High Energy Polarimetry of Prompt GRB Emission
arXiv:1611.06579 · doi:10.1016/j.newar.2016.11.001
Abstract
Evidence of polarized -ray emission ( 50 keV) from Gamma-Ray Bursts (GRBs) has been accumulated in recent years. Measurements have been reported with levels in the range of 30-80\%, typically with limited statistical significance. No clear picture has yet emerged with regards to the polarization properties of GRBs. Taken at face value, the data suggest that most GRBs have a relatively large level of polarization (typically, ), which may suggest synchrotron emission associated with an ordered magnetic field structure within the GRB jet. But these results are far from conclusive. Here, we review the observations that have been made, concentrating especially on the instrumental issues and the lessons that might be learned from these data.
Accepted for publication in New Astronomy Reviews
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Cited by in corpus (26)
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- The POLAR Gamma-Ray Burst Polarization Catalog
- Hard X-ray polarization catalog for a 5-year sample of Gamma-Ray Bursts using AstroSat CZT-Imager
- The IXPE view of GRB 221009A
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- New constraints on Lorentz invariance violation with polarized gamma-ray bursts
- Benchmarking simulations of the Compton Spectrometer and Imager with calibrations
- Spectro-polarimetric analysis of prompt emission of GRB 160325A: jet with evolving environment of internal shocks
- Testing the Einstein's equivalence principle with polarized gamma-ray bursts
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- Astrophysical and Cosmological Searches for Lorentz Invariance Violation
- Tests of Lorentz Invariance
- Precision Test of the Weak Equivalence Principle from Gamma-Ray Burst Polarization
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