99 citations · 172 across the 4 of their papers we have counts for
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Warm dense matter and cooling of supernovae remnants
Ankit Kumar, H. C. Das, S. K. Biswal +2
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 par…
Neutron skins of heavy nuclei and tidal deformability of neutron star
Bharat Kumar
In this paper, I have discussed the numerical predictions for the neutron-skin thickness (NST) of various finite nuclei starting from Ca to U using recently develope…
Implications of nuclear interaction for nuclear structure and astrophysics within the relativistic mean-field model
Bharat Kumar
In this dissertation, we have studied the implications of nuclear interaction for nuclear structure and astrophysics within the relativistic mean-field (RMF) model.
GW170817: constraining the nuclear matter equation of state from the neutron star tidal deformability
Tuhin Malik, N. Alam, M. Fortin +5
Constraints set on key parameters of the nuclear matter equation of state (EoS) by the values of the tidal deformability, inferred from GW170817, are examined by using a diverse se…
Effective relativistic mean field model for finite nuclei and neutron stars
Bharat Kumar, B. K. Agrawal, S. K. Patra
New Relativistic mean field parameter set IOPB-I has been developed.
Effects of isovector scalar meson on hyperon star
S. K. Biswal, Bharat Kumar, S. K. Patra
We study the effects of isovector-scalar ()-meson on neutron star. Influence of -meson on both static and rotating neutron star is discussed. Inclusion of -meson in a neut…