Slow Light as a Black Hole Analogue?

Details Slow Light as a Black Hole Analogue? Slow Light as a Black Hole Analogue?

Feb 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005tmgm.meet.1565u&link_type=abstract

The Tenth Marcel Grossmann Meeting. Proceedings of the MG10 Meeting held at Brazilian Center for Research in Physics (CBPF), Rio

Physics

Quantum Aspects Of Black Holes, Evaporation, Thermodynamics, Experimental Studies Of Gravity, Effects Of Atomic Coherence On Propagation, Absorption, And Amplification Of Light, Electromagnetically Induced Transparency And Absorption, Quantum Gravity

Scientific paper

The phenomenon of slow light (electromagnetically induced transparency), which would seem an ideal candidate for constructing a black hole analogue, cannot be used to simulate Hawking radiation. Even though an appropriately designed slow-light set-up may model classical features of black holes - such as horizon, mode mixing, "Bogoliubov" coefficients, etc. - it does not reproduce the related quantum effects.

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