Quark stars admixed with dark matter
High Energy Astrophysical Phenomena
2016-04-27 v1 High Energy Physics - Phenomenology
Abstract
Compact stars consisting of massless quark matter and fermionic dark matter are studied by solving the Tolman-Oppenheimer-Volkoff equations for two fluids separately. Dark matter is further investigated by incorporating inter-fermionic interactions among the dark matter particles. The properties of stars made of quark matter particles and self-interacting and free dark matter particles are explored by obtaining their mass-radius relations. The regions of stability for such a compact star are determined and it is demonstrated that the maximum stable total mass of such a star decreases approximately linearly with increasing dark matter fraction.
Keywords
Cite
@article{arxiv.1511.00238,
title = {Quark stars admixed with dark matter},
author = {Payel Mukhopadhyay and Juregen Schaffner-Bielich},
journal= {arXiv preprint arXiv:1511.00238},
year = {2016}
}