Soliton solutions and their stability for the flow of relativistic fluids through channels

Details Soliton solutions and their stability for the flow of relativistic fluids through channels Soliton solutions and their stability for the flow of relativistic fluids through channels

Mar 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980ap%26ss..68..207l&link_type=abstract

Astrophysics and Space Science, vol. 68, no. 1, Mar. 1980, p. 207-219.

Statistics

Computation

4

Channel Flow, Computational Fluid Dynamics, Perturbation Theory, Radio Galaxies, Relativistic Plasmas, Galactic Structure, Relativistic Effects

Scientific paper

The flow of a perfect relativistic fluid through channels of various cross-sections is considered with reference to models of radio galaxies. Soliton-like solutions are found and their topologies are discussed. The calculations show that these solutions are unstable. It is suggested that under realistic astrophysical conditions the growth rate of the instabilities is so slow that soliton-type blobs may persist for a significant time.

Affiliated with

Also associated with

No associations

Rating

Soliton solutions and their stability for the flow of relativistic fluids through channels 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 Soliton solutions and their stability for the flow of relativistic fluids through channels, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Soliton solutions and their stability for the flow of relativistic fluids through channels will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1568743