara Hoffman, A. H. Cruz Silva, Wolfgang Rhode, A. Meli, N. A. Stanisha, T. Anderson, M. Lesiak-Bzdak, P. Redl, Kirill Filimonov, P. Berghaus, J. Kläs, J. Kunnen, Damian Pieloth, Ali Kheirandish, A. M. Brown, T. Fuchs, L. Köpke, Physics, and Elementary Particle Physics
Subjects: J.2, Astrophysics::High Energy Astrophysical Phenomena, FOS: Physical sciences, Cosmic ray, Scale (descriptive set theory), Astrophysics, IceCube, law.invention, Telescope, law, Point (geometry), Anisotropy, astro-ph.HE, 2pt-correlation, High Energy Astrophysical Phenomena (astro-ph.HE), Physics, High Energy Physics::Phenomenology, Astrophysical neutrinos, Extraterrestrial neutrinos, Multipole analysis, Point sources, Astrophysics::Instrumentation and Methods for Astrophysics, Astronomy, Astronomy and Astrophysics, 3. Good health, 85-05, ddc:540, High Energy Physics::Experiment, Neutrino, Astrophysics - High Energy Astrophysical Phenomena, Multipole expansion, Gamma-ray burst
Abstract: Recently, IceCube found evidence for a diffuse signal of astrophysical neutrinos in an energy range of $60\,\mathrm{TeV}$ to the $\mathrm{PeV}$-scale. The origin of those events, being a key to understanding the origin of cosmic rays, is still an unsolved question. So far, analyses have not succeeded to resolve the diffuse signal into point-like sources. Searches including a maximum-likelihood-ratio test, based on the reconstructed directions and energies of the detected down- and up-going neutrino candidates, were also performed on IceCube data leading to the exclusion of bright point sources. In this paper, we present two methods to search for faint neutrino point sources in three years of IceCube data, taken between 2008 and 2011. The first method is an autocorrelation test, applied separately to the northern and southern sky. The second method is a multipole analysis, which expands the measured data in the northern hemisphere into spherical harmonics and uses the resulting expansion coefficients to separate signal from background. With both methods, the results are consistent with the background expectation with a slightly more sparse spatial distribution, corresponding to an underfluctuation. Depending on the assumed number of sources, the resulting upper limit on the flux per source in the northern hemisphere for an $E^{-2}$ energy spectrum ranges from $1.5 \cdot 10^{-8}\,\mathrm{GeV}/(\mathrm{cm}^2 \mathrm{s})$, in the case of one assumed source, to $4 \cdot 10^{-10} \,\mathrm{GeV}/(\mathrm{cm}^2 \mathrm{s})$, in the case of $3500$ assumed sources., Comment: 35 pages, 16 figures, 1 table
Published: 2015
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83. Initial performance of the COSINE-100 experiment

Author: Z. P. Pierpoint, Yong Hamb Kim, S.H. Yong, F. R. Rogers, W. A. Lynch, W.G. Kang, N.Y. Kim, Hongjoo Kim, Hansoo Park, H. Prihtiadi, N. J. C. Spooner, V. A. Kudryavtsev, P. Adhikari, E. Barbosa de Souza, A. C. Ezeribe, Stephen L. Olsen, Kangsoon Park, M. Kauer, J.S. Park, A. Scarff, J. H. Jo, Seonho Choi, Insik Hahn, W. Q. Choi, W. Kang, Liang Yang, W. G. Thompson, Govinda Adhikari, Eunju Jeon, F. Mouton, Jimmy H. M. Lee, H. W. Joo, K. E. Lim, Reina H. Maruyama, Walter C. Pettus, Hyun Su Lee, A. J. F. Hubbard, M.C. Kim, K. W. Kim, Mitra Djamal, Carsten Rott, Moo Hyun Lee, C. Ha, S. J. Ra, H. Kim, Joo Young Lee, B.H. Kim, N. Carlin, Sun Kee Kim, D. S. Leonard, Y.D. Kim, Hyang Kyu Park, Massachusetts Institute of Technology. Department of Physics, and Rogers, Field Rose
Subjects: Physics - Instrumentation and Detectors, Physics and Astronomy (miscellaneous), Dark matter, FOS: Physical sciences, lcsh:Astrophysics, 7. Clean energy, 01 natural sciences, Signal, High Energy Physics - Experiment, High Energy Physics - Experiment (hep-ex), Optics, lcsh:QB460-466, 0103 physical sciences, Trigonometric functions, ddc:530, lcsh:Nuclear and particle physics. Atomic energy. Radioactivity, 010306 general physics, Instrumentation and Methods for Astrophysics (astro-ph.IM), Engineering (miscellaneous), Physics, 010308 nuclear & particles physics, business.industry, Detector, Instrumentation and Detectors (physics.ins-det), Modulation, Electromagnetic shielding, Underground laboratory, lcsh:QC770-798, business, Astrophysics - Instrumentation and Methods for Astrophysics
Abstract: COSINE is a dark matter search experiment based on an array of low background NaI(Tl) crystals located at the Yangyang underground laboratory. The assembly of COSINE-100 was completed in the summer of 2016 and the detector is currently collecting physics quality data aimed at reproducing the DAMA/LIBRA experiment that reported an annual modulation signal. Stable operation has been achieved and will continue for at least 2 years. Here, we describe the design of COSINE-100, including the shielding arrangement, the configuration of the NaI(Tl) crystal detection elements, the veto systems, and the associated operational systems, and we show the current performance of the experiment., Institute for Basic Science ( IBS-R016-A1), University of Illinois at Urbana-Champaign, Alfred P. Sloan Foundation (Fellowship), National Science Foundation (U.S.) (Grant PHY-1457995), National Science Foundation (U.S.) (Grant PHY-1151795), National Science Foundation (U.S.) (Grant DGE-1122492), National Science Foundation (U.S.) (Grant DGE1256259), Wisconsin IceCube Particle Astrophysics Center, University of Wisconsin. Alumni Research Foundation, Yale University, United States. National Nuclear Security Administration (Grant DE-FC52-08NA28752), Science and Technology Facilities Council (Great Britain) (Grant ST/N000277/1), Science and Technology Facilities Council (Great Britain) (Grant ST/K001337/1), Conselho Nacional de Pesquisas (Brazil) (Grant 2017/02952-0 FAPESP)
Published: 2017

84. CUORE: first results and prospects

Author: A. Leder, A. Bersani, T. Wise, D. Santone, Giovanni Benato, Ioan Dafinei, M. Faverzani, Y. u. G. Kolomensky, Ettore Fiorini, J. S. Wilson, L. Taffarello, Oliviero Cremonesi, Andrea Giachero, C. Pagliarone, Laura Cardani, V. Palmieri, R. Hennings-Yeomans, Eric B. Norman, Silvio Morganti, T. D. Gutierrez, F. Terranova, T. Napolitano, B. K. Fujikawa, Stefano Pozzi, M. Biassoni, S. S. Nagorny, Vivek Singh, N. Chott, Ezio Previtali, B. Welliver, K. Alfonso, Luigi Cappelli, Davide Chiesa, Massimiliano Clemenza, Carlo Cosmelli, M. Vignati, K. E. Lim, A. Drobizhev, H. Z. Huang, L. Zanotti, Lindley Winslow, Nicholas Scielzo, Lorenzo Cassina, Laura Gladstone, Deqing Fang, C. Brofferio, Claudia Nones, J. Schmidt, Hongwei Wang, Carlo Ligi, K. Wilson, R. J. Creswick, M. A. Franceschi, T. O'Donnell, C. Rusconi, Jonathan Ouellet, G. Bari, Claudio Gotti, Marco Pallavicini, L. Pattavina, Irene Nutini, N. Casali, Yu-Gang Ma, G. Pessina, M. M. Deninno, F. Reindl, Lucia Canonica, F. Bellini, Guoqiang Zhang, V. Novati, G. Keppel, Ke Han, A. Branca, Reina H. Maruyama, Stefano Pirro, L. Marini, D. D'Aguanno, Y. Mei, M. Sakai, Xi-Guang Cao, K. M. Heeger, M. I. Martínez, A. Giuliani, N. Moggi, V. Dompè, Jeremy S. Cushman, C. Pira, Samuele Sangiorgio, Stefano Dell'Oro, A. Nucciotti, Claudia Tomei, C. Alduino, S. Zimmermann, S. Copello, S. L. Wagaarachchi, Paolo Carniti, Stefano Zucchelli, C. Bucci, B. S. Wang, O. Azzolini, L. Gironi, F. T. Avignone, Silvia Capelli, Massimiliano Nastasi, C. Rosenfeld, P. Gorla, F. Ferroni, Emanuele Ferri, Monica Sisti, C. J. Davis, A. Camacho, Maria Laura Di Vacri, B. Schmidt, A. Caminata, M. Pavan, Sergio Di Domizio, A. D'Addabbo, S. J. Freedman, Centre de Sciences Nucléaires et de Sciences de la Matière (CSNSM), 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), Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, 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), Novati, V, Alduino, C, Alfonso, K, Avignone, F, Azzolini, O, Bari, G, Bellini, F, Benato, G, Bersani, A, Biassoni, M, Branca, A, Brofferio, C, Bucci, C, Camacho, A, Caminata, A, Canonica, L, Cao, X, Capelli, S, Cappelli, L, Cardani, L, Carniti, P, Casali, N, Cassina, L, Chiesa, D, Chott, N, Clemenza, M, Copello, S, Cosmelli, C, Cremonesi, O, Creswick, R, Cushman, J, D'Addabbo, A, D'Aguanno, D, Daﬁnei, I, Davis, C, Dell'Oro, S, Deninno, M, Di Domizio, S, Di Vacri, M, Dompe, V, Drobizhev, A, Fang, D, Faverzani, M, Ferri, E, Ferroni, F, Fiorini, E, Franceschi, M, Freedman, S, Fujikawa, B, Giachero, A, Gironi, L, Giuliani, A, Gladstone, L, Gorla, P, Gotti, C, Gutierrez, T, Han, K, Heeger, K, Hennings-Yeomans, R, Huang, H, Keppel, G, Kolomensky, Y, Leder, A, Ligi, C, Lim, K, Ma, Y, Marini, L, Martinez, M, Maruyama, R, Mei, Y, Moggi, N, Morganti, S, Nagorny, S, Napolitano, T, Nastasi, M, Nones, C, Norman, E, Nucciotti, A, Nutini, I, O'Donnell, T, Ouellet, J, Pagliarone, C, Pallavicini, M, Palmieri, V, Pattavina, L, Pavan, M, Pessina, G, Pira, C, Pirro, S, Pozzi, S, Previtali, E, Reindl, F, Rosenfeld, C, Rusconi, C, Sakai, M, Sangiorgio, S, Santone, D, Schmidt, B, Schmidt, J, Scielzo, N, Singh, V, Sisti, M, Taffarello, L, Terranova, F, Tomei, C, Vignati, M, Wagaarachchi, S, Wang, B, Wang, H, Welliver, B, Wilson, J, Wilson, K, Winslow, L, Wise, T, Zanotti, L, Zhang, G, Zimmermann, S, and Zucchelli, S
Subjects: 7. Clean energy, law.invention, crystal, Nuclear physics, CUORE, bolometer, double-beta decay: (0neutrino), law, Double beta decay, [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex], Cherenkov, Sensitivity (control systems), talk: Uppsala 2017/09/25, Cherenkov radiation, scintillation counter, Physics, lifetime, Scintillation, background, Bolometer, sensitivity, Upgrade, cryogenics, Neutrinoless Double Beta Decay, Cryogenic detector, Scintillating bolometer, Scintillation counter, upgrade, upper limit, experimental results
Abstract: International audience; CUORE is the first bolometric tonne-scale experiment aiming at the investigation of neutrinoless double-beta (0$\nu$2$\beta$) decay of $^{130}$Te. The cryogenic commissioning followed by the detector installation and cool down took place during 2016. After the optimisation of all the detectors, the data-taking started in spring 2017. We report about the results of the first dataset acquired in May, which led to a limit on the 0$\nu$2$\beta$ half-life of $^{130}$Te of 6.6$\times$10$^{24}$ yr. An upgrade of CUORE, named CUPID, is planned to improve the 0$\nu$2$\beta$-decay sensitivity via passive and active background reduction and crystal enrichment. Some technologies for CUPID are currently under study and two of them are presented here, involving the detection of Cherenkov and scintillation light emitted by enriched $^{130}$TeO$_2$ and Li$^{100}_2$MoO$_4$ crystals respectively. This will allow us to reject the currently dominant a background.
Published: 2017
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85. P728Endothelin-1 modifies BMP signaling pathway to induce cyclin D1 in pulmonary artery smooth muscle cells

