Nucleosynthesis

Nucleosynthesis is the astrophysical process by which atomic nuclei are formed through nuclear reactions, distinguishing itself from other particle formation mechanisms by specifically accounting for the synthesis of elements during the early universe, stellar evolution, and supernova events.

13.4K

Publications

977.8K

Citations

27.6K

Authors

2.9K

Institutions

Publications per year

2017–2026

2.2K

Authors

27.6K

  1. FT
    F.‐K. Thielemann

    University of Basel, Switzerland

    106 publications · 18.6K citations

    63

    h-index

  2. RG
    R. Gallino

    University of Turin, Italy

    97 publications · 14.7K citations

    62

    h-index

  3. SE
    S. E. Woosley

    University of California, Santa Cruz, United States

    88 publications · 23.8K citations

    56

    h-index

  4. HJ
    Hans‐Thomas Janka

    Max Planck Institute for Astrophysics, Germany

    78 publications · 11.4K citations

    54

    h-index

  5. KN
    K. Nomoto

    The University of Tokyo, Japan

    84 publications · 14.9K citations

    53

    h-index

1–5 of 27.6K

Venues

  1. The Astrophysical Journal

    ApJ · 2.6K publications · 223.3K citations

    206

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    760 publications · 52.9K citations

    114

    h-index

  3. Astronomy and Astrophysics

    659 publications · 50.9K citations

    112

    h-index

  4. Nature

    360 publications · 44.8K citations

    100

    h-index

  5. Physics Letters B

    443 publications · 31.1K citations

    88

    h-index

1–5