V. M. Kontorovich, I. S. Spevak, V. K. Gavrikov
Published 2018-06-05Version 1
Additional high-frequency components of the pulsar radiation in Crab Nebula are considered as a result of the resonance with the surface electromagnetic wave at nonlinear reflection from of the neutron star surface. This stimulated scattering consists in generation of the surface periodic relief by the incident field and diffraction of the radiation of relativistic positrons on the relief which fly from magnetosphere to the star in the accelerating electric field of the polar gap.
Comments: 6 pages, 2 figures; The Report on the Conference "XIV INTERNATIONAL CONFERENCE "PLASMA ELECTRONICS AND NEW ACCELERATION METHODS" 27-31 August 2018, Kharkov, Ukraine, Kharkov National University; submit for publication in PAST, Kharkov, Ukraine, 2018
The Crab Pulsar at Centimeter Wavelengths II: Single Pulses
The Crab Pulsar and Nebula as seen in gamma-rays
The Crab pulsar and its pulsar-wind nebula in the optical and infrared
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