Structured Mixed Phase is Favored in Neutron Stars

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dc.creatorChristiansen, Michael B.
dc.creatorGlendenning, Norman K.
dc.date2000-08-14
dc.date.accessioned2026-07-07T01:54:55Z
dc.date.available2026-07-07T01:54:55Z
dc.descriptionWe give a general thermodynamical argument showing that in neutron stars, the Coulomb structured mixed phase is always favored for any first order phase transition involving systems in equilibrium with baryon number and electric charge as the two independent components. This finding is likely to have important consequences for many neutron star properties, e.g., glitch phenomena, transport and superfluid properties, r-mode instabilities, and the braking index.
dc.descriptionLatex, 4 pages, 2 figures
dc.identifierhttps://arxiv.org/abs/astro-ph/0008207
dc.identifierhttp://arxiv.org/abs/astro-ph/0008207
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/1481
dc.subjectAstrophysics
dc.titleStructured Mixed Phase is Favored in Neutron Stars
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