Effective field theory and inelastic dark matter results from XENON1T

被引:0
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作者
Aprile, E. [1 ]
Abe, K. [2 ,3 ]
Agostini, F. [4 ,5 ]
Maouloud, S. Ahmed [6 ]
Althueser, L. [7 ]
Andrieu, B. [6 ]
Angelino, E. [8 ,9 ]
Angevaare, J. R. [10 ,11 ]
Antochi, V. C. [12 ]
Martin, D. Anton [13 ,14 ]
Arneodo, F. [15 ]
Baudis, L. [16 ]
Baxter, A. L. [17 ]
Bellagamba, L. [4 ,5 ]
Biondi, R. [18 ,19 ]
Bismark, A. [16 ]
Brown, A. [20 ]
Bruenner, S. [10 ,11 ]
Bruno, G. [21 ]
Budnik, R. [22 ]
Cai, C. [23 ,24 ]
Capelli, C. [16 ]
Cardoso, J. M. R. [25 ]
Cichon, D. [26 ]
Clark, M. [17 ]
Colijn, A. P. [10 ,11 ]
Conrad, J. [12 ]
Cuenca-Garcia, J. J. [16 ,27 ]
Cussonneau, J. P. [21 ]
D'Andrea, V. [18 ,19 ,28 ]
Decowski, M. P. [10 ,11 ]
Di Gangi, P. [4 ,5 ]
Di Pede, S. [10 ,11 ]
Di Giovanni, A. [15 ]
Di Stefano, R. [29 ,30 ]
Diglio, S. [21 ]
Eitel, K. [27 ]
Elykov, A. [20 ]
Farrell, S. [31 ]
Ferella, A. D. [18 ,19 ,28 ]
Fischer, H. [20 ]
Fulgione, W. [8 ,9 ,18 ,19 ]
Gaemers, P. [10 ,11 ]
Gaior, R. [6 ]
Rosso, A. Gallo [12 ]
Galloway, M. [16 ]
Gao, F. [23 ,24 ]
Glade-Beucke, R. [20 ]
Grandi, L. [13 ,14 ]
Grigat, J. [20 ]
机构
[1] Columbia Univ, Dept Phys, New York, NY 10027 USA
[2] Univ Tokyo, Inst Cosm Ray Res, Kamioka Observ, Higashi Mozumi, Hida, Gifu 5061205, Japan
[3] Univ Tokyo, Kavli Inst Phys & Math Universe WPI, Higashi Mozumi, Hida, Gifu 5061205, Japan
[4] Univ Bologna, Dept Phys & Astron, I-40126 Bologna, Italy
[5] INFN Bologna, I-40126 Bologna, Italy
[6] Sorbonne Univ, CNRS, IN2P3, LPNHE, F-75005 Paris, France
[7] Westfal Wilhelms Univ Munster, Inst Kernphys, D-48149 Munster, Germany
[8] Univ Torino, Dept Phys, INAF Astrophys Observ Torino, I-10125 Turin, Italy
[9] INFN Torino, I-10125 Turin, Italy
[10] Nikhef, Sci Pk, NL-1098 XG Amsterdam, Netherlands
[11] Univ Amsterdam, Sci Pk, NL-1098 XG Amsterdam, Netherlands
[12] Stockholm Univ, Dept Phys, Oskar Klein Ctr, AlbaNova, SE-10691 Stockholm, Sweden
[13] Univ Chicago, Dept Phys, Chicago, IL 60637 USA
[14] Univ Chicago, Kavli Inst Cosmol Phys, Chicago, IL 60637 USA
[15] New York Univ Abu Dhabi, Ctr Astro Particle & Planetary Phys, Abu Dhabi, U Arab Emirates
[16] Univ Zurich, Phys Inst, CH-8057 Zurich, Switzerland
[17] Purdue Univ, Dept Phys & Astron, West Lafayette, PA 47907 USA
[18] INFN, Lab Nazl Gran Sasso, I-67100 Laquila, Italy
[19] Gran Sasso Sci Inst, I-67100 Laquila, Italy
[20] Univ Freiburg, Phys Inst, D-79104 Freiburg, Germany
[21] Nantes Univ, CNRS, IN2P3, SUBATECH,IMT Atlantique, F-44307 Nantes, France
[22] Weizmann Inst Sci, Dept Particle Phys & Astrophys, IL-7610001 Rehovot, Israel
[23] Tsinghua Univ, Dept Phys, Beijing 100084, Peoples R China
[24] Tsinghua Univ, Ctr High Energy Phys, Beijing 100084, Peoples R China
[25] Univ Coimbra, Dept Phys, LIBPhys, P-3004516 Coimbra, Portugal
[26] Max Planck Inst Kernphys, D-69117 Heidelberg, Germany
[27] Karlsruhe Inst Technol, Inst Astroparticle Phys, D-76021 Karlsruhe, Germany
[28] Univ LAquila, Dept Phys & Chem, I-67100 Laquila, Italy
[29] Univ Napoli, Dept Phys Ettore Pancini, I-80126 Naples, Italy
[30] INFN Napoli, I-80126 Naples, Italy
[31] Rice Univ, Dept Phys & Astron, Houston, TX 77005 USA
[32] Johannes Gutenberg Univ Mainz, Inst Phys & Exzellenzcluster PRISMA, D-55099 Mainz, Germany
[33] Nagoya Univ, Kobayashi Maskawa Inst Origin Particles & Univers, Furo-Cho,Chikusa-Ku, Nagoya, Aichi 4648602, Japan
[34] Nagoya Univ, Inst Space Earth Environm Res, Furo-Cho,Chikusa-Ku, Nagoya, Aichi 4648602, Japan
[35] Univ Calif San Diego, Dept Phys, La Jolla, CA 92093 USA
[36] Kobe Univ, Dept Phys, Kobe, Hyogo 6578501, Japan
[37] Coimbra Polytech, ISEC, P-3030199 Coimbra, Portugal
[38] Heidelberg Univ, Phys Inst, Heidelberg, Germany
[39] INFN, Sez Ferrara, I-44122 Ferrara, FE, Italy
[40] Univ Ferrara, Dipartimento Fis & Sci Terra, Via Giuseppe Saragat 1,Edificio C, I-44122 Ferrara, FE, Italy
基金
荷兰研究理事会; 欧盟地平线“2020”; 瑞士国家科学基金会; 美国国家科学基金会;
关键词
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中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
In this work, we expand on the XENON1T nuclear recoil searches to study the individual signals of dark matter interactions from operators up to dimension eight in a chiral effective field theory (ChEFT) and a model of inelastic dark matter (iDM). We analyze data from two science runs of the XENON1T detector totaling 1 t x yr exposure. For these analyses, we extended the region of interest from [4.9, 40.9] keV(NR) to [4.9, 54.4] keV(NR) to enhance our sensitivity for signals that peak at nonzero energies. We show that the data are consistent with the background-only hypothesis, with a small background overfluctuation observed peaking between 20 and 50 keV(NR), resulting in a maximum local discovery significance of 1.7 sigma for the Vector circle times Vector(strange) ChEFT channel for a dark matter particle of 70 GeV/c(2) and 1.8 sigma for an iDM particle of 50 GeV/c(2) with a mass splitting of 100 keV/c(2). For each model, we report 90% confidence level upper limits. We also report upper limits on three benchmark models of dark matter interaction using ChEFT where we investigate the effect of isospin-breaking interactions. We observe rate-driven cancellations in regions of the isospin-breaking couplings, leading to up to 6 orders of magnitude weaker upper limits with respect to the isospin-conserving case.
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页数:17
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