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Acceleration of particles in pulsar magnetosphere and the X-ray radiation

Oktay H. Guseinov·Askin Ankay·Sevinc O. Tagieva
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Abstract

The available data of single X-ray pulsars, their wind nebulae, and the SNRs which are connected to some of these sources are analysed. It is shown that electric field intensity of neutron stars tears off charged particles from the surface of neutron star and triggers the acceleration of particles. The charged particles are accelerated mainly in the field of magnetodipole radiation wave. Power and energy spectra of the charged particles depend on the strength of the magnetodipole radiation. Therefore, the X-ray radiation is strongly dependent on the rate of rotational energy loss and weakly dependent on the electric field intensity. Coulomb interaction between the charged particles is the main factor for the energy loss and the X-ray spectra of the charged particles.

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Oktay H. Guseinov, Askin Ankay, Sevinc O. Tagieva. 2004-01-08. Acceleration of particles in pulsar magnetosphere and the X-ray radiation. https://arxiv.org/abs/astro-ph/0401114

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