Hidden Conformal Symmetry for the Accelerating Kerr Black Holes

Siahaan, Haryanto Mangaratua

dc.contributor.author	Siahaan, Haryanto Mangaratua
dc.date.accessioned	2018-10-30T04:48:49Z
dc.date.available	2018-10-30T04:48:49Z
dc.date.issued	2018
dc.identifier	https://doi.org/10.1088/1361-6382/aacc54
dc.identifier.issn	1361-6382
dc.identifier.other	artsc327
dc.identifier.uri	http://hdl.handle.net/123456789/7088
dc.description	CLASSICAL AND QUANTUM GRAVITY; 35 (2018) 155002	en_US
dc.description.abstract	According to the Kerr/CFT correspondence, some aspects of extremal and non-extremal Kerr black holes could be explained by using a 2D CFT. This paper is devoted to show how Kerr/CFT correspondence can work for the slowly accelerating Kerr black holes, in both extremal and non-extremal cases. The equation of motion for low frequency scalar probes in the near region possesses the ‘hidden’ conformal symmetry, similar to that of the nonaccelerating version. Assuming a particular value of associated central charge, Cardy formula in 2D CFT can recover the Bekenstein–Hawking entropy for the black hole under consideration. Moreover, agreements in the scattering process between gravitational and 2D CFT dual suggest the existence of slowly accelerating Kerr/CFT duality.	en_US
dc.description.uri	\|http://iopscience.iop.org/article/10.1088/1361-6382/aacc54
dc.language.iso	en	en_US
dc.publisher	IOP Publishing UK	en_US
dc.relation.ispartofseries	CLASSICAL AND QUANTUM GRAVITY;35 (2018) 155002
dc.subject	HOLOGRAPHY	en_US
dc.subject	ACCELERATING KERR	en_US
dc.subject	Kerr/CFT	en_US
dc.title	Hidden Conformal Symmetry for the Accelerating Kerr Black Holes	en_US
dc.type	Journal Articles	en_US