Astrophysical S factors determined from asymptotic normalization coefficients measured in peripheral transfer reactions.

Result code in IS VaVaI
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Result on the web
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DOI - Digital Object Identifier
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Result language
angličtina
Original language name
Astrophysical S factors determined from asymptotic normalization coefficients measured in peripheral transfer reactions.
Original language description
Peripheral transfer reactions can be used to determine asymptotic normalization coefficients (ANC). These coefficients, which specify the normalization of the tail of the overlap function, determine astrophysical S factors for direct capture reactions atstellar energies. This technique is particularly suited for use with radioactive beams. The .sup.10 B(.sup.7 Be,.sup.8 B).sup.9 Be and .sup.14 N(.sup. 7 Be,.sup.8 B).sup.13 C reactions have been used to measure the ANC appropriate for determining the .sup.7 Be(p,.tau.) .sup.8 B rate, and the .sup.14 N(.sup.11 C,.sup.12 N).sup.13 C reaction has been used to measure the ANC required tocalculate the .sup.11 C(p,.tau.).sup.12 N rate.
Czech name
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Czech description
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Type
J<sub>x</sub> - Unclassified - Peer-reviewed scientific article (Jimp, Jsc and Jost)
CEP classification
BG - Nuclear, atomic and molecular physics, accelerators
OECD FORD branch
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Project
Result was created during the realization of more than one project. More information in the Projects tab.
Continuities
P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)

Publication year
2001
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

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