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 …

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 …

Neutrinos play a crucial role in the collapse and explosion of massive stars, governing the
infall dynamics of the stellar core, triggering and fueling the explosion and driving the …

No supernova (SN) in the Milky Way has been observed since the invention of the optical
telescope, instruments for other wavelengths, neutrino detectors, or gravitational wave …

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 …

We present a review of a broad selection of nuclear matter equations of state (EOSs)
applicable in core-collapse supernova studies. The large variety of nuclear matter …

We present a new series of supernova neutrino light curves and spectra calculated by
numerical simulations for a variety of progenitor stellar masses (13–50 M☉) and metallicities …

The equation of state (EoS) of hot and dense matter is a fundamental input to describe static
and dynamical properties of neutron stars, core-collapse supernovae and binary compact …

In this work we present a newly constructed equation of state (EoS), applicable to stellar
core collapse and neutron star mergers including the entire baryon octet. Our EoS is …

We provide the first comprehensive study of hyperons in neutron star mergers and quantify
their specific impact. We discuss the thermal behavior of hyperonic equations of state …