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dc.contributor.authorLiang, Edison
dc.contributor.authorBöttcher, Markus
dc.contributor.authorSmith, Ian
dc.date.accessioned2015-04-02T07:17:20Z
dc.date.available2015-04-02T07:17:20Z
dc.date.issued2013
dc.identifier.citationLiang, E. et al. 2013. Magnetic field generation and particle energization at relativistic shear boundaries in collisionless electron-positron plasmas. Astrophysical journal letters. 766(2): Article no L19. [https://doi.org/10.1088/2041-8205/766/2/L19]en_US
dc.identifier.issn2041-8205
dc.identifier.issn2041-8213 (Online)
dc.identifier.urihttp://hdl.handle.net/10394/13648
dc.identifier.urihttps://doi.org/10.1088/2041-8205/766/2/L19
dc.description.abstractUsing particle-in-cell simulations, we study the kinetic physics of relativistic shear flow in collisionless electron–positron (e+e−) plasmas. We find efficient magnetic field generation and particle energization at the shear boundary, driven by streaming instabilities across the shear interface and sustained by the shear flow. Nonthermal, anisotropic high-energy particles are accelerated across field lines to produce a power-law tail turning over just below the shear Lorentz factor. These results have important implications for the dissipation and radiation of jets in blazars and gamma-ray bursts.en_US
dc.language.isoenen_US
dc.publisherIOP Scienceen_US
dc.subjectGalaxies: jetsen_US
dc.subjectmagnetic fielden_US
dc.subjectplasmaen_US
dc.titleMagnetic field generation and particle energization at relativistic shear boundaries in collisionless electron-positron plasmasen_US
dc.typeArticleen_US
dc.contributor.researchID24420530 - Böttcher, Markus


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