C.
Tian
a and
A. O.
Adeyeye
*ab
aDepartment of Electrical and Computer Engineering, National University of Singapore, 117576, Singapore. E-mail: adekunle.o.adeyeye@durham.ac.uk
bDepartment of Physics, Durham University, South Rd, Durham, DH1 3LE, UK
First published on 29th January 2024
Magnonic crystals, periodic arrays of magnetic structures, have emerged as a promising platform for manipulating and controlling spin waves in magnetic materials. Magnetic antidot nanostructures, representing 2-D magnonic crystals, are versatile platforms for controlling and manipulating magnons. In this work, we systematically investigate the effects of inter-hole spacing and lattice (rhombic and honeycomb) arrangements on the dynamic properties of Ni80Fe20 antidot structures. The dynamic responses of antidot lattices of fixed hole diameter (d = 280 nm) and inter-hole spacing (s) between 90 and 345 nm are investigated using broadband ferromagnetic spectroscopy. Multiple resonance modes sensitive to s are observed due to the inhomogeneous internal field distribution induced by the presence of holes. There is a marked variation in mode frequency, mode intensity and the number of modes for rhombic antidot lattice as the inter-hole spacing and applied field direction are varied. Our experimental results are in good agreement with micromagnetic simulations. Our findings may find application in the design of magnonic-based devices.
The magnetic properties of antidot structures with square lattice are extensively studied by varying the applied field orientation and strength,17 hole diameter,10 inter-hole spacing,7 thickness,19 and hole shape.20 There are fewer reports in the literature on the experimental investigation of the effects of geometrical parameters on the magnetic properties of rhombic and honeycomb antidot lattices.12
In this study, we systematically investigated the dynamic behaviors displayed by rhombic and honeycomb Ni80Fe20 (permalloy, Py) antidots characterized by a fixed diameter (d = 280 nm) and varying inter-hole spacing (s) within the range of 90 nm to 345 nm. We observed that the FMR responses of antidot structures are highly sensitive to the s and Happ directions. Antidot lattices exhibit a significant tunability of the number of observed modes and mode frequency, which can be tailored by varying s and Happ directions.
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Fig. 2 (a) Experimental and (b) Simulated FMR spectra of 25 nm thick permalloy rhombic antidot lattices as a function of s taken at Happ = −1400 Oe along the X and Y directions. |
We have performed a series of dynamic simulations to understand further the origin of the complex FMR spectra observed. Fig. 2(b) shows the corresponding simulated FMR spectra of rhombic antidot lattices as a function of s for Happ along the X direction. There is a good agreement between the experimental results (Fig. 2(a)) and simulated FMR spectra. We have extracted the mode profile by performing FFT on in-plane magnetization components (mY) to identify the FMR modes. We have plotted the profiles for the observed modes for rhombic antidot lattices for Happ applied along the X-direction in Fig. 3(a) as a function of s. The simulated FMR spectrum of s = 90 nm identifies six distinct modes that reside along the Y-direction. We found that mode R1 is enclosed between two next-nearest neighbor holes in the same column, while modes R(2–6) are localized between the two nearest-neighbor holes. Mode R4 shows a stripe-like profile which connects two nearest-neighbor holes. Modes (R2, R3, R5, R6) show a blade-shaped profile with a strong spin precession amplitude at the edges of holes. Instead of three modes R(4–6) found in the simulation, we only observed one shoulder of mode R4 in the experiment, which may be attributed to the fact that modes (R5, R6) are too weak to be resolved in the experiment.
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Fig. 3 Spatial profiles of modes in the simulated FMR spectra taken at Happ = −1400 Oe along (a) X and (b) Y directions of 25 nm thick permalloy rhombic antidot lattices as a function of s. |
For s = 170 nm, mode R1 shows a profile similar to s = 90 nm but with a large amplitude near the hole edges. However, we observed that the R3 mode intensifies while the R2 mode weakens but persists in both the experimental and simulated data.
