Scattering of Scalar Wave by Extended Black Hole in f(R) Gravity  

作　　者：廖平 张软静 陈菊华 王永久 

机构地区：[1]College of Physics and Information Science,Hunan Normal University

出　　处：《Chinese Physics Letters》2015年第5期14-18,共5页中国物理快报（英文版）

基　　金：Supported by the National Natural Science Foundation of China under Grant No 10873004;the National Basic Research Program of China under Grant No 2010CB832803;the Program for Changjiang Scholars and Innovative Research Team in University under Grant No IRT0964

摘　　要：We analyze the Sehrodinger-type scalar wave equation of an extended black hole in f（R） gravity, and numerically investigate its absorption/scattering cross sections using the partial wave method. It is found that the dimension of length a makes the peak value of the effective scattering potential fall down, and the absorption cross section oscillates around the geometric optical value in the high frequency regime. We can also see that the scattering flux becomes stronger and its angle width becomes narrower in the forward direction, the glory peak becomes lower and the glory width becomes narrower along the backward direction when the coupling parameter α increases.We analyze the Sehrodinger-type scalar wave equation of an extended black hole in f（R） gravity, and numerically investigate its absorption/scattering cross sections using the partial wave method. It is found that the dimension of length a makes the peak value of the effective scattering potential fall down, and the absorption cross section oscillates around the geometric optical value in the high frequency regime. We can also see that the scattering flux becomes stronger and its angle width becomes narrower in the forward direction, the glory peak becomes lower and the glory width becomes narrower along the backward direction when the coupling parameter α increases.

关 键 词：GRAVITY Scattering of Scalar Wave by Extended Black Hole in f 

分 类 号：O413[理学—理论物理] P145.8[理学—物理]