The dominant neutrino fluxes at Earth from different sources are reviewed and the grand
unified neutrino spectrum ranging from meV to PeV energies is presented. For each energy …

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–matter cross sections and interaction rates are central to the core-collapse
supernova phenomenon and, very likely, to the viability of the explosion mechanism itself. In …

Previous work on neutrino emission from proto-neutron stars which employed full solutions
of the Boltzmann equation showed that the average energies of emitted electron neutrinos …

Understanding signals from neutron stars requires knowledge about the transport inside the
star. We review the transport properties and the underlying reaction rates of dense hadronic …

Supernova neutrino–nucleus astrophysics Page 1 Journal of Physics G: Nuclear and Particle
Physics Supernova neutrino–nucleus astrophysics To cite this article: AB Balantekin and GM …

A simple description of core-collapse supernovae is given. Properties of the neutrino-driven
wind, neutrino fluxes and luminosities, reaction rates and the equilibrium electron fraction in …

The steady advance in core-collapse supernova simulations requires a more precise
description of neutrino processes in hot and dense matter. In this work, we study the rates of …

We derive the charged current absorption rate of electron and antielectron neutrinos in
dense matter using a fully relativistic approach valid at arbitrary matter degeneracy. We …

ABSTRACT A new code for following the evolution and emissions of proto-neutron stars
during the first minute of their lives is developed and tested. The code is one dimensional …