Breakdown of chiral symmetry during saturation of the Tayler instability
arXiv:1204.0081 · doi:10.1103/PhysRevE.86.016313
Abstract
We study spontaneous breakdown of chiral symmetry during the nonlinear evolution of the Tayler instability. We start with an initial steady state of zero helicity. Within linearized perturbation calculations, helical perturbations of this initial state have the same growth rate for either sign of helicity. Direct numerical simulations (DNS) of the fully nonlinear equations, however, show that an infinitesimal excess of one sign of helicity in the initial perturbation gives rise to a saturated helical state. We further show that this symmetry breaking can be described by weakly nonlinear finite--amplitude equations with undetermined coefficients which can be deduced solely from symmetry consideration. By fitting solutions of the amplitude equations to data from DNS we further determine the coefficients of the amplitude equations.
arXiv comment8 pages, 5 figures, Published on Phys. Rev. E
References in corpus (12)
- Stable magnetic fields in stellar interiors
- The stability of toroidal fields in stars
- Differential rotation and magnetic fields in stellar interiors
- Homochiral growth through enantiomeric cross-inhibition
- Stability of magnetic configurations containing the toroidal and axial fields
- Non-axisymmetric instability of axisymmetric magnetic fields
- Helicity and alpha-effect by current-driven instabilities of helical magnetic fields
- Alpha effect due to buoyancy instability of a magnetic layer
- Competition between Traveling Fluid Waves of Left and Right Spiral Vortices and Their Different Amplitude Combinations
- Stability of the toroidal magnetic field in stellar radiation zones
- Spontaneous chiral parity breaking by hydromagnetic buoyancy
- Resonance instability of axially-symmetric magnetostatic equilibria
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