Is Temperature Quenching in the Early Universe Due to Particle Production, Or Quantum Occupation States, Or the Influence of Quantum Teleportation? ()
ABSTRACT
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 electroweak 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.
Share and Cite:
Beckwith, A. (2018) Is Temperature Quenching in the Early Universe Due to Particle Production, Or Quantum Occupation States, Or the Influence of Quantum Teleportation?.
Journal of High Energy Physics, Gravitation and Cosmology,
4, 60-67. doi:
10.4236/jhepgc.2018.41007.
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