Astronomy and Astrophysics – Astrophysics
Scientific paper
2001-02-02
Astronomy and Astrophysics
Astrophysics
6 pages, to appear in proceedings, 20th Texas Symposium on Relativistic Astrophysics, eds J.C. Wheeler and H. Martel
Scientific paper
10.1063/1.1419634
We discuss the results of three-dimensional magnetohydrodynamic simulations, using a pseudo-Newtonian potential, of thin disk (h/r ~ 0.1) accretion onto black holes. We find (i) that magnetic stresses persist within the marginally stable orbit, and (ii) that the importance of those stresses for the dynamics of the flow depends upon the strength of magnetic fields in the disk outside the last stable orbit. Strong disk magnetic fields (alpha > 0.1) lead to a gross violation of the zero-torque boundary condition at the last stable orbit, while weaker fields (alpha ~ 0.01) produce results more akin to traditional models for thin disk accretion onto black holes. Fluctuations in the magnetic field strength in the disk could lead to changes in the radiative efficiency of the flow on short timescales.
Armitage Philip J.
Chiang James
Reynolds Christopher S.
No associations
LandOfFree
Magnetohydrodynamic simulations of black hole accretion 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 Magnetohydrodynamic simulations of black hole accretion, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Magnetohydrodynamic simulations of black hole accretion will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-202910