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The Theory of Optical Black Hole Lasers

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arxiv 1701.05655 v2 pith:QRQZM6K5 submitted 2017-01-20 gr-qc physics.opticsquant-ph

classification gr-qcphysics.opticsquant-ph
keywords blackopticalholesystemachievedamplificationanalogueholes
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The event horizon of black holes and white holes can be achieved in the context of analogue gravity. It was proven for a sonic case that if these two horizons are close to each other their dynamics resemble a laser, a black hole laser, where the analogue of Hawking radiation is trapped and amplified. Optical analogues are also very successful and a similar system can be achieved there. In this work we develop the theory of optical black hole lasers and prove that the amplification is also possible. Then, we study the optical system by determining the forward propagation of modes, obtaining an approximation for the phase difference which governs the amplification, and performing numerical simulations of the pulse propagation of our system.

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Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Smart Holes: Analogue black holes with the right temperature and entropy

    hep-th 2024-12 conditional novelty 5.0 of 10

    The entropy of a tilted Dirac cone material, integrated across a spatially varying tilt, grows linearly with temperature behind the analogue horizon and can be mapped to BTZ black hole entropy.

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