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Astier, P., Guy, J., Regnault, N., Pain, R., Aubourg, E., Balam, D., et al. (2006) The Supernova Legacy Survey: Measurement of ΩM, ΩΛ and W from the First Year Data Set. Astronomy and Astrophysics, 447, 31-48. arXiv:astro-ph/0510447.

has been cited by the following article:

• TITLE: Looking at Quantization of a Wave Function, from Weber (1961), to Signals from Wavefunctions at the Mouth of a Wormhole

  AUTHORS: Andrew Beckwith

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

  JOURNAL NAME: Journal of High Energy Physics, Gravitation and Cosmology, Vol.7 No.3, July 7, 2021

  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.