Title

Transition From Complete to Incomplete Fusion in Asymmetric Heavy Ion Reactions

Authors

K. Hanold, Nuclear Science Division, Lawrence Berkeley Laboratory
L. G. Moretto, Nuclear Science Division, Lawrence Berkeley Laboratory
Graham F. Peaslee, Nuclear Science Division, Lawrence Berkeley LaboratoryFollow
G. J. Wozniak, Nuclear Science Division, Lawrence Berkeley Laboratory
D. R. Bowman, National Superconducting Cyclotron Laboratory and Department of Physics Astronomy Michigan State University
M. F. Mohar, National Superconducting Cyclotron Laboratory and Department of Physics Astronomy Michigan State University
D. J. Morrissey, National Superconducting Cyclotron Laboratory and Department of Physics Astronomy Michigan State University

Document Type

Article

Publication Date

8-1-1993

Publication Source

Physical Review C

Volume Number

48

Issue Number

2

First Page

723

Last Page

734

Publisher

American Physical Society

Abstract

Complex fragments with atomic numbers between those of the target and the projectile have been detected from the reactions of 26 and 31 MeV/nucleon Xe129+C, Al, Ti, and Cu. Angular distributions, cross sections, and velocity spectra of these fragments were extracted from the inclusive data. The velocity of the emitting source and Z-total distributions were reconstructed from the twofold coincidence data. These results are used to characterize the emission source of the complex fragments. The results are compared to a geometric incomplete fusion model calculation. Agreement between the model and the data is good.

Recommended Citation

Repository citation: Hanold, K.; Moretto, L. G.; Peaslee, Graham F.; Wozniak, G. J.; Bowman, D. R.; Mohar, M. F.; and Morrissey, D. J., "Transition From Complete to Incomplete Fusion in Asymmetric Heavy Ion Reactions" (1993). Faculty Publications. Paper 1159.
https://digitalcommons.hope.edu/faculty_publications/1159

Published in: Physical Review C, Volume 48, Issue 2, August 1, 1993, pages 723-734. Copyright © 1993 American Physical Society.