Constraints on the appearance of a maximum in astrophysical S-factor

For fusion reactions of astrophysical interest, the existence of a maximum of S-factor is revealed within the extended quantum diffusion approach. The available experimental data are well described. The reason and consequences of the existence of the S-factor maximum are explained. An universal form...

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Autores principales: V.V. Sargsyan, G.G. Adamian, N.V. Antonenko, H. Lenske
Formato: article
Lenguaje:EN
Publicado: Elsevier 2022
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Acceso en línea:https://doaj.org/article/b10def46323b4589b7919d90d2dd6f19
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spelling oai:doaj.org-article:b10def46323b4589b7919d90d2dd6f192021-11-30T04:13:39ZConstraints on the appearance of a maximum in astrophysical S-factor0370-269310.1016/j.physletb.2021.136792https://doaj.org/article/b10def46323b4589b7919d90d2dd6f192022-01-01T00:00:00Zhttp://www.sciencedirect.com/science/article/pii/S0370269321007322https://doaj.org/toc/0370-2693For fusion reactions of astrophysical interest, the existence of a maximum of S-factor is revealed within the extended quantum diffusion approach. The available experimental data are well described. The reason and consequences of the existence of the S-factor maximum are explained. An universal formula for the position of the maximum is proposed.V.V. SargsyanG.G. AdamianN.V. AntonenkoH. LenskeElsevierarticleAstrophysical S-factorDeep sub-barrier fusion (capture)Dissipative dynamicsPhysicsQC1-999ENPhysics Letters B, Vol 824, Iss , Pp 136792- (2022)
institution DOAJ
collection DOAJ
language EN
topic Astrophysical S-factor
Deep sub-barrier fusion (capture)
Dissipative dynamics
Physics
QC1-999
spellingShingle Astrophysical S-factor
Deep sub-barrier fusion (capture)
Dissipative dynamics
Physics
QC1-999
V.V. Sargsyan
G.G. Adamian
N.V. Antonenko
H. Lenske
Constraints on the appearance of a maximum in astrophysical S-factor
description For fusion reactions of astrophysical interest, the existence of a maximum of S-factor is revealed within the extended quantum diffusion approach. The available experimental data are well described. The reason and consequences of the existence of the S-factor maximum are explained. An universal formula for the position of the maximum is proposed.
format article
author V.V. Sargsyan
G.G. Adamian
N.V. Antonenko
H. Lenske
author_facet V.V. Sargsyan
G.G. Adamian
N.V. Antonenko
H. Lenske
author_sort V.V. Sargsyan
title Constraints on the appearance of a maximum in astrophysical S-factor
title_short Constraints on the appearance of a maximum in astrophysical S-factor
title_full Constraints on the appearance of a maximum in astrophysical S-factor
title_fullStr Constraints on the appearance of a maximum in astrophysical S-factor
title_full_unstemmed Constraints on the appearance of a maximum in astrophysical S-factor
title_sort constraints on the appearance of a maximum in astrophysical s-factor
publisher Elsevier
publishDate 2022
url https://doaj.org/article/b10def46323b4589b7919d90d2dd6f19
work_keys_str_mv AT vvsargsyan constraintsontheappearanceofamaximuminastrophysicalsfactor
AT ggadamian constraintsontheappearanceofamaximuminastrophysicalsfactor
AT nvantonenko constraintsontheappearanceofamaximuminastrophysicalsfactor
AT hlenske constraintsontheappearanceofamaximuminastrophysicalsfactor
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