Nucleosynthesis in neutrino-driven winds. I. The physical conditions

Keyphrases

• Nucleosynthesis 100%
• Physical Condition 100%
• R-process 100%
• Neutrino-driven Wind 100%
• Supernovae 50%
• Mass Loss 50%
• Numerical Methods 50%
• Rapid Expansion 50%
• Physical Parameters 50%
• Numerical Model 50%
• Neutron Stars 50%
• Mass Loss Rate 50%
• Baryons 50%
• Analytic Method 50%
• High Entropy 50%
• Numerical Calculation 50%
• Analytic Results 50%
• Neutrino Luminosity 50%
• Hydrodynamic Code 50%

Physics

• Nuclear Fusion 100%
• Baryon 50%
• Timescale Dynamics 50%
• Supernovae 50%
• Mathematical Method 50%
• Neutron Stars 50%
• Numerical Model 50%
• Hydrodynamics 50%