Author: H. Maruyama, Kazuhiro Aonuma, and S. Sakai
Subjects: Cyclin D1, Smooth muscle, business.industry, medicine.artery, Pulmonary artery, Medicine, Cardiology and Cardiovascular Medicine, business, BMP signaling pathway, Cell biology
Published: 2017
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86. P725BMP2 induces DUSP1 in pulmonary artery smooth muscle cells

Author: Shunsuke Sakai, H. Maruyama, and Kazuhiro Aonuma
Subjects: Pathology, medicine.medical_specialty, Smooth muscle, business.industry, medicine.artery, Pulmonary artery, medicine, Cardiology and Cardiovascular Medicine, business
Published: 2017
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87. Initial performance of the CUORE detector

Author: D. Santone, L. Zanotti, Carlo Ligi, Ettore Fiorini, L. Gladstone, N. Chott, K. Wilson, H. Z. Huang, Lorenzo Cassina, T. Wise, C. Pagliarone, M. Faverzani, G. Keppel, K. E. Lim, N. D. Scielzo, Stuart Freedman, R. J. Creswick, A. Drobizhev, Jonathan Ouellet, G. Bari, K. Alfonso, M. L. Di Vacri, Davide Chiesa, L. Canonica, Y. Mei, M. A. Franceschi, B. Schmidt, L. Marini, L. Taffarello, Monica Sisti, H. W. Wang, L. Gironi, F. T. Avignone, T. O'Donnell, B. S. Wang, A. Bersani, A. Giuliani, Virendra Singh, O. Azzolini, S. Morganti, M. Sakai, S. Copello, M. Pavan, Y. G. Ma, M. M. Deninno, S. S. Nagorny, Paolo Carniti, Xi-Guang Cao, K. M. Heeger, S. Zimmermann, C. Pira, I. Dafinei, John Wilson, Claudio Gotti, F. Bellini, V. Palmieri, N. Moggi, C. Rosenfeld, V. Novati, Silvia Capelli, Samuele Sangiorgio, S. L. Wagaarachchi, Massimiliano Nastasi, S. Zucchelli, A. Nucciotti, Lindley Winslow, Eric B. Norman, C. Alduino, Oliviero Cremonesi, A. Giachero, A. D'Addabbo, Guoqiang Zhang, T. Napolitano, P. Gorla, F. Ferroni, C. Tomei, Stefano Dell'Oro, S. Pirro, C. Bucci, T. D. Gutierrez, Miriam Lucio Martinez, D. Q. Fang, Yu. G. Kolomensky, Luigi Cappelli, Jeremy S. Cushman, Emanuele Ferri, M. Biassoni, N. Casali, D. D'Aguanno, C. J. Davis, F. Reindl, Ke Han, A. Branca, Reina H. Maruyama, L. Pattavina, Giovanni Benato, Irene Nutini, A. Camacho, J. Schmidt, C. Nones, R. Hennings-Yeomans, S. Di Domizio, F. Terranova, A. Caminata, Ezio Previtali, B. Welliver, Laura Cardani, Marco Pallavicini, B. K. Fujikawa, Massimiliano Clemenza, Stefano Pozzi, Carlo Cosmelli, G. Pessina, M. Vignati, C. Brofferio, C. Rusconi, A. Leder, Centre de Sciences Nucléaires et de Sciences de la Matière (CSNSM), 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), Département de Physique des Particules (ex SPP) (DPP), Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Département de Physique des Particules (ex SPP) (DPhP), Cushman, J, Alduino, C, Alfonso, K, Avignone, F, Azzolini, O, Bari, G, Bellini, F, Benato, G, Bersani, A, Biassoni, M, Branca, A, Brofferio, C, Bucci, C, Camacho, A, Caminata, A, Canonica, L, Cao, X, Capelli, S, Cappelli, L, Cardani, L, Carniti, P, Casali, N, Cassina, L, Chiesa, D, Chott, N, Clemenza, M, Copello, S, Cosmelli, C, Cremonesi, O, Creswick, R, D'Addabbo, A, D'Aguanno, D, Dafinei, I, Davis, C, Dell'Oro, S, Deninno, M, Domizio, S, Vacri, M, Drobizhev, A, Fang, D, Faverzani, M, Ferri, E, Ferroni, F, Fiorini, E, Franceschi, M, Freedman, S, Fujikawa, B, Giachero, A, Gironi, L, Giuliani, A, Gladstone, L, Gorla, P, Gotti, C, Gutierrez, T, Han, K, Heeger, K, Hennings-Yeomans, R, Huang, H, Keppel, G, Kolomensky, Y, Leder, A, Ligi, C, Lim, K, Ma, Y, Marini, L, Martinez, M, Maruyama, R, Mei, Y, Moggi, N, Morganti, S, Nagorny, S, Napolitano, T, Nastasi, M, Nones, C, Norman, E, Novati, V, Nucciotti, A, Nutini, I, O'Donnell, T, Ouellet, J, Pagliarone, C, Pallavicini, M, Palmieri, V, Pattavina, L, Pavan, M, Pessina, G, Pira, C, Pirro, S, Pozzi, S, Previtali, E, Reindl, F, Rosenfeld, C, Rusconi, C, Sakai, M, Sangiorgio, S, Santone, D, Schmidt, B, Schmidt, J, Scielzo, N, Singh, V, Sisti, M, Taffarello, L, Terranova, F, Tomei, C, Vignati, M, Wagaarachchi, S, Wang, B, Wang, H, Welliver, B, Wilson, J, Wilson, K, Winslow, L, Wise, T, Zanotti, L, Zhang, G, Zimmermann, S, and Zucchelli, S
Subjects: Cryostat, History, Cryogenics, 01 natural sciences, tellurium: oxygen, Neutrinoless Double Beta Decay, Cryogenic detector, bolometer, Education, law.invention, Nuclear physics, CUORE, double-beta decay: (0neutrino), Observatory, law, Double beta decay, 0103 physical sciences, Calibration, [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex], [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], 010306 general physics, activity report, Physics, 010308 nuclear & particles physics, Detector, Bolometer, calibration, Computer Science Applications, cryogenics, tellurium: nuclide, performance
Abstract: CUORE, the Cryogenic Underground Observatory for Rare Events, is an experiment searching for the neutrinoless double-beta decay of 130Te. The first CUORE dataset was acquired in May and June 2017 and consisted of 10.6 kg-yr of TeO2 exposure, with several days of calibration data before and after the physics dataset. We discuss here the initial performance of the CUORE detector and cryostat in this first dataset.
Published: 2017
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88. First results from the CUORE experiment

