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Optical black hole : ウィキペディア英語版 | Optical black hole An optical black hole is a phenomenon in which slow light is passed through a Bose–Einstein condensate that is itself spinning faster than the local speed of light within to create a vortex capable of trapping the light behind an event horizon just as a gravitational black hole would. Unlike other black hole analogs such as a sonic black hole in a Bose–Einstein condensate, a slow light black hole analog is not expected to mimic the quantum effects of a black hole, and thus not emit Hawking radiation. It does, however, mimic the classical properties of a gravitational black hole, making it potentially useful in studying other properties of black holes.〔W.G. Unruh and R. Schützhold, "On Slow Light as a Black Hole Analogue", Phys. Rev. D 68, 024008 (arXiv:gr-qc/0303028v2 ) (2003).〕 More recently, some physicists have developed a fiber optic based system which they believe will emit Hawking radiation.〔T. G. Philbin et al., Science 319, 1367 (arXiv:0711.4796v2 [gr-qc] ) (2008)〕 == See also ==
* Sonic Black Hole * Analog models of gravity
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