Global Dynamics of Advection-Dominated Accretion Revisited

Astronomy and Astrophysics – Astrophysics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

24 pages with 15 figures, to appear in ApJ Vol. 523

Scientific paper

10.1086/307725

We numerically solve the set of dynamical equations describing advection-dominated accretion flows (ADAF) around black holes, using a method similar to that of Chakrabarti (1996a). We choose the sonic radius of the flow $R_s$ and the integration constant in angular momentum equation $j$ as free parameters, and integrate the equations from the sonic point inwards to see if the solution can extend supersonically to the black hole horizon, and outwards to see if and where an acceptable outer boundary of the flow can be found. We recover the ADAF-thin disk solution constructed in Narayan, Kato, & Honma (1997, NKH97), an representative paper of the previous works on global ADAF solutions, although in that paper an apparently very different procedure was adopted. We obtain a complete picture in the form of $R_s-j$ parameter space which sums up the situation of ADAF solution at a glance. For comparison we also present the distribution of global solutions for inviscid flows in the $R_s-j$ space, which supports the view that there should be some similarities between the dynamical behavior of ADAF and that of adiabatic flows, and that there should be a continuous change from the properties of viscous flows to those of inviscid ones.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Global Dynamics of Advection-Dominated Accretion Revisited 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 Global Dynamics of Advection-Dominated Accretion Revisited, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Global Dynamics of Advection-Dominated Accretion Revisited will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-448346

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.