Alpha-process Nucleosynthesis

Alpha-Process Nucleosynthesis is a nucleosynthetic mechanism in stellar astrophysics wherein atomic nuclei are formed through the sequential capture of alpha particles, predominantly occurring in high-temperature environments of massive stars and supernovae, leading to the production of elements such as carbon, oxygen, neon, magnesium, silicon, sulfur, and others along the alpha ladder.

45

Publications

4.6K

Citations

168

Authors

91

Institutions

Publications per year

2017–2026

8

Variants

Alpha Process Nucleosynthesis

Authors

168

  1. BS
    B. S. Meyer

    Clemson University, United States

    4 publications · 615 citations

    4

    h-index

  2. JG
    J. Görres

    University of Notre Dame, United States

    4 publications · 378 citations

    4

    h-index

  3. JI
    Jr. Iben I.

    Joint Institute for Laboratory Astrophysics, United States

    3 publications · 587 citations

    3

    h-index

  4. MW
    M. Wiescher

    University of Notre Dame, United States

    3 publications · 325 citations

    3

    h-index

  5. SE
    S. E. Woosley

    University of California, Santa Cruz, United States

    2 publications · 827 citations

    2

    h-index

1–5 of 168

Venues

  1. The Astrophysical Journal

    ApJ · 15 publications · 2.3K citations

    15

    h-index

  2. Physical Review C

    PRC · 5 publications · 236 citations

    5

    h-index

  3. 3

    h-index

  4. Physical Review Letters

    PRL · 2 publications · 169 citations

    2

    h-index

  5. Nuclear Physics A

    2 publications · 70 citations

    2

    h-index

1–5