For s = 345 nm, however, fewer modes are observed. Instead of a single peak of mode R1 observed in the experiment, we found a dual peak with very close frequencies in the simulation. Mode R1 for s = 345 nm shows a very similar profile to that for s = 90 nm. We also noticed a satellite mode R1′, which resides along the Y direction, close to the hole edges. This may be attributed to the increasingly inhomogeneous magnetization near the edges of the holes when s/d is larger. It is possible to qualitatively understand the decrease in observed mode number as s is increased since the FMR responses of the antidot structures resemble that of the continuous un-patterned film, which has a single FMR mode with a resonance frequency fcont = 11.2 GHz in our reference film. This is similar to the frequency of mode R1 at fcont = 11.2 GHz for s = 345 nm.
The corresponding simulated FMR spectra of rhombic antidot lattices for the Happ applied along the Y direction as a function of s are shown in Fig. 2(b). The significant difference in the FMR spectra between Happ along X and Y directions for the range of s investigated is attributed to the induced configurational anisotropy of the lattice symmetry.
We have also extracted the profiles for the observed modes identified in Fig. 3(b) as a function of s. When Happ is applied along the Y direction, these observed modes reside along X. In the simulation, the excitation field hsinc, represented by a sinc wave, is applied perpendicular to the Happ. This configuration effectively stimulates the magnetization perpendicular to the hsinc direction, mimicking the actual experimental conditions.
For s = 90 nm, we found that mode R7 is localized in the area between rows of holes while mode R12 is localized between two nearest-neighbor holes of the same row. In the simulation, mode R7 is a dual peak with very close frequencies, labelled modes R7 and R7′. They display complementary spatial profiles due to a local variation in the dynamic magnetization, which is sensitive to the simulation. This dual peak manifests itself as a single peak in the experiment. Other minor modes R(8–11) show complicated spatial profiles, mainly located between rows of holes, because of hybridization effects with the higher frequency mode.16
For s = 170 nm, we found that the intensity of mode R7 becomes more pronounced than s = 90 nm, which was also confirmed in the experiment. We did not observe mode R9, probably because it is too weak to be identified. For s = 345 nm, the intensity of mode R7 is further increased, and it is confirmed in the simulation. The profile of mode R7 for s = 345 nm shows a symmetry node in the middle region between rows of holes with a peak amplitude near the holes’ edges. This is quite different when compared with the profile of mode R7 for s = 90 and 170 nm. The increase in the intensity of mode R7 as s is increased can be explained by considering its resonance area, which is extended in the area between rows of holes. When s is increased, the contribution from this area is increased due to more materials (increasing the width of the resonant area), so mode R7 becomes more pronounced. Interestingly, fewer modes are identified for s = 345 nm, probably because different modes combined or are too weak to be observed.
For Happ along the X and Y directions, we will discuss the frequency shift of the most prominent modes, i.e., R1 and R12. In the experimental spectra, we observed the frequency of mode R1 (fR1) increases while mode R12 (fR12) decreases when s is increased from 90 nm to 345 nm in agreement with the simulated FMR spectra. The frequency shift can be explained by considering the variation of the demagnetizing field with the increase of s for the resonance areas of modes R1 and R12. The X and Y components of the demagnetizing field (Hd) for Happ along the X and Y directions at point c have been extracted from OOMMF simulations as functions of s and plotted in Fig. 4. We observed that the Hd at point c becomes negative when Happ is applied along the +X direction and positive when Happ is applied along the +Y direction. From a qualitative standpoint, this behavior can be elucidated by treating the region around point c as a rectangular magnet outlined by the green dashed line. Point c experiences a greater demagnetizing field (opposite to the magnetization orientation) when Happ is along the +X direction than when Happ is along the +Y direction. This discrepancy arises because the X direction represents the short axis of the rectangular magnet, leading to a negative Hd at point c when Happ is along the +X direction. It is important to note that the actual value of Hd is influenced not only by the green magnet but also by the collective field exerted by the five magnets (one green and four yellow magnets). When Happ is applied along the +Y direction, Hd becomes positive, considering the contribution from the four yellow magnets. The absolute values of Hd exhibit a decreasing trend due to the increasing spacing between magnets. As the spacing (s) increases, the fields exerted by these five magnets diminish. Consequently, the nanostructure behaves more akin to a large film with increasing s, causing Hd-x and Hd-y to converge to 0.
