Constraints on sub-GeV dark matter boosted by cosmic rays from the CDEX-10 experiment at the China Jinping Underground Laboratory

R. Xu(Tsinghua University), L. T. Yang(Tsinghua University), Q. Yue(Tsinghua University), K. Kang(Tsinghua University), Y. J. Li(Tsinghua University), M. Agartioglu(Institute of Physics, Academia Sinica), Haipeng An(Tsinghua University), J. P. Chang(Nuctech (China)), Y. H. Chen(Yalong Hydro (China)), Jianping Cheng(Beijing Normal University), W. H. Dai(Tsinghua University), Z. Deng(Tsinghua University), C. H. Fang(Sichuan University), X. P. Geng(Tsinghua University), Haipeng Gong(Tsinghua University), X. Y. Guo(Yalong Hydro (China)), Q. Guo(Peking University), Long He(Nuctech (China)), S. M. He(Yalong Hydro (China)), J. W. Hu(Tsinghua University), Han‐Xiong Huang(China Institute of Atomic Energy), T. Huang(Sun Yat-sen University), H. T. Jia(Sichuan University), Xi Jiang(Sichuan University), H. B. Li(Institute of Physics, Academia Sinica), J. M. Li(Tsinghua University), Junli Li(Tsinghua University), Q. Y. Li(Sichuan University), R. M. J. Li(Sichuan University), X. Q. Li(Nankai University), Y. L. Li(Tsinghua University), Y. F. Liang(Tsinghua University), Bin Liao(Beijing Normal University), F. K. Lin(Institute of Physics, Academia Sinica), S. T. Lin(Sichuan University), S. K. Liu(Sichuan University), Y. Liu(Sichuan University), Y. D. Liu(Sichuan University), Y. Y. Liu(Sichuan University), Z. Z. Liu(Tsinghua University), Haitao Ma(Tsinghua University), Y. C. Mao(Peking University), Q. Y. Nie(Tsinghua University), J. H. Ning(Yalong Hydro (China)), H. Pan(Nuctech (China)), Ningchun Qi(Yalong Hydro (China)), J. Ren(China Institute of Atomic Energy), Xichao Ruan(China Institute of Atomic Energy), Kapil Saraswat(Institute of Physics, Academia Sinica), V. Sharma(Institute of Physics, Academia Sinica), Z. She(Tsinghua University), M. K. Singh(Institute of Physics, Academia Sinica), T. X. Sun(Beijing Normal University), C. J. Tang(Sichuan University), W. Y. Tang(Tsinghua University), Y. Tian(Tsinghua University), G. F. Wang(Beijing Normal University), L. Wang(Beijing Normal University), Qing Wang(Tsinghua University), Y. Wang(Peking University), Yan Wang(Peking University), H. T. Wong(Institute of Physics, Academia Sinica), S. Y. Wu(Yalong Hydro (China)), Y. C. Wu(Tsinghua University), H. Xing(Sichuan University), Y. Xu(Nankai University), T. Xue(Tsinghua University), Y. L. Yan(Sichuan University), Chih-Hsiang Yeh(Institute of Physics, Academia Sinica), Yi Nan(Tsinghua University), C. X. Yu(Nankai University), Hao Yu(Nuctech (China)), J. F. Yue(Yalong Hydro (China)), Ming Zeng(Tsinghua University), Zhi Zeng(Tsinghua University), B. T. Zhang(Tsinghua University), F. S. Zhang(Beijing Normal University), L. Zhang(Sichuan University), Z. H. Zhang(Sichuan University), Z. Y. Zhang(Tsinghua University), K. K. Zhao(Sichuan University), M. G. Zhao(Nankai University), Jingchen Zhou(Yalong Hydro (China)), Z. Zhou(China Institute of Atomic Energy), J. J. Zhu(Sichuan University)
Physical review. D/Physical review. D.
September 16, 2022
Cited by 50Open Access
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Abstract

We present new constraints on light dark matter boosted by cosmic rays (CRDM) using the 205.4 kg day data of the CDEX-10 experiment conducted at the China Jinping Underground Laboratory. The Monte Carlo simulation package cjpl_ess was employed to evaluate the Earth shielding effect. Several key factors have been introduced and discussed in our CRDM analysis, including the contributions from heavier CR nuclei than proton and helium, the inhomogeneity of CR distribution, and the impact of the form factor in the Earth attenuation calculation. Our result excludes the dark matter--nucleon elastic scattering cross section region from $1.7\ifmmode\times\else\texttimes\fi{}{10}^{\ensuremath{-}30}$ to ${10}^{\ensuremath{-}26}\text{ }\text{ }{\mathrm{cm}}^{2}$ for dark matter of $10\text{ }\text{ }\mathrm{keV}/{c}^{2}$ to $1\text{ }\text{ }\mathrm{GeV}/{c}^{2}$.


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