A next-generation liquid xenon observatory for dark matter and neutrino physics. (1st January 2023)

• Record Type: Journal Article
• Authors: Aalbers, J; AbdusSalam, S S; Abe, K; Aerne, V; Agostini, F; Ahmed Maouloud, S; Akerib, D S; Akimov, D Y; Akshat, J; Al Musalhi, A K; Alder, F; Alsum, S K; Althueser, L; Amarasinghe, C S; Amaro, F D; Ames, A; Anderson, T J; Andrieu, B; Angelides, N; Angelino, E; Angevaare, J; Antochi, V C; Antón Martin, D; Antunovic, B; Aprile, E; Araújo, H M; Armstrong, J E; Arneodo, F; Arthurs, M; Asadi, P; Baek, S; Bai, X; Bajpai, D; Baker, A; Balajthy, J; Balashov, S; Balzer, M; Bandyopadhyay, A; Bang, J; Barberio, E; Bargemann, J W; Baudis, L; Bauer, D; Baur, D; Baxter, A; Baxter, A L; Bazyk, M; Beattie, K; Behrens, J; Bell, N F; Bellagamba, L; Beltrame, P; Benabderrahmane, M; Bernard, E P; Bertone, G F; Bhattacharjee, P; Bhatti, A; Biekert, A; Biesiadzinski, T P; Binau, A R; Biondi, R; Biondi, Y; Birch, H J; Bishara, F; Bismark, A; Blanco, C; Blockinger, G M; Bodnia, E; Boehm, C; Bolozdynya, A I; Bolton, P D; Bottaro, S; Bourgeois, C; Boxer, B; Brás, P; Breskin, A; Breur, P A; Brew, C A J; Brod, J; Brookes, E; Brown, A; Brown, E; Bruenner, S; Bruno, G; Budnik, R; Bui, T K; Burdin, S; Buse, S; Busenitz, J K; Buttazzo, D; Buuck, M; Buzulutskov, A; Cabrita, R; Cai, C; Cai, D; Capelli, C; Cardoso, J M R; Carmona-Benitez, M C; Cascella, M; Catena, R; Chakraborty, S; Chan, C; Chang, S; Chauvin, A; Chawla, A; Chen, H; Chepel, V; Chott, N I; Cichon, D; Cimental Chavez, A; Cimmino, B; Clark, M; Co, R T; Colijn, A P; Conrad, J; Converse, M V; Costa, M; Cottle, A; Cox, G; Creaner, O; Cuenca Garcia, J J; Cussonneau, J P; Cutter, J E; Dahl, C E; D'Andrea, V; David, A; Decowski, M P; Dent, J B; Deppisch, F F; de Viveiros, L; Di Gangi, P; Di Giovanni, A; Di Pede, S; Dierle, J; Diglio, S; Dobson, J E Y; Doerenkamp, M; Douillet, D; Drexlin, G; Druszkiewicz, E; Dunsky, D; Eitel, K; Elykov, A; Emken, T; Engel, R; Eriksen, S R; Fairbairn, M; Fan, A; Fan, J J; Farrell, S J; Fayer, S; Fearon, N M; Ferella, A; Ferrari, C; Fieguth, A; Fieguth, A; Fiorucci, S; Fischer, H; Flaecher, H; Flierman, M; Florek, T; Foot, R; Fox, P J; Franceschini, R; Fraser, E D; Frenk, C S; Frohlich, S; Fruth, T; Fulgione, W; Fuselli, C; Gaemers, P; Gaior, R; Gaitskell, R J; Galloway, M; Gao, F; Garcia Garcia, I; Genovesi, J; Ghag, C; Ghosh, S; Gibson, E; Gil, W; Giovagnoli, D; Girard, F; Glade-Beucke, R; Glück, F; Gokhale, S; de Gouvêa, A; Gráf, L; Grandi, L; Grigat, J; Grinstein, B; van der Grinten, M G D; Grössle, R; Guan, H; Guida, M; Gumbsheimer, R; Gwilliam, C B; Hall, C R; Hall, L J; Hammann, R; Han, K; Hannen, V; Hansmann-Menzemer, S; Harata, R; Hardin, S P; Hardy, E; Hardy, C A; Harigaya, K; Harnik, R; Haselschwardt, S J; Hernandez, M; Hertel, S A; Higuera, A; Hils, C; Hochrein, S; Hoetzsch, L; Hoferichter, M; Hood, N; Hooper, D; Horn, M; Howlett, J; Huang, D