activity
20242026
most citedFermionic versus Bosonic Dark Matter in Neutron Stars: A Bayesian Study with Multi-Density Constraints

2 citations · 2 across the 5 of their papers we have counts for

collaborators

9 papers

nucl-th2026

-Driven Direct Urca Cooling in Rotating Neutron Stars: A Bayesian Study

Aprajita Shrivastava, Debanjan Guha Roy, Sarmistha Banik

We investigate the onset of antikaon () condensation and its implications for the equation of state (EoS) and cooling of neutron stars (NSs) within density-dependent relativis…

nucl-th2026

NucleiML: A machine learning framework of ground-state properties of finite nuclei for accelerated Bayesian exploration

Anagh Venneti, Chiranjib Mondal, Sk Md Adil Imam +2

The global behavior of the nuclear equation of state (EoS) is commonly studied using data from finite nuclei (FN), heavy-ion collisions, and astrophysical observations of neutron s…

nucl-th2026

Influence of Finite-Nuclei Constraints on High-Density Transitions and Neutron Star Properties

Anagh Venneti, Sarmistha Banik, Bijay K Agrawal

We construct posterior distributions of the equation of state (EoS) for matter beyond the inner crust of neutron stars by incorporating finite nuclei (FN) constraints within relati…

astro-ph.CO20252 cited

Fermionic versus Bosonic Dark Matter in Neutron Stars: A Bayesian Study with Multi-Density Constraints

Payaswinee Arvikar, Sakshi Gautam, Anagh Venneti +1

We perform a comparative Bayesian analysis of fermionic and bosonic dark matter admixed neutron stars (DMANS) by incorporating a comprehensive set of theoretical, experimental, and…

nucl-th2025

Systematic study of scalar, vector, and mixed density dependencies in relativistic mean-field descriptions of hyperonic matter in neutron stars

Aprajita Shrivastava, Prasanta Char, Sakshi Gautam +1

We investigate the equation of state (EOS) of hyperonic neutron star (NS) matter within a density-dependent relativistic mean-field (DDRMF) framework. The effects of scalar, vector…

nucl-th2025

Signatures of condensation on neutron star structure and mode frequencies

Debanjan Guha Roy, Sarmistha Banik

Antikaon () condensation within neutron star matter (NS) depends on the antikaon-nucleon interaction potential (). Appearance of generally softens the equation of s…