Thin Disk Accretion

Thin Disk Accretion is a theoretical model of accretion processes in astrophysics wherein matter spirals inward through a geometrically thin, optically thick, differentially rotating disk, dissipating gravitational energy via viscosity while maintaining approximate hydrostatic equilibrium in the vertical direction.

346

Publications

25.8K

Citations

862

Authors

457

Institutions

Publications per year

2017–2026

97

Variants

Thin Accretion Disk Theory

Authors

862

  1. RN
    Ramesh Narayan

    Center for Astrophysics Harvard & Smithsonian, United States

    12 publications · 4.6K citations

    12

    h-index

  2. CS
    C. S. Kochanek

    The Ohio State University, United States

    7 publications · 835 citations

    7

    h-index

  3. JE
    Jeffrey E. McClintock

    Center for Astrophysics Harvard & Smithsonian, United States

    6 publications · 2.1K citations

    6

    h-index

  4. CB
    Cosimo Bambi

    Fudan University, China

    6 publications · 473 citations

    6

    h-index

  5. EL
    En‐Wei Liang

    Guangxi University, China

    6 publications · 290 citations

    6

    h-index

1–5 of 862

Venues

  1. The Astrophysical Journal

    ApJ · 126 publications · 14.2K citations

    54

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    47 publications · 2.5K citations

    30

    h-index

  3. Astronomy and Astrophysics

    24 publications · 1K citations

    18

    h-index

  4. The European Physical Journal C

    19 publications · 878 citations

    18

    h-index

  5. Physical review. D/Physical review. D.

    PRD · 20 publications · 1.1K citations

    17

    h-index

1–5