Dark matter (WIMPs) direct detection
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Asia/Shanghai
B105 (CHEP)
B105
CHEP
West Building, School of Physics, PKU
Description
Dark Matter (DM) is one of the most important questions to be understood and answered in fundamental physics.
Observations with varied astronomical and cosmological technologies already pinned down that DM exists in the Universe, the Milky Way, and the Solar System. However, the understanding of DM under the language of elementary physics is still in progress.
DM direct detection aims at testing the interactive cross-section in between galactic DM particles and the nucleons of an underground detector.
Although Weakly Interactive Massive Particles (WIMPs) is the most discussed DM candidate, the null-WIMPs conclusion has been consistently addressed by most convincing experiments in the field.
We were hoping to have you at Peking University on Oct 14-16 of 2019 to discuss the challenges of DM (WIMPs) direct detection; more important, figure out possible new opportunities for us to exploit the nature of DM.
Invited speakers (including but not limited to):
Richard Gaitskell, Brown U., USA,
Dan Hooper, U. Chicago/Fermilab, USA,
Takeyasu, Ito, LANL, USA,
Isapel Lopes, U. Coimbra, Portugal,
Dan Mckinsey, UC Berkeley/LBNL, USA,
George Seidel, Brown U., USA.
Organizers:
Qing-Hong Cao, Peking U., CN,
Junhui Liao, Brown U., USA.
Peking University locates in the capital city of China, Beijing, which is dynamic and historical.
Welcome to Beijing.
Participants
Chengwei Wang
Dandan Cui
Fu-Sheng Yu
Guo-zhu（国柱） Ning*（宁）
Hao ZHANG
Isabel Lopes
Jia Liu
Jingjing Feng
Junhui Liao
Lei Wu
Lilin Yang
Limin GU
ning chen
Pengwei Xie
Qian-Fei XIANG
Qing-Hong Cao
Ran Ding
shanliang Liu
shu min zhao
Ti Gong
Tong Li
Wei Chao
Xiang Xiao
Xiao Xue
xinran li
Xue-Qian Li
Xuewen Liu
Yakefu Reyimuaji
Yalkun Nijat
Yandong Liu
Yu Gao
Yu-Jie Zhang
Yue Meng
Yue Tao
Yuehuan Wei
Zhi-Long Han
Zhong-Ying Fan
Zuowei Liu
律 吕
磊 王
Lv Lv
