Gravitational lensing by black holes

被引:255
|
作者
Bozza, Valerio [1 ,2 ,3 ]
机构
[1] Univ Salerno, Dipartimento Fis ER Caianiello, I-84084 Fisciano, Italy
[2] Ist Nazl Fis Nucl, Sez Napoli, I-80125 Naples, Italy
[3] Ist Int Alti Studi Sci, I-84019 Vietri Sul Mare, Italy
关键词
Gravitational lensing; Black holes; Galactic center; STRONG-FIELD LIMIT; RELATIVISTIC ACCRETION DISK; SAGITTARIUS-A-ASTERISK; LINE-PROFILES; GALACTIC-CENTER; TESTING THEORIES; COMPACT OBJECTS; PHOTON ORBITS; LIGHT-CURVE; IRON LINE;
D O I
10.1007/s10714-010-0988-2
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We review the theoretical aspects of gravitational lensing by black holes, and discuss the perspectives for realistic observations. We will first treat lensing by spherically symmetric black holes, in which the formation of infinite sequences of higher order images emerges in the clearest way. We will then consider the effects of the spin of the black hole, with the formation of giant higher order caustics and multiple images. Finally, we will consider the perspectives for observations of black hole lensing, from the detection of secondary images of stellar sources and spots on the accretion disk to the interpretation of iron K-lines and direct imaging of the shadow of the black hole.
引用
收藏
页码:2269 / 2300
页数:32
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