Search for Cosmic-ray Boosted Sub-GeV Dark Matter using Recoil Protons at Super-Kamiokande
Kamiokande Collaboration, K. Abe, Y. Hayato, K. Hiraide, K. Ieki, M. Ikeda, J. Kameda, Y. Kanemura, R. Kaneshima, Y. Kashiwagi, Y. Kataoka, S. Miki, S. Mine, M.… 展开作者
Kamiokande Collaboration, K. Abe, Y. Hayato, K. Hiraide, K. Ieki, M. Ikeda, J. Kameda, Y. Kanemura, R. Kaneshima, Y. Kashiwagi, Y. Kataoka, S. Miki, S. Mine, M. Miura, S. Moriyama, Y. Nakano, M. Nakahata, S. Nakayama, Y. Noguchi, K. Okamoto, K. Sato, H. Sekiya, H. Shiba, K. Shimizu, M. Shiozawa, Y. Sonoda, Y. Suzuki, A. Takeda, Y. Takemoto, A. Takenaka, H. Tanaka, S. Watanabe, T. Yano, S. Han, T. Kajita, K. Okumura, T. Tashiro, T. Tomiya, X. Wang, J. Xia, S. Yoshida, G. D. Megias, P. Fernandez, L. Labarga, N. Ospina, B. Zaldivar, B. W. Pointon, E. Kearns, J. L. Raaf, L. Wan, T. Wester, J. Bian, N. J. Griskevich, W. R. Kropp, S. Locke, M. B. Smy, H. W. Sobel, V. Takhistov, A. Yankelevich, J. Hill, R. G. Park, B. Bodur, K. Scholberg, C. W. Walter, L. Bernard, A. Coffani, O. Drapier, S. El Hedri, A. Giampaolo, Th. A. Mueller, A. D. Santos, P. Paganini, B. Quilain, T. Ishizuka, T. Nakamura, J. S. Jang, J. G. Learned, K. Choi, S. Cao, L. H. V. Anthony, D. Martin, M. Scott, A. A. Sztuc, Y. Uchida, V. Berardi, M. G. Catanesi, E. Radicioni, N. F. Calabria, L. N. Machado, G. De Rosa, G. Collazuol, F. Iacob, M. Lamoureux, M. Mattiazzi, L. Ludovici, M. Gonin, G. Pronost, C. Fujisawa, Y. Maekawa, Y. Nishimura, M. Friend, T. Hasegawa, T. Ishida, T. Kobayashi, M. Jakkapu, T. Matsubara, T. Nakadaira, K. Nakamura, Y. Oyama, K. Sakashita, T. Sekiguchi, T. Tsukamoto, T. Boschi, F. Di Lodovico, J. Gao, A. Goldsack, T. Katori, J. Migenda, M. Taani, S. Zsoldos, Y. Kotsar, H. Ozaki, A. T. Suzuki, Y. Takeuchi, C. Bronner, J. Feng, T. Kikawa, M. Mori, T. Nakaya, R. A. Wendell, K. Yasutome, S. J. Jenkins, N. McCauley, P. Mehta, K. M. Tsui, Y. Fukuda, Y. Itow, H. Menjo, K. Ninomiya, J. Lagoda, S. M. Lakshmi, M. Mandal, P. Mijakowski, Y. S. Prabhu, J. Zalipska, M. Jia, J. Jiang, C. K. Jung, M. J. Wilking, C. Yanagisawa, M. Harada, H. Ishino, S. Ito, H. Kitagawa, Y. Koshio, F. Nakanishi, S. Sakai, G. Barr, D. Barrow, L. Cook, S. Samani, D. Wark, F. Nova, J. Y. Yang, M. Malek, J. M. McElwee, O. Stone, M. D. Thiesse, L. F. Thompson, H. Okazawa, S. B. Kim, J. W. Seo, I. Yu, A. K. Ichikawa, K. D. Nakamura, S. Tairafune, K. Nishijima, K. Iwamoto, K. Nakagiri, Y. Nakajima, N. Taniuchi, M. Yokoyama, K. Martens, P. de Perio, M. R. Vagins, M. Kuze, S. Izumiyama, M. Inomoto, M. Ishitsuka, H. Ito, T. Kinoshita, R. Matsumoto, Y. Ommura, N. Shigeta, M. Shinoki, T. Suganuma, K. Yamauchi, J. F. Martin, H. A. Tanaka, T. Towstego, R. Akutsu, V. Gousy-Leblanc, M. Hartz, A. Konaka, N. W. Prouse, S. Chen, B. D. Xu, B. Zhang, M. Posiadala-Zezula, D. Hadley, M. Nicholson, M. O'Flaherty, B. Richards, A. Ali, B. Jamieson, Ll. Marti, A. Minamino, G. Pintaudi, S. Sano, S. Suzuki, K. Wada
备注：
With 1-page appendix. A bug was found in July 2023. This version is updated to match the erratum
We report a search for cosmic-ray boosted dark matter with protons using the 0.37 megaton$\times$years data collected at Super-Kamiokande experiment during the 1996-2018 period (SKI-IV phase). We searched for an excess of proton recoils above the atmospheric neutrino background from the vicinity of the Galactic Center. No such excess is observed, and limits are calculated for two reference models of dark matter with either a constant interaction cross-section or through a scalar mediator. This is the first experimental search for boosted dark matter with hadrons using directional information. The results present the most stringent limits on cosmic-ray boosted dark matter and exclude the dark matter-nucleon elastic scattering cross-section between $10^{-33}\text{ cm}^{2}$ and $10^{-27}\text{ cm}^{2}$ for dark matter mass from 10 MeV/$c^2$ to 1 GeV/$c^2$.
