Rotating neutron stars

descriptionPublicationkeyboard_double_arrow_right Part of book or chapter of book , Article , Preprint , Other literature type 26 Jun 2008Embargo end date: 01 Jan 2007 English Publisher:Springer Berlin HeidelbergFunded by:NSF | Neutron Stars as Probes f...

Authors: Weber, Fridolin; Rosenfield, Philip;

doi: 10.1007/978-3-540-76367-3_77 , 10.48550/arxiv.astro-ph/0702221

arXiv: astro-ph/0702221

Rotating neutron stars

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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.

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

Related Organizations

San Diego State University
United States
SAN DIEGO STATE UNIVERSITY FOUNDATION
United States

Keywords

Nuclear Theory (nucl-th), Nuclear Theory, Astrophysics (astro-ph), FOS: Physical sciences, Astrophysics

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