Non-axisymmetric unstable modes in a thin differentially rotating gaseous disc

Astronomy and Astrophysics – Astrophysics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

17

Accretion Disks, Gravitational Effects, Hydrodynamics, Perturbation Theory, Angular Momentum, Conservation Laws, Density (Mass/Volume), Modal Response, Vorticity

Scientific paper

The linear stability of a thin differentially rotating gaseous disk with reflecting boundaries against nonaxisymmetric perturbations is considered. The relevant conservation laws for the energy and angular momentum of linear nonaxisymmetric modes in a thin rotating disk without self-gravity are discussed, and the basic mode amplification mechanisms are illustrated with numerical solutions. How the frequency and growth rate of unstable modes depend on the distribution of the ratio of vorticity to surface density in the disk is investigated.

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

Non-axisymmetric unstable modes in a thin differentially rotating gaseous disc 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 Non-axisymmetric unstable modes in a thin differentially rotating gaseous disc, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Non-axisymmetric unstable modes in a thin differentially rotating gaseous disc will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1628078

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