In this review article, we discuss the current status and future prospects of perturbation
theory as a means of studying the equilibrium thermodynamic and near-equilibrium …

The detection of gravitational waves originating from a neutron-star merger, GW170817, by
the LIGO and Virgo Collaborations has recently provided new stringent limits on the tidal …

At high baryon chemical potential μ B, the equation of state of QCD allows a weak-coupling
expansion in the QCD coupling α s. The result is currently known up to and including the full …

In this study, we investigate the impact of weakly interacting massive particles (WIMPs) dark
matter (DM) on C–Λ universal relations, GW170817 posterior, and radial oscillations of …

We explore constraints on the equation of state (EOS) of neutron-rich matter based on
microscopic calculations up to nuclear densities and observations of neutron stars. In a …

Radio pulsars provide some of the most important constraints for our understanding of
matter at supranuclear densities. So far, these constraints are mostly given by precision …

Continued observation of PSR J0737-3039, the double pulsar, is expected to yield a precise
determination of its primary component's moment of inertia in the next few years. Since the …

The properties of a neutron star are studied in the presence of dark matter. We have
considered a relatively light weakly interacting massive particle (WIMP) as a dark matter …

In this work, we study the impact of anisotropy on slowly rotating neutron stars by extending
the Hartle–Thorne formalism in general relativity to include anisotropy in pressure up to …

We apply the renormalization group optimized perturbation theory (RGOPT) to evaluate the
QCD (matter) pressure at the two-loop level considering three flavors of massless quarks in …