Quartic scalar self-interactions on balanced two-spinning-black-hole configurations with hair produce ergoregion topology changes and restrict horizon mass fractions to attractive regimes only.
Olivares S´ anchez, Carlos Herdeiro, Dar´ ıo N´ u˜ nez, and Shuang-Yong Zhou
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Two asymptotically flat spinning black holes balanced by their self-interacting, synchronised scalar hair
Quartic scalar self-interactions on balanced two-spinning-black-hole configurations with hair produce ergoregion topology changes and restrict horizon mass fractions to attractive regimes only.