Abstract
The static charged Born–Infeld black hole is stable. We compare its stability to the linear counterpart Reissner–Nordstrom black hole stability. We use the WKB method to compute how its quasi-normal modes vary with the non-linear parameter, temperature, mass of the scalar field and the spherical index.
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Fernando, S., Holbrook, C. Stability and Quasi Normal Modes of Charged Born–Infeld Black Holes. Int J Theor Phys 45, 1630–1645 (2006). https://doi.org/10.1007/s10773-005-9024-9
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DOI: https://doi.org/10.1007/s10773-005-9024-9