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Proceedings of The Modern Physics of Compact Stars 2015 — PoS(MPCS2015)
We study the generation of the wakefields by means of the high energy radiation of pulsars. The problem is considered in the framework of a one dimensional approach. We linearize the set of governing equations consisting of the momentum equation, continuity equation and Poisson equation and show that a wavelike structure will inevitably arise relatively close to the pulsar.doi:10.22323/1.262.0015 fatcat:247obo75afcojcal3bjww2ng7i