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在氩时间投影室中进行首次核超重暗物质搜索:DarkSide-50实验

First Nuclear Ultra-Heavy Dark Matter Search in Argon Time Projection Chambers with the DarkSide-50 Experiment

Gran Sasso Science Institute(格兰萨索科学研究所);INFN Laboratori Nazionali del Gran Sasso(意大利国家核物理研究所格兰萨索国家实验室);Instituto de Física, Universidade de São Paulo(圣保罗大学物理研究所);Pacific Northwest National Laboratory(太平洋西北国家实验室);Augustana University(奥古斯塔纳大学);Physics Department, Università degli Studi di Pisa(比萨大学物理系);INFN Pisa(意大利国家核物理研究所比萨分部);Fermi National Accelerator Laboratory(费米国家加速器实验室);INFN Sezione di Roma(意大利国家核物理研究所罗马分部);INFN Cagliari(意大利国家核物理研究所卡利亚里分部);Università degli Studi di Genova(热那亚大学);INFN Genova(意大利国家核物理研究所热那亚分部);Università degli Studi Roma Tre(罗马第三大学);INFN Roma Tre(意大利国家核物理研究所罗马第三分部);Università degli Studi di Cagliari(卡利亚里大学)
P. Agnes, I. F. Albuquerque, T. Alexander, A. K. Alton, M. Ave, H. O. Back, G. Batignani, K. Biery, V. Bocci, W. M. Bonivento, B. Bottino, S. Bussino, M. Cadedd… 展开作者

P. Agnes, I. F. Albuquerque, T. Alexander, A. K. Alton, M. Ave, H. O. Back, G. Batignani, K. Biery, V. Bocci, W. M. Bonivento, B. Bottino, S. Bussino, M. Cadeddu, M. Cadoni, F. Calaprice, A. Caminata, M. D. Campos, N. Canci, M. Caravati, N. Cargioli, M. Cariello, M. Carlini, P. Cavalcante, S. Chashin, A. Chepurnov, D. D'Angelo, S. Davini, S. De Cecco, A. V. Derbin, M. D'Incecco, C. Dionisi, F. Dordei, M. Downing, M. Fairbairn, G. Fiorillo, D. Franco, F. Gabriele, C. Galbiati, C. Ghiano, C. Giganti, G. K. Giovanetti, V. Goicoechea Casanueva, A. M. Goretti, G. Grilli di Cortona, A. Grobov, M. Gromov, M. Guam, M. Gulino, B. R. Hackett, K. Herner, T. Hessel, F. Hubaut, E. V. Hungerford, A. Ianni, V. Ippolito, K. Keeter, C. L. Kendziora, M. Kimura, I. Kochanek, D. Korablev, G. Korga, A. Kubankin, J. Kumar, M. Kuss, M. La Commara, M. Lai, X. Li, M. Lissia, O. Lychagina, I. N. Machulin, L. P. Mapelli, S. M. Mari, J. Maricic, A. Messina, R. Milincic, J. Monroe, M. Morrocchi, V. N. Muratova, P. Musico, A. O. Nozdrina, A. Oleinik, F. Ortica, L. Pagani, M. Pallavicini, L. Pandola, E. Pantic, E. Paoloni, K. Pelczar, N. Pelliccia, S. Piacentini, A. Pocar, M. Poehlmann, S. Pordes, S. S. Poudel, P. Pralavorio, D. Price, F. Ragusa, M. Razeti, A. L. Renshaw, M. Rescigno, A. Romani, D. Sablone, O. Samoylov, S. Sanfilippo, C. Savarese, B. Schlitzer, D. A. Semenov, A. Shchagin, A. Sheshukov, M. D. Skorokhvatov, O. Smirnov, A. Sotnikov, S. Stracka, Y. Suvorov, R. Tartaglia, G. Testera, A. Tonazzo, E. V. Unzhakov, A. Vishneva, R. B. Vogelaar, M. Wada, H. Wang, Y. Wang, S. Westerdale, M. M. Wojcik, X. Xiao, C. Yang, G. Zuzel

AI总结:

DarkSide-50实验在氩时间投影室中首次探测核超重暗物质,通过多散射事件拓扑结构优化,排除了不同暗核子质量下的散射截面限。

摘要:

我们报告了使用DarkSide-50实验在双相液氩时间投影室中首次搜索核超重暗物质(UHDM)。与传统弱相互作用大质量粒子(WIMPs)不同,核UHDM候选者可能由许多暗核子组成,并在通过探测器时多次散射。考虑到通过地球岩层的能量损失,我们应用了优化用于多散射事件拓扑结构的选择标准,使用DarkSide-50探测器的532天低辐射活动。给出了针对暗核子质量为$ m_χ= 10, 50, 100, 500 \, \mathrm{GeV/c^2} $的UHDM-核子散射截面的排除限。

英文摘要:

We report the first search for nuclear ultra-heavy dark matter (UHDM) in a dual-phase liquid argon time projection chamber using the DarkSide-50 experiment. Unlike conventional weakly interacting massive particles (WIMPs), nuclear UHDM candidates may be composed of many dark nucleons and scatter numerous times while passing through the detector. Accounting for energy loss through the Earth's overburden, we apply selection criteria optimized for multi-scatter event topologies using the 532-day low-radiation campaign of the DarkSide-50 detector. Excluded limits on the UHDM-nucleon scattering cross section for dark nucleon masses of $m_χ= 10, 50, 100, 500 \, \mathrm{GeV/c^2}$ are presented.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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