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Phys. Rev. D 62, 044044 (2000) [7 pages]

Origin of the thermal radiation in a solid-state analogue of a black hole

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B. Reznik*
School of Physics and Astronomy, Tel-Aviv University, Tel Aviv 69978, Israel

Received 31 January 2000; published 27 July 2000

An effective black-hole-like horizon occurs for electromagnetic waves in matter at a surface of singular electric and magnetic permeabilities. In a physical dispersive medium the horizon disappears for wave numbers with k>kc, and the effective geometry becomes flat. Nevertheless, it is shown that Hawking radiation is still emitted if free field modes with k>kc are in their ground state.

© 2000 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevD.62.044044
DOI:
10.1103/PhysRevD.62.044044
PACS:
04.70.Dy

*Email address: reznik@post.tau.ac.il