Beckwith, A. (2016) Can Thermal Input from a Prior Universe Account for Relic Graviton Production and Imply Usage of the Bogomolnyi Inequality, as a Bridge between Brane World Models and Loop Quantum Gravity in Early Universe Conditions? Journal of High Energy Physics, Gravitation and Cosmology, 2, 412-431.
https://doi.org/10.4236/jhepgc.2016.23036

has been cited by the following article:

• TITLE: Examination of h(x) Real Field of Higgs Boson as Originating in Pre-Planckian Space-Time Early Universe

  AUTHORS: Andrew Walcott Beckwith

  KEYWORDS: Inflaton Physics, Modified HUP, Higgs Boson

  JOURNAL NAME: Journal of High Energy Physics, Gravitation and Cosmology, Vol.3 No.1, December 20, 2016

  ABSTRACT: We initiate working with Peskin and Schroder’s quantum field theory (1995) write up of the Higgs boson, which has a scalar field write up for Phi , with “lower part” of the spinor having h(x) as a real field, with in spatial averaging. Our treatment is to look at the time component of this h(x) as a real field in Pre-Planckian space-time to Planckian Space-time evolution, in a unitarity gauge specified potential , using a fluctuation evolution equation of the form which is in turn using with this being a modified form of the Heisenberg Uncertainty principle in Pre-Planckian space-time. From here, we can identify the formation of in the Planckian space-time regime. The inflaton is based upon Padmanabhan’s treatment of early universe models, in the case that the scale factor, and t a time factor. The initial value of the scale factor is supposed to represent a quantum bounce, along the lines of Camara, de Garcia Maia, Carvalho, and Lima, (2004) as a non zero initial starting point for expansion of the universe, using the ideas of nonlinear electrodynamics (NLED). And from there isolating .