Emission of neutrino-antineutrino pairs by hadronic bremsstrahlung processes

Abstract

We review our recent calculations of neutrino-antineutrino pair production from bremsstrahlung processes in hadronic collisions at temperature and densities relevant for core-collapse supernovae. We focus on neutron-neutron and neutron-alpha collisions.

8 pages, 4 figures, proceedings of the NN2015 conference, Catania, 21-26 June, 2015

References in corpus (7)

• Explosion Mechanisms of Core-Collapse Supernovae
• Theory of Core-Collapse Supernovae
• Perspectives on Core-Collapse Supernova Theory
• Influence of light nuclei on neutrino-driven supernova outflows
• Chiral effective field theory calculations of neutrino processes in dense matter
• Supernova matter at subnuclear densities as a resonant Fermi gas: Enhancement of neutrino rates
• Neutrino-pair bremsstrahlung from nucleon-$\alpha$ versus nucleon-nucleon scattering

Cited by in corpus (1)

• Supernovae and Weinberg's Higgs Portal Dark Radiation and Dark Matter