Effect of seed layers on the static and dynamic magnetic properties of CoIr films with negative effective magnetocrystalline anisotropy

Tianyong Ma(馬天勇), Sha Zhang(張莎), Chenhu Zhang(張晨虎), Zhiwei Li(李志偉),Tao Wang(王濤),?, and Fashen Li(李發(fā)伸)

1The Key Laboratory of Physics and Photoelectric Information Functional Materials,North Minzu University,Yinchuan 750021,China

2Key Laboratory for Magnetism and Magnetic Materials of the Ministry of Education,Lanzhou University,Lanzhou 730000,China

Keywords: seed layers,magnetic anisotropy,surface free energy,soft magnetic thin films

1.Introduction

Soft magnetic thin films (SMTFs) are widely investigated and highly desired for practical applications,such as microwave absorbers, inductors, micro-transformers, exchangecoupled composite media,and near field electromagnetic noise absorbers.[1,2]In practical application,SMTFs have to possess the basic demands including high saturation magnetizationMs,low coercivityHc, high permeability, and high natural resonance frequency(fr)as far as possible.Fe-and Co-based soft magnetic films exhibit excellent saturation magnetization,low coercivity,and high electrical resistivity.[3,4]Their microwave properties are governed by the following equation in the bianisotropy model:[5]

whereμiandfrare the initial permeability and the natural resonance frequency, respectively.γis the gyromagnetic ratio.Hgrain= 2Kgrain/Msis the effective magnetocrystalline anisotropy field with the corresponding magnetocrystalline anisotropy constantKgrain.According to our previous work,[6]oriented hcp-CoIr SMTFs with a certain Ir content have the effective negative magnetocrystalline anisotropy.It is clear that negativeKgraincan increasefrwithout affectingμifrom Eq.(1).Moreover,magnetic moments are strictly restricted in the film plane by negative magnetocrystalline anisotropy.So,the oriented hcp-CoIr film can have sufficient thickness to obtain enough magnetic flux signal in practical uses of magnetic devices.

The metal seed layers between the substrate and the magnetic film, such as Ta/Pt/Ru, Ti/Au, and Ta/Ru, have made a highly oriented hcp-CoIr film.[6,7]The higher oriented texture of CoIr films has a smaller negative magnetocrystalline anisotropy as the Cu or Cu/Ru seed layers can increase the perpendicular magnetic anisotropy of Co80Pt20films.[8]Moreover, good soft magnetic properties have also been obtained,namely,the seed layer is effective to reduceHcwithout affectingMs.Studies have reported that Co,Cu,and Ru seed layers make FeCo films magnetically softer.[9]Simultaneously, the high-frequency properties determined by the static magnetic parameters are also improved by using a seed layer, such as Fe65Co35thin films with Ru and Rh seed layers.[10]In highfrequency practical applications, the magnetic damping constantαis also a key parameter and varies a bit with the choice of seed layer.[10]With the extrinsic contribution, the lowerαvalue is associated with less magnetic inhomogeneities.[11]And the intrinsic contribution is relative to fundamental properties such asMs.[12]In other words,epitaxial growth induced by a seed layer is the most efficient method to form a higher orientation and make the films magnetically softer and to improve high-frequency properties.

CoIr grains with strong negative magnetocrystalline anisotropy have an hcp structure.As mentioned above, the hcp-Ru (002) and fcc-Au (111) seed layers were used to induce thec-axis orientation of CoIr grains.Although the fcc-(111) plane of Ni, Cu, Ir, and Pt is similar to the hcp-(002)plane of CoIr, the seed layers of these metals have not been studied for CoIr SMTFs.Moreover, lattice mismatch ratios have a tremendous influence on the crystallographic quality of epitaxial thin films[13,14](e.g.,magnetic film’s stress state and texture formation).Therefore, in order to investigate and understand the effects of other material seed layers and lattice mismatch ratios on the CoIr magnetic layer, we used the fcc-(111)Ni,Cu,Ir,Pt,and Au seed layers to induce the oriented hcp-CoIr thin films with thec-axis of grains perpendicular to the film plane.We studied the effects of different seed layers on microstructure, soft magnetic properties, and negative effective magnetocrystalline anisotropy.Besides the static magnetic properties, dynamic studies were performed using field sweep ferromagnetic resonance(FMR)measurements and the damping constant affected by seed layers was studied through a vector network analyzer(VNA).

