Hydrostatic Nucleosynthesis
Hydrostatic Nucleosynthesis is a theoretical framework in astrophysics that explains the synthesis of elements during stellar evolution through nuclear reactions occurring under conditions of hydrostatic equilibrium, distinguishing it from explosive nucleosynthesis mechanisms by its reliance on stable, sustained pressure-temperature balances within stellar cores.
29
Publications
2.8K
Citations
54
Authors
47
Institutions
Publications per year
2017–2026
2
Parents
29
Nuclear weak-interaction processes in stars
K. Langanke, G. Martı́nez-Pinedo · Reviews of Modern Physics · 2003 · 547 citations · Full text
1–5 of 29
54
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National Institute of Technology, Kumamoto College, Japan
2 publications · 50 citations
2
h-index
1–5 of 54
47

University of Basel
Basel, Switzerland
5 h-index
5 publications
895 citations

Stockholm University
Stockholm, Sweden
4 h-index
6 publications
405 citations

Mount Stromlo Observatory
Canberra, Australia
3 h-index
5 publications
754 citations
Heidelberg Institute for Theoretical Studies
Heidelberg, Germany
3 h-index
9 publications
960 citations
University of Würzburg
Würzburg, Germany
3 h-index
9 publications
2K citations
National Institute of Technology, Kumamoto College
Kumamoto, Japan
2 h-index
2 publications
50 citations

Oak Ridge National Laboratory
Oak Ridge, United States
2 h-index
4 publications
430 citations
National Astronomical Observatory of Japan
Mitaka-shi, Japan
2 h-index
2 publications
50 citations
1–8 of 47
ApJ · 9 publications · 723 citations
9
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3 publications · 187 citations
3
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2 publications · 50 citations
2
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Repository · 2 publications · 81 citations
2
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2 publications · 125 citations
2
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1–5