Rotating Neutron Stars

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dc.creatorWeber, Fridolin
dc.creatorRosenfield, Philip
dc.date2007-02-08
dc.date.accessioned2026-07-07T07:45:27Z
dc.date.available2026-07-07T07:45:27Z
dc.descriptionBecause 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.
dc.description6 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
dc.identifierhttps://arxiv.org/abs/astro-ph/0702221
dc.identifierhttp://arxiv.org/abs/astro-ph/0702221
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/123532
dc.subjectAstrophysics
dc.subjectNuclear Theory
dc.titleRotating Neutron Stars
dc.typetext

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