pith:QJ73CLYF
Greybody Factor, Resonant Frequencies, and Entropy Quantization of Charged Scalar Fields in the Kerr-EMDA Black Hole
Resonant frequencies of charged scalars in Kerr-EMDA black holes have imaginary parts spaced exactly by 1/(2M), yielding a horizon-dependent entropy quantum.
arxiv:2604.19848 v2 · 2026-04-21 · gr-qc · astro-ph.HE · hep-th · quant-ph
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Claims
Applying the CHF polynomial condition, we derive the resonant frequency spectrum whose imaginary parts are equispaced with |Δω_I| = 1/(2M), a universal spacing determined solely by the BH mass. Via the Maggiore prescription and the first law of BH thermodynamics, this yields a parameter-dependent entropy quantum δS_BH = 4π r_+/(r_+ - r_-), which reduces to 4π for Schwarzschild but diverges at extremality.
The assumption that the confluent Heun function parameters arising from the separated gauge-covariant Klein-Gordon equation in the Kerr-EMDA metric permit a polynomial termination condition that enforces the claimed universal imaginary frequency spacing independent of scalar charge q and dilaton parameter D.
Charged scalar fields on Kerr-EMDA black holes admit confluent Heun solutions yielding universal imaginary frequency spacing 1/(2M), entropy quanta 4π r_+/(r_+ - r_-), and the first analytical greybody factors for this geometry.
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| First computed | 2026-05-25T02:01:20.826771Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
827fb12f05bfd0bb5eeee66d32cf031276c22d1139221386d9b784947733c602
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Canonical record JSON
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