Published September 2006 | Version v1
Journal article Metadata-only

Neutrino-nucleus reactions based on new shell model Hamiltonians

Creators

  • 1. Department of Physics and Center for Nuclear Study, University of Tokyo, Hongo, Bunkyo-ku, Tokyo 113-0033, Japan and RIKEN, Hirosawa, Wako-shi, Saitama 351-0198 (Japan)
  • 2. National Astronomical Observatory of Japan, Mitaka, Tokyo 181-8588, Japan and Department of Astronomy, Graduate School of Science, University of Tokyo, Bunkyo-ku, Tokyo 113-0033 (Japan)
  • 3. National Astronomical Observatory of Japan, Mitaka, Tokyo 181-8588 (Japan)
  • 4. Advanced Science Research Center, Japan Atomic Energy Agency, 2-4 Shirakata-shirane, Tokai, Naka-gun, Ibaraki 319-1195 (Japan)
  • 5. Department of Physics, College of Humanities and Sciences, Nihon University, Sakurajosui 3-25-40, Setagaya-ku, Tokyo 156-8550 (Japan)

Description

A new shell model Hamiltonian for p-shell nuclei which properly takes into account important roles of spin-isospin interactions is used to obtain cross sections of neutrino-12C reactions induced by decay-at-rest neutrinos as well as supernova neutrinos. Branching ratios to various decay channels are calculated by the Hauser-Feshbach theory. Neutrino-4He reactions are also investigated by using recent shell model Hamiltonians. The reaction cross sections are found to be enhanced for both 12C and 4He compared with previous calculations. As an interesting consequence of this, a possible enhancement of the production yields of light elements, 7Li and 11B, during supernova explosions is pointed out

Additional details

Identifiers

DOI
10.1103/PhysRevC.74.034307;
arXiv
arXiv:nucl-th/0608056v1;

Publishing Information

Journal Title
Physical Review. C, Nuclear Physics
Journal Volume
74
Journal Issue
3
Journal Page Range
p. 034307-034307.9
ISSN
0556-2813
CODEN
PRVCAN

INIS

Country of Publication
United States
Country of Input or Organization
International Atomic Energy Agency (IAEA)
INIS RN
38032349
Subject category
S73: NUCLEAR PHYSICS AND RADIATION PHYSICS;
Descriptors DEI
BORON 11; BRANCHING RATIO; CARBON 12; COSMIC NEUTRINOS; CROSS SECTIONS; HAMILTONIANS; HAUSER-FESHBACH THEORY; HELIUM 4; ISOSPIN; LITHIUM 7; NEUTRINO-NUCLEON INTERACTIONS; NUCLEAR DECAY; NUCLEAR REACTION YIELD; NUCLEOSYNTHESIS; RADIOACTIVITY; SHELL MODELS; SPIN; SUPERNOVAE
Descriptors DEC
ANGULAR MOMENTUM; BINARY STARS; BORON ISOTOPES; CARBON ISOTOPES; COSMIC RADIATION; DECAY; DIMENSIONLESS NUMBERS; ELEMENTARY PARTICLES; ERUPTIVE VARIABLE STARS; EVEN-EVEN NUCLEI; FERMIONS; HELIUM ISOTOPES; INTERACTIONS; IONIZING RADIATIONS; ISOTOPES; LEPTON-BARYON INTERACTIONS; LEPTON-HADRON INTERACTIONS; LEPTON-NUCLEON INTERACTIONS; LEPTONS; LIGHT NUCLEI; LITHIUM ISOTOPES; MASSLESS PARTICLES; MATHEMATICAL MODELS; MATHEMATICAL OPERATORS; NEUTRINOS; NUCLEAR MODELS; NUCLEAR THEORY; NUCLEI; ODD-EVEN NUCLEI; PARTICLE INTERACTIONS; PARTICLE PROPERTIES; QUANTUM OPERATORS; RADIATIONS; STABLE ISOTOPES; STARS; SYNTHESIS; VARIABLE STARS; YIELDS

Optional Information

Notes
(c) 2006 The American Physical Society