Science prospects for SPHiNX - a small satellite GRB polarimetry mission
arXiv:1808.05384 · doi:10.1016/j.astropartphys.2018.08.007
Abstract
Gamma-ray bursts (GRBs) are exceptionally bright electromagnetic events occurring daily on the sky. The prompt emission is dominated by X-/-rays. Since their discovery over 50 years ago, GRBs are primarily studied through spectral and temporal measurements. The properties of the emission jets and underlying processes are not well understood. A promising way forward is the development of missions capable of characterising the linear polarisation of the high-energy emission. For this reason, the SPHiNX mission has been developed for a small-satellite platform. The polarisation properties of incident high-energy radiation (50-600 keV) are determined by reconstructing Compton scattering interactions in a segmented array of plastic and GdAlGaO(Ce) (GAGG(Ce)) scintillators. During a two-year mission, 200 GRBs will be observed, with 50 yielding measurements where the polarisation fraction is determined with a relative error 10%. This is a significant improvement compared to contemporary missions. This performance, combined with the ability to reconstruct GRB localisation and spectral properties, will allow discrimination between leading classes of emission models.
arXiv commentAccepted for publication in Astroparticle Physics
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