Abstract
Fifty-four-point angular distributions in the angular range 2.5° to 170° have been measured for the reaction to the (0.0 MeV), (0.937 MeV), and + (1.1 MeV) states in at a bombarding energy of 34 MeV. In addition, forward angle data have been measured for the (2.101 MeV), (3.725 MeV), (3.791 MeV), and (3.836 MeV) states. The angular distributions for all of the above states are forward peaked and have little structure at back angles. The general structure of the first 60° of the angular distributions can be reproduced by zero-range two-particle transfer distorted-wave Born-approximation calculations; however, the calculations are generally 3° and as much as 10° out of phase with the data past the first maximum. A zero-range distorted-wave Born-approximation normalization factor of 100 is obtained assuming the state to be a pure configuration. Finite-range distorted-wave Born-approximation calculations which include the and components of do not improve the fits to the data and are similar to zero-range calculations at forward angles. The component was shown to have little effect on the calculated angular distributions. The absolute magnitudes of the cross sections are predicted to within a factor of 2 when the shell model wave functions of Kuo and Brown are used in the finite-range distorted-wave Born-approximation calculations. Two-particle and cluster form factors used in the finite-range calculations gave equivalent fits to the data. The magnitude of the cross section at angles greater than 90° and the phase of the forward angle data could not be reproduced by any of the calculations. The failure of the distorted-wave Born-approximation calculations at back angles suggests that a more complete description of the reaction mechanism which includes the exchange of an particle in with the projectile is necessary.
NUCLEAR REACTIONS , MeV; measured lab, ; compared data to zero-range and finite-range DWBA calculations using shell model wave functions. Extracted () zero-range normalization factor.
- Received 1 March 1976
DOI:https://doi.org/10.1103/PhysRevC.14.977
©1976 American Physical Society