Spin-down of pulsars by the current: Comparison of theory with observations

Basis (linear algebra)
DOI: 10.1007/bf00650179 Publication Date: 2004-11-27T10:51:49Z
ABSTRACT
Observational data are analysed on the basis of pulsar magnetosphere theory and the Ruderman-Sutherland plasma generation mechanism. The results of theory and experiment are shown to be in good agreement. The existence of a special group of long-lived, weakly-radiating fast (the periodP≃0.1–0.4 s) and superfast (P≲0.01) pulsars is predicted.
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