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Radiative Effect on Particle Acceleration via Relativistic Electromagnetic Expansion

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arxiv astro-ph/0504561 v1 pith:7PMMBBO7 submitted 2005-04-25 astro-ph

classification astro-ph
keywords radiationdampingenergypulsecasedrpaeffectelectromagnetic
verification ladder T0 review T1 audit T2 compute T3 formal
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The radiation damping effect on the diamagnetic relativistic pulse accelerator (DRPA) is studied in two-and-half dimensional Particle-in-Cell (PIC) simulation with magnetized electron-positron plasmas. Self-consistently solved radiation damping force converts particle energy to radiation energy. The DRPA is still robust with radiation, and the Lorentz factor of the most high energy particles reach more than two thousand before they decouple from the electromagnetic pulse. Resulted emitted power from the pulse front is lower in the radiative case than the estimation from the non-radiative case due to the radiation damping. The emitted radiation is strongly linearly polarized and peaked within few degrees from the direction of Poynting flux.

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