In recent years, machine learning has emerged as a powerful computational tool and novel
problem-solving perspective for physics, offering new avenues for studying strongly …

This review aims at providing an extensive discussion of modern constraints relevant for
dense and hot strongly interacting matter. It includes theoretical first-principle results from …

Determining the sound speed cs in compact stars is an important open question with
numerous implications on the behavior of matter at large densities and hence on …

Abstract This White Paper presents an overview of the current status and future perspective
of QCD research, based on the community inputs and scientific conclusions from the 2022 …

We have investigated the systematic differences introduced when performing a Bayesian-
inference analysis of the equation of state (EOS) of neutron stars employing either variable …

A bstract We study the rotation effects of the hot and dense QCD matter in a non-perturbative
regime by the gauge/gravity duality. We use the gravitational model that is designated to …

We investigate the neutron star (NS) equation of state (EOS) by incorporating multi-
messenger data of GW170817, PSR J0030+ 0451, PSR J0740+ 6620, and state-of-the-art …

The maximum mass of a non-rotating neutron star, M TOV, plays a very important role in
deciphering the structure and composition of neutron stars and in revealing the equation of …

A considerable effort has been dedicated recently to the construction of generic equations of
state (EOSs) for matter in neutron stars. The advantage of these approaches is that they can …

Locating the critical endpoint of QCD and the region of a first-order phase transition at finite
baryon chemical potential is an active research area for QCD matter. We provide a …