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Magnetic X-ray Circular Dichroism


MXCD measurements are now routinely made on stations 1.1 and 3.4 of the Synchrotron Radiation Source (SRS). Studies are in progress into a variety of fundamentally important and topical areas such as magnetic multilayers and thin films, giant magneto-resistance (GMR) systems, and nanoscale (so-called "cluster") magnetic materials.

Magnetic X-ray Circular Dichroism (MXCD) arises because a magnetic material may have a different photon absorption cross-section at a particular photon energy for left- and right-circularly polarised light. Thus, an MXCD spectrum is essentially the difference between the absorption spectra measured with the two opposite signs of polarisation. Measuring MXCD in a material provides a wealth of information that cannot be obtained by any other technique. For example: measurement of the spin and orbital components of element-specific and site-specific magnetic moments, measurement of element specific hysteresis loops, determination of Lz/Sz ratios, and determination of absolute local moments. Magnetism is one of those special areas where fundamental research can lead directly to technological applications. Thus, the MXCD technique has relevance to many industries, for instance the Magneto-Optical recording industry and the Sensor industry.

Many measurements made at the SRS are performed using the Magnetic Spectroscopy Group's 5 Tesla superconducting magnet shown in figure 1.

Superconducting Magnet
Figure 1
The Magnetic Spectroscopy Group's 5 Tesla Superconducting Magnet installed on station 1.1

So, how does the MXCD effect arise? This is illustrated diagramatically in figure 2 below. For magnetic materials in the presence of an applied magnetic field, spin up and spin down bands are not equally populated. For an applied field in the up direction, there will be some empty spin up 3d states. In this case, because of conservation of spin, only the 2p electrons with up spin can be excited into the 3d states. When the orbital motion of the 2p states is in the same sense as the circular motion of the incident light the transition probability is larger; when the two motions are in opposite directions the transition probability is smaller.

Magnetic Circular Dichroism Effect
Figure 2
The Magnetic Circular Dichroism Effect

As a result, for light of a particular handedness, the L3 peak in the absorption spectrum, arising from the excitation of the 2p3/2 electrons, may be enhanced, whilst the L2 peak, arising from the excitation of the 2p1/2 electrons, may be reduced. When either the magnetisation direction or the polarisation direction are reversed the effects on the size of the L3 and L2 peaks is also reversed.

Figure 3 below shows the normalised absorption spectrum (as measured in total electron yield) from a 500 Angstrom film of cobalt deposited on a silicon wafer and capped with 21 Angstroms of gold. The degree of circular polarisation of the light incident on the sample was 75%. The sample was first magnetised with a 4 Tesla field resulting in the curve shown in red, then the field direction was reversed and the curve shown in blue was obtained.

Dichroism Seen in a Cobalt Film
Figure 3
Dichroism Seen in a Cobalt Film

Figure 4 below shows the difference between the two spectra. Evaluation of the areas under the L3 and L2 peaks in the dichroism (difference) spectrum, and under the L3+L2 peaks in the spectrum formed by summing the 2 curves together, allows the spin and orbital magnetic moments for each individual cobalt atom to be evaluated. Thus the technique is element specific, in contrast to other techniques such as those based on the Magneto-Optical Kerr Effect (MOKE) or the Faraday Effect.

The Dichroism Spectrum
Figure 4
The Dichroism Spectrum

Although as explained above a dichroism spectrum can be produced by reversing either the magnetisation of the sample or the polarisation of the light, in practice on a synchrotron bending magnet it is usually easier and more accurate to reverse the magnetisation direction. This is because the photons of opposite polarisation in the beamline follow different optical paths, possibly resulting in energy shifts and/or resolution changes. It is also difficult to guarantee that the degree of circular polarisation remains the same whilst being reversed in sign.

In addition to the standard MXCD mode of measurements described so far, two further variations have been successfully adopted:

  • Measurements of the absorption spectrum in transmission mode using multilayer samples deposited on thin mylar substrates. The benefits of this approach are twofold: it avoids excessive sensitivity to surface contaminants (e.g. oxidisation), and it avoids problems that can arise with total yield measurements in which the signal strength can be influenced by the local field strength and direction.
  • Magnetisation of the sample in "transverse" mode - with the helicity vector of the light perpendicular to the applied magnetic field. This is of particular importance in the study of perpendicular magnetic anisotropy.

Daresbury Laboratory  Synchrotron Radiation Source  SXR Facility Group  Surface Science Laboratory  Surface Science Techniques
Last updated October 26th 2001
Please send any comments or suggestions to Author Ian Kirkman or Web Editor Ian Kirkman