Strange stars ought to exist in the universe according to the strange quark matter hypothesis,
which states that matter made of roughly equal numbers of up, down, and strange quarks …

In this work, we study the neutron star phenomenology of R p attractor theories in the
Einstein frame. The Einstein frame R p attractor theories have the attractor property that they …

In this work we study static neutron stars in the context of several inflationary models which
are popular in cosmology. These inflationary models are nonminimally coupled scalar …

Recent advances in nuclear theory and new astrophysical observations have led to the
need for specific theoretical models applicable to dense-matter physics phenomena …

Within the metric formalism of f (R) theories of gravity, where R is the Ricci scalar, we study
the hydrostatic equilibrium structure of compact stars with the inclusion of anisotropic …

We investigate the Chandrasekhar mass limit of white dwarfs in various models of f (R)
gravity. Two equations of state for stellar matter are used: the simple relativistic polytropic …

We examine the Chandrasekhar limit for white dwarfs in f (R) gravity, with a simple polytropic
equation of state describing stellar matter. We use the most popular f (R) gravity model …

We study the structure of quark stars (QSs) adopting homogeneously confined matter inside
the star with a 3-flavor neutral charge and a fixed strange quark mass m s. We explore the …

Quark stars are terrestrial laboratories to study fundamental physics at ultrahigh densities
and temperatures. In this work, we investigate the internal structure and the physical …

We study the possible existence of strange matter in the interior of compact stars in Rastall
gravity. The main feature of the Rastall gravity is the covariant derivative of the energy …