The strong coupling in the effective quark mass was usually taken as a constant in a
quasiparticle model while it is, in fact, running with an energy scale. With a running coupling …

This paper investigates the internal structure and equation of state (EoS) of quark stars (QS)
with pressure anisotropy, incorporating recent astrophysical observations. Utilizing …

The influence of the dark matter mass (M χ) and the Fermi momentum (k F DM) on the f 0-
mode oscillation frequency, damping time parameter, and tidal deformability of hadronic …

Within the metric formalism of $ f (R, T, L_m) $ gravity theories, we investigate the hydrostatic
equilibrium structure of compact stars taking into account both isotropic and anisotropic …

Abstract Perturbative Quantum Chromodynamics (pQCD) corrections and color
superconductivity predict that strongly interacting matter can reveal new physical …

The recent discovery of gravitational waves (GWs) has opened a new avenue for
investigating the equation of state (EOS) of dense matter in compact stars, which is an …

In this work we study, within the framework of Cowling approximation, the effect of the
electric charge on the gravitational wave frequency of fluid oscillation modes of strange …

Abstract We investigate Color Flavor Locked (CFL) Strange Stars using the most basic de
Rham–Gabadadze–Tolley massive gravity model, which explains the massive graviton in …

This study investigates the conditions under which gravitational waves (GWs) are emitted
during the merger of hot white dwarfs (WDs) in a binary system. Traditionally, these systems …

Interacting quark stars, which are entirely composed of interacting quark matter including
perturbative QCD corrections and color superconductivity, can meet constraints from various …