Pith. sign in

Asymptotic iteration method for spheroidal harmonics of higher-dimensional Kerr-(A)dS black holes

1 Pith paper cite this work. Polarity classification is still indexing.

1 Pith paper citing it
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).

fields

hep-th 1

years

2026 1

verdicts

UNVERDICTED 1

representative citing papers

Quasi-bound States of Scalar field inside the Dyonic Kerr-Sen Black Hole

hep-th · 2026-06-01 · unverdicted · novelty 7.0

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.

citing papers explorer

Showing 1 of 1 citing paper.

  • Quasi-bound States of Scalar field inside the Dyonic Kerr-Sen Black Hole hep-th · 2026-06-01 · unverdicted · none · ref 28 · internal anchor

    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.