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2019

Lensing and shadow of a black hole surrounded by a heavy accretion disk

Cunha, Pedro V. P., Eiró, Nelson A., Herdeiro, Carlos A. R. et al.

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We consider a static, axially symmetric spacetime describing the superposition of a Schwarzschild black hole (BH) with a thin and heavy accretion disk.

The BH-disk configuration is a solution of the Einstein field equations within the Weyl class.
The disk is sourced by a distributional energy-momentum tensor and it is located at the equatorial plane.
It can be interpreted as two streams of counter-rotating particles, yielding a total vanishing angular momentum.

Lensing and shadow of a black hole surrounded by a heavy accretion disk · Around

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Then

O. Semerak and P. Sukova, Free motion around black holes with discs or rings: Between integrability and chaos - II , Mon. Not. Roy. Astron. Soc. 425
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P. Suková and O. Semerák, Free motion around black holes with discs or rings: Between integrability and chaos - III , Mon. Not. Roy. Astron. Soc. 436
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P. V. P. Cunha, C. A. R. Herdeiro, E. Radu and H. F. Runarsson, Shadows of Kerr black holes with scalar hair , Phys. Rev. Lett. 115
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V. Witzany, O. Semerák and P. Suková, Free motion around black holes with discs or rings: Between integrability and chaos – IV , Mon. Not. Roy. Astron. Soc. 451
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