Probing dark matter particles from evaporating primordial black holes via electron scattering in the CDEX-10 experiment

Dark matter (DM) is a major constituent of the Universe. However, no definite evidence of DM particles (denoted as “ χ ”) has been found in DM direct detection (DD) experiments to date. There is a novel concept of detecting χ from evaporating primordial black holes (PBHs). We search for χ emitted fr...

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Published inScience China. Physics, mechanics & astronomy Vol. 67; no. 10; p. 101011
Main Authors Zhang, Zhenhua, Yang, Litao, Yue, Qian, Kang, Kejun, Li, Yuanjing, An, Haipeng, Greeshma, C., Chang, Jianping, Chen, Yunhua, Cheng, Jianping, Dai, Wenhan, Deng, Zhi, Fang, Changhao, Geng, Xinping, Gong, Hui, Guo, Qiuju, Guo, Tao, Guo, Xuyuan, He, Li, He, Shengming, Hu, Jinwei, Huang, Hanxiong, Huang, Tuchen, Jiang, Lin, Karmakar, S., Li, Haubin, Li, Hanyu, Li, Jianmin, Li, Jin, Li, Qianyun, Li, Renmingjie, Li, Xueqian, Li, Yulan, Liang, Yifan, Liao, Bin, Lin, FongKay, Lin, ShinTed, Liu, Jiaxuan, Liu, Shukui, Liu, Yandong, Liu, Yu, Liu, Yuanyuan, Ma, Hao, Mao, Yucai, Nie, Qiyuan, Ning, Jinhua, Pan, Hui, Qi, Ningchun, Ren, Jie, Ruan, Xichao, Singh, Monoj Kumar, Sun, Tianxi, Tang, Changjian, Tian, Yang, Wang, Guangfu, Wang, Junzheng, Wang, Li, Wang, Qing, Wang, Yufeng, Wang, Yunxiang, Wong, Henry Tsz-King, Wu, Shiyong, Wu, Yucheng, Xing, Haoyang, Xu, Rui, Xu, Yin, Xue, Tao, Yan, Yulu, Yi, Nan, Yu, Chunxu, Yu, Haijun, Yue, Jianfeng, Zeng, Ming, Zeng, Zhi, Zhang, Bingtao, Zhang, Fengshou, Zhang, Lei, Zhang, Zhenyu, Zhao, Jizhong, Zhao, Kangkang, Zhao, Minggang, Zhou, Jifang, Zhou, Zuying, Zhu, Jingjun
Format Journal Article
LanguageEnglish
Published Beijing Science China Press 01.10.2024
Springer Nature B.V
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Summary:Dark matter (DM) is a major constituent of the Universe. However, no definite evidence of DM particles (denoted as “ χ ”) has been found in DM direct detection (DD) experiments to date. There is a novel concept of detecting χ from evaporating primordial black holes (PBHs). We search for χ emitted from PBHs by investigating their interaction with target electrons. The examined PBH masses range from 1 × 10 15 to 7 × 10 16 g under the current limits of PBH abundance f PBH . Using 205.4 kg·day data obtained from the CDEX-10 experiment conducted in the China Jinping Underground Laboratory, we exclude the χ -electron ( χ - e ) elastic-scattering cross section σ χ e ∼ 5 × 10 −29 cm 2 for χ with a mass m χ ≲ 0.1 keV from our results. With the higher radiation background but lower energy threshold (160 eV), CDEX-10 fills a part of the gap in the previous work. If ( m χ , σ χ e ) can be determined in the future, DD experiments are expected to impose strong constraints on f PBH for large M PBH s.
ISSN:1674-7348
1869-1927
DOI:10.1007/s11433-024-2446-2