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| Format: | Preprint |
| Publié: |
2024
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| Accès en ligne: | https://arxiv.org/abs/2410.04306 |
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| _version_ | 1866929529441746944 |
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| author | Malik, Zainab |
| author_facet | Malik, Zainab |
| contents | By employing an expansion in terms of the inverse multipole number, we derive analytic expressions for the quasinormal modes (QNMs) of scalar, Dirac, and Maxwell perturbations in the Hayward black hole (BH) background. The metric has three interpretations: as a model for a radiating BH, as a quantum-corrected BH owing to the running gravitational coupling in the Asymptotically Safe Gravity, and as a BH solution in the Effective Field Theory. We show that the obtained compact analytical formulas approximate QNMs with remarkable accuracy for $\ell > 0$. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2410_04306 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | Analytical QNMs of fields of various spin in the Hayward spacetime Malik, Zainab General Relativity and Quantum Cosmology By employing an expansion in terms of the inverse multipole number, we derive analytic expressions for the quasinormal modes (QNMs) of scalar, Dirac, and Maxwell perturbations in the Hayward black hole (BH) background. The metric has three interpretations: as a model for a radiating BH, as a quantum-corrected BH owing to the running gravitational coupling in the Asymptotically Safe Gravity, and as a BH solution in the Effective Field Theory. We show that the obtained compact analytical formulas approximate QNMs with remarkable accuracy for $\ell > 0$. |
| title | Analytical QNMs of fields of various spin in the Hayward spacetime |
| topic | General Relativity and Quantum Cosmology |
| url | https://arxiv.org/abs/2410.04306 |