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Neutrino–nucleus reactions and nuclear structure

Kolbe, E. and Langanke, K. and Martínez-Pinedo, G. and Vogel, P. (2003) Neutrino–nucleus reactions and nuclear structure. Journal of Physics G: Nuclear and Particle Physics, 29 (11). pp. 2569-2596. ISSN 0954-3899. https://resolver.caltech.edu/CaltechAUTHORS:KOLjpg03

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Abstract

The methods used in the evaluation of the neutrino–nucleus cross section are reviewed. Results are shown for a variety of targets of practical importance. Many of the described reactions are accessible in future experiments with neutrino sources from the pion and muon decays at rest, which might be available at the neutron spallation facilities. Detailed comparison between the experimental and theoretical results would establish benchmarks needed for verification and/or parameter adjustment of the nuclear models. Having a reliable tool for such calculation is of great importance in a variety of applications, e.g. the neutrino oscillation studies, detection of supernova neutrinos, description of the neutrino transport in supernovae and description of the r-process nucleosynthesis.


Item Type:Article
Related URLs:
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http://stacks.iop.org/0954-3899/29/2569OtherUNSPECIFIED
ORCID:
AuthorORCID
Vogel, P.0000-0003-0587-5466
Additional Information:© 2003 IOP Publishing Ltd. Received 22 August 2003. Published 14 October 2003. Print publication: Issue 11 (November 2003). The work of PV was supported in part by the US DOE and by the Institute of Physics and Astronomy at the University of A°rhus. KL is partially supported by the Danish Research Foundation. GMP is supported by the Spanish MCyT under contracts AYA2002-04094-C03-02 and AYA2003-06128.
Issue or Number:11
Record Number:CaltechAUTHORS:KOLjpg03
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:KOLjpg03
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:389
Collection:CaltechAUTHORS
Deposited By: Archive Administrator
Deposited On:08 Jun 2005
Last Modified:12 Jul 2022 19:49

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