Determination of the 3He(α, γ)7Be and 6Li(p, γ)7Be astrophysical factors down to zero energy using the asymptotic normalization coefficients
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F61389005%3A_____%2F23%3A00572943" target="_blank" >RIV/61389005:_____/23:00572943 - isvavai.cz</a>
Result on the web
<a href="https://doi.org/10.1051/epjconf/202327911001" target="_blank" >https://doi.org/10.1051/epjconf/202327911001</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1051/epjconf/202327911001" target="_blank" >10.1051/epjconf/202327911001</a>
Alternative languages
Result language
angličtina
Original language name
Determination of the 3He(α, γ)7Be and 6Li(p, γ)7Be astrophysical factors down to zero energy using the asymptotic normalization coefficients
Original language description
The p - p-chain reaction He-3(alpha, gamma)Be-7 can sensitively influence the prediction of the Be-7 and B-8 neutrino fluxes. Despite its importance, the knowledge of its reaction cross section at energies of the core of the Sun (15 keV - 30 keV) is limited and the accuracy far from the desired similar to 3% level. In the present paper the indirect measurement of the external capture contribution using the asymptotic normalization coefficient (ANC) technique is reported. The angular distributions of deuterons emitted in the Li-6(He-3,d)Be-7 alpha-transfer reactions were measured and the ANCs extracted from the scaling of distorted-wave Born approximation (DWBA) and coupled-channel (CC) calculations. Then, the astrophysical S-factor for the He-3(alpha, gamma)Be-7 reaction was calculated assuming E1 direct capture and the zero energy value turned out to be 0.534 +/- 0.025 keVb. Both our experimental and theoretical approaches were benchmarked through the analysis of the Li-6(p,gamma)Be-7 astrophysical factor, with interesting astrophysical applications to the understanding of the primordial lithium problem. In particular, the present work disfavors the occurrence of a claimed 200 keV resonance in the astrophysical factor.
Czech name
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Czech description
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Classification
Type
D - Article in proceedings
CEP classification
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OECD FORD branch
10308 - Astronomy (including astrophysics,space science)
Result continuities
Project
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Continuities
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace
Others
Publication year
2023
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Data specific for result type
Article name in the collection
EPJ Web of Confereneces
ISBN
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ISSN
2100-014X
e-ISSN
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Number of pages
6
Pages from-to
11001
Publisher name
edp sciences
Place of publication
Les Ulis
Event location
Geneva
Event date
Sep 5, 2022
Type of event by nationality
WRD - Celosvětová akce
UT code for WoS article
000995956500032