Published October 20, 2012 | Version v1
Journal article

3He+4He astrophysical factor study using activation method

Creators

  • 1. Institute of Nuclear Research (ATOMKI), H-4001 Debrecen, POB.51 (Hungary)

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

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