1109.1308 (Kazuharu Bamba et al.)

Cosmological perturbations in $k$-essence model    [PDF]

Kazuharu Bamba, Jiro Matsumoto, Shin'ichi Nojiri

Subhorizon approximation is often used in cosmological perturbation theory. In this paper, however, it is shown that the subhorizon approximation is not always a good approximation at least in case of $k$-essence model. We also show that the sound speed given by $k$-essence model exerts a huge influence on the time evolution of the matter density perturbation, and the future observations could clarify the differences between the $\Lambda$CDM model and $k$-essence model.

View original: http://arxiv.org/abs/1109.1308