In the following work I intend to present a gravitational potential ϕ in a four-dimensional space, for the attempt leading to the development of a Undulatory and Geometric Theory of Gravity, whereas, for reasons of convenience and co-variance with theoretical models intended to be integrated into the standard model, it must contain the most common and known number of dimensions of a simple space; in this case the Minkowski space M(4), is chosen, since this is a very consistent one, possesses a metric ημν that is very similar to Euclidean δij, and is sufficient to define the essentials of gravitation; a second objective is to demonstrate more conciliatory and adequately the concordance and covariance with Albert Einstein's Special Theory of Relativity that was elaborated in this same space, with some quantum connections and with the classical scheme in a dimensional boundary leading to Euclidean space E (3) in which Isaac Newton developed the classical Theory of Gravitation. Keywords: Cosmology, Fields, Gravity