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No nonminimally coupled massless scalar hair for spherically symmetric neutral black holes
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We provide a remarkably compact proof that spherically symmetric neutral black holes cannot support static nonminimally coupled massless scalar fields. The theorem is based on causality restrictions imposed on the energy-momentum tensor of the fields near the regular black-hole horizon.
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Non-equatorial scalar rings supported by rapidly spinning Gauss-Bonnet black holes
For Kerr spins above a critical threshold near 0.78, the most negative value of the Gauss-Bonnet invariant is reached at non-equatorial polar angles, which the author identifies as the location of supported massive sc...
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