GeV emission from short Gamma-Ray Bursts: the case of GRB 081024B

TL;DR

This paper examines the origin of GeV emission in short GRB 081024B, analyzing synchrotron and inverse Compton processes within internal and external shock models to explain the high energy tail observed by Fermi/LAT.

Contribution

It evaluates different shock scenarios and identifies that inverse Compton from delayed internal shocks or synchrotron/IC from external shocks can explain the high energy tail.

Findings

Inverse Compton from delayed internal shocks explains the GeV tail.

External shock synchrotron emission can account for the high energy tail if cooling starts early.

Inverse Compton in the external shock model is consistent with observations.

Abstract

We investigate whether the high energy tail detected by the Fermi/LAT for the short GRB 081024B can be caused by synchrotron and self-Compton emission in the context of either the internal or external shock models. For the internal shock scenario, we explore the possibility of generating the high energy photons directly by means of the synchrotron process, or inverse Compton emission in which target photons are synchrotron photons produced in internal shocks taking place in a lately emitted shell (delayed internal shocks). In the external shock scenario, we test whether the high energy tail can be an extension of the afterglow synchrotron emission, or alternatively the inverse Compton component associated with the afterglow synchrotron photons. For the internal shock scenario, we conclude that only an inverse Compton component from delayed internal shocks can explain the high energy tail that extends to the GeV range. In the external shock scenario, we show that the high energy tail may be interpreted as synchrotron afterglow emission, if the slow cooling phase starts as early as a few seconds after the trigger. On the other hand, the observed high energy tail is consistent with an inverse Compton component of the afterglow in the fast cooling regime.