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1. Snowmass 2021 CMB-S4 White Paper

Author

Abazajian, Kevork, Abdulghafour, Arwa, Addison, Graeme E., Adshead, Peter, Ahmed, Zeeshan, Ajello, Marco, Akerib, Daniel, Allen, Steven W., Alonso, David, Alvarez, Marcelo, Amin, Mustafa A., Amiri, Mandana, Anderson, Adam, Ansarinejad, Behzad, Archipley, Melanie, Arnold, Kam S., Ashby, Matt, Aung, Han, Baccigalupi, Carlo, Baker, Carina, Bakshi, Abhishek, Bard, Debbie, Barkats, Denis, Barron, Darcy, Barry, Peter S., Bartlett, James G., Barton, Paul, Thakur, Ritoban Basu, Battaglia, Nicholas, Beall, Jim, Bean, Rachel, Beck, Dominic, Belkner, Sebastian, Benabed, Karim, Bender, Amy N., Benson, Bradford A., Besuner, Bobby, Bethermin, Matthieu, Bhimani, Sanah, Bianchini, Federico, Biquard, Simon, Birdwell, Ian, Bischoff, Colin A., Bleem, Lindsey, Bocaz, Paulina, Bock, James J., Bocquet, Sebastian, Boddy, Kimberly K., Bond, J. Richard, Borrill, Julian, Bouchet, Francois R., Brinckmann, Thejs, Brown, Michael L., Bryan, Sean, Buza, Victor, Byrum, Karen, Calabrese, Erminia, Calafut, Victoria, Caldwell, Robert, Carlstrom, John E., Carron, Julien, Cecil, Thomas, Challinor, Anthony, Chan, Victor, Chang, Clarence L., Chapman, Scott, Charles, Eric, Chauvin, Eric, Cheng, Cheng, Chesmore, Grace, Cheung, Kolen, Chinone, Yuji, Chluba, Jens, Cho, Hsiao-Mei Sherry, Choi, Steve, Clancy, Justin, Clark, Susan, Cooray, Asantha, Coppi, Gabriele, Corlett, John, Coulton, Will, Crawford, Thomas M., Crites, Abigail, Cukierman, Ari, Cyr-Racine, Francis-Yan, Dai, Wei-Ming, Daley, Cail, Dart, Eli, Daues, Gregorg, de Haan, Tijmen, Deaconu, Cosmin, Delabrouille, Jacques, Derylo, Greg, Devlin, Mark, Di Valentino, Eleonora, Dierickx, Marion, Dober, Brad, Doriese, Randy, Duff, Shannon, Dutcher, Daniel, Dvorkin, Cora, Dünner, Rolando, Eftekhari, Tarraneh, Eimer, Joseph, Bouhargani, Hamza El, Elleflot, Tucker, Emerson, Nick, Errard, Josquin, Essinger-Hileman, Thomas, Fabbian, Giulio, Fanfani, Valentina, Fasano, Alessandro, Feng, Chang, Ferraro, Simone, Filippini, Jeffrey P., Flauger, Raphael, Flaugher, Brenna, Fraisse, Aurelien A., Frisch, Josef, Frolov, Andrei, Galitzki, Nicholas, Gallardo, Patricio A., Galli, Silvia, Ganga, Ken, Gerbino, Martina, Giannakopoulos, Christos, Gilchriese, Murdock, Gluscevic, Vera, Goeckner-Wald, Neil, Goldfinger, David, Green, Daniel, Grimes, Paul, Grin, Daniel, Grohs, Evan, Gualtieri, Riccardo, Guarino, Vic, Gudmundsson, Jon E., Gullett, Ian, Guns, Sam, Habib, Salman, Haller, Gunther, Halpern, Mark, Halverson, Nils W., Hanany, Shaul, Hand, Emma, Harrington, Kathleen, Hasegawa, Masaya, Hasselfield, Matthew, Hazumi, Masashi, Heitmann, Katrin, Henderson, Shawn, Hensley, Brandon, Herbst, Ryan, Hervias-Caimapo, Carlos, Hill, J. Colin, Hills, Richard, Hivon, Eric, Hlozek, Renée, Ho, Anna, Holder, Gil, Hollister, Matt, Holzapfel, William, Hood, John, Hotinli, Selim, Hryciuk, Alec, Hubmayr, Johannes, Huffenberger, Kevin M., Hui, Howard, nez, Roberto Ibá, Ibitoye, Ayodeji, Ikape, Margaret, Irwin, Kent, Jacobus, Cooper, Jeong, Oliver, Johnson, Bradley R., Johnstone, Doug, Jones, William C., Joseph, John, Jost, Baptiste, Kang, Jae Hwan, Kaplan, Ari, Karkare, Kirit S., Katayama, Nobuhiko, Keskitalo, Reijo, King, Cesiley, Kisner, Theodore, Klein, Matthias, Knox, Lloyd, Koopman, Brian J., Kosowsky, Arthur, Kovac, John, Kovetz, Ely D., Krolewski, Alex, Kubik, Donna, Kuhlmann, Steve, Kuo, Chao-Lin, Kusaka, Akito, Lähteenmäki, Anne, Lau, Kenny, Lawrence, Charles R., Lee, Adrian T., Legrand, Louis, Leitner, Matthaeus, Leloup, Clément, Lewis, Antony, Li, Dale, Linder, Eric, Liodakis, Ioannis, Liu, Jia, Long, Kevin, Louis, Thibaut, Loverde, Marilena, Lowry, Lindsay, Lu, Chunyu, Lubin, Phil, Ma, Yin-Zhe, Maccarone, Thomas, Madhavacheril, Mathew S., Maldonado, Felipe, Mantz, Adam, Marques, Gabriela, Matsuda, Frederick, Mauskopf, Philip, May, Jared, McCarrick, Heather, McCracken, Ken, McMahon, Jeffrey, Meerburg, P. Daniel, Melin, Jean-Baptiste, Menanteau, Felipe, Meyers, Joel, Millea, Marius, Miranda, Vivian, Mitchell, Don, Mohr, Joseph, Moncelsi, Lorenzo, Monzani, Maria Elena, Moshed, Magdy, Mroczkowski, Tony, Mukherjee, Suvodip, Münchmeyer, Moritz, Nagai, Daisuke, Nagarajappa, Chandan, Nagy, Johanna, Namikawa, Toshiya, Nati, Federico, Natoli, Tyler, Nerval, Simran, Newburgh, Laura, Nguyen, Hogan, Nichols, Erik, Nicola, Andrina, Niemack, Michael D., Nord, Brian, Norton, Tim, Novosad, Valentine, O'Brient, Roger, Omori, Yuuki, Orlando, Giorgio, Osherson, Benjamin, Osten, Rachel, Padin, Stephen, Paine, Scott, Partridge, Bruce, Patil, Sanjaykumar, Petravick, Don, Petroff, Matthew, Pierpaoli, Elena, Pilleux, Mauricio, Pogosian, Levon, Prabhu, Karthik, Pryke, Clement, Puglisi, Giuseppe, Racine, Benjamin, Raghunathan, Srinivasan, Rahlin, Alexandra, Raveri, Marco, Reese, Ben, Reichardt, Christian L., Remazeilles, Mathieu, Rizzieri, Arianna, Rocha, Graca, Roe, Natalie A., Rotermund, Kaja, Roy, Anirban, Ruhl, John E., Saba, Joe, Sailer, Noah, Salatino, Maria, Saliwanchik, Benjamin, Sapozhnikov, Leonid, Rao, Mayuri Sathyanarayana, Saunders, Lauren, Schaan, Emmanuel, Schillaci, Alessandro, Schmitt, Benjamin, Scott, Douglas, Sehgal, Neelima, Shandera, Sarah, Sherwin, Blake D., Shirokoff, Erik, Shiu, Corwin, Simon, Sara M., Singari, Baibhav, Slosar, Anze, Spergel, David, Germaine, Tyler St., Staggs, Suzanne T., Stark, Antony A., Starkman, Glenn D., Steinbach, Bryan, Stompor, Radek, Stoughton, Chris, Suzuki, Aritoki, Tajima, Osamu, Tandoi, Chris, Teply, Grant P., Thayer, Gregg, Thompson, Keith, Thorne, Ben, Timbie, Peter, Tomasi, Maurizio, Trendafilova, Cynthia, Tristram, Matthieu, Tucker, Carole, Tucker, Gregory, Umiltà, Caterina, van Engelen, Alexander, van Marrewijk, Joshiwa, Vavagiakis, Eve M., Vergès, Clara, Vieira, Joaquin D., Vieregg, Abigail G., Wagoner, Kasey, Wallisch, Benjamin, Wang, Gensheng, Wang, Guo-Jian, Watson, Scott, Watts, Duncan, Weaver, Chris, Wenzl, Lukas, Westbrook, Ben, White, Martin, Whitehorn, Nathan, Wiedlea, Andrew, Williams, Paul, Wilson, Robert, Winch, Harrison, Wollack, Edward J., Wu, W. L. Kimmy, Xu, Zhilei, Yefremenko, Volodymyr G., Yu, Cyndia, Zegeye, David, Zivick, Jeff, and Zonca, Andrea