2.Experiment

All magnetic thin films studied in this work were prepared by the DC magnetron sputtering technique, which is similar to our earlier work with a layered structure of substrate/Ti/M/CoIr (M=Ni, Cu, Ir, Pt, Au, none) as shown in Fig.1(a).A Si wafer with surface oxidation was used as the substrate, and the amorphous Ti layer (8 nm) was deposited on the substrate in order to provide a clean and flat surface.The oriented seed layerM(Ni, Cu, Ir, Pt, Au) of about 25 nm was grown on the Ti layer to help the CoIr magnetic layer reach about 50 nm.Compared with other films,the film was fabricated without a seed layer between the Ti layer and the magnetic layer.When fabricating the Ti and seed layers, purity Ar was used as the sputtering working gas at a pressure of 0.25 Pa.Then under the condition of 0.3 Pa purity Ar, CoIr magnetic layers were sputter deposited using a Co target with five Ir chips symmetrically placed on the Co target.About 10 cm away from the targets, the substrates were mounted on the center of the sample turntable.Chemical composition has been characterized by energy dispersive spectrometry (EDS).The crystalline structures were studied using the x-ray diffraction technique(XRD).The morphologies were observed by transmission electron microscopy (TEM).The static magnetic properties were measured with a vibrating sample magnetometer (VSM).Total out-of-plane anisotropy fields and the effective negative magnetocrystalline anisotropy were thoroughly investigated by electron spin resonance measurements (ESR).The damping constants for all films were thoroughly investigated by a VNA.

3.Results and discussion

Schematic diagrams of the hcp-CoIr(002)plane and fcc-M(111) plane are shown in Fig.1(b).Half of the regular hexagon is seen on both the hcp-CoIr(002)plane and the fcc-M(111)plane,suggesting that lattice mismatches come from the difference in inter-atomic distance.The inter-atomic distances of fcc-(111)Ni,Cu,Ir,Pt,and Au are 2.49 ?A,2.55 ?A,2.72 ?A,2.77 ?A,and 2.88 ?A,respectively.The lattice mismatch ratios are about-0.81%,1.59%,8.37%,10.36%,and 14.74%for the lattice spacing of hcp-Co(002)of～2.51 ?A.

Fig.1.(a) Schematic of the layer structure of our samples.(b) The crystal structures of fcc-(111)Ni,Cu,Ir,Pt,Au,and hcp-CoIr(002),half of the regular hexagon on M(111)plane and CoIr(002)plane are marked with red dotted lines.

XRD patterns of the samples measured with aθ-2θscan are shown in Fig.2(a).Only two diffraction peaks corresponding to theM(111) plane and the CoIr (002) plane can be seen.For the sample without a seed layer, only CoIr (002)has a diffraction peak.Obviously,the intensity of theM(111)peak gradually increases and the position shifts to low 2θbecause of the enlargement of the lattice parameters from Ni to Au.With the lattice mismatch ratio,the positions of the CoIr(002) peak show no obvious changes, and the intensity first showed small changes,then rapidly became strong and sharp.However, for the film without a seed layer, there is a significant right drift of the CoIr (002) peak, which indicates that the lattice constant of the CoIr phase becomes small.The smaller lattice constant results from the decreasing number of Ir atoms successfully entering the crystal structure of hcp-(CoIr).Meanwhile, the CoIr (002) peak gets broader and its intensity becomes weaker.Therefore, the films with a seed layer are more textured along thec-axis alignment than the film without a seed layer.And the degree of orientation improved by increasing the lattice mismatch ratio.However,the intensity of the CoIr (002) peak for the Au seed layer film is about 11 times that of the Ni seed layer film, which is inexplicable.As shown in Fig.2(b), we plot the crystalclattice parameter and FWHM determined from the profile fit to the CoIr(002)peak.One can see thatcshows little change with the exception of the first one.The mean value of 0.4125 nm is about 0.13%larger than that of the firstcparameter,which has been explained previously.Moreover, the values of the FWHM increase from 0.31 for the Ni seed layer film to 0.35 for the film with an Ir seed layer,then inversely reach 0.28 for the Au seed layer film.Obviously, the value of the no-seed layer film becomes about 1.4 times larger than that of the Au seed layer film.The smaller FWHM of the magnetic layer can be caused either by the reduction in defects and/or internal stress or by the increased crystallite size of the film or both of the reasons above.[15]In Fig.3, we present the images of the morphology of the CoIr films with Au and Ni seed layers from TEM measurements.For the Au seed layer film,the grain size is uniform and grain boundaries are distinct,whereas the size of the crystallization areas is uneven and there are no clear boundaries for the Ni seed layer film.Significantly,the figure showing the Ni seed layer film reveals the mixing of crystallite regions and amorphous regions,which provides an explanation for the large peak intensity ratio.Moreover, Co and Ir atoms may reside at the interstitial site or fill in the interspace between individual grains, which may lead to an increase in defects and/or internal stress.

