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A next-generation liquid xenon observatory for dark matter and neutrino physics
J. Aalbers, Shehu AbdusSalam, K. Abe, Valentino Aerne, F. Agostini, S. Ahmed Maouloud, D. S. Akerib, D. Akimov, J Akshat, A. K. Al Musalhi, F. Alder, S. Alsum, L. Althueser, C. S. Amarasinghe, F. D. Amaro, A. Ames, Tyler Anderson, B. Andrieu, N. Angelides, E. Angelino, J. R. Angevaare, V. C. Antochi, D. Antón Martin, B. Antunović, E. Aprile, H. M. Araújo, J. E. Armstrong, F. Arneodo, M. Arthurs, Pouya Asadi, Seungwon Baek, X. Bai, D. Bajpai, Alexander A. Baker, J. Balajthy, S. Balashov, M. Balzer, A. Bandyopadhyay, J. Bang, E. L. Barberio, J. W. Bargemann, L. Baudis, D. Bauer, D. Baur, A. Baxter, M. Bazyk, K. Beattie, J. Behrens, Nicole F. Bell, L. Bellagamba, P. Beltrame, M. L. Benabderrahmane, E. P. Bernard, Gianfranco Bertone, Pijushpani Bhattacharjee, A. Bhatti, A. Biekert, T. P. Biesiadzinski, A R Binau, R. Biondi, Y. Biondi, H. J. Birch, Fady Bishara, A. Bismark, Carlos Blanco, G. M. Blockinger, E. Bodnia, A. Bolozdynya, Patrick D. Bolton, Salvatore Bottaro, C. Bourgeois, B. Boxer, P. Brás, A. Breskin, P. A. Breur, C. Brew, Joachim Brod, E. J. Brookes, A. Brown, S. Bruenner, G. Bruno, R. Budnik, S. Burdin, S Buse, J.K. Busenitz, Dario Buttazzo, M. Buuck, A. Buzulutskov, R. Cabrita, Ce Cai, Dingbang Cai, C. Capelli, J. M. R. Cardoso, M. C. Carmona-Benitez, M. Cascella, Riccardo Catena, Sabyasachi Chakraborty, C. Chan, Spencer Chang, A. Chauvin, A. Chawla, H. Chen, V. Chepel, N. Chott, D. Cichon, A Cimental Chavez, B. Cimmino, M. Clark, Raymond T. Co, A. P. Colijn, J. M. Conrad, M. V. Converse, Marco Costa, A. Cottle, G. A. Cox, Oisín Creaner, J J Cuenca Garcia, J. P. Cussonneau, J. E. Cutter, C. E. Dahl, V. D’Andrea, A. David, M. P. Decowski, James B. Dent, Frank F. Deppisch, L. de Viveiros, P. Di Gangi, A. Di Giovanni, S. Di Pede, J. Dierle, S. Diglio, J. E. Y. Dobson, M Doerenkamp, Delphine Douillet, G. Drexlin, E. Druszkiewicz, David I. Dunsky, K. Eitel, A. Elykov, Timón Emken, R. Engel, S. R. Eriksen, Malcolm Fairbairn, A. Fan, JiJi Fan, S. Farrell, Simon Fayer, N. M. Fearon, A. D. Ferella, C. Ferrari, A. Fieguth, S. Fiorucci, H. Fischer, H. Flaecher, M. Flierman, Tess Florek, R. Foot, P. J. Fox, Roberto Franceschini, E. D. Fraser, Carlos S. Frenk, Steffen Fröhlich, T. Fruth, W. Fulgione, C. Fuselli, P. Gaemers, R. Gaïor, R. J. Gaitskell, M. Galloway, F. Gao, J. Genovesi, C. Ghag, S. Ghosh, E. F. Gibson, W Gil, D. Giovagnoli, F. Girard, R. Glade-Beucke, F. Glück, S. Gokhale, A. de Gouvêa, Lukas Graf, L. Grandi, J. Grigat, Benjamı́n Grinstein, M. G. D. van der Grinten, R. Grössle, H. Guan, M. Guida, R Gumbsheimer, C. B. Gwilliam, C. Hall, L. J. Hall, R. Hammann, K. Han, V. Hannen, S. Hansmann-Menzemer, R Harata, S P Hardin, Edward Hardy, C. A. Hardy, Keisuke Harigaya, Roni Harnik, S. J. Haselschwardt, S. A. Hertel, A. Higuera, C. Hils, S. Hochrein, L. Hoetzsch, Martin Hoferichter, Nicky