#### 79 Citations

1 Bose – Einstein condensates in neutron stars

- 2021

In the two decades since the appearance of the book “Bose–Einstein Condensation” in 1995, there have been a number of developments in our understanding of dense matter. After a brief overview of… Expand

Quark matter and quark stars in a quasiparticle model

- Physics
- 2021

We investigate the properties of the equation of state of strange-quark matter and u-d quark matter, the sound velocity of quark matter, the stability region for star matter, the maximum mass of… Expand

Quark star matter at finite temperature in a quasiparticle model

- Physics
- The European Physical Journal C
- 2021

We study the thermodynamic properties of asymmetric quark matter, large mass quark stars (QSs), and proto-quark stars (PQSs) within the quasiparticle model. Considering the effects of temperature… Expand

Quark star matter in heavy quark stars

- 2021

We study the thermodynamic properties of asymmetric quark matter and large mass quark stars within the confined-isospin-density-dependent-quark-mass model. We find that the quark matter symmetry… Expand

Strange quark star and the parameter space of the quasi-particle model

- Physics
- Communications in Theoretical Physics
- 2021

The properties of strange quark stars are studied within the quasi-particle model. Taking into account chemical equilibrium and charge neutrality, the equation of state (EOS) of (2+1) -flavor quark… Expand

Unified interacting quark matter and its astrophysical implications

- Physics
- 2021

We investigate interacting quark matter (IQM), including the perturbative QCD correction and color superconductivity, for both up-down quark matter ($ud$QM) and strange quark matter (SQM). We first… Expand

Chandrasekhar limit for rotating quark stars

- Physics
- 2020

The limiting mass is a significant characteristic for compact exotic stars including quark stars and can be expressed in terms of fundamental constants and the Bag constant. In the present work,… Expand

From QCD to Neutron Stars and Back-Probing the Fundamental Properties of Dense Matter

- 2020

The first theoretical attempts to study neutron stars — the immensely dense remnants of massive stars — were conducted in the 1930s, but it took nearly 40 years for the first one to be detected. Ever… Expand

On the stability of two-flavor and three-flavor quark matter in quark stars within the framework of NJL model

- Physics
- 2020

Following our recently proposed self-consistent mean field approximation approach, we have done some researches on the chiral phase transition of strong interaction matter within the framework of N...

Proto-strange quark star structure

- Physics
- 2020

In this paper, we investigate the newborn strange quark stars with constant entropy. We also use the MIT bag model to calculate the thermodynamic properties in two cases; the density-dependent bag… Expand