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

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I.2 Magnetically Supported Accretion DiskStable?Or not?Abramowiczet al. (1995)Standard model withno magnetic fieldOdaet al. (2009)toroidal magnetic fields incorporated5
II.1 Equations <strong>of</strong> Local Disk SolutionsPtot=12Ω2KΣH····vertical hydrostatic equilibriumPtotTQrϕ=+visPgas+Prad+Pmag=kmΣTH1•∧= −2αPtotH= − ΩKM (1 − 3/ R)2π− −= Qrad+ QadvBH+13aT24< Bϕ>•2 23Q+ − 16cPradvis= − ΩKTrϕ, Q =2κΣ, − ξ M ΩKH( radQadv=2 )2πR+8π····equation <strong>of</strong> state····viscosity prescription & angular momentum conservation····energy equation6
Page 1 and 2: Revisiting the Thermal Stability of
Page 3 and 4: I.1 Instability of the SSD• Shaku
Page 5: I.2 Accretion Disks with Toroidal M
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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