Keplerian Disk Dynamics

Keplerian Disk Dynamics is a theoretical framework that describes the orbital motion and viscous evolution of accretion disks in which angular momentum transport is governed by a balance between gravitational forces and centrifugal support, with angular velocity decreasing as the inverse square root of the radial distance from the central mass.

169

Publications

14.3K

Citations

379

Authors

305

Institutions

Publications per year

2017–2026

21

Variants

Keplerian Accretion Disk Dynamics

Authors

379

  1. SK
    Sandip K. Chakrabarti

    Indian Centre for Space Physics, India

    7 publications · 463 citations

    7

    h-index

  2. ST
    Scott Tremaine

    Institute for Advanced Study, United States

    5 publications · 376 citations

    5

    h-index

  3. JT
    Jihad Touma

    American University of Beirut, Lebanon

    4 publications · 155 citations

    4

    h-index

  4. GI
    Gordon I. Ogilvie

    University of Cambridge, United Kingdom

    4 publications · 128 citations

    4

    h-index

  5. SA
    Steven A. Balbus

    University of Virginia, United States

    4 publications · 861 citations

    4

    h-index

1–5 of 379

Venues

  1. The Astrophysical Journal

    ApJ · 73 publications · 8.3K citations

    44

    h-index

  2. Astronomy and Astrophysics

    18 publications · 798 citations

    17

    h-index

  3. 14

    h-index

  4. Springer Link (Chiba Institute of Technology)

    Repository · 6 publications · 216 citations

    6

    h-index

  5. 5

    h-index

1–5