R-process Nucleosynthesis

r-Process Nucleosynthesis is a rapid neutron-capture process within the astrophysical framework of heavy-element synthesis, distinguished from other nucleosynthetic mechanisms by its occurrence in high neutron-density environments where successive neutron absorptions proceed faster than β-decay, leading to the production of neutron-rich isotopes that decay to form stable, heavy nuclei beyond iron.

572

Publications

57.3K

Citations

1.5K

Authors

580

Institutions

Publications per year

2017–2026

189

Variants

Rapid Neutron-capture NucleosynthesisRapid Neutron-capture Process

Authors

1.5K

  1. FT
    F.‐K. Thielemann

    University of Basel, Switzerland

    35 publications · 6.1K citations

    29

    h-index

  2. JJ
    J. J. Cowan

    University of Oklahoma, United States

    26 publications · 2.9K citations

    22

    h-index

  3. AA
    Almudena Arcones

    Technische Universität Darmstadt, Germany

    22 publications · 3.3K citations

    21

    h-index

  4. MR
    Matthew R. Mumpower

    Los Alamos National Laboratory, United States

    24 publications · 1.1K citations

    21

    h-index

  5. RS
    Rebecca Surman

    University of Notre Dame, United States

    24 publications · 1.3K citations

    21

    h-index

1–5 of 1.5K

Venues

  1. The Astrophysical Journal

    ApJ · 178 publications · 18.7K citations

    71

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    51 publications · 4.8K citations

    34

    h-index

  3. The Astrophysical Journal Letters

    29 publications · 4.9K citations

    25

    h-index

  4. Physical Review C

    PRC · 18 publications · 1.6K citations

    18

    h-index

  5. Astronomy and Astrophysics

    18 publications · 1.3K citations

    15

    h-index

1–5