Collapse With Rotation

Collapse with Rotation is a theoretical model in astrophysics that describes the asymmetric implosion of a massive stellar core under self-gravity while conserving angular momentum, leading to the formation of a compact object with rotational dynamics and associated phenomena such as accretion disks and jet formation.

142

Publications

11.2K

Citations

313

Authors

170

Institutions

Publications per year

2017–2026

19

Authors

313

  1. AP
    Alan P. Boss

    Carnegie Institution for Science, United States

    8 publications · 375 citations

    8

    h-index

  2. CD
    Christian D. Ott

    California Institute of Technology, United States

    6 publications · 922 citations

    6

    h-index

  3. SY
    Shoichi Yamada

    Waseda University, Japan

    5 publications · 370 citations

    5

    h-index

  4. MS
    Masaru Shibata

    Kyoto University, Japan

    5 publications · 465 citations

    5

    h-index

  5. JE
    Joel E. Tohline

    Louisiana State University, United States

    5 publications · 159 citations

    5

    h-index

1–5 of 313

Venues

  1. The Astrophysical Journal

    ApJ · 57 publications · 4K citations

    33

    h-index

  2. 12

    h-index

  3. Physical Review Letters

    PRL · 7 publications · 820 citations

    7

    h-index

  4. 6

    h-index

  5. Progress of Theoretical Physics

    6 publications · 229 citations

    6

    h-index

1–5