A next-generation liquid xenon observatory for dark matter and neutrino physics

被引：83

作者：

Aalbers, J. ^{[1
,2
]}

AbdusSalam, S. S. ^{[3
]}

Abe, K. ^{[4
,5
]}

Aerne, V ^{[6
]}

Agostini, F. ^{[7
,8
]}

Maouloud, S. Ahmed ^{[9
]}

Akerib, D. S. ^{[1
,2
]}

Akimov, D. Y. ^{[10
]}

Akshat, J. ^{[11
]}

Al Musalhi, A. K. ^{[12
]}

Alder, F. ^{[13
]}

Alsum, S. K. ^{[14
]}

Althueser, L. ^{[15
]}

Amarasinghe, C. S. ^{[16
]}

Amaro, F. D. ^{[17
]}

Ames, A. ^{[1
,2
]}

Anderson, T. J. ^{[1
,2
]}

Andrieu, B. ^{[9
]}

Angelides, N. ^{[18
]}

Angelino, E. ^{[19
,20
]}

Angevaare, J. ^{[21
,22
]}

Antochi, V. C. ^{[23
]}

Martin, D. Anton ^{[24
,25
]}

Antunovic, B. ^{[26
,27
]}

Aprile, E. ^{[28
]}

Araujo, H. M. ^{[18
]}

Armstrong, J. E. ^{[29
]}

Arneodo, F. ^{[30
]}

Arthurs, M. ^{[16
]}

Asadi, P. ^{[31
]}

Baek, S. ^{[32
]}

Bai, X. ^{[33
]}

Bajpai, D. ^{[34
]}

Baker, A. ^{[18
]}

Balajthy, J. ^{[35
]}

Balashov, S. ^{[36
]}

Balzer, M. ^{[37
]}

Bandyopadhyay, A. ^{[38
]}

Bang, J. ^{[39
]}

Barberio, E. ^{[40
]}

Bargemann, J. W. ^{[41
]}

Baudis, L. ^{[6
]}

Bauer, D. ^{[18
]}

Baur, D. ^{[42
]}

Baxter, A. ^{[43
]}

Baxter, A. L. ^{[11
]}

Bazyk, M. ^{[44
]}

Beattie, K. ^{[45
]}

Behrens, J. ^{[46
]}

Bell, N. F. ^{[40
]}

机构：

[1] SLAC Natl Accelerator Lab, Menlo Pk, CA 94025 USA

[2] Stanford Univ, Kavli Inst Particle Astrophys & Cosmol, Stanford, CA 94305 USA

[3] Shahid Beheshti Univ, Dept Phys, Tehran, Iran

[4] Univ Tokyo, Inst Cosm Ray Res, Kamioka Observ, Hida, Gifu 5061205, Japan

[5] Univ Tokyo, Kavli Inst Phys & Math Universe WPI, Kashiwa, Chiba 2778582, Japan

[6] Univ Zurich, Phys Inst, CH-8057 Zurich, Switzerland

[7] Univ Bologna, Dept Phys & Astron, I-40126 Bologna, Italy

[8] INFN Bologna, I-40126 Bologna, Italy

[9] Sorbonne Univ, LPNHE, CNRS IN2P3, F-75005 Paris, France

[10] Natl Res Nucl Univ, MEPhI Moscow Engn Phys Inst, Moscow 115409, Russia

[11] Purdue Univ, Dept Phys & Astron, W Lafayette, IN 47907 USA

[12] Univ Oxford, Dept Phys, Keble Rd, Oxford OX1 3RH, England

[13] UCL, Dept Phys & Astron, London WC1E 6BT, England

[14] Univ Wisconsin, Dept Phys, Madison, WI 53706 USA

[15] Westfalische Wilhelms Univ Munster, Inst Kernphys, D-48149 Munster, Germany

[16] Univ Michigan, Randall Lab Phys, Ann Arbor, MI 48109 USA

[17] Univ Coimbra, Dept Phys, LIBPhys, P-3004516 Coimbra, Portugal

[18] Imperial Coll London, Dept Phys, Blackett Lab, London, England

[19] Univ Torino, Dept Phys, INAF Astrophys Observ Torino, I-10125 Turin, Italy

[20] INFN Torino, I-10125 Turin, Italy

[21] Nikhef, Sci Pk, NL-1098 XG Amsterdam, Netherlands

[22] Univ Amsterdam, Sci Pk, NL-1098 XG Amsterdam, Netherlands

[23] Stockholm Univ, Oskar Klein Ctr, Dept Phys, AlbaNova, SE-10691 Stockholm, Sweden

