Relativistic Jet Simulations of the Weibel Instability in the Slab Model to Cylindrical Jets with Helical Magnetic Fields

The particle-in-cell (PIC) method was developed to investigate microscopic phenomena, and with the advances in computing power, newly developed codes have been used for several fields, such as astrophysical, magnetospheric, and solar plasmas. PIC applications have grown extensively, with large compu...

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Detalles Bibliográficos
Autores: Nishikawa, Ken-Ichi, Mizuno, Yosuke, Gómez Fernández, José L., Duţan, Ioana, Meli, Athina, Niemiec, Jacek, Kobzar, Oleh, Pohl, Martin, Sol, Helene, MacDonald, Nicholas, Hartmann, Dieter H.
Tipo de recurso: artículo
Estado:Versión publicada
Fecha de publicación:2019
País:España
Institución:Consejo Superior de Investigaciones Científicas (CSIC)
Repositorio:DIGITAL.CSIC. Repositorio Institucional del CSIC
OAI Identifier:oai:digital.csic.es:10261/178917
Acceso en línea:http://hdl.handle.net/10261/178917
Access Level:acceso abierto
Palabra clave:Particle-in-cell simulations
Relativistic jets
The Weibel instability
Kink-like instability
Mushroom instability
Global jets
Helical magnetic fields
Recollimation shocks
ddc:520
ddc:530
Descripción
Sumario:The particle-in-cell (PIC) method was developed to investigate microscopic phenomena, and with the advances in computing power, newly developed codes have been used for several fields, such as astrophysical, magnetospheric, and solar plasmas. PIC applications have grown extensively, with large computing powers available on supercomputers such as Pleiades and Blue Waters in the US. For astrophysical plasma research, PIC methods have been utilized for several topics, such as reconnection, pulsar dynamics, non-relativistic shocks, relativistic shocks, and relativistic jets. PIC simulations of relativistic jets have been reviewed with emphasis placed on the physics involved in the simulations. This review summarizes PIC simulations, starting with the Weibel instability in slab models of jets, and then focuses on global jet evolution in helical magnetic field geometry. In particular, we address kinetic Kelvin-Helmholtz instabilities and mushroom instabilities.