TY - JOUR
T1 - Search for Light Dark Matter from the Atmosphere in PandaX-4T
AU - (PandaX Collaboration)
AU - Ning, Xuyang
AU - Abdukerim, Abdusalam
AU - Bo, Zihao
AU - Chen, Wei
AU - Chen, Xun
AU - Cheng, Chen
AU - Cheng, Zhaokan
AU - Cui, Xiangyi
AU - Fan, Yingjie
AU - Fang, Deqing
AU - Fu, Changbo
AU - Fu, Mengting
AU - Geng, Lisheng
AU - Giboni, Karl
AU - Gu, Linhui
AU - Guo, Xuyuan
AU - Han, Chencheng
AU - Han, Ke
AU - He, Changda
AU - He, Jinrong
AU - Huang, Di
AU - Huang, Yanlin
AU - Huang, Junting
AU - Huang, Zhou
AU - Hou, Ruquan
AU - Hou, Yu
AU - Ji, Xiangdong
AU - Ju, Yonglin
AU - Li, Chenxiang
AU - Li, Jiafu
AU - Li, Mingchuan
AU - Li, Shuaijie
AU - Li, Tao
AU - Lin, Qing
AU - Liu, Jianglai
AU - Lu, Congcong
AU - Lu, Xiaoying
AU - Luo, Lingyin
AU - Luo, Yunyang
AU - Ma, Wenbo
AU - Ma, Yugang
AU - Mao, Yajun
AU - Meng, Yue
AU - Qi, Ningchun
AU - Qian, Zhicheng
AU - Ren, Xiangxiang
AU - Shaheed, Nasir
AU - Shang, Xiaofeng
AU - Shao, Xiyuan
AU - Tan, Andi
N1 - Publisher Copyright:
© 2023 authors. Published by the American Physical Society.
PY - 2023/7/28
Y1 - 2023/7/28
N2 - We report a search for light dark matter produced through the cascading decay of η mesons, which are created as a result of inelastic collisions between cosmic rays and Earth's atmosphere. We introduce a new and general framework, publicly accessible, designed to address boosted dark matter specifically, with which a full and dedicated simulation including both elastic and quasielastic processes of Earth attenuation effect on the dark matter particles arriving at the detector is performed. In the PandaX-4T commissioning data of 0.63 tonne·year exposure, no significant excess over background is observed. The first constraints on the interaction between light dark matter generated in the atmosphere and nucleus through a light scalar mediator are obtained. The lowest excluded cross section is set at 5.9×10-37 cm2 for a dark matter mass of 0.1 MeV/c2 and mediator mass of 300 MeV/c2. The lowest upper limit of η to the dark matter decay branching ratio is 1.6×10-7.
AB - We report a search for light dark matter produced through the cascading decay of η mesons, which are created as a result of inelastic collisions between cosmic rays and Earth's atmosphere. We introduce a new and general framework, publicly accessible, designed to address boosted dark matter specifically, with which a full and dedicated simulation including both elastic and quasielastic processes of Earth attenuation effect on the dark matter particles arriving at the detector is performed. In the PandaX-4T commissioning data of 0.63 tonne·year exposure, no significant excess over background is observed. The first constraints on the interaction between light dark matter generated in the atmosphere and nucleus through a light scalar mediator are obtained. The lowest excluded cross section is set at 5.9×10-37 cm2 for a dark matter mass of 0.1 MeV/c2 and mediator mass of 300 MeV/c2. The lowest upper limit of η to the dark matter decay branching ratio is 1.6×10-7.
UR - https://www.scopus.com/pages/publications/85166732162
UR - https://www.scopus.com/pages/publications/85166732162#tab=citedBy
U2 - 10.1103/PhysRevLett.131.041001
DO - 10.1103/PhysRevLett.131.041001
M3 - Article
C2 - 37566838
AN - SCOPUS:85166732162
SN - 0031-9007
VL - 131
JO - Physical review letters
JF - Physical review letters
IS - 4
M1 - 041001
ER -