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Non-minimal Einstein-Yang-Mills black holes: fundamental quasinormal mode and grey-body factors versus outburst of overtones

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dc.rights.license CC BY eng
dc.contributor.author Lütfüoglu, Bekir Can cze
dc.date.accessioned 2025-12-05T15:43:06Z
dc.date.available 2025-12-05T15:43:06Z
dc.date.issued 2025 eng
dc.identifier.issn 1434-6044 eng
dc.identifier.uri http://hdl.handle.net/20.500.12603/2397
dc.description.abstract Recently, an exact black hole solution in non-minimal Einstein-Yang-Mills theory was obtained, and its quasinormal modes were subsequently analyzed using the JWKB approximation (Gogoi and Ponglertsakul in Eur. Phys. J. C 84:652, 2024. https://doi.org/10.1140/epjc/s10052-024-12946-9. arXiv:2402.06186 [gr-qc]). However, we demonstrate that this analysis lacks sufficient accuracy when studying modes with & ell;<= n\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$\ell \le n$$\end{document}, where & ell;\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$\ell $$\end{document} is the multipole number and n is the overtone number. To address this, we compute the quasinormal frequencies using the precise Leaver method. Our results show that while the fundamental mode deviates only slightly from the Schwarzschild value, the first few overtones exhibit significantly larger deviations, with the discrepancy growing rapidly with the overtone number. Moreover, beginning with the second overtone, we observe a striking phenomenon: the real part of the frequency tends to zero quickly as the non-minimal coupling constant increases. This combination of spectral stability in the fundamental mode and high sensitivity of the overtones suggests that the Yang-Mills contribution primarily deforms the metric in the near-horizon region, while the geometry quickly transitions back to a Schwarzschild-like form at larger radii. In addition, we compute the grey-body factors and confirm that they represent a more stable characteristic of the geometry, exhibiting a correspondence with quasinormal modes already at the first multipole. The Yang-Mills coupling enhances the grey-body factors, further increasing the transmission probability. eng
dc.format p. &quot;Article Number: 630&quot; eng
dc.language.iso eng eng
dc.publisher SPRINGER eng
dc.relation.ispartof European Physical Journal C, volume 85, issue: 6 eng
dc.subject gauss-bonnet eng
dc.subject normal frequencies eng
dc.subject stability eng
dc.subject shadow eng
dc.subject field eng
dc.title Non-minimal Einstein-Yang-Mills black holes: fundamental quasinormal mode and grey-body factors versus outburst of overtones eng
dc.type article eng
dc.identifier.obd 43882046 eng
dc.identifier.wos 001503866600002 eng
dc.identifier.doi 10.1140/epjc/s10052-025-14380-x eng
dc.publicationstatus postprint eng
dc.peerreviewed yes eng
dc.source.url https://link.springer.com/article/10.1140/epjc/s10052-025-14380-x cze
dc.relation.publisherversion https://link.springer.com/article/10.1140/epjc/s10052-025-14380-x eng
dc.rights.access Open Access eng


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