Subjects
Astrophysics - Cosmology and Nongalactic Astrophysics, Astrophysics - Instrumentation and Methods for Astrophysics, General Relativity and Quantum Cosmology, High Energy Physics - Experiment, High Energy Physics - Phenomenology
Abstract

This Snowmass 2021 White Paper describes the Cosmic Microwave Background Stage 4 project CMB-S4, which is designed to cross critical thresholds in our understanding of the origin and evolution of the Universe, from the highest energies at the dawn of time through the growth of structure to the present day. We provide an overview of the science case, the technical design, and project plan., Comment: Contribution to Snowmass 2021. arXiv admin note: substantial text overlap with arXiv:1908.01062, arXiv:1907.04473

Published
2022

2. Neutrino Physics with JUNO

Author

An, Fengpeng, An, Guangpeng, An, Qi, Antonelli, Vito, Baussan, Eric, Beacom, John, Bezrukov, Leonid, Blyth, Simon, Brugnera, Riccardo, Avanzini, Margherita Buizza, Busto, Jose, Cabrera, Anatael, Cai, Hao, Cai, Xiao, Cammi, Antonio, Cao, Guofu, Cao, Jun, Chang, Yun, Chen, Shaomin, Chen, Shenjian, Chen, Yixue, Chiesa, Davide, Clemenza, Massimiliano, Clerbaux, Barbara, Conrad, Janet, D'Angelo, Davide, De Kerret, Herve, Deng, Zhi, Deng, Ziyan, Ding, Yayun, Djurcic, Zelimir, Dornic, Damien, Dracos, Marcos, Drapier, Olivier, Dusini, Stefano, Dye, Stephen, Enqvist, Timo, Fan, Donghua, Fang, Jian, Favart, Laurent, Ford, Richard, Goger-Neff, Marianne, Gan, Haonan, Garfagnini, Alberto, Giammarchi, Marco, Gonchar, Maxim, Gong, Guanghua, Gong, Hui, Gonin, Michel, Grassi, Marco, Grewing, Christian, Guan, Mengyun, Guarino, Vic, Guo, Gang, Guo, Wanlei, Guo, Xin-Heng, Hagner, Caren, Han, Ran, He, Miao, Heng, Yuekun, Hsiung, Yee, Hu, Jun, Hu, Shouyang, Hu, Tao, Huang, Hanxiong, Huang, Xingtao, Huo, Lei, Ioannisian, Ara, Jeitler, Manfred, Ji, Xiangdong, Jiang, Xiaoshan, Jollet, Cecile, Kang, Li, Karagounis, Michael, Kazarian, Narine, Krumshteyn, Zinovy, Kruth, Andre, Kuusiniemi, Pasi, Lachenmaier, Tobias, Leitner, Rupert, Li, Chao, Li, Jiaxing, Li, Weidong, Li, Weiguo, Li, Xiaomei, Li, Xiaonan, Li, Yi, Li, Yufeng, Li, Zhi-Bing, Liang, Hao, Lin, Guey-Lin, Lin, Tao, Lin, Yen-Hsun, Ling, Jiajie, Lippi, Ivano, Liu, Dawei, Liu, Hongbang, Liu, Hu, Liu, Jianglai, Liu, Jianli, Liu, Jinchang, Liu, Qian, Liu, Shubin, Liu, Shulin, Lombardi, Paolo, Long, Yongbing, Lu, Haoqi, Lu, Jiashu, Lu, Jingbin, Lu, Junguang, Lubsandorzhiev, Bayarto, Ludhova, Livia, Luo, Shu, Lyashuk, Vladimir, Mollenberg, Randolph, Ma, Xubo, Mantovani, Fabio, Mao, Yajun, Mari, Stefano M., McDonough, William F., Meng, Guang, Meregaglia, Anselmo, Meroni, Emanuela, Mezzetto, Mauro, Miramonti, Lino, Mueller, Thomas, Naumov, Dmitry, Oberauer, Lothar, Ochoa-Ricoux, Juan Pedro, Olshevskiy, Alexander, Ortica, Fausto, Paoloni, Alessandro, Peng, Haiping, Peng, Jen-Chieh, Previtali, Ezio, Qi, Ming, Qian, Sen, Qian, Xin, Qian, Yongzhong, Qin, Zhonghua, Raffelt, Georg, Ranucci, Gioacchino, Ricci, Barbara, Robens, Markus, Romani, Aldo, Ruan, Xiangdong, Ruan, Xichao, Salamanna, Giuseppe, Shaevitz, Mike, Sinev, Valery, Sirignano, Chiara, Sisti, Monica, Smirnov, Oleg, Soiron, Michael, Stahl, Achim, Stanco, Luca, Steinmann, Jochen, Sun, Xilei, Sun, Yongjie, Taichenachev, Dmitriy, Tang, Jian, Tkachev, Igor, Trzaska, Wladyslaw, van Waasen, Stefan, Volpe, Cristina, Vorobel, Vit, Votano, Lucia, Wang, Chung-Hsiang, Wang, Guoli, Wang, Hao, Wang, Meng, Wang, Ruiguang, Wang, Siguang, Wang, Wei, Wang, Yi, Wang, Yifang, Wang, Zhe, Wang, Zheng, Wang, Zhigang, Wang, Zhimin, Wei, Wei, Wen, Liangjian, Wiebusch, Christopher, Wonsak, Bjorn, Wu, Qun, Wulz, Claudia-Elisabeth, Wurm, Michael, Xi, Yufei, Xia, Dongmei, Xie, Yuguang, Xing, Zhi-zhong, Xu, Jilei, Yan, Baojun, Yang, Changgen, Yang, Chaowen, Yang, Guang, Yang, Lei, Yang, Yifan, Yao, Yu, Yegin, Ugur, Yermia, Frederic, You, Zhengyun, Yu, Boxiang, Yu, Chunxu, Yu, Zeyuan, Zavatarelli, Sandra, Zhan, Liang, Zhang, Chao, Zhang, Hong-Hao, Zhang, Jiawen, Zhang, Jingbo, Zhang, Qingmin, Zhang, Yu-Mei, Zhang, Zhenyu, Zhao, Zhenghua, Zheng, Yangheng, Zhong, Weili, Zhou, Guorong, Zhou, Jing, Zhou, Li, Zhou, Rong, Zhou, Shun, Zhou, Wenxiong, Zhou, Xiang, Zhou, Yeling, Zhou, Yufeng, and Zou, Jiaheng

