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arXiv · 2011.06948

Dependence of the WIMP Angular Kinetic-Energy Distribution on the Solar Galactic Orbital Velocity

Chung-Lin Shan
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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.

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Chung-Lin Shan. 2020-11-13. Dependence of the WIMP Angular Kinetic-Energy Distribution on the Solar Galactic Orbital Velocity. https://arxiv.org/abs/2011.06948

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