Jul 12 – 23, 2021
Online
Europe/Berlin timezone

Gamma-Ray Polarization Results of the POLAR Mission and Future Prospects

Jul 14, 2021, 6:00 PM
1h 30m
04

04

Talk GAD | Gamma Ray Direct Discussion

Speaker

Merlin Kole (University of Geneva)

Description

Despite over 50 years of observations of Gamma-Ray Bursts (GRBs) many open questions remain about their nature and their environments in which the emission takes place. Polarization measurements of the GRB prompt emission have long been theorized to be able to answer most of these questions. The POLAR detector was a dedicated GRB polarimeter developed by a Swiss, Chinese and Polish collaboration. The instrument was launched, together with the second Chinese Space Lab, the Tiangong-2, in September 2016 after which it took 6 months of scientific data. During this period POLAR detected 55 GRBs as well as several pulsars. From the analysis of the GRB polarization catalog we see that the prompt emission is lowly or fully unpolarized. There is, however, the caveat that within single pulses there are strong hints of an evolving polarization angle which washes out the polarization degree in the time integrated analysis. Although the POLAR results thereby exclude a large portion of the polarization parameter space, to fully probe GRB polarization a significantly more sensitive detector is required. Such a detector, called POLAR-2, was recently approved for launch in 2024 and is currently being developed by a Swiss, Chinese, Polish and German collaboration. Here we will present a full overview of the POLAR mission and all its scientific measurement results. Additionally, we will present a short overview of the follow-up mission: POLAR-2, and how it will answer some of the questions raised by the POLAR results.

Keywords

Gamma-Ray Burst, Gamma-Ray, Polarization, Analysis, POLAR, POLAR-2

other Collaboration POLAR & POLAR-2
Subcategory Experimental Results

Primary authors

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