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Cited by 356

The DOI matches its Crossref record; 14 of the 14 references it cites were found in a registry or an index.

Polarization of the prompt γ-ray emission from the γ-ray burst of 6 December 2002

Open access
Coburn, Wayne, Boggs, Steven E.·2003·Nature

Abstract

Observations of the afterglows of γ-ray bursts (GRBs) have revealed that they lie at cosmological distances, and so correspond to the release of an enormous amount of energy. The nature of the central engine that powers these events and the prompt γ-ray emission mechanism itself remain enigmatic because, once a relativistic fireball is created, the physics of the afterglow is insensitive to the nature of the progenitor. Here we report the discovery of linear polarization in the prompt γ-ray emission from GRB021206, which indicates that it is synchrotron emission from relativistic electrons in a strong magnetic field. The polarization is at the theoretical maximum, which requires a uniform, large-scale magnetic field over the γ-ray emission region. A large-scale magnetic field constrains possible progenitors to those either having or producing organized fields. We suggest that the large magnetic energy densities in the progenitor environment (comparable to the kinetic energy densities of the fireball), combined with the large-scale structure of the field, indicate that magnetic fields drive the GRB explosion.

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Metadata

Authors
Coburn, W., & Boggs, S. E.
Venue
Nature
Published
2003-05
Volume
423
Issue
6938
Pages
415-417
ISSN
  • 0028-0836 (ISSN-L)
  • 1476-4687
OpenAlex
W1544875189
Cited by
356
References
14
FWCI
29.96
Type
journal article
Language
en
Open access
green

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CoChat. (2026). Citation check: Polarization of the prompt γ-ray emission from the γ-ray burst of 6 December 2002. https://app.cochat.ai/papers/10.1038/nature01612
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Coburn, W., & Boggs, S. E. (2003). Polarization of the prompt γ-ray emission from the γ-ray burst of 6 December 2002. Nature. https://doi.org/10.1038/nature01612

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