Nuclear fusion reactions generate the energies by which stars stabilize during their long lives in hydrostatic equilibrium. In late-stage stellar evolution and during core collapse of massive stars nuclear reactions mediated by the weak force are essential. Finally, a large network of nuclear reacti
Surrogate nuclear reaction methods for astrophysics
✍ Scribed by Jutta E. Escher; Frank S. Dietrich; Christian Forssén
- Publisher
- Elsevier Science
- Year
- 2007
- Tongue
- English
- Weight
- 413 KB
- Volume
- 261
- Category
- Article
- ISSN
- 0168-583X
No coin nor oath required. For personal study only.
📜 SIMILAR VOLUMES
We review the Hartree-Fock-Bogolyubov mass models of the Brussels-Montreal group and compare their suitability for astrophysical purposes with three other modern mass formulas: the FRDM of Möller et al., the KUTY model of Koura et al., and the Duflo-Zuker 1995 model. In addition to considering the q
Gamma-ray astronomy presents an extraordinary scientific potential for the study of the most powerful sources and the most violent events in the Universe. In order to take full advantage of this potential, the next generation of instrumentation for this domain will have to achieve an improvement in