Compton drag as a mechanism for very high linear polarization in gamma-ray bursts

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Abstract

The recent claim by Coburn & Boggs to have detected a very high degree of linear polarization in the prompt emission of GRB 021206 has stimulated interest in how much polarization could arise in gamma-ray bursts (GRBs) from synchrotron emission. Alternatively, as Shaviv & Dar have shown, GRB polarization could be produced by inverse Compton scattering in the point-source limit. We discuss polarization from a fireball that upscatters a soft radiation field. We show that, after the proper angular integration, the residual polarization can be large, in some cases approaching the point-source limit. We discuss the probability of realizing the geometrical conditions in which a large polarization is obtained showing that, for a particularly bright burst such as GRB 021206, the detection of polarization at the first attempt in the Compton drag scenario is not unlikely.

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Lazzati, D., Rossi, E., Ghisellini, G., & Rees, M. J. (2004). Compton drag as a mechanism for very high linear polarization in gamma-ray bursts. Monthly Notices of the Royal Astronomical Society, 347(1). https://doi.org/10.1111/j.1365-2966.2004.07387.x

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