Possibility of Radio-wave Radiation Production Inside a Pulsar

The influence of general-relativistic effects on charge distribution inside a neutron star is investigated. The qualitative distinction of space charge distribution inside the conducting crust from that inside the superconducting core allows us to propose a possible mechanism of radio-wave radiation produced in the intermediate medium inside a pulsar. The possibility of modeling this radiation in laboratory experiments in a rotating frame of reference is analysed.

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