Author: M. Faverzani, N. Casali, A. Bersani, C. Nones, Davide Chiesa, Ettore Fiorini, S. L. Wagaarachchi, C. Rosenfeld, K. Wilson, S. S. Nagorny, F. Reindl, C. Bucci, T. D. Gutierrez, Miriam Lucio Martinez, P. Gorla, F. Ferroni, A. Giuliani, C. Tomei, Jonathan Ouellet, Andrea Giachero, Guoqiang Zhang, G. Bari, Emanuele Ferri, Yu. G. Kolomensky, N. Chott, T. Wise, Marco Pallavicini, S. Di Domizio, J. Schmidt, C. J. Davis, A. Camacho, Jeremy S. Cushman, L. Gladstone, H. Z. Huang, Lindley Winslow, S. Morganti, C. Pagliarone, L. Gironi, Laura Cardani, Carlo Cosmelli, L. Taffarello, B. K. Fujikawa, G. Pessina, G. Keppel, K. E. Lim, F. T. Avignone, Monica Sisti, Stefano Pozzi, Carlo Ligi, Giovanni Benato, Ke Han, A. Branca, Reina H. Maruyama, Virendra Singh, K. Alfonso, Stuart J. Freedman, N. Moggi, Lorenzo Cassina, M. L. Di Vacri, V. Palmieri, S. Zucchelli, C. Pira, Samuele Sangiorgio, A. Drobizhev, S. Zimmermann, Eric B. Norman, N. D. Scielzo, M. Vignati, A. Nucciotti, L. Pattavina, B. Schmidt, T. Napolitano, F. Terranova, Stefano Dell'Oro, C. Alduino, R. J. Creswick, B. S. Wang, M. Clemenza, Claudio Gotti, V. Novati, Silvia Capelli, Massimiliano Nastasi, O. Azzolini, C. Brofferio, V. Dompè, M. Biassoni, A. D'Addabbo, Y. Mei, C. Rusconi, I. Dafinei, John Wilson, H. W. Wang, M. Sakai, T. O'Donnell, Xi-Guang Cao, M. A. Franceschi, K. M. Heeger, Oliviero Cremonesi, S. Copello, A. Caminata, Ezio Previtali, Paolo Carniti, B. Welliver, M. M. Deninno, M. Pavan, Y. G. Ma, Irene Nutini, F. Bellini, R. Hennings-Yeomans, L. Cappelli, Stefano Pirro, D. D'Aguanno, D. Q. Fang, L. Canonica, L. Marini, A. Leder, D. Santone, L. Zanotti, Centre de Sciences Nucléaires et de Sciences de la Matière (CSNSM), 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), Département de Physique des Particules (ex SPP) (DPP), Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Alduino, C, Alfonso, K, Avignone, F, Azzolini, O, Bari, G, Bellini, F, Benato, G, Bersani, A, Biassoni, M, Branca, A, Brofferio, C, Bucci, C, Camacho, A, Caminata, A, Canonica, L, Cao, X, Capelli, S, Cappelli, L, Cardani, L, Carniti, P, Casali, N, Cassina, L, Chiesa, D, Chott, N, Clemenza, M, Copello, S, Cosmelli, C, Cremonesi, O, Creswick, R, Cushman, J, D'Addabbo, A, D'Aguanno, D, Dafinei, I, Davis, C, Dell'Oro, S, Deninno, M, Domizio, S, Vacri, M, Dompe, V, Drobizhev, A, Fang, D, Faverzani, M, Ferri, E, Ferroni, F, Fiorini, E, Franceschi, M, Freedman, S, Fujikawa, B, Giachero, A, Gironi, L, Giuliani, A, Gladstone, L, Gorla, P, Gotti, C, Gutierrez, T, Han, K, Heeger, K, Hennings-Yeomans, R, Huang, H, Keppel, G, Kolomensky, Y, Leder, A, Ligi, C, Lim, K, Ma, Y, Marini, L, Martinez, M, Maruyama, R, Mei, Y, Moggi, N, Morganti, S, Nagorny, S, Napolitano, T, Nastasi, M, Nones, C, Norman, E, Novati, V, Nucciotti, A, Nutini, I, O'Donnell, T, Ouellet, J, Pagliarone, C, Pallavicini, M, Palmieri, V, Pattavina, L, Pavan, M, Pessina, G, Pira, C, Pirro, S, Pozzi, S, Previtali, E, Reindl, F, Rosenfeld, C, Rusconi, C, Sakai, M, Sangiorgio, S, Santone, D, Schmidt, B, Schmidt, J, Scielzo, N, Singh, V, Sisti, M, Taffarello, L, Terranova, F, Tomei, C, Vignati, M, Wagaarachchi, S, Wang, B, Wang, H, Welliver, B, Wilson, J, Wilson, K, Winslow, L, Wise, T, Zanotti, L, Zhang, G, Zimmermann, S, Zucchelli, S, and Département de Physique des Particules (ex SPP) (DPhP)
Subjects: History, Cryogenic system, hierarchy, [PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex], 01 natural sciences, 030218 nuclear medicine & medical imaging, Education, Neutrinoless Double Beta Decay, Cryogenic detector, bolometer, Combinatorics, decoupling, 03 medical and health sciences, 0302 clinical medicine, CUORE, double-beta decay: (0neutrino), bolometer, Double beta decay, tellurium, 0103 physical sciences, [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex], Physics, lifetime, 010308 nuclear & particles physics, temperature, sensitivity, Double beta decay - Cryogenic equipment - Majorana neutrino, Computer Science Applications, talk: Sudbury 2017/07/24, observatory, cryogenics, mass: Majorana, experimental results
Abstract: Author(s): Alduino, C; Alfonso, K; Avignone, FT; Azzolini, O; Bari, G; Bellini, F; Benato, G; Bersani, A; Biassoni, M; Branca, A; Brofferio, C; Bucci, C; Camacho, A; Caminata, A; Canonica, L; Cao, XG; Capelli, S; Cappelli, L; Cardani, L; Carniti, P; Casali, N; Cassina, L; Chiesa, D; Chott, N; Clemenza, M; Copello, S; Cosmelli, C; Cremonesi, O; Creswick, RJ; Cushman, JS; D'Addabbo, A; D'Aguanno, D; Dafinei, I; Davis, CJ; Dell'Oro, S; Deninno, MM; Domizio, SD; Vacri, MLD; Dompe, V; Drobizhev, A; Fang, DQ; Faverzani, M; Ferri, E; Ferroni, F; Fiorini, E; Franceschi, MA; Freedman, SJ; Fujikawa, BK; Giachero, A; Gironi, L; Giuliani, A; Gladstone, L; Gorla, P; Gotti, C; Gutierrez, TD; Han, K; Heeger, KM; Hennings-Yeomans, R; Huang, HZ; Keppel, G; Kolomensky, YG; Leder, A; Ligi, C; Lim, KE; Ma, YG; Marini, L; Martinez, M; Maruyama, RH; Mei, Y; Moggi, N; Morganti, S; Nagorny, SS; Napolitano, T; Nastasi, M; Nones, C; Norman, EB; Novati, V; Nucciotti, A; Nutini, I; O'Donnell, T; Ouellet, JL; Pagliarone, CE; Pallavicini, M; Palmieri, V; Pattavina, L | Abstract: CUORE (Cryogenic Underground Observatory for Rare Events) is a ton-scale experiment aiming to the search of neutrino-less double beta decay in 130Te with a projected sensitivity on the Majorana effective mass close to the inverted hierarchy region. The CUORE detector consists of a segmented array of 988 TeO2 bolometers, organized in 19 towers and operated at a temperature of about 10 mK thanks to a custom cryogenic system which, besides the uncommon scale, observes several constraints from the radio-purity of the materials to the mechanical decoupling of the cooling systems. The successful commissioning of the CUORE cryogenic system has been completed early in 2016 and represents an outstanding achievement by itself. The installation of the detector proceeded along 2016 followed by the cooldown to base temperature at the beginning of 2017. The CUORE detector is now operational and has been taking science data since Spring 2017. With the first ∼3 weeks of collected data, we present here the most stringent constraint on the 130Te half-live for the neutrino-less double beta decay.
Published: 2017
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89. SU-E-T-497: Study of Restricted Mass Stopping Power Ratio in Small Electron Tube Fields

Author: T Yamagishi, R Baba, K Ebe, H Takatou, K Tokuyama, Keisuke Sasai, Shuichi Ozawa, Satoru Sugimoto, and H Maruyama
Subjects: Field (physics), law, Ionization chamber, Vacuum tube, Monte Carlo method, General Medicine, Electron, Stopping power, Atomic physics, Beam (structure), Percentage depth dose curve, law.invention, Mathematics
Abstract: Purpose:Electron tubes with small radii are useful to treat narrow regions which cannot accommodate normal electron applicators. In small electron fields, it is not trivial to estimate restricted mass stopping power ratio (MSR), which is needed to evaluate dose from ion chamber measurement. We studied MSRs in small electron tube fields using the Monte Carlo simulation.Methods:Electron tubes with radii, 3 and 2.5 cm, were used in this study. Nominal electron energies were 6 and 9 MeV. There were two types of tubes. One has a normal cut but the other has a 45‐degree cut. For the normal cut tube, percent depth dose (PDD) in water was evaluated along the center of axis (CAX) of a beam. For the 45‐degree cut tube, PDD was evaluated along the vertical line from the intersection of the CAX and the phantom surface with 45‐degree gantry angle. The MSRs and mean electron energies were calculated using the Monte Carlo simulation.Results: We found good agreement between the measured and calculated PDDs. The changes of mean energies from those in the 10×10 cm2 field at the depth of maximum dose (dmax) were very small for the normal cut electron tubes. For the 45‐degree cut tubes, the changes of mean energies at dmax were less than 1 MeV. The MSRs in the normal cut tube fields were almost the same as those in the 10×10 cm2 field at the corresponding depths. The MSRs for the 45‐degree cut tubes deviated from those in the 10×10 cm2 by about 1% (1.5 % at most). Conclusions: We evaluated the mean energies and MSRs in small electron tube fields. The deviations of them from the values in the 10×10 cm2 were small. The maximum difference of MSR was 1.5% in 45‐degree cut tube fields. This work was supported by KAKENHI (23791449), Japan Society for the Promotion of Science, and Cancer Professional Training Plan, The Ministry of Education, Culture, Sports, Science and Technology, Japan.
Published: 2017

