DarkMix: Mixture Models for the Detection and Characterization of Dark Matter Halos
Abstract
Dark matter simulations require statistical techniques to properly identify and classify their halos and structures. Nonparametric solutions provide catalogs of these structures but lack the additional learning of a model-based algorithm and might misclassify particles in merging situations. With mixture models, we can simultaneously fit multiple density profiles to the halos that are found in a dark matter simulation. In this work, we use the Einasto profile to model the halos found in a sample of the Bolshoi simulation, and we obtain their location, size, shape, and mass. Our code is implemented in the R statistical software environment and can be accessed on https://github.com/LluisHGil/darkmix.
- Publication:
-
The Astrophysical Journal
- Pub Date:
- November 2022
- DOI:
- 10.3847/1538-4357/ac88d4
- arXiv:
- arXiv:2208.04194
- Bibcode:
- 2022ApJ...939...34H
- Keywords:
-
- Dark matter distribution;
- Galaxy dark matter halos;
- Spatial point processes;
- Mixture model;
- 356;
- 1880;
- 1915;
- 1932;
- Astrophysics - Astrophysics of Galaxies
- E-Print:
- 25 pages, 22 figures, 5 tables