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摘要:
In this work we introduced a new proposal to study the gravitational lensing theory by spherical lenses, starting from its surface mass density ∑(x) written in terms of a decreasing function f of a dimensionless coordinate x on the lens plane. The main result is the use of the function f(x) to find directly the lens properties, at the same time that the lens problem is described by a first order differential equation which encodes all information about the lens. SIS and NIS profiles are used as examples to find their functions f(x). Using the Poisson equation we find that the deflection angle is directly proportional to f(x), and therefore the lens equation can be written in terms of the function and the parameters of the lens. The critical and caustic curves, as well as image formation and magnification generated by the lens are analyzed. As an example of this method, the properties of a lens modeled by a NFW profile are determined. Although the puntual mass is spherically symmetric, its mass density is not continuous so that its f(x) function is discussed in Appendix 1.
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篇名 Gravitational Lensing by Spherical Lenses
来源期刊 天文学与天体物理学国际期刊(英文) 学科 数学
关键词 GRAVITATIONAL LENSING STRONG DARK MATTER
年,卷(期) 2014,(2) 所属期刊栏目
研究方向 页码范围 340-352
页数 13页 分类号 O1
字数 语种
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DARK
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天文学与天体物理学国际期刊(英文)
季刊
2161-4717
武汉市江夏区汤逊湖北路38号光谷总部空间
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333
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