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Spontaneous decay of periodic magnetostatic equilibria

Journal Article · · Physical Review Letters
In order to understand the conditions which lead a highly magnetized, relativistic plasma to become unstable, and in such cases how the plasma evolves, we study a prototypical class of magnetostatic equilibria where the magnetic field satisfies ∇ x B = αB , where \alpha is spatially uniform, on a periodic domain. Using numerical solutions we show that generic examples of such equilibria are unstable to ideal modes (including incompressible ones) which are marked by exponential growth in the linear phase. We characterize the unstable mode, showing how it can be understood in terms of merging magnetic and current structures, and explicitly demonstrate its instability using the energy principle. Following the nonlinear evolution of these solutions, we find that they rapidly develop regions with relativistic velocities and electric fields of comparable magnitude to the magnetic field, liberating magnetic energy on dynamical timescales and eventually settling into a configuration with the largest allowable wavelength. Furthermore, these properties make such solutions a promising setting for exploring the mechanisms behind extreme cosmic sources of gamma rays.
Research Organization:
SLAC National Accelerator Laboratory (SLAC), Menlo Park, CA (United States)
Sponsoring Organization:
USDOE
Grant/Contract Number:
AC02-76SF00515
OSTI ID:
1326977
Alternate ID(s):
OSTI ID: 1213281
Report Number(s):
SLAC-PUB--16715
Journal Information:
Physical Review Letters, Journal Name: Physical Review Letters Journal Issue: 9 Vol. 115; ISSN 0031-9007; ISSN PRLTAO
Publisher:
American Physical Society (APS)Copyright Statement
Country of Publication:
United States
Language:
English

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Cited By (10)

Magnetoluminescence book January 2017
Magnetoluminescence journal June 2017
The evolution of primordial magnetic fields since their generation journal September 2016
The imprint of pulsar parameters on the morphology of Pulsar Wind Nebulae journal July 2016
Black hole magnetosphere with small-scale flux tubes – II. Stability and dynamics journal June 2019
The imprint of pulsar parameters on the morphology of Pulsar Wind Nebulae text January 2016
On the Broadband Synchrotron Spectra of Pulsar Wind Nebulae journal February 2019
The evolution of primordial magnetic field since its generation text January 2015
On the broad-band synchrotron spectra of pulsar wind nebulae text January 2018
Black hole magnetosphere with small scale flux tubes--II. Stability and dynamics text January 2019

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