2026-07-072026-07-07http://salesiana.dossiersoluciones.com/handle/123456789/202241The Brill-Lindquist time-symmetric initial-value solution for two uncharged black holes is rederived using the Hamiltonian constraint equation with Dirac delta distributions as a source for the binary black-hole field. The bare masses of the Brill-Lindquist black holes are introduced in a way which is applied, after straightforward modification, to the Misner-Linquist binary black-hole solution.LaTeX, 4 pagesGeneral Relativity and Quantum Cosmologytext