Black holes in a Chaplygin-like dark fluid have an upper charge bound for horizons of Q ≈ 0.556 M and a critical fluid parameter bound B_c Q_c^4 = 4/3^9 for multi-horizon solutions, with stronger curvature than RNdS.
First Sagittarius A* Event Horizon Telescope Results. VII. Polarization of the Ring,
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Causal structure of black holes immersed in a Chaplygin-like dark fluid environment: Horizons and singularities
Black holes in a Chaplygin-like dark fluid have an upper charge bound for horizons of Q ≈ 0.556 M and a critical fluid parameter bound B_c Q_c^4 = 4/3^9 for multi-horizon solutions, with stronger curvature than RNdS.