New Holographic Dark Energy Model in Brans-Dicke Theory
We study the cosmic evolution of the Bianchi type I universe by using new holographic dark energy model in the context of the Brans-Dicke theory for both non-interacting and interacting cases between dark energy and dark matter. We evaluate the equation of state for dark energy ω D a...
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doaj-afa0aa9ec9094e11b7ea272fde03a3732020-11-24T21:41:00ZengMDPI AGSymmetry2073-89942018-05-0110515310.3390/sym10050153sym10050153New Holographic Dark Energy Model in Brans-Dicke TheoryM. Sharif0Syed Asif Ali Shah1Kazuharu Bamba2Department of Mathematics, University of the Punjab, Quaid-e-Azam Campus, Lahore 54590, PakistanDepartment of Mathematics, University of the Punjab, Quaid-e-Azam Campus, Lahore 54590, PakistanDivision of Human Support System, Faculty of Symbiotic Systems Science, Fukushima University, Fukushima 960-1296, JapanWe study the cosmic evolution of the Bianchi type I universe by using new holographic dark energy model in the context of the Brans-Dicke theory for both non-interacting and interacting cases between dark energy and dark matter. We evaluate the equation of state for dark energy ω D and draw the ω D − ω ˙ D plane, where the dot denotes the time derivative. It is found that a stage in which the cosmic expansion is accelerating can be realized in both cases. In addition, we investigate the stability of the model by analyzing the sound speed. As a result, it is demonstrated that for both cases, the behavior of the sound speed becomes unstable. Furthermore, with the Om-diagnostic tool, it is shown that the quintessence region of the universe can exist.http://www.mdpi.com/2073-8994/10/5/153brans-dicke theorydark energy modelcosmological parameters |
collection |
DOAJ |
language |
English |
format |
Article |
sources |
DOAJ |
author |
M. Sharif Syed Asif Ali Shah Kazuharu Bamba |
spellingShingle |
M. Sharif Syed Asif Ali Shah Kazuharu Bamba New Holographic Dark Energy Model in Brans-Dicke Theory Symmetry brans-dicke theory dark energy model cosmological parameters |
author_facet |
M. Sharif Syed Asif Ali Shah Kazuharu Bamba |
author_sort |
M. Sharif |
title |
New Holographic Dark Energy Model in Brans-Dicke Theory |
title_short |
New Holographic Dark Energy Model in Brans-Dicke Theory |
title_full |
New Holographic Dark Energy Model in Brans-Dicke Theory |
title_fullStr |
New Holographic Dark Energy Model in Brans-Dicke Theory |
title_full_unstemmed |
New Holographic Dark Energy Model in Brans-Dicke Theory |
title_sort |
new holographic dark energy model in brans-dicke theory |
publisher |
MDPI AG |
series |
Symmetry |
issn |
2073-8994 |
publishDate |
2018-05-01 |
description |
We study the cosmic evolution of the Bianchi type I universe by using new holographic dark energy model in the context of the Brans-Dicke theory for both non-interacting and interacting cases between dark energy and dark matter. We evaluate the equation of state for dark energy ω D and draw the ω D − ω ˙ D plane, where the dot denotes the time derivative. It is found that a stage in which the cosmic expansion is accelerating can be realized in both cases. In addition, we investigate the stability of the model by analyzing the sound speed. As a result, it is demonstrated that for both cases, the behavior of the sound speed becomes unstable. Furthermore, with the Om-diagnostic tool, it is shown that the quintessence region of the universe can exist. |
topic |
brans-dicke theory dark energy model cosmological parameters |
url |
http://www.mdpi.com/2073-8994/10/5/153 |
work_keys_str_mv |
AT msharif newholographicdarkenergymodelinbransdicketheory AT syedasifalishah newholographicdarkenergymodelinbransdicketheory AT kazuharubamba newholographicdarkenergymodelinbransdicketheory |
_version_ |
1725923734382968832 |