Technical Physics Letters
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The use of advanced Bragg reflectors for frequency stabilization and tuning in planar surface-wave oscillators
Peskov N. Yu.
1,2,3, Zaslavsky V. Yu.
1,2,3, Leshcheva K.A.
1,2,3
1Federal Research Center A.V. Gaponov-Grekhov Institute of Applied Physics of the Russian Academy of Sciences, Nizhny Novgorod, Russia
2Budker Institute of Nuclear Physics, Siberian Branch, Russian Academy of Sciences, Novosibirsk, Russia
3Lobachevsky State University, Nizhny Novgorod, Russia
2Budker Institute of Nuclear Physics, Siberian Branch, Russian Academy of Sciences, Novosibirsk, Russia
3Lobachevsky State University, Nizhny Novgorod, Russia
Email: peskov@ipfran.ru, zas-vladislav@ipfran.ru, leshcheva@ipfran.ru
To achieve high coherence of radiation in oversized Cherenkov surface-wave oscillators (SWO), the use of an additional resonant Bragg reflector of an advanced type based on the coupling of paraxial and quasi-cutoff waves is proposed. Within the framework of the conducted 3D PIC - simulations, it is shown that the reflectors of this type make it possible to provide a stable narrow-band generation regime in SWO of a planar geometry with excitation of the fundamental mode of the slow-wave structure at an oversize parameter (width) of about 7-10 radiation wavelengths. An additional advantage of the proposed planar generator is the possibility of mechanical frequency tuning when changing the gap size of the resonant reflector. The parameters for the implementation of powerful W-band SWO based on the high-current accelerator complex "ELMI" (BINP RAS) have been evaluated. Keywords: relativistic Cherenkov generators, high-power microwave radiation, Bragg resonators, mode selection.
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