Twistor-Beam Excitations of Black-Holes and Prequantum Kerr-Schild Geometry

Details Twistor-Beam Excitations of Black-Holes and Prequantum Kerr-Schild Geometry Twistor-Beam Excitations of Black-Holes and Prequantum Kerr-Schild Geometry

2009-11-29

arxiv.org/abs/0911.5499v2

Theoretical and Mathematical Physics, v. 163 (3), 782-787 (2010)

Physics

High Energy Physics

High Energy Physics - Theory

7 pages, 3 Figures. Published version. Talk at the SFT09 conference, MIAN (Steklov Math. Institute), April 2009

Scientific paper

Exact Kerr-Schild (KS) solutions for electromagnetic excitations of black-holes, have the form of singular beams supported on twistor lines of the KS geometry. These beams have a very strong back-reaction on the metric and horizon and create a fluctuating KS geometry occupying an intermediate position between the classical and quantum gravities. We consider the Kerr theorem, which determines the twistor structure of the KS geometry and the corresponding holographic prequantum space-time adapted to subsequent quantum treatment.

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