Abstract
Two-dimensional particle simulations of a relativistic Harris current sheet of pair (e±) plasmas have demonstrated that the system is unstable to the relativistic drift kink instability and that a new kind of acceleration process takes place in the deformed current sheet. This process contributes to the generation of nonthermal particles and contributes to the fast magnetic dissipation in the current sheet structure. The acceleration mechanism and a brief comparison with relativistic magnetic reconnection are presented.
Sign-in/Register to access full text options 
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a callDisclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.
