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 which are in line with modifications of the Friedman equation in a quantum bounce, with removal of the Penrose theorem initial singularity. In line with super negative pressure being applied, so as to understand what we can present as far as H = 0 ( quantum bounce) in terms of density of the Universe. And also considering what to expect when . I.e. we have a negative energy density in Pre Planckian space-time.
Comments: 6 Pages.
[v1] 2017-02-07 10:15:33
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