Quantum Gravity and String Theory

    

Does Temperature Quenching in the Early Universe Exist in Part Due to Particle Production? or Quantum Occupation States? and How to Relate This to the Subsequent Deceleration Parameter? as an Open Question?

Authors: A.W. 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 contributiosn. 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 at/before the electro weak era. We hope that this temperature quenching so mentioned can be tied into the deceleration parameter as given in the appendix. I.e.how could a slow down of expansion, lead to , much later rapid increase in cosmological expansion a billion years ago.

Comments: 10 Pages. possible inclusion as a prespacetime publication

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Submission history

[v1] 2013-04-16 02:22:12

Unique-IP document downloads: 152 times

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