S-process Nucleosynthesis

s-Process Nucleosynthesis is a nucleosynthesis mechanism in which neutron capture occurs at a slow rate relative to beta decay, allowing unstable isotopes to decay before capturing additional neutrons, thereby producing heavier elements primarily in asymptotic giant branch stars.

318

Publications

27.1K

Citations

799

Authors

327

Institutions

Publications per year

2017–2026

61

Variants

Slow Neutron Capture Process

Authors

799

  1. RG
    R. Gallino

    University of Turin, Italy

    40 publications · 6.4K citations

    33

    h-index

  2. ML
    Maria Lugaro

    Monash University, Australia

    25 publications · 2.4K citations

    19

    h-index

  3. MB
    M. Busso

    University of Perugia, Italy

    18 publications · 2.6K citations

    17

    h-index

  4. OS
    O. Straniero

    Collurania Teramo Observatory, Italy

    18 publications · 2.8K citations

    17

    h-index

  5. MP
    M. Pignatari

    University of Hull, United Kingdom

    16 publications · 1.5K citations

    15

    h-index

1–5 of 799

Venues

  1. The Astrophysical Journal

    ApJ · 134 publications · 12.5K citations

    64

    h-index

  2. Astronomy and Astrophysics

    41 publications · 5K citations

    30

    h-index

  3. Monthly Notices of the Royal Astronomical Society

    27 publications · 1.7K citations

    20

    h-index

  4. Publications of the Astronomical Society of Australia

    PASA · 8 publications · 989 citations

    8

    h-index

  5. The Astrophysical Journal Letters

    7 publications · 347 citations

    7

    h-index

1–5