Rapidly rotating pulsar radiation in vacuum nonlinear electrodynamics
arXiv:1610.06017 · doi:10.1140/epjc/s10052-016-4464-3
Abstract
In this paper we investigate vacuum nonlinear electrodynamics corrections on rapidly rotating pulsar radiation and spin-down in the perturbative QED approach (post-Maxwellian approximation). An analytical expression for the pulsar's radiation intensity has been obtained and analyzed.
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