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...
| Main Authors: | , , |
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| Format: | Article |
| Language: | English |
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Institute of Physics Publishing
2014
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| Online Access: | http://psasir.upm.edu.my/id/eprint/36420/ http://psasir.upm.edu.my/id/eprint/36420/1/An%20interacting%20scenario%20for%20dark%20energy%20in%20a%20Bianchi%20type.pdf |
| _version_ | 1848848327158792192 |
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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 |
| building | UPM Institutional Repository |
| collection | Online Access |
| 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. |
| first_indexed | 2025-11-15T09:32:44Z |
| format | Article |
| id | upm-36420 |
| institution | Universiti Putra Malaysia |
| institution_category | Local University |
| language | English |
| last_indexed | 2025-11-15T09:32:44Z |
| publishDate | 2014 |
| publisher | Institute of Physics Publishing |
| recordtype | eprints |
| repository_type | Digital Repository |
| spelling | upm-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/ http://psasir.upm.edu.my/id/eprint/36420/ http://psasir.upm.edu.my/id/eprint/36420/1/An%20interacting%20scenario%20for%20dark%20energy%20in%20a%20Bianchi%20type.pdf |