Geometry of the universe and its relation to entropy and information
dc.contributor.author | Haranas, Ioannis | |
dc.contributor.author | Gkigkitzis, Ioannis | |
dc.date.accessioned | 2020-04-02T18:11:11Z | |
dc.date.available | 2020-04-02T18:11:11Z | |
dc.date.issued | 2013-09-16 | |
dc.description.abstract | 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. | en_US |
dc.identifier.doi | 10.1155/2013/809695 | |
dc.identifier.uri | http://hdl.handle.net/10342/7781 | |
dc.title | Geometry of the universe and its relation to entropy and information | en_US |
dc.type | Article | en_US |
ecu.journal.issue | 809695 | en_US |
ecu.journal.name | Advances in Astronomy | en_US |
ecu.journal.pages | 1-4 | en_US |
ecu.journal.volume | 2013 | en_US |
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