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Dark matter direct search sensitivity of the PandaX-4T experiment
by
Chen, YunHua
, Gu, LinHui
, Cui, XiangYi
, Yan, BinBin
, Han, Ke
, Wang, Meng
, Zhou, Ning
, Huang, XingTao
, Ning, JinHua
, Wang, QiuHong
, Wu, ShiYong
, Fu, ChangBo
, Wang, HongWei
, Wang, SiGuang
, Liu, HuaXuan
, Abdukerim, Abdusalam
, Ren, XiangXiang
, Ji, Peng
, Yu, ChunXu
, Chen, Xun
, Zhang, Dan
, Lin, Heng
, Li, ShaoLi
, Giuliani, Franco
, Dong, BinBin
, Zhou, XiaoPeng
, Zheng, QiBin
, Ji, XiangDong
, Wang, Zhou
, Huang, Zhou
, Mao, YaJun
, Xiao, MengJiao
, Zhang, HongGuang
, Tan, AnDi
, Shi, Fang
, Xie, PengWei
, Yuan, JuMin
, Li, Yao
, Fang, DeQing
, He, ChangDa
, Wang, Cheng
, Liu, JiangLai
, Yang, Yong
, Zhang, Tao
, Ni, KaiXiang
, Yue, JianFeng
, Ju, YongLin
, Ma, YuGang
, Xia, JingKai
, Zhao, Li
, Giboni, Karl
, Yang, JiJun
, Guo, ZhiFan
, Wang, AnQing
, Wang, XiuLi
, Chen, Wei
, Wang, XuMing
, Guo, XuYuan
, Wu, MengMeng
, He, ShengMing
, Huang, Di
, Zhou, JiFang
in
Astronomy
/ Classical and Continuum Physics
/ Cosmic rays
/ Cosmology
/ Dark matter
/ Experiments
/ Laboratories
/ Observations and Techniques
/ Particle physics
/ Physics
/ Physics and Astronomy
/ Recoil
/ Sensitivity
/ Sensors
2019
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Dark matter direct search sensitivity of the PandaX-4T experiment
by
Chen, YunHua
, Gu, LinHui
, Cui, XiangYi
, Yan, BinBin
, Han, Ke
, Wang, Meng
, Zhou, Ning
, Huang, XingTao
, Ning, JinHua
, Wang, QiuHong
, Wu, ShiYong
, Fu, ChangBo
, Wang, HongWei
, Wang, SiGuang
, Liu, HuaXuan
, Abdukerim, Abdusalam
, Ren, XiangXiang
, Ji, Peng
, Yu, ChunXu
, Chen, Xun
, Zhang, Dan
, Lin, Heng
, Li, ShaoLi
, Giuliani, Franco
, Dong, BinBin
, Zhou, XiaoPeng
, Zheng, QiBin
, Ji, XiangDong
, Wang, Zhou
, Huang, Zhou
, Mao, YaJun
, Xiao, MengJiao
, Zhang, HongGuang
, Tan, AnDi
, Shi, Fang
, Xie, PengWei
, Yuan, JuMin
, Li, Yao
, Fang, DeQing
, He, ChangDa
, Wang, Cheng
, Liu, JiangLai
, Yang, Yong
, Zhang, Tao
, Ni, KaiXiang
, Yue, JianFeng
, Ju, YongLin
, Ma, YuGang
, Xia, JingKai
, Zhao, Li
, Giboni, Karl
, Yang, JiJun
, Guo, ZhiFan
, Wang, AnQing
, Wang, XiuLi
, Chen, Wei
, Wang, XuMing
, Guo, XuYuan
, Wu, MengMeng
, He, ShengMing
, Huang, Di
, Zhou, JiFang
in
Astronomy
/ Classical and Continuum Physics
/ Cosmic rays
/ Cosmology
/ Dark matter
/ Experiments
/ Laboratories
/ Observations and Techniques
/ Particle physics
/ Physics
/ Physics and Astronomy
/ Recoil
/ Sensitivity
/ Sensors
2019
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Do you wish to request the book?
Dark matter direct search sensitivity of the PandaX-4T experiment
by
Chen, YunHua
, Gu, LinHui
, Cui, XiangYi
, Yan, BinBin
, Han, Ke
, Wang, Meng
, Zhou, Ning
, Huang, XingTao
, Ning, JinHua
, Wang, QiuHong
, Wu, ShiYong
, Fu, ChangBo
, Wang, HongWei
, Wang, SiGuang
, Liu, HuaXuan
, Abdukerim, Abdusalam
, Ren, XiangXiang
, Ji, Peng
, Yu, ChunXu
, Chen, Xun
, Zhang, Dan
, Lin, Heng
, Li, ShaoLi
, Giuliani, Franco
, Dong, BinBin
, Zhou, XiaoPeng
, Zheng, QiBin
, Ji, XiangDong
, Wang, Zhou
, Huang, Zhou
, Mao, YaJun
, Xiao, MengJiao
, Zhang, HongGuang
, Tan, AnDi
, Shi, Fang
, Xie, PengWei
, Yuan, JuMin
, Li, Yao
, Fang, DeQing
, He, ChangDa
, Wang, Cheng
, Liu, JiangLai
, Yang, Yong
, Zhang, Tao
, Ni, KaiXiang
, Yue, JianFeng
, Ju, YongLin
, Ma, YuGang
, Xia, JingKai
, Zhao, Li
, Giboni, Karl
, Yang, JiJun
, Guo, ZhiFan
, Wang, AnQing
, Wang, XiuLi
, Chen, Wei
, Wang, XuMing
, Guo, XuYuan
, Wu, MengMeng
, He, ShengMing
, Huang, Di
, Zhou, JiFang
in
Astronomy
/ Classical and Continuum Physics
/ Cosmic rays
/ Cosmology
/ Dark matter
/ Experiments
/ Laboratories
/ Observations and Techniques
/ Particle physics
/ Physics
/ Physics and Astronomy
/ Recoil
/ Sensitivity
/ Sensors
2019
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Dark matter direct search sensitivity of the PandaX-4T experiment
Journal Article
Dark matter direct search sensitivity of the PandaX-4T experiment
2019
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Overview
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
−1
d
−1
keV
−1
. The nuclear recoil background in the same region is 2:8 × 10
−7
kg
−1
d
−1
keV
−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
cm
2
at a dark matter mass of 40 GeV/
c
2
.
Publisher
Science China Press,Springer,Springer Nature B.V
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