1 Addressing strength of GW radiation affected by additional dimensions

Abstract: We examine whether gravitational waves would be generated during the initial phase, 0δ of the universe when triggered by changes in space-time geometry; i.e. We hope to find traces of the breakdown of the Entropy/QM space-time regime during 0δ. In particular, we look at if higher dimensions affect the relative strength of GWΩ, and comment as to how this magnitude may affect opportunities for detection of GW from relic sources. In particular, we will explain the reason why GWΩ of the pre big bang model is so strong, up to 10 to the – 6 power, while the GWΩ of ordinary inflation is so weak. In relic conditions