The Spacetime Metric

In one minute

Procopio, Aguero-Santacruz, Bermudez and Leonhardt address an open question: Hawking radiation draws its energy from the field around a black hole, but how field quanta create Hawking quanta was unknown. In a fibre-optical analogue of an event horizon, they present experimental and theoretical evidence for the generating process. Where a complicated cascade had been assumed, they identify a simple direct process and observe how it reacts back on the field. Such analogues rest on waves in a medium whose flow comes to exceed the wave speed. The findings point to an equally direct process in other analogues and perhaps in gravity, shedding light on how black holes might radiate.

Backreaction of stimulated Hawking radiation in an optical analogue

  1. Lorenzo M. Procopio(Author)
  2. Raul Aguero-Santacruz(Author)
  3. David Bermudez(Author)
  4. Ulf Leonhardt(Author)

Publication and identifiers

Work type
Paper
Year
2026

Rights and access

This page presents metadata and links. It does not grant permission to reproduce, download or redistribute the source.

Recorded rights status
Linking only
Rights holder
Springer Science and Business Media LLC

Citation fields

These are the recorded citation fields; no citation style or missing edition has been inferred.

Original title
Backreaction of stimulated Hawking radiation in an optical analogue
Attribution
  1. Lorenzo M. Procopio(Author)
  2. Raul Aguero-Santacruz(Author)
  3. David Bermudez(Author)
  4. Ulf Leonhardt(Author)
Year
2026