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Tidal deformation of an anisotropic neutron star
Paper link : BB + SB (2019), PRD
Information obtained from GW170817 are used to constrain the amount of pressure anisotropy inside neutron star.
Role of crustal physics in the tidal deformation of a neutron star
Paper link : Bhaskar+2019, PRD
Neutron star in a binary system is believed to have solid crust. In this publication, effect of solid crust is discussed on the emitted gvatiotational wave signal in binary neutron star merger.
Constraining neutron star equation of state
Paper link : Bhaskar+2020, arXiv
One of the key challenges of current astrophysics is to constrain neutron star (NS) equation of state (EoS). Recent observations of NS macroscopic properties by LIGO and NICER collaborations are combined under Bayesian formalism to place a joint constraint on NS EoS based on nuclear physics-informed prior knowledges.
