Elemental Nucleosynthesis

Elemental Nucleosynthesis is a theoretical framework in astrophysics that describes the process by which new atomic nuclei are formed through nuclear fusion reactions in the extreme conditions following a supernova explosion, distinguishing it from primordial and stellar nucleosynthesis by its reliance on explosive nucleosynthetic pathways and shock-induced reactions.

948

Publications

88.7K

Citations

2.2K

Authors

745

Institutions

Publications per year

2017–2026

179

Authors

2.2K

  1. FT
    F.‐K. Thielemann

    University of Basel, Switzerland

    25 publications · 4.1K citations

    22

    h-index

  2. MP
    M. Pignatari

    University of Hull, United Kingdom

    23 publications · 2K citations

    20

    h-index

  3. KN
    K. Nomoto

    The University of Tokyo, Japan

    21 publications · 4.1K citations

    19

    h-index

  4. SE
    S. E. Woosley

    University of California, Santa Cruz, United States

    21 publications · 8.3K citations

    19

    h-index

  5. MW
    M. Wiescher

    University of Notre Dame, United States

    17 publications · 2.4K citations

    17

    h-index

1–5 of 2.2K

Venues

  1. The Astrophysical Journal

    ApJ · 296 publications · 29.6K citations

    86

    h-index

  2. Astronomy and Astrophysics

    75 publications · 7.9K citations

    44

    h-index

  3. Monthly Notices of the Royal Astronomical Society

    65 publications · 4.8K citations

    35

    h-index

  4. The Astrophysical Journal Letters

    27 publications · 2.6K citations

    23

    h-index

  5. Nuclear Physics A

    27 publications · 2K citations

    20

    h-index

1–5