Relativistic Correction to the Movement of Magnetic Poles

Details Relativistic Correction to the Movement of Magnetic Poles Relativistic Correction to the Movement of Magnetic Poles

May 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010apj...714..675n&link_type=abstract

The Astrophysical Journal, Volume 714, Issue 1, pp. 675-679 (2010).

Astronomy and Astrophysics

Astronomy

1

Magnetic Fields, Pulsars: General, Pulsars: Individual: Psr B1828-11, Stars: Magnetic Field, Stars: Neutron

Scientific paper

The equations of motion, modified by the relativistic correction to a rotating inclined magnetic field, are discussed. It is shown that the magnetic moment would precess under the influence of the retardation torques identifiable by several higher-order terms in the relativistic correction. The observed cyclical behaviors from the clock-like pulse-emitting pulsars reported by many researchers are likely to be the consequences of the retardation effect produced by an inclined magnetic moment of a spinning body. The results, which come from the study of two independently rotating magnetic moments, are in agreement with the observed pulsar data for the pulsar PSR B1828-11. These electromagnetic driving forces are presented for further exploration and discussion.

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