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Hawking radiation in an electro-magnetic wave-guide?

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arxiv quant-ph/0408145 v2 pith:H6SUUH6I submitted 2004-08-23 quant-ph gr-qc

classification quant-phgr-qc
keywords electro-magnetichawkingradiationwave-guideamplifiedanalogousapartappropriately
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It is demonstrated that the propagation of electro-magnetic waves in an appropriately designed wave-guide is (for large wave-lengths) analogous to that within a curved space-time -- such as around a black hole. As electro-magnetic radiation (e.g., micro-weaves) can be controlled, amplified, and detected (with present-day technology) much easier than sound, for example, we propose a set-up for the experimental verification of the Hawking effect. Apart from experimentally testing this striking prediction, this would facilitate the investigation of the trans-Planckian problem. PACS: 04.70.Dy, 04.80.-y, 42.50.-p, 84.40.Az.

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Cited by 3 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. OpenAlex reports about 177 citations worldwide. Full citation record

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    Thermal Hawking-like radiation in moving-mirror cavities is robust only for selected expanding configurations and low frequencies; all other configurations tested show non-thermal spectra.

  3. Non-local correlations of a test quantum field in gravitational collapse

    gr-qc 2025-05 conditional novelty 6.0 of 10

    Equal-time vacuum correlations of a test quantum field on a dynamically collapsing, horizon-forming spacetime develop non-local peaks across the apparent horizon, and the outside peak moves away from the horizon over time.

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