Authors: Andrew Beckwith
We examine the role of particle nucleation in the initial universe, and argue that there is a small effect due to particle nucleation in terms of lowering initial temperature, in tandem with energy density and scale factor contributions. If such scaling exists as a major order effect, then quenching of temperature proportional to a vacuum nucleation at or before the electro weak era is heavily influenced by a number, n, which is either a quantum number (quantum cosmology) or a ‘particle count before the electro weak era. If the supposition is for a particle count, say of gravitons from a prior universe to today's universe, initially, we can compare via a thermodynamic argument compared as to a modified Heisenberg uncertainty principle as to what this says about particle count information, we have a richer cosmological picture to contend with. We close with a speculation as to how a quantum teleportation picture for Pre- Planckian space-time physics may influence our physics discussion.
Comments: 11 Pages. Cleaned up version which has been accepted by JHEPGC for publishing later
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