analogue gravity · july 2026
Dumb Holes
When a fluid flows faster than sound, phonons cannot swim upstream. That sonic surface is an acoustic event horizon — a laboratory window onto Hawking radiation.
Dumb holes (acoustic black holes) are laboratory systems in which sound waves play the role that light plays near a gravitational event horizon. When a fluid flows faster than the local speed of sound, phonons cannot propagate upstream past the sonic surface — an acoustic horizon. The same kinematic arguments that yield Hawking radiation for black holes then predict thermal phononic emission from that surface.
This site packages a source-grounded literature synthesis:
- Paper — full manuscript with verified DOIs
- Findings — figures and comparative timeline
- Methods — how sources were selected and claims classified
- Data — downloads (manuscript, citation ledger, figures)
Thesis in one sentence
Analogue gravity experiments have established that the kinematic core of the Hawking effect is robust and laboratory-accessible; they have not (and cannot by themselves) prove gravitational black-hole evaporation, but they make the underlying quantum-field-on-curved-background machinery far less speculative.
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| Route | What you get |
|---|---|
| /paper/ | Full academic manuscript |
| /findings/ | Horizon geometry + timeline figures |
| /methods/ | Literature protocol + unit contract |
| /data/ | Machine-readable sources + downloads |