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- W2006188110 abstract "Many gamma-ray bursts (GRBs) have been observed with the Burst Alert Telescope and X-Ray Telescope of the Swift satellite. The successive pulses of these GRBs end with a fast decline and a fast spectral softening, until they are overtaken by another pulse or the last pulse's decline is overtaken by a less rapidly varying afterglow. The fast-decline phase has been attributed, in the currently explored standard fireball model of GRBs, to synchrotron emission from a collision of two conical shells. This high-latitude emission does not explain the observed spectral softening. In contrast, the temporal behavior and the spectral evolution during the fast-decline phase agree with the predictions of the cannonball model for GRBs." @default.
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- W2006188110 date "2008-07-10" @default.
- W2006188110 modified "2023-09-24" @default.
- W2006188110 title "The Rapid Decline of the Prompt Emission in Gamma‐Ray Bursts" @default.
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