Search for inelastic scattering of WIMP dark matter in XENON1T

被引：22

作者：

Aprile, E. ^{[1
]}

Aalbers, J. ^{[2
]}

Agostini, F. ^{[3
,4
]}

Alfonsi, M. ^{[5
]}

Althueser, L. ^{[6
]}

Amaro, F. D. ^{[7
]}

Andaloro, S. ^{[8
]}

Angelino, E. ^{[9
,10
]}

Angevaare, J. R. ^{[11
,12
]}

Antochi, V. C. ^{[2
]}

Arneodo, F. ^{[13
]}

Baudis, L. ^{[14
]}

Bauermeister, B. ^{[2
]}

Bellagamba, L. ^{[3
,4
]}

Benabderrahmane, M. L. ^{[13
]}

Brown, A. ^{[14
]}

Brown, E. ^{[15
]}

Bruenner, S. ^{[11
,12
]}

Bruno, G. ^{[13
]}

Budnik, R. ^{[16
,39
,40
]}

Capelli, C. ^{[14
]}

Cardoso, J. M. R. ^{[7
]}

Cichon, D. ^{[17
]}

Cimmino, B. ^{[18
,19
]}

Clark, M. ^{[20
]}

Coderre, D. ^{[21
]}

Colijn, A. P. ^{[11
,12
,41
]}

Conrad, J. ^{[2
]}

Cuenca, J. ^{[22
]}

Cussonneau, J. P. ^{[23
]}

Decowski, M. P. ^{[11
,12
]}

Depoian, A. ^{[20
]}

Di Gangi, P. ^{[3
,4
]}

Di Giovanni, A. ^{[13
]}

Di Stefano, R. ^{[18
,19
]}

Diglio, S. ^{[23
]}

Elykov, A. ^{[21
]}

Ferella, A. D. ^{[24
,25
,26
]}

Fulgione, W. ^{[9
,10
,25
,26
]}

Gaemers, P. ^{[11
,12
]}

Gaior, R. ^{[27
]}

Galloway, M. ^{[14
]}

Gao, F. ^{[1
,28
,29
]}

Grandi, L. ^{[30
,31
]}

Hils, C. ^{[5
]}

Hiraide, K. ^{[32
,33
]}

Hoetzsch, L. ^{[17
]}

Howlett, J. ^{[1
]}

Iacovacci, M. ^{[18
,19
]}

Itow, Y. ^{[34
,35
]}

机构：

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

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

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

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

[5] Johannes Gutenberg Univ Mainz, Inst Phys & Exzellenzcluster PRISMA, D-55099 Mainz, Germany

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

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

[8] Rice Univ, Dept Phys & Astron, Houston, TX 77005 USA

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

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

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

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

[13] New York Univ Abu Dhabi, Abu Dhabi, U Arab Emirates

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

[15] Rensselaer Polytech Inst, Dept Phys Appl Phys & Astron, Troy, NY 12180 USA

[16] Weizmann Inst Sci, Dept Particle Phys & Astrophys, IL-7610001 Rehovot, Israel

[17] Max Planck Inst Kernphys, D-69117 Heidelberg, Germany

[18] Univ Napoli, Dept Phys Ettore Pancini, I-80126 Naples, Italy

[19] INFN Napoli, I-80126 Naples, Italy

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

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

[22] Karlsruhe Inst Technol, Inst Astroparticle Phys, D-76021 Karlsruhe, Germany

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

[24] Univ Aquila, Dept Phys & Chem, I-67100 Laquila, Italy

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

[26] Gran Sasso Sci Inst, I-67100 Laquila, Italy

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

[28] Tsinghua Univ, Dept Phys, Beijing 100084, Peoples R China

[29] Tsinghua Univ, Ctr High Energy Phys, Beijing 100084, Peoples R China

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

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

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

[33] Univ Tokyo, Kavli Inst Phys & Math Universe WPI, Hida, Gifu 5061205, Japan

[34] Nagoya Univ, Kobayashi Maskawa Inst Origin Particles & Univers, Chikusa Ku, Furo Cho, Nagoya, Aichi 4648602, Japan

[35] Nagoya Univ, Inst Space Earth Environm Res, Chikusa Ku, Furo Cho, Nagoya, Aichi 4648602, Japan

[36] Univ Calif San Diego, Dept Phys, La Jolla, CA 92093 USA

[37] Univ Paris Saclay, IJCLab, CNRS IN2P3, F-91405 Orsay, France

[38] Kobe Univ, Dept Phys, Kobe, Hyogo 6578501, Japan

[39] SUNY Stony Brook, Simons Ctr Geometry & Phys, Stony Brook, NY 11794 USA

[40] SUNY Stony Brook, CN Yang Inst Theoret Phys, Stony Brook, NY 11794 USA

[41] Univ Utrecht, Inst Subatom Phys, NL-3584 CC Utrecht, Netherlands

[42] Nagoya Univ, Inst Adv Res, Nagoya, Aichi 4648601, Japan

[43] Coimbra Polytech ISEC, P-3030199 Coimbra, Portugal

[44] Univ Ferrara, Sez Ferrara, Ist Nazl Fis Nucl, Via G Saragat 1,Edificio C, I-44122 Ferrara, FE, Italy

[45] Univ Ferrara, Dip Fis & Sci Terra, Via G Saragat 1,Edificio C, I-44122 Ferrara, FE, Italy

来源：

PHYSICAL REVIEW D | 2021年 / 103卷 / 06期

基金：

瑞士国家科学基金会; 欧盟地平线“2020”; 美国国家科学基金会;

关键词：

NUCLEAR-DATA SHEETS; CANDIDATES;

D O I：

10.1103/PhysRevD.103.063028

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We report the results of a search for the inelastic scattering of weakly interacting massive particles (WIMPs) in the XENON1T dark matter experiment. Scattering off Xe-129 is the most sensitive probe of inelastic WIMP interactions, with a signature of a 39.6 keV deexcitation photon detected simultaneously with the nuclear recoil. Using an exposure of 0.83 tonne-years, we find no evidence of inelastic WIMP scattering with a significance of more than 2 sigma. A profile-likelihood ratio analysis is used to set upper limits on the cross section of WIMP-nucleus interactions. We exclude new parameter space for WIMPs heavier than 100 GeV/c(2), with the strongest upper limit of 3.3 x 10(-39) cm(2) for 130 GeV/c(2) WIMPs at 90% confidence level.

引用

页数：10

共 50 条

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不详
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