The importance of neutrino opacities for the accretion luminosity in spherically symmetric supernova models

2002/03/15 by M. Liebendoerfer, Liebendoerfer, M., Bronson Messer +12 · 1 citation
Physics and Astronomy · #Astrophysics (astro-ph) #FOS: Physical sciences #Gamma-ray bursts and supernovae #Neutrino Physics Research #Particle physics theoretical and experimental studies #astro-ph

paper · pdf · doi:10.48550/arxiv.astro-ph/0203260

4 pages, 3 figures, to appear in W. Hillebrandt and E. Mueller, eds., Proceedings of the 11th Workshop on "Nuclear Astrophysics" held at Rinberg Castle, February 11-16, 2002

arxiv created 2002/03/15 · openalex publication_date 2002/03/15 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28

Abstract

Based on general relativistic three-flavor Boltzmann neutrino transport, we compare simulations of the postbounce evolution for five different stellar progenitors with 13 and 20 solar masses (Nomoto & Hashimoto '88), and 15, 25, and 40 solar masses (Woosley & Weaver '95).

Cited by

• Exploiting the neutronization burst of a galactic supernova

Related

• Neutrino-driven supernovae: Boltzmann neutrino transport and the explosion mechanism
• Solar and Supernova Constraints on Cosmologically Interesting Neutrinos
• Neutrino refractive effects during their decoupling era in the early universe
• Long-term evolution of massive star explosions
• Old Data, New Forensics: The First Second of SN 1987A Neutrino Emission