In this work, we study the implications of GW230529 on gravity theories and the charge of black holes. The GW230529, which was initially released in O4a, is most likely neutron star-black hole (NSBH) mergers. We reanalyze the data from the GW230529 event to obtain bounds on the Einstein-dilation-Gauss-Bonnet (EdGB) gravity parameter √αEdGB and the electric charge of black holes. The event places a $90%$ credible upper bounds on √αEdGB of 0.298 km. After including high order corrections of EdGB gravity, the bounds improve to √αEdGB 0.260 km. Analyses of GW230529 also yield a $90%$ credible upper bounds on charge-to-mass ratio ζ 0.024. The constraints are more stringent than those derived from previously observed single gravitational wave merger event.
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Gao et al. (2024) studied this question.
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