Dependence of the WIMP Angular Kinetic-Energy Distribution on the Solar Galactic Orbital Velocity
High Energy Astrophysical Phenomena
2020-11-16 v1 Astrophysics of Galaxies
Solar and Stellar Astrophysics
High Energy Physics - Phenomenology
Abstract
In this article, we study in a little more detail the angular kinetic-energy distribution of halo Weakly Interacting Massive Particles (WIMPs) and consider two simple modifications with the Solar Galactic orbital velocity in our Monte Carlo simulations of the 3-dimensional WIMP velocity as the first trial of future investigations on distinguishing models of the Galactic structure of Dark Matter particles by using directional direct detection data.
Keywords
Cite
@article{arxiv.2011.06948,
title = {Dependence of the WIMP Angular Kinetic-Energy Distribution on the Solar Galactic Orbital Velocity},
author = {Chung-Lin Shan},
journal= {arXiv preprint arXiv:2011.06948},
year = {2020}
}
Comments
9 pages, 5 figures (45 pdf plots); material prepared originally for the IDM 2020 Workshop