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Special Beam Physics Seminar

Tuesday, June 29, 2004, 9:30 AM
ARC Bldg. Room 231/233

Lawbreakers? The Physics of Superluminal Sources

John Singleton
Los Alamos National Lab

The emission of electromagnetic radiation from a superluminal (faster-than-light in vacuo) charged particle was first studied by Sommerfeld in 1904. However, the Special Theory of Relativity was published just a few months later; prevailing scientific opinion then effectively curtailed the research field until Ginzburg and coworkers pointed out in the 1980s that no physical principle forbids emission by extended, massless superluminal sources. A polarization current density (dP/dt; see Maxwell's fourth equation) can provide such a source; the individual charged particles creating the polarization do not move faster than the speed of light, and yet it is relatively trivial to make the envelope of the polarization current density to do so.

Based on this idea (originally derived as a model for pulsars), the author and coworkers H and A Ardavan have constructed and demonstrated a machine (the Polarization Synchrotron) for animating superluminal polarization currents. The emitted electromagnetic radiation has several intriguing features; e.g. there is a component with an intensity that decays as 1/distance, rather than as the inverse square law, and the simultaneous spherically-decaying emission shows a fixed angular width out to hundreds of Fresnel distances. To reproduce the latter characteristic, a conventional antenna would have to be many, many times larger in area than the Polarization Synchrotron.

This talk will give a simplified description of the theory of superluminal sources. A particularly important point is that the radiation detected by a point-like observer over a short time period in his/her inertial frame can correspond to emission over an extended period of source time. This becomes especially marked with a rotating superluminal source (like the Polarization Synchrotron), where a volume of the source can approach the observer at the speed of light with zero acceleration; under such conditions, the emission from this volume is effectively coherent (i.e. like a laser, although the mechanism is completely different). The predictions of theory will be shown to account for the recent experimental data obtained from the Polarization Synchrotron.

The "Lawbreakers" part of the title is a quotation from an article in the "Economist" magazine about the Polarization Synchrotron. In spite of the (at first sight) surprising nature of some of the data, no physical laws are broken by the machine; it should merely be thought of as an experimental implementation of a little-considered problem in electrodynamics or as a ground-based astronomy experiment!

(Two papers on the theory of superluminal sources have been published in J. Optical Society of America A; these, and an experimental preprint may be found under the name "Singleton" at the server. This lecture will be only the third public showing of the experimental data from the Polarization Synchrotron and will present new data not previously seen.)

Talk Slides: ( slides)

For more information, please contact Dr. Alex Bogacz, Chair of CASA Seminar Committee

Updated May 11, 2016
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