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Shalyt-Margolin, A.E. (2005) Chapter 2. The Density Matrix Deformation in Physics of the Early Universe and Some of Its Implications. Quantum Cosmology Research Trends. In: Horizons in World Physics, Vol. 246, Nova Science Publishers, Inc., Hauppauge, 49-91.

has been cited by the following article:

• TITLE: How to Use Starobinsky Inflationary Potential Plus Argument from Alder, Bazin, and Schiffer as Radial Acceleration to Obtain First Order Approximation as to Where/When Cosmological Constant May Form

  AUTHORS: Andrew Walcott Beckwith

  KEYWORDS: Radial Acceleration, Cosmological Constant, Raviton

  JOURNAL NAME: Journal of High Energy Physics, Gravitation and Cosmology, Vol.8 No.4, October 13, 2022

  ABSTRACT: Using the Klauder enhanced quantization as a way to specify the cosmological constant as a baseline for the mass of a graviton, we eventually come up and then we will go to the Starobinsky potential as a replacement for the term N used in Equation (3) and Equation (4). From there we will read in a way to describe conditions allowing for where the cosmological constant may be set. The idea also is to describe a regime of space-time where the initial perturbation/start to inflation actually occurred, as is alluded to in the final part of the document.