Trapping of one-armed corrugation waves revised

Details Trapping of one-armed corrugation waves revised Trapping of one-armed corrugation waves revised

Feb 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991pasj...43...95k&link_type=abstract

Astronomical Society of Japan, Publications (ISSN 0004-6264), vol. 43, no. 1, 1991, p. 95-111.

Astronomy and Astrophysics

Astronomy

13

Accretion Disks, Black Holes (Astronomy), Density Wave Model, Relativistic Effects, Active Galactic Nuclei, Periodic Variations, Perturbation Theory, X Ray Binaries

Scientific paper

A previous paper discussed how one-armed corrugation waves can be trapped in the innermost region of geometrically thin relativistic accretion disks. The analyses were, however, inaccurate and the results were incorrect. This problem is reexamined here rigorously in the case of special disk models. It is found that the trapping does certainly occur, although the results crucially depend on the pressure distributions within the disk. This confirms the suggestion in the previous paper that examinations of trapping in realistic disks are worthwhile in relation to QPO's phenomena.

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