Bremen 2017 – scientific programme

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GR: Fachverband Gravitation und Relativitätstheorie

GR 14: Postersitzung

GR 14.4: Poster

Thursday, March 16, 2017, 14:00–16:00, SFG 0150

Visualizing a Rotating Black Hole — •Thomas Reiber — Universität Hildesheim

The Kerr solution of the Einstein field equation describes the spacetime around a rotating Black Hole. It can be extended over the event horizons to connect distant regions of spacetime. Ray tracing in the maximal analytic extension of Kerr spacetime is used to calculate the view of an observer in the interior region of a black hole.