Nucleosynthesis
Nucleosynthesis is the astrophysical process by which atomic nuclei are formed through nuclear reactions, distinguishing itself from other particle formation mechanisms by specifically accounting for the synthesis of elements during the early universe, stellar evolution, and supernova events.
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2017–2026
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Abundances of the elements: Meteoritic and solar
Edward Anders, N. Grevesse · Geochimica et Cosmochimica Acta · 1989 · 10.5K citations
Solar System Abundances and Condensation Temperatures of the Elements
K. Lodders · The Astrophysical Journal · 2003 · 4.8K citations · Full text
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California Institute of Technology
Pasadena, United States
122 h-index
1.2K publications
147.2K citations
The University of Tokyo
Tokyo, Japan
114 h-index
1.4K publications
151.2K citations
Max Planck Institute for Astrophysics
Garching, Germany
113 h-index
697 publications
98.4K citations

Centre National de la Recherche Scientifique
Paris, France
108 h-index
2.1K publications
185.3K citations
University of Chicago
Chicago, United States
104 h-index
791 publications
84.7K citations
University of California, Berkeley
Berkeley, United States
96 h-index
760 publications
86K citations
Los Alamos National Laboratory
Los Alamos, United States
92 h-index
797 publications
59.8K citations
University of California, Santa Cruz
Santa Cruz, United States
87 h-index
308 publications
61.4K citations
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ApJ · 2.6K publications · 223.3K citations
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760 publications · 52.9K citations
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659 publications · 50.9K citations
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360 publications · 44.8K citations
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443 publications · 31.1K citations
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