Subjects
Physics - Instrumentation and Detectors, High Energy Physics - Experiment
Abstract

The Jiangmen Underground Neutrino Observatory (JUNO), a 20 kton multi-purpose underground liquid scintillator detector, was proposed with the determination of the neutrino mass hierarchy as a primary physics goal. It is also capable of observing neutrinos from terrestrial and extra-terrestrial sources, including supernova burst neutrinos, diffuse supernova neutrino background, geoneutrinos, atmospheric neutrinos, solar neutrinos, as well as exotic searches such as nucleon decays, dark matter, sterile neutrinos, etc. We present the physics motivations and the anticipated performance of the JUNO detector for various proposed measurements. By detecting reactor antineutrinos from two power plants at 53-km distance, JUNO will determine the neutrino mass hierarchy at a 3-4 sigma significance with six years of running. The measurement of antineutrino spectrum will also lead to the precise determination of three out of the six oscillation parameters to an accuracy of better than 1\%. Neutrino burst from a typical core-collapse supernova at 10 kpc would lead to ~5000 inverse-beta-decay events and ~2000 all-flavor neutrino-proton elastic scattering events in JUNO. Detection of DSNB would provide valuable information on the cosmic star-formation rate and the average core-collapsed neutrino energy spectrum. Geo-neutrinos can be detected in JUNO with a rate of ~400 events per year, significantly improving the statistics of existing geoneutrino samples. The JUNO detector is sensitive to several exotic searches, e.g. proton decay via the $p\to K^++\bar\nu$ decay channel. The JUNO detector will provide a unique facility to address many outstanding crucial questions in particle and astrophysics. It holds the great potential for further advancing our quest to understanding the fundamental properties of neutrinos, one of the building blocks of our Universe., Comment: Version submitted to Journal of Physics G, with minor typo corrections. 222 Pages, 147 figures

Published
2015
Full Text
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3. Neutrino physics with JUNO

Author

An, Fengpeng, An, Guangpeng, An, Qi, Antonelli, Vito, Baussan, Eric, Beacom, John, Bezrukov, Leonid, Blyth, Simon, Brugnera, Riccardo, Avanzini, Margherita Buizza, Busto, Jose, Cabrera, Anatael, Cai, Hao, Cai, Xiao, Cammi, Antonio, Cao, Guofu, Cao, Jun, Chang, Yun, Chen, Shaomin, Chen, Shenjian, Chen, Yixue, Chiesa, Davide, Clemenza, Massimiliano, Clerbaux, Barbara, Conrad, Janet, D’Angelo, Davide, De Kerret, Hervé, Deng, Zhi, Deng, Ziyan, Ding, Yayun, Djurcic, Zelimir, Dornic, Damien, Dracos, Marcos, Drapier, Olivier, Dusini, Stefano, Dye, Stephen, Enqvist, Timo, Fan, Donghua, Fang, Jian, Favart, Laurent, Ford, Richard, Göger-Neff, Marianne, Gan, Haonan, Garfagnini, Alberto, Giammarchi, Marco, Gonchar, Maxim, Gong, Guanghua, Gong, Hui, Gonin, Michel, Grassi, Marco, Grewing, Christian, Guan, Mengyun, Guarino, Vic, Guo, Gang, Guo, Wanlei, Guo, Xin-Heng, Hagner, Caren, Han, Ran, He, Miao, Heng, Yuekun, Hsiung, Yee, Hu, Jun, Hu, Shouyang, Hu, Tao, Huang, Hanxiong, Huang, Xingtao, Huo, Lei, Ioannisian, Ara, Jeitler, Manfred, Ji, Xiangdong, Jiang, Xiaoshan, Jollet, Cécile, Kang, Li, Karagounis, Michael, Kazarian, Narine, Krumshteyn, Zinovy, Kruth, Andre, Kuusiniemi, Pasi, Lachenmaier, Tobias, Leitner, Rupert, Li, Chao, Li, Jiaxing, Li, Weidong, Li, Weiguo, Li, Xiaomei, Li, Xiaonan, Li, Yi, Li, Yufeng, Li, Zhi-Bing, Liang, Hao, Lin, Guey-Lin, Lin, Tao, Lin, Yen-Hsun, Ling, Jiajie, Lippi, Ivano, Liu, Dawei, Liu, Hongbang, Liu, Hu, Liu, Jianglai, and Liu, Jianli

Subjects
Affordable and Clean Energy, reactor neutrino experiments, large scintillator detectors, neutrino physics, neutrino astronomy, physics.ins-det, hep-ex, Atomic, Molecular, Nuclear, Particle and Plasma Physics, Nuclear & Particles Physics
Abstract

