[HTML][HTML] Exploring the macroscopic properties of proto-neutron stars: Effects of entropy and lepton fraction
Neutron stars (NSs) have generally been considered as cold, zero-temperature entities.
Recent progress in computational methods and theoretical modelling has opened up the …
Recent progress in computational methods and theoretical modelling has opened up the …
Exploring the impact of the -cut scheme on neutron star oscillations and thermal relaxations
The σ-cut scheme was recently proposed as a method of stiffening the neutron-star equation
of state (EoS) at high densities without altering its behavior around the nuclear saturation …
of state (EoS) at high densities without altering its behavior around the nuclear saturation …
[引用][C] Constraining neutron star properties and dark matter admixture with the NITR-I equation of state: Insights from observations and universal relations
P Routaray, HC Das, JA Pattnaik… - International Journal of …, 2024 - World Scientific
A recent observational study has set a constraint on the maximum mass of neutron stars
(NSs), specifically focusing on PSR J0952-0607 and the compact star remnant HESS J1731 …
(NSs), specifically focusing on PSR J0952-0607 and the compact star remnant HESS J1731 …