Three-dimensional general relativistic radiation magnetohydrodynamical simulation of super-Eddington accretion, using a new code HARMRAD with M1 closure

Monthly Notices of the Royal Astronomical Society

Volumn 441, Issue 4, 2014, Pages 3177-3208

  McKinney, Jonathan C ^a   Tchekhovskoy, Alexander ^b   Sadowski, Aleksander ^c   Narayan, Ramesh ^c  

^a University of Maryland   (United States)

^b UNIVERSITY OF CALIFORNIA   (United States)

^c HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

Author keywords

Accretion, accretion discs; Black hole physics; Gravitation; Hydrodynamics; Methods: numerical; MHD

Indexed keywords

BLACK HOLES; EFFICIENCY; FLOW STRUCTURE; GRAVITATION; LUMINANCE; MAGNETOPLASMA; NUMERICAL METHODS; RADIATION; STARS;

ACCRETION: ACCRETION DISKS; ACTIVE GALACTIC NUCLEI; BLACK HOLE ACCRETION; BLACK HOLE PHYSICS; BLACK HOLES; ELECTROMAGNETICS; HOLE SPIN; METHOD: NUMERICAL; RADIATIVE EFFICIENCY; RELATIVISTICS;

MAGNETOHYDRODYNAMICS;

EID: 84903216969     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1093/mnras/stu762     Document Type: Article

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