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红外背景的畸变
引用本文:吴建新,王建诚.红外背景的畸变[J].中国天文和天体物理学报,1988(2).
作者姓名:吴建新  王建诚
作者单位:湘潭大学物理系 (吴建新),中国科学院云南天文台(王建诚)
摘    要:本文研究了引力透镜和富星系团在宇宙中作为一种分布,对红外背景畸变的统计效应。其中包括富系团的热电子对红外背景畸变的Sunyaev-Zel’dovich效应,以及引力透镜对红外背景畸变的引力效应。本文给出了z=4范围内的红外背景的总畸变,其结果是:Sunyaev-Zel’-dovich效应为:(△T_r)/T_r~10~(-2)—10~(-3),纯引力效应为(△T_r)/T_r~10~(-3)—10~(-4)。

关 键 词:观测宇宙学  背景辐射  引力透镜效应

Distortion of Infrared Background Radiation
Wu Jiangxin Wang Jiangcheng.Distortion of Infrared Background Radiation[J].Chinese Journal of Astronomy and Astrophysics,1988(2).
Authors:Wu Jiangxin Wang Jiangcheng
Abstract:In this paper, we discuss the statistical effect of the IR background distortion due to gravitational lens and rich galactic clusters, both of which have a definite distribution within the universe. The effect includes the distortion on IR background due to the Sunyeav-ZePdovich effect of the hot electrons in rich galactic clusters and that due to gravitational effect of gravitational lens. The total distorition within Z-4 is presented. The conclusions are (1) thedistortion due to the Sunyaev-Zel'dovich effect is ; (2) the distortion due tothe gravitational effect of gravitational lens is .
Keywords:Observational cosmology-background radiation-gravitational lensing effect  
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