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 an Poisson equation and show that a
wavelike structure will inevitably arise relatively close to the pulsar.Comment: 10 pages, 0 figures, The Modern Physics of Compact Stars 2015 30
September 2015 - 3 October 2015 Yerevan, Armeni