2026-07-072026-07-07http://salesiana.dossiersoluciones.com/handle/123456789/109972In the framework of 4D Einstein-Maxwell Dilaton-Axion theory we show how to obtain a family of both unpolarized and polarized S^1XS^2 Gowdy cosmological models endowed with nontrivial axion, dilaton and electromagnetic fields from a solitonic rotating black hole-type solution by interchanging the r and t coordinates in the region located between the horizons of the black hole configuration. We also get a family of Kantowski-Sachs cosmologies with topology R^1XS^2 from the polarized Gowdy cosmological models by decompactifying one of the compact dimensions.7 pages in latex, no figures, Talk presented at the V Mexican Workshop on Gravitation and Mathematical Physics, Morelia, Michoacan, Mexico, November 24-28, 2003High Energy Physics - Theorytext