Abstract
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 (γ 0 ≃10) and ultrarelativistic (γ 0 ≃ 100) energies that directly correspond to the regimes of internal and external shell collisions, respectively, in GRB synchrotron emission models. Simulated systems comprise 5 × 10 8 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 ε B ∼12%, exceeding the respective internal ratios by nearly a power of 10. Enhanced ε 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.
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CITATION STYLE
Jaroschek, C. H., Lesch, H., & Treumann, R. A. (2005). Ultrarelativistic Plasma Shell Collisions in γ‐Ray Burst Sources: Dimensional Effects on the Final Steady State Magnetic Field. The Astrophysical Journal, 618(2), 822–831. https://doi.org/10.1086/426066
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