Analytical Afterglow Light Curves of Gamma-ray Bursts: the Case of a Flat Electron Spectrum
2012
Abstract In the standard afterglow model, the swept electrons have a single power-law energy distribution dn/dγe ∝ γ−p e (p ∼ 2.3), owing to the first order Fermi acceleration process. However, in some events people find a lot of evidence for a flat electron spectrum (i.e., p
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