## Creating a (Quantum?) Constraint, in Pre Planckian Space-Time Early Universe Via the Einstein Cosmological Constant in a One to One and Onto Comparison Between Two Action Integrals. (Text of Talk for FFP 15, Spain November 30, 11 am-11:30 Am, Conference

**Authors:** Andrew Beckwith

** NOTE, this is a “30 minute” Communications talk approved by Jesus, of FFP15
For November 30, 2017. Presumably for the conference proceedings**
We are looking at comparison of two action integrals and we identify the Lagrangian multiplier as setting up a constraint equation (on cosmological expansion). Two action integrals, one which is connected with quantum gravity is called equivalent to another action integral, and the 2nd action integral has a Lagrangian multiplier in it. Using the idea of a Lagrangian multiplier as a constraint equation, we draw our conclusions in a 1 to 1 and onto assumed equivalence between the two action integrals. The viability of the 1 to 1 and onto linkage between the two action integrals is open to question, but if this procedure is legitimate , the conclusions so assumed are fundamentally important. We also state this procedure should be streamed toward giving substance to the paper entitled “Fast optimization algorithms and the cosmological constant”, by Ning Bao, et.al.2017 , as a way to find conditions for restricting the size of the cosmological constant to be of 10^ - 120 for reasons we discuss as a future works project. We come up with relic GW which are after 65 e folds of inflationary expansion leading to 10 ^ 36 GHz high frequency GW being possible at the site of formation of the 10^-120 sized cosmological constant, for 10 GHz HFGW today. After 65 e folds of inflationary expansion
Key words, Ricci Scalar, inflaton physics.

**Comments:** 9 Pages. FFP 15 talk, half an hour, November 30, 11-11:30 AM

**Download:** **PDF**

### Submission history

[v1] 2017-11-19 00:11:03

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