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 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 ,, 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 constructions are relevant in the Planckian regime of space time.
Comments: 15 pages
[v1] 18 Oct 2010
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