2026-07-072026-07-07http://salesiana.dossiersoluciones.com/handle/123456789/219311The cosmological model with two phantom scalar fields with the special choice of field's potential is considered. The obtained regular solution describes a bounce with a subsequent transition to the de Sitter stage of the expansion of the Universe. This solution also could be interpreted as a S-brane solution.one reference and new interpretation of the solution are added, and the title is changedGeneral Relativity and Quantum Cosmologytext