The astrophysical r-process: A comparison of calculations following adiabatic expansion with classical calculations based on neutron densities and temperatures

Keyphrases

• Neutron Temperature 100%
• Neutron Density 100%
• Adiabatic Expansion 100%
• R-process 100%
• Nuclear Mass Models 33%
• B-stability 33%
• Neutron 33%
• Unstable nuclei 33%
• Freeze-out 33%
• Number Density 33%
• Nuclear Structure 33%
• Wind Scenario 33%
• Neutrinos 33%
• High Entropy 33%
• E-value 33%
• Rapid Neutron-capture Process 33%
• Nuclear Properties 33%
• Supernova Explosion 33%
• Entropy-based 33%
• Abundance Trends 33%
• Supernovae 33%
• Low Entropy 33%
• Mass Range 33%
• Neutron Stars 33%

Physics

• Hubble Time 100%
• Supernovae 100%
• Nuclear Structure 50%
• Neutron Stars 50%