Topics
Studying how fermionic and bosonic dark matter modifies the structure, stability, and observable properties of neutron stars using a relativistic two-fluid framework. Constraints from NICER, GW170817, and PSR J0952-0607.
Modelling thermal evolution of neutron stars including superfluidity, pairing gaps, and direct URCA processes. Constraining gap parameters using observed surface temperature data and mass distributions.
Computing inspiral waveforms, f-mode and r-mode oscillation frequencies, and tidal Love numbers for dark matter admixed neutron stars. Connecting to multi-messenger observations from LIGO–Virgo–KAGRA.
Exploring the nuclear equation of state using relativistic mean-field models, symmetry energy, pressure anisotropy, pasta phases, and crustal properties. Bridging finite-nucleus physics with astrophysical observables.
Recent Articles
Research Visualizations
Key figures from published work — click arrows or indicators to browse
Mass-Radius relations for Dark Matter Admixed Neutron Stars
Cooling of Neutron Stars
Constraints on scale parameters of pairing superfluidity gaps using cooling data and mass distribution
Cooling of Dark Matter Admixed Neutron Stars
Curvature inside the Dark Matter Admixed Neutron Stars
Inspiral waveforms of Dark Matter Admixed Neutron Stars
Anisotropy inside Neutron Stars
Mass-Radius Relations for the Two-Fluid Dark Matter Model
