Photonic band structure enables understanding how confined electromagnetic modes propagate within a photonic crystal. In photonic crystals that incorporate magnetic elements, such confined and resonant optical modes are accompanied by enhanced and modified magneto-optical activity. We describe a measurement procedure to extract the magneto-optical band structure by Fourier space microscopy.
Photonic crystals are periodic nanostructures that can support a variety of confined electromagnetic modes. Such confined modes are usually accompanied by local enhancement of electric field intensity that strengthens light-matter interactions, enabling applications such as surface-enhanced Raman scattering (SERS) and surface plasmon enhanced sensing. In the presence of magneto-optically active materials, the local field enhancement gives rise to anomalous magneto-optical activity. Typically, the confined modes of a given photonic crystal depend strongly on the wavelength and incidence angle of the incident electromagnetic radiation. Thus, spectral and angular-resolved measurements are needed to fully identify them as well as to establish their relationship with the magneto-optical activity of the crystal. In this article, we describe how to use a Fourier-plane (back focal plane) microscope to characterize magneto-optically active samples. As a model system, here we use a plasmonic grating built out of magneto-optically active Au/Co/Au multilayer. In the experiments, we apply a magnetic field on the grating in situ and measure its reciprocal space response, obtaining the magneto-optical response of the grating over a range of wavelengths and incident angles. This information enables us to build a complete map of the plasmonic band structure of the grating and the angle and wavelength dependent magneto-optical activity. These two images allow us to pinpoint the effect that the plasmon resonances have on the magneto-optical response of the grating. The relatively small magnitude of magneto-optical effects requires a careful treatment of the acquired optical signals. To this end, an image processing protocol for obtaining magneto-optical response from the acquired raw data is laid out.
Confined electromagnetic modes in photonic crystals can arise from a variety of different origins, such as plasmon resonances around metal/dielectric interfaces or Mie resonances in high refractive index dielectric nanostructures1,2,3, and can be designed to appear at specifically defined frequencies4,5. Their presence gives rise to many fascinating phenomena such as photonic band gaps6,7,8, strong photon localization9, slow light10 and Dirac cones11. Fourier plane microscopy and spectroscopy are basic tools for characterization of photonic nanostructures as they enable capturing many essential properties of confined modes occurring in them. In Fourier space microscopy, as opposed to conventional real plane imaging, the information is presented as the function of angular coordinates12,13. It is alternatively known as back focal plane (BFP) imaging as the angular decomposition of the light emanating from the sample is recorded from the back focal plane of the microscope objective. The angular spectrum, i.e., the far field emission pattern of the sample is related to the momentum of light emanating from it (ħk). In particular, it represents its in-plane momentum (kx,ky) distribution14.
In magneto-optically active samples, the presence of confined photonic excitations has been shown to result in considerable enhancement of the magneto-optical response15,16,17,18,19. Magneto-optical effects depend on the mutual geometry of the magnetic field and the incident electromagnetic radiation. Most commonly encountered magneto-optical geometries for linearly polarized light and their nomenclature are depicted in Figure 1. Here, we demonstrate a setup that can be used to explore two magneto-optical effects that are observed in reflection: transverse and longitudinal magneto-optical Kerr effects, abbreviated, respectively, as TMOKE and LMOKE. TMOKE is an intensity effect, where the reflectivities of the opposing magnetization states are different while LMOKE manifests as a rotation of the reflected light polarization axis. The effects are distinguished by the orientation of the magnetization with respect to the light incidence, where for LMOKE, the magnetization is oriented parallel to the in plane component of the wave vector of the light while for TMOKE it is transverse to it. For normally incident light, both in-plane components of the momentum of light are null (kx = ky = 0) and, consequently, both effects are zero. Configurations where both effects are present can be easily conceived. However, to simplify the data analysis, in this demonstration we limit ourselves to situations where only one of the effects is present, namely TMOKE.
Several optical configurations can be used to measure the angular distribution of light emitted from magnetophotonic crystals. For example, in Kalish et al.20 and Borovkova et al.21, such a setup was successfully used in transmission geometry to unveil plasmon influence on magneto-optical phenomena. As an illustration, in Kurvits et al.22, some possible configurations are presented for a microscope that uses an infinity corrected objective lens. In our configuration, depicted in Figure 2A, we use an infinity corrected lens where the light coming from a given point in the sample is directed by the objective lens into collinear beams. In Figure 2A, beams emerging from the top (dashed lines) and the bottom (solid lines) of the sample are schematically depicted. Then, a collecting lens is used to refocus these beams to form an image at the image plane (IP). A second lens, also known as Bertrand lens, is then placed after the image plane to separate the incoming light at its focal plane into angular components, depicted in Figure 2A in red, blue and black. From this back focal plane, the angular distribution of the light emitted by the sample can be measured with a camera. Effectively, the Bertrand lens performs a Fourier transform on the light beam arriving at it. The spatial intensity distribution at the BFP corresponds to the angular distribution of the incident radiation. A full reciprocal space reflectance map of the sample can be established by illuminating the sample with the same objective that is used to collect the response of the sample. The incoming and out going beams are separated using a beam splitter. The complete setup is depicted in Figure 3A. To obtain a spectrum, a tunable light source or a monochromator is needed. The measurement can then be repeated over different wavelengths, keeping in mind that due to the spectrum of standard light sources, the results need to be normalized to the reflectivity of a control sample. For this purpose, one can use a mirror or a part of the sample that has been purposefully left unpatterned to allow for a high reflectivity. To assist in positioning, we show how to integrate the setup with an additional optical system that enables real-space imaging of the sample, shown in Figure 2B.
