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Hairy rotating black holes in cubic Galileon theory

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arxiv 1910.08451 v2 pith:OMN7ZVGJ submitted 2019-10-18 gr-qc

Karim Van Aelst , Eric Gourgoulhon , Philippe Grandclément , Christos Charmousis This is my paper · ORCID
classification gr-qc
keywords blackholescubicgalileonkerrrotatingtheoryangular
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abstract

Numerical solutions for asymptotically flat rotating black holes in the cubic Galileon theory are presented. These black holes are endowed with a nontrivial scalar field and exhibit a non-Schwarzschild behaviour: faster than $1/r$ convergence to Minkowski spacetime at spatial infinity and hence vanishing of the Komar mass. The metrics are compared with the Kerr metric for various couplings and angular velocities. Their physical properties are extracted and show significant deviations from the Kerr case.

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  1. Compact Objects in Einstein-scalar-Gauss-Bonnet Theory and beyond

    gr-qc 2024-12 unverdicted novelty 2.0 of 10

    A review of compact-object solutions in Einstein-scalar-Gauss-Bonnet and Horndeski theories, emphasizing scalarized black holes, traversable wormholes, and bubble-like particle solutions.

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