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 Tools annual

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 Tools monthly

Global: Zendy Plus monthly

Presents the access of premium content as premium feature

Premium Content

Global: Zendy Plus annual

Global: Zendy Free Plan

A number of disparate observational and theoretical pieces of evidenceindicate that, contrary to the conventional wisdom, neutron stars' closed fieldlines are populated by dense, hot plasma and may be responsible for producingsome radio and high energy emission. This conclusion is based on eclipsemodeling of the binary pulsar system PSR J0737-3039A/B (Lyutikov & Thompson2005), a quantitative theory of Crab giant pulses (Lyutikov 2007) and a numberof theoretical works related to production of non-thermal spectra in magnetarsthrough resonant scattering. In magnetars, dense pair plasma is produced bytwisting magnetic field lines and associated electric fields required to liftthe particles from the surface. In long period pulsars, hot particles on closedfield lines can be efficiently trapped by magnetic mirroring, so thatrelatively low supply rate, e.g. due to a drift from open field lines, mayresult in high density. In short period pulsars, magnetic mirroring does notwork; large densities may still be expected at the magnetic equator near theY-point.

Neutron star magnetospheres: the binary pulsar, Crab and magnetars