The Jiangmen Underground Neutrino Observatory (JUNO), a 20 kton multi-purpose underground liquid scintillator detector, was proposed with the determination of the neutrino mass hierarchy (MH) as a primary physics goal. The excellent energy resolution and the large fiducial volume anticipated for the JUNO detector offer exciting opportunities for addressing many important topics in neutrino and astro-particle physics. In this document, we present the physics motivations and the anticipated performance of the JUNO detector for various proposed measurements. Following an introduction summarizing the current status and open issues in neutrino physics, we discuss how the detection of antineutrinos generated by a cluster of nuclear power plants allows the determination of the neutrino MH at a 3-4σ significance with six years of running of JUNO. The measurement of antineutrino spectrum with excellent energy resolution will also lead to the precise determination of the neutrino oscillation parameters sin2θ12, Δm212, and | Δmee2 to an accuracy of better than 1%, which will play a crucial role in the future unitarity test of the MNSP matrix. The JUNO detector is capable of observing not only antineutrinos from the power plants, but also neutrinos/antineutrinos from terrestrial and extra-terrestrial sources, including supernova burst neutrinos, diffuse supernova neutrino background, geoneutrinos, atmospheric neutrinos, and solar neutrinos. As a result of JUNO's large size, excellent energy resolution, and vertex reconstruction capability, interesting new data on these topics can be collected. For example, a neutrino burst from a typical core-collapse supernova at a distance of 10 kpc would lead to ∼5000 inverse-beta-decay events and ∼2000 all-flavor neutrino-proton ES events in JUNO, which are of crucial importance for understanding the mechanism of supernova explosion and for exploring novel phenomena such as collective neutrino oscillations. Detection of neutrinos from all past core-collapse supernova explosions in the visible universe with JUNO would further provide valuable information on the cosmic star-formation rate and the average core-collapse neutrino energy spectrum. Antineutrinos originating from the radioactive decay of uranium and thorium in the Earth can be detected in JUNO with a rate of ∼400 events per year, significantly improving the statistics of existing geoneutrino event samples. Atmospheric neutrino events collected in JUNO can provide independent inputs for determining the MH and the octant of the θ23 mixing angle. Detection of the 7Be and 8B solar neutrino events at JUNO would shed new light on the solar metallicity problem and examine the transition region between the vacuum and matter dominated neutrino oscillations. Regarding light sterile neutrino topics, sterile neutrinos with 10-5 eV2 < Δm412 < 10-2 eV2 and a sufficiently large mixing angle θ14 could be identified through a precise measurement of the reactor antineutrino energy spectrum. Meanwhile, JUNO can also provide us excellent opportunities to test the eV-scale sterile neutrino hypothesis, using either the radioactive neutrino sources or a cyclotron-produced neutrino beam. The JUNO detector is also sensitive to several other beyondthe-standard-model physics. Examples include the search for proton decay via the p → K+ + ν decay channel, search for neutrinos resulting from dark-matter annihilation in the Sun, search for violation of Lorentz invariance via the sidereal modulation of the reactor neutrino event rate, and search for the effects of non-standard interactions. The proposed construction of the JUNO detector will provide a unique facility to address many outstanding crucial questions in particle and astrophysics in a timely and cost-effective fashion. It holds the great potential for further advancing our quest to understanding the fundamental properties of neutrinos, one of the building blocks of our Universe.

