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...

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Bibliographic Details

Published in:	Journal of the Utah Academy of Sciences, Arts & Letters Vol. 102; p. 379
Main Authors:	Glazer, Daniel, Joyce, Austin, Rodriguez, Maria J., Santoni, Luca, Solomon, Adam R., Temoche, Luis Fernando
Format:	Article
Published:	Utah Academy of Sciences, Arts & Letters 2025
Subjects:	Black holes Kerr black holes Physical constants Spacetime
Online Access:	View this record in EBSCOhost