x-ray magnetic circular dichroism study of multiferroic...
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X-ray Magnetic Circular Dichroism
Study of Multiferroic and Dilute
Magnetic Materials
Doctor Thesis
Virendra Kumar Verma
Department of Physics
Faculty of Science & Graduate School of Science
THE UNIVERSITY OF TOKYO
July, 2012
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Abstract
Spintronics materials like multiferroics and dilute magnetic
semiconductors (DMSs) have attracted a great deal of attention in
the scientific community from the viewpoints of both academic
research and practical applications. In order to elucidate the origin
of ferromagnetism of these spintronics materials, it is necessary to
investigate the electronic structure. Advances in experimental
techniques such as synchrotron radiation and electron
spectroscopies provide us with great opportunities to unravel the
underling physics producing the magnetic properties of the
materials. In this thesis, I have investigated the electronic
structure of spintronics materials using x-ray absorption
spectroscopy (XAS) and x-ray magnetic circular dichroism (XMCD).
Recently, thin films consisting of alternating ferrimagnetic
spinel-type NiFe2O4 (NFO) and ferroelectric perovskite-type
BaTiO3 (BTO) layers BTO/(NFO/BTO)n were prepared and
exhibited the coexistence of ferroelectric and ferromagnetic
ordering with strong magnetoelectric (ME) coupling between them
[1, 2], but the origin of ME coupling is still remains unclear because
in previous studies, the techniques used to characterize the ME
coupling of NFO/BTO heterostructures were mostly measure
macroscopic quantities. For that purpose, XAS and XMCD at the
both Ni and Fe 2 → 3 absorption edges are an ideal technique to
clarify this issue because they are element-specific microscopic
probes. Here, I have studied the local electronic and magnetic
states of Ni and Fe ions in the NFO/BTO multilayers grown on
(001)-SrTiO3 substrates using pulsed laser deposition with various
NFO and BTO thicknesses by XAS and XMCD in the bulk-sensitive
total-fluorescence yield (TFY) mode at room temperature. The
measured Ni 2p and Fe 2p spectra indicate that the Ni ions are
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octahedrally coordinated by oxygen and are divalent (Ni2+) and that
the Fe ions are trivalent (Fe3+) and are tetrahedrally or
octahedrally coordinated by oxygen with opposite spin directions,
consistent with the inverse spinel structure of NiFe2O4. With
increasing number of layers, both Ni and Fe magnetic moments
decrease. With decreasing NFO layer thickness, the average
magnetic moment of the Ni ions decreases while the average
magnetic moment of the Fe ions remain unaffected, meaning that
Ni ions replaced by Fe ions at the interface lose ferromagnetic
ordering. I found clear correlation between the ME coupling
strength and the ferromagnetic moment of Fe. This suggests that
the enhancement of ME coupling occurs at interfacial Fe-TiO2
bonding. The Fe-TiO2 bonding creates oxygen vacancies and the
oxygen vacancies at the interface may play an important role to
enhance the ME coupling.
Further, I performed XAS and the XMCD studies of
Cd1-x-yMnxCryTe thin films with Cr content y varied from 0 to 0.04
while keeping the Mn content x fixed around 0.20 grown on GaAs
(001) substrates by the molecular beam epitaxy (MBE) technique.
The prototypical DMS Cd1-xMnxTe is a spin-glass (x<0.6) or
antiferromagentic (x>0.6). Shen et al. [3] found that Cr doping into
Cd1-xMnxTe turns the system from the antiferromagnetic spin glass
to a ferromagnet. In order to elucidate the origin of ferromagnetism,
interaction between Mn and Cr has to be clarified. I found that both
Cr and Mn ions are divalent and that the spins alignment of Cr and
Mn are parallel. The ferromagnetic moment of Mn increases with
Cr concentration. I found the equal concentration of ferromagnetic
Cr and Mn ions in Cd0.76Mn0.2Cr0.04Te sample. These results
suggest that in the presence of Cr ions in Cd1-x-yMnxCryTe, the
interaction between Mn spins changes from antiferromagnetic to
ferromagnetic mediated by the Cr ions and the possible mechanism
of ferromagnetic ordering between Mn and Cr ions is due to the
double exchange interaction.
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Next, I have studied the possible existence of orbital magnetic
moment in multiferroic MnWO4 using the Mn L2;3-edge XMCD.
