Recent years have seen extensive applications of the Nambu-Jona-Lasinio (NJL) model in the study of matter at high density. There is a good deal of interest in the predictions of diquark condensation and color superconductivity, with suggested applications to the study the properties of neutron stars. As the researchers in this field note, the NJL model does not describe confinement, so that one is limited to the study of the deconfined phase, which may set in at several times nuclear matter density. Recently, we have extended the NJL model to include a covariant confinement model. Our model may be used to study the properties of the full range of light mesons, including their radial excitations, in the 1-3 GeV energy domain. Most recently we have used our extended model to provide an excellent fit to the properties of the η(547) and η ′ (958) mesons and their radial excitations. The mixing angles and decay constants are given successfully in our model. In the present work our goal is to include a phenomenological model of deconfinement at finite matter density, using some analogy to what is known concerning "string breaking" and deconfinement at finite temperature. Various models may be used, but for this work we choose a specific model for the density dependence of the parameters of our confining interaction. We perform relativistic random- of the confinement potential, other than that used in this work, maybe considered in future work, particularly if we are able to obtain further insight in the dynamics of deconfinement at finite matter density.