We present a study of the dynamic magnetic properties of TiN-buffered epitaxial thin films of the Heusler alloy Fe1.5CoGe. Thickness series annealed at different temperatures are prepared and the magnetic damping is measured, a lowest value of α = 2.18 × 10−3 is obtained. The perpendicular magnetic anisotropy properties in Fe1.5CoGe/MgO are also characterized. The evolution of the interfacial perpendicular anisotropy constant KS with the annealing temperature is shown and compared with the widely used CoFeB/MgO interface. A large volume contribution to the perpendicular anisotropy of (4.3 ± 0.5) × 105 J/m3 is also found, in contrast with vanishing bulk contribution in common Co- and Fe-based Heusler alloys.

The need for strong perpendicular magnetic anisotropy (PMA)1–5 and low damping properties6–9 in next-generation spin-transfer-torque magnetic memory (STT-MRAM) generates a large interest towards Heusler alloys. In addition, large tunneling magnetoresistance (TMR) ratios with MgO tunneling barriers have been reported for several of them.10,11 For the application in devices based on STT switching, a low damping parameter α is important since the critical switching current is proportional to αMS212 for in-plane magnetized films, where MS is the saturation magnetization. With perpendicular magnetization, the critical current is further reduced and it is proportional to αMS.13 Therefore, a large effort is directed to study the PMA properties of Heusler alloys with low damping.

For the PMA of thin Heusler films, the interface-induced perpendicular anisotropy is essential and its strength is given by the perpendicular interfacial anisotropy constant KS. The interface properties, and therefore the value of KS, are strongly influenced by the conditions of the annealing, which is required to improve the crystalline order of the Heusler and MgO layers and to achieve large TMR values.

Here, we report the evolution of the PMA properties with annealing of the PMA properties in Fe1.5CoGe with a MgO interface, by measuring different thickness series and a comparison is made with the well-known CoFeB/MgO interface. The Gilbert damping parameter α changes with varying thickness and annealing temperature is also discussed.

The films were grown by sputtering, Rf-sputtering was used for the MgO deposition and dc-sputtering for the rest. For Fe1.5CoGe, the layer stack is MgO(S)/TiN(30)/Fe1.5CoGe(d)/MgO(7)/Si(2) with d = 80, 40, 20, 15, 11 and 9 nm. Four series were deposited and three of them annealed for one hour at 320°C, 400°C and 500°C. For CoFeB, the layer stack structure is MgO(s)/Ta(5)/Ru(30)/Ta(10)/MgO(7)/CoFeB(d)/MgO(7)/Ta(5)/Ru(2) d = 80, 40, 20, 15, 11, 9, 7 and 5 nm. The annealing was performed at 325°C and 360°C.

The dynamic properties and material parameters were studied by measuring the ferromagnetic resonance using a strip-line vector network analyzer (VNA-FMR). For this, the samples were placed facing the strip-line and the S12 transmission parameter was recorded.

Crystallographic properties of the CFA thin films were determined using x-ray diffraction (XRD) measurements in a Philips X’Pert Pro diffractometer with a Cu anode.

The XRD data corresponding to two 40 nm thick samples in the as-deposited state and annealed at 500°C are shown in Fig. 1(a). The (002) superlattice and the fundamental (004) peak of Fe1.5CoGe can be observed already for the as-deposited state but they experience a strong intensity increase with the thermal treatment. The TiN layer acts as a seed layer and its role in improving growth has been reported also for other alloys.1,14 Due to the similar lattice constant of TiN and MgO, the TiN film diffraction peaks are close to the substrate reflections and therefore difficult to separate. The films are B2-ordered, the presence of the (111) is not proven and therefore L21 order cannot be confirmed.

FIG. 1.

(a) X-ray diffraction patterns of 40 nm thin Fe1.5CoGe layers as-deposited, and annealed at 500°C. The (002) superlattice and the fundamental (004) peak of the Fe1.5CoGe are clearly visible, confirming the partial B2 crystalline order. (b) X-ray reflectometry data corresponding to the samples in (a).

