Author(s)

Andrew Beckwith

Physics Department, College of Physics, Chongqing University, Chongqing, China.

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.

Minimum Scale Factor, Cosmological Constant, Space-Time Bubble, Bouncing Cosmologies

Beckwith, A. (2021) Looking at Quantization of a Wave Function, from Weber (1961), to Signals from Wavefunctions at the Mouth of a Wormhole. Journal of High Energy Physics, Gravitation and Cosmology, 7, 1037-1048. doi: 10.4236/jhepgc.2021.73062.