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

Sutapa Ghosh·Somenath Chakrabarty
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Abstract

It 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.

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Sutapa Ghosh, Somenath Chakrabarty. 2001-10-05. Instability of Quark Matter Core in a Compact Newborn Neutron Star With Moderately Strong Magnetic Field. https://doi.org/10.1007/bf02707009

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