The radial-azimuthal instability of a radiation-pressure-dominated accretion disk with advection.

Details The radial-azimuthal instability of a radiation-pressure-dominated accretion disk with advection. The radial-azimuthal instability of a radiation-pressure-dominated accretion disk with advection.

Jun 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000cotph..33..655d&link_type=abstract

Commun. Theor. Phys., Vol. 33, No. 4, p. 655 - 660

Other

Accretion Disks: Advection

Scientific paper

A radial-azimuthal instability analysis of a radiation-pressure-dominated accretion disk with advection is presented. The authors find that the including of a very little advection has significant effect on two acoustic modes, which are no longer complex conjugates of each other. With the increase of azimuthal perturbations, the thermal mode becomes more unstable and the viscous mode more stable, but there has no effect on acoustic mode. For geometrically slim and advection-dominated disks, the azimuthal perturbation and increasing of advection do not affect the stability of all the modes.

Affiliated with

Also associated with

No associations

Rating

The radial-azimuthal instability of a radiation-pressure-dominated accretion disk with advection. 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 The radial-azimuthal instability of a radiation-pressure-dominated accretion disk with advection., we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The radial-azimuthal instability of a radiation-pressure-dominated accretion disk with advection. will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1347860