Rotating Neutron Stars
Astrophysics
2007-05-23 v1 Nuclear Theory
Abstract
Because of the tremendous densities that exist in the cores of neutron stars, a significant fraction of the matter in the cores of such stars is likely to exist in the form of hyperons. Depending on spin frequency, the hyperon content changes dramatically in rotating neutron stars, as discussed in this paper.
Cite
@article{arxiv.astro-ph/0702221,
title = {Rotating Neutron Stars},
author = {Fridolin Weber and Philip Rosenfield},
journal= {arXiv preprint arXiv:astro-ph/0702221},
year = {2007}
}
Comments
6 pages, 12 figures, paper presented at the IX International Conference on Hypernuclear and Strange Particle Physics, 10-14 October 2006, Johannes Gutenberg-Universitaet Mainz, Mainz, Germany