Numerical simulations of neutron star–neutron star and neutron star–black hole binaries
play an important role in our ability to model gravitational-wave and electromagnetic signals …

The recent experimental determination of the parity violating asymmetry A PV in Ca 48 and
Pb 208 at Jefferson Lab is important for our understanding on how neutrons and protons …

We perform a general-relativistic neutrino-radiation magnetohydrodynamic simulation of a
one second-long binary neutron star merger on the Japanese supercomputer Fugaku using …

We return to interpreting the historical SN 1987A neutrino data from a modern perspective.
To this end, we construct a suite of spherically symmetric supernova models with the …

Using numerical relativity simulations with a subgrid dynamo prescription to generate strong
initial magnetic fields, we investigate the possibility of launching a jet-like outflow from the …

In nuclear matter in isolated neutron stars, the flavor content (eg, proton fraction) is subject to
weak interactions, establishing flavor (β-) equilibrium. However, there can be deviations …

We present the second data release of gravitational waveforms from binary neutron star
(BNS) merger simulations performed by the Computational Relativity (CoRe) collaboration …

Since the release of the 2015 Long Range Plan in Nuclear Physics, major events have
occurred that reshaped our understanding of quantum chromodynamics (QCD) and nuclear …

Hot QCD physics studies the nuclear strong force under extreme temperature and densities.
Experimentally these conditions are achieved via high-energy collisions of heavy ions at the …

The concept of symmetry under various transformations of quantities describing basic
natural phenomena is one of the fundamental principles in the mathematical formulation of …