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.
Volume 262 -
The Modern Physics of Compact Stars 2015 (MPCS2015) -
Session iii neutron star dynamics
Excitation of wakefield around pulsars
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Published on:
December 30, 2016
Abstract
DOI: https://doi.org/10.22323/1.262.0015
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Copyright owned by the author(s) under the term of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License.