Computational and Applied Math Proseminar

Department of Mathematics, Arizona State University

Tuesday, April 13, 1999, 12:15 p.m in GWC 604

J.V. Moloney

Department of Mathematics, University of Arizona,

An Optically Turbulent Atmospheric Light Guide

Abstract The onset and recurrence of multiple filamentary structures during the propagation of high power 200 femtosecond laser pulse in air, is reminiscent of the features observed in strong turbulence phenomena in physics. This highly explosive behavior is modeled by a higher dimensional Nonlinear Schroedinger equation which displays a blow-up singularity in finite time. Usually dissipation at short scales is invoked as a means of regularization of this collapse singularity. The NLS theory has been extremely successful in explaining Langmuir turbulence in plasmas and similar phenomena in fluids. The present situation with high power ultrashort laser pulses shows some added novel behavior. Collapse regularization through small scale dissipation is not the key player. Instead, narrow plasma filaments created in the nonlinear focal region, induce a strong defocusing lens which evaluates most of the light energy behind the light intensity hot-spot. Little energy is therefore dissipated per collapse event and this is important as the means of driving and sustaining the nucleation of such structures persists for only 100-200 femtoseconds.

For further information please contact: mittelmann@asu.edu