Six-dimensional non-extremal Reissner-Nordstrom black hole, charged massive scalar perturbation and black hole bomb

Zhao, Run-Dong; Huang, Jia-Hui

doi:10.1016/j.physletb.2022.137286

Cited by 3 publications

(2 citation statements)

References 54 publications

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“…Compared to four-dimensional cases, the (in)stability of higher-dimensional BHs are more complicated. The higher-dimensional spherically symmetric Schwarzschild-Tangherlini spacetime and Reissner-Nordström (RN) BHs were proven to be stable when perturbed by external fields [26][27][28][29][30][31][32]. However, the black strings and p-branes constructed from the spherically symmetric BHs are generally unstable, this is known as the Gregory-Laflamme instability [33].…”

Section: Introductionmentioning

confidence: 99%

Five-dimensional Myers-Perry black holes under massive scalar perturbation: bound states and quasinormal modes

Li,

Lu,

LiMing

et al. 2024

Phys. Scr.

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The stability of five-dimensional singly rotating Myers-Perry Black Holes against massive scalar perturbations is studied. Both the quasibound states and quasinormal modes of the massive scalar field are considered. For the quasibound states, we use an analytical method to discuss the effective potential felt by the scalar field, and found that there is no potential well outside the event horizon. Thus, singly rotating Myers-Perry Black Holes are stable against the perturbation of quasibound states of massive scalar fields. Then, we use continued fraction method based on solving a seven-term recurrence relations to compute the spectra of the quasinormal modes.For different values of the black hole rotation parameter $a$, scalar mass parameter $\mu$ and angular quantum numbers, all found quasinormal modesare damped. Besides, when the scalar mass $\mu$ becomes relatively large, the long-living quasiresonances are also found as in other rotating black hole models. Our results complement previous arguments on the stability of five-dimensional singly rotating Myers-Perry black holes against massive scalar perturbations.

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Section: Introductionmentioning

confidence: 99%

Five-dimensional Myers-Perry black holes under massive scalar perturbation: bound states and quasinormal modes

Li,

Lu,

LiMing

et al. 2024

Phys. Scr.

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show abstract

“…Recently, an analytical method based on the Descartes' rule of signs has been used to study the superradiant stability of higher dimensional RN black holes under charged massive scalar perturbation [62][63][64]. It proved that there is no black hole bombs for five-and sixdimensional (non-)extremal RN black holes under charged massive scalar perturbations and the system is superradiantly stable.…”

Section: Introductionmentioning

confidence: 99%

No black hole bomb for D-dimensional extremal Reissner–Nordstrom black holes under charged massive scalar perturbation

Huang

2022

Eur. Phys. J. C

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The superradiant stability of asymptotically flat D-dimensional extremal Reissner–Nordstrom black holes under charged massive scalar perturbation is analytically studied. Recently, an analytical method has been proposed by the author and used to prove that five and six-dimensional extremal Reissner–Nordstrom black holes are superradiantly stable under charged massive scalar perturbation. We apply this analytical method in the D-dimensional extremal Reissner–Nordstrom black hole case and prove that there is no black hole bomb for D-dimensional Reissner–Nordstrom black hole under charged massive scalar perturbation and the system is superradiantly stable.

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No black hole bomb for D -dimensional nonextremal Reissner-Nordström black holes against charged massive scalar perturbation

Huang

2024

Phys. Rev. D

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Six-dimensional non-extremal Reissner-Nordstrom black hole, charged massive scalar perturbation and black hole bomb

Cited by 3 publications

References 54 publications

Five-dimensional Myers-Perry black holes under massive scalar perturbation: bound states and quasinormal modes

Five-dimensional Myers-Perry black holes under massive scalar perturbation: bound states and quasinormal modes

No black hole bomb for D-dimensional extremal Reissner–Nordstrom black holes under charged massive scalar perturbation

No black hole bomb for D -dimensional nonextremal Reissner-Nordström black holes against charged massive scalar perturbation

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