The quantization of a Kerr-AdS black hole

We apply our model of quantum gravity to a Kerr-AdS space-time of dimension , , where all rotational parameters are equal, resulting in a wave equation in a quantum space-time which has a sequence of solutions that can be expressed as a product of stationary and temporal eigenfunctions. The stationa...

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Bibliographic Details
Main Author: Gerhardt, Claus (Author)
Format: Article (Journal)
Language:English
Published: 5 February 2018
In: Advances in mathematical physics
Year: 2018, Pages: 1-10
ISSN:1687-9139
DOI:10.1155/2018/4328312
Online Access:Verlag, kostenfrei, Volltext: http://dx.doi.org/10.1155/2018/4328312
Verlag, kostenfrei, Volltext: https://www.hindawi.com/journals/amp/2018/4328312/
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Author Notes:Claus Gerhardt
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Summary:We apply our model of quantum gravity to a Kerr-AdS space-time of dimension , , where all rotational parameters are equal, resulting in a wave equation in a quantum space-time which has a sequence of solutions that can be expressed as a product of stationary and temporal eigenfunctions. The stationary eigenfunctions can be interpreted as radiation and the temporal ones as gravitational waves. The event horizon corresponds in the quantum model to a Cauchy hypersurface that can be crossed by causal curves in both directions such that the information paradox does not occur. We also prove that the Kerr-AdS space-time can be maximally extended by replacing in a generalized Boyer-Lindquist coordinate system the variable by such that the extended space-time has a timelike curvature singularity in .
Item Description:Gesehen am 28.05.2018
Physical Description:Online Resource
ISSN:1687-9139
DOI:10.1155/2018/4328312