Gravitational Tidal Deformations of Rotating Black Holes.
Black holes are influenced by external gravitational fields in the universe, which are generated by other astrophysical objects in their surroundings. Because of this gravitational interaction, they experience tidal deformations of their event horizons. To quantify this effect, we compute the so-cal...
| Publicado en: | Journal of the Utah Academy of Sciences, Arts & Letters Vol. 102; p. 379 |
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| Autores principales: | , , , , , |
| Formato: | Artículo |
| Publicado: |
Utah Academy of Sciences, Arts & Letters
2025
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| Materias: | |
| Acceso en línea: | Ver este registro en EBSCOhost |