Da Costa, A.A. and Diver, D.A. (2001) Pulsar geometrodynamics: limitations for the gamma-ray radiation. In: High Energy Gamma-Ray Astronomy: International Symposium, Heidelberg, Germany, 26-30 June 2000, 823 -826. ISBN 1563969904 (doi: 10.1063/1.1370885)
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Publisher's URL: http://dx.doi.org/10.1063/1.1370885
Abstract
Following the strict single particle approach, when collective effects are not considered, electron-positron plasma flow in pulsar magnetospheres may reach very high energies, and therefore become quasi-classical as charged particles have stochastic trajectories due to the radiation of very high energy photons, in the hard gamma-ray domain. The associated energy balance imposes an upper limit on the energy of the radiated photons, well below the TeV range. However such an upper limit might be enhanced provided the quasi-classical single particle approach incorporates collective effects, namely the ones produced in the plasma rest frame.
Item Type: | Conference Proceedings |
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Status: | Published |
Refereed: | Yes |
Glasgow Author(s) Enlighten ID: | Diver, Professor Declan |
Authors: | Da Costa, A.A., and Diver, D.A. |
Subjects: | Q Science > QB Astronomy Q Science > QC Physics |
College/School: | College of Science and Engineering > School of Physics and Astronomy |
Journal Name: | AIP Conference Proceedings |
ISSN: | 0094-243X |
ISBN: | 1563969904 |
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