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• W1997480483 abstract "In this paper, a unified dark fluid with constant adiabatic sound speed is decomposed into cold dark matter interacting with vacuum energy. Based on a Markov-chain Monte Carlo method, we constrain this model by jointing the geometry and dynamical measurement. The geometry test includes cosmic microwave background radiation from Planck, baryon acoustic oscillation, and type-Ia supernovae; the dynamic measurement is $f{ensuremath{sigma}}_{8}(z)$ data points, which is obtained from the growth rate via redshift space distortion, and ${ensuremath{sigma}}_{8}(z)$ is the root-mean-square amplitude of the density contrast $ensuremath{delta}$ at the comoving $8{h}^{ensuremath{-}1}text{ }text{ }mathrm{Mpc}$ scale. The jointed constraint shows that $ensuremath{alpha}=0.00066{2}_{ensuremath{-}0.000662}^{+0.000173}$ and ${ensuremath{alpha}}_{8}=0.82{4}_{ensuremath{-}0.0166}^{+0.0128}$. The CMB and matter power spectra are both similar for the case of $ensuremath{alpha}=text{mean}$ value and that of $ensuremath{alpha}=0$. However, the evolutionary curves of $f{ensuremath{sigma}}_{8}(z)$ are different. This means that, to some extent, the data points of the growth rate could break the degeneracy of the dark energy models." @default.
• W1997480483 created "2016-06-24" @default.
• W1997480483 creator A5018656868 @default.
• W1997480483 creator A5026828765 @default.
• W1997480483 creator A5032140571 @default.
• W1997480483 creator A5041966023 @default.
• W1997480483 date "2014-02-20" @default.
• W1997480483 modified "2023-10-01" @default.
• W1997480483 title "Constraints on a decomposed dark fluid with constant adiabatic sound speed by jointing the geometry test and growth rate after Planck data" @default.
• W1997480483 cites W1555237261 @default.
• W1997480483 cites W1586190921 @default.
• W1997480483 cites W1596384349 @default.
• W1997480483 cites W1597749799 @default.
• W1997480483 cites W1701014456 @default.
• W1997480483 cites W1792393415 @default.
• W1997480483 cites W1853767801 @default.
• W1997480483 cites W1938366638 @default.
• W1997480483 cites W1946863394 @default.
• W1997480483 cites W1977473468 @default.
• W1997480483 cites W1978012230 @default.
• W1997480483 cites W1983965028 @default.
• W1997480483 cites W1986352386 @default.
• W1997480483 cites W1988475329 @default.
• W1997480483 cites W1988819556 @default.
• W1997480483 cites W1989563518 @default.
• W1997480483 cites W1989713766 @default.
• W1997480483 cites W1992788985 @default.
• W1997480483 cites W1993290196 @default.
• W1997480483 cites W1994429583 @default.
• W1997480483 cites W1999192875 @default.
• W1997480483 cites W2000273225 @default.
• W1997480483 cites W2001900257 @default.
• W1997480483 cites W2002999176 @default.
• W1997480483 cites W2004996876 @default.
• W1997480483 cites W2005274494 @default.
• W1997480483 cites W2011316491 @default.
• W1997480483 cites W2017158856 @default.
• W1997480483 cites W2018064521 @default.
• W1997480483 cites W2021033533 @default.
• W1997480483 cites W2021155634 @default.
• W1997480483 cites W2021820901 @default.
• W1997480483 cites W2022291108 @default.
• W1997480483 cites W2023724948 @default.
• W1997480483 cites W2027268976 @default.
• W1997480483 cites W2027588865 @default.
• W1997480483 cites W2028804673 @default.
• W1997480483 cites W2033849390 @default.
• W1997480483 cites W2047053204 @default.
• W1997480483 cites W2048446165 @default.
• W1997480483 cites W2051737331 @default.
• W1997480483 cites W2066715867 @default.
• W1997480483 cites W2070913392 @default.
• W1997480483 cites W2073832139 @default.
• W1997480483 cites W2074252869 @default.
• W1997480483 cites W2074586383 @default.
• W1997480483 cites W2081467532 @default.
• W1997480483 cites W2082050761 @default.
• W1997480483 cites W2087400522 @default.
• W1997480483 cites W2087661199 @default.
• W1997480483 cites W2100711791 @default.
• W1997480483 cites W2108313227 @default.
• W1997480483 cites W2113869105 @default.
• W1997480483 cites W2118265220 @default.
• W1997480483 cites W2124601931 @default.
• W1997480483 cites W2124639732 @default.
• W1997480483 cites W2124947510 @default.
• W1997480483 cites W2129729174 @default.
• W1997480483 cites W2139900404 @default.
• W1997480483 cites W2147875900 @default.
• W1997480483 cites W2150124329 @default.
• W1997480483 cites W2152820281 @default.
• W1997480483 cites W2153208487 @default.
• W1997480483 cites W2157138706 @default.
• W1997480483 cites W2160253850 @default.
• W1997480483 cites W2162757877 @default.
• W1997480483 cites W2165172508 @default.
• W1997480483 cites W2241524116 @default.
• W1997480483 cites W2596716325 @default.
• W1997480483 cites W2952589162 @default.
• W1997480483 cites W3038049795 @default.
• W1997480483 cites W3099007593 @default.
• W1997480483 cites W3100185151 @default.
• W1997480483 cites W3100453045 @default.
• W1997480483 cites W3100514957 @default.
• W1997480483 cites W3101164871 @default.
• W1997480483 cites W3101198552 @default.
• W1997480483 cites W3102156100 @default.
• W1997480483 cites W3102474852 @default.
• W1997480483 cites W3102728719 @default.
• W1997480483 cites W3102871705 @default.
• W1997480483 cites W3103392358 @default.
• W1997480483 cites W3104062933 @default.
• W1997480483 cites W3104337690 @default.
• W1997480483 cites W3105162136 @default.
• W1997480483 cites W3122149089 @default.
• W1997480483 cites W3122309993 @default.
• W1997480483 cites W3122618695 @default.
• W1997480483 cites W3125508083 @default.
• W1997480483 cites W767497580 @default.
• W1997480483 doi "https://doi.org/10.1103/physrevd.89.043511" @default.

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