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 …

Despite their long history and astrophysical importance, some of the key properties of
neutron stars are still uncertain. The extreme conditions encountered in their interiors …

We report a precision measurement of the parity-violating asymmetry A PV in the elastic
scattering of longitudinally polarized electrons from Pb 208. We measure A PV= 550±16 …

Laboratory experiments sensitive to the equation of state of neutron rich matter in the vicinity
of nuclear saturation density provide the first rung in a “density ladder” that connects …

The historical first detection of a binary neutron star merger by the LIGO-Virgo Collaboration
[BP Abbott et al., Phys. Rev. Lett. 119, 161101 (2017) PRLTAO 0031-9007 …

In this article, I introduce ideas and techniques to extract information about the equation of
state of matter at very high densities from gravitational waves emitted before, during and …

This contribution reviews the present status on the available constraints to the nuclear
equation of state (EoS) around saturation density from nuclear structure calculations on …

The cross section for coherent elastic neutrino-nucleus scattering (CE ν NS) depends on the
response of the target nucleus to the external current, in the Standard Model (SM) mediated …

Background: Theoretical approaches based on density functional theory provide the only
tractable method to incorporate the wide range of densities and isospin asymmetries …

The symmetry energy describes how the energy of nuclear matter rises as one goes away
from equal numbers of neutrons and protons. This is very important to describe neutron rich …