Effects of inelastic neutrino-nucleus scattering on supernova dynamics and radiated neutrino spectra

Based on the shell model for Gamow-Teller and the random phase approximation for forbidden transitions, we calculate cross sections for inelastic neutrino-nucleus scattering (INNS) under supernova (SN) conditions, assuming a matter composition given by nuclear statistical equilibrium. The cross sect...

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Veröffentlicht in:Physical review letters 2008-01, Vol.100 (1), p.011101-011101, Article 011101
Hauptverfasser: Langanke, K, Martínez-Pinedo, G, Müller, B, Janka, H-Th, Marek, A, Hix, W R, Juodagalvis, A, Sampaio, J M
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container_end_page 011101
container_issue 1
container_start_page 011101
container_title Physical review letters
container_volume 100
creator Langanke, K
Martínez-Pinedo, G
Müller, B
Janka, H-Th
Marek, A
Hix, W R
Juodagalvis, A
Sampaio, J M
description Based on the shell model for Gamow-Teller and the random phase approximation for forbidden transitions, we calculate cross sections for inelastic neutrino-nucleus scattering (INNS) under supernova (SN) conditions, assuming a matter composition given by nuclear statistical equilibrium. The cross sections are incorporated into state-of-the-art stellar core-collapse simulations with detailed energy-dependent neutrino transport. While no significant effect on the SN dynamics is observed, INNS increases the neutrino opacities noticeably and strongly reduces the high-energy tail of the neutrino spectrum emitted in the neutrino burst at shock breakout. Relatedly the expected event rates for the observation of such neutrinos by earthbound detectors are reduced by up to about 60%.
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subjects CROSS SECTIONS
EMISSION SPECTRA
ENERGY DEPENDENCE
FORBIDDEN TRANSITIONS
GAMOW-TELLER RULES
INELASTIC SCATTERING
NEUTRINO-NUCLEON INTERACTIONS
NEUTRINOS
PHYSICS OF ELEMENTARY PARTICLES AND FIELDS
RANDOM PHASE APPROXIMATION
SHELL MODELS
SIMULATION
SUPERNOVAE
title Effects of inelastic neutrino-nucleus scattering on supernova dynamics and radiated neutrino spectra
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