Quantum Gravity and String Theory


Gedankerexperiment for Contributions to Cosmological Constant Initial Conditions from Kinematic Viscosity in Non-Singular Pre Plank Space-Time

Authors: Andrew Beckwith

This paper is to address using what a fluctuation of a metric tensor leads to, in pre Planckian physics, namely . If so then, we pick the conditions for an equality, with a small , to come up with restraints initial temperature, particle count and entropy as would be affected by a small nonsingular region of space-time. The resulting density will be of the form with the first term, on the right viscosity, of space-time, the 2nd on the right the square of an initial expansion rate, and due to the non singular nature of initial space time the fourth power of a scale factor, with This leads to an initial graviton production due to a minimum magnetic field, as established in our analysis. Which we relate to the inflaton as it initially would be configured and evaluated; with , and with the change in the initial cosmological constant Keywords: Emergent time, heavy gravity, metric tensor perturbations, HUP

Comments: 8 Pages.

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Submission history

[v1] 2017-02-01 16:20:13

Unique-IP document downloads: 16 times

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