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Conditions for the onset of the current filamentation instability in the laboratory

机译:实验室中当前丝锥不稳定性发作的条件

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The current filamentation instability (CFI) is capable of generating strong magnetic fields relevant to the explanation of radiation processes in astrophysical objects and leads to the onset of particle acceleration in collisionless shocks. Probing such extreme scenarios in the laboratory is still an open challenge. In this work, we investigate the possibility of using neutral e(-)e(+) beams to explore the CFI with realistic parameters, by performing two-dimensional particle-in-cell simulations. We show that CFI can occur unless the rate at which the beam expands due to finite beam emittance is larger than the CFI growth rate and as long as the role of the competing electrostatic two-stream instability (TSI) is negligible. We also show that the longitudinal energy spread, typical of plasma-based accelerated electron-positron fireball beams, plays a minor role in the growth of CFI in these scenarios.
机译:当前的细丝不稳定性(CFI)能够产生与天体物理物体中辐射过程的解释相关的强磁场,并导致碰撞冲击中的粒子加速度的开始。 探讨实验室的这种极端情景仍然是一个开放的挑战。 在这项工作中,我们通过执行二维粒子内模拟来研究使用中性E( - - )e(+)光束与现实参数探索CFI的可能性。 我们表明,除非梁由于有限的光束发射率而大于CFI生长速率,否则可以发生CFI并且只要竞争静电两流不稳定(TSI)的角色可以忽略不计。 我们还表明,基于等离子体的加速电子 - 正电子正电流束典型的纵向能量扩散,在这些场景中发挥了CFI的生长作用。

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