ESTIMATE OF THE SHAKURA–SUNYAEV VISCOSITY PARAMETER IN THE KEPLERIAN ACCRETION DISK FROM HYDRODYNAMIC TURBULENCE

DOI10.1142/S0218271808012139zbMath1157.85003MaRDI QIDQ3532160

Banibrata Mukhopadhyay

Publication date: 3 November 2008

Published in: International Journal of Modern Physics D (Search for Journal in Brave)

zbMATH Keywords

turbulenceaccretion diskhydrodynamics instabilitytransporting matter

Mathematics Subject Classification ID

Galactic and stellar structure (85A15) Hydrodynamic and hydromagnetic problems in astronomy and astrophysics (85A30)

Related Items (1)

Growing pseudo-eigenmodes and positive logarithmic norms in rotating shear flows

Cites Work

• Accretion disk instability revisited
• Hydrodynamic stability of rotationally supported flows: Linear and nonlinear 2D shearing box results

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