Exact quasi-bound scalar field states in dyonic Kerr-Sen black holes are expressed as confluent Heun functions with quantized frequencies showing exponential growth for positive real parts inside the horizons, supporting chronology protection.
Asymptotic iteration method for spheroidal harmonics of higher-dimensional Kerr-(A)dS black holes
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abstract
In this work we calculate the angular eigenvalues of the $(n+4)$-dimensional {\it simply} rotating Kerr-(A)dS spheroidal harmonics using the Asymptotic Iteration Method (AIM). We make some comparisons between this method and that of the Continued Fraction Method (CFM) and use the latter to check our results. We also present analytic expressions for the small rotation limit up to $O(c^3)$ with the coefficient of each power up to $O(\alpha^2)$, where $c=a\omega$ and $\alpha=a^2 \Lambda$ ($a$ is the angular velocity, $\omega$ the frequency and $\Lambda$ the cosmological constant).
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Quasi-bound States of Scalar field inside the Dyonic Kerr-Sen Black Hole
Exact quasi-bound scalar field states in dyonic Kerr-Sen black holes are expressed as confluent Heun functions with quantized frequencies showing exponential growth for positive real parts inside the horizons, supporting chronology protection.