Neutrino-nucleus reactions in the energy range 1-100 MeV
arXiv:nucl-th/0601068 · doi:10.1016/j.nuclphysbps.2006.08.023
Abstract
We review some salient aspects of calculations of the neutrino-nucleus reaction cross sections in the low energy range (1-100 MeV).
arXiv comment6 pages:Invited talk at NuInt05 (Fourth International Workshop on Neutrino- Nucleus Interactions in the Few-GeV Region), Okayama, Japan. September 26 - 29, 2005, ver2 corrected typos and references
References in corpus (25)
- An accurate nucleon-nucleon potential with charge-independence breaking
- Measurement of the rate of nu_e + d --> p + p + e^- interactions produced by 8B solar neutrinos at the Sudbury Neutrino Observatory
- The high-precision, charge-dependent Bonn nucleon-nucleon potential (CD-Bonn)
- Nucleon-Nucleon Scattering from Effective Field Theory
- Evolution of Nuclear Spectra with Nuclear Forces
- Ab initio shell model with a genuine three-nucleon force for the p-shell nuclei
- Structure of Light Unstable Nuclei Studied with Antisymmetrized Molecular Dynamics
- Parameter-free effective field theory calculation for the solar proton-fusion and hep processes
- Neutrino-Deuteron Scattering in Effective Field Theory at Next-to-Next-to Leading Order
- Neutrino Reactions on Deuteron
- Supernova Inelastic Neutrino-Nucleus Cross Sections from High-Resolution Electron Scattering Experiments and Shell-Model Calculations
- Neutrino-Nucleus Reactions
- Neutrino-deuteron reactions at solar neutrino energies
- Weak proton capture on 3He
- Measurements of Charged Current Reactions of muon neutrinos on C12
- Elastic and Inelastic Neutrino-Deuteron Scattering in Effective Field Theory
- The Solar Proton Burning Process Revisited In Chiral Perturbation Theory
- Neutrino-12C scattering in the ab initio shell model with a realistic three-body interaction
- Realistic Calculation of the hep Astrophysical Factor
- The capture rate in effective field theory
- Solar-neutrino reactions on deuteron in effective field theory
- Quasielastic neutrino scattering from oxygen and the atmospheric neutrino problem
- Effective Field Theory For Nuclei: Confronting Fundamental Questions in Astrophysics
- Tests of the random phase approximation for transition strengths
- RPA puzzle in C(12) weak decay processes