%0 Journal Article
%T How to Use Starobinsky Inflationary Potential Plus Argument from Alder, Bazin, and Schiffer as Radial Acceleration to Obtain First Order Approximation as to Where/When Cosmological Constant May Form
%A Andrew Walcott Beckwith
%J Journal of High Energy Physics, Gravitation and Cosmology
%P 1012-1018
%@ 2380-4335
%D 2022
%I Scientific Research Publishing
%R 10.4236/jhepgc.2022.84071
%X Using the Klauder enhanced quantization as a way to specify the cosmological constant as a baseline for the mass of a graviton, we eventually come up and then we will go to the Starobinsky potential as a replacement for the term N used in Equation (3) and Equation (4). From there we will read in a way to describe conditions allowing for where the cosmological constant may be set. The idea also is to describe a regime of space-time where the initial perturbation/start to inflation actually occurred, as is alluded to in the final part of the document.
%K Radial Acceleration
%K Cosmological Constant
%K Raviton
%U http://www.scirp.org/journal/PaperInformation.aspx?PaperID=120376