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 accessAbstract
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.
Overview
The claims and statistics of this paper haven’t been checked yet.
Run the check — free, no account needed. It reads the open-access text and checks the sources it cites.
Integrity signals
Registry
Cites
Statistics
Verification
Claims the paper makes
The claims and statistics of this paper haven’t been checked yet.
Run the check — free, no account needed. It reads the open-access text and checks the sources it cites.
Self-check
Percentages, sums and reported differences re-computed from the paper’s own numbers.
The self-check needs the paper’s full text.
Citations
Cites
Electromagnetic extraction of energy from Kerr black holes
Blandford, R. D., & Znajek, R. L. (1977) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/179.3.433 · Cited by 5,116
Radiative processes in astrophysics
(1979) · Astronomy Quarterly · doi:10.1016/0364-9229(79)90019-8 · Cited by 2,916
Particle acceleration at astrophysical shocks: A theory of cosmic ray origin
Blandford, R., & Eichler, D. (1987) · Physics Reports · doi:10.1016/0370-1573(87)90134-7 · Cited by 1,964
Unsteady outflow models for cosmological gamma-ray bursts
Rees, M. J., & Meszaros, P. (1994) · The Astrophysical Journal · doi:10.1086/187446 · Cited by 1,272
Millisecond pulsars with extremely strong magnetic fields as a cosmological source of γ-ray bursts
Usov, V. V. (1992) · Nature · doi:10.1038/357472a0 · Cited by 1,037
Mészáros, P. (2002) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev.astro.40.060401.093821 · Cited by 714
Unsteady outflow models for cosmological gamma-ray burstsPreprint
Rees, M. J., & Mészáros, P. (1994) · Cited by 680
Thompson, C. (1994) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/270.3.480 · Cited by 679
Poynting Jets from Black Holes and Cosmological Gamma-Ray Bursts
Mészáros, P., & Rees, M. J. (1997) · The Astrophysical Journal · doi:10.1086/310692 · Cited by 413
Paradijs, J. V., Kouveliotou, C., & Wijers, R. A. M. J. (2000) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev.astro.38.1.379 · Cited by 318
Cited by
Modern Tests of Lorentz Invariance
Mattingly, D. (2005) · Living Reviews in Relativity · doi:10.12942/lrr-2005-5 · Cited by 1,061
The physics of gamma-ray bursts & relativistic jets
Kumar, P., & Zhang, B. (2015) · Physics Reports · doi:10.1016/j.physrep.2014.09.008 · Cited by 952
GAMMA-RAY BURSTS: PROGRESS, PROBLEMS & PROSPECTS
ZHANG, B., & MÉSZÁROS, P. (2004) · International Journal of Modern Physics A · doi:10.1142/s0217751x0401746x · Cited by 783
McKinney, J. C. (2006) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2006.10256.x · Cited by 599
Zhang, B., Kobayashi, S., & Meszaros, P. (2003) · The Astrophysical Journal · doi:10.1086/377363 · Cited by 301
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
About these checks
Registry, retraction, Cites and statistics results are computed, not judged, with one exception: a printed reference that no index lists is read once by a model before it counts as a citation error. Claims are extracted by a model and kept only when their quote appears verbatim in the text; each cited source is then checked, with a model’s help, for whether it says what the claim relies on. Those verdicts can be wrong — read the claim’s quote and the cited source before relying on one.
Statistics and arithmetic are recomputed, not judged.
Confidence bands are shown only for fields calibrated on our annotated test set. None is calibrated yet, so no band is shown.
What counts as a claim ›How we measure confidence ›How we check this ›
Are you an author, or do you see a problem with this page? Request a review
How to cite
Cite CoChat for the checks on this page, and the paper for its own findings.
- This page
- 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
- The paper
- 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
Data sources
Bibliographic data: Semantic Scholar, OpenAlex, Crossref.
Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).
Semantic Scholar’s data is described in: Kinney, R., et al. (2023). The Semantic Scholar Open Data Platform. arXiv:2301.10140.