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Phase Space Structure in Optical Emission

The emission directionality of the well-studied Robnik billiard conforms well to the classical prediction we made in Opt. Lett. 19, 1693 (1994).
Robnik billiard wavefunction Shown here is the Robnik billiard at fractional deformation 0.045 and refractive index n=2. The wavenumber on the outside is kR=43.1 (R is the undeformed radius), corresponding to kR=86.2 on the inside. The resonant state depicted here corresponds to classical rays for which the angle of incidence χ with respect to the surface normal roughly satisfies sin χ=0.7. Such rays lie in the chaotic region of phase space. One sees tangential escape from the high-curvature regions.
Robnik billiard SOS The Poincaré section of the Robnik billiard at this deformation shows the extent of chaos and island structure.

This page © Copyright Jens Uwe Nöckel, 06/2003

Last modified: Sun Jun 7 14:19:43 PDT 2009