90. PINGU: a vision for neutrino and particle physics at the South Pole

Author: A. Olivas, F. Huang, G. Neer, S. Euler, J. van Santen, M. Day, Kael Hanson, Janet Conrad, Hrvoje Dujmovic, Ignacio Taboada, Steven W. Barwick, Christian Bohm, D. Hebecker, Aongus O'Murchadha, Segev BenZvi, R. Cross, M. Wolf, M. Jurkovic, M. Rongen, M. Kauer, B. Relethford, Christian Spiering, Spencer Klein, Konstancja Satalecka, M. Song, T. L. Carver, Mike Richman, Maximilian Meier, Thomas Meures, Christoph Raab, Paolo Desiati, George Japaridze, M. Schimp, G. Krückl, P. Schlunder, Hermann Kolanoski, B. Hansmann, Roger Moore, G. C. Hill, E. Friedman, D. Tosi, H. Taavola, J. Lünemann, L. Brayeur, Sally Robertson, M. Kroll, S. Hickford, A. Meli, Kara Hoffman, K. D. de Vries, T. Ehrhardt, N. van Eijndhoven, Justin Vandenbroucke, M. Leuermann, E. Blaufuss, D. J. Boersma, K. Mase, Elisa Resconi, K. Hoshina, C. Krüger, Kurt Woschnagg, Paul Evenson, D. Seckel, S. Fahey, Sebastian Böser, M. Kowalski, G. H. Collin, C. Haack, M. J. Weiss, A. R. Fazely, Tyce DeYoung, P. A. Toale, S. Márka, M. Labare, U. Naumann, D. Berley, W. Giang, M. Quinnan, C. Kopper, J. Braun, T. Kittler, S. Flis, Glenn Spiczak, G. Golup, Gisela Anton, M. Dunkman, J. L. Lanfranchi, R. Reimann, Imre Bartos, Stijn Blot, K. Krings, M. Glagla, Karim Ghorbani, S. Seunarine, E. Pinat, Dmitry Chirkin, L. Mohrmann, R. Hoffmann, S. Kopper, Antonio Palazzo, Simona Toscano, M. Voge, Spencer Axani, M. Mandelartz, S. Coenders, T. R. Wood, S. C. Nowicki, T. C. Arlen, G. Merino, Wolfgang Rhode, N. Wandkowsky, Alexander Kappes, A. Christov, Minjin Jeong, J. L. Kelley, S. In, L. Gladstone, G. Karagiorgi, S. Mandalia, R. Koirala, Donglian Xu, R. Nahnhauer, Carlos Arguelles, S. Schoenen, J. J. Beatty, K. Abraham, L. Wills, Olga Botner, S. Miarecki, Christopher Wiebusch, J. Feintzeig, D. Heereman, A. Bernhard, M. Lesiak-Bzdak, Darren Grant, Juanan Aguilar, K. Wiebe, Azadeh Keivani, A. Haj Ismail, J. Kiryluk, F. Bos, Teppei Katori, K. H. Becker, E. Unger, D. Z. Besson, F. McNally, V. Baum, Francis Halzen, D. R. Nygren, Aya Ishihara, D. Rysewyk, Subir Sarkar, Allan Hallgren, D. V. Pankova, L. Classen, J. Haugen, K. Rawlins, I. Ansseau, M. J. Larson, A. Franckowiak, Marjon Moulai, S. Yoshida, M. Casier, B. Riedel, J. P. A. M. de André, M. Bissok, K. Jero, A. Stößl, A. Terliuk, E. Jacobi, M. G. Aartsen, S. Wickmann, J. Auffenberg, T. Stezelberger, T. Hansmann, G. W. Sullivan, M. H. Shaevitz, Reina H. Maruyama, A. Turcati, R. Maunu, J. Kunnen, Damian Pieloth, Ali Kheirandish, B. Eichmann, H. Dembinski, C. Walck, James Madsen, M. S. Kim, James Pinfold, Michael Sutherland, H.-P. Bretz, A. Stasik, N. L. Strotjohann, Lu Lu, Sarah Mancina, S. De Ridder, B. J. P. Jones, M. Stahlberg, L. Schumacher, A. Steuer, D. Bindig, M. van Rossem, Gerald Przybylski, T. Fuchs, Y. Xu, M. N. Tobin, E. Hansen, M. E. Huber, E. Pino del Rosendo, M. Börner, Klas Hultqvist, Z. Griffith, R. C. Bay, J. C. Díaz-Vélez, D. Bose, J. P. Dumm, M. Relich, K. Meagher, T. Karg, Ch. Weaver, L. Gerhardt, Maryon Ahrens, O. Kalekin, K. Andeen, Teresa Montaruli, P. Sandstrom, Frederik Tenholt, M. Rameez, M. Archinger, M. Medici, Kendall Mahn, Frederik Hermann Lauber, H. Niederhausen, L. Köpke, T. Palczewski, Julian Kemp, M. Zoll, G. Kohnen, Carsten Rott, G. Maggi, J. Tatar, S. Westerhoff, Albrecht Karle, M. Wallraff, Xianwu Xu, J. Sandroos, D. Altmann, P. Berghaus, T. Anderson, B. Eberhardt, C. De Clercq, C. Pérez de los Heros, R. Ström, G. Tešić, T. Kuwabara, Kirill Filimonov, D. J. Koskinen, Ö. Penek, S. Söldner-Rembold, Dirk Lennarz, Thorsten Glusenkamp, D. Soldin, S. Schöneberg, Z. Márka, K. Helbing, U. Katz, L. Rädel, Alexander Burgman, Hiroyuki Tanaka, Jenni Adams, Akimichi Taketa, J. Leuner, R. G. Stokstad, Killian Holzapfel, Chris Wendt, C.-C. Fösig, R. Konietz, M. Vehring, J. M. LoSecco, Joshua Hignight, H. Pandya, T. Kintscher, Javier Gonzalez, C. B. Krauss, E. Woolsey, G. Binder, Joshua Pepper, P. B. Price, D. Ryckbosch, Markus Ackermann, N. Kurahashi, B. J. Whelan, Todor Stanev, R. Hellauer, Dawn Williams, G. de Wasseige, Elisa Bernardini, M. Tselengidou, Thomas K. Gaisser, G. B. Yodh, J. Becker Tjus, J. Veenkamp, A. Goldschmidt, Troels Petersen, S. Kunwar, S. Wren, L. Sabbatini, T. Ruhe, S. Tilav, J. P. Yanez, T. Schmidt, L. Wille, S. E. Sanchez Herrera, E. Cheung, M. Usner, V. di Lorenzo, T. Menne, C. Finley, A. Wallace, K. Clark, D. F. Cowen, Stijn Vanheule, Philipp Eller, A. Sandrock, J. Felde, Xinhua Bai, A. Obertacke Pollmann, Markus Ahlers, M. Vraeghe, J. J. Evans, Samvel Ter-Antonyan, Jay Gallagher, Faculty of Sciences and Bioengineering Sciences, Physics, Vriendenkring VUB, and Elementary Particle Physics
Subjects: Physics - Instrumentation and Detectors, Physics::Instrumentation and Detectors, mixing [neutrino], atmospheric neutrinos, IceCube Neutrino Observatory, neutrino oscillations, PINGU, Nuclear and High Energy Physics, pole, 7. Clean energy, 01 natural sciences, IceCube, High Energy Physics - Experiment, Observatory, Physics, solar [WIMP], precision measurement, Astrophysics::Instrumentation and Methods for Astrophysics, oscillation [neutrino], solar [dark matter], atmosphere [neutrino], threshold [energy], mass difference [neutrino], observatory, High Energy Physics - Phenomenology, Upgrade, Neutrino detector, upgrade, Neutrino, KM3NET, performance, Particle physics, supernova [neutrino], particle identification [neutrino/tau], Astrophysics::High Energy Astrophysical Phenomena, SUPERNOVA DETECTION, 0103 physical sciences, OSCILLATIONS, mass: low [dark matter], unitarity, ddc:530, 010306 general physics, Neutrino oscillation, 010308 nuclear & particles physics, Astronomy, sensitivity, KM3NeT, Physics and Astronomy, mass [neutrino], beam [neutrino], High Energy Physics::Experiment, galaxy, ATMOSPHERIC NEUTRINOS, MATTER, SYSTEM, Lepton, mixing angle [neutrino], experimental results
Abstract: The Precision IceCube Next Generation Upgrade (PINGU) is a proposed low-energy in-fill extension to the IceCube Neutrino Observatory. With detection technology modeled closely on the successful IceCube example, PINGU will provide a 6Mton effective mass for neutrino detection with an energy threshold of a few GeV. With an unprecedented sample of over 60,000 atmospheric neutrinos per year in this energy range, PINGU will make highly competitive measurements of neutrino oscillation parameters in an energy range over an order of magnitude higher than long-baseline neutrino beam experiments. PINGU will measure the mixing parameters $\theta_{\rm 23}$ and $\Delta m^2_{\rm 32}$, including the octant of $\theta_{\rm 23}$ for a wide range of values, and determine the neutrino mass ordering at $3\sigma$ median significance within 4 years of operation. PINGU's high precision measurement of the rate of ${\nu_\tau}$ appearance will provide essential tests of the unitarity of the $3\times 3$ PMNS neutrino mixing matrix. PINGU will also improve the sensitivity of searches for low mass dark matter in the Sun, use neutrino tomography to directly probe the composition of the Earth's core, and improve IceCube's sensitivity to neutrinos from Galactic supernovae. Reoptimization of the PINGU design has permitted substantial reduction in both cost and logistical requirements while delivering performance nearly identical to configurations previously studied. This document summarizes the results of detailed studies described in a more comprehensive document to be released soon., Comment: 28 pages, 10 figures, submitted to J. Phys. G
Published: 2017
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91. Performance of the low threshold Optimum Trigger on CUORE data