FIG. 1.

(a) X-ray diffraction patterns of 40 nm thin Fe1.5CoGe layers as-deposited, and annealed at 500°C. The (002) superlattice and the fundamental (004) peak of the Fe1.5CoGe are clearly visible, confirming the partial B2 crystalline order. (b) X-ray reflectometry data corresponding to the samples in (a).

Close modal

Figure 1(b) shows X-ray reflectometry (XRR) data for the same films as in the (a) panel. The large number of oscillations prove the low roughness of the interfaces. This is due to the low roughness below 1 nm of the TiN buffer.14 The similarity between both data sets also proves that the topology of the interfaces do not vary in the studied temperature range.

Figure 2 shows the dependence of the field linewidth ΔH of the FMR peak on the resonance frequency fFMR for the sample series with no thermal treatment (as-deposited) and for the series annealed at 320°C and 400°C. In order to prevent poor visibility due to data overlap, the sets are shifted in the vertical axis, except the one corresponding to 320°C. The actual linewidth at 6 GHz is in the range 3.25 ± 0.15 mT. The lines represent the result to a linear fit to Eq. 1 to extract the damping parameter α:

(1)

Here, ΔH0 is the inhomogeneous broadening and is related to film quality, and γ is the gyromagnetic ratio.

FIG. 2.

Linewidth dependence on the frequency for Fe1.5CoGe thin films with a thickness of 20 nm for different annealing temperatures. The data sets have a vertical offset to improve visibility (+0.5 and +2 mT for the 400°C and as-deposited series, respectively). The lines correspond to a linear fit to extract the damping parameter α. The hollow points are not considered for the fits.

FIG. 2.

Linewidth dependence on the frequency for Fe1.5CoGe thin films with a thickness of 20 nm for different annealing temperatures. The data sets have a vertical offset to improve visibility (+0.5 and +2 mT for the 400°C and as-deposited series, respectively). The lines correspond to a linear fit to extract the damping parameter α. The hollow points are not considered for the fits.

Close modal

A deviation from this simple linear behavior is observed for the lower frequency range and these points have not been considered for the fit (hollow circles). This faster increase of linewidth with frequency is common in fully epitaxial Heusler layers7,15 and has been related with an increased anisotropic two-magnon scattering in the thin films for low frequency values resulting in an anisotropic ΔH. This anisotropy is not exclusive to Heusler alloys but it is expected in any epitaxial ferromagnetic film.16–18 The exact conditions for observation, however, depend on the material parameters and the spin-wave dispersion. For instance, in epitaxial Fe films, the low frequency ΔH behavior deviates only from a linear behavior when magnetic dragging due to crystalline anisotropy is dominant.19 

An additional sample set annealed at 500°C showed no visible FMR peak pointing to a degradation of the magnetic properties of Fe1.5CoGe for high annealing temperature. This is in constrast with Co-based Heusler alloys where large temperatures are typically required for optimal properties. For instance, for Co2FeAl, lowest damping is achieved at 600°C7 and for Co2MnSi, very low damping is still present at 750°C.20 

The results for the damping parameter α obtained from the linear fits are summarized in Fig. 3. A reduction of damping is observed when comparing the as-deposited samples to the annealed ones but the samples annealed at 400°C show larger damping than the ones annealed at 320°C. Combined with the absence of an FMR peak for 500°C, this reinforces the conclusion that the optimal annealing temperature for good dynamic properties of Fe1.5CoGe is low. The lowest damping is 2.18 ± 0.03 × 10−3 for the 20 nm thick film annealed at 320°C. For Co-based Heusler alloys, the lowest reported damping is achieved to be 7 × 10−4 in Co2MnSi.20 For Co2FeAl, values around 1-3 × 10−3 are reported depending on the annealing conditions.7,8 Concerning Fe-based alloys, values in the range of 1.2-1.9 × 10−3 are reported for Fe1+xCo2−xSi,9 for Fe2Cr1−xCoxSi α varies between 9 × 10−3 with the lowest value of 8 × 10−4 for Fe2CoSi.21 Therefore, the obtained value for the damping parameter in our alloy is in the lower range of previously reported ones and slightly reduced compared to those reported for the related alloy CoFeGe.22 It is also smaller than the ones reported for widely used polycrystalline CoFeB23,24 and permalloy.25–28 

FIG. 3.

