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论文类型：期刊论文

发表时间：2016-04-01

发表刊物：GENERAL RELATIVITY AND GRAVITATION

收录刊物：SCIE

卷号：48

期号：4

ISSN号：0001-7701

关键字：Interacting dark energy model; Perturbation theory; mcmc cosmic constraint

摘要：We apply the interacting parametrized post-Friedmann (IPPF) method to coupled dark energy models where the interaction is proportional to dark matter density at background level. In the first case, the dark components are treated as fluids and the growth of dark matter perturbations only feel the interaction via the modification of background quantities provided dark matter follows geodesic. We also perform a Markov Chain Monte-Carlo analysis which combines several cosmological probes including the cosmic microwave background(WMAP9+ Planck) data, baryon acoustic oscillation (BAO) measurements, JLA sample of supernovae, Hubble constant (HST), and redshift-space distortion (RSD) measurements through the f sigma(8)(z) data points. The joint observational analysis of Planck + WP+ JLA+ BAO+ HST+ RSD data leads to a coupling parameter, xi(c) = 0.00140(-0.00080)(+0.00079) at 1 sigma level for vanishing momentum transfer potential. On the other hand, we deal with a coupled quintessence model which exhibits a violation of the equivalence principle coming form a coupling term in the modified Euler equation; as a result of that the local Hubble expansion rate and the effective gravitational coupling are both enhanced. Provided that the interaction is parallel to scalar field velocity themomentum transfer potential is switched on, leading to a lower interaction coupling xi(c) = 0.00136(-0.00073)(+0.00080) at 1 sigma level when Planck+ WP+ JLA + BAO + HST + RSD data are combined. Besides, the CMB power spectrum shows up a correlation between the coupling parameter xi(c) and the position of acoustic peaks or their amplitudes. The first peak's height increases when xi(c) takes larger values and its position is shifted. We also obtain the matter power spectrum may be affected by the strength of interaction coupling over scales bigger than 10(-2)hMpc(-1), reducing its amplitude in relation to the vanilla model.