Nucleosynthesis in massive stars using extended adaptive nuclear reaction networks

Keyphrases

• Reaction Network 100%
• Massive Stars 100%
• Nuclear Reactions 100%
• S-process 100%
• Nucleosynthesis 100%
• Hydrogen Burning 66%
• Weak Interaction Rates 33%
• Stable Isotopes 33%
• IStar 33%
• Solar Energy Production 33%
• Mass Loss 33%
• Gamma Process 33%
• Stellar Models 33%
• Proton-rich Isotopes 33%
• Presupernova 33%
• Opacity 33%
• Supernova Explosion 33%
• Type II Supernovae 33%
• Solar Abundances 33%
• Stellar Winds 33%
• Mass number 33%
• Helium Burning 33%
• Nuclear Data 33%
• Overproduction 33%

Physics

• Nuclear Reaction 100%
• Nuclear Fusion 100%
• Massive Star 100%
• Hydrogen Burning 100%
• Stellar Wind 50%
• Stellar Model 50%
• Weak Interaction 50%
• Type II Supernovae 50%
• Solar Abundances 50%
• Helium Burning 50%
• Stable Isotope 50%
• Supernovae 50%