Effects of Rotation and Deformation of Central Black Holes on the Structure of Rotating Disks

Details Effects of Rotation and Deformation of Central Black Holes on the Structure of Rotating Disks Effects of Rotation and Deformation of Central Black Holes on the Structure of Rotating Disks

Apr 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986pthph..75..828k&link_type=abstract

Progress of Theoretical Physics, Vol. 75, No. 4, pp. 828-835

Physics

Scientific paper

The structure of the fluid disks around black holes is studied in a family of space-time with Tomimatsu-Sato metrics which are parametrized by deformation delta and rotation q. The specific angular momentum of the fluid is taken to be constant in the disk. The thick disk is formed when the rotation parameter q is large and the deformation parameter delta is small. When the rotation parameter q is large, the disk feature is mainly determined by q. If q is small, the disk feature is more affected by the deformation parameter delta than q.

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