We now proceed to establish a method for measuring the angular resolved magneto-optical spectrum of a photonic crystal, using as a representative sample, a DVD grating covered with an Au/Co/Au film where the presence of ferromagnetic cobalt gives rise to considerable magneto-optical activity23. The periodic corrugation of the DVD grating enables surface plasmon polariton (SPP) resonances at distinct wavelength-angle combinations that are given by
where n is the refractive index of the surrounding environment, k0 the wave vector of light in free space, θ0 the incidence angle, d the periodicity of the grating and m is an integer denoting the order of the SPP. The SPP wave vector is given by where ε1 and ε2 are the permittivities of the metallic layer and the surrounding dielectric environment. Due to the thickness of the gold/cobalt multilayer film, we can assume that SPPs are only excited on top of the multilayer film.
1. Mounting the setup
2. Measurement procedure
3. Data analysis
Figure 4A shows a scanning electron microscope (SEM) micrograph of a commercial DVD grating covered with Au/Co/Au multilayer that was used a demonstration sample in our experiments. Its optical and magneto-optical spectra are shown in Figure 4B,C respectively. Details on sample fabrication are presented elsewhere23. Black lines in Figure 4A,B show the plasmon dispersion relations calculated from equation 1. The permittivity of the Au/Co/Au multilayer is taken from Supplementary Data File 1 in Cichelero et al.24 where a similar multilayer was measured using spectroscopic ellipsometry. Periodicity of the grating is assumed to be 740 nm. The calculated dispersion lines correspond to a conspicuous dip in reflectivity in Figure 4A that results from the incident radiation being converted into SPPs and dissipated via ohmic damping.
The relationship between the pixel positions in the back focal plane (Figure 3C) and angle of emission can be established as follows: the maximum angle θmax at which the objective can accept light is given by formula and depends on the numerical aperture NA = 0.8 and refractive index of the surrounding medium (air, n = 1). This is the angle that corresponds to the extremes of the illuminated area of the Fourier plane. The pixels between them can be assigned a number in a linear manner from –NA to +NA that reflects the numerical aperture at their position and their corresponding angle is then given by the inverse sine of this number (divided by n if necessary).
Figure 4C depicts the magneto-optical spectrum of the plasmonic grating. Here, the plasmon lines are accompanied by an increase in magneto-optical activity that abruptly reverses at the SPP. The line shape can be explained by the fact that the magnetization slightly changes the SPP excitation conditions, thus resulting in two different SPPs for opposite magnetization states. When the reflectivities of the two slightly displaced states are subtracted from each other, a characteristic derivative line shape is obtained15,16,17. The plasmon linewidths of the plasmon resonances as well as the resulting magneto-optical spectra depend strongly on the material parameters of the metal multilayer25,26.
We note that due to the geometry of the grating, the magnetic easy axis is oriented along the grating itself and very large magnetic fields are needed to saturate it out of this plane, for this reason LMOKE measurements are not feasible with this particular sample.
Figure 1: Different geometries where magneto-optical effects can be observed.
Polar (A), longitudinal (B) and transverse (C) magneto-optical Kerr effects are observed in reflection while Faraday (D) and Voigt (E) effects occur in transmission through magnetized medium. Please click here to view a larger version of this figure.
Figure 2: Optical setup.
(A) Schematic depiction of light propagation in the Fourier plane microscopic setup. The distinct angular components (depicted with red, black and blue rays) are spatially separated at the back focal plane. (B) Schematic depiction of the light propagation in the real space microscope. Lenses L1 and L2 form a telescope that images at the image plane to the camera. The distances between the components on the optical table are highlighted below each setup. Red numbers indicate that the distance is critical for image formation. Distances are in millimeters. Please click here to view a larger version of this figure.
Figure 3: Fourier space microscope and measurements.
(A) Components of the Fourier space microscope. (B) Schematic depiction of the polarization states of the light focused by the objective. Incident linearly (along x-direction) polarized light impinges on the sample as both TE- and TM-polarized depending on the part of the objective where the ray originates. (C) Intensity at the back focal plane of the microscope at λ = 600 nm when measuring the DVD grating. The black absorptive lines indicate SPP resonances that are also visible in Figure 4B,C. AOI can be chosen as the blue rectangle to measure response to TM-polarized light or red for TE-polarized. (D) Schematic hysteresis loop of a ferromagnetic material demonstrating the typical nonlinear response to applied magnetic fields. Please click here to view a larger version of this figure.
