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ICS as a Limiting Factor for Electron Energies in Pulsar Magnetospheres
Published online by Cambridge University Press: 12 April 2016
Abstract
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Based on the polar cap model, we investigated in the energy loss of accelerated electrons in a neutron star magnetosphere by inverse Compton scattering of thermal photospheric radiation. An analytical treatment is presented, which turns out ranges in the magnetic field strength and thermal temperature where ultrarelativistic electrons can not survive.
- Type
- Part 6. Emission and Plasma Theory
- Information
- International Astronomical Union Colloquium , Volume 177: Pulsar Astronomy - 2000 and Beyond , 2000 , pp. 469 - 472
- Copyright
- Copyright © Astronomical Society of the Pacific 2000
References
Kardashev, N.S., Mitrofanov, I.G., & Novikov, I.D.
1984, Astronomische Zeitschrift, 61, 1113
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