Author: A. Branca, D. Q. Adams, C. Alduino, K. Alfonso, F. T. Avignone III, O. Azzolini, G. Bari, F. Bellini, G. Benato, M. Biassoni, C. Brofferio, C. Bucci, J. Camilleri, A. Caminata, A. Campani, L. Canonica, X. G. Cao, S. Capelli, L. Cappelli, L. Cardani, P. Carniti, N. Casali, D. Chiesa, M. Clemenza, S. Copello, C. Cosmelli, O. Cremonesi, R. J. Creswick, A. D'Addabbo, D. D'Aguanno, I. Dafinei, C. J. Davis, F. Del Corso, S. Dell'Oro, S. Di Domizio, V. Dompè, D. Q. Fang, G. Fantini, M. Faverzani, E. Ferri, F. Ferroni, E. Fiorini, M. A. Franceschi, S. J. Freedman, B. K. Fujikawa, A. Giachero, L. Gironi, A. Giuliani, P. Gorla, C. Gotti, T. D. Gutierrez, K. Han, K. M. Heeger, R. G. Huang, H. Z. Huang, J. Johnston, G. Keppel, Yu. G. Kolomensky, C. Ligi, L. Ma, Y. G. Ma, L. Marini, R. H. Maruyama, Y. Mei, N. Moggi, S. Morganti, T. Napolitano, M. Nastasi, J. Nikkel, C. Nones, E. B. Norman, V. Novati, A. Nucciotti, I. Nutini, T. O'Donnell, J. L. Ouellet, C. E. Pagliarone, L. Pagnanini, M. Pallavicini, L. Pattavina, M. Pavan, G. Pessina, V. Pettinacci, C. Pira, S. Pirro, S. Pozzi, E. Previtali, A. Puiu, C. Rosenfeld, C. Rusconi, M. Sakai, S. Sangiorgio, B. Schmidt, N. D. Scielzo, V. Sharma, V. Singh, M. Sisti, D. Speller, L. Taffarello, F. Terranova, C. Tomei, M. Vignati, S. L. Wagaarachchi, B. S. Wang, B. Welliver, J. Wilson, K. Wilson, L. A. Winslow, L. Zanotti, S. Zimmermann, S. Zucchelli, Branca, A, Adams, D, Alduino, C, Alfonso, K, Avignone III, F, Azzolini, O, Bari, G, Bellini, F, Benato, G, Biassoni, M, Brofferio, C, Bucci, C, Camilleri, J, Caminata, A, Campani, A, Canonica, L, Cao, X, Capelli, S, Cappelli, L, Cardani, L, Carniti, P, Casali, N, Chiesa, D, Clemenza, M, Copello, S, Cosmelli, C, Cremonesi, O, Creswick, R, D'Addabbo, A, D'Aguanno, D, Dafinei, I, Davis, C, Del Corso, F, Dell'Oro, S, Di Domizio, S, Dompè, V, Fang, D, Fantini, G, Faverzani, M, Ferri, E, Ferroni, F, Fiorini, E, Franceschi, M, Freedman, S, Fujikawa, B, Giachero, A, Gironi, L, Giuliani, A, Gorla, P, Gotti, C, Gutierrez, T, Han, K, Heeger, K, Huang, R, Huang, H, Johnston, J, Keppel, G, Kolomensky, Y, Ligi, C, Ma, L, Ma, Y, Marini, L, Maruyama, R, Mei, Y, Moggi, N, Morganti, S, Napolitano, T, Nastasi, M, Nikkel, J, Nones, C, Norman, E, Novati, V, Nucciotti, A, Nutini, I, O'Donnell, T, Ouellet, J, Pagliarone, C, Pagnanini, L, Pallavicini, M, Pattavina, L, Pavan, M, Pessina, G, Pettinacci, V, Pira, C, Pirro, S, Pozzi, S, Previtali, E, Puiu, A, Rosenfeld, C, Rusconi, C, Sakai, M, Sangiorgio, S, Schmidt, B, Scielzo, N, Sharma, V, Singh, V, Sisti, M, Speller, D, Taffarello, L, Terranova, F, Tomei, C, Vignati, M, Wagaarachchi, S, Wang, B, Welliver, B, Wilson, J, Wilson, K, Winslow, L, Zanotti, L, Zimmermann, S, and Zucchelli, S
Subjects: Physics, History, Particle physics, CUORE, Optimal Trigger, CUORE, low energy, dark matter, WIMP, neutrino, Computer Science Applications, Education
Abstract: The Optimum Trigger (OT) is based on a threshold algorithm applied on waveforms filtered by exploiting the matched filter technique. The OT trigger thresholds improve by 60 – 90% with respect to the thresholds obtained with the standard trigger, ranging between ~ 20 and 100 keV. Low trigger thresholds open the way to Dark Matter searches and to improvements in the neutrinoless double beta decay analysis. Nevertheless, running the OT on CUORE data is demanding from the computational resources point of view. For this reason, the algorithm has been revised and adapted to cope with CUORE data. The work done to implement OT in CUORE and its performances will be discussed.
Published: 2020
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92. Padronização da técnica de nanopartícula de ouro não modificada (AuNPs) para detecção de Actinobacillus pleuropneumoniae em pulmões de suínos

Author: Givago Faria Ribeiro da Silva, Catia Silene Klein, Luciano Nakazato, Fernanda H. Maruyama, Laila Natasha Santos Brandão, Letícia Camara Pitchenin, Valéria Dutra, and Cristiane Silva Chitarra
Subjects: Veterinary medicine, lcsh:Veterinary medicine, General Veterinary, biology, Chemistry, Actinobacillus pleuropneumoniae, Diagnostic test, biology.organism_classification, Molecular biology, nanopartícula de ouro, AuNP, lcsh:SF600-1100, Pneumonia suína
Abstract: Testes diagnósticos baseados na detecção de ácidos nucleicos sem amplificação prévia através da utilização de nanopartículas de ouro (AuNPs) têm sido descritos para várias enfermidades. Este trabalho teve como objetivo desenvolver uma técnica de AuNPs não modificada para detecção de Actinobacillus pleuropneumoniae (App). Utilizaram-se 70 amostras de pulmão de suínos, 17 sem lesão e 53 com lesões características de pneumonia, objetivando a detecção de App. O oligonucleotídeo utilizado foi baseado no gene ApxIV. O teste de AuNPs apresentou sensibilidade de 93,8% e especificidade de 84,6% quando comparado com a detecção pela PCR. Os resultados mostraram boa concordância entre os testes de AuNPs e a PCR, sendo que a técnica pode ser utilizada como alternativa aos testes convencionais, já que é de fácil e rápida execução e não exige infraestrutura e mão de obra especializada.
Published: 2014

93. Memory Embedded VLSI Gate Array Testing.

Author: M. Shimizu, N. Okino, J. Nishiura, and H. Maruyama
Published: 1985

94. PROEDIT - A Screen Oriented Prolog Programming Environment.

Author: Masayuki Numao and H. Maruyama
Published: 1985
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95. Search for sterile neutrino mixing using three years of IceCube DeepCore data

Author: Janet Conrad, M. Rongen, M. S. Sutherland, M. Kauer, G. Merino, D. Bose, Francis Halzen, J. P. Dumm, I. Ansseau, A. Terliuk, E. Vogel, Christian Bohm, B. Eberhardt, Aongus O'Murchadha, Christoph Raab, Jenni Adams, R. Nahnhauer, D. Berley, G. C. Hill, Juanan Aguilar, Hrvoje Dujmovic, L. Gladstone, C. Krüger, D. Seckel, S. Fahey, S. Miarecki, E. Jacobi, Tyce DeYoung, R. Maunu, A. Ishihara, P. A. Toale, Sander Vanheule, T. Kuwabara, T. Karg, Ch. Weaver, S. Hickford, R. G. Stokstad, A. Kyriacou, Joonghan Kim, J. Feintzeig, K. Mase, Minjin Jeong, G. Tešić, Tim Ruhe, E. Friedman, C.-C. Fösig, Darren Grant, N. L. Strotjohann, I. Al Samarai, A. Karle, J. Becker Tjus, Karim Ghorbani, Sarah Nowicki, C. H. Wiebusch, J. P. A. M. de André, K. Filimonov, Spencer Axani, M. Leuermann, G. Kohnen, J. P. Yanez, G. Maggi, Alexander Burgman, M. Kroll, C. Walck, D. Z. Besson, H.-P. Bretz, T. Menne, M. J. Larson, G. Krückl, Frank McNally, Chunfai Tung, Carlos Arguelles, E. V. Hansen, D. Tosi, J. Stachurska, C. Pérez de los Heros, Jessie Micallef, Z. Griffith, M. Kowalski, A. Stasik, R. Konietz, G.M. Spiczak, Joakim Sandroos, Azadeh Keivani, Konstancja Satalecka, J. J. Beatty, Joanna Kiryluk, K. Meagher, M. Day, Dirk Lennarz, M. Zoll, A. Franckowiak, Marjon Moulai, H. Dembinski, K. Rawlins, Theo Glauch, S. Westerhoff, Gerald Przybylski, D. Rysewyk, M. Quinnan, D. Soldin, M. Dunkman, K. Clark, S. Yoshida, T. Hansmann, A. Stößl, B. J. Whelan, Christian Spiering, Thorsten Glusenkamp, Reina H. Maruyama, David R. Williams, Todor Stanev, Claudio Kopper, C. Wendt, K. D. Hoffman, Justin Vandenbroucke, G. W. Sullivan, S. Schöneberg, James E. Braun, James Madsen, Lu Lu, L. Schumacher, M. Casier, E. del Pino Rosendo, W. Giang, G. de Wasseige, J. L. Lanfranchi, J. Lünemann, Subir Sarkar, R. Hoffmann, Martin Wolf, R. C. Bay, Olga Botner, J. Tatar, N. van Eijndhoven, Gisela Anton, Juan Carlos Diaz-Velez, M. Archinger, K. Helbing, Thomas Meures, V. Baum, D.F. Cowen, M. Tselengidou, R. Cross, Andrea Turcati, Teresa Montaruli, J. Stettner, Thomas K. Gaisser, G. B. Yodh, L. Sabbatini, P. Peiffer, J. van Santen, Stijn Blot, K. D. de Vries, K. Hoshina, M. Mandelartz, Kendall Mahn, U. Katz, T. Kintscher, Gary Binder, A. Sandrock, George Japaridze, S. Tilav, B. J. P. Jones, A. R. Fazely, J. L. Kelley, E. Woolsey, M. E. Huber, Joshua Pepper, J. S. Gallagher, M. Richman, K. Wiebe, M. Tobin, J. Hignight, U. Naumann, M. Lesiak-Bzdak, Seongjin In, F. Lauber, A. Olivas, E. Pinat, Hermann Kolanoski, E. Unger, Elisa Resconi, Elisa Bernardini, Simona Toscano, C. De Clercq, F. Tenholt, Richard G. Strom, Philipp Eller, Kael Hanson, Carsten Rott, Markus Ackermann, S. Bron, T. Fuchs, S. W. Barwick, Maximilian Meier, Segev BenZvi, Paolo Desiati, A. Goldschmidt, S. Kunwar, F. Huang, Xianwu Xu, D. Altmann, Timothy W. Schmidt, K.-H. Becker, Yiqian Xu, J. Felde, S. Seunarine, E. Cheung, A. Steuer, M. Usner, A. Kheirandish, Dirk Ryckbosch, A. Obertacke Pollmann, F. Bos, J. G. Gonzalez, P. Schlunder, Hershal Pandya, Markus Ahlers, Wolfgang Rhode, V. di Lorenzo, Allan Hallgren, T. Palczewski, S. Schoenen, Sandro Kopper, C. Finley, D. Heereman, Samvel Ter-Antonyan, L. Brayeur, Naoko Kurahashi, I. Taboada, Dustin Hebecker, T. Anderson, K. Jero, S. R. Klein, M. G. Aartsen, Thomas Ehrhardt, Ramesh Koirala, H. Taavola, E. Blaufuss, K. Woschnagg, L. Classen, N. Wandkowsky, M. Relich, M. Wallraff, M. S. Kim, L. Wills, M. Voge, K. Krings, Woosik Kang, S. De Ridder, Benedikt Riedel, M. van Rossem, L. Gerhardt, Maryon Ahrens, M. Rameez, S. Euler, M. Medici, S. Coenders, M. Labare, J. Kunnen, D. V. Pankova, D. R. Nygren, Damian Pieloth, L. Wille, S. E. Sanchez Herrera, S. Wickmann, J. Auffenberg, Hans Niederhausen, A. Wallace, X. Bai, G. Neer, L. Köpke, Da Xu, R. Hellauer, G. Momenté, M. Vehring, M. Song, T. L. Carver, Sally Robertson, Sebastian Böser, P. B. Price, A. Waza, C. Haack, M. J. Weiss, T. Kittler, S. Flis, T. R. Wood, R. Reimann, Matthias Vraeghe, Sarah Mancina, Paul Evenson, M. Börner, Klas Hultqvist, K. Andeen, D. J. Koskinen, Björn Eichmann, Ö. Penek, L. Rädel, Gabriel Collin, Dmitry Chirkin, Alexander Kappes, A. Christov, B. Relethford, Daniel Bindig, T. Stezelberger, Physics, Elementary Particle Physics, Faculty of Sciences and Bioengineering Sciences, and Vriendenkring VUB
Subjects: FLUX, Sterile neutrino, Particle physics, Physics and Astronomy (miscellaneous), Physics::Instrumentation and Detectors, Solar neutrino, Astrophysics::High Energy Astrophysical Phenomena, FOS: Physical sciences, 01 natural sciences, High Energy Physics - Experiment, OSCILLATION EXPERIMENTS, High Energy Physics - Experiment (hep-ex), High Energy Physics - Phenomenology (hep-ph), 0103 physical sciences, TRACK RECONSTRUCTION, ddc:530, 010306 general physics, Neutrino oscillation, Physics, 010308 nuclear & particles physics, High Energy Physics::Phenomenology, Astronomy, Solar neutrino problem, LINE-EXPERIMENT-SIMULATOR, MODEL, High Energy Physics - Phenomenology, Neutrino detector, Physics and Astronomy, Measurements of neutrino speed, High Energy Physics::Experiment, Neutrino astronomy, Neutrino
Abstract: Physical review / D 95(11), 112002(2017). doi:10.1103/PhysRevD.95.112002, We present a search for a light sterile neutrino using three years of atmospheric neutrino data from the DeepCore detector in the energy range of approximately 10–60 GeV. DeepCore is the low-energy subarray of the IceCube Neutrino Observatory. The standard three-neutrino paradigm can be probed by adding an additional light (Δm$^{2}_{41}$ ∼ 1 eV2) sterile neutrino. Sterile neutrinos do not interact through the standard weak interaction and, therefore, cannot be directly detected. However, their mixing with the three active neutrino states leaves an imprint on the standard atmospheric neutrino oscillations for energies below 100 GeV. A search for such mixing via muon neutrino disappearance is presented here. The data are found to be consistent with the standard three-neutrino hypothesis. Therefore, we derive limits on the mixing matrix elements at the level of $|U_{μ4}|^{2}, Published by APS, Woodbury, NY
Published: 2017
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96. The detector calibration system for the CUORE cryogenic bolometer array

