Slowly rotating black holes in Einstein-æther theory

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Slowly rotating black holes in Einstein-æther theory

We study slowly rotating, asymptotically flat black holes in Einstein-æther 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 indepen...

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Bibliographic Details
Main Authors:	Barausse, Enrico, Sotiriou, Thomas P., Vega, Ian
Format:	Article
Published:	American Physical Society 2016
Online Access:	https://eprints.nottingham.ac.uk/39495/

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