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Monthly Notices of the Royal Astronomical Society

Volumn 383, Issue 2, 2008, Pages 683-690

The fundamental difference between shear alpha viscosity and turbulent magnetorotational stresses

(3) Pessah, Martin E a,b,c Chan, Chi Kwan c,d Psaltis, Dimitrios b,c

a INSTITUTE FOR ADVANCED STUDY (United States)

b Astronomy Department (United States)

c Physics Department (United States)

d HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS (United States)

Author keywords

Accretion, accretion discs; Black hole physics; Instabilities; MHD; Turbulence

Indexed keywords

BLACK HOLES; NUMERICAL MODELS; SHEAR FLOW; SHEAR VISCOSITY;

ACCRETION DISCS; ACCRETION: ACCRETION DISKS; BLACK HOLE PHYSICS; DYNAMICAL MODELING; LINEARLY PROPORTIONAL; MAGNETOROTATIONAL INSTABILITY; MOMENTUM TRANSPORTS; ROTATING FLOW; THE STANDARD MODEL; VELOCITY PROFILES;

MAGNETOHYDRODYNAMICS;

EID: 37849018739 PISSN: 00358711 EISSN: 13652966 Source Type: Journal
DOI: 10.1111/j.1365-2966.2007.12574.x Document Type: Article

Times cited : (47)

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