Exploring the extreme physics of compact objects
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.