Toroidal magnetic field in pulsars

Details Toroidal magnetic field in pulsars Toroidal magnetic field in pulsars

Oct 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006ap.....49..523s&link_type=abstract

Astrophysics, Volume 49, Issue 4, pp.523-529

Astronomy and Astrophysics

Astrophysics

Magnetic Fields, Pulsars

Scientific paper

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.

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