## Is a Vev Due to the Bunch-Davies Vacuum Fluctuation a Way to Obtain Octonionic Quantum Gravity in the Planckian Regime of Space Time? Yes, But Only After Planck Time T_{planck}

**Authors:** Andrew Beckwith, L Glinka

Linking a shrinking prior universe via a wormhole solution for a pseudo time dependent Wheeler-De Witt
equation permits the formation of a short-term quintessence scalar field. We claim that our model and the addition of
the wormhole is tied to an initial configuration of the Einstein field equations, allowing for high-frequency gravitational
waves (HFGW) at the onset of inflation. We examine Bunch-Davies vacuum fluctuations[1] of a scalar field,
(see paper for equation), if we use the wave function for an average value of the Hubble parameter
(see paper for equation) , with VeV resulting from Ψ of a pseudo time dependent WdW wave
function [2],[3], and H from initial values of the Friedman equation. The benefit from defining the
Bunch-Davies vacuum fluctuation this way is that there would be a way to obtain partial time evolution of the VeV
and also to ask if Octonionic quantum gravity[2] constructions are relevant in the Planckian regime of
space time.

**Comments:** 15 pages

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### Submission history

[v1] 18 Oct 2010

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