Astronomy and Astrophysics – Astrophysics
Scientific paper
2004-03-17
Mon.Not.Roy.Astron.Soc. 351 (2004) 1187
Astronomy and Astrophysics
Astrophysics
Accepted for publication in MNRAS
Scientific paper
10.1111/j.1365-2966.2004.07847.x
We show how the viscous evolution of Keplerian accretion discs can be understood in terms of simple kinetic theory. Although standard physics texts give a simple derivation of momentum transfer in a linear shear flow using kinetic theory, many authors, as detailed by Hayashi & Matsuda 2001, have had difficulties applying the same considerations to a circular shear flow. We show here how this may be done, and note that the essential ingredients are to take proper account of, first, isotropy locally in the frame of the fluid and, second, the geometry of the mean flow.
Clarke Catherine J.
Pringle James E.
No associations
LandOfFree
Kinetic theory viscosity 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 Kinetic theory viscosity, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Kinetic theory viscosity will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-151490