Nonsingular FRW cosmology and nonlinear electrodynamics

2017

We are looking at what if the initial cosmological constant is inflaton value/squared which supports Corda's assumptions in the Gravity's breath Electronic Journal of theoretical physics article. We close with an idea to be worked in further detail as to density matrices and how it may relate to gravitons traversing from a Pre-Planckian to Planckian space-time regime. We will write up an idea in far greater detail in a future publication.

Section: Conclusion: Examining the Contribution Of The Inflatonmentioning

confidence: 99%

“…We will examine the consequences of these assumptions as to what this says about the NLED approximation for the initial scale factor, as given in [7].…”

Section: Using the Section 1 Materials To Isolate A Minimum Value Of Tmentioning

confidence: 99%

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Constraints, in Pre-Planckian Space-Time via Padmabhan’s &Lambda;initial&middot;H-2initial&asymp;o(1) Approximation Leading to Initial Inflaton Constraints and Its Relation to Early Universe Graviton Production

2017

“…This could, in the minimum radii expected by a quantum induced scale factor, min a [13] [14], as well as the details of [15] as to how to form tt g , lead to in time to, if we take the minimum uncertainty given by Equation. Equation (16) leads to making the following equivalence, i.e.…”

Section: Conclusion Looking At Arguments As To Applying Equation (1mentioning

confidence: 99%

Is Temperature Quenching in the Early Universe Due to Particle Production, Or Quantum Occupation States, Or the Influence of Quantum Teleportation?

2018

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.

“…Here, we have that min a is a minimum value of the scale factor presumably given by [2] as a tiny but non zero value. Or at least a quantum bounce as given by [1].…”

Section: Specifying the Particulars Of The Two First Integrals In Prementioning

confidence: 99%

Creating a (Quantum?) Constraint, in Pre Planckian Space-Time Early Universe via the Einstein Cosmological Constant in a One to One and Onto Comparison between Two Action Integrals

2017

We are looking at comparison of two action integrals and we identify the Lagrangian multiplier as setting up a constraint equation (on cosmological expansion). Two action integrals, one which is connected with quantum gravity is called equivalent to another action integral, and the 2 nd action integral has a Lagrangian multiplier in it. Using the idea of a Lagrangian multiplier as a constraint equation, we draw our conclusions in a 1 to 1 and onto assumed equivalence between the two action integrals. The viability of the 1 to 1 and onto linkage between the two action integrals is open to question, but if this procedure is legitimate, the conclusions so assumed are fundamentally important.