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 physics of hyperons and Δ-resonances in dense matter in compact stars. The
covariant density functional approach to the equation of state and composition of dense …

Nuclear matter and finite nuclei exhibit the property of superfluidity by forming Cooper pairs.
We review the microscopic theories and methods that are being employed to understand 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 …

We develop new hyperon equation of state (EoS) tables for core-collapse supernova
simulations and neutron stars. These EoS tables are based on a density-dependent …

The explosion of core-collapse supernova depends on a sequence of events taking place in
less than a second in a region of a few hundred kilometers at the centre of a supergiant star …

Since the discovery of neutron stars with masses around $2\;{{M} _ {\odot}} $ the
composition of matter in the central part of these massive stars has been intensively …

Employing recently proposed metamodeling for the nucleonic matter equation of state, we
analyze neutron star global properties such as masses, radii, momentum of inertia, and …

We use covariant density functional theory to obtain the equation of state (EoS) of matter in
compact stars at non-zero temperature, including the full baryon octet as well as the Δ …