Speaker
Dr
Chung-Lin SHAN
(Xinjiang Astronomical Observatory, Chinese Academy of Sciences)
Description
In this talk, we discuss the effects of a non-negligible threshold energy on our model-independent methods developed for reconstructing WIMP properties by using measured recoil energies in direct Dark Matter detection experiments directly. Our expressions for reconstructing the mass and the (ratios between the) spin-independent and the spin-dependent WIMP-nucleon couplings have been modified. We will focus on low-mass (m_chi <~ 50 GeV) WIMPs and present some (preliminary) numerical results obtained by Monte-Carlo simulations.
Primary author
Dr
Chung-Lin SHAN
(Xinjiang Astronomical Observatory, Chinese Academy of Sciences)
