Toroidal magnetic field in pulsars |
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Authors: | D M Sedrakian R Krikorian |
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Institution: | (1) Department of Physics, Yerevan State University, Armenia;(2) College de France and Institute d’Astrophysyque, Paris, France |
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Abstract: | The differential rotation of plasma in the core of pulsars (Ωs ≠ Ωe) generates convective currents increasing with time which in turn generates the toroidal magnetic field. To avoid difficulties
of physical interpretation inherent to the theory of general relativity we have adopted the tetrad approach to discuss the
generation of the magnetic field in the core of the neutron stars. The results which we have obtained are in agreement with
those obtained earlier.
Published in Astrofizika, Vol. 49, No. 4, pp. 613–620 (August 2006). |
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Keywords: | magnetic fields pulsars |
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