2012

Attractor Solutions in f(T) Cosmology

Jamil, Mubasher, Momeni, D., Myrzakulov, Ratbay

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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.

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