Discrepancies Between Limits and Measurements of Warm Dark Matter Properties

Fuente: arXiv
Gespeichert in:
Bibliographische Detailangaben
1. Verfasser: Hoeneisen, Bruce
Format: Preprint
Veröffentlicht: 2025
Schlagworte:
Online-Zugang:
Tags: Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
_version_ 1866913812481835008
author Hoeneisen, Bruce
author_facet Hoeneisen, Bruce
contents A limit on the expansion parameter a_hNR at which dark matter becomes non-relativistic has been obtained from the observed minimum halo mass hosting Milky Way satellites. This limit is in disagreement with measurements. In the present study, we attempt to understand this disagreement. We find that the limit does not include the following phenomena: non-linear regeneration of the power spectrum of density perturbations, the stripping of galaxy halos by neighboring galaxies, and baryons that act as cold dark matter. Considering these phenomena, we find that there is no longer a significant discrepancy between the limit and the measurements.
format Preprint
id arxiv_https___arxiv_org_abs_2504_21031
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Discrepancies Between Limits and Measurements of Warm Dark Matter Properties
Hoeneisen, Bruce
Astrophysics of Galaxies
A limit on the expansion parameter a_hNR at which dark matter becomes non-relativistic has been obtained from the observed minimum halo mass hosting Milky Way satellites. This limit is in disagreement with measurements. In the present study, we attempt to understand this disagreement. We find that the limit does not include the following phenomena: non-linear regeneration of the power spectrum of density perturbations, the stripping of galaxy halos by neighboring galaxies, and baryons that act as cold dark matter. Considering these phenomena, we find that there is no longer a significant discrepancy between the limit and the measurements.
title Discrepancies Between Limits and Measurements of Warm Dark Matter Properties
topic Astrophysics of Galaxies
url https://arxiv.org/abs/2504.21031