Dependence of the Gilbert damping parameter α on the thickness d for three sample series: as-deposited, annealed at 320°C, and annealed at 400°C.

FIG. 3.

Dependence of the Gilbert damping parameter α on the thickness d for three sample series: as-deposited, annealed at 320°C, and annealed at 400°C.

Close modal

The thickness dependence of α shows a minimum around 20 nm and an increase for larger and smaller thicknesses. This behavior has been already observed for Co2FeAl,8 and the reasons are similar to that alloy and different for the two thickness ranges. For soft magnetic thin films, a strong damping increase with increasing thickness is expected starting at a certain value. An example can be found for NiFe in the literature.29 The reason is a non-homogeneous magnetization state for thicker films which opens new loss channels via increased magnon scattering and other effects.30,31 An increase due to eddy current losses, which scale with d2, may also contribute to this behavior.46 For the thinner films, the damping increase is due to two reasons. When the thickness is reduced and the effect of the interface anisotropy is becoming larger the magnetization state is becoming more inhomogeneous due to the counterplay between the demagnetization field and the anisotropy field.32 In addition, other effects related to an increased role of surface roughness with decreasing film thickness play also a role.

The effective magnetization Meff is extracted using a fit to Kittel’s formula33 to the dependence of the resonance field HFMR on the resonance frequency fFMR. For a more detailed description of the FMR measurement and analysis procedure see Ref. 34. Meff is related to the saturation magnetization of the film by36–38 

(2)

where KS and KV are the perpendicular surface (or interfacial) and the bulk anisotropy constants, respectively.

Figure 4 shows the dependence of Meff on the inverse thickness 1/d for the three sample series: as-deposited, annealed at 320°C and annealed at 400°C. The slope provides the value of KS. The constant shows a positive value for the as-deposited series, 0.41 ± 0.12 mJ/m2, i.e. favouring a perpendicular orientation of the magnetization. However, the value is small in absolute value and it grows only slightly upto 0.51 ± 0.17 mJ/m2 when the samples are treated at 320°C. The annealing at 400°C changes the situation drastically. The value of KS is much larger, −1.36 ± 0.14 mJ/m2, but it also suffers a change of sign which implies that the interface induces an in-plane orientation of the magnetization. It is remarkable that this change of the magnetic properties of the interface developes without a large modification of the morphology, as proven by the XRR data shown in Fig. 1(b). The inset in Fig. 4 summarizes the dependence of KS on the annealing temperature.

FIG. 4.

Dependence of Meff extracted from the Kittel fit on the inverse thickness 1/d for three Fe1.5CoGe sample series: as-deposited, annealed at 320°C and annealed at 400°C. The lines are a fit to Equation 2. The inset shows the evolution of KS with the annealing temperature.

FIG. 4.

Dependence of Meff extracted from the Kittel fit on the inverse thickness 1/d for three Fe1.5CoGe sample series: as-deposited, annealed at 320°C and annealed at 400°C. The lines are a fit to Equation 2. The inset shows the evolution of KS with the annealing temperature.

Close modal

The evolution of KS, including the sign change, is caused by a rearrangement of atoms at the immediate interface and is not connected to a roughness modification. Theoretical studies45 for the Heusler/MgO interface show that for the interface originated PMA properties, the termination of the Heusler film and the strength of the hybridization of certain orbitals in ordered interfaces are critical. By locally improving the crystalline order, the hybridization of the orbitals is modified and also the termination can be changed due to the fact that thermal energy is required for formation of a certain termination.