Fig.2.(a)XRD patterns of the oriented hcp-Co81Ir19 films with different seed layers.(b)Lattice parameters c and FWHM,obtained by fitting the CoIr(002)peak shown in panel(a),with different seed layers.

Fig.3.Images of the morphology of the CoIr films with Au and Ni seed layers,respectively.

The in-plane magnetic hysteresis loops of all the films are shown in Fig.4(a).These loops were measured with the applied magnetic field parallel to the easy axis during measurements.The remanence ratios of all loops are above 0.92 and the nearly rectangular loops are clearly observed.Furthermore, the determined saturation magnetization 4πMsand coercivityHcfrom the above hysteresis measurements are plotted in Fig.4(b).There are no obvious changes in 4πMsabout 12.4 kOe for the CoIr magnetic layer,which agrees well with reported values.[7]For the Ni seed layer film,4πMsof only the CoIr magnetic layer is 12.8 kOe as shown in Fig.4(b),whereas the saturation magnetization containing both a Ni seed layer and CoIr layer is about 10.7 kOe.With increasing the lattice mismatch ratio,Hcincreases from 54.9 Oe for the Ni seed layer film to 74.3 Oe for the film with a Cu seed layer,then decreases gradually to 27.4 Oe.The reduction in coercivity can be linked drastically to the reduction of defects and/or internal stress,[16]the reduction of the crystallite size,and the increase in exchange coupling between the crystallites.[17]Considering that the tendency ofHcis similar to that of the FWHM with the lattice mismatch ratio, we speculate that the main reason for the change inHcand FWHM is the same.As is known, the change in crystallite size may cause the opposite tendency of the FWHM and coercivity.Therefore,the change inHcand FWHM may be mainly attributed to the reduction of defects and/or internal stress with the lattice mismatch ratio.For the film without seed layer,the value remarkably reaches 103.5 Oe about 3.8 times larger than the smallest one.This very large value may come from many defects and/or strong internal stress and/or the large in-plane component of the magnetocrystalline anisotropy field.

Fig.4.(a) Normalized in-plane magnetic hysteresis loops of the oriented hcp-Co81Ir19 films with different seed layers.(b) The seed layer dependence of the determined 4πMs and Hc for the oriented hcp-Co81Ir19 films.

As emphasized in our earlier work,[6]we now investigate the magnetic anisotropy properties of our films using ESR measurements.The resonance fields were measured with an external magnetic field applied to the film plane.The microwave magnetic field of about 9 GHz was applied perpendicular to the film plane.As shown in Figs.5(a)-5(f), the resonance fields of all films display a well-defined in-plane uniaxial symmetry as a function of field orientationφH, suggesting the samples have an in-plane uniaxial anisotropy.[18]The uniaxial anisotropy is induced by the slight oblique deposition angle,and can be explained within the framework of the so-called self-shadowing model.[19]TakingHuandHθas adjustable parameters, we fitted the experimental data by the following equations:[20]

