Gravitational lensing

被引：305
|
作者：
Bartelmann, Matthias [1 ]
机构：
[1] Heidelberg Univ, Zentrum Astron, Inst Theoret Astrophys, D-69120 Heidelberg, Germany
来源：
CLASSICAL AND QUANTUM GRAVITY | 2010年 / 27卷 / 23期
关键词：
LARGE-SCALE STRUCTURE; COLD DARK-MATTER; DIGITAL SKY SURVEY; LARGE-MAGELLANIC-CLOUD; HUBBLE-SPACE-TELESCOPE; REALISTIC CLUSTER POTENTIALS; RAY-LUMINOUS CLUSTERS; COSMIC SHEAR ANALYSIS; MICROWAVE BACKGROUND ANISOTROPIES; QUASAR-GALAXY CORRELATIONS;
D O I：
10.1088/0264-9381/27/23/233001
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
Gravitational lensing has developed into one of the most powerful tools for the analysis of the dark universe. This review summarizes the theory of gravitational lensing, its main current applications and representative results achieved so far. It has two parts. In the first, starting from the equation of geodesic deviation, the equations of thin and extended gravitational lensing are derived. In the second, gravitational lensing by stars and planets, galaxies, galaxy clusters and large-scale structures is discussed and summarized.
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页数：72
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