Investigating Initial Conditions of the WdW Equation in Flat Space in a Transition from the Pre-Planckian Physics Era to the Electroweak Regime of Space-Time

Andrew W. Beckwith

Physics Department, Chongqing University, Chongqing, China.

DOI: 10.4236/jmp.2012.329165                

Abstract

This document is due to reviewing an article by Maydanyuk and Olkhovsky, of a Nova Science conpendium as of “The big bang, theory assumptions and Problems”, as of 2012, which uses the Wheeler De Witt equation as an evolution equation assuming a closed universe. Having the value of k, not as the closed universe, but nearly zero of a nearly flat universe, which leads to serious problems of interpretation of what initial conditions are. These problems of interpretations of initial conditions tie in with difficulties in using QM as an initial driver of inflation. And argue in favor of using a different procedure as far as forming a wave function of the universe initially. The author wishes to thank Abhay Ashtekar for his well thought out criticism but asserts that limitations in space-time geometry largely due to when is formed from semi classical reasoning, i.e. Maxwell’s equation involving a close boundary value regime between Octonionic geometry and flat space non Octonionic geometry is a datum which Abhay Ashekhar may wish to consider in his quantum bounce model and in loop quantum gravity in the future.

Keywords

Wheeler De Witt Equation; Planck’s Constant; Wavefunction of the Universe; Octonionic Geometry; Quantum Mechanics

Conflicts of Interest

The authors declare no conflicts of interest.

References

[1]	S. Maydanyuk and V. Olkhovsky, “ Fully Quantum Study of the FRW Model with Radiation and Chaplygin Gas,” In: J. O’Connell and A. Hale, Eds., The Big Bang, Theory, Assumptions and Problems, Nova Science Publishers, New York, 2012, pp. 185-196.
[2]	M. Maggiore, “Gravitational Waves, Volume 1: Theory and Experiment,” Oxford University Press, Oxford, 2008.
[3]	G. A. Monerat, et al., “Dynamics of the Early Universe and the Initial Conditions for Inflation in a Model with Radiation and a Chaplygin Gas,” Physical Review D, Vol. 76, No. 2, 2007, p. 024017. doi:10.1103/PhysRevD.76.024017
[4]	A. Ashtekar, “Private Communications with the Author,” Monday 9 July 2012.
[5]	A. Beckwith, “Is Quantum Mechanics Involved at the Start of Cosmological Evolution? Does a Machian Relationship Between Gravitons and Gravitinos Answer This Question?” 2012. http://vixra.org/abs/1206.0023
[6]	A. W. Beckwith, “Is There a Change in the Baryonic Structure Formation if Quark Strings and Domain Walls Exist at About the Electro-Weak Era?” 2012. http://vixra.org/abs/1207.0034
[7]	U. Bruchholz, “Derivation of Planck’s Constant from Maxwell’s Electrodynamics,” Progress in Physics, Vol. 4, 2009, p. 67.
[8]	U. Bruzchholz, “Key Notes on a Geometric Theory of Fields,” Progress in Physics, Vol. 2, 2009, pp. 107-113.
[9]	G. ‘t Hooft, “Determinism beneath Quantum Mechanics,” In: Beyond the Quantum, Th. M. Nieuwenhuizen, et al., Eds., World Press Scientific, Singapore, 2002. http://arxiv.org/PS_cache/quant-ph/pdf/0212/0212095v1.pdf
[10]	G. ‘t Hooft, “The Mathematical Basis for Deterministic Quantum Mechanics,” In: Beyond the Quantum, Th. M. Nieuwenhuizen, et al., Eds., World Press Scientific, Singapore, 2006. http://arxiv.org/PS_cache/quant-ph/pdf/0604/0604008v2.pdf