Geometry of the Universe and Its Relation to Entropy and Information

In an effort to investigate a possible relation between geometry and information, we establish a relation of the Ricci scalar in the Robertson-Walker metric of the cosmological Friedmann model to the number of information N and entropy S. This is with the help of a previously derive...

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Main Authors: Ioannis Haranas, Ioannis Gkigkitzis
Format: Article
Language:English
Published: Wiley 2013-01-01
Series:Advances in Astronomy
Online Access:http://dx.doi.org/10.1155/2013/809695
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author Ioannis Haranas
Ioannis Gkigkitzis
author_facet Ioannis Haranas
Ioannis Gkigkitzis
author_sort Ioannis Haranas
collection DOAJ
description In an effort to investigate a possible relation between geometry and information, we establish a relation of the Ricci scalar in the Robertson-Walker metric of the cosmological Friedmann model to the number of information N and entropy S. This is with the help of a previously derived result that relates the Hubble parameter to the number of information N. We find that the Ricci scalar has a dependence which is inversely proportional to the number of information N and entropy S. Similarly, a nonzero number of information would imply a finite Ricci scalar, and therefore space time will unfold. Finally, using the maximum number of information existing in the universe, we obtain a numerical value for the Ricci scalar to be O(10-52) m-2.
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spelling doaj-art-08a29367b41440b68da890b039d6f2562025-02-03T05:52:45ZengWileyAdvances in Astronomy1687-79691687-79772013-01-01201310.1155/2013/809695809695Geometry of the Universe and Its Relation to Entropy and InformationIoannis Haranas0Ioannis Gkigkitzis1Department of Physics and Astronomy, York University, 4700 Keele Street, Toronto, ON, M3J 1P3, CanadaDepartment of Mathematics, East Carolina University, 124 Austin Building, East Fifth Street, Greenville, NC 27858-4353, USAIn an effort to investigate a possible relation between geometry and information, we establish a relation of the Ricci scalar in the Robertson-Walker metric of the cosmological Friedmann model to the number of information N and entropy S. This is with the help of a previously derived result that relates the Hubble parameter to the number of information N. We find that the Ricci scalar has a dependence which is inversely proportional to the number of information N and entropy S. Similarly, a nonzero number of information would imply a finite Ricci scalar, and therefore space time will unfold. Finally, using the maximum number of information existing in the universe, we obtain a numerical value for the Ricci scalar to be O(10-52) m-2.http://dx.doi.org/10.1155/2013/809695
spellingShingle Ioannis Haranas
Ioannis Gkigkitzis
Geometry of the Universe and Its Relation to Entropy and Information
Advances in Astronomy
title Geometry of the Universe and Its Relation to Entropy and Information
title_full Geometry of the Universe and Its Relation to Entropy and Information
title_fullStr Geometry of the Universe and Its Relation to Entropy and Information
title_full_unstemmed Geometry of the Universe and Its Relation to Entropy and Information
title_short Geometry of the Universe and Its Relation to Entropy and Information
title_sort geometry of the universe and its relation to entropy and information
url http://dx.doi.org/10.1155/2013/809695
work_keys_str_mv AT ioannisharanas geometryoftheuniverseanditsrelationtoentropyandinformation
AT ioannisgkigkitzis geometryoftheuniverseanditsrelationtoentropyandinformation