Effects of Toroidal Magnetic Fields on the Thermal Instability of Thin Accretion Disks

Physics

Scientific paper

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Accretion, Accretion Disks, Black Hole Physics, Instabilities

Scientific paper

The standard thin disk model predicts that when the accretion rate is moderately high, the disk is radiation-pressure-dominated and thermally unstable. However, observations indicate the opposite, namely the disk is quite stable. We present an explanation in this work by taking into account the role of the magnetic field which was ignored in the previous analysis.

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