Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3502
Title: Radio emission by particles due to pulsar spin
Authors: Thomas, R. M. C
Gangadhara, R. T
Keywords: Pulsars General;Radiation Mechanisms: Non-Thermal;Stars: Rotation;Magnetic Fields;Radio Continuum: General
Issue Date: Jul-2005
Publisher: EDP Sciences
Citation: Astronomy and Astrophysics, Vol. 437, No. 2, pp. 537 - 543
Abstract: We present a relativistic model for the motion of charged particles in rotating magnetic field lines projected onto a plane perpendicular to the rotation axis. By making an approximation that the projected field lines are straight, an analytical expression is obtained for the particle trajectory. The motive behind developing this model is to elucidate some of the effects of rotation in pulsar profiles. There is significant contribution to the curvature of a particle trajectory due to the rotation of the pulsar, which is in addition to the inherent curvature of the field lines. The asymmetry in the observed pulse shapes can be explained by considering the aberration-retardation effects. The single sign circular polarization observed in many pulsars might be due to the relative orientation of sight line with respect to the particle trajectory plane.
URI: http://hdl.handle.net/2248/3502
ISSN: 0004-6361
???metadata.dc.relation.uri???: http://arxiv.org/abs/astro-ph/0501315
http://dx.doi.org/10.1051/0004-6361:20041319
Appears in Collections:IIAP Publications

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