Do relativistic corrections affect microlensing amplification?
被引:14
作者:
Ebina, J
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机构:
Hirosaki Univ, Fac Sci & Technol, Hirosaki, Aomori 0368561, JapanHirosaki Univ, Fac Sci & Technol, Hirosaki, Aomori 0368561, Japan
Ebina, J
[1
]
Osuga, T
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h-index: 0
机构:Hirosaki Univ, Fac Sci & Technol, Hirosaki, Aomori 0368561, Japan
Osuga, T
Asada, H
论文数: 0引用数: 0
h-index: 0
机构:Hirosaki Univ, Fac Sci & Technol, Hirosaki, Aomori 0368561, Japan
Asada, H
Kasai, M
论文数: 0引用数: 0
h-index: 0
机构:Hirosaki Univ, Fac Sci & Technol, Hirosaki, Aomori 0368561, Japan
Kasai, M
机构:
[1] Hirosaki Univ, Fac Sci & Technol, Hirosaki, Aomori 0368561, Japan
[2] Max Planck Inst Astrophys, D-85741 Garching, Germany
来源:
PROGRESS OF THEORETICAL PHYSICS
|
2000年
/
104卷
/
06期
关键词:
D O I:
10.1143/PTP.104.1317
中图分类号:
O4 [物理学];
学科分类号:
0702 ;
摘要:
Studies of gravitational microlensing are usually based on the lens equation, which is valid only to first order in the gravitational constant G. However, the amplification factor of microlensing is a second-order quantity with respect to G. Despite this fact, conventional studies are still based on the lowest-order lens equation. Then the question naturally arises: Why are these conventional studies justified? We carefully study the relativistic correction to the amplification factor at O(G(2)). We show that the amplification factor for each image is corrected. However, the total amplification remains unchanged at this order.