The dynamical behavior of $f(T)$ theory

Details The dynamical behavior of $f(T)$ theory The dynamical behavior of $f(T)$ theory

2010-07-14

arxiv.org/abs/1007.2348v2

Physics Letters B 692 (2010) 176-179

Astronomy and Astrophysics

Astrophysics

Cosmology and Extragalactic Astrophysics

10 pages, 1 figure; accepted by PLB

Scientific paper

Recently, a new model obtained from generalizing teleparallel gravity, named $f(T)$ theory, is proposed to explain the present cosmic accelerating expansion with no need of dark energy. In this paper, we analyze the dynamical property of this theory. For a concrete power law model, we obtain that the dynamical system has a stable de Sitter phase along with an unstable radiation dominated phase and an unstable matter dominated one. We show that the Universe can evolve from a radiation dominated era to a matter dominated one, and finally enter an exponential expansion phase.

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