2009/11/30 by Alexander Burinskii, A. Ya. Burinskii · 5 citations
Physics and Astronomy · #Astrophysical Phenomena and Observations #Black Holes and Theoretical Physics #Black hole (networking) #Horizon #Metric (unit) #Position (finance) #Pulsars and Gravitational Waves Research #Quantum #Twistor theory #gr-qc #hep-th #quant-ph
paper · pdf · doi:10.1007/s11232-010-0062-y
published in Theoretical and Mathematical Physics 163(3), 782-787 (Pleiades Publishing) · 7 pages, 3 Figures. Published version. Talk at the SFT09 conference, MIAN (Steklov Math. Institute), April 2009
openalex publication_date 2010/06/01 · arxiv created 2010/07/01 · arxiv updated 2015/05/14 · openalex created_date 2019/06/27 · openalex updated_date 2026/08/05
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.