2012/02/29 by Mubasher Jamil, D. Momeni, Ratbay Myrzakulov · 1 citation
Physics and Astronomy · #physics.gen-ph
paper · pdf · doi:10.1140/epjc/s10052-012-1959-4
published as Eur. Phys. J. C (2012) 72:1959 · 10 pages, 23 figures, version accepted for publication in European Physical Journal C (2012)
arxiv created 2012/03/12 · arxiv updated 2012/03/27
In this paper, we explore the cosmological implications of interacting dark energy model in a torsion based gravity namely f(T). Assuming dark energy interacts with dark matter and radiation components, we examine the stability of this model by choosing different forms of interaction terms. We consider three different forms of dark energy: cosmological constant, quintessence and phantom energy. We then obtain several attractor solutions for each dark energy model interacting with other components. This model successfully explains the coincidence problem via the interacting dark energy scenario.