Varying Constants Entropic-ΛCDM Cosmology

We formulate the basic framework of thermodynamical entropic force cosmology which allows variation of the gravitational constant G and the speed of light c. Three different approaches to the formulation of the field equations are presented. Some cosmological solutions for each framework are given a...

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Main Authors: Mariusz P. Da̧browski, Hussain Gohar, Vincenzo Salzano
Format: Article
Language:English
Published: MDPI AG 2016-02-01
Series:Entropy
Subjects:
Online Access:http://www.mdpi.com/1099-4300/18/2/60
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spelling doaj-c92a7b7e82b243458fd78cee028100f92020-11-25T00:11:57ZengMDPI AGEntropy1099-43002016-02-011826010.3390/e18020060e18020060Varying Constants Entropic-ΛCDM CosmologyMariusz P. Da̧browski0Hussain Gohar1Vincenzo Salzano2Institute of Physics, University of Szczecin, Wielkopolska 15, 70-451 Szczecin, PolandInstitute of Physics, University of Szczecin, Wielkopolska 15, 70-451 Szczecin, PolandInstitute of Physics, University of Szczecin, Wielkopolska 15, 70-451 Szczecin, PolandWe formulate the basic framework of thermodynamical entropic force cosmology which allows variation of the gravitational constant G and the speed of light c. Three different approaches to the formulation of the field equations are presented. Some cosmological solutions for each framework are given and one of them is tested against combined observational data (supernovae, BAO, and CMB). From the fit of the data, it is found that the Hawking temperature numerical coefficient γ is two to four orders of magnitude less than usually assumed on the geometrical ground theoretical value of O(1) and that it is also compatible with zero. In addition, in the entropic scenario, we observationally test that the fit of the data is allowed for the speed of light c growing and the gravitational constant G diminishing during the evolution of the universe. We also obtain a bound on the variation of c to be Δc / c ∝ 10-5 > 0 , which is at least one order of magnitude weaker than the quasar spectra observational bound.http://www.mdpi.com/1099-4300/18/2/60varying constantsentropic forcegravitational thermodynamics
collection DOAJ
language English
format Article
sources DOAJ
author Mariusz P. Da̧browski
Hussain Gohar
Vincenzo Salzano
spellingShingle Mariusz P. Da̧browski
Hussain Gohar
Vincenzo Salzano
Varying Constants Entropic-ΛCDM Cosmology
Entropy
varying constants
entropic force
gravitational thermodynamics
author_facet Mariusz P. Da̧browski
Hussain Gohar
Vincenzo Salzano
author_sort Mariusz P. Da̧browski
title Varying Constants Entropic-ΛCDM Cosmology
title_short Varying Constants Entropic-ΛCDM Cosmology
title_full Varying Constants Entropic-ΛCDM Cosmology
title_fullStr Varying Constants Entropic-ΛCDM Cosmology
title_full_unstemmed Varying Constants Entropic-ΛCDM Cosmology
title_sort varying constants entropic-λcdm cosmology
publisher MDPI AG
series Entropy
issn 1099-4300
publishDate 2016-02-01
description We formulate the basic framework of thermodynamical entropic force cosmology which allows variation of the gravitational constant G and the speed of light c. Three different approaches to the formulation of the field equations are presented. Some cosmological solutions for each framework are given and one of them is tested against combined observational data (supernovae, BAO, and CMB). From the fit of the data, it is found that the Hawking temperature numerical coefficient γ is two to four orders of magnitude less than usually assumed on the geometrical ground theoretical value of O(1) and that it is also compatible with zero. In addition, in the entropic scenario, we observationally test that the fit of the data is allowed for the speed of light c growing and the gravitational constant G diminishing during the evolution of the universe. We also obtain a bound on the variation of c to be Δc / c ∝ 10-5 > 0 , which is at least one order of magnitude weaker than the quasar spectra observational bound.
topic varying constants
entropic force
gravitational thermodynamics
url http://www.mdpi.com/1099-4300/18/2/60
work_keys_str_mv AT mariuszpdabrowski varyingconstantsentropiclcdmcosmology
AT hussaingohar varyingconstantsentropiclcdmcosmology
AT vincenzosalzano varyingconstantsentropiclcdmcosmology
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