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 are known to play important roles in many astrophysical scenarios from the early
period of the big bang to current stellar evolution being a unique messenger of the fusion …

We investigate nuclear matter at a finite temperature and density, including the formation of
light clusters up to the α particle (1⩽ A⩽ 4). The novel feature of this work is to include the …

A statistical model for the equation of state and the composition of supernova matter is
presented. It consists of an ensemble of nuclei and interacting nucleons in nuclear statistical …

We discuss three new equations of state (EOS) in core-collapse supernova simulations. The
new EOS are based on the nuclear statistical equilibrium model of Hempel and Schaffner …

We perform state-of-the-art large-scale shell-model calculations of the structure factors for
elastic spin-dependent WIMP scattering off Xe 129, 131, I 127, Ge 73, F 19, Na 23, Al 27 …

The LIT method has allowed ab initio calculations of electroweak cross sections in light
nuclear systems. This review presents a description of the method from both a general and a …

The description of nuclear reactions induced by supernova neutrinos has witnessed
significant progress during the recent years. On one hand this progress is due to …

We generate a second equation of state (EOS) of nuclear matter for a wide range of
temperatures, densities, and proton fractions for use in supernovae, neutron star mergers …

We extend our virial approach to study the neutral-current neutrino response of nuclear
matter at low densities. In the long-wavelength limit, the virial expansion makes model …