Quasinormal Modes of a Noncommutative-Geometry-Inspired Schwarzschild Black Hole  

作　　者：Jun Liang 梁钧(School of Arts and Sciences, Shannxi University of Science and Technology)

机构地区：[1]School of Arts and Sciences, Shannxi University of Science and Technology

出　　处：《Chinese Physics Letters》2018年第1期14-17,共4页中国物理快报（英文版）

基　　金：Supported by the Natural Science Foundation of Education Department of Shannxi Province under Grant No 15JK1077;the Doctorial Scientific Research Starting Fund of Shannxi University of Science and Technology under Grant No BJ12-02

摘　　要：The quasinormal modes（QNMs） of massless scalar field perturbation in a noncommutative-geometry-inspired Schwarzschild black hole spacetime are studied using the third-order Wentzel-Kramers-Brillouin approximative approach. The result shows that the noncommutative parameter plays an important role for the quasinormal（QNM） frequencies.The quasinormal modes（QNMs） of massless scalar field perturbation in a noncommutative-geometry-inspired Schwarzschild black hole spacetime are studied using the third-order Wentzel-Kramers-Brillouin approximative approach. The result shows that the noncommutative parameter plays an important role for the quasinormal（QNM） frequencies.

关 键 词：In WKB Quasinormal Modes of a Noncommutative-Geometry-Inspired Schwarzschild Black Hole 

分 类 号：P145.8[天文地球—天体物理] X928.706[天文地球—天文学]