Effects of nuclear molecular configurations on the astrophysical S-factor for $^{16}$O + $^{16}$O

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dc.creatorDiaz-Torres, A.
dc.creatorGasques, L. R.
dc.creatorWiescher, M.
dc.date2007-08-17
dc.date.accessioned2026-07-07T10:36:22Z
dc.date.available2026-07-07T10:36:22Z
dc.descriptionThe impact of nuclear molecular configurations on the astrophysical S-factor for $^{16}$O + $^{16}$O is investigated within the realistic two-center shell model based on Woods-Saxon potentials. These molecular effects refer to the formation of a neck between the interacting nuclei and the radial dependent collective mass parameter. It is demonstrated that the former is crucial to explain the current experimental data with high accuracy and without any free parameter, whilst in addition the latter predicts a pronounced maximum in the S-factor. In contrast to very recent results by Jiang et al., the S-factor does not decline towards extremely low values as energy decreases.
dc.descriptionIn press in Physics Letters B
dc.identifierhttps://arxiv.org/abs/0708.2317
dc.identifierhttp://arxiv.org/abs/0708.2317
dc.identifierPhys.Lett.B652:255-258,2007
dc.identifierdoi:10.1016/j.physletb.2007.06.077
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/180025
dc.subjectNuclear Theory
dc.titleEffects of nuclear molecular configurations on the astrophysical S-factor for $^{16}$O + $^{16}$O
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