Wave growth in an oscillating model of pulsar magnetospheres

Details Wave growth in an oscillating model of pulsar magnetospheres Wave growth in an oscillating model of pulsar magnetospheres

Feb 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aipc..983..133v&link_type=abstract

40 YEARS OF PULSARS: Millisecond Pulsars, Magnetars and More. AIP Conference Proceedings, Volume 983, pp. 133-135 (2008).

Physics

1

Pulsars, Neutron Stars, Magnetohydrodynamics And Plasmas, Radiation Mechanisms, Polarization

Scientific paper

The pulsar radio emission mechanism has yet to be identified unambiguously. The counter-streaming instability is a possible wave growth mechanism, but the growth rate in conventional models is too low. Here we argue that the growth rate in an oscillating model of the pulsar magnetosphere is much higher than in conventional models, and might account for the observed emission.

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