P. K. Chattopadhyay

Probing mass-radius and tidal properties of strange stars and GW190814 with the CFL phase equation of state

We propose a new class of compact star models by adopting the Durgapal IV metric potential for the temporal component g tt , together with a physically motivated anisotropic pressure distribution. To identify the conditions under which the interior matter configuration replicates...

Baryon number density dependent charged compact star admixed with dark energy: consistent with recent observational results

In this work, we investigate an anisotropic charged compact star model interpreted as a strange quark star in [Formula: see text]-equilibrium admixed with dark energy. The effects of finite strange quark mass ([Formula: see text]) and baryon number density ([Formula: see text]) a...