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2012 | 10 | 5 | 1065-1071
Article title

Phase space analysis of interacting dark energy in f(T) cosmology

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Abstracts
EN
In this paper, we examine the interacting dark energy model in f(T) cosmology. We assume dark energy as a perfect fluid and choose a specific cosmologically viable form f(T) = β√T. We show that there is one attractor solution to the dynamical equation of f(T) Friedmann equations. Further we investigate the stability in phase space for a general f(T) model with two interacting fluids. By studying the local stability near the critical points, we show that the critical points lie on the sheet u* = (c − 1)v* in the phase space, spanned by coordinates (u, v, Ω, T). From this critical sheet, we conclude that the coupling between the dark energy and matter c ∈ (−2, 0).
Keywords
Publisher
Journal
Year
Volume
10
Issue
5
Pages
1065-1071
Physical description
Dates
published
1 - 10 - 2012
online
21 - 11 - 2012
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bwmeta1.element.-psjd-doi-10_2478_s11534-012-0103-2
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