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 =0 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 V= c1 h(x)^2 + C2 h(x)^3 + C3 h(x)^4, using a fluctuation evolution equation of the form (d (delta h)/dt)^2 + V(delta h)= Delta E, which is in turn using (Delta E) times (Delta t) ~ h(bar)/ g(t,t), with this being a modified form of the Heisenberg Uncertainty principle in Pre-Planckian space-time. From here, we can identify the formation of delta h(x) in the Planckian space-time regime. Furthermore, it gets a special dependence upon the change in the metric tensor g(t,t)~(a(t))^2 times (inflaton). The inflaton is based upon Padmanabhan’s treatment of early universe models, in the case that the scale factor, a(t) ~ a(initial) times t ^ (beta), with beta a numerical value, and t a time factor. The a(initial) 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 delta h(x)