Dependence of the WIMP Angular Kinetic-Energy Distribution on the Solar Galactic Orbital Velocity
arXiv:2011.06948
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.
arXiv comment9 pages, 5 figures (45 pdf plots); material prepared originally for the IDM 2020 Workshop
References in corpus (7)
- Supersymmetric Dark Matter
- A review of the discovery reach of directional Dark Matter detection
- The case for a directional dark matter detector and the status of current experimental efforts
- Readout strategies for directional dark matter detection beyond the neutrino background
- Can we overcome the neutrino floor at high masses?
- Time-integrated directional detection of dark matter
- Simulations of the 3-Dimensional Velocity Distribution of Halo Weakly Interacting Massive Particles for Directional Dark Matter Detection Experiments