An accretion disk without angular momentum near a black hole

Details An accretion disk without angular momentum near a black hole An accretion disk without angular momentum near a black hole

Jan 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012arep...56....1b&link_type=abstract

Astronomy Reports, Volume 56, Issue 1, pp.1-8

Astronomy and Astrophysics

Astronomy

Scientific paper

We have studied the two-dimensional structure of an accretion disk without angular momentum near a black hole using the Grad-Shafranov equation. When the two-dimensional structure of the flow is systematically taken into account, the singularity of the hydrodynamic equations is located at the sonic surface, rather than at a displaced surface, as occurs when the disk thickness is estimated using the standard technique. A transonic flow can also exist for negative energies, which is not possible when the accretion is strictly radial.

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