Quasinormal Modes of a Noncommutative-Geometry-Inspired Schwarzschild Black Hole
Jun LiangSchool of Arts and Sciences, Shannxi University of Science and Technology, Xi’an 710021
2018en
ABI
Abstract
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.
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