Research Article

Switched Magnetospheric Regulation of Pulsar Spin-Down

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Science  24 Jun 2010:
1186683
DOI: 10.1126/science.1186683

Abstract

Pulsars are famed for their rotational clocklike stability and their highly repeatable pulse shapes. However, it has long been known that there are unexplained deviations (often termed "timing noise") from the rate at which we predict these clocks should run. We show that timing behavior often results from typically two different spin-down rates. Pulsars switch abruptly between these states, often quasiperiodically, leading to the observed spin-down patterns. We show that for six pulsars the timing noise is correlated with changes in the pulse shape. Many pulsar phenomena including mode-changing, nulling, intermittency, pulse shape variability, and timing noise are therefore linked and caused by changes in the pulsar's magnetosphere. We consider the possibility that high-precision monitoring of pulse profiles could lead to the formation of highly stable pulsar clocks.