Hood, D Hooper, M. Horn, J. Howlett, D. Q. Huang, Yuping Huang, Donald F. Hunt, M. Iacovacci, G. Iaquaniello, Ryushin Ide, C. M. Ignarra, G Iloglu, Y. Itow, E. Jacquet, O. Jahangir, J. Jakob, R. S. James, A. Jansen, W. Ji, X Ji, F. Joerg, J. Johnson, A. Joy, A. C. Kaboth, Leila Kalhor, A. Kamaha, K Kanezaki, Kamales Kar, M. Kara, Natsuko Kato, P. Kavrigin, S. Kazama, A W Keaveney, J. Kellerer, D. Khaitan, A. Khazov, G. Khundzakishvili, I. Khurana, B. Kilminster, M. Kleifges, Pyungwon Ko, M. Kobayashi, D. Kodroff, G. Koltmann, A. Kopec, A. Kopmann, Joachim Kopp, L. Korley, В. Н. Корноухов, E. V. Korolkova, H. Kraus, Lawrence M. Krauss, S. Kravitz, L. Kreczko, V. A. Kudryavtsev, F. Kuger, Jason Kumar, B. López Paredes, L. LaCascio, R. Laha, Quentin Lainé, H. Landsman, R. F. Lang, E. Leason, J. Lee, D. S. Leonard, K. T. Lesko, L. J. Levinson, C. Levy, I. Li, S. Li, T. Li, S. Liang, C. S. Liebenthal, J. Lin, Q. Lin, S. Lindemann, M. Lindner, A. Lindote, R. Linehan, W. H. Lippincott, Xiang Liu, K. Liu, Jun Liu, J. Loizeau, F. Lombardi, J. Long, I. Lopes, E. Lopez Asamar, W. Lorenzon, Chih-Ting Lu, S. Luitz, Y. Ma, P. Machado, C. Macolino, T. Maeda, J. Mahlstedt, P. A. Majewski, A. Manalaysay, A. Mancuso, L. Manenti, A. Manfredini, R. L. Mannino, N. Marangou, John March-Russell, F Marignetti, T. Marrodán Undagoitia, K. Martens, R. Martin, I Martinez-Soler, J. Masbou, D. Masson, E. Masson, S. Mastroianni, M Mastronardi, J. A. M. Lopes, M. E. McCarthy, Nathalie McFadden, Emma McGinness, D. N. McKinsey, K. McMichael, P. Meinhardt, J. Menéndez, Yue Meng, M. Messina, Rajiv Midha, D. Milisavljević, EJ Miller, B Milosevic, S. Milutinovic, S. Mitra, K. Miuchi, E. Mizrachi, K. Mizukoshi, A. Molinario, A. Monte, C. M. B. Monteiro, M. E. Monzani, J. Steven Moore, K. Morå, J. A. Morad, J. D. Morales Mendoza, S. Moriyama, E. Morrison, E. Morteau, Y. Mosbacher, B. J. Mount, J. Mueller, A. St. J. Murphy, M. Murra, D. Naim, Shunsuke Nakamura, E.F. Nash, N Navaieelavasani, A. Naylor, C. Nedlik, H. N. Nelson, F. Neves, Jayden L. Newstead, K. Ni, J. A. Nikoleyczik, Viviana Niro, U. Oberlack, M Obradović, K. Odgers, C O'Hare, Panagiotis Oikonomou, I. Olcina, K. C. Oliver-Mallory, A Oranday, J. Orpwood, I. Ostrovskiy, K. Ozaki, B. Paetsch, S. K. Pal, J. Palacio, K. J. Palladino, J. D. Palmer, Paolo Panci, M. Pandurović, A Parlati, N. Parveen, Simon Patton, V. Pec, Q. Pellegrini, B. Penning, G Pereira, R Peres, Yuber F. Perez-Gonzalez, E Perry, T. Pershing, Rudin Petrossian-Byrne, J. Pienaar, A. Piepke, G. Pieramico, M. Pierre, M. Piotter, V. Pizzella, G. Plante, T. R. Pollmann, D. Porzio, Jing-Zhao Qi, Y. Qie, J. Qin, F. Quevedo, Nirmal Raj, Mariana Rajado Silva, K Ramanathan, D. Ramírez García, Julia Ravanis, L Redard-Jacot, Diego Redigolo, S. Reichard, J. Reichenbacher, C. A. Rhyne, A. Richards, Q. Riffard, G. R. C. Rischbieter, A. Rocchetti, S L Rosenfeld, R. Rosero, N. Rupp, T. Rushton, S. Saha, P Salucci, L