The interpretation of the Swift GRB X-ray afterglows

Details The interpretation of the Swift GRB X-ray afterglows The interpretation of the Swift GRB X-ray afterglows

2006-12-14

arxiv.org/abs/astro-ph/0612375v1

Nuovo Cim.B121:1247-1251,2006

Astronomy and Astrophysics

Astrophysics

5 pages including 1 figure, to appear in "Il Nuovo Cimento"

Scientific paper

10.1393/ncb/i2007-10247-4

We discuss the current interpretations of the {\it Swift} GRB X-ray afterglows, mainly focusing on the sharp decline at the prompt tail emission, and the shallow decay afterward, which is then followed by the conventional pre-\emph{Swift} decay behavior, and the possible X-ray flares during the latter two stages. We emphasize the role of the central engine in interpreting the GRB afterglows.

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