[24] Univ Chicago, Dept Phys, Chicago, IL 60637 USA

[25] Univ Chicago, Kavli Inst Cosmol Phys, Chicago, IL 60637 USA

[26] Univ Belgrade, Vinca Inst Nucl Sci, Mihajla Petrov Alasa 12-14, Belgrade, Serbia

[27] Univ Banja Luka, Fac Architecture, Bulevar Vojvode Petra Bojovica 1a, Banja Luka 78000, Bosnia & Herceg

[28] Columbia Univ, Phys Dept, New York, NY 10027 USA

[29] Univ Maryland, Dept Phys, College Pk, MD 20742 USA

[30] New York Univ Abu Dhabi, Div Sci, Abu Dhabi, U Arab Emirates

[31] MIT, Ctr Theoret Phys, Cambridge, MA 02139 USA

[32] Korea Univ, Dept Phys, Anam Ro 145, Seoul 02841, South Korea

[33] South Dakota Sch Mines & Technol, Rapid City, SD 57701 USA

[34] Univ Alabama, Dept Phys & Astron, Tuscaloosa, AL 34587 USA

[35] Univ Calif Davis, Dept Phys, One Shields Ave, Davis, CA 95616 USA

[36] STFC Rutherford Appleton Lab RAL, Didcot OX11 0QX, Oxon, England

[37] Karlsruhe Inst Technol, Inst Data Proc & Elect, Karlsruhe, Germany

[38] Ramakrishna Mission Vivekananda Educ & Res Inst, Belur Math 711202, Howrah, India

[39] Brown Univ, Dept Phys, 182 Hope St, Providence, RI 02912 USA

[40] Univ Melbourne, ARC Ctr Excellence Dark Matter Particle Phys, Sch Phys, Melbourne, Vic 3010, Australia

[41] Univ Calif Santa Barbara, Dept Phys, Santa Barbara, CA 93106 USA

[42] Univ Freiburg, Phys Inst, D-79104 Freiburg, Germany

[43] Univ Liverpool, Dept Phys, Liverpool L69 7ZE, Merseyside, England

[44] Univ Nantes, IMT Atlantique, SUBATECH, CNRS IN2P3, F-44307 Nantes, France

[45] Lawrence Berkeley Natl Lab, Berkeley, CA 94720 USA

[46] Karlsruhe Inst Technol, Inst Astroparticle Phys, Karlsruhe, Germany

[47] Vatican Observ, V-00120 Vatican City, Vatican

[48] Univ Calif Berkeley, Dept Phys, Berkeley, CA 94720 USA

[49] HBNI, Saha Inst Nucl Phys, 1-AF Bidhannagar, Kolkata 700064, India

[50] Ist Nazl Fis Nucl, Lab Nazl Gran Sasso, I-67100 Laquila, Italy

来源：

JOURNAL OF PHYSICS G-NUCLEAR AND PARTICLE PHYSICS | 2023年 / 50卷 / 01期

基金：

欧洲研究理事会; 澳大利亚研究理事会; 荷兰研究理事会; 新加坡国家研究基金会; 瑞典研究理事会; 瑞士国家科学基金会; 美国国家科学基金会;

关键词：

dark matter; neutrinoless double-beta decay; neutrinos; supernova; direct detection; astroparticle physics; xenon; DOUBLE-BETA-DECAY; DUAL-PHASE XENON; HALF-LIFE VALUES; ANNUAL MODULATION; IONIZATION YIELD; SOLAR NEUTRINOS; ELECTROMAGNETIC-INTERACTIONS; CRYOGENIC DISTILLATION; CHROMATOGRAPHIC SYSTEM; MILLICHARGED PARTICLES;

D O I：

10.1088/1361-6471/ac841a

中图分类号：

O57 [原子核物理学、高能物理学];

学科分类号：

070202 ;

摘要：

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.

引用

页数：115

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