activity
20142022
most citedGW170817: constraining the nuclear matter equation of state from the neutron star tidal deformability

267 citations · 1.1k across the 27 of their papers we have counts for

collaborators

28 papers

astro-ph.HE2022★ 43 cited

Dark Matter Effects on the Compact Star Properties

H. C. Das, Ankit Kumar, Bharat Kumar +1

The neutron star properties are generally determined by the equation of state of -equilibrated dense matter. In this work, we consider the interaction of fermionic dark matter (…

gr-qc2021★ 1 cited

Universal relations between the quasinormal modes of neutron star and tidal deformability

Hajime Sotani, Bharat Kumar

Universal relations independently of the equation of state (EOS) for neutron star matter are valuable, if they exist, for extracting the neutron star properties, which generally de…

astro-ph.HE2020★ 2 cited

Correlation between the curvature and some properties of the neutron star

S. K. Biswal, H. C. Das, Ankit Kumar +4

According to the general theory of relativity, a massive body induces curvature in the surrounding spacetime. In this study, the surface curvature (SC) of neutron stars is computed…

nucl-th2020★ 20 cited

BigApple force and its implications to finite nuclei and astrophysical objects

H. C. Das, Ankit Kumar, Bharat Kumar +2

The secondary component of the GW190814 event left us with a question, "whether it is a supermassive neutron star or lightest black-hole?". Recently, Fattoyev et al. have obtained…

nucl-th2020★ 54 cited

Impacts of dark matter on the curvature of the neutron star

H. C. Das, Ankit Kumar, Bharat Kumar +2

The effects of dark matter (DM) on the curvatures of the neutron star (NS) are examined by using the stiff and soft relativistic mean-field equation of states. The curvatures of th…

nucl-th2020★ 30 cited

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…