An interacting scenario for dark energy in a Bianchi type-I universe

We study the interaction between dark energy (DE) and dark matter in the scope of anisotropic Bianchi type-I space-time. First we derive the general form of the DE equation of state (EoS) parameter in both non-interacting and interacting cases and then we examine its future by applying a hyperbolic...

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Main Authors: Amirhashchi, Hassan, Qazi, Syed Nasrullah Ali, Zainuddin, Hishamuddin
Format: Article
Language:English
Published: Institute of Physics Publishing 2014
Online Access:http://psasir.upm.edu.my/id/eprint/36420/1/An%20interacting%20scenario%20for%20dark%20energy%20in%20a%20Bianchi%20type.pdf
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author Amirhashchi, Hassan
Qazi, Syed Nasrullah Ali
Zainuddin, Hishamuddin
author_facet Amirhashchi, Hassan
Qazi, Syed Nasrullah Ali
Zainuddin, Hishamuddin
author_sort Amirhashchi, Hassan
collection UPM
description We study the interaction between dark energy (DE) and dark matter in the scope of anisotropic Bianchi type-I space-time. First we derive the general form of the DE equation of state (EoS) parameter in both non-interacting and interacting cases and then we examine its future by applying a hyperbolic scale factor. It is shown that in the non-interacting case, depending on the value of the anisotropy parameter K, the DE EoS parameter varies from phantom to quintessence whereas in the interacting case the EoS parameter varies in the quintessence region. However, in both cases, the DE EoS parameter ωde ultimately (i.e. at z = −1) tends to the cosmological constant (ωde = −1). Moreover, we fix the cosmological bound on the anisotropy parameter K by using recent observational data about the Hubble parameter.
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spelling upm.eprints-364202015-09-01T03:46:35Z http://psasir.upm.edu.my/id/eprint/36420/ An interacting scenario for dark energy in a Bianchi type-I universe Amirhashchi, Hassan Qazi, Syed Nasrullah Ali Zainuddin, Hishamuddin We study the interaction between dark energy (DE) and dark matter in the scope of anisotropic Bianchi type-I space-time. First we derive the general form of the DE equation of state (EoS) parameter in both non-interacting and interacting cases and then we examine its future by applying a hyperbolic scale factor. It is shown that in the non-interacting case, depending on the value of the anisotropy parameter K, the DE EoS parameter varies from phantom to quintessence whereas in the interacting case the EoS parameter varies in the quintessence region. However, in both cases, the DE EoS parameter ωde ultimately (i.e. at z = −1) tends to the cosmological constant (ωde = −1). Moreover, we fix the cosmological bound on the anisotropy parameter K by using recent observational data about the Hubble parameter. Institute of Physics Publishing 2014 Article PeerReviewed application/pdf en http://psasir.upm.edu.my/id/eprint/36420/1/An%20interacting%20scenario%20for%20dark%20energy%20in%20a%20Bianchi%20type.pdf Amirhashchi, Hassan and Qazi, Syed Nasrullah Ali and Zainuddin, Hishamuddin (2014) An interacting scenario for dark energy in a Bianchi type-I universe. Research in Astronomy and Astrophysic, 14 (11). pp. 1383-1392. ISSN 1674-4527 10.1088/1674-4527/14/11/002
spellingShingle Amirhashchi, Hassan
Qazi, Syed Nasrullah Ali
Zainuddin, Hishamuddin
An interacting scenario for dark energy in a Bianchi type-I universe
title An interacting scenario for dark energy in a Bianchi type-I universe
title_full An interacting scenario for dark energy in a Bianchi type-I universe
title_fullStr An interacting scenario for dark energy in a Bianchi type-I universe
title_full_unstemmed An interacting scenario for dark energy in a Bianchi type-I universe
title_short An interacting scenario for dark energy in a Bianchi type-I universe
title_sort interacting scenario for dark energy in a bianchi type i universe
url http://psasir.upm.edu.my/id/eprint/36420/1/An%20interacting%20scenario%20for%20dark%20energy%20in%20a%20Bianchi%20type.pdf
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