P-Process Nucleosynthesis is a nucleosynthetic mechanism, belonging to the class of stellar processes that produce heavy atomic nuclei, distinguished by its formation of proton-rich isotopes through the photodisintegration of pre-existing nuclei in high-temperature environments, typically during explosive stellar events such as supernovae or neutron star mergers.
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rp-process nucleosynthesis at extreme temperature and density conditions
H. Schatz, A. Aprahamian, J. Görres et al. · Physics Reports · 1998 · 672 citations · Full text
S. E. Woosley, W. M. Howard · The Astrophysical Journal Supplement Series · 1978 · 382 citations
Natural Sciences, Astronomy, Physics +14
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University of Basel
Basel, Switzerland
12 h-index
20 publications
3.1K citations
The University of Tokyo
Tokyo, Japan
9 h-index
15 publications
728 citations
Université Libre de Bruxelles
Brussels, Belgium
8 h-index
16 publications
1.9K citations
University of Notre Dame
Notre Dame, United States
7 h-index
26 publications
3.9K citations
National Astronomical Observatory of Japan
Mitaka-shi, Japan
7 h-index
20 publications
1.7K citations
Joint Institute for Nuclear Astrophysics
East Lansing, United States
5 h-index
34 publications
1.8K citations
Kyushu University
Fukuoka, Japan
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10 publications
488 citations
GSI Helmholtz Centre for Heavy Ion Research
Darmstadt, Germany
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ApJ · 24 publications · 2K citations
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