Author: Daniel Lenz, Kyungeun E. Lim, Samuele Sangiorgio, A. Nucciotti, T. Wise, K. M. Heeger, Larissa M. Ejzak, Reina H. Maruyama, A. Dally, C. J. Davis, Jeremy S. Cushman, Cushman, J, Dally, A, Davis, C, Ejzak, L, Lenz, D, Lim, K, Heeger, K, Maruyama, R, Nucciotti, A, Sangiorgio, S, and Wise, T
Subjects: Cryostat, Nuclear and High Energy Physics, Physics - Instrumentation and Detectors, Physics::Instrumentation and Detectors, Nuclear engineering, Bolometer, Cryogenic, FOS: Physical sciences, Cryogenics, 01 natural sciences, law.invention, Nuclear physics, CUORE, Observatory, law, 0103 physical sciences, Calibration, Dilution refrigerator, Nuclear Experiment (nucl-ex), Nuclear Experiment, 010306 general physics, Instrumentation, Low background, Physics, 010308 nuclear & particles physics, Detector, Astrophysics::Instrumentation and Methods for Astrophysics, Instrumentation and Detectors (physics.ins-det), Neutrino physics, High Energy Physics::Experiment
Abstract: The Cryogenic Underground Observatory for Rare Events (CUORE) is a ton-scale cryogenic experiment designed to search for neutrinoless double-beta decay of $^{130}$Te and other rare events. The CUORE detector consists of 988 TeO$_2$ bolometers operated underground at 10 mK in a dilution refrigerator at the Laboratori Nazionali del Gran Sasso. Candidate events are identified through a precise measurement of their energy. The absolute energy response of the detectors is established by the regular calibration of each individual bolometer using gamma sources. The close-packed configuration of the CUORE bolometer array combined with the extensive shielding surrounding the detectors requires the placement of calibration sources within the array itself. The CUORE Detector Calibration System is designed to insert radioactive sources into and remove them from the cryostat while respecting the stringent heat load, radiopurity, and operational requirements of the experiment. This paper describes the design, commissioning, and performance of this novel source calibration deployment system for ultra-low-temperature environments., 16 pages, 19 figures
Published: 2017

97. Results from CUORE and CUORE-0

Author: C. Rosenfeld, P. Gorla, F. Ferroni, C. Tomei, Emanuele Ferri, H. W. Wang, C. J. Davis, A. Camacho, Carlo Ligi, S. J. Freedman, M. M. Deninno, H. Z. Huang, N. D. Scielzo, E. Fiorini, N. Moggi, Massimiliano Clemenza, Lucia Canonica, Yu. G. Kolomensky, Luigi Cappelli, C. Pagliarone, S. S. Nagorny, Monica Sisti, F. Bellini, Samuele Sangiorgio, R. Hennings-Yeomans, S. Pozzi, Oliviero Cremonesi, S. Zimmermann, A. Nucciotti, B. Schmidt, A. Caminata, C. Alduino, M. Faverzani, T. Wise, R. J. Creswick, K. Alfonso, C. Bucci, Miriam Lucio Martinez, Marco Pallavicini, L. Pattavina, A. Woodcraft, Lindley Winslow, Jonathan Ouellet, B. Welliver, M. L. Di Vacri, G. Pessina, G. Bari, L. Taffarello, C. Brofferio, P. J. Mosteiro, Guimin Zhang, L. Gironi, F. T. Avignone, Lorenzo Cassina, V. Singh, S. L. Wagaarachchi, Giovanni Benato, C. Pira, N. Casali, C. Cosmelli, C. Nones, V. Palmieri, T. D. Gutierrez, E. Previtali, F. Terranova, C. Rusconi, Eric B. Norman, A. D'Addabbo, M. Sakai, T. Napolitano, Simone Capelli, N. Chott, L. Marini, V. Novati, D. D'Aguanno, M. Biassoni, S. Copello, S. Morganti, Paolo Carniti, Ke Han, A. Branca, Reina H. Maruyama, Y. Mei, Stefano Dell'Oro, Stefano Zucchelli, Xi-Guang Cao, K. M. Heeger, J. Schmidt, T. O'Donnell, Yu-Gang Ma, G. Keppel, D. R. Artusa, M. Pavan, Massimiliano Nastasi, A. Giuliani, A. Bersani, I. Dafinei, Davide Chiesa, K. E. Lim, Jeremy S. Cushman, L. Zanotti, A. Leder, A. Drobizhev, D. Santone, J. S. Wilson, B. S. Wang, O. Azzolini, M. A. Franceschi, C. Gotti, A. Giachero, D. Q. Fang, L. Gladstone, S. Pirro, S. Di Domizio, Laura Cardani, B. K. Fujikawa, M. Vignati, Centre de Sciences Nucléaires et de Sciences de la Matière (CSNSM), 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), Département de Physique des Particules (ex SPP) (DPhP), Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Département de Physique des Particules (ex SPP) (DPP), Moggi, N, Alduino, C, Alfonso, K, Artusa, D, Avignone, F, Azzolini, O, Bari, G, Bellini, F, Benato, G, Bersani, A, Biassoni, M, Branca, A, Brofferio, C, Bucci, C, Camacho, A, Caminata, A, Canonica, L, Cao, X, Capelli, S, Cappelli, L, Cardani, L, Carniti, P, Casali, N, Cassina, L, Chiesa, D, Chott, N, Clemenza, M, Copello, S, Cosmelli, C, Cremonesi, O, Creswick, R, Cushman, J, D'Addabbo, A, D'Aguanno, D, Dafinei, I, Davis, C, Dell'Oro, S, Deninno, M, Di Domizio, S, Di Vacri, M, Drobizhev, A, Fang, D, Faverzani, M, Ferri, E, Ferroni, F, Fiorini, E, Franceschi, M, Freedman, S, Fujikawa, B, Giachero, A, Gironi, L, Giuliani, A, Gladstone, L, Gorla, P, Gotti, C, Gutierrez, T, Han, K, Heeger, K, Hennings-Yeomans, R, Huang, H, Keppel, G, Kolomensky, Y, Leder, A, Ligi, C, Lim, K, Ma, Y, Marini, L, Martinez, M, Maruyama, R, Mei, Y, Morganti, S, Mosteiro, P, Nagorny, S, Napolitano, T, Nastasi, M, Nones, C, Norman, E, Novati, V, Nucciotti, A, O'Donnell, T, Ouellet, J, Pagliarone, C, Pallavicini, M, Palmieri, V, Pattavina, L, Pavan, M, Pessina, G, Pira, C, Pirro, S, Pozzi, S, Previtali, E, Rosenfeld, C, Rusconi, C, Sakai, M, Sangiorgio, S, Santone, D, Schmidt, B, Schmidt, J, Scielzo, N, Singh, V, Sisti, M, Taffarello, L, Terranova, F, Tomei, C, Vignati, M, Wagaarachchi, S, Wang, B, Wang, H, Welliver, B, Wilson, J, Winslow, L, Wise, T, Woodcraft, A, Zanotti, L, Zhang, G, Zimmermann, S, Zucchelli, S, Moggi, N., Alduino, C., Alfonso, K., Artusa, D. R., Avignone, F. T., Azzolini, O., Bari, G., Bellini, F., Benato, G., Bersani, A., Biassoni, M., Branca, A., Brofferio, C., Bucci, C., A., Camacho, Caminata, A., Canonica, L., Cao, X. G., Capelli, S., Cappelli, L., Cardani, L., Carniti, P., Casali, N., Cassina, L., Chiesa, D., Chott, N., Clemenza, M., Copello, S., Cosmelli, C., Cremonesi, O., Creswick, R. J., Cushman, J. S., D'Addabbo, A., D'Aguanno, D., Dafinei, I., Davis, C. J., Dell'Oro, S., Deninno, M. M., Di Domizio, S., Di Vacri, M. L., Drobizhev, A., Fang, D. Q., Faverzani, M., Ferri, E., Ferroni, F., Fiorini, E., Franceschi, M. A., Freedman, S. J., Fujikawa, B. K., Giachero, A., Gironi, L., Giuliani, A., Gladstone, L., Gorla, P., Gotti, C., Gutierrez, T. D., Han, K., Heeger, K. M., Hennings-Yeomans, R., Huang, H. Z., Keppel, G., Kolomensky, Yu. G., Leder, A., Ligi, C., Lim, K. E., Ma, Y. G., Marini, L., Martinez, M., Maruyama, R. H., Mei, Y., Morganti, S., Mosteiro, P. J., Nagorny, S. S., Napolitano, T., Nastasi, M., Nones, C., Norman, E. B., Novati, V., Nucciotti, A., O'Donnell, T., Ouellet, J. L., Pagliarone, C. E., Pallavicini, M., Palmieri, V., Pattavina, L., Pavan, M., Pessina, G., Pira, C., Pirro, S., Pozzi, S., Previtali, E., Rosenfeld, C., Rusconi, C., Sakai, M., Sangiorgio, S., Santone, D., Schmidt, B., Schmidt, J., Scielzo, N. D., Singh, V., Sisti, M., Taffarello, L., Terranova, F., Tomei, C., Vignati, M., Wagaarachchi, S. L., Wang, B. S., Wang, H. W., Welliver, B., Wilson, J., Winslow, L. A., Wise, T., Woodcraft, A., Zanotti, L., Zhang, G. Q., S., Zimmermann, Zucchelli, S., and 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)
Subjects: Cryostat, Particle physics, detector: performance, Physics::Instrumentation and Detectors, [PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex], 01 natural sciences, 7. Clean energy, tellurium: oxygen, law.invention, Physics and Astronomy (all), CUORE, background: low, Contamination, double-beta decay: (0neutrino), bolometer, Observatory, law, Double beta decay, Validation, 0103 physical sciences, Neutrino Physics, 010306 general physics, Double Beta Decay, Particle Physics, Physics, Neutrino Physics, Double Beta Decay, Particle Physics, 010308 nuclear & particles physics, Bolometer, Detector, observatory, cryogenics, High Energy Physics::Experiment, tellurium: nuclide, experimental results
Abstract: International audience; The Cryogenic Underground Observatory for Rare Events (CUORE) is the first bolometric experiment searching for neutrinoless double beta decay that has been able to reach the 1-ton scale. The detector consists of an array of 988 TeO2 crystals arranged in a cylindrical compact structure of 19 towers. The construction of the experiment and the installation of all towers in the cryostat was completed in August 2016: the experiment is now in data taking phase. In this talk, beyond updating the physics results from CUORE-0, we will discuss the achievements and technical challenges of the CUORE construction phase, with particular emphasis on the background reduction strategy, the performance of the detector during pre-operation and the projected first results from the full detector run.
Published: 2017
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98. CUORE sensitivity to $0\nu \beta \beta $ decay

