Curvature effect of a non-power-law spectrum and spectral evolution of GRB X-ray tails

Abstract

The apparent spectral evolution observed in the steep decay phase of many gamma-ray burst (GRB) early afterglows raises great concern about the high-latitude "curvature effect" interpretation of this phase. However, previous curvature effect models only invoked a simple power-law spectrum upon the cessation of the prompt internal emission. We investigate a model that invokes the "curvature effect" of a more general non-power-law spectrum and test this model with the Swift/XRT data of some GRB<inf>s</inf>. We show that one can reproduce both the observed lightcurve and the apparent spectral evolution of several GRB<inf>s</inf> using a model invoking a power-law spectrum with an exponential cut off. GRB 050814 is presented as an example. © 2009. The American Astronomical Society.