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We consider the propagation of X-ray and gamma ray emissions in strongmagnetic and gravitational fields of the pulsar in nonlinear vacuumelectrodynamics. We show that the radiation will spread from the pulsar to thedetecting device in the form of two normal modes polarized in mutuallyorthogonal planes, and having different velocities. We have calculated thedelay between the two modes, as they propagate from the pulsar to the detectingdevice.

Some effects of nonlinear vacuum electrodynamics in strong magnetic and gravitational fields of the pulsar