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Modified Chaplygin gas as a unified dark matter and dark energy model and cosmic constraints

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Indexed by:期刊论文

Date of Publication:2012-03-01

Journal:EUROPEAN PHYSICAL JOURNAL C

Included Journals:SCIE、Scopus

Volume:72

Issue:3

Page Number:1-6

ISSN No.:1434-6044

Abstract:A modified Chaplygin gas model ( MCG), rho(MCG)/rho(MCG0) = [ B-s + ( 1 - B-s)a(-3(1+B)(1+alpha))](1/(1+alpha)), as a unified dark matter model and dark energy model, is constrained by using current available cosmic observational data points which include type Ia supernovae, baryon acoustic oscillation and the 7-year full WMAP data points. As a contrast to the consideration in the literature, we do not separate the MCG into two components, i.e. dark mater and dark energy component, but we take it as a whole energy component-a unified dark sector. By using a Markov Chain Monte Carlo method, a tight constraint is obtained: alpha = 0.000727(-0.00140-0.00234)(+0.00142+0.00391), B = 0.000777(-0.000302-0.000697)(+0.000201+0.000915) and B-s = 0.782(-0.0162-0.0329)(+0.0163+0.0307).

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