activity
20242026
most citedImplications of Fermionic Dark Matter Interactions on Anisotropic Neutron Stars

9 citations · 17 across the 9 of their papers we have counts for

collaborators

9 papers

hep-ph2026

Testing selectively enhanced QCD axions couplings as an explanation of the RX J1856.5-3754 hard X-ray excess

Charul Rathod, Madhukar Mishra, P. K Das

We explore the possibility of explaining hard X-ray data obtained from one of the Magnificent Seven (M7) neutron-stars (NSs) employing QCD axion-converted photons. The emission of…

astro-ph.CO2026

Bayesian Constraints on Inverse-Tangent Inflation with Constant-EOS Reheating and a Dynamical Reheating Analysis

Mayur Abhisheki, Prasanta Kumar Das

We perform a Bayesian inference analysis of an inflationary model based on an inverse-tangent potential, incorporating reheating dynamics in both constant and dynamical equation-of…

astro-ph.CO2026

First Constraints on the Ellipticities of Self-Interacting Fermionic Dark Matter Admixed Neutron Stars from Continuous Gravitational-Wave Searches

Premachand Mahapatra, Andrew L. Miller, Prasanta Kumar Das

We investigate continuous gravitational-wave (CW) emission from rapidly rotating, non-axisymmetric, isolated neutron stars admixed with self-interacting fermionic dark matter (DM)…

astro-ph.CO2025

Reheating and Inflationary dynamics driven by an inverse tangent potential

Mayur Abhisheki, Prasanta Kumar Das

In this work, we study the early universe inflation and the post-inflation reheating era employing an inverse tangent potential of the form $V=V_0 \cdot[tan^{-1}(\frac{κϕ}{m_p})]^2…

gr-qc2025

Structural Properties of Magnetized Neutron Stars under f (R, T ) Gravity Framework

Charul Rathod, M. Mishra, Prasanta Kumar Das

The current work investigates the structural properties of neutron stars in the presence of a strong magnetic field within the framework of f(R,T) modified gravity, where the matte…

astro-ph.HE2025★ 7 cited

Revealing Dark Matter's Role in Neutron Stars Anisotropy: A Bayesian Approach Using Multi-messenger Observations

Xue-Zhi Liu, Premachand Mahapatra, Chun Huang +3

Dark matter (DM) continues to evade direct detection, but neutron stars (NSs) serve as natural laboratories where even a modest DM component can alter their structure. While many s…

gr-qc2024

Thermal Evolution of Magnetars under f(R, T) Gravity

Charul Rathod, M. Mishra, Prasanta Kumar Das +1

The present study explores the thermal evolution and emission properties of neutron stars within the framework of modified gravity by solving the coupled energy-balance a…

astro-ph.CO2024★ 9 cited

Implications of Fermionic Dark Matter Interactions on Anisotropic Neutron Stars

Premachand Mahapatra, Chiranjeeb Singha, Ayush Hazarika +1

The presence of Dark matter (DM) within a neutron star (NS) can substantially influence the macroscopic properties. It is commonly assumed that the pressure inside an NS is isotrop…

astro-ph.CO2024★ 1 cited

Impacts of {} gravity on neutron stars study within the relativistic mean-field model framework in light of GW170817, Pulsars and NICER data

Premachand Mahapatra, Prasanta Kumar Das

In this work, we investigate the neutron star structure in conservative gravity with , where denotes the matter--geometry coupling. The modified stellar…