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

Hairy rotating black holes in cubic Galileon theory