Published
2016

4. Neutrino Physics with JUNO

Author

Jilei Xu, Andre Kruth, Yuguang Xie, Wei Wang, S. M. Chen, Janet Conrad, Xingtao Huang, V. Vorobel, Jose Busto, Qi An, Alexander Olshevskiy, Jiaxing Li, Cécile Jollet, Xiangdong Ji, Ran Han, Sandra Zavatarelli, Dmitriy Taichenachev, F. Yermia, Georg G. Raffelt, R. Möllenberg, Yong Zhong Qian, Ugur Yegin, Yu Yao, Wenxiong Zhou, Siguang Wang, Zheng Wang, Zhenyu Zhang, Rupert Leitner, M. Göger-Neff, Lino Miramonti, Qun Wu, O. Drapier, Donghua Fan, Jen-Chieh Peng, D. W. Liu, Stephen T. Dye, Hao Cai, John F. Beacom, Lucia Votano, Massimiliano Clemenza, Juan Pedro Ochoa-Ricoux, Davide Chiesa, Tao Hu, Igor Tkachev, Fabio Mantovani, Hongbang Liu, Jiawen Zhang, J. G. Lu, Shulin Liu, Baojun Yan, Weili Zhong, Changgen Yang, A. Garfagnini, Antonio Cammi, Liangjian Wen, Guofu Cao, Christopher Wiebusch, Michael Wurm, Anselmo Meregaglia, Xubo Ma, Boxiang Yu, G. Meng, Damien Dornic, Vladimir Lyashuk, Björn Wonsak, Anatael Cabrera, Y. H. Zhou, Jochen Steinmann, M. Soiron, S. Dusini, Xiaomei Li, Honghao Zhang, Yajun Mao, Gang Guo, Y. B. Hsiung, Z. V. Krumshteyn, Marco Grassi, Guanghua Gong, Guang Yang, Zhi Deng, Laurent Favart, Shaomin Chen, Jun Cao, Lothar Oberauer, Xilei Sun, Herve De Kerret, Hao Liang, Ara Ioannisian, Yufei Xi, Monica Sisti, Chao Li, Yuekun Heng, Yifang Wang, Alessandro Paoloni, Stefan van Waasen, Qingmin Zhang, Meng Wang, Shouyang Hu, Jing Zhou, Dongmei Xia, Yongjie Sun, G. Salamanna, Ezio Previtali, Mengyun Guan, Thomas Mueller, Bayarto Lubsandorzhiev, Xin Heng Guo, Guorong Zhou, Xiao Cai, Guey-Lin Lin, Zhimin Wang, Margherita Buizza Avanzini, Mauro Mezzetto, Barbara Ricci, Hu Liu, Chiara Sirignano, William F. McDonough, Xichao Ruan, Dmitry V. Naumov, Jiajie Ling, Ziyan Deng, Haoqi Lu, Jianglai Liu, Paolo Lombardi, Xiang Zhou, Manfred Jeitler, Weiguo Li, Christian Grewing, Barbara Clerbaux, Jianli Liu, Jian Fang, Yi Chen, Ming Qi, Oleg Smirnov, L. B. Bezrukov, Narine Kazarian, Yangheng Zheng, Wanlei Guo, Marcos Dracos, Jinchang Liu, Hui Gong, Ivano Lippi, Michael Karagounis, Stefano Maria Mari, Vito Antonelli, Miao He, Zhengyun You, Yayun Ding, Richard Ford, Zelimir Djurcic, Qian Liu, Zhonghua Qin, Jian Tang, E. Meroni, Shubin Liu, Ruiguang Wang, Jingbo Zhang, Rong Zhou, Timo Enqvist, Zhe Wang, V. V. Sinev, Simon Blyth, Zhenghua Zhao, Yi Wang, Yumei Zhang, Yi Li, Zeyuan Yu, Tobias Lachenmaier, Marco Giammarchi, Yongbing Long, Maxim Gonchar, Wei Wei, D. D'Angelo, Sen Qian, Shu Luo, Caren Hagner, Claudia-Elisabeth Wulz, H. Peng, Jiaheng Zou, Liang Zhan, Yifan Yang, Chunxu Yu, Wei Li, Markus Robens, Fengpeng An, Xiaoshan Jiang, Yen-Hsun Lin, Pasi Kuusiniemi, Zhibing Li, Luca Stanco, Fausto Ortica, Chao Zhang, Guangpeng An, Xiangdong Ruan, R. Brugnera, Achim Stahl, Eric Baussan, Yufeng Li, Livia Ludhova, Chung Hsiang Wang, Lei Huo, Vic Guarino, Tao Lin, X. N. Li, Haonan Gan, Lei Yang, Hao Wang, M. Gonin, Ye-Ling Zhou, Yun Chang, M. H. Shaevitz, Xin Qian, Wladyslaw Henryk Trzaska, Li Zhou, C. G. Yang, Zhi-zhong Xing, Jingbin Lu, Aldo Romani, Shun Zhou, Cristina Volpe, Li Kang, Junguang Lu, Gioacchino Ranucci, Hanxiong Huang, Guo-Li Wang, Jun Hu, Institut Pluridisciplinaire Hubert Curien (IPHC), Université de Strasbourg (UNISTRA)-Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Laboratoire