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...
Gespeichert in:
| 1. Verfasser: | |
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| Dokumenttyp: | Article (Journal) |
| Sprache: | Englisch |
| Veröffentlicht: |
5 February 2018
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| In: |
Advances in mathematical physics
Year: 2018, Pages: 1-10 |
| ISSN: | 1687-9139 |
| DOI: | 10.1155/2018/4328312 |
| Online-Zugang: | 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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| Verfasserangaben: | Claus Gerhardt |
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| 520 | |a 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 . | ||
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