With the effective chiral model, the finite temperature properties of nuclear matter have been
studied at different temperatures. For symmetric nuclear matter, I particularly focused on the …

We study the thermal effects on the nuclear matter (NM) properties such as binding energy,
incompressibility, free symmetry energy and its coefficients using NL3, G3 and IU-FSU …

Neutron stars (NSs) have generally been considered as cold, zero-temperature entities.
Recent progress in computational methods and theoretical modelling has opened up the …

In this work, we reinvestigate the electron fraction Ye and electron Fermi energy EF (e) of
neutron stars, based on our previous work, in which we first deduce a special solution to EF …

The low braking index pulsar PSR J1734− 3333 could be born with a superhigh internal
magnetic field of 1014–1016 G, and undergo a supercritical accretion soon after its …

Neutron Stars (NSs) are often treated as cold, zero-temperature objects in the conventional
method of research. However, the recent advances in computational techniques and …

We present a methodical study of the thermal and nuclear properties for the hot nuclear
matter using relativistic-mean field theory. We examine the effects of temperature on the …

A detailed description of the baryon direct Urca processes A: $ n\to p+ e+{\bar {\nu}} _ {e} $,
B: $\Lambda\to p+ e+{\bar {\nu}} _ {e} $ and C: ${\Xi}^{-}\to\Lambda+ e+{\bar {\nu}} _ {e} …