期刊
PHYSICS LETTERS B
卷 644, 期 1, 页码 16-19出版社
ELSEVIER SCIENCE BV
DOI: 10.1016/j.physletb.2006.11.028
关键词
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We examine observational constraints on the generalized Chaplygin gas (GCG) model for dark energy from the 9 Hubble parameter data points, the 115 SNLS Sue la data and the size of baryonic acoustic oscillation peak at redshift, z = 0.35. At a 95.4% confidence level, a combination of three data sets gives 0.67 <= A(s) <= 0.83 and -0.21 <= alpha <= 0.42, which is within the allowed parameters ranges of the GCG as a candidate of the unified dark matter and dark energy. It is found that the standard Chaplygin gas model (alpha = 1) is ruled out by these data at the 99.7% confidence level. (c) 2006 Elsevier B.V. All rights reserved.
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