In this paper, we compute quasi-normal modes of ABG black holes (which has a nonlinear electrodynamical source) using the WKB methods and AIM. A comparison between the spectrum of QNMs calculated by both methods is made. We analyse how the spectrum of QNMs depends on the black hole parameters, multipole number and overtone number and establish that the ABG black hole is stable against the scalar field.
机构:
Department of Physics, Aristotle University of Thessaloniki, ThessalonikiDepartment of Physics, Aristotle University of Thessaloniki, Thessaloniki
Kokkotas K.D.
Schmidt B.G.
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机构:
Max Planck Institute for Gravitational Physics, Albert Einstein Institute, GolmDepartment of Physics, Aristotle University of Thessaloniki, Thessaloniki