activity
20062024
most citedThe conversion of Neutron star to Strange star : A two step process

56 citations · 396 across the 41 of their papers we have counts for

collaborators

42 papers

astro-ph.HE2024★ 1 cited

Effect of Magnetised Discontinuity on Diffusive Shock Acceleration

Anshuman Verma, Saksham Chandna, Divyansh Tripathi +1

We investigate the impact of magnetic fields and diffusion mechanisms on the energy spectra of particles accelerated via diffusive shock acceleration. We analyse magnetised shock j…

nucl-th2023

Quarkyonic Model for Neutron Star Matter: A Relativistic Mean-Field Approach

Ankit Kumar, Debabrata Dey, Shamim Haque +2

The concept of quarkyonic matter presents a promising alternative to the conventional models used to describe high-density matter and provides a more nuanced and detailed understan…

gr-qc2023★ 10 cited

Universal Relations For Generic Family Of Neutron Star Equations Of State

KamalKrishna Nath, Ritam Mallick, Sagnik Chatterjee

Universal relations are important in testing many theories of physics. In the case of general relativity, we have the celebrated no-hair theorem for black holes. Unfortunately, the…

astro-ph.HE2023★ 15 cited

Analyzing the speed of sound in neutron star with machine learning

Sagnik Chatterjee, Harsha Sudhakaran, Ritam Mallick

Matter properties at the intermediate densities are still unknown to us. In this work, we use a neural network approach to study matter at intermediate densities to analyze the var…

astro-ph.HE2022★ 2 cited

Gravitational wave signatures of phase transition from hadronic to quark matter in isolated neutron stars and binaries

Ritam Mallick

The fundamental constituent of matter at high temperature and density has intrigued physicists for quite some time. Recent results from heavy-ion colliders have enriched the Quantu…

astro-ph.HE2022

The importance of general relativistic shock calculation in the light of neutron star physics

Anshuman Verma, Ritam Mallick

Numerical simulation of hydrodynamic equations forms the central part of solving various modern astrophysical problems. In the case of shocks, one can have either dynamical equatio…