Abstract
Background: The reaction has been used as an indirect method to calculate the astrophysical factor for the ( reaction at Gamow energy (300 keV).
Purpose: The reaction is usually interpreted in terms of direct transfer. In this work we investigate the reaction mechanism and determine the effects of breakup on transfer and therefore on the extracted spectroscopic amplitudes.
Method: The deuteron angular distributions for the has been measured at 20 MeV, populating discrete states of . continuum discretized coupled channel-coupled reaction channel (CDCC-CRC) calculations have been used to analyze the data.
Results: Results show a new reaction mechanism, where transfer occurs after the breakup of the loosely bound in the population of some bound states of . A comparison of the CDCC-CRC calculations with respect to the measured data were used to determine the spectroscopic amplitudes and factors for the different states of . Using the spectroscopic amplitudes obtained in this work, the factor for the (,) reaction has been calculated in the framework of a two-body potential model and compared to measurements.
Conclusions: The present study very clearly shows that the breakup and transfer coupling effects are strong in the reaction. The present work extracts, in the framework of a coupled reaction channel theory, the spectroscopic amplitudes of the bound and unbound states of . All previous analysis and new measurements should therefore be reexamined from this viewpoint to extract the astrophysical observables correctly.
- Received 23 April 2013
- Revised 3 March 2014
DOI:https://doi.org/10.1103/PhysRevC.89.044618
©2014 American Physical Society