Trans-Planckian origin and laboratory analogs of Hawking radiation

Black holes should glow faintly (Hawking radiation), but the calculation traces each emitted particle back to wavelengths far shorter than any known physics can describe. Flowing ultracold gases (Bose-Einstein condensates) and other fluids with sonic horizons, places where the flow outruns sound, let experiments test whether this glow survives changes at short distances.

Why it matters

Laboratory analogs are the only experimental access to Hawking's prediction, and the trans-Planckian question decides whether that prediction depends on unknown Planck-scale physics.

Review

C. Barcelo, S. Liberati, M. Visser, Analogue Gravity, Living Reviews in Relativity, 2005. https://arxiv.org/abs/gr-qc/0505065 reference checked

Timestamp record

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Entry 225, in checkpoint 2,123
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Block 969,698, 2026-10-03

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