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?

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. A Introduction We start off with a treatment of entropy initially using Muller and Loustos results [1] as of 2007 as to black hole entropy and also the entropy of the early universe. Afterwards, we refer to a paper by Crowell [2] as to a treatment of black hole entropy and a partition function argument which we generalize to work with early entropy. In dong so, we also refer to an argument given by Park et al [3] as far as the temperature dependence of the vacuum energy via quintessence ( string theory result) to come up with an early universe model as far as how to isolate temperature of the early universe. Once this is done, the next step will be, seeing that this derived temperature, which is decreased by a certain amount depending upon energy, numerical count and also other factors while being divided by a time interval to a given power. This relationship as stated establishes the role which nucleation of particles or essential quanta plays in lowering temperature. Afterwards, the author initiates a discuxsion as to what role a re interpretation of the HUP as far as uncertainty may play as far as