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Constraining extra dimensions using observations of black hole quasi-normal modes
The presence of extra dimensions generically modify the spacetime geometry of a rotating black hole, by adding an additional hair, besides the mass M and the angular momentum J, known as the ‘tidal charge’ parameter, [Formula: see text] . In a braneworld scenario with one extra spatial dimension, th...
| Autores principales: | , , |
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| Formato: | Online Artículo Texto |
| Lenguaje: | English |
| Publicado: |
Springer Berlin Heidelberg
2022
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| Materias: | |
| Acceso en línea: | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC9483322/ https://www.ncbi.nlm.nih.gov/pubmed/36158115 http://dx.doi.org/10.1140/epjc/s10052-022-10788-x |