We review the current status and recent progress of microscopic many-body approaches
and phenomenological models, which are employed to construct the equation of state of …

We review the present status of the experimental and theoretical developments in the field of
strangeness in nuclei and neutron stars. We start by discussing the K ̄ N interaction, that is …

Extensions of nuclear physics to the strange sector are reviewed, covering data and models
of Λ and other hypernuclei, multistrange matter, and antikaon bound states and …

Neutron stars are composed of the densest form of matter known to exist in our Universe, the
composition and properties of which are still theoretically uncertain. Measurements of the …

We report on the first femtoscopic measurement of baryon pairs, such as pp, p-Λ, and Λ-Λ,
measured by ALICE at the Large Hadron Collider (LHC) in proton-proton collisions at s= 7 …

We perform an O (α s 2) perturbative calculation of the equation of state of cold but dense
QCD matter with two massless and one massive quark flavor, finding that perturbation theory …

In this work we review the role of hyperons on the properties of neutron and proto-neutron
stars. In particular, we revise the so-called “hyperon puzzle”, go over some of the solutions …

With the discovery of massive neutron stars such as PSR J1614-2230, the question has
arisen of whether exotic matter such as hyperons can exist in the neutron star core. We …

We derive a new equation of state (EoS) for neutron stars (NS) from the outer crust to the
core based on modern microscopic calculations using the Argonne v 18 potential plus three …

We study the dark matter (DM) effects on the nuclear matter (NM) parameters characterizing
the equation of states of super dense neutron-rich nucleonic matter. The observables of the …