Structure and stability of rotating fluid disks around massive objects. II - General relativistic formulation

Details Structure and stability of rotating fluid disks around massive objects. II - General relativistic formulation Structure and stability of rotating fluid disks around massive objects. II - General relativistic formulation

Jun 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982japa....3..193c&link_type=abstract

Journal of Astrophysics and Astronomy, vol. 3, June 1982, p. 193-206.

Astronomy and Astrophysics

Astronomy

6

Accretion Disks, Black Holes (Astronomy), Relativity, Rotary Stability, Rotating Fluids, Perturbation, Rotating Disks, Steady State

Scientific paper

The structure of a thick, perfect fluid disk of constant density rotating around a Schwarzschild black hole is considered, along with its stability under axisymmetric perturbation. The inner edge of this type of disk cannot lie within 4m. The critical gammac for neutral stability is found to be significantly less than 4/3, suggesting that the disks are generally stable.

Affiliated with

Also associated with

No associations

Rating

Structure and stability of rotating fluid disks around massive objects. II - General relativistic formulation 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 Structure and stability of rotating fluid disks around massive objects. II - General relativistic formulation, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Structure and stability of rotating fluid disks around massive objects. II - General relativistic formulation will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1354396