Author: L. Gladstone, T. I. Banks, James R. Wilson, D. R. Artusa, Vasundhara Singh, R. J. Creswick, Monica Sisti, M. Faverzani, B. Schmidt, B. S. Wang, Ettore Fiorini, S. Copello, K. Alfonso, M. L. Di Vacri, Lindley Winslow, C. Bucci, T. D. Gutierrez, O. Azzolini, Paolo Carniti, A. Bersani, L. Zanotti, G. Piperno, Claudio Gotti, L. Pattavina, M. M. Deninno, A. D'Addabbo, Stefano Dell'Oro, Guimin Zhang, Jeremy S. Cushman, M. Maino, Massimiliano Nastasi, L. Gironi, S. L. Wagaarachchi, E. V. Hansen, N. Casali, F. T. Avignone, H. W. Wang, F. Bellini, S. Zimmermann, S. Pirro, Carlo Ligi, Simone Capelli, R. W. Kadel, T. O'Donnell, M. Tenconi, C. Pira, S. Trentalange, A. Leder, C. Pagliarone, N. Moggi, T. Wise, M. Pavan, Oliviero Cremonesi, H. Z. Huang, G. Keppel, Davide Chiesa, C. Rosenfeld, D. Santone, Samuele Sangiorgio, K. E. Lim, Ioan Dafinei, C. Nones, P. Gorla, A. Nucciotti, F. Ferroni, Jeffrey W. Beeman, C. Tomei, C. Alduino, B. X. Zhu, V. Novati, V. Pettinacci, Emanuele Ferri, Eugene E. Haller, S. Morganti, M. I. Martínez, Nicholas Scielzo, A. Giuliani, G. Fernandes, A. Camacho, N. Chott, Alan R. Smith, C. J. Davis, Marco Pallavicini, G. Pessina, L. Taffarello, Massimiliano Clemenza, Carlo Cosmelli, C. Brofferio, P. J. Mosteiro, C. Rusconi, Y. Mei, M. Sakai, S. Di Domizio, R. Hennings-Yeomans, Xi-Guang Cao, Laura Cardani, K. M. Heeger, B. K. Fujikawa, Stefano Pozzi, A. Drobizhev, M. Vignati, Giovanni Benato, M. A. Franceschi, Ke Han, A. Branca, Reina H. Maruyama, Stuart J. Freedman, S. Zucchelli, A. Woodcraft, V. Palmieri, Eric B. Norman, T. Napolitano, F. Terranova, Jonathan Ouellet, G. Bari, M. Biassoni, A. Giachero, D. Q. Fang, L. Canonica, L. Marini, Kevin Hickerson, Y. G. Ma, J. Schmidt, L. Carbone, Yu. G. Kolomensky, Luigi Cappelli, Lorenzo Cassina, A. Caminata, Ezio Previtali, B. Welliver, Centre de Sciences Nucléaires et de Sciences de la Matière (CSNSM), 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), Département de Physique des Particules (ex SPP) (DPP), Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, CUORE, 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), Centre de Sciences Nucléaires et de Sciences de la Matière ( CSNSM ), 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 ), Département de Physique des Particules (ex SPP) ( DPP ), Institut de Recherches sur les lois Fondamentales de l'Univers ( IRFU ), Commissariat à l'énergie atomique et aux énergies alternatives ( CEA ) -Université Paris-Saclay-Commissariat à l'énergie atomique et aux énergies alternatives ( CEA ) -Université Paris-Saclay, and Département de Physique des Particules (ex SPP) (DPhP)
Subjects: Particle physics, Physics - Instrumentation and Detectors, Physics and Astronomy (miscellaneous), Data division, energy resolution, [PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex], 01 natural sciences, statistics: Bayesian, CUORE, double-beta decay: (0neutrino), Double beta decay, 0103 physical sciences, Beta (velocity), Sensitivity (control systems), [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], [ PHYS.NEXP ] Physics [physics]/Nuclear Experiment [nucl-ex], 010306 general physics, Nuclear Experiment, Engineering (miscellaneous), [ PHYS.PHYS.PHYS-INS-DET ] Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], Physics, 010308 nuclear & particles physics, background, sensitivity, Beta decay, Background level, numerical calculations: Monte Carlo, Energy (signal processing)
Abstract: We report a study of the CUORE sensitivity to neutrinoless double beta ($0\nu\beta\beta$) decay. We used a Bayesian analysis based on a toy Monte Carlo (MC) approach to extract the exclusion sensitivity to the $0\nu\beta\beta$ decay half-life ($T_{1/2}^{0\nu}$) at $90\%$ credibility interval (CI) -- i.e. the interval containing the true value of $T_{1/2}^{0\nu}$ with $90\%$ probability -- and the $3 \sigma$ discovery sensitivity. We consider various background levels and energy resolutions, and describe the influence of the data division in subsets with different background levels. If the background level and the energy resolution meet the expectation, CUORE will reach a $90\%$ CI exclusion sensitivity of $2\cdot10^{25}$ yr with $3$ months, and $9\cdot10^{25}$ yr with $5$ years of live time. Under the same conditions, the discovery sensitivity after $3$ months and $5$ years will be $7\cdot10^{24}$ yr and $4\cdot10^{25}$ yr, respectively., Comment: 10 pages, 3 figures, 4 tables
Published: 2017
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99. The Cryogenic Underground Observatory for Rare Events: Status and Prospects

