Nucleosynthesis: a field with still many open nuclear physics questions
- 1. Institut d'Astronomie et d'Astrophysique, Universite Libre de Bruxelles, Campus de la Plaine, CP 226 1050 Brussels (Belgium)
Description
Stellar nucleosynthesis is a vastly interdisciplinary field. There is a large number of different problems invoked calling for a variety of different and complementary research fields. Impressive progress has been made for the last decades in the various fields related to nucleosynthesis, especially in experimental and theoretical nuclear physics, as well as in ground-based or space astronomical observations and astrophysical modellings. In spite of that success, major problems and puzzles remain. The three major nucleosynthesis processes called for to explain the origin of the elements heavier than iron are described and the major pending questions discussed. As far as nuclear physics is concerned, good quality nuclear data is known to be a necessary condition for a reliable modelling of stellar nucleosynthesis. Through some specific examples, the need for further theoretical or experimental developments is also critically discussed in view of their impact on nucleosynthesis predictions.
Additional details
Identifiers
- DOI
- 10.1063/1.3455926;
Publishing Information
- Journal Title
- AIP Conference Proceedings
- Journal Volume
- 1238
- Journal Issue
- 1
- Journal Page Range
- p. 18-25
- ISSN
- 0094-243X
- CODEN
- APCPCS
Conference
- Title
- 7. Tours symposium on nuclear physics and astrophysics
- Dates
- 16-20 Nov 2009
- Place
- Kobe (Japan)
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 41096650
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- ASTROPHYSICS; IRON; METEORITES; NEUTRON STARS; NUCLEAR EXPLOSIONS; NUCLEAR PHYSICS; NUCLEOSYNTHESIS; SIMULATION
- Descriptors DEC
- ELEMENTS; EXPLOSIONS; METALS; PHYSICS; STARS; SYNTHESIS; TRANSITION ELEMENTS
Optional Information
- Notes
- (c) 2010 American Institute of Physics
- Collaborations
- S.G. is FNRS senior research assistant