Leprince-Ringuet (LLR), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-École polytechnique (X)-Centre National de la Recherche Scientifique (CNRS), Centre de Physique des Particules de Marseille (CPPM), Aix Marseille Université (AMU)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Laboratoire SUBATECH Nantes (SUBATECH), Mines Nantes (Mines Nantes)-Université de Nantes (UN)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), JUNO, An, F, An, G, An, Q, Antonelli, V, Baussan, E, Beacom, J, Bezrukov, L, Blyth, S, Brugnera, R, Avanzini, M, Busto, J, Cabrera, A, Cai, H, Cai, X, Cammi, A, Cao, G, Cao, J, Chang, Y, Chen, S, Chen, Y, Chiesa, D, Clemenza, M, Clerbaux, B, Conrad, J, D'Angelo, D, De Kerret, H, Deng, Z, Ding, Y, Djurcic, Z, Dornic, D, Dracos, M, Drapier, O, Dusini, S, Dye, S, Enqvist, T, Fan, D, Fang, J, Favart, L, Ford, R, Göger Neff, M, Gan, H, Garfagnini, A, Giammarchi, M, Gonchar, M, Gong, G, Gong, H, Gonin, M, Grassi, M, Grewing, C, Guan, M, Guarino, V, Guo, G, Guo, W, Guo, X, Hagner, C, Han, R, He, M, Heng, Y, Hsiung, Y, Hu, J, Hu, S, Hu, T, Huang, H, Huang, X, Huo, L, Ioannisian, A, Jeitler, M, Ji, X, Jiang, X, Jollet, C, Kang, L, Karagounis, M, Kazarian, N, Krumshteyn, Z, Kruth, A, Kuusiniemi, P, Lachenmaier, T, Leitner, R, Li, C, Li, J, Li, W, Li, X, Li, Y, Li, Z, Liang, H, Lin, G, Lin, T, Lin, Y, Ling, J, Lippi, I, Liu, D, Liu, H, Liu, J, Liu, Q, Liu, S, Lombardi, P, Long, Y, Lu, H, Lu, J, Lubsandorzhiev, B, Ludhova, L, Luo, S, Lyashuk, V, Möllenberg, R, Ma, X, Mantovani, F, Mao, Y, Mari, S, Mcdonough, W, Meng, G, Meregaglia, A, Meroni, E, Mezzetto, M, Miramonti, L, Mueller, T, Naumov, D, Oberauer, L, Ochoa Ricoux, J, Olshevskiy, A, Ortica, F, Paoloni, A, Peng, H, Peng, J, Previtali, E, Qi, M, Qian, S, Qian, X, Qian, Y, Qin, Z, Raffelt, G, Ranucci, G, Ricci, B, Robens, M, Romani, A, Ruan, X, Salamanna, G, Shaevitz, M, Sinev, V, Sirignano, C, Sisti, M, Smirnov, O, Soiron, M, Stahl, A, Stanco, L, Steinmann, J, Sun, X, Sun, Y, Taichenachev, D, Tang, J, Tkachev, I, Trzaska, W, Van Waasen, S, Volpe, C, Vorobel, V, Votano, L, Wang, C, Wang, G, Wang, H, Wang, M, Wang, R, Wang, S, Wang, W, Wang, Y, Wang, Z, Wei, W, Wen, L, Wiebusch, C, Wonsak, B, Wu, Q, Wulz, C, Wurm, M, Xi, Y, Xia, D, Xie, Y, Xing, Z, Xu, J, Yan, B, Yang, C, Yang, G, Yang, L, Yang, Y, Yao, Y, Yegin, U, Yermia, F, You, Z, Yu, B, Yu, C, Yu, Z, Zavatarelli, S, Zhan, L, Zhang, C, Zhang, H, Zhang, J, Zhang, Q, Zhang, Y, Zhang, Z, Zhao, Z, Zheng, Y, Zhong, W, Zhou, G, Zhou, J, Zhou, L, Zhou, R, Zhou, S, Zhou, W, Zhou, X, Zhou, Y, Zou, J, Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université de Strasbourg (UNISTRA)-Centre National de la Recherche Scientifique (CNRS), Centre National de la Recherche Scientifique (CNRS)-École polytechnique (X)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université de Nantes (UN)-Mines Nantes (Mines Nantes), An, Fengpeng, An, Guangpeng, An, Qi, Antonelli, Vito, Baussan, Eric, Beacom, John, Bezrukov, Leonid, Blyth, Simon, Brugnera, Riccardo, Avanzini, Margherita Buizza, Busto, Jose, Cabrera, Anatael, Cai, Hao, Cai, Xiao, Cammi, Antonio, Cao, Guofu, Cao, Jun, Chang, Yun, Chen, Shaomin, Chen, Shenjian, Chen, Yixue, Chiesa, Davide, Clemenza, Massimiliano, Clerbaux, Barbara, Conrad, Janet, D’Angelo, Davide, Kerret, Hervé