In this review article, we describe the role of holography in deciphering the physics of dense
QCD matter, relevant for the description of compact stars and their binary mergers. We …

In the present work, we investigate the image of a power-Yang-Mills black hole and its
luminosity under distinctive accretion models. Meanwhile, a special emphasis is put on the …

We present a novel framework for the equation of state of dense and hot quantum
chromodynamics (QCD), which focuses on the region of the phase diagram relevant for …

I review holographic models for (dense and cold) nuclear matter, neutron stars, and their
mergers. I start by a brief general discussion on current knowledge of cold QCD matter and …

Abstract Using full 3+ 1 dimensional general-relativistic hydrodynamic simulations of equal-
and unequal-mass neutron-star binaries with properties that are consistent with those …

We establish a holographic bottom-up model which covers both the baryonic and quark
matter phases in cold and dense QCD. This is obtained by including the baryons using …

We employ the recently improved description of dense baryonic matter within the Witten-
Sakai-Sugimoto model to construct neutron stars. In contrast to previous holographic …

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 …

Ab initio methods using weakly interacting nucleons give a good description of condensed
nuclear matter up to densities comparable to the nuclear saturation density. At higher …

We use the holographic V-QCD models to analyse the physics of dense QCD and neutron
stars. Accommodating lattice results for thermodynamics of QCD enables us to make generic …