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Strange quark mass dependence of strange quark star properties [PDF]
European Physical Journal C: Particles and Fields, 2021 The effects of strange quark mass on masses, radii, and tidal deformabilities of strange quark stars are studied via the quasiparticle model that includes the non-perturbative features of QCD in low density region. The constraints of $$M_{\mathrm {TOV}} >
Bo-Lin Li, Yan Yan, Jia-Lun Ping
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Model Study of a Quark Star [PDF]
Physical Review D, 2011 In this paper we apply the equation of state (EOS) of QCD at finite chemical potential and zero temperature proposed in H. S. Zong and W. M. Sun [Int. J. Mod. Phys. {\bf A23}, 3591 (2008)] to the study of properties of quark star.
Jiang, Yu +3 more
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Quark star matter within an extended quasiparticle model [PDF]
European Physical Journal C: Particles and FieldsIn this work, we extend the quasiparticle model to include the chemical potential dependence of the coupling constant g and consider the density-dependent bag constant $$B_m$$ B m in order to satisfy the asymptotic freedom feature.
Peng-Cheng Chu +6 more
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Instability of quark matter core in a compact newborn neutron star with moderately strong magnetic field [PDF]
Pramana - Journal of Physics, 2003 Sutapa Ghosh, Somenath Chakrabarty
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Frontiers in Astronomy and Space SciencesEmploying the Korea-IBS-Daegu-SKKU (KIDS) density functional for the hadron phase and the MIT bag model with vector (vBag) model for the quark phase, we obtain hadron-quark phase transition in neutron stars considering Maxwell construction.
Debashree Sen, Chang Ho Hyun
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The Effect of a Density-Dependent Bag Constant on the Structure of a Hot Neutron Star with a Quark Core [PDF]
Astrophysics, 2013 Gholam Hossein Bordbar
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Hybrid and quark star matter based on a nonperturbative equation of state [PDF]
Physical Review D, 2020 Konstantin Otto +2 more
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Cooling of neutron stars with quark-hadron continuity [PDF]
EPJ Web of Conferences, 2022 Neutron stars are high-density objects formed by the gravitational collapse of massive stars, and the whole star can be likened to a giant nucleus. The interior of a neutron star is considered to contain exotic particles and states which do not appear in
Noda Tsuneo +4 more
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The Structure and the Density of a Bare Quark Star in a Cold Genesis Theory of Particles [PDF]
Journal of High Energy Physics Gravitation and CosmologyMarius Arghirescu
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The Macro-Physics of the Quark-Nova: Astrophysical Implications
Universe, 2022 A quark-nova is a hypothetical stellar evolution branch where a neutron star converts explosively into a quark star. Here, we discuss the intimate coupling between the micro-physics and macro-physics of the quark-nova and provide a prescription for how ...
Rachid Ouyed
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