Abstract
Reconnection of alternating magnetic fields is an important energy transformation mechanism in Poyntingdominated outflows. We show that the reconnection is facilitated by the Kruskal-Schwarzschild instability of current sheets separating the oppositely directed fields. This instability, which is a magnetic counterpart of the Rayleigh-Taylor instability, develops if the flow is accelerated. Then the plasma drips out of the current sheet, providing conditions for rapid reconnection. Since the magnetic dissipation leads to the flow acceleration, the process is self-sustaining. In pulsar winds, this process could barely compete with the earlier proposed dissipation mechanisms. However, the novel mechanism turns out to be very efficient at active galactic nucleus and gamma-ray burst conditions.
Original language | English |
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Pages (from-to) | L234-L238 |
Journal | Astrophysical Journal Letters |
Volume | 725 |
Issue number | 2 PART 2 |
DOIs | |
State | Published - 20 Dec 2010 |
Keywords
- Galaxies:jets
- Gamma-ray burst:general
- Instabilities
- Magnetic reconnection
- Magnetohydrodynamics (MHD)
- Relativity
ASJC Scopus subject areas
- Astronomy and Astrophysics
- Space and Planetary Science