EPJ Web of Conferences
Volume 109, 2016The 13th International Symposium on Origin of Matter and Evolution of Galaxies (OMEG2015)
|Number of page(s)||7|
|Section||Theoretical Nuclear Physics for Astrophysics|
|Published online||12 February 2016|
Neutrino-induced Reactions and Neutrino Scattering with Nuclear Targets
1 Dept. of Physics, Soongsil Univ., Seoul 156-743, Korea
2 School of Liberal Arts and Science, Korea Aerospace University, Goyang 412-791, Korea
3 National Astronomical Observatory of Japan, Tokyo 181-8588, Japan and Department of Astronomy, Graduate School of Science, University of Tokyo, Hongo 7-3-1, Bunkyo-ku, Tokyo 113-0033, Japan
a e-mail: firstname.lastname@example.org
Published online: 12 February 2016
We reviewed present status regarding experimental data and theoretical approaches for neutrino-induced reactions and neutrino scattering. With a short introduction of relevant data, our recent calculations by distorted-wave Born approximation for quasielastic region are presented for MiniBooNE data. For much higher energy neutrino data, such as NOMAD data, elementary process approach was shown to be useful instead of using complicated nuclear models. But, in the low energy region, detailed nuclear structure model, such as QRPA and shell model, turn out to be inescapable to explain the reaction data. Finally, we discussed that one step-process in the reaction is comparable to the two-step process, which has been usually used in the neutrino-nucleosynthesis.
© Owned by the authors, published by EDP Sciences, 2016
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