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Origin of the p-Nuclei in Explosive Nucleosynthesis
T. Rauscher
Centre for Astrophysics Research (CAR)
School of Physics, Engineering & Computer Science
Research output
:
Chapter in Book/Report/Conference proceeding
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Conference contribution
187
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Physics
Stellar Structure
100%
Massive Star
100%
Nuclides
100%
Heavy Nuclei
100%
Type Ia Supernovae
100%
Temperature Profile
100%
Explosive Nucleosynthesis
100%
Keyphrases
Explosive nucleosynthesis
100%
P-nuclei
100%
Gamma Process
57%
Explosives
28%
Production Process
14%
Process Conditions
14%
Seed Composition
14%
Photodisintegration
14%
Reaction Network
14%
Unstable nuclei
14%
Processing Temperature
14%
Stellar Evolution
14%
Massive Stars
14%
Production Site
14%
Heavy nuclei
14%
Low-mass
14%
High Temperature
14%
Reaction Rate
14%
Intermediate nucleus
14%
S-process
14%
νp-process
14%
Proton Rich
14%
Stellar Structure
14%
Two-mass
14%
Type Ia Supernovae
14%
R-process
14%
Temperature Profile
14%
Material Science
Phase Composition
100%