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.
Chains of rotating boson stars with quartic or sextic self-interaction.Eur
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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.