Taking into account the saturation magnetization Ms obtained by alternating gradient magnetometer (AGM), 1100 ± 120 kA/m, it is possible to determine also the volume contribution to the perpendicular anisotropy to be (4.3±0.5)×105Jm3. This large value ensures, that for a 1.5 nm thin film and even for the 320°C case, the PMA properties are dominated by the bulk contribution. Recently, we reported the evolution of the PMA properties of the Co2FeAl/MgO interface8 and the situation is very different for that alloy. First, no interface-generated PMA is present in the as-deposited samples and it only appears after annealing. Second, KS is always positive and larger than for Fe1.5CoGe/MgO and the absence of a remarkable volume contribution makes the PMA there controlled only by the interface. Also in the related alloy Co20Fe50Ge30 there is no bulk contribution to the perpendicular anisotropy and a interface contribution (0.9 mJ/m2) larger than that obtained here.35 The most probable reason for the difference is the lower Fe content in our case. The presence of this strong bulk contribution to PMA is quite remarkable since it is absent in common Co- and Fe-based Heusler alloys and only observed in tetragonally distorted MnGa or MnGe related Heusler alloys.39–41 

For comparison, the PMA properties of the widely used CoFeB/MgO interface were also measured. The data is shown in Fig. 5 for annealing temperatures of 325°C and 360°C. An as-deposited series was not characterized since CoFeB is amorphous in that state. The lines are a fit to Eq. 2 with a prefactor 2 before KS to account for the presence of two interfaces since a trilayer system MgO/CoFeB/MgO was used.

FIG. 5.

Dependence of Meff extracted from the Kittel fit on the inverse thickness 1/d for two MgO/CoFeB/MgO sample series: annealed at 325°C and annealed at 360°C. The lines are a fit to Equation 2 with a prefactor 2 (see text).

FIG. 5.

Dependence of Meff extracted from the Kittel fit on the inverse thickness 1/d for two MgO/CoFeB/MgO sample series: annealed at 325°C and annealed at 360°C. The lines are a fit to Equation 2 with a prefactor 2 (see text).

Close modal

The CoFeB/MgO interface shows a robust interface perpendicular anisotropy, three times larger than for Fe1.5CoGe/MgO, and slightly decreases with temperature. The bulk contribution is zero or too small to be detectable. These results are comparable to the literature.42–44 We conclude that while the Co2FeAl8 and CoFeB/MgO are very similar in absolute values, thermal evolution and relative weight of interface and bulk contribution to PMA, Fe1.5CoGe/MgO differ strongly.

The exact meaning of the concept of inhomogeneous magnetization used to describe our films, and of the counterplay between demagnetizing field and anisotropy field need to be described with more detail: in an ideal thin film with smooth interfaces and in the case of KS=0, the demagnetizing field induces ideally a perfect in-plane orientation of the magnetization and a homogeneous state with an external applied field. For the case of a large enough KS>0 and for a thickness below a critical value (d < dmin) the magnetization is again fully homogeneous but oriented perpendicularly and for d > dmax an homogeneous in-plane state is expected. In between, for a transition region dmin < d < dmax different inhomogeneous states can be formed. Some of them can be modelled by a simple analytical model or by micromagnetic simulations as for instance in Ref. 32 but in most cases they will be also influenced by defects and magnetic history and would be difficult to model. It has to be noted that an inhomogeneous magnetization state near the interface is always present due to the fact that the interface anisotropy acts only locally. The effective anisotropy field commonly used for comparing the strength does not imply that it is there is a field applied homogenously on the film.

