Disk Instability Theory

Disk Instability Theory is a theoretical model of planetary formation in which gravitational instabilities within a protoplanetary disk lead to the direct collapse of gas and dust into planet-sized bodies, distinguishing it from core accretion models that require gradual solid core growth followed by gas capture.

151

Publications

14.3K

Citations

392

Authors

272

Institutions

Publications per year

2017–2026

25

Variants

Gravitational Instability ModelGravitational Instability Theory

Authors

392

  1. AP
    Alan P. Boss

    Carnegie Institution for Science, United States

    7 publications · 1K citations

    7

    h-index

  2. YO
    Yoji Osaki

    The University of Tokyo, Japan

    6 publications · 681 citations

    6

    h-index

  3. SM
    Shin Mineshige

    Kyoto University, Japan

    5 publications · 197 citations

    5

    h-index

  4. JP
    J. P. Lasota

    Centre National de la Recherche Scientifique, France

    4 publications · 203 citations

    4

    h-index

  5. RH
    Ravit Helled

    University of Zurich, Switzerland

    4 publications · 195 citations

    4

    h-index

1–5 of 392

Venues

  1. The Astrophysical Journal

    ApJ · 57 publications · 8K citations

    38

    h-index

  2. 14

    h-index

  3. Astronomy and Astrophysics

    14 publications · 647 citations

    13

    h-index

  4. 10

    h-index

  5. The Astrophysical Journal Letters

    8 publications · 389 citations

    8

    h-index

1–5