Dark matter stars
Cosmology and Nongalactic Astrophysics
2022-03-25 v2 High Energy Physics - Phenomenology
High Energy Physics - Theory
Abstract
The dark matter in the CGF cosmology is a cosmological SU(2)-weak gauge field (the CGF). The TOV stellar structure equations are solved numerically for stars composed of this dark matter. The star mass M can take any value up to a maximum M_sun. For each value of M the star radius R lies between 5.23cm and 13.6cm. More than one value of R is possible when M > M_sun. For those stars, a transition from larger to smaller R would release gravitational energy on the order of J in a time on the order of s.
Cite
@article{arxiv.2203.12181,
title = {Dark matter stars},
author = {Daniel Friedan},
journal= {arXiv preprint arXiv:2203.12181},
year = {2022}
}
Comments
6 pages. Calculations are shown in ancillary files. v2 Insert permanent arXiv.org identifier for 1 cross reference