We review the nuclear physics input necessary for the study of the collapse of massive stars as precursor to supernova explosions. Recent theoretical advances for the calculation of the relevant weak-interaction processes and their influence in the collapse and postbounce dynamics are discussed. Fut
Nuclear structure input for supernova modeling
✍ Scribed by Gabriel Martínez-Pinedo
- Publisher
- Elsevier Science
- Year
- 2004
- Tongue
- English
- Weight
- 168 KB
- Volume
- 746
- Category
- Article
- ISSN
- 0375-9474
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✦ Synopsis
Radioactive nuclear beams offer the possibility of studying the detailed properties of nuclei far away from stability. This manuscript gives a review of the main weak-interaction processes involving nuclei relevant for core collapse supernovae. Special emphasis is given to the necessity of constraining the theoretical models by experimental information. Examples of key experimental inputs are given. * The results presented in this talk have been obtained in collaboration with D.
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