Quasinormal Modes of a Charged Black Hole with Scalar Hair
Abstract
:1. Introduction
2. The Charged Black Hole
3. Perturbation Equations
3.1. Scalar Field
3.2. Electromagnetic Field
3.3. Gravitational Field
4. Computing QNMs
4.1. Solving Frequency
4.2. Time Evolution
5. Conclusions
Author Contributions
Funding
Data Availability Statement
Acknowledgments
Conflicts of Interest
References
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l | n | AIM | WKB | ||
---|---|---|---|---|---|
Re() | Im() | Re() | Im() | ||
0 | 0 | 0.220856 | −0.166592 | 0.219664 | −0.166443 |
1 | 0.186884 | −0.534457 | 0.193004 | −0.537457 | |
1 | 0 | 0.586476 | −0.158533 | 0.586679 | −0.158525 |
1 | 0.554754 | −0.488295 | 0.556358 | −0.487138 | |
2 | 0 | 0.967669 | −0.157641 | 0.967666 | −0.157648 |
1 | 0.946096 | −0.478040 | 0.946082 | −0.478076 |
l | n | AIM | WKB | ||
---|---|---|---|---|---|
Re() | Im() | Re() | Im() | ||
1 | 0 | 0.513377 | −0.152855 | 0.513302 | −0.153142 |
1 | 0.476438 | −0.474101 | 0.476701 | −0.537457 | |
2 | 0 | 0.924716 | −0.155637 | 0.924714 | −0.155649 |
1 | 0.901934 | −0.472399 | 0.901941 | −0.472447 | |
3 | 0 | 1.32049 | −0.156374 | 1.32049 | −0.156375 |
1 | 1.30408 | −0.471908 | 1.30408 | −0.471914 |
l | n | AIM | WKB | ||
---|---|---|---|---|---|
Re() | Im() | Re() | Im() | ||
2 | 0 | 0.810272 | −0.147554 | 0.810467 | −0.147398 |
1 | 0.785979 | −0.449209 | 0.787063 | −0.447841 | |
3 | 0 | 1.24218 | −0.152877 | 1.24220 | −0.152875 |
1 | 1.22506 | −0.461665 | 1.22529 | −0.461580 | |
4 | 0 | 1.65149 | −0.154694 | 1.65149 | −0.154694 |
1 | 1.63833 | −0.465851 | 1.63831 | −0.465856 |
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Guo, W.-D.; Tan, Q. Quasinormal Modes of a Charged Black Hole with Scalar Hair. Universe 2023, 9, 320. https://doi.org/10.3390/universe9070320
Guo W-D, Tan Q. Quasinormal Modes of a Charged Black Hole with Scalar Hair. Universe. 2023; 9(7):320. https://doi.org/10.3390/universe9070320
Chicago/Turabian StyleGuo, Wen-Di, and Qin Tan. 2023. "Quasinormal Modes of a Charged Black Hole with Scalar Hair" Universe 9, no. 7: 320. https://doi.org/10.3390/universe9070320