Shanavas et al. [4] reported a finite but very small orbital magnetic
moment from ab initio electronic-structure calculations. By
applying the orbital sum rule to the XMCD spectrum, despite the d5
configuration of Mn2+ ion, a significantly large orbital magnetic
moment was deduced. The distorted (MnO6)10- octrahedra play an
important role in giving rise to the apparently large orbital
magnetic and electric polarization in MnWO4. The orbital magnetic
moment is in the same direction of the spin magnetic moment,
indicating that Mn 3d states are more than half-filled. Using the CI
cluster-model analysis, I found that the average 3d occupancy, n3d,
is equal to 5.09.
References
[1] C. Deng, Y. Zhang, J. Ma, Yuanhua Lin, and C. W. Nan, J. Appl.
Phys. 102, 074114 (2007).
[2] J. Liu, Y. Zhang, Yuanhua Lin, and C. W. Nan, J. Appl. Phys.
105, 083915 (2009).
[3] S. Shen, X. Liu, Y. J. Cho, J. K. Furdyna, M. Dobrowolska, Y. H.
Hwang, and Y. H. Um, Appl. Phys. Lett. 94, 142507 (2009).
[4] K. V. Shanavas, Debraj Choudhury, I. Dasgupta, Surinder M.
Sharma, and D. D. Sarma, Phys. Rev. B 81, 212406 (2010).
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Contents
Page
Abstract 3
Chapter 1: Introduction 11
1.1 Spintronics 11
1.2 Multiferroics 12
1.2.1 Multiferroic materials and magnetoelectric effect 12
1.2.2 Single-phase multiferroics 13
1.2.3 Physical properties of MnWO4 15
1.2.3.1 Structural properties of MnWO4 15
1.2.3.2 Multiferroic properties of MnWO4 16
1.2.4 Composite multiferroics (Two-phase systems) 20
1.2.4.1 Multiferroic CoFe2O4-BaTiO3
nanostructures
20
1.2.4.2 Multiferroic NiFe2O4-BaTiO3
Heterostructure
21
1.3 Diluted magnetic semiconductors 24
1.3.1 Transition metal doped CdTe 29
References 30
Chapter 2 Principles of x-ray magnetic circular dichroism 37
2.1 X-ray absorption spectroscopy 37
2.2 X-ray magnetic circular dichroism 39
2.3 XMCD sum rules 42
2.4 Configuration-interaction cluster model 43
References 48
Chapter 3 Experimental Details 51
3.1 NSRRC BL-11A 51
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3.2 KEK-Photon Factory BL-16A 55
3.3 SPring-8 BL23SU 58
References 60
Chapter 4 Origin of enhanced magnetoelectric coupling in
BaTiO3/NiFe2O4 multilayers studied by x-ray
magnetic circular dichroism
63
4.1 Introduction 64
4.2 Experimental 65
4.3 Results and discussion 67
4.4 Conclusions 77
References 78
Chapter 5 Cr-doping induced ferromagnetism in the
antiferromagnetic spin glass Cd1-xMnxTe
81
5.1 Introduction 82
5.2 Experimental 83
5.3 Results and discussion 84
5.4 Conclusions 94
References 95
Chapter 6 Orbital magnetic moment in multiferroic MnWO4
studied by x-ray magnetic circular dichroism
99
6.1 Introduction 99
6.2 Experimental 102
6.3 Results and discussion 102
6.4 Conclusions 108
References 110
Chapter 7 Summary and outlook 115
Appendix Orbital magnetic moment in FeCr2S4 studied by x-
ray magnetic circular dichroism
121
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A.1 Introduction 121
A.2 Experimental 122
A.3 Results and discussion 123
A.4 Conclusions 132
References 133
Acknowledgements 137
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Chapter 1
Introduction
1.1 Spintronics
Spintronics (or spin based electronics) also known as
magnetoelectronics, in which charge and spin degrees of freedom of
electrons, can be used simultaneously in order to develop a new
generation of useful electronics devices, and processes with new
functionality have become the subjects of growing interest for
researchers [1.1, 2, 3]. Spintronic devices are expected to develop
upon conventional electronics and photonic devices, allowing for
enhancement in the form of less power consumption, faster device
operation, and new forms of information computation. Possible
applications of spintronics devices include high-speed magnetic
filters, spin-polarized LEDs, sensors, spin-field effect transistors
(SFETs), quantum transistors, and spin-based qubits for quantum
computers [1.4, 5, 6, 7]. The key advantage of spintronic device is
that multiple functions can be integrated in the same chip, which
can function simultaneously as a memory and amplifier. The
utilization of electron spin in practical devices has already been
proven as spin valves, which are used as magnetic tunnel junctions
in magnetic random access memories (MRAM). Since electron spin
exists in either spin-up or spin-down configuration, spintronic
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materials would also open a door for the development of rewritable
devices that are nonvolatile.
