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• W2207535356 abstract "We study slowly rotating, asymptotically flat black holes in Einstein-ae{}ther theory and show that solutions that are free from naked finite area singularities form a two-parameter family. These parameters can be thought of as the mass and angular momentum of the black hole, while there are no independent ae{} ther charges. We also show that the ae{} ther has nonvanishing vorticity throughout the spacetime, as a result of which there is no hypersurface that resembles the universal horizon found in static, spherically symmetric solutions. Moreover, for experimentally viable choices of the coupling constants, the frame-dragging potential of our solutions only shows percent-level deviations from the corresponding quantities in General Relativity and Hoifmmode check{r}else v{r}fi{}ava gravity. Finally, we uncover and discuss several subtleties in the correspondence between Einstein-ae{}ther theory and Hoifmmode check{r}else v{r}fi{}ava gravity solutions in the ${c}_{ensuremath{omega}}ensuremath{rightarrow}ensuremath{infty}$ limit." @default.
• W2207535356 created "2016-06-24" @default.
• W2207535356 creator A5007046394 @default.
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• W2207535356 date "2016-02-16" @default.
• W2207535356 modified "2023-10-14" @default.
• W2207535356 title "Slowly rotating black holes in Einstein-æther theory" @default.
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• W2207535356 doi "https://doi.org/10.1103/physrevd.93.044044" @default.
• W2207535356 hasPublicationYear "2016" @default.
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