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• W3179492021 abstract "We constrain the equation of state of quark stars within the Bayesian statistical approach using the mass and radius measurements of PSR J0030+0451 from NICER. Three types of bag models, with and without non-zero finite quark mass and/or superfluidity, are employed for quark stars made up with self-bound strange quark matter. We find the $90%$ posterior credible boundary around the most probable values of the quark star maximum mass is $M_{rm TOV}=2.38_{-0.23}^{+0.26},M_{odot}$, within the model flexibility of the finite quark mass, the quark pairing gap, and the perturbative contribution from the one-gluon exchange. The radius of a canonical $1.4,M_{odot}$ quark star is $R_{rm 1.4}sim12.3,{rm km}$, smaller than the results based on neutron star models." @default.
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• W3179492021 date "2021-07-16" @default.
• W3179492021 modified "2023-10-03" @default.
• W3179492021 title "Bayesian inference of quark star equation of state using the <i>NICER</i> PSR J0030+0451 data" @default.
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• W3179492021 doi "https://doi.org/10.1093/mnras/stab2029" @default.
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