De, Deng, Zhi, Deng, Ziyan, Ding, Yayun, Djurcic, Zelimir, Dornic, Damien, Dracos, Marco, Drapier, Olivier, Dusini, Stefano, Dye, Stephen, Enqvist, Timo, Fan, Donghua, Fang, Jian, Favart, Laurent, Ford, Richard, Göger Neff, Marianne, Gan, Haonan, Garfagnini, Alberto, Giammarchi, Marco, Gonchar, Maxim, Gong, Guanghua, Gong, Hui, Gonin, Michel, Grassi, Marco, Grewing, Christian, Guan, Mengyun, Guarino, Vic, Guo, Gang, Guo, Wanlei, Guo, Xin Heng, Hagner, Caren, Han, Ran, He, Miao, Heng, Yuekun, Hsiung, Yee, Hu, Jun, Hu, Shouyang, Hu, Tao, Huang, Hanxiong, Huang, Xingtao, Huo, Lei, Ioannisian, Ara, Jeitler, Manfred, Ji, Xiangdong, Jiang, Xiaoshan, Jollet, Cécile, Kang, Li, Karagounis, Michael, Kazarian, Narine, Krumshteyn, Zinovy, Kruth, Andre, Kuusiniemi, Pasi, Lachenmaier, Tobia, Leitner, Rupert, Li, Chao, Li, Jiaxing, Li, Weidong, Li, Weiguo, Li, Xiaomei, Li, Xiaonan, Li, Yi, Li, Yufeng, Li, Zhi Bing, Liang, Hao, Lin, Guey Lin, Lin, Tao, Lin, Yen Hsun, Ling, Jiajie, Lippi, Ivano, Liu, Dawei, Liu, Hongbang, Liu, Hu, Liu, Jianglai, Liu, Jianli, Liu, Jinchang, Liu, Qian, Liu, Shubin, Liu, Shulin, Lombardi, Paolo, Long, Yongbing, Lu, Haoqi, Lu, Jiashu, Lu, Jingbin, Lu, Junguang, Lubsandorzhiev, Bayarto, Ludhova, Livia, Luo, Shu, Vladimir Lyashuk, Null, Möllenberg, Randolph, Ma, Xubo, Mantovani, Fabio, Mao, Yajun, Mari, Stefano Maria, Mcdonough, William F, Meng, Guang, Meregaglia, Anselmo, Meroni, Emanuela, Mezzetto, Mauro, Miramonti, Lino, Thomas Mueller, Null, Naumov, Dmitry, Oberauer, Lothar, Ochoa Ricoux, Juan Pedro, Olshevskiy, Alexander, Ortica, Fausto, Paoloni, Alessandro, Peng, Haiping, Jen Chieh Peng, Null, Previtali, Ezio, Qi, Ming, Qian, Sen, Qian, Xin, Qian, Yongzhong, Qin, Zhonghua, Raffelt, Georg, Ranucci, Gioacchino, Ricci, Barbara, Robens, Marku, Romani, Aldo, Ruan, Xiangdong, Ruan, Xichao, Salamanna, Giuseppe, Shaevitz, Mike, Valery Sinev, Null, Sirignano, Chiara, Sisti, Monica, Smirnov, Oleg, Soiron, Michael, Stahl, Achim, Stanco, Luca, Steinmann, Jochen, Sun, Xilei, Sun, Yongjie, Taichenachev, Dmitriy, Tang, Jian, Tkachev, Igor, Trzaska, Wladyslaw, Waasen, Stefan van, Volpe, Cristina, Vorobel, Vit, Votano, Lucia, Wang, Chung Hsiang, Wang, Guoli, Wang, Hao, Wang, Meng, Wang, Ruiguang, Wang, Siguang, Wang, Wei, Wang, Yi, Wang, Yifang, Wang, Zhe, Wang, Zheng, Wang, Zhigang, Wang, Zhimin, Wei, Wei, Wen, Liangjian, Wiebusch, Christopher, Wonsak, Björn, Wu, Qun, Wulz, Claudia Elisabeth, Wurm, Michael, Xi, Yufei, Xia, Dongmei, Xie, Yuguang, Zhi zhong Xing, Null, Xu, Jilei, Yan, Baojun, Yang, Changgen, Yang, Chaowen, Yang, Guang, Yang, Lei, Yang, Yifan, Yao, Yu, Yegin, Ugur, Yermia, Frédéric, You, Zhengyun, Yu, Boxiang, Yu, Chunxu, Yu, Zeyuan, Zavatarelli, Sandra, Zhan, Liang, Zhang, Chao, Zhang, Hong Hao, Zhang, Jiawen, Zhang, Jingbo, Zhang, Qingmin, Zhang, Yu Mei, Zhang, Zhenyu, Zhao, Zhenghua, Zheng, Yangheng, Zhong, Weili, Zhou, Guorong, Zhou, Jing, Zhou, Li, Zhou, Rong, Zhou, Shun, Zhou, Wenxiong, Zhou, Xiang, Zhou, Yeling, Zhou, Yufeng, Zou, Jiaheng, Université de Strasbourg (UNISTRA)-Centre National de la Recherche Scientifique (CNRS), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Aix Marseille Université (AMU), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), Massachusetts Institute of Technology. Department of Physics, and Conrad, Janet Marie

