The Many Ways a Shock Wave can Oscillate Close to a Black Hole

Details The Many Ways a Shock Wave can Oscillate Close to a Black Hole The Many Ways a Shock Wave can Oscillate Close to a Black Hole

Dec 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002nmgm.meet.2257m&link_type=abstract

"THE NINTH MARCEL GROSSMANN MEETING On Recent Developments in Theoretical and Experimental General Relativity, Gravitation and R

Physics

Scientific paper

The accretion disks are usually supposed symmetric to reflection on the Z=0 plane. Asymmetries in the flow are usually supposed to be very small. However they can have a important role in the case of subkeplerian accretion flows onto black holes leading to the formation of shocks. This is due to the development of the KH instability triggered by the small turbulences at the layer separating the incoming flow from the outcoming shocked flow. The consequence of this phenomenon is the production of asymmetric outflows of matter and quasi periodic oscillations of the inner disk regions up and down the Z=0 plane.

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