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Quasinormal Modes of a Noncommutative-Geometry-Inspired Schwarzschild Black Hole |
Jun Liang** |
School of Arts and Sciences, Shannxi University of Science and Technology, Xi'an 710021
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Cite this article: |
Jun Liang 2018 Chin. Phys. Lett. 35 010401 |
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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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Received: 18 August 2017
Published: 17 December 2017
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Fund: Supported by the Natural Science Foundation of Education Department of Shannxi Province under Grant No 15JK1077, and the Doctorial Scientific Research Starting Fund of Shannxi University of Science and Technology under Grant No BJ12-02. |
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