E Kolbe et al 2003 J. Phys. G: Nucl. Part. Phys. 29 2569 doi:10.1088/0954-3899/29/11/010
E Kolbe1, K Langanke2, G Martínez-Pinedo3,4 and P Vogel5
Show affiliationsThe 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.
25.30.Pt Neutrino-induced reactions
26.30.-k Nucleosynthesis in novae, supernovae, and other explosive environments
96.60.Vg Particle emission, solar wind
26.50.+x Nuclear physics aspects of novae, supernovae, and other explosive environments
Issue 11 (November 2003)
Received 22 August 2003
Published 14 October 2003
E Kolbe et al 2003 J. Phys. G: Nucl. Part. Phys. 29 2569
G Contopoulos et al 2003 J. Phys. A: Math. Gen. 36 8639
M H Annaby and Z S Mansour 2005 J. Phys. A: Math. Gen. 38 3775
Ilya Avdeev et al 2004 J. Micromech. Microeng. 14 1491
Alan B. Whiting et al. 2007 The Astronomical Journal 133 715
J Hlinka et al 2003 J. Phys.: Condens. Matter 15 4249
Markus A Cirone et al 2001 J. Phys. B: At. Mol. Opt. Phys. 34 4571
I Aref'eva, D J Fernández, V Hussin, J Negro, L M Nieto and B F Samsonov 2004 J. Phys. A: Math. Gen. 37
Holly K Gibbs et al 2008 Environ. Res. Lett. 3 034001
D A Wisniacki et al 2007 J. Phys. A: Math. Theor. 40 14353