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首页> 外文期刊>The Astrophysical journal >Ultrarelativistic Plasma Shell Collisions in γ-Ray Burst Sources: Dimensional Effects on the Final Steady State Magnetic Field
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Ultrarelativistic Plasma Shell Collisions in γ-Ray Burst Sources: Dimensional Effects on the Final Steady State Magnetic Field

机译:γ射线爆裂源中的超相对论性等离子体壳碰撞:对最终稳态磁场的尺寸影响

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摘要

Ultrarelativistic electron-positron plasma shell collisions as an integral part of generic γ-ray burst (GRB) fireball models are studied in the framework of self-consistent three-dimensional particle-in-cell simulations. We compare scenarios at moderately relativistic (γ0 10) and ultrarelativistic (γ0 100) energies that directly correspond to the regimes of internal and external shell collisions, respectively, in GRB synchrotron emission models. Simulated systems comprise 5 × 108 particles, applying a relativistic, fully electromagnetic, massively parallelized code. It is found that Weibel-generated, steady state magnetic equipartition ratios in external collisions reach up to B ~ 12%, exceeding the respective internal ratios by nearly a power of 10. Enhanced B yields can be explained theoretically by the effective reduction of dimensionality in the ultrarelativistic limit, i.e., the energy-dependent confinement of the three-dimensional Weibel instability within quasi-two-dimensional plasma shell slices.
机译:在自洽的三维单元格粒子模拟框架内研究了超相对论性电子-正电子等离子体壳碰撞作为通用γ射线爆裂(GRB)火球模型的组成部分。我们比较了在GRB同步加速器发射模型中分别相对于内壳碰撞和外壳碰撞状态的中等相对论(γ010)和超相对论(γ0100)能量下的情景。模拟系统包含5×108个粒子,应用相对论,完全电磁的大规模并行化代码。发现在外部碰撞中,由Weibel生成的稳态磁均分比达到B〜12%,比各自的内部比高出将近10的幂。在理论上,有效降低B的尺寸可以解释B产量的提高。超相对论极限,即准二维等离子体壳层中三维维贝尔不稳定性的能量依赖范围。

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