Supernova theory, numerical and analytic, has made remarkable progress in the past
decade. This progress was made possible by more sophisticated simulation tools, especially …

We investigate how current and proposed observations of neutron stars can lead to an
understanding of the state of their interiors and the key unknowns: the typical neutron star …

Many of the currently available equations of state for core-collapse supernova simulations
give large neutron star radii and do not provide large enough neutron star masses, both of …

Advances in our understanding and the modeling of stellar core-collapse and supernova
explosions over the past 15 years are reviewed, concentrating on the evolution of …

This paper presents a detailed assessment of the ability of the 240 Skyrme interaction
parameter sets in the literature to satisfy a series of criteria derived from macroscopic …

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 …

Recent experimental data and progress in nuclear structure modeling have led to improved
descriptions of astrophysically important weak-interaction processes. This review discusses …

An 8.8 M⊙ electron-capture supernova was simulated in spherical symmetry consistently
from collapse through explosion to essentially complete deleptonization of the forming …

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 …

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 …