http://arxiv.org/abs/1906.11189
We perform the stability analysis against radial oscillations for quark stars obtained using the equation of state for cold quark matter from perturbative QCD. We find a distinguishable splitting between zero-mode periods in neutron stars and quark stars taking into account the recent gravitational wave constraint on the maximum masses of compact stars.
J. Jiménez and E. Fraga
Thu, 27 Jun 19
58/62
Comments: 7 pages, 4 figures
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