In summary, the damping properties of the Heusler alloy Fe1.5CoGe and the perpendicular magnetic anisotropy of the Fe1.5CoGe/MgO system have been studied. From the thickness dependent magnetic properties for as-deposited and annealed series we obtained a minimum value for α of 2.18 ± 0.03 × 10−3 for a 20 nm thick film. The evolution of the interface perpendicular anisotropy constant on the annealing temperature is shown and compared with the standard interface CoFeB/MgO. We found a large and dominant volume contribution to the PMA, which differs from CoFeB or other well studied alloys as Co2FeAl and the interface contribution suffers a sign change depending on the annealing temperature. We explained the increase on damping with decreasing thickness in terms of a counterplay between demagnetizing field and interface PMA and correlate it with the obtained values for KS.

Financial support by M-era.Net through the HEUMEM project is gratefully acknowledged.

1.
A.
Niesen
,
J.
Ludwig
,
M.
Glas
,
R.
Silber
,
J.-M.
Schmalhorst
,
E.
Arenholz
, and
G.
Reiss
,
J. Appl. Phys.
121
,
223902
(
2017
).
2.
Y.
Takamura
,
T.
Suzuki
,
Y.
Fujino
, and
S.
Nakagawa
,
J. Appl. Phys.
115
,
17C732
(
2014
).
3.
T.
Kamada
,
T.
Kubota
,
S.
Takahashi
,
Y.
Sonobe
, and
K.
Takanashi
,
IEEE Trans. on Magn.
50
,
1
(
2014
).
4.
B. M.
Ludbrook
,
B. J.
Ruck
, and
S.
Granville
,
J. Appl. Phys.
120
,
013905
(
2016
).
5.
B. M.
Ludbrook
,
B. J.
Ruck
, and
S.
Granville
,
Appl. Phys. Lett.
110
,
062408
(
2017
).
6.
M.
Oogane
,
R.
Yilgin
,
M.
Shinano
,
S.
Yakata
,
Y.
Sakuraba
,
Y.
Ando
, and
T.
Miyazaki
,
J. Appl. Phys.
101
,
09J501
(
2007
).
7.
S.
Mizukami
,
D.
Watanabe
,
M.
Oogane
,
Y.
Ando
,
Y.
Miura
,
M.
Shirai
, and
T.
Miyazaki
,
J. Appl. Phys.
105
,
07D306
(
2009
).
8.
A.
Conca
,
A.
Niesen
,
G.
Reiss
, and
B.
Hillebrands
,
J. Phys. D: Appl. Phys.
51
,
165303
(
2018
).
9.
C.
Sterwerf
,
S.
Paul
,
B.
Khodadadi
,
M.
Meinert
,
J.-M.
Schmalhorst
,
M.
Buchmeier
,
C. K. A.
Mewes
,
T.
Mewes
, and
G.
Reiss
,
J. Appl. Phys.
120
,
083904
(
2016
).
10.
N.
Tezuka
,
N.
Ikeda
,
S.
Sugimoto
, and
K.
Inomata
,
Jpn. J. Appl. Phys.
46
,
L454
(
2007
).
11.
S.
Tsunegi
,
Y.
Sakuraba
,
M.
Oogane
,
K.
Takanashi
, and
Y.
Ando
,
Appl. Phys. Lett.
