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Pulsar electrodynamics revisited

Published online by Cambridge University Press:  20 March 2013

D. B. Melrose  and
R. Yuen
D. B. Melrose
Affiliation:
SIfA, School of Physics, The University of SydneyNSW 2006, Australia email: [email protected]
R. Yuen
Affiliation:
SIfA, School of Physics, The University of SydneyNSW 2006, Australia email: [email protected]
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Abstract

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The inductive electric field is unjustifiably neglected in most models for pulsar electrodynamics; it cannot be screened by the magnetospheric plasma, and it is not small in comparison with the corotation electric field. The perpendicular component of the inductive electric field implies a drift motion that is inconsistent with corotation at any angular velocity. Some implications of the inductive electric field and the associated drift motion are discussed.

Keywords

pulsars: generalplasmasmagnetic fields
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 8 , Symposium S291: Neutron Stars and Pulsars: Challenges and Opportunities after 80 years , August 2012 , pp. 283 - 286
Copyright
Copyright © International Astronomical Union 2013

References

Bai, X.-N. & Spitkovsky, A. 2010 ApJ, 715, 1270Google Scholar
Beloborodov, A. M. & Thompson, C. 2007 ApJ, 657, 967Google Scholar
Deutsch, A. J. 1955 Ann. Astrophys., 18, 1Google Scholar
Goldreich, P. & Julian, W. H. 1969 ApJ, 157, 869Google Scholar
Kramer, M.et al. 2006 Science, 312, 549CrossRefGoogle Scholar
Levinson, A., Melrose, D., Judge, A., & Luo, Q. 2005 ApJ, 631, 456Google Scholar
Luo, Q. & Melrose, D. B. 2008 MNRAS, 387, 1291Google Scholar
Lyne, A.et al. 2010 Science, 329, 408Google Scholar
Melrose, D. B. & Yuen, R. 2012 ApJ, 745, 169CrossRefGoogle Scholar
Michel, F. C. 2004 Adv. Space Res., 33, 542Google Scholar
Ruderman, M. A. & Sutherland, P. G. 1975 ApJ, 196, 51CrossRefGoogle Scholar
Song, Y. & Lysak, R. L. 2006 Phys. Rev. Lett., 96, 145002CrossRefGoogle Scholar
Sturrock, P. A. 1971 ApJ, 164, 529CrossRefGoogle Scholar
Takata, J., Wang, Y., & Cheng, C. S. 2010 ApJ, 726, 44Google Scholar
Timokhin, A. N. 2010 MNRAS, 408, 2092CrossRefGoogle Scholar