Pair-instability Supernovae

Pair-Instability Supernovae is a theoretical model of stellar explosion that belongs to the class of core-collapse supernovae, distinguished by the triggering mechanism involving photon–photon interactions producing electron–positron pairs, which reduce radiation pressure, induce catastrophic core contraction, and lead to explosive oxygen burning in very massive stars (typically 140–260 solar masses).

195

Publications

21.7K

Citations

612

Authors

351

Institutions

Publications per year

2017–2026

86

Variants

Pisn

Authors

612

  1. AH
    Alexander Heger

    Monash University, Australia

    13 publications · 3.8K citations

    13

    h-index

  2. SE
    S. E. Woosley

    University of California, Santa Cruz, United States

    12 publications · 4.3K citations

    12

    h-index

  3. DJ
    Daniel J. Whalen

    University of Portsmouth, United Kingdom

    10 publications · 731 citations

    10

    h-index

  4. DE
    D. E. Holz

    University of Chicago, United States

    9 publications · 1K citations

    9

    h-index

  5. TJ
    Takashi J. Moriya

    National Astronomical Observatory of Japan, Japan

    9 publications · 967 citations

    9

    h-index

1–5 of 612

Venues

  1. The Astrophysical Journal

    ApJ · 64 publications · 9.2K citations

    44

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    43 publications · 2.8K citations

    31

    h-index

  3. Astronomy and Astrophysics

    17 publications · 2.2K citations

    17

    h-index

  4. The Astrophysical Journal Letters

    18 publications · 1.3K citations

    14

    h-index

  5. Physical Review Letters

    PRL · 5 publications · 1.2K citations

    5

    h-index

1–5