Quantum Gravity and String Theory

    

Geddankenexperiment for Quark Star Idea, Quantum Wavelength Limit, Minimum Time, and Early Universe Temperature, from First Principles

Authors: A.W. Beckwith

We initially look at a non singular universe representation as given by Rovelli and Vidotto, in terms of a quantum bounce, via quark stars, as a start of how to estimate of entropy and also of the number of operations of an expanding universe. The bench mark used is, to after considering a quark star, to look at the mass of a universe, estimated, and from there, we can obtain the entropy if we look at the Schwartzshield radii of a universe, and then the radii of the universe about 380,000 years after the big bang. In the latter, we show how to get the number of operations as akin to the reasoning used by Seth Lloyd , in 2001, and also from there close with a few comments as to the ‘naturalness’ of heavy Gravity from this formulation of entropy, which is based upon a start of considering what is a Planck star, as far as minimum quantum effects in Black hole physics, and by extension early universe cosmology.

Comments: 7 Pages. Will be brought up in Marcel Grossman Meeting, Rome

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Submission history

[v1] 2015-07-02 04:14:17

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