This review concentrates on the two principle methods used to evolve nuclear abundances within astrophysical simulations, evolution via rate equations and via equilibria. Because in general the rate equations in nucleosynthetic applications form an extraordinarily sti system, implicit methods have p
✦ LIBER ✦
Nuclear quests for supernova dynamics and nucleosynthesis
✍ Scribed by K. Langanke; G. Martínez-Pinedo; I. Petermann; F.K. Thielemann
- Publisher
- Elsevier Science
- Year
- 2011
- Tongue
- English
- Weight
- 666 KB
- Volume
- 66
- Category
- Article
- ISSN
- 0146-6410
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