Quasinormal Modes of a Noncommutative-Geometry-Inspired Schwarzschild Black Hole: Gravitational, Electromagnetic and Massless Dirac Perturbations

doi:10.1088/0256-307X/35/5/050401

Chin. Phys. Lett.

2018, Vol. 35

Issue (5): 050401 DOI: 10.1088/0256-307X/35/5/050401

GENERAL

Quasinormal Modes of a Noncommutative-Geometry-Inspired Schwarzschild Black Hole: Gravitational, Electromagnetic and Massless Dirac Perturbations

Jun Liang^**

School of Arts and Sciences, Shannxi University of Science and Technology, Xi'an 710021

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Jun Liang 2018 Chin. Phys. Lett. 35 050401

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Abstract In our previous work [Chin. Phys. Lett. 35 (2018) 010410], the quasinormal modes 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. In this study, we extend the work to the cases of gravitational, electromagnetic and massless Dirac perturbations. The result further confirms that the noncommutative parameter plays an important role for the quasinormal frequencies.

Received: 28 December 2017 Published: 30 April 2018

PACS:	04.70.-s	(Physics of black holes)
	04.30.-w	(Gravitational waves)

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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https://cpl.iphy.ac.cn/10.1088/0256-307X/35/5/050401 OR https://cpl.iphy.ac.cn/Y2018/V35/I5/050401

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