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Dual fluid for the Kerr black hole

Lysov, Vyacheslav (2018) Dual fluid for the Kerr black hole. Journal of High Energy Physics, 2018 (6). Art. No. 80. ISSN 1126-6708. doi:10.1007/JHEP06(2018)080.

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Rotating black holes are algebraically special solutions to the vacuum Einstein equation. Using properties of the algebraically special solutions we construct the dual fluid, which flows on black hole horizon. An explicit form of the Kerr solution allows us to write an explicit dual fluid solution and investigate its stability using energy balance equation. We show that the dual fluid is stable because of high algebraic speciality of the Kerr solution.

Item Type:Article
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Additional Information:© 2018 The Author(s). This article is distributed under the terms of the Creative Commons Attribution License (CC-BY 4.0), which permits any use, distribution and reproduction in any medium, provided the original author(s) and source are credited. Article funded by SCOAP3. Received: April 11, 2018; Accepted: June 8, 2018; Published: June 18, 2018. Author is grateful to A. Strominger for useful discussions on early stages of this work. This work was supported in part by DOE grant DE-SC0011632 and the Sherman Fairchild scholarship.
Group:Walter Burke Institute for Theoretical Physics
Funding AgencyGrant Number
Department of Energy (DOE)DE-SC0011632
Sherman Fairchild FoundationUNSPECIFIED
Subject Keywords:Black Holes; Classical Theories of Gravity; Holography and condensed matter physics (AdS/CMT)
Issue or Number:6
Record Number:CaltechAUTHORS:20180619-100118222
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Official Citation:Lysov, V. J. High Energ. Phys. (2018) 2018: 80.
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:87217
Deposited By: Tony Diaz
Deposited On:19 Jun 2018 17:10
Last Modified:15 Nov 2021 20:46

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