whereHθis the total effective out-of-plane anisotropy field,Hris the resonance field,φ0is the value ofφMwith the equilibrium positions,ωis the angular frequency of about 18π, andγis the gyromagnetic ratio.The fitted results are consistent in the measured datum and drawn in Figs.5(a)-5(f) as black solid lines.The extracted in-plane uniaxial anisotropy fieldsHuare shown in Fig.5(g) as open black squares.Obviously,Huchanges slightly around 18 Oe because of the slight oblique deposition angle.ForHθshown in Fig.5(h),the deduced values increase from 10.9-26 kOe with the lattice mismatch ratio,whereas they reduce to 23.2 kOe for the film without a seed layer.For the Ni seed layer film,the correctedHθis 11.6 kOe when the perpendicular anisotropy of the Ni seed layer is eliminated.According to the equationsHθ=4πMs-HgrainandHgrain=2Kgrain/Ms,the calculatedKgrainis shown in Fig.5(i).The values are all negative and different from each other,suggesting thatKgrainis affected by a seed layer and the seed layer material.

Fig.5.(a)-(f) Angle dependence of the in-plane resonance field for the oriented hcp-Co81Ir19 films with different seed layers.The black solid lines denote the theoretical fits to the experimental datum represented by red dots.(g) The determined in-plane anisotropy field Hu,(h)the total effective out-of-plane anisotropy field Hθ, (i)the deduced magnetocrystalline anisotropy constant Kgrain as a function of the lattice mismatch ratios for different seed layers.

According to the reported literature,[21,22]Kgrainis sensitive to the lattice geometry and microstructure, which is restricted by the growth mode of the magnetic layer.The growth modes are mainly governed by the seed-layer surfacefree energyγs, the magnetic layer surface free energyγf, the strain energyγe, and the interface energyγi.[23]Except for Ir(3.231 J·m-2), the surface free energies of Ni (2.364 J·m-2),Cu(1.934 J·m-2),Pt(2.691 J·m-2),Au(1.626 J·m-2),and Ti(2.570 J·m-2)are smaller than that of Co(2.709 J·m-2).[24,25]As the Ir atomic diameter is bigger than that of Co, the lattice constant of the hcp-CoIr phase becomes bigger with the increase in Ir.We speculate that the surface-free energy of Co is smaller than that of CoIr.Furthermore, theγsfor the Ni,Cu, Pt, an Au seed layer and Ti amorphous layer is smaller than theγfof the CoIr magnetic layer, whereas theγsof Ir may be slightly greater than theγfof the CoIr layer.Again takingγiandγeinto consideration,it is easy to satisfy the relationshipγs-γf-γe-γi<0.Therefore,the deposited magnetic layer forms three-dimensional islands or clusters at the initial stage, then the following growth has the trend of random orientation distribution and rough surface.As reported in the literature,[26]defects and/or internal stress and/or dislocations may appear at the interface.However, with increasing the lattice mismatch ratio, the mismatch strain between the seed layer and the magnetic layer varies from compressive stress to tensile stress, and tensile stress gradually becomes larger.In order to relieve the mismatch strain, the degree of the orientation of the hcp-CoIr grains may be improved, the microstructure and appearance may be changed,the defects and/or internal stress may be reduced,the crystallite width may be refined,and dislocations may be decreased.We find that the main contribution is both the increasing degree of orientation and the reduction in defects and/or internal stress so that it is consistent with the reason for decreasedHcand FWHM values.The reduced strain energyγeis favorable to the layer-by-layer growth of the magnetic layer.During the growth process,the layer-by-layer growth is conducive to improving the degree of the orientation and to reducing the defects and/or internal stress;[27]hence, a smallerKgrainis obtained.Apart from these, the different stacking structure ratios and crystallinity and atomic site ordering can also be linked drastically toKgrain.[21]For the Ni seed layer film,amorphous regions appear as shown in Fig.3.And it is difficult to form the hcp-CoIr phase with an easy plane and to improve the degree of orientation because the Ni(111)direction perpendicular to the film plane is an easy axis of magnetization; thus,Kgrainis approximately zero.Despite easily forming hcp stacking,the film without a seed layer has much more random orientation grains and defects, holes, and grain boundaries because of the three-dimensional islands’ growth and un-epitaxial growth.[28]Besides, the different seed layer metals have different seed layer thickness ranges,which yield the highlyc-axis oriented hcp-(CoIr)films.[29]The seed layer thickness of about 25 nm is optimal for Au metal,whereas the range of the thickness of other metals is not discussed.The other seed layer fixed at 25 nm thickness may be not conducive to the realization of thec-axis oriented growth and hcp stacking.Therefore,the Au seed layer film has the minimumKgrainof about-5.299×106erg·cm-3.

