Charged boson stars can form horizonless frozen states with a de Sitter interior and a Reissner-Nordstrom exterior, using either scalar self-interaction or negative Horndeski vector-tensor coupling.
Penrose: Gravitational collapse: The role of general relativity, Riv
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Frozen states of charged boson stars
Charged boson stars can form horizonless frozen states with a de Sitter interior and a Reissner-Nordstrom exterior, using either scalar self-interaction or negative Horndeski vector-tensor coupling.