Subjects
Particle physics, Sterile neutrino, Nuclear and High Energy Physics, Physics - Instrumentation and Detectors, Geoneutrino, reactor neutrino experiment, Physics::Instrumentation and Detectors, Solar neutrino, media_common.quotation_subject, Astrophysics::High Energy Astrophysical Phenomena, Dark matter, FOS: Physical sciences, 7. Clean energy, 01 natural sciences, NO, High Energy Physics - Experiment, neutrino astronomy, High Energy Physics - Experiment (hep-ex), neutrino physics, 0103 physical sciences, [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex], ddc:530, neutrino, mass hierarchy, reactor, liquid scintillator, 010306 general physics, Jiangmen Underground Neutrino Observatory, media_common, Physics, 010308 nuclear & particles physics, High Energy Physics::Phenomenology, neutrino physic, Instrumentation and Detectors (physics.ins-det), Universe, reactor neutrino experiments, large scintillator detectors, Supernova, 13. Climate action, Physics::Space Physics, large scintillator detector, High Energy Physics::Experiment, Neutrino
Abstract

The Jiangmen Underground Neutrino Observatory (JUNO), a 20 kton multi-purpose underground liquid scintillator detector, was proposed with the determination of the neutrino mass hierarchy as a primary physics goal. It is also capable of observing neutrinos from terrestrial and extra-terrestrial sources, including supernova burst neutrinos, diffuse supernova neutrino background, geoneutrinos, atmospheric neutrinos, solar neutrinos, as well as exotic searches such as nucleon decays, dark matter, sterile neutrinos, etc. We present the physics motivations and the anticipated performance of the JUNO detector for various proposed measurements. By detecting reactor antineutrinos from two power plants at 53-km distance, JUNO will determine the neutrino mass hierarchy at a 3-4 sigma significance with six years of running. The measurement of antineutrino spectrum will also lead to the precise determination of three out of the six oscillation parameters to an accuracy of better than 1\%. Neutrino burst from a typical core-collapse supernova at 10 kpc would lead to ~5000 inverse-beta-decay events and ~2000 all-flavor neutrino-proton elastic scattering events in JUNO. Detection of DSNB would provide valuable information on the cosmic star-formation rate and the average core-collapsed neutrino energy spectrum. Geo-neutrinos can be detected in JUNO with a rate of ~400 events per year, significantly improving the statistics of existing geoneutrino samples. The JUNO detector is sensitive to several exotic searches, e.g. proton decay via the $p\to K^++\bar\nu$ decay channel. The JUNO detector will provide a unique facility to address many outstanding crucial questions in particle and astrophysics. It holds the great potential for further advancing our quest to understanding the fundamental properties of neutrinos, one of the building blocks of our Universe., Comment: Version submitted to Journal of Physics G, with minor typo corrections. 222 Pages, 147 figures

Published
2016

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