Neutrino-nuclear response and photonuclear reactions

H. Ejiri, A. I. Titov, M. Boswell, and A. Young
Phys. Rev. C 88, 054610 – Published 18 November 2013

Abstract

Photonuclear reactions are shown to be used for studying neutrino (weak) nuclear responses involved in astroneutrino nuclear interactions and double beta decays. Charged current weak responses for ground and excited states are studied by using photonuclear reactions through isobaric analog states of those states, while neutral current weak responses for excited states are studied by using photonuclear reactions through the excited states. The weak interaction strengths are studied by measuring the cross sections of the photonuclear reactions, and the spin and parity of the states are studied by measuring angular correlations of particles emitted from the photonuclear reactions. Medium-energy polarized photons obtained from laser photons scattered off GeV electrons are very useful. Nuclear responses studied by photonuclear reactions are used to evaluate neutrino (weak) nuclear responses, i.e., nuclear beta and double beta matrix elements and neutrino-nuclear interactions, and to verify theoretical calculations for them.

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  • Received 26 March 2013

DOI:https://doi.org/10.1103/PhysRevC.88.054610

©2013 American Physical Society

Authors & Affiliations

H. Ejiri*

  • Research Center for Nuclear Physics, Osaka University, Ibaraki, Osaka 567-0047, Japan and Nuclear Science, Czech Technical University, Prague, Czech Republic

A. I. Titov

  • Joint Institute of Nuclear Research, 141980 Dubna, Russia

M. Boswell

  • Los Alamos National Laboratory, Los Alamos, New Mexico, USA

A. Young

  • Department of Physics, North Carolina State University, Raleigh, North Carolina, USA

  • *ejiri@rcnp.osaka-u.ac.jp

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Vol. 88, Iss. 5 — November 2013

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