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Teoreticheskaya i Matematicheskaya Fizika, 2010, Volume 163, Number 3, Pages 467–474
DOI: https://doi.org/10.4213/tmf6515 (Mi tmf6515) 		 
This article is cited in 5 scientific papers (total in 5 papers)

Twistor-beam excitations of black holes and prequantum Kerr–Schild geometry

A. Ya. Burinskii

Nuclear Safety Institute, RAS, Moscow, Russia
Full-text PDF (502 kB) Citations (5)
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DOI: https://doi.org/10.4213/tmf6515
Abstract: Exact Kerr–Schild (KS) solutions for electromagnetic excitations of black holes are 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 a subsequent quantum treatment.
Keywords: black hole, twistor, Kerr theorem, singular beam, quantum gravity.
English version:
Theoretical and Mathematical Physics, 2010, Volume 163, Issue 3, Pages 782–787
DOI: https://doi.org/10.1007/s11232-010-0062-y
Bibliographic databases:
Document Type: Article
Language: Russian
Citation: A. Ya. Burinskii, “Twistor-beam excitations of black holes and prequantum Kerr–Schild geometry”, TMF, 163:3 (2010), 467–474; Theoret. and Math. Phys., 163:3 (2010), 782–787
Citation in format AMSBIB
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    • This publication is cited in the following 5 articles:
    Citing articles in Google Scholar: Russian citations, English citations
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    		Теоретическая и математическая физика Theoretical and Mathematical Physics
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