Is the Cosmological Constant, a “Vacuum” Field? We Explore This by Squeezing Early Universe “Coherent-Semi Classical States”, and Compare This to Energy from the Early Universe Heisenberg Uncertainty Principle

Andrew Walcott Beckwith

doi:10.4236/jhepgc.2016.24047

Andrew Walcott Beckwith

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https://doi.org/10.4236/jhepgc.2016.24047

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Our question delves into the nature of early universe vacuum fields, and if this initial vacuum field corresponds to a configuration of early universe space-time at the start of inflation. The answer as to this came out due to wanting to know if a cosmological constant, as given in the Einstein field equations is commensurate with the byproduct of squeezed states. We compare our answer, with the influx of energy as given by a modified Heinsenberg uncertainty principle, at the start of the inflationary era. The so called influx of energy is tied into the squeezed state phenomena as written up in the onset of this article. The impetus to writing this document came from Dr. Karim, in an e mail which the author relates to, in the introduction. Our claim is that the smallness of is what is driving the existence of the squeezed states.

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How to Introduce the Physics of Our InquiryDr Karim mailed the author with the following question which will be put in quotes: [1].The challenge of resolving the following question: At the Big Bang the only form of energy released is in the form of geometry—gravity
We will review first an HUP used in the initial configuration of space-time and tie it into initial squeezed states, and from there ask about forming an initial vacuum field
The work done in [2] is relevant to [3] where we look at how worm holes connect gravitational waves, as far as initial vacuum states

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How to Introduce the Physics of Our InquiryDr Karim mailed the author with the following question which will be put in quotes: [1].The challenge of resolving the following question: At the Big Bang the only form of energy released is in the form of geometry—gravity. Answering this question delves into what the initial state of the universe should be, in terms of a flux of energy and space-time, and how this relates to squeezed states.

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