Instability of Quark Matter Core in a Compact Newborn Neutron Star With Moderately Strong Magnetic Field

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dc.creatorGhosh, Sutapa
dc.creatorChakrabarty, Somenath
dc.date2001-10-05
dc.date.accessioned2026-07-07T11:08:01Z
dc.date.available2026-07-07T11:08:01Z
dc.descriptionIt is explicitly shown that if phase transition occurs at the core of a newborn neutron star with moderately strong magnetic field strength, which populates only the electron's Landau levels, then in the $β$-equilibrium condition, the quark core is energetically much more unstable than the neutron matter of identical physical condition.
dc.descriptionSix pages REVTEX file, one .eps file (included)
dc.identifierhttps://arxiv.org/abs/astro-ph/0110135
dc.identifierhttp://arxiv.org/abs/astro-ph/0110135
dc.identifierPramana60:901-908,2002
dc.identifierdoi:10.1007/BF02707009
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/190000
dc.subjectAstrophysics
dc.titleInstability of Quark Matter Core in a Compact Newborn Neutron Star With Moderately Strong Magnetic Field
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