3He+4He astrophysical factor study using activation method
Description
In 1998, [2] pointed out the big difference for the S34(0) ('old' experimental data) when experimental results were grouped starting from the main two methods: S34(0) = 0.507(16)keVb for the direct capture and S34(0) = 0.572(26)keVb for the activation. Its importance for the Standard Solar Model was the reason to ask for new measurements to understand the discrepancy. 'New' results solved this issue by equalizing the above values, but introduced a new situation to clarify: a discrepancy between the S34(E) variations for 'old' and 'new' data at higher energies than ECM 1.0MeV. 'Old' theoretical models, used for extrapolating the S34(E) to the stellar energies, couldn't explain this new behavior. New experimental data was required, again, by theorists. We started this project with the main goal to clarify the situation. Here are the results.
Additional details
Identifiers
- DOI
- 10.1063/1.4764257;
Publishing Information
- Journal Title
- AIP Conference Proceedings
- Journal Volume
- 1491
- Journal Issue
- 1
- Journal Page Range
- p. 281-284
- ISSN
- 0094-243X
- CODEN
- APCPCS
Conference
- Title
- Conference on nuclear structure and dynamics 2012
- Dates
- 9-13 Jul 2012
- Place
- Opatija (Croatia)
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 44034709
- Subject category
- S73: NUCLEAR PHYSICS AND RADIATION PHYSICS; S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- ASTROPHYSICS; CAPTURE; ENERGY-LEVEL TRANSITIONS; HELIUM 3; HELIUM 4; MASS NUMBER; SPECTROSCOPIC FACTORS; STAR MODELS; VARIATIONS
- Descriptors DEC
- DIMENSIONLESS NUMBERS; EVEN-EVEN NUCLEI; EVEN-ODD NUCLEI; HELIUM ISOTOPES; ISOTOPES; LIGHT NUCLEI; MATHEMATICAL MODELS; NUCLEI; PHYSICS; STABLE ISOTOPES
Optional Information
- Notes
- (c) 2012 American Institute of Physics