1.2 Multiferroics
1.2.1 Multiferroic materials and magnetoelectric
effect
Multiferroic is a material that simultaneously possesses two
or more of the ferroic order. These ferroic order parameters are
ferroelectricity, ferromagnetism, and ferroelasticity. The phase
control in ferroics and multiferroics are shown in fig. 1.1. Coupling
interaction between the different order parameters could produce
additional effects, such as magnetoelectric (ME) effect. The
magnetoelectric (ME) effect is the phenomenon of inducing
magnetization by applying an external electric field and/or the
Figure 1.1: The phase control in ferroics and multiferroics [1.9]
phenomenon of inducing electric polarization by applying an
external magnetic field. Though the mechanisms that allow
ferroelectricity and ferromagnetism seem to be incompatible, there
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are a select few materials in which ferroelectricity and
ferromagnetism are both present. Theoretical studies have shown
that the usual atomic-level mechanisms driving ferromagnetism
and ferroelectricity are mutually exclusive, because
ferromagnetism and ferroelectricity require empty and partially
filled transition metal orbitals, respectively [1.8].
1.2.2 Single-phase multiferroics
ME response has been found in a relatively small number of
single-phase multiferroic materials. The first ferromagnetic
ferroelectric material to be discovered is nickel iodine boracite,
Ni3B7O13I [1.10]. This discovery was followed by the synthesis of
several multiferroic boracites compounds, all of these compounds
have complex structures with many atoms per formula unit and
more than one formula unit per unit cell. In these materials, the
essential factors of causing the multiferroicity and the nature of the
coupling between the magnetic and electric polarization and
structural order parameters are a number of inter-ionic interaction.
Nickel iodine boracite can be thought of as the ‘Rochelle salt’ of
magnetic ferroelectrics and it has wide applicability and contribute
to our increased understanding in the field. Other ferromagnetic
ferroelectrics materials were also searched by replacement of some
of the d0 B cations in ferroelectric perovskite oxides (ABO3) by
magnetic dn cations. (1-x)Pb(Fe2/3W1/3)O3 – xPb(Mg1/2W1/2)O3 [1.11]
is an example of first synthetic ferroelectric ferromagnetic material
in which Mg and W ions are diamagnetic and cause the
ferroelectricity, and the formally d5 Fe3+ ion is responsible for the
magnetic ordering. In the past few years, there has been renewed
interest in studying a number of other perovskite-based
multiferroic materials, such as manganites of small rare earth
elements [1.12, 13] and yttrium [1.14] and a few compounds in
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which Bi [1.15] is the large cation, which have large
magnetoelectric effects.
In the spiral type-II type of multiferroic materials, the
electrical polarization is caused by a spiral order of the magnetic
moments. The relevant exchange striction in these spiral magnets
is associated with the antisymmetric part of the exchange coupling,
known as the Dzyaloshinskii-Moriya interaction (DMI) [1.16].
Table 1.1 lists some of the known single phase multiferroic
materials adapted from [1.17]
Table 1.1 Example of single phase multiferroic materials that
exhibit ME effect.
Compound Type of
electric order
Type of
magnetic order
Tc (K) TN (K)
Pb (Fe2/3W1/3)O3 FE AFM 178 363
Pb (Fe1/2Nb1/2)O3 FE AFM 387 143
Pb (Co1/2W1/2)O3 FE WFM 68 9
Pb (Mn2/3W1/3)O3 AFE? AFM 473 203
Pb (Fe1/2Ta1/2)O3 FE AFM 233 180
Eu1/2Ba1/2TiO3 FE FM 165 4.2
BiFeO3 FE AFM 1123 650
BiMnO3 AFE FM 773 103
YMnO3 FE AFM 913 80
YbMnO3 FE AFM/WFM 983 87.3
HoMnO3 FE AFM/WFM 873 76
ErMnO3 FE AFM 833 79
Ni3B7O13I FE WFM 64 64
Ni3B7O13Br FE WFM 398 30, 40
Co3B7O13I FE WFM 197 38
*FE – Ferroelectric, AFE – Antiferroelectric, FM – Ferromagnetic, AFM –
Antiferromagnetic, and WFM – Weak ferromagnetic.
