A copy of this work was available on the public web and has been preserved in the Wayback Machine. The capture dates from 2018; you can also visit the original URL.
The file type is
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 otherdoi:10.1140/epjc/s10052-012-1959-4 fatcat:pypxldlz3jfifbau4aa4m7ctju