12 citations · 31 across the 18 of their papers we have counts for
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Causality and perturbative-QCD constraints on first-order phase transitions in neutron stars
Asim kumar Saha, Ritam Mallick
Causality bounds the compactness and maximum mass of neutron stars. We generalise this bound to equations of state (EOSs) with a first-order phase transition between maximally stif…
Analyzing the dense matter equation of states in the light of the compact object HESS J1731-347
Skund Tewari, Sagnik Chatterjee, Deepak Kumar +1
The recent mass () and radius () measurement of HESS J1731-347 made it one of the most fascinating object if it i…
Modification of the universal relation between mass, radius and nonradial -mode oscillation in proto-neutron stars
Deepak Kumar, Asit Karan, Anshuman Verma +2
Neutron stars are usually assumed to be cold; however, in certain dynamical astrophysical scenarios such as newly born neutron stars or binary star mergers, the temperature effects…
The prospect of confining the equation of state of neutron star with future mass and radius measurement
Asim Kumar Saha, Ritam Mallick
Simultaneous measurement of mass and radius with high precision is essential to unravel the equation of state of matter at the centre of neutron stars. Measurement of massive pulsa…
Prospect of unraveling the first-order phase transition in neutron stars with and modes
Pratik Thakur, Sagnik Chatterjee, Kamal Krishna Nath +1
Quasi-normal modes of neutron stars are an exciting prospect for analyzing the internal composition of NSs and studying matter at high densities. In this work, we focus on studying…
Deciphering Accretion-Driven Starquakes in Recycled Millisecond Pulsars using Gravitational Waves
Sagnik Chatterjee, Kamal Krishna Nath, Ritam Mallick
Recycled millisecond pulsars are susceptible to starquakes as they are continuously accreting matter from their binary companion. A starquake happens when the rotational frequency…