Astronomy and Astrophysics – Astrophysics
Scientific paper
2003-04-28
Astrophys.J.593:992-1006,2003
Astronomy and Astrophysics
Astrophysics
12 figures
Scientific paper
10.1086/376615
We examine the small-scale dynamics of black hole accretion disks in which radiation pressure exceeds gas pressure. Local patches of disk are modeled by numerically integrating the equations of radiation MHD in the flux-limited diffusion approximation. The shearing-box approximation is used, and the vertical component of gravity is neglected. Magneto-rotational instability (MRI) leads to turbulence in which accretion stresses are due primarily to magnetic torques. When radiation is locked to gas over the length and time scales of fluctuations in the turbulence, the accretion stress, density contrast, and dissipation differ little from those in the corresponding calculations with radiation replaced by extra gas pressure. However, when radiation diffuses each orbit a distance that is comparable to the RMS vertical wavelength of the MRI, radiation pressure is less effective in resisting squeezing. Large density fluctuations occur, and radiation damping of compressive motions converts PdV work into photon energy. The accretion stress in calculations having a net vertical magnetic field is found to be independent of opacity over the range explored, and approximately proportional to the square of the net field. In calculations with zero net magnetic flux, the accretion stress depends on the portion of the total pressure that is effective in resisting compression. The stress is lower when radiation diffuses rapidly with respect to the gas. We show that radiation-supported Shakura-Sunyaev disks accreting via internal magnetic stresses are likely in their interiors to have radiation marginally coupled to turbulent gas motions.
Krolik Julian H.
Sano Takayoshi
Stone James M.
Turner Neal James
No associations
LandOfFree
Local Three-Dimensional Simulations of Magneto-Rotational Instability in Radiation-Dominated Accretion Disks does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Local Three-Dimensional Simulations of Magneto-Rotational Instability in Radiation-Dominated Accretion Disks, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Local Three-Dimensional Simulations of Magneto-Rotational Instability in Radiation-Dominated Accretion Disks will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-333356