Finite size effects and the mixed quark-hadron phase in neutron stars

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dc.creatorChristiansen, Michael B.
dc.creatorGlendenning, Norman K.
dc.date1997-06-05
dc.date.accessioned2026-07-07T11:08:24Z
dc.date.available2026-07-07T11:08:24Z
dc.descriptionWe demonstrate that the form and location (not the size or spacing) of the energetically preferred geometrical structure of the crystalline quark-hadron mixed phase in a neutron star is very sensitive to finite size terms beyond the surface term. We consider two independent approaches of including further finite size terms, namely the multiple reflection expansion of the bag model and an effective surface tension description. Thus care should be taken in any model requiring detailed knowledge of these crystalline structures.
dc.description8 pages, 5 figures, Revtex. (May 13, submitted to PRC)
dc.identifierhttps://arxiv.org/abs/astro-ph/9706056
dc.identifierhttp://arxiv.org/abs/astro-ph/9706056
dc.identifierPhys.Rev.C56:2858-2864,1997
dc.identifierdoi:10.1103/PhysRevC.56.2858
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/190124
dc.subjectAstrophysics
dc.subjectNuclear Theory
dc.titleFinite size effects and the mixed quark-hadron phase in neutron stars
dc.typetext

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