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dc.contributor.authorLiang, Edison
dc.contributor.authorFu, Wen
dc.contributor.authorBoettcher, Markus
dc.contributor.authorSmith, Ian
dc.contributor.authorRoustazadeh, Parisa
dc.date.accessioned2015-04-02T07:37:29Z
dc.date.available2015-04-02T07:37:29Z
dc.date.issued2013
dc.identifier.citationLiang, E. et al. 2013. Relativistic positron-electron-ion shear flows and application to gamma-ray bursts. Astrophysical journal letters. 779(L27):1-8. [http://iopscience.iop.org/2041-8205]en_US
dc.identifier.issn2041-8205
dc.identifier.issn2041-8213 (Online)
dc.identifier.urihttp://hdl.handle.net/10394/13650
dc.description.abstractWe present particle-in-cell simulation results of relativistic shear flows for hybrid positron–electron–ion plasmas and compare to those for pure e+e− and pure e− ion plasmas. Among the three types of relativistic shear flows, we find that only hybrid shear flow is able to energize the electrons to form a high-energy spectral peak plus a hard power law tail. Such electron spectra are needed to model the observational properties of gamma-ray bursts.en_US
dc.description.urihttp://iopscience.iop.org/2041-8205/779/2/L27/article
dc.description.urihttp://iopscience.iop.org/2041-8205
dc.description.urihttp://dx.doi.org/10.1088/2041-8205/779/2/L27
dc.language.isoenen_US
dc.publisherIOP Scienceen_US
dc.subjectGamma-ray burst: generalen_US
dc.subjectmagnetic fieldsen_US
dc.subjectplasmasen_US
dc.subjectrelativistic processesen_US
dc.titleRelativistic positron-electron-ion shear flows and application to gamma-ray burstsen_US
dc.typeArticleen_US
dc.contributor.researchID24420530 - Böttcher, Markus


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