We study a model of quantum cosmology originating from a classical model of
gravitation where a self interacting scalar field is coupled to gravity with
the metric undergoing a signature transition. We show that there are dual
classical signature changing solutions, one at large scales and the other at
small scales. It is possible to fine-tune the physics in both scales with an
infinitesimal effective cosmological constant.Comment: 10 pages, LaTeX, To appear in Phys. Lett.