Kommemi's nonzero asymptotic charge conjecture

Let $\mathcal{Q}^+$ be the quotient spacetime, $\mathcal{I}^+$ future null infinity, and let the black-hole asymptotic charge mean the limiting charge appearing in the model. Nonzero asymptotic charge conjecture. Among all admissible data, there exists a generic subclass such that, if $\mathcal{Q}^+\cap J^-(\mathcal{I}^+)\neq\emptyset$, then the black-hole asymptotic charge is nonzero. This is the second generic property used in the paper's late-time assumptions, and it remains open in the supplied text.