An External Inverse Compton Emission Model of Gamma-Ray Burst High-Energy Lags

TL;DR

This paper proposes an external inverse Compton emission model to explain the delayed high-energy gamma-ray emission observed in some GRBs, linking the delay to the physical properties of the GRB progenitor.

Contribution

It introduces a novel model combining synchrotron-self-Compton and external inverse Compton processes to explain high-energy delays in GRB emissions, specifically applied to GRB 080916C.

Findings

The model successfully explains the observed high-energy delay in GRB 080916C.

External inverse Compton scattering can account for high-energy emission delays in Fermi-LAT GRBs.

The delay timescale is connected to the physical characteristics of the GRB progenitor.

Abstract

The Fermi satellite has been reporting the detailed temporal properties of gamma-ray bursts (GRBs) in an extremely broad spectral range, 8 keV - 300 GeV, in particular, the unexpected delays of the GeV emission onsets behind the MeV emission of some GRBs. We focus on GRB 080916C, one of the Fermi-LAT GRBs for which the data of the delayed high-energy emission are quite extensive, and we show that the behavior of the high-energy emission of this burst can be explained by a model in which the prompt emission consists of two components: one is the MeV component due to the synchrotron-self-Compton radiation of electrons accelerated in the internal shock of the jet and the other is the high-energy component due to inverse Compton scattering of the photospheric X-ray emission of the expanding cocoon off the same electrons in the jet. Such an external inverse Compton effect could be important for other Fermi-LAT GRBs, including short GRBs as well. In this model, the delay timescale is directly linked to the physical properties of GRB progenitor.