Cosmological Parameters from Observations of Galaxy Clusters

被引：910

作者：

Allen, Steven W. ^{[1
]}

Evrard, August E. ^{[2
,3
,4
,5
]}

Mantz, Adam B. ^{[6
]}

机构：

[1] Stanford Univ, Dept Phys, Kavli Inst Particle Astrophys & Cosmol, Stanford, CA 94305 USA

[2] SLAC Natl Accelerator Lab, Menlo Pk, CA 94025 USA

[3] Univ Michigan, Dept Phys, Ann Arbor, MI 48109 USA

[4] Univ Michigan, Dept Astron, Ann Arbor, MI 48109 USA

[5] Univ Michigan, Michigan Ctr Theoret Phys, Ann Arbor, MI 48109 USA

[6] NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA

来源：

ANNUAL REVIEW OF ASTRONOMY AND ASTROPHYSICS, VOL 49 | 2011年 / 49卷

关键词：

cosmology; dark energy; dark matter; galaxy clusters; intracluster medium; large-scale structure; X-RAY LUMINOSITY; HALO MASS FUNCTION; COLD DARK-MATTER; DIGITAL SKY SURVEY; INTERACTION CROSS-SECTION; PROBE WMAP OBSERVATIONS; LARGE-SCALE STRUCTURE; FLUX-LIMITED SAMPLE; OBSERVED GROWTH; POWER SPECTRUM;

D O I：

10.1146/annurev-astro-081710-102514

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Studies of galaxy clusters have proved crucial in helping to establish the standard model of cosmology, with a Universe dominated by dark matter and dark energy. A theoretical basis that describes clusters as massive, multicomponent, quasi-equilibrium systems is growing in its capability to interpret multiwavelength observations of expanding scope and sensitivity. We review current cosmological results, including contributions to fundamental physics, obtained from observations of galaxy clusters. These results are consistent with and complementary to those from other methods. We highlight several areas of opportunity for the next few years, and emphasize the need for accurate modeling of survey selection and sources of systematic error. Capitalizing on these opportunities will require a multiwavelength approach and the application of rigorous statistical frameworks, utilizing the combined strengths of observers, simulators, and theorists.

引用

页码：409 / 470

页数：62

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