Sanchez, P. Sánchez-Lucas, D. Santone, J.M.F. dos Santos, I. Sarnoff, G. Sartorelli, A. B. M. R. Sazzad, M Scheibelhut, R. W. Schnee, M. Schrank, J. Schreiner, P. Schulte, D Schulte, H. Schulze Eißing, M. Schümann, T Schwemberger, A. Schwenk, Thomas Schwetz, L. Scotto Lavina, P. R. Scovell, H. Sekiya, M. Selvi, Е. В. Семенов, F. Semeria, P. Shagin, S. Shaw, S. Shi, E. Shockley, T. Shutt, R Si-Ahmed, J. J. Silk, C. Silva, Maria Clara da Rocha dos Santos Silva, H. Simgen, F. Šimkovic, G. Sinev, R. Singh, W. Skulski, Juri Smirnov, R. J. E. Smith, M. Solmaz, V. N. Solovov, P. Sørensen, J. Soria, Tobias Sparmann, I. Stancu, M. Steidl, A. Stevens, K. Stifter, Louis E. Strigari, Dragan Subotic, B. Suerfu, Anna M. Suliga, T. J. Sumner, P Szabo, M. Szydagis, A. Takeda, Y. Takeuchi, P.-L. Tan, Carla Taricco, WC Taylor, D. J. Temples, A. Terliuk, P. A. Terman, D. Thers, K. Thieme, T. Thümmler, D. R. Tiedt, M. Timalsina, W. To, F. Toennies, Z Tong, F. Toschi, D. R. Tovey, Jemima Tranter, M. Trask, G. Trinchero, M. Tripathi, D. R. Tronstad, Roberto Trotta, Y D Tsai, C D Tunnell, W. Turner, R. Ueno, P. Urquijo, U. Utku, A. Vaitkus, K Valerius, Mirella Dimitrova Vassilev, S. Vecchi, V. Velan, S Vetter, Angela Vincent, Ludovico Vittorio, G Volta, B. von Krosigk, M von Piechowski, D. Vorkapic, Carlos E. M. Wagner, Ann Miao Wang, B Wang, Y. Wang, Xiang-Gao Wang, J J Wang, L-T Wang, Meng Wang, Ye Wang, Jean Watson, Y. Wei, C. Weinheimer, Evan Weisman, M. Weiss, D. Wenz, Stephen M. West, T. J. Whitis, M. Williams, M J Wilson, D. Winkler, C. Wittweg, J. Wolf, T. M. H. Wolf, F. L. H. Wolfs, S. Woodford, D. Woodward, Chris J. Wright, V. H. S. Wu, P Wu, S. Wüstling, M. Wurm, Q. Xia, X. Xiang, Y. Xing, Jing Xu, Z. Xu, Dong Xu, M. Yamashita, Ryo Yamazaki, Hu Yan, Lili Yang, Yong Yang, Ye J, M. Yeh, Ian T. Young, Hai-Bo Yu, Tingfeng Yu, L. Yuan, G. Zavattini, S. Zerbo, Y. Zhang, M Zhong, N. Zhou, Xiaopeng Zhou, Tong Zhu, Y. Zhu, Yuan Zhuang, J. P. Zopounidis, K. Zuber, Jure Zupan
Bibliographic record
VenueJournal of Physics G Nuclear and Particle Physics · 2022
Typearticle
Languageen
FieldPhysics and Astronomy
TopicDark Matter and Cosmic Phenomena
Canadian institutionsQueen's UniversityTRIUMF
FundersDivision of PhysicsFundação para a Ciência e a TecnologiaOffice of ScienceInstitute for Basic ScienceNederlandse Organisatie voor Wetenschappelijk OnderzoekDeutsche ForschungsgemeinschaftScience and Technology Facilities CouncilUniversity College LondonNational Research FoundationUniversity of EdinburghU.S. Department of EnergyEuropean CommissionNational Science FoundationImperial College LondonNational Research Foundation of KoreaSchweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung
KeywordsPhysicsDark matterNeutrinoXenonTime projection chamberObservatoryParticle physicsCosmologyAstroparticle physicsSolar neutrinoParticle identificationWeakly interacting massive particlesNeutrino detectorPhysics beyond the Standard ModelDetectorSolar neutrino problemAstrophysicsNuclear physicsAstronomyNeutrino oscillationDark energyScalar field dark matterElectron
