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

Authors

54

  1. WD
    W. David Arnett

    University of Arizona, United States

    7 publications · 390 citations

    7

    h-index

  2. FT
    F.‐K. Thielemann

    University of Basel, Switzerland

    5 publications · 538 citations

    5

    h-index

  3. SE
    S. E. Woosley

    University of California, Santa Cruz, United States

    2 publications · 56 citations

    2

    h-index

  4. MO
    M. Ono

    Université Libre de Bruxelles, Belgium

    2 publications · 50 citations

    2

    h-index

  5. SF
    Shin‐ichiro Fujimoto

    National Institute of Technology, Kumamoto College, Japan

    2 publications · 50 citations

    2

    h-index

1–5 of 54

Venues

  1. The Astrophysical Journal

    ApJ · 9 publications · 723 citations

    9

    h-index

  2. Astronomy and Astrophysics

    3 publications · 187 citations

    3

    h-index

  3. Progress of Theoretical Physics

    2 publications · 50 citations

    2

    h-index

  4. Springer Link (Chiba Institute of Technology)

    Repository · 2 publications · 81 citations

    2

    h-index

  5. Nuclear Physics A

    2 publications · 125 citations

    2

    h-index

1–5