Strange stars ought to exist in the universe according to the strange quark matter hypothesis,
which states that matter made of roughly equal numbers of up, down, and strange quarks …

Upon application of both the general ensemble theory and basic thermodynamical
principles, we derive in detail the thermodynamics of strange matter with density-dependent …

We present three-dimensional numerical simulations of turbulent combustion converting a
neutron star into a quark star. Hadronic matter, described by a microphysical finite …

The previous treatments for strange quark matter in the quark mass-density-dependent
model have unreasonable vacuum limits. We provide a method to obtain the quark mass …

We study the properties of strange quark matter in equilibrium with normal nuclear matter.
Instead of using the conventional bag model in quark sector, we achieve the confinement by …

The previous thermodynamic treatment for models with density and/or temperature
dependent quark masses is shown to be inconsistent with the requirement of fundamental …

Thermodynamic formulas for investigating systems with density-and/or temperature-
dependent particle masses are generally derived from the fundamental derivation equality of …

We investigate the existence of possible stable strange matter and related stability windows
at finite temperature for different models that are generally applied to describe quark stars …

We present a modified version of quark mass scaling via considering the important one-
gluon-exchange interaction between quarks in the quark mass density-dependent model …

We present a significant extension of the quark-mass density-dependent model (QMDDM),
initially revised in our prior study [Phys. Rev. D 107, 043025 (2023) PRVDAQ 2470-0010 …