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.
Fetched live from OpenAlex and de-inverted. Abstracts are not stored in this database: the inverted indexes are 8.6 GB of the frame’s 9.3 GB of text, and the host has 13 GB free.
How this classification was reachedexpand
Full frame machine prediction
Teacher imitationNot calibrated prevalence, not ground truth. Human validation pending. The Gemma side is a direct model label for every work in the frame, read from the title-only record. The Codex side is a classifier learned from the 10,348 direct Codex labels and calibrated to design-weighted sample rates; fields without enough sample support carry no Codex call. Candidate is the union of the two sides; consensus is their intersection. These outputs are machine_predicted_unvalidated and are not human labels.
metaresearch head score (Codex)0.001
metaresearch head score (Gemma)0.000
Version: metacan-v3-hybrid-931329e0061cValidation status: machine_predicted_unvalidated
Candidate categoriesnone
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Bench or experimental · Consensus signal: none
GenreCandidate signal: Empirical · Consensus signal: none
Teacher disagreement score0.005
Threshold uncertainty score0.015
Distilled classifier scores by category (both heads)
| Category | Codex | Gemma |
|---|---|---|
| Metaresearch | 0.001 | 0.000 |
| Meta-epidemiology (narrow) | 0.000 | 0.000 |
| Meta-epidemiology (broad) | 0.000 | 0.000 |
| Bibliometrics | 0.001 | 0.001 |
| Science and technology studies | 0.001 | 0.001 |
| Scholarly communication | 0.001 | 0.002 |
| Open science | 0.001 | 0.002 |
| Research integrity | 0.001 | 0.001 |
| Insufficient payload (model declined to judge) | 0.005 | 0.001 |
Machine scores (provisional)
The two teacher heads of the student model, read on this work. A score orders the frame for review; it never asserts a category, and the validation status ships verbatim with every row.
Baseline scores from an immature model (maturity gate not passed, 7 training rounds). Scores rank; they never assert a category.
Opus teacher head0.038
GPT teacher head0.241
Teacher spread0.203 · how far apart the two teachers sit on this one work
Validation status
score_only:v0-immature-baseline · verbatim from the scoring run: score_only means the number may rank works, and no category label ships from itClassification
machine, unvalidatedMachine predicted; a candidate call from one source (direct Gemma or distilled Codex), not a consensus.
The models applied no category: nothing in the taxonomy fit this work.
Study designBench or experimental
Domainnot available
GenreEmpirical
How this classification was reached, model by model and score by score, is at the end of the page under "How this classification was reached".
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Citations155
Published2022
Admission routes1
Has abstractyes