arXiv Analytics

Sign in

arXiv:2309.04834 [astro-ph.HE]AbstractReferencesReviewsResources

Particle-in-cell simulations of pulsar magnetospheres: transition between electrosphere and force-free regimes

Fábio Cruz, Thomas Grismayer, Alexander Y. Chen, Anatoly Spitkovsky, Ricardo A. Fonseca, Luis O. Silva

Published 2023-09-09Version 1

Global particle-in-cell (PIC) simulations of pulsar magnetospheres are performed with a volume, surface and pair production-based plasma injection schemes to systematically investigate the transition between electrosphere and force-free pulsar magnetospheric regimes. A new extension of the PIC code OSIRIS to model pulsar magnetospheres using a two-dimensional axisymmetric spherical grid is presented. The sub-algorithms of the code and thorough benchmarks are presented in detail, including a new first-order current deposition scheme that conserves charge to machine precision. It is shown that all plasma injection schemes produce a range of magnetospheric regimes. Active solutions can be obtained with surface and volume injection schemes when using artificially large plasma injection rates, and with pair production-based plasma injection for sufficiently large separation between kinematic and pair production energy scales.

Related articles: Most relevant | Search more
arXiv:2105.09351 [astro-ph.HE] (Published 2021-05-19)
The novel mechanism of pair creation in pulsar magnetospheres
arXiv:1910.11387 [astro-ph.HE] (Published 2019-10-24)
Proton acceleration in pulsar magnetospheres
arXiv:1611.04331 [astro-ph.HE] (Published 2016-11-14)
Electrodynamics of pulsar magnetospheres