93
,
112506
(
2008
).
12.
Z.
Diao
,
Z.
Li
,
S.
Wang
,
Y.
Ding
,
A.
Panchula
,
E.
Chen
,
L.-C.
Wang
, and
Y.
Huai
,
J. Phys. D: Appl. Phys.
19
,
165209
(
2007
).
13.
K. L.
Wang
,
J. G.
Alzate
, and
P. K.
Amiri
,
J. Phys. D: Appl. Phys.
46
,
074003
(
2013
).
14.
A.
Niesen
,
M.
Glas
,
J.
Ludwig
,
J.-M.
Schmalhorst
,
R.
Sahoo
,
D.
Ebke
,
E.
Arenholz
, and
G.
Reiss
,
J. Appl. Phys.
118
,
243904
(
2015
).
15.
M.
Oogane
and
S.
Mizukami
,
Phil. Trans. R. Soc. A
369
,
3037
(
2011
).
16.
G.
Woltersdorf
and
B.
Heinrich
,
Phys. Rev. B
69
,
184417
(
2004
).
17.
R.
Arias
and
D. L.
Mills
,
Phys. Rev. B
60
,
7395
(
1999
).
18.
Kh.
Zakeri
,
J.
Lindner
,
I.
Barsukov
,
R.
Meckenstock
,
M.
Farle
,
U.
von Hörsten
,
H.
Wende
,
W.
Keune
,
J.
Rocker
,
S. S.
Kalarickal
,
K.
Lenz
,
W.
Kuch
,
K.
Baberschke
, and
Z.
Frait
,
Phys. Rev. B
76
,
104416
(
2007
).
19.
A.
Conca
,
S.
Keller
,
M. R.
Schweizer
,
E. Th.
Papaioannou
, and
B.
Hillebrands
,
Phys. Rev. B
98
,
214439
(
2018
).
20.
S.
Andrieu
,
A.
Neggache
,
T.
Hauet
,
T.
Devolder
,
A.
Hallal
,
M.
Chshiev
,
A. M.
Bataille
,
P.
Le Fèvre
, and
F.
Bertran
,
Phys. Rev. B
93
,
094417
(
2016
).
21.
S.
He
,
Y.
Liu
,
Y.
Zheng
,
Q.
Qin
,
Z.
Wen
,
Q.
Wu
,
Y.
Yang
,
Y.
Wang
,
Y.
Feng
,
K.
Leong Teo
, and
C.
Panagopoulos
,
Phys. Rev. Materials.
1
,
064401
(
2017
).
22.
H.
Lee
,
Y.-H. A.
Wang
,
C. K. A.
Mewes
,
W. H.
Butler
,
T.
Mewes
,
S.
Maat
,
B.
York
,
M. J.
Carey
, and
J. R.
Childress
,
Appl. Phys. Lett.
95
,
082502
(
2009
).
23.
C.
Bilzer
,
T.
Devolder
,
J.-V.
Kim
,
G.
Counil
,
C.
Chappert
,
S.
Cardoso
, and
P. P.
Freitas
,
J. Appl. Phys.
100
,
053903
(
2006
).
24.
A.
Conca
,
E. Th.
Papaioannou
,
S.
Klingler
,
J.
Greser
,
T.
Sebastian
,
B.
Leven
,
J.
Lösch
, and
B.
Hillebrands
,
Appl. Phys. Lett.
104
,
182407
(
2014
).
25.
A.
Ruiz-Calaforra
,
T.
Brächer
,
V.
Lauer
,
P.
Pirro
,
B.
Heinz
,
M.
Geilen
,
A. V.
Chumak
,
A.
Conca
,
B.
Leven
, and
B.
Hillebrands
,
J. Appl. Phys.
117
,
163901
(
2015
).
26.
C.
Luo
,
Z.
Feng
,
Y.
Fu
,
W.
Zhang
,
P. K. J.
Wong
,
Z. X.
Kou
,
Y.
Zhai
,
H. F.
Ding
,
M.
Farle
,
J.
Du
, and
H. R.
Zhai
,
Phys. Rev. B
89
,
184412
(
2014
).
27.
J. O.
Rantschler
,
R. D.
McMichael
,
A.
Castillo
,
A. J.
Shapiro
,
W. F.
Egelhoff
,
B. B.
Maranville
,
D.
