Kerr black string flow

Kerr black string flow

We give a general illumination of a rotating black string falling into a rotating horizon in dimension D=5. It is a configuration of one smooth intersection between these two objects when the spacetime is axisymmetric and in the limit that the thickness of the black hole is much larger than the thic...

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Main Authors: Meng Sun, Yong-Chang Huang
Format: Article
Language:English
Published: Elsevier 2015-08-01
Series:Nuclear Physics B
Online Access:http://www.sciencedirect.com/science/article/pii/S0550321315001777
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spelling doaj-2c600b9e3b5a4cfa90472a87269f81e32020-11-24T23:41:42ZengElsevierNuclear Physics B0550-32131873-15622015-08-01897C9811010.1016/j.nuclphysb.2015.05.017Kerr black string flowMeng Sun0Yong-Chang Huang1Institute of Theoretical Physics, Beijing University of Technology, 100124, Beijing, ChinaInstitute of Theoretical Physics, Beijing University of Technology, 100124, Beijing, ChinaWe give a general illumination of a rotating black string falling into a rotating horizon in dimension D=5. It is a configuration of one smooth intersection between these two objects when the spacetime is axisymmetric and in the limit that the thickness of the black hole is much larger than the thickness of the black string. Following this configuration, we further extend them to the rotating and charged flows.http://www.sciencedirect.com/science/article/pii/S0550321315001777
collection DOAJ
language English
format Article
sources DOAJ
author Meng Sun
Yong-Chang Huang
spellingShingle Meng Sun
Yong-Chang Huang
Kerr black string flow
Nuclear Physics B
author_facet Meng Sun
Yong-Chang Huang
author_sort Meng Sun
title Kerr black string flow
title_short Kerr black string flow
title_full Kerr black string flow
title_fullStr Kerr black string flow
title_full_unstemmed Kerr black string flow
title_sort kerr black string flow
publisher Elsevier
series Nuclear Physics B
issn 0550-3213
1873-1562
publishDate 2015-08-01
description We give a general illumination of a rotating black string falling into a rotating horizon in dimension D=5. It is a configuration of one smooth intersection between these two objects when the spacetime is axisymmetric and in the limit that the thickness of the black hole is much larger than the thickness of the black string. Following this configuration, we further extend them to the rotating and charged flows.
url http://www.sciencedirect.com/science/article/pii/S0550321315001777
work_keys_str_mv AT mengsun kerrblackstringflow
AT yongchanghuang kerrblackstringflow
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