Q; Huang, Y; Hunt, D; Iacovacci, M; Iaquaniello, G; Ide, R; Ignarra, C M; Iloglu, G; Itow, Y; Jacquet, E; Jahangir, O; Jakob, J; James, R S; Jansen, A; Ji, W; Ji, X; Joerg, F; Johnson, J; Joy, A; Kaboth, A C; Kalhor, L; Kamaha, A C; Kanezaki, K; Kar, K; Kara, M; Kato, N; Kavrigin, P; Kazama, S; Keaveney, A W; Kellerer, J; Khaitan, D; Khazov, A; Khundzakishvili, G; Khurana, I; Kilminster, B; Kleifges, M; Ko, P; Kobayashi, M; Kodroff, D; Koltmann, G; Kopec, A; Kopmann, A; Kopp, J; Korley, L; Kornoukhov, V N; Korolkova, E V; Kraus, H; Krauss, L M; Kravitz, S; Kreczko, L; Kudryavtsev, V A; Kuger, F; Kumar, J; López Paredes, B; LaCascio, L; Laha, R; Laine, Q; Landsman, H; Lang, R F; Leason, E A; Lee, J; Leonard, D S; Lesko, K T; Levinson, L; Levy, C; Li, I; Li, S C; Li, T; Liang, S; Liebenthal, C S; Lin, J; Lin, Q; Lindemann, S; Lindner, M; Lindote, A; Linehan, R; Lippincott, W H; Liu, X; Liu, K; Liu, J; Loizeau, J; Lombardi, F; Long, J; Lopes, M I; Lopez Asamar, E; Lorenzon, W; Lu, C; Luitz, S; Ma, Y; Machado, P A N; Macolino, C; Maeda, T; Mahlstedt, J; Majewski, P A; Manalaysay, A; Mancuso, A; Manenti, L; Manfredini, A; Mannino, R L; Marangou, N; March-Russell, J; Marignetti, F; Marrodán Undagoitia, T; Martens, K; Martin, R; Martinez-Soler, I; Masbou, J; Masson, D; Masson, E; Mastroianni, S; Mastronardi, M; Matias-Lopes, J A; McCarthy, M E; McFadden, N; McGinness, E; McKinsey, D N; McLaughlin, J; McMichael, K; Meinhardt, P; Menéndez, J; Meng, Y; Messina, M; Midha, R; Milisavljevic, D; Miller, E H; Milosevic, B; Milutinovic, S; Mitra, S A; Miuchi, K; Mizrachi, E; Mizukoshi, K; Molinario, A; Monte, A; Monteiro, C M B; Monzani, M E; Moore, J S; Morå, K; Morad, J A; Morales Mendoza, J D; Moriyama, S; Morrison, E; Morteau, E; Mosbacher, Y; Mount, B J; Mueller, J; Murphy, A St J; Murra, M; Naim, D; Nakamura, S; Nash, E; Navaieelavasani, N; Naylor, A; Nedlik, C; Nelson, H N; Neves, F; Newstead, J L; Ni, K; Nikoleyczik, J A; Niro, V; Oberlack, U G; Obradovic, M; Odgers, K; O'Hare, C A J; Oikonomou, P; Olcina, I; Oliver-Mallory, K; Oranday, A; Orpwood, J; Ostrovskiy, I; Ozaki, K; Paetsch, B; Pal, S; Palacio, J; Palladino, K J; Palmer, J; Panci, P; Pandurovic, M; Parlati, A; Parveen, N; Patton, S J; Pěč, V; Pellegrini, Q; Penning, B; Pereira, G; Peres, R; Perez-Gonzalez, Y; Perry, E; Pershing, T; Petrossian-Byrne, R; Pienaar, J; Piepke, A; Pieramico, G; Pierre, M; Piotter, M; Pizzella, V; Plante, G; Pollmann, T; Porzio, D; Qi, J; Qie, Y; Qin, J; Quevedo, F; Raj, N; Rajado Silva, M; Ramanathan, K; Ramírez García, D; Ravanis, J; Redard-Jacot, L; Redigolo, D; Reichard, S; Reichenbacher, J; Rhyne, C A; Richards, A; Riffard, Q; Rischbieter, G R C; Rocchetti, A; Rosenfeld, S L; Rosero, R; Rupp, N; Rushton, T; Saha, S; Salucci, P; Sanchez, L; Sanchez-Lucas, P; Santone, D; dos Santos, J M F; Sarnoff, I; Sartorelli, G; Sazzad, A B M R; Scheibelhut, M; Schnee, R W; Schrank, M; Schreiner, J; Schulte, P; Schulte, D; Schulze