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 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 numerical results on two-(2D) and three-dimensional (3D) hydrodynamic core-
collapse simulations of an 11.2 M☉ star. By changing numerical resolutions and seed …

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 …

The formation of α-particle clusters on the surface of heavy nuclei is described in a
generalized relativistic mean-field model with explicit cluster degrees of freedom. The effects …

We have constructed a nuclear equation of state (EOS) that includes a full nuclear ensemble
for use in core-collapse supernova simulations. It is based on the EOS for uniform nuclear …

The modification of the ground state properties of light atomic nuclei in the nuclear and
stellar medium is addressed, using chemical equilibrium constants evaluated from a new …

Herein, we review the nuclear equations of state (EOSs) and the constituent nuclei of core-
collapse supernovae (CCSNe) and their roles in CCSN simulations. Various nuclei such as …

We perform an extensive study of the influence of nuclear weak interactions on core-
collapse supernovae, paying particular attention to consistency between nuclear …

We present a newly developed moving-mesh technique for the multi-dimensional Boltzmann-
Hydro code for the simulation of core-collapse supernovae (CCSNe). What makes this …