We study how the indirect observation of dark matter substructures in the
Milky Way, using recent stellar stream studies, translate into constraints for
different dark matter models. We obtain the lower bounds $m_WDM >
3.2\,keV$ and $m_FDM > 5.210^-21\,eV$ on the warm
dark matter and fuzzy dark matter particle mass, respectively. When dark matter
is coupled to a dark radiation bath, we find that kinetic decoupling must take
place at temperatures higher than $T_kd > 0.7\,keV$. We also
discuss future prospects of stellar stream observations.
Описание
Implications of Milky Way Substructures for the Nature of Dark Matter
%0 Generic
%1 benito2020implications
%A Benito, María
%A Criado, Juan Carlos
%A Hütsi, Gert
%A Raidal, Martti
%A Veermäe, Hardi
%D 2020
%K tifr
%T Implications of Milky Way Substructures for the Nature of Dark Matter
%U http://arxiv.org/abs/2001.11013
%X We study how the indirect observation of dark matter substructures in the
Milky Way, using recent stellar stream studies, translate into constraints for
different dark matter models. We obtain the lower bounds $m_WDM >
3.2\,keV$ and $m_FDM > 5.210^-21\,eV$ on the warm
dark matter and fuzzy dark matter particle mass, respectively. When dark matter
is coupled to a dark radiation bath, we find that kinetic decoupling must take
place at temperatures higher than $T_kd > 0.7\,keV$. We also
discuss future prospects of stellar stream observations.
@misc{benito2020implications,
abstract = {We study how the indirect observation of dark matter substructures in the
Milky Way, using recent stellar stream studies, translate into constraints for
different dark matter models. We obtain the lower bounds $m_{\rm WDM} >
3.2\,{\rm keV}$ and $m_{\rm FDM} > 5.2\times 10^{-21}\,{\rm eV}$ on the warm
dark matter and fuzzy dark matter particle mass, respectively. When dark matter
is coupled to a dark radiation bath, we find that kinetic decoupling must take
place at temperatures higher than $T_{\rm kd} > 0.7\,{\rm keV}$. We also
discuss future prospects of stellar stream observations.},
added-at = {2020-01-30T08:13:33.000+0100},
author = {Benito, María and Criado, Juan Carlos and Hütsi, Gert and Raidal, Martti and Veermäe, Hardi},
biburl = {https://www.bibsonomy.org/bibtex/23e6f4b8092a554a3f9464c4c18af6c85/citekhatri},
description = {Implications of Milky Way Substructures for the Nature of Dark Matter},
interhash = {896fa3b11ef951283da7ab34a2ae4733},
intrahash = {3e6f4b8092a554a3f9464c4c18af6c85},
keywords = {tifr},
note = {cite arxiv:2001.11013Comment: 10 pages, 4 figures},
timestamp = {2020-01-30T08:13:33.000+0100},
title = {Implications of Milky Way Substructures for the Nature of Dark Matter},
url = {http://arxiv.org/abs/2001.11013},
year = 2020
}