Dipanjan Mitra, G. Melikidze, Janusz Gil
Published 2015-10-01Version 1
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.
Comments: 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
Coherent radio emission from a twisted magnetosphere after magnetar-quake
Bunch Expansion as a cause for Pulsar Radio Emissions
Spectral variation across Pulsar Profile due to Coherent Curvature Radiation
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