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Fusion Cross Sections of Astrophysics Interest Within the STELLA Project
- Source :
- JPS Conf. Proc., 14th International Symposium on Nuclei in the Cosmos (NIC2016), 14th International Symposium on Nuclei in the Cosmos (NIC2016), Jun 2016, Niigata, Japan. pp.021001, ⟨10.7566/JPSCP.14.021001⟩
- Publication Year :
- 2016
- Publisher :
- HAL CCSD, 2016.
-
Abstract
- International audience; Low energy fusion between light heavy-ions is a key feature of the evolution of massive stars. In systems of astrophysical interest, the process may be strongly affected by molecular configurations of the compound nucleus, leading to resonant S factors. In particular, the 12C+12C fusion reaction has been the object of numerous experimental investigations. The STELLA project has been developed to extend these investigations to lower energies towards the Gamow window.
Details
- Language :
- English
- Database :
- OpenAIRE
- Journal :
- JPS Conf. Proc., 14th International Symposium on Nuclei in the Cosmos (NIC2016), 14th International Symposium on Nuclei in the Cosmos (NIC2016), Jun 2016, Niigata, Japan. pp.021001, ⟨10.7566/JPSCP.14.021001⟩
- Accession number :
- edsair.doi.dedup.....49675338d41985d9fb2df4e2225e5c06
- Full Text :
- https://doi.org/10.7566/JPSCP.14.021001⟩