As a result, point c has a larger internal field (Hint) for Happ applied along Y (Hint = Happ + Hd) than Happ along X (Hint = Happ − Hd). This explains the larger resonance frequency of mode R12 compared to mode R1 for all the s investigated. We also observed that the absolute value of Hd decreases with an increase in s for both Happ directions. Consequently, for mode R1, the Hint of its resonance area increases as s increases, while for mode R12, the Hint decreases as s increases. It explains how fR1 increases while fR12 decreases with an increase in s.
We can also understand the change of fR1 and fR12 with s qualitatively. As s increases, the antidot structure will behave more like a continuous un-patterned film with a resonance frequency (fcont = 11.2 GHz in our reference film) independent of Happ directions. So fR1 and fR12 approach the fcont of the continuous film when s is increased. This may, therefore, explain the convergent trend of fR1 and fR12 as s is increased.
Fig. 5(a) shows the experimental FMR absorption spectra of honeycomb antidot lattices taken at Happ = −1400 Oe along the X and Y directions as a function of s. Unlike rhombic lattices, the FMR spectra for Happ along X and Y directions are similar. The corresponding simulated FMR spectra of honeycomb antidot lattices for Happ along the X and Y directions as a function of s are shown in Fig. 5(b). There is good agreement between the experimental and simulated results.
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Fig. 5 (a) Experimental and (b) Simulated FMR spectra of 25 nm thick permalloy honeycomb antidot lattices as a function of s taken at Happ = −1400 Oe along the X and Y directions. |
For s = 90 nm, three distinct modes H1 (9.1 GHz), H2 (12.1 GHz) and H3 (15.8 GHz) is observed for the spectrum of Happ along X direction and three modes H4 (9.9 GHz), H5 (12 GHz) and H6 (16.5 GHz) for Happ along Y direction. As s is increased to 170 nm, we observed that the prominent mode H2 splits and the frequency of prominent mode H5 (fH5) decreases to 11.8 GHz. As s is further increased to 345 nm, mode H2 (fH2) frequency decreases to 11.6 GHz, and mode H5 (fH5) decreases to 11.5 GHz. We have observed an overall convergence of modes H (1–3) and H(4–6) as s increases.
We have plotted the profiles for the observed modes H (1–6) for different s in Fig. 6. For s = 90 nm, we found that mode H1 extends as a continuous resonant stripe along Y while mode H4 extends as another continuous stripe along X enclosed by the holes. Note that there is only a single stripe for mode H1 within one honeycomb unit cell, while there are two stripes for mode H4. Modes H2 and H5 are localized at the central region of the honeycomb unit cell. Mode H3 is enclosed between two nearest-neighbor holes in the rows of holes along directions, and H6 is enclosed between two nearest-neighbor holes in the horizontal rows of holes. For s = 170 nm, modes H1, H4, H5 and H6 show a similar profile to that for s = 90 nm. Mode H2 becomes triplet modes and is localized in different areas within the hexagonal unit cell. Mode H3 is enclosed between two nearest-neighbor holes in the rows of holes along
directions. For s = 345 nm, mode H1 extends as a more uniform resonant stripe along Y compared with the cases of s = 90 and 170 nm, which show a more concentrated spin precession amplitude between two horizontal nearest-neighbor holes. Mode H3 becomes too weak to be identified, while Mode H4 displays a symmetry node in the middle region between rows of holes with a peak amplitude near the holes’ edges. This mode profile evolution of H4 is similar to that of mode R7 in the rhombic antidot lattice.
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Fig. 6 Spatial profiles of modes in the simulated FMR spectra taken at Happ = −1400 Oe along X and Y directions of 25 nm thick permalloy honeycomb antidot lattices as a function of s. |
It is worth noting that the resonance frequency variations with Happ direction and s are less pronounced in the honeycomb antidot lattice than in the rhombic antidot lattice discussed earlier. For example, as s is increased from 90 nm to 345 nm, the frequency shifts of prominent modes H2 and H5 are small (∼0.5 GHz) compared with what was observed for rhombic antidot lattice where a distinct frequency shift of 1.7 GHz for mode R1 and 2.7 GHz for mode R12 with s increasing from 90 nm to 345 nm. The marked difference between rhombic and honeycomb antidot lattices is attributed to an additional hole at the central region of the hexagonal unit cell in the rhombic lattice. The presence of an additional hole induces a larger variation in demagnetisation field as a function of s. Consequently, it produces a larger resonance frequency modification with s and different Happ directions.
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