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Revisiting the time-integrated polarizations of gamma-ray burst prompt phase.

Authors :
Sui, Li-Qiang
Lan, Mi-Xiang
Source :
Monthly Notices of the Royal Astronomical Society. Apr2024, Vol. 529 Issue 4, p4287-4294. 8p.
Publication Year :
2024

Abstract

In previous studies, the time evolution information is missed in deducing the time-integrated polarizations of gamma-ray burst prompt emission. Here, it is considered and the time-integrated polarizations is investigated through the summation of the time-resolved ones. The statistical properties of the distribution of the time-integrated polarization degree (Π) can be read from the q– Π curve, where q ≡ θ V /θ j . θ V and θ j are the observational and jet half-opening angles, respectively. Hence, only the q– Π curves are studied. In addition to a toroidal magnetic field in the radiation region, an aligned field is also discussed. We found the predicted time-integrated polarization degree is around |$(40\!-\!50)\,\, \mathrm{ per\,cent}$| for High-energy Polarimetry Detector (HPD) onboard POLAR-2 and is roughly |$(30\!-\!40)\,\, \mathrm{ per\,cent}$| for its Low-energy Polarimetry Detector (LPD). Therefore, Π value detected by the HPD will be larger than that of the LPD in statistics and the result of the former estimations will underestimate the value of Π in an ordered field. There are mainly two types of the q –Π curve profiles, corresponding to two ordered magnetic field configurations. [ABSTRACT FROM AUTHOR]

Details

Language :
English
ISSN :
00358711
Volume :
529
Issue :
4
Database :
Academic Search Index
Journal :
Monthly Notices of the Royal Astronomical Society
Publication Type :
Academic Journal
Accession number :
176725680
Full Text :
https://doi.org/10.1093/mnras/stae808