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We perform general-relativistic simulations of charged black holes targetingGW150914. We show that the inspiral is most efficient for detecting black holecharge through gravitational waves and that GW150914 is compatible with havingcharge-to-mass ratio as high as 0.3. Our work applies to electric and magneticcharge, and to theories with black holes endowed with U(1) (hidden or dark)charges. Using our results we place an upper bound on the deviation fromgeneral relativity in the dynamical, strong-field regime of the so-calledtheory of MOdified Gravity (MOG).

General relativistic simulations of the quasi-circular inspiral and merger of charged black holes: GW150914 and fundamental physics implications