Published September 23, 2011
| Version v1
Journal article
Do we understand heavy-ion fusion reactions of importance in stellar evolution?
- 1. Physics Division, Argonne National Laboratory, Argonne, IL 60439 (United States)
- 2. Physics Department, University of Notre Dame, Notre Dame, IN 46556 (United States)
Description
Since the first observation of hindrance in heavy-ion fusion, many extrapolated cross sections for astrophysically interesting fusion reactions, such as 12C + 12C, 12C + 16O, 16O + 16O, 24O etc. need to be reexamined. In this contribution, the effects of fusion hindrance at extreme low energies are discussed.
Availability note (English)
Available from http://dx.doi.org/10.1088/1742-6596/312/4/042011Additional details
Identifiers
Publishing Information
- Journal Title
- Journal of Physics. Conference Series (Online)
- Journal Volume
- 312
- Journal Issue
- 4
- Journal Page Range
- [6 p.]
- ISSN
- 1742-6596
Conference
- Title
- International nuclear physics conference 2010
- Acronym
- INPC2010
- Dates
- 4-9 Jul 2010
- Place
- Vancouver, BC (Canada)
INIS
- Country of Publication
- United Kingdom
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 43076481
- Subject category
- S73: NUCLEAR PHYSICS AND RADIATION PHYSICS; S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- ASTROPHYSICS; CARBON 12 REACTIONS; CARBON 12 TARGET; CROSS SECTIONS; ENERGY DEPENDENCE; HEAVY ION FUSION REACTIONS; OXYGEN 16 REACTIONS; OXYGEN 16 TARGET; OXYGEN 24; STAR EVOLUTION
- Descriptors DEC
- BETA DECAY RADIOISOTOPES; BETA-MINUS DECAY RADIOISOTOPES; EVEN-EVEN NUCLEI; EVOLUTION; HEAVY ION REACTIONS; ISOTOPES; LIGHT NUCLEI; MILLISECONDS LIVING RADIOISOTOPES; NUCLEAR REACTIONS; NUCLEI; NUCLEOSYNTHESIS; OXYGEN ISOTOPES; PHYSICS; RADIOISOTOPES; SYNTHESIS; TARGETS