http://arxiv.org/abs/1409.7706
A suitable interaction between dark matter with an energy density $\rho_{M}$ and dark energy with an energy density $\rho_{X}$ is known to give rise to a non-canonical scaling $\rho_{M} \propto \rho_{X}a^{-\xi}$ where $\xi$ is a parameter which generally deviates from $\xi =3$. Here we present a covariant generalization of this class of models and investigate the corresponding perturbation dynamics. The resulting matter power spectrum for the special case of a decaying Lambda model is compared with data from the SDSS DR7 catalogue. We find a large degeneracy in $\xi$, equivalent to a poor restriction of the interaction but our results are compatible with the LCDM model which corresponds to the noninteracting limit with $\xi =3$ and an equation-of-state parameter $w=-1$.
A. Fu%7Bn%7Do, W. Hipolito-Ricaldi and W. Zimdahl
Tue, 30 Sep 14
45/81
Comments: 23 pages, 8 figures
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