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If at least one of the members of a compact binary coalescence is charged,the inspiral of the two members would generate a Poynting flux with anincreasing power, giving rise to a brief electromagnetic counterpart temporallyassociated with the chirp signal of the merger (with possibly a small temporaloffset), which we term as the {\em charged Compact Binary Coalescence} (cCBC)signal. We develop a general theory of cCBC for any mass and amount of chargefor each member. Neutron stars (NSs), as spinning magnets, are guaranteed to becharged, so the cCBC signal should accompany all neutron star mergers. The cCBCsignal is clean in a BH-NS merger with a small mass ratio ($q \equiv m_2/m_1 <0.2$), in which the NS plunges into the BH as a whole, and itsluminosity/energy can reach that of a fast radio burst if the NS is Crab-like.The strength of the cCBC signal in Extreme Mass Ratio Inspiral Systems (EMRIs)is also estimated.

Charged Compact Binary Coalescence Signal and Electromagnetic Counterpart of Plunging BH-NS mergers