Preprint Article Version 1 Preserved in Portico This version is not peer-reviewed

Looking at Quantization of a Wave Function, From Weber (1961), to Signals From Wavefunctions at the Mouth of a Wormhole

Version 1 : Received: 1 June 2021 / Approved: 2 June 2021 / Online: 2 June 2021 (09:05:37 CEST)

How to cite: Beckwith, A.W. Looking at Quantization of a Wave Function, From Weber (1961), to Signals From Wavefunctions at the Mouth of a Wormhole. Preprints 2021, 2021060057 (doi: 10.20944/preprints202106.0057.v1). Beckwith, A.W. Looking at Quantization of a Wave Function, From Weber (1961), to Signals From Wavefunctions at the Mouth of a Wormhole. Preprints 2021, 2021060057 (doi: 10.20944/preprints202106.0057.v1).

Abstract

We utilize how Weber in 1961 initiated the process of quantization of early universe fields to the problem of what may be emitted at the mouth of a wormhole. While the wormhole models are well developed, there is as of yet no consensus as to how, say GW or other signals from a wormhole mouth could be quantized, or made to be in adherence to a procedure Weber cribbed from Feynman, in 1961. In addition, we utilize an approximation for the Hubble parameter parameterized from Temperature using Sarkar’s H ~ Temperature relations, as given in the text . Finally after doing this we go to the Energy as E also ~ Temperature, and from there use E (energy) as ~ signal frequency. This gives us an idea of how to estimate frequency generated at the mouth of a wormhole.

Subject Areas

Minimum scale factor; cosmological constant; space-time bubble; bouncing cosmologies

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