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The Status of Pulsar Emission Theory

Published online by Cambridge University Press:  12 April 2016

D.B. Melrose
D.B. Melrose*
Affiliation:
School of Physics, University of Sydney, NSW 2006, AUSTRALIA

Abstract

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It is argued that there is now a preferred pulsar radio emission mechanism, involving beam-driven Langmuir turbulence. A testable prediction is that, at least in a statistical sense, features in the spectra of pulsars should scale with the plasma frequency, υGJ, implied by the Goldreich-Julian number density.

Type
Part 11. The Future – Where to go?
Information
International Astronomical Union Colloquium , Volume 177: Pulsar Astronomy - 2000 and Beyond , 2000 , pp. 721 - 726
Copyright
Copyright © Astronomical Society of the Pacific 2000

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