Magnetic bubbles behave differently than other magnetic defects (w/ video)

Dec 10, 2012 by Lisa Zyga feature
Magnetic bubbles behave differently than other magnetic defects
Model of a skyrmion bubble (dashed line) with propagating waves (red line) on its edges. See movie below for wave dynamics. Image credit: Oleg Tchernyshyov

(Phys.org)—Magnetism may be one of the most fundamental concepts in physics, but under the surface, magnetism holds complex secrets that scientists are still trying to unravel. One of these areas involves the dynamics of magnetic topological defects in thin films of ferromagnetic materials. In a new study, physicists have demonstrated that magnetic topological defects called skyrmions, which resemble swirling eddies or bubbles, behave differently than do other magnetic defects. The scientists show that skyrmions' unusual behavior arises from the strange occurrence of waves on the bubbles' edges that travel with different speeds in opposite directions.

The physicists, Imam Makhfudz and Oleg Tchernyshyov at the Johns Hopkins University in Baltimore, Maryland, US, and Benjamin Krüger at the University of Hamburg in Germany, have reported their discovery of some intriguing dynamics of skyrmion bubbles in a study recently published in .

Scientists have previously known that skyrmions aren't like other magnetic defects that exist in thin-film ferromagnets. The dynamics of a more typical defect, a vortex, has been described as resembling the motion of charged massless particles in a magnetic field. Scientists originally expected skyrmions to move in a similar way. However, recent simulations have shown that the behavior of skyrmion magnetic bubbles significantly deviates from this model. Whereas displaced from an equilibrium position follow a circular trajectory, the trajectory of the center of a skyrmion bubble follows roughly a more complicated curve, namely a hypocycloid.

To explain this puzzling trajectory, the physicists here have shown that skyrmion bubbles must possess . The mass is generated not at the center of a bubble but rather at its edge. According to the ' equations, waves on the boundary of a bubble travel left and right at different speeds. While the slow waves are insensitive to inertia, the fast waves involve magnetic oscillations, giving the bubbles mass.

"The greatest significance of our work, in my view, is the existence of these funny waves that travel back and forth with different speeds," Tchernyshyov told Phys.org. "This is very unusual, as normally waves travel with equal speeds in opposite directions. There are a few examples of physical systems where that happens, e.g., the edge of a Quantum Hall liquid, where electrons move in one direction only. Such systems know right from left, so they are called 'chiral.' Ours is another example of waves in chiral systems."

When skyrmion bubbles are modeled as objects with mass that contain propagating waves on their edges, the equations accurately describe the observed motion. This understanding of the dynamics of these odd magnetic entities is not only interesting from a basic physics perspective, but also for potential applications.

"Magnetic bubbles and other topological defects can be used as memory or logic elements," Tchernyshyov said. "Stuart Parkin at IBM has made some with his concept of racetrack memory, in which he uses domain walls in magnetic nanowires for computational purposes. Whether skyrmions will be eventually used in technological applications is anyone's guess. Our work is directed more at understanding the basic physics of magnets."

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Model of a skyrmion bubble with propagating waves on its edges. The dashed line is the undisturbed bubble in its lowest-energy state. The scientists then created a deformation of a specific form, in this case a wave that fits three times on the circumference, and let it go. On a skrymion bubble, the waves traveling left and right have different speeds, unlike standing waves, which are made of waves that have equal speeds even when traveling in opposite directions. If the same deformation were created on a regular taut string instead of a skyrmion bubble, it would result in two running waves traveling in opposite directions with equal speeds. Their superposition would be a standing wave that is going nowhere and merely oscillates in place, keeping its shape. The behavior of the waves on the skyrmion bubble changes in time because the faster wave decays faster. As time goes on, its amplitude diminishes and by the end of the movie you are only seeing a single running wave traveling clockwise. Credit: Oleg Tchernyshyov

This video is not supported by your browser at this time.
Model of a slow clockwise traveling wave. The superposition of this wave and a fast counterclockwise traveling wave (see other movie) results in the wave that forms on a skyrmion bubble. Movie credit: Oleg Tchernyshyov

This video is not supported by your browser at this time.
Model of a fast counterclockwise traveling wave. The superposition of this wave and a slow clockwise traveling wave (see other movie) results in the wave that forms on a skyrmion bubble. Movie credit: Oleg Tchernyshyov

Tchernyshyov added that this investigation of the dynamics of skyrmion is just one part of the researchers' broader goals of better understanding magnetic defects in general.

"This work was part of a larger scheme," he said. "The motion of topological defects in magnets is a complex phenomenon. A few years ago we came up with a new approach to its theoretical description. We proposed a simple and economical theory to describe the most important aspects of their motion [Phys. Rev. Lett. 100, 127204 (2008)]. The current paper is one of the applications of this new language. We are currently working on classifying magnetic textures by topology in three-dimensional magnets, as opposed to two-dimensional ."

Explore further: Information storage for the next generation of plastic computers

More information: Imam Makhfudz, et al. "Inertia and chiral edge modes of a skyrmion magnetic bubble." Physical Review Letters, 109, 217201 (2012). DOI: 10.1103/PhysRevLett.109.217201 . Also available at arXiv:1208.3123 [cond-mat.mes-hall] http://arxiv.org/abs/1208.3123

Journal reference: Physical Review Letters search and more info website

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jdbertron
not rated yet Dec 10, 2012
That reminds me of Saturn's hexagonal north pole.
Jeweller
1 / 5 (1) Dec 16, 2012
Could these magnetic bubbles be similar to the ones that Voyager1 is passing through right now at the outer limits of our Solar System ?
antialias_physorg
5 / 5 (1) Dec 16, 2012
Could these magnetic bubbles be similar to the ones that Voyager1 is passing through right now at the outer limits of our Solar System ?

No. This is behaviour of magnetic fields in thin film materials.
(In the future please read more than the headline before commenting. Thank you.)
Jeweller
not rated yet Dec 17, 2012
There's no need to be rude.
antialias_physorg
not rated yet Dec 17, 2012
I wasn't trying to be rude. I very deliberately put a 'please' and 'thank you' in there.

If I'd tried to be rude my choice of words would have been somewhat different.

But if you think it was rude: How would YOU have told someone that he shouldn't comment on things he doesn't bother to read (or at the very least make a minimal effort of googling stuff before typing things that don't make any sense into a comment box)?

I'd be very interested to hear your approach.

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