Strong cosmic censorship for the massless charged scalar field in the Reissner-Nordstrom–de Sitter spacetime - INSPIRE

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Strong cosmic censorship for the massless charged scalar field in the Reissner-Nordstrom–de Sitter spacetime

Yuyu Mo
(
- Yangzhou U. and
- Beijing Normal U.
)
,
Yu Tian
(
- Beijing, GUCAS
)
,
Bin Wang
(
- Yangzhou U. and
- Shanghai Jiaotong U.
)
,
Hongbao Zhang
(
- Beijing Normal U. and
- Intl. Solvay Inst., Brussels
)
,
Zhen Zhong
(
- Beijing Normal U.
)

Aug 10, 2018

7 pages

Published in:

Phys.Rev.D 98 (2018) 12, 124025

Published: Dec 20, 2018

e-Print:

1808.03635 [gr-qc]

DOI:

10.1103/PhysRevD.98.124025 (publication)

View in:

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Abstract: (APS)

It has recently been shown that the strong cosmic censorship conjecture can be violated by the massless neutral scalar field in the nearly extremal Reissner-Nordstrom–de Sitter black hole. However, the formation of such a black hole by gravitational collapse necessitates the presence of the charged sector on top of the Einstein-Maxwell system. Thus, we numerically calculate the quasinormal modes for a massless charged scalar field in the Reissner-Nordstrom–de Sitter spacetime by generalizing the characteristic formulation to the charged case. As a result, the strong cosmic censorship is recovered by our massless charged scalar field except in the highly extremal limit Q→Qm, where the violation still occurs when the scalar field is appropriately charged.

Note:

figures refined and added, references updated and added, version to appear in Physical Review D

General relativity, alternative theories of gravity

References(24)

Figures(11)

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