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）
Search for boosted low-mass resonances decaying into hadrons produced in association with a photon in pp collisions at $\sqrt{s}=$13 TeV with the ATLAS detector
本研究利用ATLAS探测器140 fb⁻¹的13 TeV pp碰撞数据，通过初始态辐射光子触发并搜索与光子反冲的双分支子结构大半径喷注不变质量谱，寻找20-100 GeV低质量强子衰变共振态，结果与标准模型一致并设定Z'耦合上限。
Setting limits on blazar-boosted dark matter with xenon-based detectors
University of Zurich（苏黎世大学）；The University of Sydney（悉尼大学）；European Southern Observatory（欧洲南方天文台）；New York University Abu Dhabi（阿布扎比纽约大学）；University of Oslo（奥斯陆大学）；University of California（加利福尼亚大学）
Primordial black holes as cosmic accelerators of light dark matter: Novel direct detection constraints
State Key Laboratory of Dark Matter Physics, Tsung-Dao Lee Institute & School of Physics and Astronomy, Shanghai Jiao Tong University（上海交通大学物理与天文学院、紫江研究院暗物质国家重点实验室）；Key Laboratory for Particle Astrophysics and Cosmology (MOE) & Shanghai Key Laboratory for Particle Physics and Cosmology, Shanghai Jiao Tong University（上海交通大学粒子天体物理与宇宙学教育部重点实验室、上海粒子物理与宇宙学重点实验室）；Indian Institute of Science Education and Research - Bhopal（印度科学教育研究所博帕尔分校）
Dark Parton Shower Effects for Cosmic Ray Boosted Dark Matter
College of Physics, Sichuan University（四川大学物理学院）；Institute of Physics, Henan Academy of Sciences（河南省科学院物理研究所）；Institute of Theoretical Physics, Chinese Academy of Sciences（中国科学院理论物理研究所）
Cosmic Ray Boosted Dark Matter in COSINUS: Modeling and Constraints
Max-Planck-Institut für Physik（马克斯·普朗克物理研究所）；Marietta-Blau-Institut für Teilchenphysik der Österreichischen Akademie der Wissenschaften（奥地利科学院玛丽塔·布劳粒子物理研究所）；Atominstitut, Technische Universität Wien（维也纳工业大学原子研究所）；INFN - Sezione di Roma（罗马国家核物理研究所分部）；Gran Sasso Science Institute（格兰萨索科学研究所）；INFN - Laboratori Nazionali del Gran Sasso（格兰萨索国家实验室）；Dipartimento di Scienze Fisiche e Chimiche, Università degli Studi dell’Aquila（阿奎拉大学物理与化学系）
Measurement of the solar neutrino interaction rate below 3.49 MeV in Super-Kamiokande-IV
University of California, Irvine（加州大学尔湾分校）；Kamioka Observatory, Institute for Cosmic Ray Research, University of Tokyo（东京大学宇宙射线研究所神冈观测站）；Kavli Institute for the Physics and Mathematics of the Universe (WPI), The University of Tokyo Institutes for Advanced Study, University of Tokyo（东京大学前沿研究机构 Kavli宇宙物理与数学研究所）
Search for a heavy resonance decaying into a Z and a Higgs boson in events with an energetic jet and two electrons, two muons, or missing transverse momentum in proton-proton collisions at $\sqrt{s}$ = 13 TeV
Constraints on Sub-MeV Dark Matter from Solar Reflection with DAMIC-M
University of Washington（华盛顿大学）；Pacific Northwest National Laboratory (PNNL)（太平洋西北国家实验室）；Sorbonne Université, Université Paris Cité, CNRS/IN2P3（索邦大学，巴黎西岱大学，法国国家科学研究中心/法国国家粒子物理研究所）；CNRS/IN2P3, IJCLab, Université Paris-Saclay（法国国家科学研究中心/法国国家粒子物理研究所，IJCLab，巴黎萨克雷大学）；Instituto de Física de Cantabria (IFCA), CSIC - Universidad de Cantabria（坎塔布里亚物理研究所，西班牙高等科学研究委员会-坎塔布里亚大学）；Kavli Institute for Cosmological Physics and The Enrico Fermi Institute, The University of Chicago（卡弗里宇宙物理学研究所和恩里科·费米研究所，芝加哥大学）；LPSC LSM, CNRS/IN2P3, Université Grenoble-Alpes（LPSC LSM，法国国家科学研究中心/法国国家粒子物理研究所，格勒诺布尔阿尔卑斯大学）
研究利用 DAMIC - M 探测器约 1.3 kg - 天数据，通过分析低能电子反冲空间扩散特征，给出太阳反射暗物质在重介质和超轻介质基准下暗物质 - 电子散射截面 90%置信水平上限，探测了相关参数空间。
All-electron dark matter-electron scattering with random-phase approximation dielectric screening and local field effects
Stony Brook University（石溪大学）；Flatiron Institute（平顿研究所）；C. N. Yang Institute for Theoretical Physics, Stony Brook University（石溪大学杨振宁理论物理研究所）；Institute for Advanced Computational Sciences, Stony Brook University（石溪大学高级计算科学研究院）
