How can Brane World physics influence Axion temperature dependence, initial vacuum states, and permissible solutions to the Wheeler-De Witt equation?

TL;DR

This paper explores how brane world physics can influence the temperature dependence of axions, initial vacuum states, and solutions to the Wheeler-De Witt equation, aiming to reconcile early universe conditions with inflationary models.

Contribution

It proposes a novel approach linking brane world effects to axion physics, initial vacuum states, and quantum cosmology solutions, extending the understanding of early universe conditions.

Findings

A model connecting brane world physics with axion temperature dependence.

A framework for initial vacuum states compatible with high-temperature conditions.

Insights into solutions of the Wheeler-De Witt equation incorporating brane effects.

Abstract

We are investigating if the Jeans instability criteria mandading a low entropy,low temperature initial pre inflation state configuration can be recociled with thermal conditions of temperature at or above ten to the 12 power Kelvin, or higher,when cosmic inflation physics takes over. We justify this by pointing to the Akshenkar, Pawlowski, and Singh (2006) article about a prior universe being modeled via their quantum bounce which states that this prior universe geometrically can be modeled via a discretized Wheeler - De Witt equation. This allows a way of getting around the fact that conventional cosmological CMB is limited by a barrier as of a red shift limit of about z = 1000,as to photons, and to come up with a working model of quintessence scalar fields which permits relic generation of dark matter/dark energy as well as relic gravitons.