Year: 2015
Type: preprint
Abstract: We review a physical model where the high brightness temperature of 10$^{25}-10^{30}$ K observed in pulsar radio emission is explained by coherent curvature radiation excited in the relativistic electron-positron plasma in the pulsar magnetosphere.
Source: arXiv (Cornell University)
Authors: Mitra, Dipanjan, Melikidze, G., Gil, Janusz
Language: English
Subfield: Astronomy and Astrophysics
Field: Physics and Astronomy
Domain: Physical Sciences
Open Access status: green
OpenAlex ID: W2239620350