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
Unique-IP document downloads: 96 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.