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Guth, A. (1982) Phase Transitions in the Early Universe. 171-204, In: Gibbons, G., Hawkin, S. and Siklos, S., Eds., The Very Early Universe, Proceedings of the Nuffield Workship, Cambridge, 21 June-9 July 1982, Cambridge University Press, 1982, Cambridge, UK.

has been cited by the following article:

• TITLE: Structure Formation and Non Linear Electrodynamics with Attendant Changes in Gravitational Potential and Its Relationship to the 3 Body Problem

  AUTHORS: Andrew Walcott Beckwith

  KEYWORDS: Inflation, Modified Gravity, 3 Body Problem

  JOURNAL NAME: Journal of High Energy Physics, Gravitation and Cosmology, Vol.4 No.4, October 24, 2018

  ABSTRACT: We find that having the scale factor close to zero due to a given magnetic field value, an early universe magnetic field affects how we would interpret Mukhanov’s chapter on “self reproduction of the universe”. We extend such arguments, and refer to the possibility of modified gravity. We hope that some of the issues raised by Kobayashi and Seto as to allowed inflation models may be addressed, once further refinement of these preliminary results commences. We close with statements as to the value of α in a gravitational potential proportional to r−α and how this adjustment affects the 3 body problem.