Method of the Particle-in-Cell Simulation for the Y-point in the Pulsar Magnetosphere

Details Method of the Particle-in-Cell Simulation for the Y-point in the Pulsar Magnetosphere Method of the Particle-in-Cell Simulation for the Y-point in the Pulsar Magnetosphere

2009-12-18

arxiv.org/abs/0912.3582v1

Astronomy and Astrophysics

Astrophysics

High Energy Astrophysical Phenomena

18 pages, 17 figures, accepted for publication in PASJ

Scientific paper

Recent observations in X-ray and Gamma-ray suggest that the emission region of the pulsar magnetosphere can be multifold. In particular, the open-close boundary of the magnetic field, so-called the Y-point, can be the new candidate place where magnetic field energy converts into the plasma heat and/or flow energy. Here, we present a new Particle-in-Cell code, which can be applied to the Y-point of the pulsar magnetosphere in axisymmetric geometry. The electromagnetic solver is used in the two-dimensional grid points with the cylindrical coordinate (R, z), while the particle solver operates in the three-dimensional Cartesian coordinate (x, y, z), where the Buneman-Boris method is used. The particle motion is treated in special relativity. The inner boundary conditions are set up to generate rotation of the magnetosphere by use of the force-free semi-analytic solution given by Uzdensky (2003, ApJ, 598, 446). The code has been verified by dispersion relations of all the wave modes in electron-positron plasmas. The initial test run is also presented to demonstrate the Y-shaped structure at the top of the dead zone on the light cylinder. We suggest that the structure is variable with quasi-periodicity associated with magnetic reconnection and that plasma will be accelerated and/or heated. In a time-averaged point of view, break up of the ideal-MHD condition takes place in the vicinity of the Y-point.

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