Abstract: DaMaSCUS calculates the density and velocity distribution of dark matter (DM) at any detector of given depth and latitude to provide dark matter particle trajectories inside the Earth. Provided a strong enough DM-matter interaction, the particles scatter on terrestrial atoms and get decelerated and deflected. The resulting local modifications of the DM velocity distribution and number density can have important consequences for direct detection experiments, especially for light DM, and lead to signatures such as diurnal modulations depending on the experiment's location on Earth. The code involves both the Monte Carlo simulation of particle trajectories and generation of data as well as the data analysis consisting of non-parametric density estimation of the local velocity distribution functions and computation of direct detection event rates.
Credit: Emken, Timon; Kouvaris, Chris
https://ui.adsabs.harvard.edu/abs/2017J ... E/abstract
Preferred citation method: https://ui.adsabs.harvard.edu/abs/2017ascl.soft06003E and https://ui.adsabs.harvard.edu/abs/2017JCAP...10..031E