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Guth, A. (1986) Inflationary Universe: A Possible Solution to the Horizon and Flatness Problems. In: Bernstein, J. and Feinberg, G., Eds., Of Cosmological Constants Papers in Modern Cosmology, Columbia University Press, New York, 299-320.

has been cited by the following article:

• TITLE: Pre-Octonionic to Octonionic Gravity and Could Kinetic Energy Be Larger than Potential Energy before Inflation?

  AUTHORS: Andrew Walcott Beckwith

  KEYWORDS: Octonionic Geometry, Cyclic Conformal Cosmology (Penrose), Modified HUP

  JOURNAL NAME: Journal of High Energy Physics, Gravitation and Cosmology, Vol.3 No.4, October 23, 2017

  ABSTRACT: We look at early universe space-time which is characterized by a transition from Pre-Planckian to Planckian space-time. In doing so we also invoke the geometry of Octonionic non-commutative structure and when it breaks down. Doing so is also equivalent to a speculation given earlier by the author as to the kinetic energy of Pre-Planckian space-time being significantly larger than the Potential energy, which is the opposite of what happens after the onset of Inflation, with the assumption as to how this is justified given in a (Pre- Planckian) Hubble Parameter set as of Equation (16), and we close with a comparison of this proposal with string cosmology, as represented in the 2nd reference in this paper.