English (United Kingdom)

https://curated-unify.zendy.io/wp-json/zendy-region/v1/featured_content/oa?rat=en

https://curated-unify.zendy.io/wp-json/zendy-region/v1/highlighted_journal/

Global: Zendy Plus annual

Presents the access of premium content as premium feature

Premium Content

Presents the keyphrase highlighting as premium feature

Keyphrase Highlighting

Presents the summarisation as premium feature

Summarisation

Insights

Presents the pdf analysis as premium feature

PDF Analysis

Presents the zaia usage as premium feature

ZAIA

Global: Zendy Plus monthly

Global: Zendy Tools annual

Global: Zendy Tools monthly

Global: Zendy Free Plan

We examine timing noise in both magnetars and regular pulsars, and find thatthere exists a component of the timing noise with strong magnetic fielddependence above B ~ 10^{12.5} G. The dependence of the timing noise floor onthe magnetic field is also reflected in the smallest observable glitch size. Wefind that magnetospheric torque variation cannot explain this component oftiming noise. We calculate the moment of inertia of the magnetic field outsideof a neutron star and show that this timing noise component may be due tovariation of this moment of inertia, and could be evidence of rapid globalmagnetospheric variability.

Timing Noise in Pulsars and Magnetars and the Magnetospheric Moment of Inertia