Energy accumulating, geometrically thin disk accretion around a Kerr black hole.

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Scientific paper

In the inner regions of an accretion disk the non-dissipative forces in
the disk material must be considered in relation to the dissipative
forces because they may increase to the order of them. The properties of
this region in the accretion disk - resulting from an extension of the
disk theory - are worked out.

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