Dark Matter Mass and Anisotropy in Directional Detector
Cosmology and Nongalactic Astrophysics
2019-09-20 v1 High Energy Physics - Experiment
High Energy Physics - Phenomenology
Abstract
Velocity distribution of dark matter is supposed to be isotropic Maxwell-Boltzmann distribution in most cases, however, other distribution models including anisotropic one are suggested by simulations. Directional direct detection of dark matter is expected to be a hopeful way to discriminate isotropic distribution from anisotropic one. We investigate the possibility to obtain the anisotropy and WIMP mass by Monte-Carlo simulation supposing the directional detector.
Keywords
Cite
@article{arxiv.1909.08861,
title = {Dark Matter Mass and Anisotropy in Directional Detector},
author = {Keiko I. Nagao},
journal= {arXiv preprint arXiv:1909.08861},
year = {2019}
}
Comments
3pages, 8 figures. Proceedings for PPAP 2019 (2nd workshop on Phenomenology for Particle and Anti-Particle 2019)