Evolution of the polarization of the optical afterglow of the γ-ray burst GRB030329

Jochen Greiner, Sylvio Klose, Klaus Reinsch, Hans Martin Schmid, Re'Em Sari, Dieter H. Hartmann, Chryssa Kouveliotou, Arne Rau, Eliana Palazzi, Christian Straubmeier, Bringfried Stecklum, Sergej Zharikov, Gaghik Tovmassian, Otto Bärnbantner, Christoph Ries, Emmanuel Jehin, Arne Henden, Anlaug A. Kaas, Tommy Grav, Jens HjorthHolger Pedersen, Ralph A M J Wijers, Andreas Kaufer, Hye Sook Park, George G Williams, Olaf Reimer

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Abstract

The association of a supernova with GRB030329 strongly supports the 'collapsar' model of γ-ray bursts, where a relativistic jet forms after the progenitor star collapses. Such jets cannot be spatially resolved because γ-ray bursts lie at cosmological distances; their existence is instead inferred from 'breaks' in the light curves of the afterglows, and from the theoretical desire to reduce the estimated total energy of the burst by proposing that most of it comes out in narrow beams. Temporal evolution of the polarization of the afterglows may provide independent evidence for the jet structure of the relativistic outflow. Small-level polarization (∼1-3 per cent) has been reported for a few bursts, but its temporal evolution has yet to be established. Here we report polarimetric observations of the afterglow of GRB030329. We establish the polarization light curve, detect sustained polarization at the per cent level, and find significant variability. The data imply that the afterglow magnetic field has a small coherence length and is mostly random, probably generated by turbulence, in contrast with the picture arising from the high polarization detected in the prompt γ-rays from GRB021206 (ref. 18).

Original languageEnglish (US)
Pages (from-to)157-159
Number of pages3
JournalNature
Volume426
Issue number6963
DOIs
StatePublished - Nov 13 2003

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Greiner, J., Klose, S., Reinsch, K., Schmid, H. M., Sari, RE., Hartmann, D. H., ... Reimer, O. (2003). Evolution of the polarization of the optical afterglow of the γ-ray burst GRB030329. Nature, 426(6963), 157-159. https://doi.org/10.1038/nature02077

Evolution of the polarization of the optical afterglow of the γ-ray burst GRB030329. / Greiner, Jochen; Klose, Sylvio; Reinsch, Klaus; Schmid, Hans Martin; Sari, Re'Em; Hartmann, Dieter H.; Kouveliotou, Chryssa; Rau, Arne; Palazzi, Eliana; Straubmeier, Christian; Stecklum, Bringfried; Zharikov, Sergej; Tovmassian, Gaghik; Bärnbantner, Otto; Ries, Christoph; Jehin, Emmanuel; Henden, Arne; Kaas, Anlaug A.; Grav, Tommy; Hjorth, Jens; Pedersen, Holger; Wijers, Ralph A M J; Kaufer, Andreas; Park, Hye Sook; Williams, George G; Reimer, Olaf.

In: Nature, Vol. 426, No. 6963, 13.11.2003, p. 157-159.

Research output: Contribution to journalArticle

Greiner, J, Klose, S, Reinsch, K, Schmid, HM, Sari, RE, Hartmann, DH, Kouveliotou, C, Rau, A, Palazzi, E, Straubmeier, C, Stecklum, B, Zharikov, S, Tovmassian, G, Bärnbantner, O, Ries, C, Jehin, E, Henden, A, Kaas, AA, Grav, T, Hjorth, J, Pedersen, H, Wijers, RAMJ, Kaufer, A, Park, HS, Williams, GG & Reimer, O 2003, 'Evolution of the polarization of the optical afterglow of the γ-ray burst GRB030329', Nature, vol. 426, no. 6963, pp. 157-159. https://doi.org/10.1038/nature02077
Greiner J, Klose S, Reinsch K, Schmid HM, Sari RE, Hartmann DH et al. Evolution of the polarization of the optical afterglow of the γ-ray burst GRB030329. Nature. 2003 Nov 13;426(6963):157-159. https://doi.org/10.1038/nature02077
Greiner, Jochen ; Klose, Sylvio ; Reinsch, Klaus ; Schmid, Hans Martin ; Sari, Re'Em ; Hartmann, Dieter H. ; Kouveliotou, Chryssa ; Rau, Arne ; Palazzi, Eliana ; Straubmeier, Christian ; Stecklum, Bringfried ; Zharikov, Sergej ; Tovmassian, Gaghik ; Bärnbantner, Otto ; Ries, Christoph ; Jehin, Emmanuel ; Henden, Arne ; Kaas, Anlaug A. ; Grav, Tommy ; Hjorth, Jens ; Pedersen, Holger ; Wijers, Ralph A M J ; Kaufer, Andreas ; Park, Hye Sook ; Williams, George G ; Reimer, Olaf. / Evolution of the polarization of the optical afterglow of the γ-ray burst GRB030329. In: Nature. 2003 ; Vol. 426, No. 6963. pp. 157-159.
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AU - Sari, Re'Em

AU - Hartmann, Dieter H.

AU - Kouveliotou, Chryssa

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AU - Ries, Christoph

AU - Jehin, Emmanuel

AU - Henden, Arne

AU - Kaas, Anlaug A.

AU - Grav, Tommy

AU - Hjorth, Jens

AU - Pedersen, Holger

AU - Wijers, Ralph A M J

AU - Kaufer, Andreas

AU - Park, Hye Sook

AU - Williams, George G

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N2 - The association of a supernova with GRB030329 strongly supports the 'collapsar' model of γ-ray bursts, where a relativistic jet forms after the progenitor star collapses. Such jets cannot be spatially resolved because γ-ray bursts lie at cosmological distances; their existence is instead inferred from 'breaks' in the light curves of the afterglows, and from the theoretical desire to reduce the estimated total energy of the burst by proposing that most of it comes out in narrow beams. Temporal evolution of the polarization of the afterglows may provide independent evidence for the jet structure of the relativistic outflow. Small-level polarization (∼1-3 per cent) has been reported for a few bursts, but its temporal evolution has yet to be established. Here we report polarimetric observations of the afterglow of GRB030329. We establish the polarization light curve, detect sustained polarization at the per cent level, and find significant variability. The data imply that the afterglow magnetic field has a small coherence length and is mostly random, probably generated by turbulence, in contrast with the picture arising from the high polarization detected in the prompt γ-rays from GRB021206 (ref. 18).

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