Potential inversion with sub-barrier fusion data reexamined
Creators
- 1. Department of Physics, Tohoku University, Sendai 980-8578 (Japan)
Description
We invert experimental data for heavy-ion fusion reactions at energies well below the Coulomb barrier in order to directly determine the internucleus potential between the colliding nuclei. In contrast to the previous applications of the inversion formula, we explicitly take into account the effect of channel couplings on fusion reactions, by assuming that fusion cross sections at deep sub-barrier energies are governed by the lowest barrier in the barrier distribution. We apply this procedure to the 16O+144Sm and 16O+208Pb reactions, and find that the inverted internucleus potential are much thicker than phenomenological potentials. A relation to the steep fall-off phenomenon of fusion cross sections recently found at deep sub-barrier energies is also discussed
Additional details
Identifiers
- DOI
- 10.1103/PhysRevC.76.021601;
- arXiv
- arXiv:0706.2526v1;
Publishing Information
- Journal Title
- Physical Review. C, Nuclear Physics
- Journal Volume
- 76
- Journal Issue
- 2
- Journal Page Range
- p. 021601-021601.4
- ISSN
- 0556-2813
- CODEN
- PRVCAN
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 39076748
- Subject category
- S73: NUCLEAR PHYSICS AND RADIATION PHYSICS; S70: PLASMA PHYSICS AND FUSION TECHNOLOGY; S71: CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS;
- Descriptors DEI
- COULOMB FIELD; CROSS SECTIONS; DISTRIBUTION; HEAVY ION FUSION REACTIONS; LEAD 208; LEAD 208 TARGET; NUCLEAR POTENTIAL; OXYGEN 16; OXYGEN 16 REACTIONS; SAMARIUM 144; SAMARIUM 144 TARGET
- Descriptors DEC
- ELECTRIC FIELDS; EVEN-EVEN NUCLEI; HEAVY ION REACTIONS; HEAVY NUCLEI; INTERMEDIATE MASS NUCLEI; ISOTOPES; LEAD ISOTOPES; LIGHT NUCLEI; NUCLEAR REACTIONS; NUCLEI; NUCLEOSYNTHESIS; OXYGEN ISOTOPES; POTENTIALS; RARE EARTH NUCLEI; SAMARIUM ISOTOPES; STABLE ISOTOPES; SYNTHESIS; TARGETS
Optional Information
- Notes
- (c) 2007 The American Physical Society