Coherent Radio Emission from Pulsars
arXiv:1510.00103
Abstract
We review a physical model where the high brightness temperature of 10 K observed in pulsar radio emission is explained by coherent curvature radiation excited in the relativistic electron-positron plasma in the pulsar magnetosphere.
4 pages, To appear in Recent Trends in the Study of Compact Objects (RETCO-II): Theory and Observation ASI Conference Series, 2015, Vol. 12, pp 1-4 Edited by Indranil Chattopadhyay, Anuj Nandi, Santabrata Das and Samir Mandal