Figure 4: Measurements on a DVD grating sample.
(A) SEM micrograph of a commercial DVD grating covered with Au/Co/Au multilayer. Angular resolved reflectivity (B) and magneto-optical activity map (C) of the DVD grating with periodicity of 740 nm. Please click here to view a larger version of this figure.
We have introduced a measurement setup and protocol to obtain angular resolved magneto-optical spectra of optical crystals. In particular, the case of ferromagnetic materials, that requires additional data analysis to account for the nonlinear permeability of the material, has been laid out. Angular resolved magneto-optical spectroscopy presents an additional advantage over non-angular resolved methods that the confined modes can be more readily identified as they appear as clearly defined bands in both optical and magneto-optical spectra. The approach we show here can be readily adapted to various kinds of photonic crystals and is not limited to surface plasmon resonances.
Most common modification to the technique would be its adaptation to measure longitudinal and/or polar Kerr effects, that manifest as polarization rotation rather than intensity effects. To measure polarization rotation, an additional polarizer must be placed between the beam splitter and the collector lens to make the intensity detected at the camera proportional to polarization rotation. This polarizer should be placed at a 45° angle with the polarization of the light incident on the sample to maximize the magneto-optical signal27.
Common pitfalls in the measurement technique include incorrect mounting of the sample so that it can move when a magnetic field is applied. This can be aggravated by using magnetic metal such as iron in the sample holder. Even small quantities of magnetic metals such as small screws can result in movements that mask the magneto-optical effect entirely. A moving sample results typically in a “banana-like” incorrect hysteresis loop. Therefore, proper care needs to be taken in mounting the sample and making sure it is firmly in place before measurements. To confirm proper mounting of the sample, it is recommended to measure hysteresis loops using a wavelength/angle combination that is known to result in good signal and to confirm that its shape is as expected and that any artefacts from sample movement or other aberrations are not present.
As the measurement of the hysteresis loop requires looping over a range of applied magnetic field, the measurement takes some time. If the intensity level of the source is not stable over time, the magnetic field should be looped quickly to avoid power drift affecting the measured hysteresis loops. Typically, source power levels drift more slowly than a hysteresis loop can be measured, making it possible to measure the TMOKE contrast even under these conditions. If the signal is noisy and more averaging is needed, the averaging can be realized by increasing the number of loops measured rather than the number of frames at each magnetic field point.
This technique relies on applying the magnetic field in situ. While ferromagnetic materials usually maintain their magnetization state in the absence of applied magnetic fields, due to the small magnitude of the magneto-optical effects, removing the sample for manipulating the magnetization results in failure due to the difficulty of re-inserting the sample into exactly the same position as it was before the magnetization reversal.
The method that we have presented here relies on sensitive detection equipment and stable light sources. In standard magneto-optical Kerr spectrometry in longitudinal or polar Kerr configuration, a photoelastic modulator is often used to enhance the signal-to-noise ratio and to separate rotation and ellipticity components from each other27,28. However, the modulation frequency of a photoelastic modulator is typically more than 50 kHz which makes it very difficult to use with a microscope camera. Therefore, to obtain the best possible signal-to-noise ratio for a Fourier space magneto-optical microscope, it is necessary to invest in cameras and light sources with good stability.
In longitudinal and polar magneto-optical measurements, the intensity of light incident on the camera is greatly reduced due to the crossed polarizer placed before it, which puts additional requirements on the camera equipment needed for to detect the much weaker signal.
The authors have nothing to disclose.
We acknowledge financial support by the Spanish Ministerio de Economía y Competitividad through projects MAT2017-85232-R (AEI/FEDER,UE), Severo, Ochoa (SEV-2015-0496) and by the Generalitat de Catalunya (2017, SGR 1377), by CNPq – Brazil, and by the European Comission (Marie Skłodowska-Curie IF EMPHASIS – DLV-748429).
Beam splitter | Thorlabs | BSW27 | |
Bertrand lens | Thorlabs | LA1608 | f = 75 mm |
CCD Camera | Thorlabs | 1500M-GE-TE | Camera for real space imaging |
Collecting lens | Thorlabs | ITL200 | f = 200 mm |
Collimating lens | Zeiss | 420640-9800 | Magnification 10x NA 0.3 |
Flip mirror | Thorlabs | CCM1-P01/M | |
Flip mirror mount | Thorlabs | FM90/M | |
L1-lens | Thorlabs | LA1986 | f = 125 mm |
L2-lens | Thorlabs | LA1461 | f = 250 mm |
Objective lens | Nikon | MUE10500 | Magnification 50x NA 0.8 |
Pinhole | Thorlabs | ID8/M | |
Polarizer | Thorlabs | GTH10M | For LMOKE measurements, two polarizers are needed |
sCMOS camera | Andor | ZYLA-4.2P-USB3 |