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 scalar rings.
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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 scalar rings.