Revisiting the Thermal Stability of Radiation ... - Users' Pages

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I.1 “Black hole accretion discs: reality confronts theory”High Luminosity X-ray BinariesL = 0.01~0.5 L EddGierliński & Done,MNRAS, 20043
I.2 Accretion Disks with Toroidal Magnetic Fields• Inclusion of the effect of magnetic fields(e.g., Oda et al., ApJ, 2009)• The ViscosityThe α viscosity law is qualitatively right (Hirose etal. 2009, Pessah et al. 2007), when considering the MRIdriven turbulence.Trϕ= −2αH( Pgas+ Prad+ Pmag)• The vertical hydrostatic equilibrium12Ω 2KΣH = P + P +gasradPmagP mag=2Bϕ / 8π4
Page 1 and 2: Revisiting the Thermal Stability of
Page 3: I.1 Instability of the SSD• Shaku
Page 7 and 8: II.1 Equations of Local Disk Soluti
Page 9 and 10: II.2 Perturbation Analysis• Relat
Page 11 and 12: II.3 Thermal Instability Properties
Page 13 and 14: III. Summary• By assuming that th

Revisiting the Thermal Stability of Radiation ... - Users' Pages

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