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arXiv · 1611.03735

Emission of extremely bright gamma-ray pulsar in the Large Magellanic Cloud

George Machabeli·Andria Rogava·Nino Chkheidze
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Abstract

In the present paper a theoretical interpretation of observational characteristics of the pulsar PSR J0540-6919 is suggested. In particular, we provide a theoretical model explaining the presence of two peaks in the radio domain and the brooding of these peaks at higher frequencies. The model also explains the pulse-phase coincidence of emission peaks at different frequencies and shows the physical, 'genetic' connection between the radio remission at frequencies of the order of GHz with gamma-ray emission up to GeV energies.

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George Machabeli, Andria Rogava, Nino Chkheidze. 2016-11-10. Emission of extremely bright gamma-ray pulsar in the Large Magellanic Cloud. https://arxiv.org/abs/1611.03735

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