New constraints on the variable equation of state parameter from x-ray gas mass fractions and Sne Ia

被引:24
|
作者
Cunha, J. V. [1 ]
Marassi, L. [1 ]
Santos, R. C. [1 ]
机构
[1] Univ Fed Rio Grande do Norte, Dept Fis, BR-59072970 Natal, RN, Brazil
来源
INTERNATIONAL JOURNAL OF MODERN PHYSICS D | 2007年 / 16卷 / 2-3期
关键词
cosmology; dark energy; equation of state; X-ray; supernovae;
D O I
10.1142/S0218271807010183
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Recent measurements are suggesting that we live in a flat Universe and that its present accelerating stage is driven by a dark energy component whose equation of state may evolve in time. Assuming two different parametrizations for the function omega(z), we constrain their free parameters from a joint analysis involving measurements from X-ray luminosity of galaxy clusters and SNe type Ia data.
引用
收藏
页码:403 / 409
页数:7
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