Jul 4 – 11, 2018
COEX, SEOUL
Asia/Seoul timezone

A frequentist analysis of proton-philic spin-dependent inelastic Dark Matter (pSIDM) as an explanation of the DAMA effect

Jul 6, 2018, 3:25 PM
17m
105 (COEX, Seoul)

105

COEX, Seoul

Parallel Dark Matter Detection Dark Matter Detection

Speaker

Jong-Hyun Yoon (Sogang University)

Description

In the proton-philic spin-dependent inelastic Dark Matter (pSIDM) scenario, the yearly modulation effect in the DAMA experiment is consistent with other available constraints: from the latest experimental bounds from XENON1T, PANDAX-II, SuperCDMS, PICO-60 and CDMSlite, we obtain updated ranges of its parameters by constructing their approximate frequentist confidence intervals both in a halo-independent approach and adopting a truncated Maxwellian for the Weakly Interacting Massive Particles (WIMP) velocity distribution. In our halo–independent analysis we have implemented the WIMP halo function in terms of a step–wise parameterization. Our results confirm the present viability of the pSIDM scenario as a possible explanation of the DAMA effect.

Primary authors

Jong-Hyun Yoon (Sogang University) Mr Stefano Scopel (Sogang University) Mr Sunghyun Kang (Sogang University)

Presentation materials