Extra twist in magnetic bubbles.

نویسنده

  • Achim Rosch
چکیده

I n the hard disk of a computer, the memory is stored in the local direction of the magnetization of a magnetic alloy. Here, just two directions of the magnetization (e.g., parallel and antiparallel to the disk) are used. Magnets can, however, form much more complex structures. Examples are bubble domains (1), where in thin magnetic layers, a regular arrangement of magnetic bubbles is induced by small magnetic fields. In PNAS, the work by Yu et al. (2) uses EM to reveal the local orientation of the magnetization in magnetic bubbles and stripes. The magnetization shows surprising twists: instead of rotating always in one direction, it twists back and forth. Such twist may be important for the manipulation of magnetism by electric currents and electric fields. Because magnetic fields bend the path of an electron, one can measure the local orientation of the magnetization of a thin magnetic layer by shooting electrons through it and carefully analyzing the images obtained by this method. This technique, Lorentz transmission EM, is used in the work by Yu et al. (2) to investigate how the magnetization twists in a layer of a certain magnetic material—a hexaferrite. It allows for taking pictures with nanometer resolution of the magnetization parallel to the layer. Because the amplitude of the magnetization is approximately constant, one can reconstruct the direction of the magnetization at each point in space. The simplest example of a magnetic structure with a rotating magnetization is a helix where the magnetization winds in one direction like the ridge of a screw. The sense of rotation, clockwise or anticlockwise when looking parallel to the helix, determines the so-called helicity. Fig. 1A shows such a helix, which first winds by 180° in one direction and then by 180° in the opposite direction. The work by Yu et al. (2) finds that such reversals of helicity occur frequently in the stripe phase of a thin magnetic layer, where dipolar forces (see below) enforce rotations of the magnetization. A small magnetic field converts the stripes into a regular array of magnetic bubbles. Fig. 1 B and C shows such bubbles where the magnetization winds smoothly from one direction in the center to the opposite direction at the edge of the figure. Models in Fig. 1 B and C differ by their helicity, and in typical bubble domains, both helicities occur with equal probability. Surprisingly, the experiments in the work by Yu et al. (2) reveal that the internal structure of small magnetic bubbles can display helicity reversals. A simplified example of such a helicity reversal is shown in Fig. 1D. In contrast to the random helicity reversals within the stripe phase or the random changes of helicity from one bubble to the next, these internal twists appear in a much more regular way. The theoretical analysis shows that such extra twists are stabilized by dipolar forces between the magnetic moments (2). Such dipolar forces are, for example, familiar from the magnetic field of the earth: when moving from the equator to the magnetic North Pole, the relative orientation of the compass needle to the magnetic dipole, which gives rise to the magnetic field of the eart, changes from parallel to antiparallel. The work by Yu et al. (2) shows how such directional dependencies favor complex magnetic structures with extra twists in the magnetization. Changes in the helicity can be fully avoided in materials where the crystal structure itself prefers one of the two helicities. Such chiral magnets [derived from the Greek χειρ (kheir) for hand] prefer either leftor right-handed helices. In a small magnetic field, they display perfectly regular arrangements of the magnetic structures shown in Fig. 1B, which are named skyrmions in this context. Furthermore, because they are not stabilized by the rather weak dipolar forces but favored more directly by the chiral atomic configuration, they can be much smaller in size (10–100 nm instead of 100– 1,000 nm). First discovered in chiral magnets by neutron scattering (3), these skyrmions and the associated winding of the magnetic structure can be imaged directly using Lorentz transmission EM (4). Such magnetic structures are also interesting, because they can be manipulated by ultrasmall electric currents (5, 6). Here, the main mechanism is that the magnetic moment (the spin) of an electron moving across the magnetic structures adjusts locally to the complex magnetization pattern. By this movement, it picks up a quantum mechanical phase. The associated forces can efficiently be described by artificial electromagnetic fields, which in turn, can be used to detect the motion of the magnetic structure (6). It is an interesting open question how the extra helicity reversals discovered in the work by Yu et al. (2) will affect the manipulation of the magnetic structure by electric fields and currents. In a recent preprint, the work by Roostaei and Nattermann (7) shows that a domain wall in a helical magnet (i.e., a plane in a 3D Fig. 1. The work by Yu et al. (2) in PNAS reveals that changes of the helicity (i.e., the direction of rotation) are common in magnetic films. The small arrows in A show a magnetic helix with reversal of its helicity (i.e., of the direction of rotation). The helix winds first by 180° in the clockwise direction and then, by 180° in the counterclockwise direction. In small magnetic fields, magnetic bubbles form with a characteristic winding of the magnetic structure. B–D show such configurations (so-called skyrmions) schematically, where the magnetization in the center is opposite to the magnetization in the edge. B and C differ only by their helicity. In B and C, there is only one sense of rotation (i.e., one fixed helicity), whereas in D, an extra twist of the magnetization gives rise to a reversal of the helicity inside the skyrmion.

برای دانلود متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

ثبت نام

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

منابع مشابه

Localization of denaturation bubbles in random DNA sequences.

We study the thermodynamic and dynamic behaviors of twist-induced denaturation bubbles in a long, stretched random sequence of DNA. The small bubbles associated with weak twist are delocalized. Above a threshold torque, the bubbles of several tens of bases or larger become preferentially localized to AT-rich segments. In the localized regime, the bubbles exhibit "aging" and move around subdiffu...

متن کامل

Formation of Semi-relativistic Jets from Magnetospheres of Accreting Neutron Stars: Injection of Hot Bubbles into a Magnetic Tower

We present the results of 2.5-dimensional resistive magnetohydrodynamic (MHD) simulations of the magnetic interaction between a weakly magnetized neutron star and its accretion disk. General relativistic effects are simulated by using the pseudo-Newtonian potential. We find that well-collimated jets traveling along the rotation axis of the disk are formed by the following mechanism: (1) The mag...

متن کامل

Magnetic Bubbles and Extramixing in Stars

The possible role of magnetic flux tubes in transporting matter from near the H shell through the radiative zone and into the convective envelope is explored. It is shown that the required rates of mass transport necessary to provide nuclear processed material to the envelope can be achieved if large magnetic fields are present just above the H shell in AGB and RGB stars. The required fields in...

متن کامل

Dynamics of magnetic bubbles in acoustic and magnetic fields.

We report on shelled bubbles that can be manipulated with magnetic fields. The magnetic shell consists of self-assembled magnetic nanoparticles. The magnetic susceptibility of the bubbles is proportional to the surface area, chi_{b}=(9+/-3x10;{-6} m)r;{2} where r is the radius. Magnetic bubbles are compressible in moderate acoustic fields. A bubble with a radius of 121 mum oscillates in resonan...

متن کامل

Magnetic field induced motion behavior of gas bubbles in liquid

The oxygen evolution reaction generally exists in electrochemical reactions. It is a ubiquitous problem about how to control the motion of oxygen bubbles released by the reaction. Here we show that oxygen bubbles during oxygen evolution reaction exhibit a variety of movement patterns in the magnetic field, including directional migration and rotational motion of oxygen bubbles when the magnet i...

متن کامل

ذخیره در منابع من


  با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید

برای دانلود متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

ثبت نام

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

عنوان ژورنال:
  • Proceedings of the National Academy of Sciences of the United States of America

دوره 109 23  شماره 

صفحات  -

تاریخ انتشار 2012