The nuclear equation of state (EOS) is at the center of numerous theoretical and
experimental efforts in nuclear physics. With advances in microscopic theories for nuclear …

Transport models are the main method to obtain physics information on the nuclear equation
of state and in-medium properties of particles from low to relativistic-energy heavy-ion …

We have conducted 19 state-of-the-art 3D core-collapse supernova simulations spanning a
broad range of progenitor masses. This is the largest collection of sophisticated 3D …

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 …

Neutrino flavor instabilities have the potential to shuffle neutrinos between electron, mu, and
tau flavor states, possibly modifying the core-collapse supernova mechanism and the heavy …

In this paper, we present the results of our three-dimensional, multigroup, multineutrino-
species radiation/hydrodynamic simulation using the state-of-the-art code fornax of the …

Neutrino masses and mixings produce vacuum oscillations, an established quantum
mechanical phenomenon. In matter, the Mikheev-Smirnov-Wolfenstein effect, due to …

Most supernova explosions accompany the death of a massive star. These explosions give
birth to neutron stars and black holes, and eject solar masses of heavy elements. However …

We performed a detailed analysis of the detectability of a wide range of gravitational waves
derived from core-collapse supernova simulations using gravitational-wave detector noise …

A century ago, nuclear physics entered astrophysics, giving birth to a new field of science
referred to as “Nuclear Astrophysics”. With time, it developed at an impressive pace into a …