D. Yu. Akimov, H. M. Araujo, E. J. Barnes, V. A. Belov, A. Bewick, A. A. Burenkov, R. Cashmore, V. Chepel, A. Currie, D. Davidge, J. Dawson, T. Durkin, B. Edwar… 展开作者
D. Yu. Akimov, H. M. Araujo, E. J. Barnes, V. A. Belov, A. Bewick, A. A. Burenkov, R. Cashmore, V. Chepel, A. Currie, D. Davidge, J. Dawson, T. Durkin, B. Edwards, C. Ghag, A. Hollingsworth, M. Horn, A. S. Howard, A. J. Hughes, W. G. Jones, G. E. Kalmus, A. S. Kobyakin, A. G. Kovalenko, V. N. Lebedenko, A. Lindote, I. Liubarsky, M. I. Lopes, R. Luscher, K. Lyons, P. Majewski, A. StJ. Murphy, F. Neves, S. M. Paling, J. Pinto da Cunha, R. Preece, J. J. Quenby, L. Reichhart, P. R. Scovell, C. Silva, V. N. Solovov, N. J. T. Smith, P. F. Smith, V. N. Stekhanov, T. J. Sumner, C. Thorne, L. de Viveiros, R. J. Walker
备注：
4 pages, 5 figures. Updated with 1.17 ton.year DAMA results.
We present limits on the WIMP-nucleon cross section for inelastic dark matter derived from the 2008 run of ZEPLIN-III. Cuts, notably on scintillation pulse shape and scintillation-to-ionisation ratio, give a net exposure of 63 kg.days in the range 20-80keV nuclear recoil energy, in which 6 events are observed. Upper limits on signal rate are derived from the maximum empty patch in the data. Under standard halo assumptions a small region of parameter space consistent, at 99% CL, with causing the 1.17 ton.year DAMA modulation signal is allowed at 90% CL: it is in the mass range 45-60 GeV with a minimum CL of 88%, again derived from the maximum patch. This is the tightest constraint on that explanation of the DAMA result yet presented using a xenon target.
Inelastic Self-interacting Dark Matter and LUX-ZEPLIN 248 keV Event in a Dirac Modular Inverse Seesaw
Salbari College（萨尔巴里学院）；University of Silesia（西里西亚大学）；Indian Institute of Technology Goa（印度理工学院果阿分校）；Indian Institute of Technology Hyderabad（印度理工学院海德拉巴分校）
Kaluza--Klein Dark-Photon Mediation of Inelastic Dark Matter at LUX-ZEPLIN
Center for Fundamental Physics, School of Artificial Intelligence, Hubei Polytechnic University（湖北理工学院人工智能学院基础物理中心）；Physics Department, Theory Division, University of Ioannina（伊奥尼纳大学理论部物理系）
A scalar-extended ${\rm U(1)_{L_μ-L_τ}}$ explanation of the LUX-ZEPLIN 248 keV excess
Institute of Physics（印度物理研究所）；Homi Bhabha National Institute, BARC Training School Complex（霍米·巴巴国立学院，BARC培训学院）；Laboratoire de Physique Subatomique et de Cosmologie, Université Grenoble-Alpes, CNRS/IN2P3（法国格勒诺布尔阿尔卑斯大学亚原子物理与宇宙学实验室）
Interpreting the High-Recoil LUX-ZEPLIN Event with Bino-/Singlino-like and Higgsino Dark Matter
Argonne National Laboratory（阿贡国家实验室）；University of Cincinnati（辛辛那提大学）；Johannes Gutenberg University（约翰内斯·古腾堡大学）；University of Chicago（芝加哥大学）；Perimeter Institute for Theoretical Physics（理论物理珀米特研究所）
Inelastic Dark Matter and High-Energy Recoil Signatures in LZ
Department of Physics, Tsinghua University（清华大学物理系）；Center for High Energy Physics, Peking University（北京大学高能物理中心）；Department of Physics and Jockey Club Institute for Advanced Study, The Hong Kong University of Science and Technology（香港科技大学物理系及赛马会高等研究院）
Inelastic from the Other Side: Xenon Excitation Signals in Light of the LZ High-Recoil Event
Nanjing Normal University（南京师范大学）；Institute of Theoretical Physics, Chinese Academy of Sciences（中国科学院理论物理研究所）；University of Chinese Academy of Sciences（中国科学院大学）；Xinjiang University（新疆大学）
Inelastic Singlet-Doublet Fermion Dark Matter in light of the 248 keV LZ event
Indian Institute of Technology Guwahati（印度理工学院古瓦哈提分校）；Indian Institute of Technology Hyderabad（印度理工学院海德拉巴分校）；Institute of Mathematical Sciences（数学科学研究所）
Search for dark matter particle interactions in an extended nuclear recoil energy window with the LUX-ZEPLIN (LZ) experiment
SLAC National Accelerator Laboratory（斯坦福直线加速器中心）；Kavli Institute for Particle Astrophysics and Cosmology, Stanford University（斯坦福大学卡弗里粒子天体物理与宇宙学研究所）；University College London (UCL)（伦敦大学学院）；Brown University（布朗大学）；University of California, Santa Barbara（加州大学圣塔芭芭拉分校）；Lawrence Berkeley National Laboratory (LBNL)（劳伦斯伯克利国家实验室）；University of Zurich（苏黎世大学）；Imperial College London（帝国理工学院）；STFC Rutherford Appleton Laboratory (RAL)（英国科学与技术设施委员会卢瑟福阿普尔顿实验室）；University of Maryland（马里兰大学）；King’s College London（伦敦国王学院）
Inelastic Dark Matter at LZ from Radiative Dirac Neutrino Mass Paradigm
Indian Institute of Technology Guwahati（印度理工学院古瓦哈提分校）；Indian Institute of Technology Goa（印度理工学院果阿分校）；Indian Institute of Technology (BHU)（印度理工学院（贝拿勒斯印度教大学））
High-Energy Nuclear Recoils from Boosted Dark Matter for the LZ 248-keV Event: Beyond the Halo-Dependent High-Velocity Tail
Jazan University（扎赞大学）；University of South Dakota（南达科他大学）；University of Kansas（堪萨斯大学）；Chungnam National University（忠南国立大学）；Jeonbuk National University（全北国立大学）；Korea Institute for Advanced Study（韩国高等研究院）；Institute for Basic Science（基础科学研究院）
Projected Sensitivity of Paleo-Detectors to Dark Matter Effective Interactions with Nuclei
The University of Texas at Austin（德克萨斯大学奥斯汀分校）；Stockholm University（斯德哥尔摩大学）；KTH Royal Institute of Technology（皇家理工学院）；University of North Florida（北佛罗里达大学）；Jožef Stefan Institute（约瑟夫·斯蒂芬研究所）
