Theory of GRB Afterglow

Astronomy and Astrophysics – Astrophysics

Scientific paper

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A short review, invited talk in the second Rome GRb meeting. To appear in the procceedings

Scientific paper

10.1007/10853853_80

The most interesting current open question in the theory of GRB afterglow is the propagation of jetted afterglows during the sideway expansion phase. Recent numerical simulations show hydrodynamic behavior that differs from the one suggested by simple analytic models. Still, somewhat surprisingly, the calculated light curves show a `jet break' at about the expected time. These results suggest that the expected rate of orphan optical afterglows should be smaller than previously estimated.

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