Published June 2011
| Version v1
Journal article
Precise and accurate determination of the 8B decay spectrum
Creators
- 1. Department of Physics and Astronomy, Aarhus University, DK-8000 Aarhus C (Denmark)
- 2. Instituto de Estructura de la Materia, CSIC, Serrano 113 bis, E-28006 Madrid (Spain)
- 3. Instituut voor Kern-en Stralingsfysica, Katholieke Universiteit Leuven, B-3001 Leuven (Belgium)
- 4. Department of Physics, University of Jyvaeskylae, FIN-40351 Jyvaeskylae (Finland)
Description
Accurate measurements of the 8B neutrino spectrum are important for the interpretation of solar neutrino data. Experimentally, the 8B neutrino spectrum can be obtained from the measurement of the β-delayed α spectrum. We report on an α-α coincidence measurement performed at the IGISOL facility in Jyvaeskylae, Finland. Our measurement allows extensive cross-checks to be performed and gives a more intense neutrino spectrum at high energies compared to the present standard. The deviation reaches 4% at the end point of the spectrum. Below 11 MeV, the deviation is less than 1%.
Additional details
Identifiers
Publishing Information
- Journal Title
- Physical Review. C, Nuclear Physics
- Journal Volume
- 83
- Journal Issue
- 6
- Journal Page Range
- p. 065802-065802.21
- ISSN
- 0556-2813
- CODEN
- PRVCAN
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 42094637
- Subject category
- S73: NUCLEAR PHYSICS AND RADIATION PHYSICS;
- Descriptors DEI
- ACCURACY; ALPHA SPECTRA; BORON 8; COINCIDENCE METHODS; MEV RANGE 01-10; NUCLEAR DECAY; SOLAR NEUTRINOS
- Descriptors DEC
- BETA DECAY RADIOISOTOPES; BETA-PLUS DECAY RADIOISOTOPES; BORON ISOTOPES; COUNTING TECHNIQUES; DECAY; ELEMENTARY PARTICLES; ENERGY RANGE; FERMIONS; ISOTOPES; LEPTONS; LIGHT NUCLEI; MASSLESS PARTICLES; MEV RANGE; MILLISECONDS LIVING RADIOISOTOPES; NEUTRINOS; NUCLEI; ODD-ODD NUCLEI; RADIATIONS; RADIOISOTOPES; SOLAR PARTICLES; SOLAR RADIATION; SPECTRA; STELLAR RADIATION
Optional Information
- Notes
- (c) 2011 American Institute of Physics