## 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

**Download:** **PDF**

### Submission history

[v1] 18 Oct 2010

**Unique-IP document downloads:** 120 times

**Add your own feedback and questions here:**

*You are equally welcome to be positive or negative about any paper but please be polite. If you are being critical you must mention at least one specific error, otherwise your comment will be deleted as unhelpful.*

*
*