activity
19952022
most citedNew Hyperon Equations of State for Supernovae and Neutron Stars in Density-dependent Hadron Field Theory

250 citations · 2k across the 60 of their papers we have counts for

collaborators

60 papers

astro-ph.IM2022★ 4 cited

Pulsar timing irregularities and the Neutron Star interior in the era of SKA: An Indian Outlook

Jaikhomba Singha, Bhal Chandra Joshi, Debades Bandyopadhyay +4

There are two types of timing irregularities seen in pulsars: glitches and timing noise. Both of these phenomena can help us probe the interior of such exotic objects. This article…

astro-ph.HE2021★ 32 cited

Equation of State table with hyperon and antikaon for supernova and neutron star merger

Tuhin Malik, Sarmistha Banik, Debades Bandyopadhyay

We develop a new equation of state (EoS) table involving thermal (anti)kaons, Bose-Einstein condensate of mesons and -hyperons for core-collapse supernova and neutron st…

astro-ph.HE2020★ 14 cited

New equation of state involving Bose-Einstein condensate of antikaon for supernova and neutron star merger simulations

Tuhin Malik, Sarmistha Banik, Debades Bandyopadhyay

We compute a new equation of state table including Bose-Einstein condensate of mesons for core collapse supernova and neutron star merger simulations. Nuclei and interactin…

astro-ph.HE2019★ 15 cited

Properties of binary components and remnant in GW170817 using equations of state in finite temperature field theory models

Shriya Soma, Debades Bandyopadhyay

We investigate gross properties of binary components and remnant in GW170817 using equations of state within the finite temperature field theoretical models. We also adopt finite t…

astro-ph.HE2018★ 17 cited

Neutron star equation of state and GW170817

Sajad A. Bhat, Debades Bandyopadhyay

Properties of neutron stars in GW170817 are investigated using different equations of state (EoS) involving nucleons, hyperons, quarks resulting in neutron stars.…

astro-ph.HE2018★ 20 cited

Glitch Behavior of Pulsars and Contribution from Neutron Star Crust

Avishek Basu, Prasanta Char, Rana Nandi +2

Pulsars are highly magnetized rotating neutron stars with a very stable rotation speed. Irrespective of their stable rotation rate, many pulsars have been observed with the sudden…