Abstract
The extrapolations of cross sections for fusion reactions involving and nuclei down to energies relevant for explosive stellar burning have been reexamined. Based on a systematic study of fusion in heavier systems, it is expected that a suppression of the fusion process will also be present in these light heavy-ion systems at extreme sub-barrier energies due to the saturation properties of nuclear matter. Previous phenomenological extrapolations of the factor for light heavy-ion fusion based on optical model calculations may therefore have overestimated the corresponding reaction rates. A new “recipe” is proposed to extrapolate factors for light heavy-ion reactions to low energies taking the hindrance behavior into account. It is based on a fit to the logarithmic derivative of the experimental cross section which is much less sensitive to overall normalization discrepancies between different data sets than other approaches. This method, therefore, represents a significant improvement over other extrapolations. The impact on the astrophysical reaction rates is discussed.
5 More- Received 6 October 2006
DOI:https://doi.org/10.1103/PhysRevC.75.015803
©2007 American Physical Society