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Nonlinear-electrodynamic effects in the electromagnetic field of a rotating pulsar

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Moscow University Physics Bulletin Aims and scope

Abstract

This paper is concerned with the calculation of nonlinear-electrodynamic effects in the field of a rapidly rotating pulsar. For an electromagnetic wave, exact and asymptotic equations of electrodynamic rays and the law thereof are proposed. The time for the nonlinear-electrodynamic delay is shown to be 3.5 times greater than that for rapidly rotating pulsars or pulsars at rest and the angle of nonlinear-electrodynamic bending of rays is shown to be higher by almost 1.7 times.

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Authors and Affiliations

  1. Department of Applied Mathematics and Information Technologies, Faculty of Applied Mathematics, Mechanics and Computer Science, Tsiolkovskii Russian State Technological University, ul. Orshanskaya 3, Moscow, 121552, Russia

    M. I. Vasil’ev

  2. Department of Quantum Theory and Physics of High Energy, Faculty of Physics, Moscow State University, Moscow, 119991, Russia

    V. A. Sokolov

Authors
  1. M. I. Vasil’ev
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  2. V. A. Sokolov
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Correspondence to M. I. Vasil’ev.

Additional information

Original Russian Text © M.I. Vasil’ev, V.A. Sokolov, 2012, published in Vestnik Moskovskogo Universiteta. Fizika, 2012, No. 5, pp. 8–12.

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Vasil’ev, M.I., Sokolov, V.A. Nonlinear-electrodynamic effects in the electromagnetic field of a rotating pulsar. Moscow Univ. Phys. 67, 418–422 (2012). https://doi.org/10.3103/S002713491205013X

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  • DOI: https://doi.org/10.3103/S002713491205013X

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