http://arxiv.org/abs/1610.06017
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.
V. Denisov, I. Denisova, A. Pimenov, et. al.
Thu, 20 Oct 16
11/44
Comments: N/A