We Begin with a “Trivial” Condition on Massive Gravitons, and Use That to Examine Nonsingular Starts to Inflation, for GW, with GW Strength and Possible Polarization States?

Abstract

Our Methodology is to construct using a "trivial" solution to massive gravitons, and a nonsingular start for expansion of the universe. Our methodology has many unintended consequences, not the least is a relationship between a small time step, t, the minimum scale factor and even the tension or property values of the initial space-time wall, and that is a consequence of a "trivial" solution taking into account "massive" gravitons. I.e. this solution has a mass How to cite this paper: Beckwith, A.W.

How Kieffer Density Matrix Formalism Aids Different Initial Time Steps, Leading to Lorentz Violations, and Breakup of Primordial Black Holes for GW Generation

“…Journal of High Energy Physics, Gravitation and Cosmology Furthermore, we have from applying a reference from the author, [21] and [22], using pages 212-213 of reference [22] ( )…”