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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 .

journal of high energy physics gravitation and cosmology

Examination of &amp;lt;i&amp;gt;h&amp;lt;/i&amp;gt;(&amp;lt;i&amp;gt;x&amp;lt;/i&amp;gt;) Real Field of Higgs Boson as Originating in Pre-Planckian Space-Time Early Universe