TY - JOUR
T1 - Limits on Axion Couplings from the First 80 Days of Data of the PandaX-II Experiment
AU - (PandaX-II Collaboration)
AU - Fu, Changbo
AU - Zhou, Xiaopeng
AU - Chen, Xun
AU - Chen, Yunhua
AU - Cui, Xiangyi
AU - Fang, Deqing
AU - Giboni, Karl
AU - Giuliani, Franco
AU - Han, Ke
AU - Huang, Xingtao
AU - Ji, Xiangdong
AU - Ju, Yonglin
AU - Lei, Siao
AU - Li, Shaoli
AU - Liu, Huaxuan
AU - Liu, Jianglai
AU - Ma, Yugang
AU - Mao, Yajun
AU - Ren, Xiangxiang
AU - Tan, Andi
AU - Wang, Hongwei
AU - Wang, Jimin
AU - Wang, Meng
AU - Wang, Qiuhong
AU - Wang, Siguang
AU - Wang, Xuming
AU - Wang, Zhou
AU - Wu, Shiyong
AU - Xiao, Mengjiao
AU - Xie, Pengwei
AU - Yan, Binbin
AU - Yang, Yong
AU - Yue, Jianfeng
AU - Zhang, Hongguang
AU - Zhang, Tao
AU - Zhao, Li
AU - Zhou, Ning
N1 - Publisher Copyright:
© 2017 American Physical Society.
PY - 2017/11/1
Y1 - 2017/11/1
N2 - We report new searches for solar axions and galactic axionlike dark matter particles, using the first low-background data from the PandaX-II experiment at China Jinping Underground Laboratory, corresponding to a total exposure of about 2.7×104 kg day. No solar axion or galactic axionlike dark matter particle candidate has been identified. The upper limit on the axion-electron coupling (gAe) from the solar flux is found to be about 4.35×10-12 in the mass range from 10-5 to 1 keV/c2 with 90% confidence level, similar to the recent LUX result. We also report a new best limit from the Fe57 deexcitation. On the other hand, the upper limit from the galactic axions is on the order of 10-13 in the mass range from 1 to 10 keV/c2 with 90% confidence level, slightly improved compared with the LUX.
AB - We report new searches for solar axions and galactic axionlike dark matter particles, using the first low-background data from the PandaX-II experiment at China Jinping Underground Laboratory, corresponding to a total exposure of about 2.7×104 kg day. No solar axion or galactic axionlike dark matter particle candidate has been identified. The upper limit on the axion-electron coupling (gAe) from the solar flux is found to be about 4.35×10-12 in the mass range from 10-5 to 1 keV/c2 with 90% confidence level, similar to the recent LUX result. We also report a new best limit from the Fe57 deexcitation. On the other hand, the upper limit from the galactic axions is on the order of 10-13 in the mass range from 1 to 10 keV/c2 with 90% confidence level, slightly improved compared with the LUX.
UR - https://www.scopus.com/pages/publications/85032727947
U2 - 10.1103/PhysRevLett.119.181806
DO - 10.1103/PhysRevLett.119.181806
M3 - 文章
C2 - 29219572
AN - SCOPUS:85032727947
SN - 0031-9007
VL - 119
JO - Physical Review Letters
JF - Physical Review Letters
IS - 18
M1 - 181806
ER -