Accretion Disk Simulations
Accretion Disk Simulations is a computational methodology within numerical astrophysics that specifically models the dynamical, radiative, and magnetic processes in rotating gaseous structures around compact celestial objects by numerically solving the equations of hydrodynamics or magnetohydrodynamics under general relativistic or Newtonian gravitational frameworks.
463
Publications
40.8K
Citations
700
Authors
360
Institutions
Publications per year
2017–2026
93
463
Hyperaccreting Black Holes and Gamma‐Ray Bursts
Robert Popham, S. E. Woosley, Chris L. Fryer · The Astrophysical Journal · 1999 · 818 citations · Full text
Natural Sciences, Astronomy, Physics +16
1–5 of 463
700
13
h-index
Center for Astrophysics Harvard & Smithsonian, United States
12 publications · 2.5K citations
12
h-index
12
h-index
11
h-index
11
h-index
1–5 of 700
360
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
23 h-index
51 publications
6.2K citations
Princeton University
Princeton, United States
20 h-index
35 publications
2.2K citations

Centre National de la Recherche Scientifique
Paris, France
20 h-index
67 publications
4.1K citations
University of Maryland, College Park
College Park, United States
18 h-index
37 publications
3.5K citations
University of Cambridge
Cambridge, United Kingdom
18 h-index
40 publications
3.4K citations
University of Virginia
Charlottesville, United States
17 h-index
24 publications
5.5K citations
Max Planck Institute for Astronomy
Heidelberg, Germany
17 h-index
44 publications
3.3K citations

Cornell University
Ithaca, United States
16 h-index
40 publications
4.2K citations
1–8 of 360
ApJ · 174 publications · 19.4K citations
68
h-index
123 publications · 10.5K citations
54
h-index
39 publications · 2.2K citations
25
h-index
Repository · 10 publications · 986 citations
10
h-index
10 publications · 982 citations
10
h-index
1–5