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An exact black hole spacetime with scalar field and its shadow together with quasinormal modes

Shuang Yu
(
- NAOC, Beijing and
- Beijing, GUCAS
)
,
Changjun Gao
(
- NAOC, Beijing and
- Beijing, GUCAS
)

Jan 4, 2020

17 pages

Published in:

Mod.Phys.Lett.A 35 (2020) 31, 2050256

Published: Aug 6, 2020

e-Print:

2001.01137 [gr-qc]

DOI:

10.1142/S0217732320502569 (publication)

View in:

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Abstract: (WSP)

We find an exact black hole solution with a minimally coupled scalar field. The corresponding spacetime has two horizons and one of them is the black hole event horizon and the other is the cosmic horizon. In this sense, the solution is analogous to the Schwarzschild-de Sitter (or anti-de Sitter) spacetime. We investigate the thermodynamics and construct the first law of thermodynamics. At the same time, we make a study on the shadow and quasinormal modes of this black hole solution.

Note:

9 pages, 4 figures

04.70.Bw
04.20.Jb
04.40.-b
11.27.+d
Black hole solution
quasinormal modes
scalar field
black hole shadow
thermodynamics
field theory: scalar

References(150)

Figures(4)

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