Abstract
Background: Accurate knowledge of the reaction cross section is important for the understanding of the process in asymptotic giant branch stars, since it is considered to be the main source of neutrons. The subthreshold state at excitation energy of 6.356 MeV in has a strong influence on the reaction cross section at energies relevant for astrophysics. Several experiments have been performed to determine the contribution of this state to the reaction rate. Nevertheless, significant discrepancies between different measurements remain.
Purpose: The aim of this work is to investigate these discrepancies.
Method: An 8 MeV beam (below the Coulomb barrier) was used to study the -transfer reaction .
Results: The squared Coulomb-modified asymptotic normalization coefficient of the state in measured in this work is .
Conclusions: Discrepancy between the results of -transfer experiments have been resolved. However, some discrepancy with the most recent measurement using the Trojan Horse method remains.
- Received 22 January 2015
DOI:https://doi.org/10.1103/PhysRevC.91.048801
©2015 American Physical Society