Fig.6.(a)-(f)Permeability spectra of the oriented hcp-Co81Ir19 films with different seed layers.(g)The initial permeabilityμi,(h)the natural resonance frequency fr, (i) the derived damping constant α for different seed layers.The anshown as solid black squares aredetermined from the measured spectra.The calculated values using the determined 4πMs and the in-plane anisotropy field from the VSM and ESR measurements are also shown for comparison.

In high-frequency applications,the dimensionless damping constantαis one of the key parameters of ultra-high frequency devices.[30]Restricted by the damping constant, the complex permeability spectra can be described by the following formula deduced from the Landau-Lifshitz-Gilbert(LLG)equation[31]

in whichω1=γ(4πMs-Hgrain+Hu) =γ(Hθ+Hu),ω2=γHu, whereωis the angular frequency andαis the damping constant.Using the in-plane anisotropy field andαas the free fitting parameters, we fitted the experimental curves by Eq.(3)as shown in Figs.6(a)-6(f).The extracted in-plane anisotropy fields are 221 Oe,220 Oe,220 Oe,220 Oe,228 Oe,and 231 Oe for the Ni,Cu,Ir,Pt,Au,and no seed layer films,respectively.These values are very close to the extractedHuplus 200 Oe applied field.As given in Fig.6(i), the obtainedαincreases from 0.063 for the Ni seed layer film to 0.075 for the film with a Cu seed layer,then decreases gradually to 0.034 for the Au seed layer film.However,the value of the no seed layer film reaches 0.06,which is about 1.76 times larger than the smallest one.It is well known that the damping constant consists of two parts, namely, the intrinsic and extrinsic contributions.The intrinsic part largely depends on fundamental properties such asMsand the spin-orbit coupling effect.[11,32]AsMsis extremely close to a constant except for in the Ni seed layer film,this part has no influence onα.With the same origin in spin-orbit coupling,[33]the serious fluctuation inKgrainindicates thatαis subject to variation.In general, there is no linear relationship betweenKgrainandα.Besides, the extrinsic part is generally explained by the defect-induced two magnon model and/or the local resonance model,[34]both of which are associated with magnetic inhomogeneities within the material (e.g., due to anisotropy dispersion and surface or interface roughness).As mentioned above, the improved orientation in the grains and the reduced defects and/or internal stress result in the decrease in magnetic inhomogeneities.With increasing the lattice mismatch ratio,a decreasing trend is shown in both FWHM andα,while the discrepancy is also obvious.Therefore, the extrinsic part plays a vital role in the variation inα, and the intrinsic part is also a supplemental factor.Interestingly,because of the smallest extrinsic part,the minimum ofαis inevitable for the Au seed layer film.

4.Conclusion

In summary,c-axis oriented hcp-Co81Ir19magnetic films were successfully prepared on different seed layers(Ni,Cu,Ir,Pt,Au,and no seed),and were investigated thoroughly by different measurement techniques.The orientation and defects of thec-axis oriented hcp-(CoIr) grains are strongly affected by the seed layer.The coercivityHcandKgrainare strongly dependent on the seed layer and seed layer material.While the determined saturation magnetization 4πMsand in-plane uniaxial anisotropy fieldsHuare independent of the lattice parameters, microstructure, and material of the seed layer.As expected,the initial permeability has little relation to the seed layer, while the natural resonance frequency is strongly restricted throughKgrainaffected by the lattice mismatch ratio.The extracted lowerαis relative to the improved grain orientation and the reduced defects and/or internal stress.Among all the films, the film for the Au seed layer has the optimal performance of soft magnetic properties and microwave properties.We expect that these results can further help us improve the static and dynamic frequency properties for further applications.

Acknowledgements

Project supported by the Natural Science Foundation of Ningxia in China (Grant No.2022AAC03288)and the Ningxia New Solid Electronic Materials and Devices Research and Development Innovation Team (Grant No.2020CXTDLX12).