Supernova neutrinos: Flavor-dependent fluxes and spectra

Autor:	GEORG G. RAFFELT, MATHIAS TH. KEIL, ROBERT BURAS, HANS-THOMAS JANKA, MARKUS RAMPP
Rok vydání:	2003
Předmět:	Physics Accretion (meteorology) Astrophysics::High Energy Astrophysical Phenomena Monte Carlo method Astrophysics (astro-ph) Phase (waves) FOS: Physical sciences Astrophysics Solver Spectral line symbols.namesake Supernova Boltzmann constant symbols High Energy Physics::Experiment Neutrino
DOI:	10.48550/arxiv.astro-ph/0303226
Popis:	Transporting nu_mu and nu_tau in a supernova (SN) core involves several processes that have been neglected in traditional simulations. Based on a Monte Carlo study we find that the flavor-dependent spectral differences are much smaller than is often stated in the literature. A full-scale SN simulation using a Boltzmann solver and including all relevant neutrino reactions confirms these results. The flavor-dependent flux differences are largest during the initial accretion phase. Comment: Proceedings NOON 03, Kanazawa, 10-14 Feb 2003
Databáze:	OpenAIRE
Externí odkaz:	https://explore.openaire.eu/search/publication?articleId=doi_dedup___::05ce0a74fb5d00bfcaae55b1db3f0065 Zobrazit plný text záznamu