Pulugurtha
,
A. P.
Chen
, and
L. M.
Connors
,
J. Appl. Phys.
101
,
033911
(
2007
).
28.
P.
Krautscheid
,
R. M.
Reeve
,
D.
Schönke
,
I.
Boventer
,
A.
Conca
,
A. V.
Chumak
,
B.
Hillebrands
,
J.
Ehrler
,
J.
Osten
,
J.
Fassbender
, and
M.
Kläui
,
Phys. Rev. B
98
,
214406
(
2018
).
29.
Y.
Chen
,
D.
Hung
,
Y.
Yao
,
S.
Lee
,
H.
Ji
, and
C.
Yu
,
J. Appl. Phys.
101
,
09C104
(
2007
).
30.
J.
Foros
,
A.
Brataas
,
Y.
Tserkovnyak
, and
G. E. W.
Bauer
,
Phys. Rev. B
78
,
140402
(
2008
).
31.
S.
Zhang
and
S. S.-L.
Zhang
,
Phys. Rev. Lett.
102
,
086601
(
2009
).
32.
N. A.
Usov
and
O. N.
Serebryakova
,
J. Appl. Phys.
121
,
133905
(
2017
).
34.
A.
Conca
,
S.
Keller
,
L.
Mihalceanu
,
T.
Kehagias
,
G. P.
Dimitrakopulos
,
B.
Hillebrands
, and
E. Th.
Papaioannou
,
Phys. Rev. B
93
,
134405
(
2016
).
35.
M.
Dinga
and
S. J.
Poon
,
Appl. Phys. Lett.
101
,
122408
(
2012
).
36.
M.
Johnson
,
P.
Bloemen
,
F.
Den Broeder
, and
J.
De Vries
,
Rep. Prog. Phys.
59
,
1409
(
1996
).
37.
J.-M. L.
Beaujour
,
W.
Chen
,
A. D.
Kent
, and
J. Z.
Sun
,
J. Appl. Phys.
99
,
08N503
(
2006
).
38.
M.
Belmeguenai
,
H.
Tuzcuoglu
,
M. S.
Gabor
,
T.
Petrisor
, Jr.
,
C.
Tiusan
,
D.
Berling
,
F.
Zighem
,
T.
Chauveau
,
S. M.
Chérif
, and
P.
Moch
,
Phys. Rev. B
87
,
184431
(
2013
).
39.
A.
Niesen
,
N.
Teichert
,
T.
Matalla-Wagner
,
J.
Balluf
,
N.
Dohmeier
,
M.
Glas
,
C.
Klewe
,
E.
Arenholz
,
J.-M.
Schmalhorst
, and
G.
Reiss
,
J. Appl. Phys.
123
,
113901
(
2018
).
40.
A.
Niesen
,
C.
Sterwerf
,
M.
Glas
,
J.-M.
Schmalhorst
, and
G.
Reiss
,
IEEE Trans. on Magn.
52
,
1
(
2016
).
41.
K. Z.
Suzuki
,
A.
Ono
,
R.
Ranjbar
,
A.
Sugihara
, and
S.
Mizukami
,
IEEE Trans. on Magn.
53
,
1
(
2017
).
42.
D. C.
Worledge
,
G.
Hu
,
D. W.
Abraham
,
J. Z.
Sun
,
P. L.
Trouilloud
,
J.
Nowak
,
S.
Brown
,
M. C.
Gaidis
,
E. J.
O’Sullivan
, and
R. P.
Robertazzi
,
Appl. Phys. Lett.
98
,
022501
(
2011
).
43.
X.
Liu
,
W.
Zhang
,
M. J.
Carter
, and
G.
Xiao
,
J. Appl. Phys.
110
,
033910
(
2011
).
44.
T.
Liu
,
Y.
Zhang
,
J. W.
Cai
, and
H. Y.
Pan
,
Sci. Rep.
4
,
5895
(
2014
).
45.
R.
Vadapoo
,
A.
Hallal
,
H.
Yang
, and
M.
Chshiev
,
Phys. Rev. B
94
,
104418
(
2016
).
46.
M. A. W.
Schoen
,
J. M.
Shaw
,
H. T.
Nembach
,
M.
Weiler
, and
T. J.
Silva
,
Phys. Rev. B
92
,
184417
(
2015
).