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- W2894024806 abstract "We investigate the expected radio emission from the reverse shock of short GRBs, using the fitted afterglow parameters. In light of recent results suggesting that in some cases the radio afterglow is due to emission from the reverse shock, we examine the extent to which this component is detectable for short GRBs. In some GRBs, the standard synchrotron shock model predicts detectable radio emission from the reverse shock when none was seen. Many physical parameters play a role in these estimates, and our results highlight the need to explore the fundamental processes involved in GRB particle acceleration and emission more deeply. However, with a more rapid follow-up, we can test our standard model of GRBs, which predicts an early, radio bright reverse shock in many cases." @default.
- W2894024806 created "2018-10-05" @default.
- W2894024806 creator A5029719593 @default.
- W2894024806 date "2018-09-28" @default.
- W2894024806 modified "2023-09-26" @default.
- W2894024806 title "Reverse Shock Emission from Short GRBs" @default.
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- W2894024806 doi "https://doi.org/10.3390/galaxies6040103" @default.
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