The oscillatory shape of the stationary twisted disc around a Kerr black hole

Details The oscillatory shape of the stationary twisted disc around a Kerr black hole The oscillatory shape of the stationary twisted disc around a Kerr black hole

Feb 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997mnras.285..394i&link_type=abstract

Monthly Notices of the Royal Astronomical Society, Volume 285, Issue 2, pp. 394-402.

Physics

26

Accretion, Accretion Discs, Black Hole Physics, Relativity, Celestial Mechanics, Stellar Dynamics.

Scientific paper

We consider the twisted accretion disc around a Kerr black hole and derive the stationary twist equation in the leading order on small parameters of relative thickness delta, viscosity alpha and relativistic corrections r_g/r. We take into account post-Newtonian corrections which determine the shape of the stationary twisted accretion disc in the limit of small viscosity, alpha

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