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.
作者
Jun Liang
梁钧(School of Arts and Sciences, Shannxi University of Science and Technology)
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
