The Effect of de-Sitter Like Background on Increasing the Zero Point Budget of Dark Energy

During this work, using subtraction renormalization mechanism, zero point quantum fluctuations for bosonic scalar fields in a de-Sitter like background are investigated. By virtue of the observed value for spectral index, ns(k), for massive scalar field the best value for the first slow roll paramet...

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Main Authors: Haidar Sheikhahmadi, Ali Aghamohammadi, Khaled Saaidi
Format: Article
Language:English
Published: Wiley 2016-01-01
Series:Advances in High Energy Physics
Online Access:http://dx.doi.org/10.1155/2016/2594189
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author Haidar Sheikhahmadi
Ali Aghamohammadi
Khaled Saaidi
author_facet Haidar Sheikhahmadi
Ali Aghamohammadi
Khaled Saaidi
author_sort Haidar Sheikhahmadi
collection DOAJ
description During this work, using subtraction renormalization mechanism, zero point quantum fluctuations for bosonic scalar fields in a de-Sitter like background are investigated. By virtue of the observed value for spectral index, ns(k), for massive scalar field the best value for the first slow roll parameter, ϵ, is achieved. In addition, the energy density of vacuum quantum fluctuations for massless scalar field is obtained. The effects of these fluctuations on other components of the universe are studied. By solving the conservation equation, for some different examples, the energy density for different components of the universe is obtained. In the case which all components of the universe are in an interaction, the different dissipation functions, Q~i, are considered. The time evolution of ρDE(z)/ρcri(z) shows that Q~=3γH(t)ρm has the best agreement in comparison to observational data including CMB, BAO, and SNeIa data set.
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spelling doaj-art-3b1ec99fe6a0454a9ad529d81888dc0b2025-02-03T01:02:42ZengWileyAdvances in High Energy Physics1687-73571687-73652016-01-01201610.1155/2016/25941892594189The Effect of de-Sitter Like Background on Increasing the Zero Point Budget of Dark EnergyHaidar Sheikhahmadi0Ali Aghamohammadi1Khaled Saaidi2Institute for Advanced Studies in Basic Sciences (IASBS), Gava Zang, Zanjan 45137-66731, IranIslamic Azad University, Sanandaj Branch, Pasdaran Street, P.O. Box 618, Sanandaj, IranDepartment of Physics, Faculty of Science, University of Kurdistan, Pasdaran Street, Sanandaj 66177-15175, IranDuring this work, using subtraction renormalization mechanism, zero point quantum fluctuations for bosonic scalar fields in a de-Sitter like background are investigated. By virtue of the observed value for spectral index, ns(k), for massive scalar field the best value for the first slow roll parameter, ϵ, is achieved. In addition, the energy density of vacuum quantum fluctuations for massless scalar field is obtained. The effects of these fluctuations on other components of the universe are studied. By solving the conservation equation, for some different examples, the energy density for different components of the universe is obtained. In the case which all components of the universe are in an interaction, the different dissipation functions, Q~i, are considered. The time evolution of ρDE(z)/ρcri(z) shows that Q~=3γH(t)ρm has the best agreement in comparison to observational data including CMB, BAO, and SNeIa data set.http://dx.doi.org/10.1155/2016/2594189
spellingShingle Haidar Sheikhahmadi
Ali Aghamohammadi
Khaled Saaidi
The Effect of de-Sitter Like Background on Increasing the Zero Point Budget of Dark Energy
Advances in High Energy Physics
title The Effect of de-Sitter Like Background on Increasing the Zero Point Budget of Dark Energy
title_full The Effect of de-Sitter Like Background on Increasing the Zero Point Budget of Dark Energy
title_fullStr The Effect of de-Sitter Like Background on Increasing the Zero Point Budget of Dark Energy
title_full_unstemmed The Effect of de-Sitter Like Background on Increasing the Zero Point Budget of Dark Energy
title_short The Effect of de-Sitter Like Background on Increasing the Zero Point Budget of Dark Energy
title_sort effect of de sitter like background on increasing the zero point budget of dark energy
url http://dx.doi.org/10.1155/2016/2594189
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