An Optical Analog of a Black Holes

dc.creatorRoyston, Andrew
dc.creatorGass, Richard
dc.date2002-12-30
dc.date.accessioned2026-07-07T03:27:28Z
dc.date.available2026-07-07T03:27:28Z
dc.descriptionUsing media with extremely low group velocities one can create an optical analog of a curved space-time. Leonhardt and Piwnicki have proposed that a vortex flow will act as an optical black hole. We show that although the Leonhardt - Piwnicki flow has an orbit of no return and an infinite red-shift surface, it is not a true black hole since it lacks a null hypersurface. However a radial flow will produce a true optical black hole that has a Hawking temperature and obeys the first law of black hole mechanics. By combining the Leonhardt - Piwnicki flow with a radial flow we obtain the analog of the Kerr black hole.
dc.descriptionfour pages, 1 figure
dc.identifierhttps://arxiv.org/abs/gr-qc/0212122
dc.identifierhttp://arxiv.org/abs/gr-qc/0212122
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/34444
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleAn Optical Analog of a Black Holes
dc.typetext

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