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- W3100114920 abstract "We investigate the possibility of constraining Chaplygin dark energy models with current Integrated Sachs Wolfe effect data. In the case of a flat universe we found that generalized Chaplygin gas models must have an energy density such that $Omega_c >0.55$ and an equation of state $w <-0.6$ at 95% c.l.. We also investigate the recently proposed Silent Chaplygin models, constraining $Omega_c >0.55$ and $w <-0.65$ at 95% c.l.. Better measurements of the CMB-LSS correlation will be possible with the next generation of deep redshift surveys. This will provide independent and complementary constraints on unified dark energy models such as the Chaplygin gas." @default.
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- W3100114920 date "2006-05-26" @default.
- W3100114920 modified "2023-10-12" @default.
- W3100114920 title "Chaplygin gas in light of recent integrated Sachs–Wolfe effect data" @default.
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- W3100114920 doi "https://doi.org/10.1088/0264-9381/23/12/009" @default.
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