Rotating stealth black holes with a cohomogeneity-1 metric
Olaf Baake, Mokhtar Hassaine

TL;DR
This paper constructs rotating stealth black hole solutions in five dimensions with scalar hair, showing invariance under disformal transformations and extending results to higher dimensions and Kerr-(A)dS cases.
Contribution
It introduces a class of rotating stealth black holes with scalar hair in higher dimensions and demonstrates their invariance under disformal transformations.
Findings
Stealth black hole solutions with scalar hair are constructed in five and higher odd dimensions.
Disformal transformations with constant disformality leave Myers-Perry metrics invariant.
Conditions for invariance of cohomogeneity-1 metrics under disformal transformations are identified.
Abstract
In five dimensions we consider a general shift symmetric and parity preserving scalar tensor action that contains up to second order covariant derivatives of the scalar field. A rotating stealth black hole solution is constructed where the metric is given by the Myers-Perry spacetime with equal momenta and the scalar field is identified with the Hamilton-Jacobi potential. This nontrivial scalar field has an extra hair associated with the rest mass of the test particle, and the solution does not require any fine tuning of the coupling functions of the theory. Interestingly enough, we show that the disformal transformation, generated by this scalar field, and with a constant degree of disformality, leaves invariant (up to diffeomorphisms) the Myers-Perry metric with equal momenta. This means that the hair of the scalar field, along with the constant disformality parameter, can be…
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