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arXiv · astro-ph/0304325

WMAP and the Generalized Chaplygin Gas

L. Amendola·F. Finelli·C. Burigana·D. Carturan
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Abstract

We compare the WMAP temperature power spectrum and SNIa data to models with a generalized Chaplygin gas as dark energy. The generalized Chaplygin gas is a component with an exotic equation of state, p_X=-A/ρ^α_X (a polytropic gas with negative constant and exponent). Our main result is that, restricting to a flat universe and to adiabatic pressure perturbations for the generalized Chaplygin gas, the constraints at 95% CL to the present equation of state w_X = p_X / ρ_X and to the parameter αare -1\leq w_X < -0.8, 0 \leq α<0.2, respectively. Moreover, we show that a Chaplygin gas (α=1) as a candidate for dark energy is ruled out by our analysis at more than the 99.99% CL. A generalized Chaplygin gas as a unified dark matter candidate (Ω_{CDM}=0) appears much less likely than as a dark energy model, although its χ^2 is only two sigma away from the expected value.

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L. Amendola, F. Finelli, C. Burigana, D. Carturan. 2003-05-06. WMAP and the Generalized Chaplygin Gas. https://doi.org/10.1088/1475-7516%2F2003%2F07%2F005

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