Author: L. Cardani, Massimiliano Clemenza, Carlo Cosmelli, Y. Mei, K. M. Heeger, L. Gladstone, A. Bersani, N. Moggi, A. Woodcraft, Lorenzo Cassina, Ke Han, A. Branca, Reina H. Maruyama, Stuart J. Freedman, F. Terranova, N. Casali, Samuele Sangiorgio, A. Nucciotti, R. J. Creswick, Marco Pallavicini, C. Alduino, L. Zanotti, G. Piperno, G. Pessina, M. Faverzani, C. Brofferio, P. J. Mosteiro, Carlo Ligi, Yu-Gang Ma, Jeremy S. Cushman, M. Pavan, Oliviero Cremonesi, A. R. Smith, A. Caminata, Xu Cao, C. Nones, M. M. Deninno, I. Dafinei, E. Previtali, L. Canonica, A. Drobizhev, Davide Chiesa, K. E. Lim, S. Zucchelli, L. Marini, Kevin Hickerson, M. Tenconi, M. A. Franceschi, S. Morganti, R. Hennings-Yeomans, A. Giachero, V. Palmieri, Jeffrey W. Beeman, G. Fernandes, D. Q. Fang, Yu. G. Kolomensky, Luigi Cappelli, Eric B. Norman, C. Bucci, T. D. Gutierrez, Miriam Lucio Martinez, Jonathan Ouellet, T. Napolitano, A. Leder, N. Chott, G. Bari, L. Pattavina, Claudio Gotti, A. Giuliani, M. Biassoni, L. Carbone, S. Trentalange, D. Santone, C. Pagliarone, H. C. Huang, N. D. Scielzo, James R. Wilson, T. Wise, G. Keppel, D. R. Artusa, Monica Sisti, L. Gironi, S. Zimmermann, B. S. Wang, F. T. Avignone, O. Azzolini, S. Copello, Paolo Carniti, Stefano Dell'Oro, A. D'Addabbo, L. Taffarello, M. Maino, H. W. Wang, T. O'Donnell, Virendra Singh, Ettore Fiorini, C. Rosenfeld, Guimin Zhang, P. Gorla, F. Ferroni, C. Tomei, Emanuele Ferri, Eugene E. Haller, C. Pira, A. Camacho, K. Alfonso, M. L. Di Vacri, E. V. Hansen, T. I. Banks, C. Rusconi, B. X. Zhu, V. Novati, V. Pettinacci, Stefano Pirro, C. J. Davis, S. L. Wagaarachchi, Lindley Winslow, Simone Capelli, R. W. Kadel, F. Bellini, S. Di Domizio, B. K. Fujikawa, Stefano Pozzi, M. Vignati, Centre de Sciences Nucléaires et de Sciences de la Matière (CSNSM), 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), Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Massachusetts Institute of Technology. Department of Physics, Massachusetts Institute of Technology. Department of Nuclear Science and Engineering, and 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)
Subjects: Physics, CUORE, nucleus, Solar neutrino problem, tellurium: oxygen, Gran Sasso, Nuclear physics, observatory, MAJORANA, talk: Adelaide 2016/09/11, mass: hierarchy, bolometer, double-beta decay: (0neutrino), Observatory, Double-beta decay: (0neutrino) | observatory | neutrino: Majorana | neutrino: mass | mass: hierarchy | Gran Sasso | nucleus | CUORE | tellurium: oxygen | bolometer | experimental results, Double beta decay, [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex], neutrino: Majorana, Dilution refrigerator, neutrino: mass, Neutrino, Neutrino oscillation, experimental results
Abstract: International audience; The Cryogenic Underground Observatory for Rare Events (CUORE) is a large-scale double beta decay experiment utilizing cryogenic bolometers that is currently being commissioned at the Gran Sasso National Laboratory (LNGS) in Italy. Its primary focus is to search for the neutrinoless double beta decay of 130Te with a projected sensitivity to Majorana neutrino masses near the inverted mass hierarchy region. The detector is composed of 988 5x5x5-cm3 TeO2 crystals of natural isotopic composition arranged in 19 towers of 52 crystals each, all housed in a common dilution refrigerator. A single CUORE-like tower, CUORE-0, was assembled and operated as a stand-alone detector for a period of approximately two years. In this report, the results from CUORE-0 and the current status and physics potential of CUORE are presented.
Published: 2016
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100. Search for a diffuse flux of astrophysical muon neutrinos with the IceCube 59-string configuration

Author: J. Kläs, A. Stasik, Carsten Rott, I. Taboada, W. Huelsnitz, G. Binder, D. Pieloth, K. Rawlins, Dustin Hebecker, T. Fischer-Wasels, D. T. Grandmont, B. J. Whelan, J. J. Beatty, D. L. Xu, A. H. Cruz Silva, M. Lesiak-Bzdak, Juanan Aguilar, S. C. Nowicki, P. Redl, L. Schulte, J. Becker Tjus, E. Pinat, C. Finley, T. Schmidt, Sofia Vallecorsa, S. Flis, J. Daughhetee, M. Bissok, G. T. Przybylski, F. Huang, Olga Botner, K. Jero, N. L. Strotjohann, S. Schöneberg, D. Heinen, Jenni Adams, K. Hoshina, M. Kauer, G. Golup, K. Woschnagg, M. N. Tobin, F. Scheriau, A. Stößl, J. P. Rodrigues, T. Glüsenkamp, G. M. Spiczak, H. Landsman, H. P. Bretz, M. W.E. Smith, G. Yodh, A. Fedynitch, D. J. Koskinen, Reina H. Maruyama, K. Krings, Teresa Montaruli, J. Feintzeig, M. Stamatikos, O. Schulz, C. De Clercq, M. Vraeghe, G. S. Japaridze, P. B. Price, G. C. Hill, D. Chirkin, A. Schönwald, S. Coenders, M. Dunkman, Markus Ahlers, M. Labare, P. Gretskov, E. Unger, Y. Sestayo, M. Schmitz, K. D. de Vries, Maria Tselengidou, S. Ter-Antonyan, C. Sheremata, B. Eberhardt, P. Desiati, B. Kaminsky, D. Altmann, M. Wolf, J. Madsen, M. Rameez, T. Fuchs, D. Soldin, F. Clevermann, T. Ruhe, A. Groß, S. De Ridder, P. Zarzhitsky, D. Bindig, Tyce DeYoung, P. O. Hulth, A. Karle, L. Brayeur, M. Richman, R. Nahnhauer, A. M. Brown, S. Cohen, K. Hultqvist, C. Walck, M. Wellons, A. R. Fazely, Dariusz Gora, C. Bohm, L. Gladstone, G. Kroll, S. Miarecki, T. Waldenmaier, X. Bai, M. Krasberg, N. Whitehorn, R. C. Bay, J. Casey, B. Eichmann, Carlos Arguelles, S. Toscano, A. Olivas, S. Böser, S. Schoenen, S. R. Klein, B. Christy, T. Palczewski, Hermann Kolanoski, Segev BenZvi, S. Yoshida, Rezo Shanidze, M. Day, J. C. Díaz-Vélez, J. P. Yanez, M. Ribordy, R. Reimann, L. Paul, A. Haj Ismail, S. Seunarine, J. G. Gonzalez, S. Westerhoff, Elisa Bernardini, C. Ha, E. Middell, M. Wallraff, Thomas Meures, S. Tilav, T. R. Wood, D. J. Boersma, E. A. Strahler, J. C. Groh, Giorgio Maggi, K. Wiebe, M. Vehring, A. Omairat, L. Köpke, P. Hallen, M. Voge, Ch Weaver, J. Posselt, Elisa Resconi, D. Bose, M. Kowalski, A. Franckowiak, Markus Ackermann, D. Grant, C. Wendt, J. L. Kelley, J. A. Goodman, M. Danninger, U. Naumann, Todor Stanev, J. A. Pepper, H. Niederhausen, X. W. Xu, R. Hoffmann, Christian Spiering, J. Blumenthal, A. Ishihara, M. Casier, G. Tešić, H. G. Sander, D. Heereman, Wolfgang Rhode, R. G. Stokstad, Thomas K. Gaisser, S. Euler, T. Stezelberger, Subir Sarkar, K. Mase, D. Seckel, D. Berley, Stephanie Hickford, C. Pfendner, S. M. Saba, S. Kopper, J. C. Davis, J. Lünemann, G. Kohnen, Marcos Santander, A. Goldschmidt, J. Eisch, S. Odrowski, H. S. Matis, Kael Hanson, N. A. Stanisha, K. D. Hoffman, S. Hussain, B. Ruzybayev, Steven W. Barwick, K. Meagher, L. Gerhardt, Francis Halzen, P. A. Toale, K. Helbing, K. Filimonov, J. Van Santen, J. H. Köhne, T. Kuwabara, A. O'Murchadha, N. Milke, E. Blaufuss, N. Kurahashi, M. G. Aartsen, J. Leute, C. Kopper, R. Morse, O. Fadiran, J. Jacobsen, A. Van Overloop, R. Eagan, H. Wissing, V. Baum, K. Frantzen, P. A. Evenson, J. Ziemann, L. Mohrmann, S. Zierke, A. Obertacke, H. Taavola, R. Bruijn, M. Usner, P. Berghaus, T. Karg, C. H. Wiebusch, Oscar Macias, K. Jagielski, O. Jlelati, A. Bernhard, A. Kriesten, T. Feusels, R. Hellauer, G. W. Sullivan, J. P. A. M. de André, Allan Hallgren, J. S. Gallagher, L. Classen, M. Baker, M. Merck, B. Riedel, J. Auffenberg, E. Jacobi, A. Homeier, A. Tepe, A. Tamburro, M. Zoll, D. Z. Besson, L. Rädel, J. Miller, A. Christov, J. Kunnen, T. C. Arlen, N. Van Eijndhoven, C. Pérez De Los Heros, D. F. Cowen, M. J. Larson, D. R. Nygren, J. Kiryluk, Sally Robertson, M. Leuermann, K. Clark, D. R. Williams, Rasha Abbasi, Alexander Kappes, K. Schatto, D. Ryckbosch, F. McNally, R. Ström, A. Schukraft, K. H. Becker, and M. Quinnan
Subjects: SELECTION, HIGH-ENERGY NEUTRINOS, Nuclear and High Energy Physics, TELESCOPE, Astrophysics::High Energy Astrophysical Phenomena, Flux, FOS: Physical sciences, Cosmic ray, Astrophysics, 7. Clean energy, IceCube Neutrino Observatory, RATIO, Observatory, DETECTORS, ddc:530, Muon neutrino, Zenith, Physics, High Energy Astrophysical Phenomena (astro-ph.HE), Muon, ICE, PERFORMANCE, Physics and Astronomy, High Energy Physics::Experiment, Neutrino, Astrophysics - High Energy Astrophysical Phenomena
Abstract: A search for high-energy neutrinos was performed using data collected by the IceCube Neutrino Observatory from May 2009 to May 2010, when the array was running in its 59-string configuration. The data sample was optimized to contain muon neutrino induced events with a background contamination of atmospheric muons of less than 1%. These data, which are dominated by atmospheric neutrinos, are analyzed with a global likelihood fit to search for possible contributions of prompt atmospheric and astrophysical neutrinos, neither of which have yet been identified. Such signals are expected to follow a harder energy spectrum than conventional atmospheric neutrinos. In addition, the zenith angle distribution differs for astrophysical and atmospheric signals. A global fit of the reconstructed energies and directions of observed events is performed, including possible neutrino flux contributions for an astrophysical signal and atmospheric backgrounds as well as systematic uncertainties of the experiment and theoretical predictions. The best fit yields an astrophysical signal flux for $\nu_\mu + \bar\nu_\mu $ of $E^2 \cdot \Phi (E) = 0.25 \cdot 10^{-8} \textrm{GeV} \textrm{cm}^{-2} \textrm{s}^{-1} \textrm{sr}^{-1}$, and a zero prompt component. Although the sensitivity of this analysis for astrophysical neutrinos surpasses the Waxman and Bahcall upper bound, the experimental limit at 90% confidence level is a factor of 1.5 above at a flux of $E^2 \cdot \Phi (E) = 1.44 \cdot 10^{-8} \textrm{GeV} \textrm{cm}^{-2} \textrm{s}^{-1} \textrm{sr}^{-1}$., Comment: 18 pages, 13 figures. Submitted to Phys. Rev. D
Published: 2016
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