activity
20222026
most citedNearly model-independent constraints on dense matter equation of state in a Bayesian approach

32 citations · 84 across the 9 of their papers we have counts for

collaborators

9 papers

astro-ph.CO2026

Prospects for Direct Detection of Ultralight Dark Matter candidates in deci-Hz Band with IndIGO-D

Md. Emanuel Hoque, Andrew L. Miller, Arunava Mukherjee

We investigate the sensitivity of IndIGO-D, a proposed space-based decihertz gravitational-wave interferometer, to different classes of ultralight dark matter. IndIGO-D will probe…

nucl-th2026

On the effect of higher order symmetry energy corrections in Skyrme models for neutron star matter

Md. Emanuel Hoque, Arunava Mukherjee

Neutron stars consist of cold, dense, neutron-rich nuclear matter under charge neutrality and -equilibrium. In most nuclear equation of state (EOS) studies, the isospin dependen…

astro-ph.HE2025

A White Paper on The Multi-Messenger Science Landscape in India

Samsuzzaman Afroz, Sanjib Kumar Agarwalla, Dipankar Bhattacharya +35

The multi-messenger science using different observational windows to the Universe such as Gravitational Waves (GWs), Electromagnetic Waves (EMs), Cosmic Rays (CRs), and Neutrinos o…

astro-ph.HE2025

Astrophysics with Compact Objects: An Indian Perspective, Present Status and Future Vision

Manjari Bagchi, Prasanta Bera, Aru Beri +18

Astrophysical compact objects, viz., white dwarfs, neutron stars, and black holes, are the remnants of stellar deaths at the end of their life cycles. They are ideal testbeds for v…

gr-qc2024★ 3 cited

Rapid neutron star equation of state inference with Normalising Flows

Jordan McGinn, Arunava Mukherjee, Jessica Irwin +3

The first direct detection of gravitational waves from binary neutron stars on the 17th of August, 2017, (GW170817) heralded the arrival of a new messenger for probing neutron star…

nucl-th2023★ 12 cited

Direct mapping of tidal deformability to the iso-scalar and iso-vector nuclear matter parameters

Sk Md Adil Imam, Arunava Mukherjee, B. K. Agrawal +1

Background: The equations of state (EoSs) which determine the properties of neutron stars (NSs) are often characterized by the iso-scalar and iso-vector nuclear matter parameters (…

nucl-th2023★ 31 cited

Systematic analysis of the impacts of symmetry energy parameters on neutron star properties

N. K. Patra, Anagh Venneti, Sk Md Adil Imam +2

The impacts of various symmetry energy parameters on the properties of neutron stars (NSs) have been recently investigated, and the outcomes are at variance, as summarized in Table…

gr-qc2022★ 6 cited

Implementation of a new weave-based search pipeline for continuous gravitational waves from known binary systems

Arunava Mukherjee, Reinhard Prix, Karl Wette

Scorpius X-1 (Sco X-1) has long been considered one of the most promising targets for detecting continuous gravitational waves with ground-based detectors. Observational searches f…

nucl-th2022★ 32 cited

Nearly model-independent constraints on dense matter equation of state in a Bayesian approach

N. K. Patra, Sk Md Adil Imam, B. K. Agrawal +2

We apply Bayesian approach to construct a large number of minimally constrained equations of state (EOSs) and study their correlations with a few selected properties of a neutron s…