Massive Scalar Field Perturbations of Black Holes Surrounded by Dark Matter
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| Main Authors: | , , , |
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| Format: | Preprint |
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2023
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| _version_ | 1866929263701131264 |
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| author | Bécar, Ramón González, P. A. Papantonopoulos, Eleftherios Vásquez, Yerko |
| author_facet | Bécar, Ramón González, P. A. Papantonopoulos, Eleftherios Vásquez, Yerko |
| contents | We consider scalar field perturbations in the background of black holes immersed in perfect fluid dark matter (PFDM). We find, by using the sixth order Wentzel-Kramers-Brillouin (WKB) approximation, that the longest-lived modes are the ones with higher angular number, for a scalar field mass smaller than a critical value, known as anomalous decay rate of the quasinormal modes, while that beyond this critical value the behaviour is inverted. Moreover, we show that it is possible to recover the real part of the quasinormal frequencies (QNFs), the imaginary part of the QNFs, and the critical scalar field mass, of the Schwarzschild background for different values of the PFDM intensity parameter $k$, respectively. For values of $k$ smaller than these values, the mentioned quantities are greater than the Schwarzschild background. However, beyond of these values of $k$, these quantities are smaller than the Schwarzschild background. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2310_00857 |
| institution | arXiv |
| publishDate | 2023 |
| record_format | arxiv |
| spellingShingle | Massive Scalar Field Perturbations of Black Holes Surrounded by Dark Matter Bécar, Ramón González, P. A. Papantonopoulos, Eleftherios Vásquez, Yerko General Relativity and Quantum Cosmology High Energy Physics - Theory We consider scalar field perturbations in the background of black holes immersed in perfect fluid dark matter (PFDM). We find, by using the sixth order Wentzel-Kramers-Brillouin (WKB) approximation, that the longest-lived modes are the ones with higher angular number, for a scalar field mass smaller than a critical value, known as anomalous decay rate of the quasinormal modes, while that beyond this critical value the behaviour is inverted. Moreover, we show that it is possible to recover the real part of the quasinormal frequencies (QNFs), the imaginary part of the QNFs, and the critical scalar field mass, of the Schwarzschild background for different values of the PFDM intensity parameter $k$, respectively. For values of $k$ smaller than these values, the mentioned quantities are greater than the Schwarzschild background. However, beyond of these values of $k$, these quantities are smaller than the Schwarzschild background. |
| title | Massive Scalar Field Perturbations of Black Holes Surrounded by Dark Matter |
| topic | General Relativity and Quantum Cosmology High Energy Physics - Theory |
| url | https://arxiv.org/abs/2310.00857 |