Dark matter direct search sensitivity of the PandaX-4T experiment

Hong Guang Zhang, Abdusalam Abdukerim, Wei Chen, Xun Chen, Yun Hua Chen, Xiang Yi Cui, Bin Bin Dong, De Qing Fang, Chang Bo Fu, Karl Giboni, Franco Giuliani, Lin Hui Gu, Xu Yuan Guo, Zhi Fan Guo, Ke Han, Chang Da He, Sheng Ming He, Di Huang, Xing Tao Huang, Zhou HuangPeng Ji, Xiang Dong Ji, Yong Lin Ju, Shao Li Li, Yao Li, Heng Lin, Hua Xuan Liu, Jiang Lai Liu, Yu Gang Ma, Ya Jun Mao, Kai Xiang Ni, Jin Hua Ning, Xiang Xiang Ren, Fang Shi, An Di Tan, An Qing Wang, Cheng Wang, Hong Wei Wang, Meng Wang, Qiu Hong Wang, Si Guang Wang, Xiu Li Wang, Xu Ming Wang, Zhou Wang, Meng Meng Wu, Shi Yong Wu, Jing Kai Xia, Meng Jiao Xiao, Peng Wei Xie, Bin Bin Yan, Ji Jun Yang, Yong Yang, Chun Xu Yu, Ju Min Yuan, Jian Feng Yue, Dan Zhang, Tao Zhang, Li Zhao, Qi Bin Zheng, Ji Fang Zhou, Ning Zhou, Xiao Peng Zhou

Research output: Contribution to journalArticlepeer-review

160 Scopus citations

Abstract

The PandaX-4T experiment, a 4-ton scale dark matter direct detection experiment, is being planned at the China Jinping Un- derground Laboratory. In this paper we present a simulation study of the expected background in this experiment. In a 2.8-ton fiducial mass and the signal region between 1–10 keV electron equivalent energy, the total electron recoil background is found to be 4:9 × 10−5 kg−1d−1keV−1. The nuclear recoil background in the same region is 2:8 × 10−7 kg−1d−1keV−1. With an exposure of 5.6 ton-years, the sensitivity of PandaX-4T could reach a minimum spin-independent dark matter-nucleon cross section of 6 × 10−48 cm2 at a dark matter mass of 40 GeV/c2.

Original languageEnglish (US)
Article number31011
JournalScience China: Physics, Mechanics and Astronomy
Volume62
Issue number3
DOIs
StatePublished - Mar 1 2019
Externally publishedYes

All Science Journal Classification (ASJC) codes

  • General Physics and Astronomy

Keywords

  • WIMPs
  • dark matter
  • direct detection
  • xenon

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