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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

References

Arons, J., and Barnard, J.J. 1986, ApJ, 302, 120 Google Scholar
Asseo, E., and Melikidze, G.I. 1998, MNRAS, 301, 59 CrossRefGoogle Scholar
Blaskiewicz, M., Cordes, J.M., and Wasserman, I. 1991, ApJ, 370, 643 CrossRefGoogle Scholar
Bougeret, J.-L., and Steinberg, J.-L. 1977, Solar Phys., 61, 777 Google Scholar
Daugherty, J.K., and Harding, A.K. 1983, ApJ, 273, 761 CrossRefGoogle Scholar
Duncan, R.A. 1979, Solar Phys., 63, 398 CrossRefGoogle Scholar
von Hoensbroech, A., Lesch, H., and Kunzl, T. 1998, A&A, 336, 209 Google Scholar
Kunzl, T., Lesch, H., Jessner, A., and von Hoensbroech, A. 1998, ApJ, 505, L139 CrossRefGoogle Scholar
Lominadze, D.G., Mikhailovskii, A.B., and Sagdeev, R.Z. 1979, Sov. Phys. JETP, 50, 927 Google Scholar
Lyutikov, M. 1998, MNRAS, 293, 447 CrossRefGoogle Scholar
Machabeli, G.Z., Usov, V.V. 1979, Sov. Astron. Lett., 5, 238 Google Scholar
Melrose, D.B. 1991, ARA&A, 29, 31 Google Scholar
Melrose, D.B. 1995, J.Astrophys. Astr., 16, 137 CrossRefGoogle Scholar
Melrose, D.B., and Gedalin, M. 1999, ApJ, 521, 351 CrossRefGoogle Scholar
Radhakrishnan, V., and Cooke, D.J. 1969, Astrophys. Lett., 3, 225 Google Scholar
Rankin, J.M. 1990, ApJ, 352, 247 Google Scholar
Ruderman, M.A., and Sutherland, P.G. 1975, ApJ, 196, 51 CrossRefGoogle Scholar
Stinebring, D.R., et al. 1984, ApJS, 55, 247 Google Scholar
Usov, V.V. 1987, ApJ, 320, 333 CrossRefGoogle Scholar