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Breakdown of the Goldreich–Julian relation in a neutron star

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Abstract

The electromagnetic field in a magnetized neutron star and the underlying volume charges and currents are found. A general case of a rigidly rotating neutron star with infinite conductivity, arbitrary distribution of the internal magnetic field, arbitrarily changing angular velocity, and arbitrary surface velocity less than the velocity of light is considered. Quaternions are used to describe rotation and determine the magnetic field. It is shown that the charge density is not equal to and can exceed significantly the common Goldreich–Julian density. Moreover, corrections to the magnetic field due to stellar rotation are zero. For a rotating neutron star, twisting magnetic field lines causes charge accumulation and current flows. This fact shows a possible link between changing internal magnetic field topology and observed activity of neutron stars.

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Authors and Affiliations

  1. Tamm Division of Theoretical Physics, Lebedev Physical Institute, Russian Academy of Sciences, Leninskii pr. 53, Moscow, 119991, Russia

    D. N. Sob’yanin

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  1. D. N. Sob’yanin
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Correspondence to D. N. Sob’yanin.

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Published in Russian in Pis’ma v Astronomicheskii Zhurnal, 2016, Vol. 42, No. 11, pp. 818–825.

The article was translated by the author.

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Sob’yanin, D.N. Breakdown of the Goldreich–Julian relation in a neutron star. Astron. Lett. 42, 745–751 (2016). https://doi.org/10.1134/S1063773716110049

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  • DOI: https://doi.org/10.1134/S1063773716110049

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