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Smith-Purcell radiation from time grating

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arxiv 2311.07381 v1 pith:KQZK7EI7 submitted 2023-11-13 physics.optics physics.app-phphysics.plasm-ph

classification physics.opticsphysics.app-phphysics.plasm-ph
keywords gratingelectronemissionmodulationradiationt-sprtemporalcompensation
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Smith-Purcell radiation (SPR) occurs when an electron skims above a spatial grating, but the fixed momentum compensation from the static grating imposes limitations on the emission wavelength. It has been discovered that a temporally periodic system can provide energy compensation to generate light emissions in free space. Here, we introduce temporal SPR (t-SPR) emerging from a time grating and propose a generalized t-SPR dispersion equation to predict the relationship between radiation frequency, direction, electron velocity, modulation period, and harmonic orders. Compared to conventional SPR, t-SPR can: 1) Provide a versatile platform for manipulating SPR emission through temporal modulation (e.g., period, amplitude, wave shape). 2) Exhibit strong robustness to the electron-grating separation, alleviating the constraints associated with extreme electron near-field excitation. 3) Introduce additional energy channels through temporal modulation, enhancing and amplifying emission.

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    A spatiotemporal wedge formed by two subluminal moving interfaces can compress and amplify pulses through cascaded Doppler reflections, with critical opening and orientation angles separating focusing from superfocusing.

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