Comparing P-stars with Observations
Astrophysics
2009-11-13 v2 High Energy Physics - Phenomenology
Abstract
P-stars are compact stars made of up and down quarks in -equilibrium with electrons in a chromomagnetic condensate. P-stars are able to account for compact stars as well as stars with radius comparable with canonical neutron stars. We compare p-stars with different available observations. Our results indicate that p-stars are able to reproduce in a natural manner several observations from isolated and binary pulsars.
Cite
@article{arxiv.astro-ph/0703523,
title = {Comparing P-stars with Observations},
author = {Paolo Cea},
journal= {arXiv preprint arXiv:astro-ph/0703523},
year = {2009}
}
Comments
15 pages, 2 figures; accepted for publication in Astrophysical Journal