Charged scalar perturbations around Garfinkle–Horowitz–Strominger black holes
We examine the stability of the Garfinkle–Horowitz–Strominger (GHS) black hole under charged scalar perturbations. Employing the appropriate numerical methods, we show that the GHS black hole is always stable against charged scalar perturbations. This is different from the results obtained in the de...
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Series: | Nuclear Physics B |
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doaj-28c1d4e52a6b4ceb846a2b81a47932932020-11-24T22:42:41ZengElsevierNuclear Physics B0550-32131873-15622015-10-01899C375410.1016/j.nuclphysb.2015.07.030Charged scalar perturbations around Garfinkle–Horowitz–Strominger black holesCheng-Yong Zhang0Shao-Jun Zhang1Bin Wang2IFSA Collaborative Innovation Center, Department of Physics and Astronomy, Shanghai Jiao Tong University, Shanghai 200240, ChinaInstituto de Física, Universidade de São Paulo, C.P. 66318, 05315-970 São Paulo, SP, BrazilIFSA Collaborative Innovation Center, Department of Physics and Astronomy, Shanghai Jiao Tong University, Shanghai 200240, ChinaWe examine the stability of the Garfinkle–Horowitz–Strominger (GHS) black hole under charged scalar perturbations. Employing the appropriate numerical methods, we show that the GHS black hole is always stable against charged scalar perturbations. This is different from the results obtained in the de Sitter and anti-de Sitter black holes. Furthermore, we argue that in the GHS black hole background there is no amplification of the incident charged scalar wave to cause the superradiance, so that the superradiant instability cannot exist in this spacetime.http://www.sciencedirect.com/science/article/pii/S0550321315002709 |
collection |
DOAJ |
language |
English |
format |
Article |
sources |
DOAJ |
author |
Cheng-Yong Zhang Shao-Jun Zhang Bin Wang |
spellingShingle |
Cheng-Yong Zhang Shao-Jun Zhang Bin Wang Charged scalar perturbations around Garfinkle–Horowitz–Strominger black holes Nuclear Physics B |
author_facet |
Cheng-Yong Zhang Shao-Jun Zhang Bin Wang |
author_sort |
Cheng-Yong Zhang |
title |
Charged scalar perturbations around Garfinkle–Horowitz–Strominger black holes |
title_short |
Charged scalar perturbations around Garfinkle–Horowitz–Strominger black holes |
title_full |
Charged scalar perturbations around Garfinkle–Horowitz–Strominger black holes |
title_fullStr |
Charged scalar perturbations around Garfinkle–Horowitz–Strominger black holes |
title_full_unstemmed |
Charged scalar perturbations around Garfinkle–Horowitz–Strominger black holes |
title_sort |
charged scalar perturbations around garfinkle–horowitz–strominger black holes |
publisher |
Elsevier |
series |
Nuclear Physics B |
issn |
0550-3213 1873-1562 |
publishDate |
2015-10-01 |
description |
We examine the stability of the Garfinkle–Horowitz–Strominger (GHS) black hole under charged scalar perturbations. Employing the appropriate numerical methods, we show that the GHS black hole is always stable against charged scalar perturbations. This is different from the results obtained in the de Sitter and anti-de Sitter black holes. Furthermore, we argue that in the GHS black hole background there is no amplification of the incident charged scalar wave to cause the superradiance, so that the superradiant instability cannot exist in this spacetime. |
url |
http://www.sciencedirect.com/science/article/pii/S0550321315002709 |
work_keys_str_mv |
AT chengyongzhang chargedscalarperturbationsaroundgarfinklehorowitzstromingerblackholes AT shaojunzhang chargedscalarperturbationsaroundgarfinklehorowitzstromingerblackholes AT binwang chargedscalarperturbationsaroundgarfinklehorowitzstromingerblackholes |
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1725698996651950080 |