activity
20092025
most citedHybrid stars in the light of GW170817

98 citations · 538 across the 29 of their papers we have counts for

collaborators

29 papers

astro-ph.HE2025

Distinct Signatures of the Nature of Phase Transition in Binary Neutron Star Mergers

Sagnik Chatterjee, Shamim Haque, Kamal Krishna Nath +2

Binary neutron-star mergers offer crucial insights into the matter properties of neutron stars. We present the possible imprints in the gravitational wave signal from the nature of…

astro-ph.HE2024★ 1 cited

Inferring neutron star properties through gravitational waves from r-modes and their relativistic counterparts

Dhanvarsh Annamalai, Rana Nandi

We present two frameworks to infer some of the properties of neutron stars from their electromagnetic radiation and the emission of continuous gravitational waves due to r-modes an…

nucl-th2024

MURCA driven Bulk viscosity in neutrino trapped baryonic matter

Sreemoyee Sarkar, Rana Nandi

We examine bulk viscosity, taking into account trapped neutrinos in baryonic matter, in the context of binary neutron star mergers. Following the merging event, the binary star can…

nucl-th2021

Low Density Neutron Star Matter with Quantum Molecular Dynamics: The Role of Vector Interactions

Parit Mehta, Rana Nandi, R. O. Gomes +2

The effect of isospin-dependent nuclear forces on the inner crust of neutron stars is modeled within the framework of Quantum Molecular Dynamics (QMD). To successfully control the…

astro-ph.HE2021★ 4 cited

Semi Universal relation to understand matter properties at neutron star interiors

Ritam Mallick, Debojoti Kuzur, Rana Nandi

The occurrence of quark matter at the center of neutron stars is still in debate. This study defines some semi-empirical parameters that quantify the occurrence and the amount of q…

astro-ph.HE2020★ 5 cited

Maximum mass of hybrid star formed via shock induced phase transition in cold neutron stars

Ritam Mallick, Shailendra Singh, Rana Nandi

This article studies the maximum mass limit of the quark star formed after the shock-induced phase transition of a cold neutron star. By employing hadronic and quark equation of st…