Entropy in the Present and Early Universe: New Small Parameters and Dark Energy Problem

It is demonstrated that entropy and its density play a significant role in solving the problem of the vacuum energy density (cosmological constant) of the Universe and hence the dark energy problem. Taking this in mind, two most popular models for dark energy—Holographic Dark Energy Model and Agegra...

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Main Author: Alexander Shalyt-Margolin
Format: Article
Language:English
Published: MDPI AG 2010-04-01
Series:Entropy
Subjects:
Online Access:http://www.mdpi.com/1099-4300/12/4/932/
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author Alexander Shalyt-Margolin
author_facet Alexander Shalyt-Margolin
author_sort Alexander Shalyt-Margolin
collection DOAJ
description It is demonstrated that entropy and its density play a significant role in solving the problem of the vacuum energy density (cosmological constant) of the Universe and hence the dark energy problem. Taking this in mind, two most popular models for dark energy—Holographic Dark Energy Model and Agegraphic Dark Energy Model—are analysed. It is shown that the fundamental quantities in the first of these models may be expressed in terms of a new small dimensionless parameter that is naturally occurring in High Energy Gravitational Thermodynamics and Gravitational Holography (UV-limit). On this basis, the possibility of a new approach to the problem of Quantum Gravity is discussed. Besides, the results obtained on the uncertainty relation of the pair “cosmological constant–volume of space-time”, where the cosmological constant is a dynamic quantity, are reconsidered and generalized up to the Generalized Uncertainty Relation.
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spelling doaj.art-12c6cec6b13c431babf88eb2cd0d216b2022-12-22T04:24:58ZengMDPI AGEntropy1099-43002010-04-0112493295210.3390/e12040932Entropy in the Present and Early Universe: New Small Parameters and Dark Energy ProblemAlexander Shalyt-MargolinIt is demonstrated that entropy and its density play a significant role in solving the problem of the vacuum energy density (cosmological constant) of the Universe and hence the dark energy problem. Taking this in mind, two most popular models for dark energy—Holographic Dark Energy Model and Agegraphic Dark Energy Model—are analysed. It is shown that the fundamental quantities in the first of these models may be expressed in terms of a new small dimensionless parameter that is naturally occurring in High Energy Gravitational Thermodynamics and Gravitational Holography (UV-limit). On this basis, the possibility of a new approach to the problem of Quantum Gravity is discussed. Besides, the results obtained on the uncertainty relation of the pair “cosmological constant–volume of space-time”, where the cosmological constant is a dynamic quantity, are reconsidered and generalized up to the Generalized Uncertainty Relation.http://www.mdpi.com/1099-4300/12/4/932/dark energydeformed quantum theorynew small parameters
spellingShingle Alexander Shalyt-Margolin
Entropy in the Present and Early Universe: New Small Parameters and Dark Energy Problem
Entropy
dark energy
deformed quantum theory
new small parameters
title Entropy in the Present and Early Universe: New Small Parameters and Dark Energy Problem
title_full Entropy in the Present and Early Universe: New Small Parameters and Dark Energy Problem
title_fullStr Entropy in the Present and Early Universe: New Small Parameters and Dark Energy Problem
title_full_unstemmed Entropy in the Present and Early Universe: New Small Parameters and Dark Energy Problem
title_short Entropy in the Present and Early Universe: New Small Parameters and Dark Energy Problem
title_sort entropy in the present and early universe new small parameters and dark energy problem
topic dark energy
deformed quantum theory
new small parameters
url http://www.mdpi.com/1099-4300/12/4/932/
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