Quark star matter at finite temperature in a quasiparticle model
نویسندگان
چکیده
Abstract We study the thermodynamic properties of asymmetric quark matter, large mass stars (QSs), and proto-quark (PQSs) within quasiparticle model. Considering effects temperature model can significantly influence EOS entropy strange matter (SQM), fractions in SQM, as well tidal deformability maximum PQSs along star evolution line. Our results indicate that recent discovered heavy compact PSR J0348+0432, MSR J0740+6620, J2215+5135, especially GW190814’s secondary component $$m_2$$ m 2 be described QSs The for describing is extremely large, which not describe GW170817 QSs, heating process will further increase PQSs.
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ژورنال
عنوان ژورنال: European Physical Journal C
سال: 2021
ISSN: ['1434-6044', '1434-6052']
DOI: https://doi.org/10.1140/epjc/s10052-021-09353-9