Quantum Gravity and String Theory

    

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

Authors: Andrew W. Beckwith

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 Eq. (3) and Eq,. (4). From there we will read in a way to describe conditions allowing for where the cosmological constant may be set. The ideaalso is to describe a regime of space-time where the initial perturbation/ start to inflation actually occurred, as is alluded to in thefinal part of the document.

Comments: 7 Pages. submitted to JHEPGC for evaluation

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Submission history

[v1] 2022-09-27 01:53:53

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