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Main Authors: Cruz, Fábio, Grismayer, Thomas, Chen, Alexander Y., Spitkovsky, Anatoly, Fonseca, Ricardo A., Silva, Luis O.
Format: Preprint
Published: 2023
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Online Access:https://arxiv.org/abs/2309.04834
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author Cruz, Fábio
Grismayer, Thomas
Chen, Alexander Y.
Spitkovsky, Anatoly
Fonseca, Ricardo A.
Silva, Luis O.
author_facet Cruz, Fábio
Grismayer, Thomas
Chen, Alexander Y.
Spitkovsky, Anatoly
Fonseca, Ricardo A.
Silva, Luis O.
contents 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.
format Preprint
id arxiv_https___arxiv_org_abs_2309_04834
institution arXiv
publishDate 2023
record_format arxiv
spellingShingle Particle-in-cell simulations of pulsar magnetospheres: transition between electrosphere and force-free regimes
Cruz, Fábio
Grismayer, Thomas
Chen, Alexander Y.
Spitkovsky, Anatoly
Fonseca, Ricardo A.
Silva, Luis O.
High Energy Astrophysical Phenomena
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.
title Particle-in-cell simulations of pulsar magnetospheres: transition between electrosphere and force-free regimes
topic High Energy Astrophysical Phenomena
url https://arxiv.org/abs/2309.04834