Published October 2002
| Version v1
Journal article
Fusion and breakup in the reactions of 6Li and 7Li nuclei with 209Bi
Creators
- 1. Department of Nuclear Physics, Research School of Physical Sciences and Engineering, Australian National University, Canberra ACT 0200 (Australia)
- 2. Yukawa Institute for Theoretical Physics, Kyoto University, Kyoto 606-8502 (Japan)
- 3. Instituto de Fisica, Universidade Federal Fluminense, Av. Litoranea, Niteroi, RJ, 24210-340 (Brazil)
- 4. Instituto de Fisica, Universidade de Sao Paulo, Sao Paulo, S.P. (Brazil)
Description
Excitation functions have been measured for the fusion of the weakly bound nuclei 6Li and 7Li with 209Bi. The complete-fusion cross sections are lower than those predicted by fusion models, being only 65% and 75% for 6Li and 7Li, respectively. Within the uncertainties, this suppression is independent of beam energy. Distinguishing complete fusion from incomplete fusion, both experimentally and in theoretical models, is essential to understand the fusion process of weakly bound nuclei. A simple classical trajectory model which makes this distinction is presented. Further developments of the concepts of this model could be used for realistic predictions for the fusion of unstable weakly bound nuclei
Additional details
Identifiers
Publishing Information
- Journal Title
- Physical Review. C, Nuclear Physics
- Journal Volume
- 66
- Journal Issue
- 4
- Journal Page Range
- p. 041602-041602.4
- ISSN
- 0556-2813
- CODEN
- PRVCAN
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 36012636
- Subject category
- S73: NUCLEAR PHYSICS AND RADIATION PHYSICS;
- Descriptors DEI
- BISMUTH 209 TARGET; COMPARATIVE EVALUATIONS; CROSS SECTIONS; EXCITATION FUNCTIONS; HEAVY ION FUSION REACTIONS; LITHIUM 6 REACTIONS; LITHIUM 7 REACTIONS
- Descriptors DEC
- CROSS SECTIONS; DIFFERENTIAL CROSS SECTIONS; EVALUATION; FUNCTIONS; HEAVY ION REACTIONS; NUCLEAR REACTIONS; NUCLEOSYNTHESIS; SYNTHESIS; TARGETS
Optional Information
- Notes
- (c) 2002 The American Physical Society