Eissing, H; Schumann, M; Schwemberger, T; Schwenk, A; Schwetz, T; Scotto Lavina, L; Scovell, P R; Sekiya, H; Selvi, M; Semenov, E; Semeria, F; Shagin, P; Shaw, S; Shi, S; Shockley, E; Shutt, T A; Si-Ahmed, R; Silk, J J; Silva, C; Silva, M C; Simgen, H; Šimkovic, F; Sinev, G; Singh, R; Skulski, W; Smirnov, J; Smith, R; Solmaz, M; Solovov, V N; Sorensen, P; Soria, J; Sparmann, T J; Stancu, I; Steidl, M; Stevens, A; Stifter, K; Strigari, L E; Subotic, D; Suerfu, B; Suliga, A M; Sumner, T J; Szabo, P; Szydagis, M; Takeda, A; Takeuchi, Y; Tan, P-L; Taricco, C; Taylor, W C; Temples, D J; Terliuk, A; Terman, P A; Thers, D; Thieme, K; Thümmler, T; Tiedt, D R; Timalsina, M; To, W H; Toennies, F; Tong, Z; Toschi, F; Tovey, D R; Tranter, J; Trask, M; Trinchero, G C; Tripathi, M; Tronstad, D R; Trotta, R; Tsai, Y D; Tunnell, C D; Turner, W G; Ueno, R; Urquijo, P; Utku, U; Vaitkus, A; Valerius, K; Vassilev, E; Vecchi, S; Velan, V; Vetter, S; Vincent, A C; Vittorio, L; Volta, G; von Krosigk, B; von Piechowski, M; Vorkapic, D; Wagner, C E M; Wang, A M; Wang, B; Wang, Y; Wang, W; Wang, J J; Wang, L-T; Wang, M; Wang, Y; Watson, J R; Wei, Y; Weinheimer, C; Weisman, E; Weiss, M; Wenz, D; West, S M; Whitis, T J; Williams, M; Wilson, M J; Winkler, D; Wittweg, C; Wolf, J; Wolf, T; Wolfs, F L H; Woodford, S; Woodward, D; Wright, C J; Wu, V H S; Wu, P; Wüstling, S; Wurm, M; Xia, Q; Xiang, X; Xing, Y; Xu, J; Xu, Z; Xu, D; Yamashita, M; Yamazaki, R; Yan, H; Yang, L; Yang, Y; Ye, J; Yeh, M; Young, I; Yu, H B; Yu, T T; Yuan, L; Zavattini, G; Zerbo, S; Zhang, Y; Zhong, M; Zhou, N; Zhou, X; Zhu, T; Zhu, Y; Zhuang, Y; Zopounidis, J P; Zuber, K; Zupan, J;
• Is Part Of: Journal of physics. Volume 50:Number 1(2023)
• Publication Date: 2023-01-01
• Subjects: dark matter -- neutrinoless double-beta decay -- neutrinos -- supernova -- direct detection -- astroparticle physics -- xenon; Nuclear physics -- Periodicals; Particles (Nuclear physics) -- Periodicals; Physique nucléaire -- Périodiques; Particules (Physique nucléaire) -- Périodiques; Kernfysica; Elementaire deeltjes; 539.7
• DOI: 10.1088/1361-6471/ac841a
• Languages: English
• ISSNs: 0954-3899

Abstract

Abstract: The nature of dark matter and properties of neutrinos are among the most pressing issues in contemporary particle physics. The dual-phase xenon time-projection chamber is the leading technology to cover the available parameter space for weakly interacting massive particles, while featuring extensive sensitivity to many alternative dark matter candidates. These detectors can also study neutrinos through neutrinoless double-beta decay and through a variety of astrophysical sources. A next-generation xenon-based detector will therefore be a true multi-purpose observatory to significantly advance particle physics, nuclear physics, astrophysics, solar physics, and cosmology. This review article presents the science cases for such a detector.