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A&A 369, 694-705 (2001)
DOI: 10.1051/0004-6361:20010131
Large scale magnetic fields and their dissipation in GRB fireballs
H. C. Spruit, F. Daigne and G. DrenkhahnMax-Planck-Institut für Astrophysik, Postfach 1317, 85741 Garching bei München, Germany
(Received 21 April 2000 / Accepted 17 January 2001 )
Abstract
We consider possible geometries of magnetic fields in GRB outflows,
and their evolution with distance from the source. For magnetically
driven outflows, with an assumed ratio of magnetic to kinetic energy
density of order unity, the field strengths are sufficient for
efficient production of
-rays by synchrotron emission in the
standard internal shock scenario, without the need for local
generation of small scale fields. In these conditions, the MHD
approximation is valid to large distances (
1019 cm). In
outflows driven by nonaxisymmetric magnetic fields, changes of
direction of the field cause dissipation of magnetic energy by
reconnection. Much of this dissipation takes place outside the
photosphere of the outflow, and can convert a significant fraction
of the magnetic energy flux into radiation.
Key words: gamma-ray bursts -- magnetic fields -- radiation mechanisms: nonthermal -- shock waves
Offprint request: H. C. Spruit, henk@mpa-garching.mpg.de
© ESO 2001
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