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 …

A review is given of various theoretical approaches for the equation of state (EoS) of dense
matter, relevant for the description of core-collapse supernovae, compact stars, and compact …

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 …

With the first observation of a binary neutron star merger through gravitational waves and
light, GW170817, compact binary mergers have now taken the center stage in nuclear …

The onset of hyperons in the core of neutron stars and the consequent softening of the
equation of state have been questioned for a long time. Controversial theoretical predictions …

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 …

Results for the ΛN and ΣN interactions obtained at next-to-leading order in chiral effective
field theory are reported. At the order considered there are contributions from one-and two …

We discuss the formation of Δ isobars in neutron star matter. We show that their threshold
density strictly correlates with the density derivative of the symmetry energy of nuclear …

The recent measurement of a 1.97±0.04 solar-mass pulsar places a stringent lower bound
on the maximum mass of compact stars and therefore challenges the existence of any …