Resonant Stimulated Emission from Black Hole Horizons

May 10, 2026Open Access

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Key Points

The aim is to modify Hawking emission into stimulated radiation using resonance perturbations on photon geodesics.
Applied periodic resonance perturbation to photon geodesic equations in Schwarzschild/Kerr spacetime.
Derived corrections to the Bogoliubov coefficient in the near-horizon limit.
Computed second-order coherence for specific drive amplitude and frequency.
Identified 3:2 sub-harmonic resonance condition as optimal for maximizing stimulated emission.
Predicted second-order coherence g(2)(0) = 0.556 for drive amplitude A = 0.28 and frequency 1.35.
Proposed laboratory tests using analogue gravity systems.

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Examines stimulated radiation from black holes, suggesting new insights into Hawking emission.

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Harley Sandow (2026) studied this question.

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