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PIC simulations of magnetic reconnection

PIC simulations of magnetic reconnection. Cerutti et al. 2013. 3D PIC simulations of relativistic pair plasma reconnection ( Zeltron code) Includes Radiation reaction force ( Lorentz -Abraham- Dirac equation ) Guide field Results :

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PIC simulations of magnetic reconnection

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  1. PIC simulations of magneticreconnection

  2. Cerutti et al. 2013 • 3D PIC simulations of relativisticpair plasma reconnection (Zeltron code) • Includes • Radiationreaction force (Lorentz-Abraham-Diracequation) • Guide field Results: • Tearinginstability and fast reconnection (xy-plane): 70% of the magneticenergydissipated in particleacceleration. • Kinkinstability of the currentsheet (yz-plane): 55% of the total magnetic energy is dissipated. • Relativistickinkinstabilitydisrupt the layer (seealso, e.g., Zenitani & Hoshino 2008, Sironi & Spitkovsky 2011). • A moderate guide fieldstabilizes the layer and enableparticleacceleration

  3. Tearinginstability

  4. Tearinginstability

  5. Tearinginstability

  6. Tearinginstability

  7. Kinkinstability of the currentsheet

  8. Kinkinstability of the currentsheet

  9. Kinkinstability of the currentsheet

  10. Ratio of the inductive electric field |EY| to the magnetic field |Btotal| = (BX2+BZ2)1/2 Particle acceleration in reconnection takes place mainly around the X-type neutral region, where the amplitudes of magnetic fields are weak and charged particles become unmagnetized. They are accelerated by an inductive electric field perpendicular to the two-dimensional reconnection magnetic fields(Zenitani & Hoshino 2001).

  11. Baty, Petri, Zenitani 2013 • Resistive relativistic 2D MHD simulations • Fast reconnectionduring double tearingmodes in relativistic plasma • Time scale of instabilityweaklydepending on the Lundquistnumber

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