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      Rapidly rotating pulsar radiation in vacuum nonlinear electrodynamics

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          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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          The Extreme Light Infrastructure: Optics’ Next Horizon

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            Author and article information

            Journal
            2016-10-19
            Article
            1610.06017
            a96f56cd-a1e0-4332-a013-036787628249

            http://creativecommons.org/licenses/by/4.0/

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            astro-ph.HE

            High energy astrophysical phenomena
            High energy astrophysical phenomena

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