Quartic scalar self-interactions reshape ergoregions, increase hair without heavier horizons for repulsive cases, and alter bifurcation structures in two spinning black holes with synchronized scalar hair and related configurations.
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Two asymptotically flat spinning black holes balanced by their self-interacting, synchronised scalar hair
Quartic scalar self-interactions reshape ergoregions, increase hair without heavier horizons for repulsive cases, and alter bifurcation structures in two spinning black holes with synchronized scalar hair and related configurations.