| Issue |
EAS Publications Series
Volume 11, 2004
The Future Astronuclear Physics
|
|
|---|---|---|
| Page(s) | 191 - 197 | |
| DOI | https://doi.org/10.1051/eas:2004013 | |
| Published online | 12 July 2004 | |
A. Jorissen, S. Goriely, M. Rayet, L. Siess and H. Boffin (eds)
EAS Publications Series, 11 (2004) 191-197
Experimental Nuclear Physics for Astrophysics
TRIUMF, 4004 Wesbrook Mall, Vancouver, BC, Canada V6T 2A3
Corresponding author: This email address is being protected from spambots. You need JavaScript enabled to view it.
Abstract
The interpretation of many astrophysical phenomena relies on an in depth understanding of different areas of physics. Nuclear physics has a particularly influential role in determining the energy and matter evolution at stellar sites. As more extensive observational data is gathered from earth and space observatories, an ever-greater demand is placed on our knowledge of the basic physical processes that underpin astrophysical phenomena. Some of the associated challenges for nuclear physics are outlined in this paper.
© EAS, EDP Sciences, 2004
