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- W2028804673 abstract "We investigate the linear growth function for the large scale structures of the universe considering modified Chaplygin gas as dark energy. Taking into account observational growth data for a given range of redshift from the Wiggle-Z measurements and rms mass fluctuations from Ly-$alpha$ measurements we numerically analyze cosmological models to constrain the parameters of the MCG. The observational data of Hubble parameter with redshift ($Z$) is also considered. The Wang-Steinhardt ansatz for growth index $gamma$ and growth function $f$ (defined as $f=Omega_{m}^{gamma} (a)$) are considered for the numerical analysis. The best-fit values of the equation of state parameters obtained here is employed to study the growth function $(f)$, growth index ($gamma$) and state parameter ($omega$) with redshift $z$. We note that MCG satisfactorily accommodates an accelerating phase followed by a matter dominated universe." @default.
- W2028804673 created "2016-06-24" @default.
- W2028804673 creator A5071585115 @default.
- W2028804673 creator A5080185380 @default.
- W2028804673 date "2013-11-22" @default.
- W2028804673 modified "2023-09-25" @default.
- W2028804673 title "Observational constraints on modified Chaplygin gas from cosmic growth" @default.
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- W2028804673 doi "https://doi.org/10.1088/1475-7516/2013/11/052" @default.
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