Nucleosynthesis in neutrino-driven supernovae
✍ Scribed by C. Fröhlich; W.R. Hix; G. Martínez-Pinedo; M. Liebendörfer; F.-K. Thielemann; E. Bravo; K. Langanke; N.T. Zinner
- Publisher
- Elsevier Science
- Year
- 2006
- Tongue
- English
- Weight
- 137 KB
- Volume
- 50
- Category
- Article
- ISSN
- 1387-6473
No coin nor oath required. For personal study only.
📜 SIMILAR VOLUMES
Among the major uncertainties involved in the Chandrasekhar mass models for Type Ia supernovae are the companion star of the accreting white dwarf (or the accretion rate that determines the carbon ignition density) and the flame speed after ignition. We present nucleosynthesis results from relativel
We briefly summarize some recent work on nucleosynthesis in massive stars and supernovae. Here we explore: 1) the effect of including additional sources of nucleosynthesis besides massive stars into the mixture -especially classical novae and several varieties of Type Ia supernovae; 2) the sensitivi