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Efficient acceleration and radiation in Poynting flux powered GRB outflows

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Drenkhahn, G., Spruit, H. C.·2002·Astronomy & Astrophysics

Abstract

We investigate the effects of magnetic energy release by local magnetic dissipation processes in Poynting flux-powered GRBs. For typical GRB parameters (energy and baryon loading) the dissipation takes place mainly outside the photosphere, producing non-thermal radiation. This process converts the total burst energy into prompt radiation at an efficiency of 10–50%. At the same time the dissipation has the effect of accelerating the flow to a large Lorentz factor. For higher baryon loading, the dissipation takes place mostly inside the photosphere, the efficiency of conversion of magnetic energy into radiation is lower, and an X-ray flash results instead of a GRB. We demonstrate these effects with numerical one-dimensional steady relativistic MHD calculations.

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Metadata

Authors
Drenkhahn, G., & Spruit, H. C.
Venue
Astronomy & Astrophysics
Publisher
EDP Sciences
Published
2002-08-09
Volume
391
Issue
3
Pages
1141-1153
ISSN
  • 0004-6361 (ISSN-L)
  • 1432-0746
OpenAlex
W2110178167
Cited by
433
References
0
FWCI
7.19
Type
journal article
Language
en
Open access
bronze

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CoChat. (2026). Citation check: Efficient acceleration and radiation in Poynting flux powered GRB outflows. https://app.cochat.ai/papers/10.1051/0004-6361:20020839
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Drenkhahn, G., & Spruit, H. C. (2002). Efficient acceleration and radiation in Poynting flux powered GRB outflows. Astronomy & Astrophysics. https://doi.org/10.1051/0004-6361%3A20020839

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Semantic Scholar’s data is described in: Kinney, R., et al. (2023). The Semantic Scholar Open Data Platform. arXiv:2301.10140.