The nuclear equation of state (EOS) is at the center of numerous theoretical and
experimental efforts in nuclear physics. With advances in microscopic theories for nuclear …

The density dependence of nuclear symmetry energy is among the most uncertain parts of
the Equation of State (EOS) of dense neutron-rich nuclear matter. It is currently poorly known …

We demonstrate in a general and analytic way how high-density information about the
equation of state (EOS) of strongly interacting matter obtained using perturbative quantum …

Determining the Equation of State (EOS) of dense neutron-rich nuclear matter is a shared
goal of both nuclear physics and astrophysics. Except possible phase transitions, the density …

Various kinds of isovector nucleon effective masses are used in the literature to characterize
the momentum/energy dependence of the nucleon symmetry potential or self-energy due to …

By numerically inverting the Tolman-Oppenheimer-Volkov (TOV) equation using an explicitly
isospin-dependent parametric Equation of State (EOS) of dense neutron-rich nucleonic …

In this paper, we consider a spherical symmetric metric to extract the hydrostatic equilibrium
equation of stars in (3+ 1)-dimensional gravity's rainbow in the presence of cosmological …

Using as references the posterior probability distribution functions of the equation of state
(EOS) parameters inferred from the radii of canonical neutron stars (NSs) reported by the …

Deviations from the predictions of general relativity due to energy-momentum squared
gravity (EMSG) are expected to become pronounced in the high density cores of neutron …

Motivated by the recent interests in spin− 2 massive gravitons, we study the structure of
neutron star in the context of massive gravity. The modifications of TOV equation in the …