Hairy rotating black holes in cubic Galileon theory
arXiv:1910.08451 · doi:10.1088/1361-6382/ab6391
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 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.
arXiv comment31 pages, 9 figures; v2 minor improvements, added references, minor typos corrected, version published in Classical and Quantum Gravity
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