Successful Prediction of Total α -Induced Reaction Cross Sections at Astrophysically Relevant Sub-Coulomb Energies Using a Novel Approach

The prediction of stellar ( γ , α ) reaction rates for heavy nuclei is based on the calculation of ( α , γ ) cross sections at sub-Coulomb energies. These rates are essential for modeling the nucleosynthesis of so-called p nuclei. The standard calculations in the statistical model show a dramatic se...

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Veröffentlicht in:	Physical review letters 2020-06, Vol.124 (25), p.1-252701, Article 252701
Hauptverfasser:	Mohr, P., Fülöp, Zs, Gyürky, Gy, Kiss, G. G., Szücs, T.
Format:	Artikel
Sprache:	eng
Schlagworte:	Cross-sections Heavy nuclei Low temperature Nuclear fusion Parameter uncertainty Sensitivity Statistical models
Online-Zugang:	Volltext
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