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Among the multiferroic manganates, MnWO4 takes a special
place as it does not contain a rare-earth ion, leaving Mn formally as
the only magnetic ion. It has already been proved that
ferroelectricity in MnWO4 can appear in the cycloidal-spiral spin
phase without centrosymmetry [1.18, 19]. Multiferroicity in which
electrical polarization is caused by the spiral order of magnetic
moments is explained by the spin-current model [1.20, 21]. If the
spin-rotation axis ê is not parallel to the magnetic propagation
vector Q, nonvanishing spontaneous polarization P α ê ×Q develop.
The research presented in chapter 6 is focused on the magnetic
properties of MnWO4.
1.2.3 Physical properties of MnWO4
1.2.3.1 Structural properties of MnWO4
The structure of MnWO4 is a wolframite structure, which
belongs to the monoclinic space group P2/c with β ~ 91º at room
temperature. Figure 1.2 (a) shows the crystal structure of MnWO4.
The crystal structure is characterized by alternative stacking of
manganese and tungsten layers parallel to the (100) plane as
shown in Fig. 1.2 (b). Mn2+ ions are surrounded by distorted oxygen
octahedra and aligned in zigzag chains along the c axis. Due to
distortion, the three different bond lengths of Mn-O in MnO6
octahedron are 2.09 Å, 2.18 Å, and 2.27 Å, respectively [1.23]. In
AF1 and AF3, magnetic moments collinearly align in the ac plane
forming an angle of about 35º with the a axis, whereas in AF2 an
additional component in the (010) direction exists, as shown in Figs.
1.2 (b) and 1.2 (c), respectively.
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Figure 1.2: (a) Crystal structure of MnWO4 viewed along the a axis:
each Mn atom (purple) is surrounded by an oxygen (red) octahedron.
W atoms (gray) separate zigzag chains of Mn atoms. (b) Collinear
magnetic structure in AF1 and AF3: magnetic moments lie in the ac
plane and canted to the a axis by about 35º. (c) Elliptical spiral spin
structure in AF2: basal plane of spiral is inclined to the ab plane.
[1.22]
1.2.3.2 Multiferroic properties of MnWO4
MnWO4 exhibits three different magnetic phase transitions at
T1 = 7.6 K, T2 = 12.7 K and TN = 13.5 K [1.24] to three long
wavelength antiferromagnetic (AF) ordering states. According to
neutron diffraction results, AF1 (T < T1), AF2 (T1 < T < T2), and AF3
(T2 < T < TN) are a commensurate collinear antiferromagnetic
phase, an incommensurate cycloidal spiral-spin phase, and an
incommensurate collinear antiferromagnetic phase, respectively.
The magnetic structure of the AF1 state is commensurate with the
propagation vector (−1/4, 1/2, 1/2), while that of the AF3 and AF2
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Figure 1.3: (a) Magnetic susceptibility for each crystal axis as a
function of temperature in 0.1 T. (b) Dielectric constant for E // b in
0 T. (c) Electric polarization ∆P // b in 0 T. During the measurement
of pyroelectric current to obtain ∆P, an electric field of 500 kV/m
was continuously applied along the b axis in a cooling process. ∆P
was calculated by integrating the measured pyroelectric current
with respect to time. [1.22]
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states are incommensurate with the propagation vector (−0.214, 1/2,
0.457). Figure 1.3 (a) shows the temperature dependence of the
magnetic susceptibility (χ) at magnetic field of 0.1 T parallel to the a,
b, and c axis, respectively. In all direction, a cusp is observed in χ at
Neel temperature TN ~ 13.5 K. Above TN, χ(T) follows the
Curie-Weiss law with a negative Weiss temperature (θ ~ 78 K). At
the transition temperature T1, χb shows a steep rise, while χa and χc
show a sharp drop. This behavior is consistent with the neutron
diffraction result that the easy axis of the Mn2+ moments is within
the ac plane in AF1 [1.24]. Figures 1.3 (b) and (c) display
temperature dependence of dielectric constant (εb) and electric
polarization (∆Pb) in zero magnetic field. εb shows a sharp peak at
T2, and a very small drop (~0.08%) at T1. As seen in Fig. 1.3 (c), the
spontaneous polarization exists in the AF2 phase between T1 and
T2. These results clearly indicate that MnWO4 becomes
ferroelectric simultaneously when the AF2 phase with the spiral
spin configuration appears.
Recently, Hollmann et al. [1.23] studied magnetic anisotropy
in multiferroic MnWO4 by soft x-ray absorption spectroscopy (XAS)
at room temperature. They found that Mn ions in MnWO4 are in
the high-spin Mn2+ electronic configuration and a crystal-field level
scheme is different from octahedral (Oh) for the MnWO4 system.
Figure 1.4 shows the room temperature Mn L2,3 XAS spectra of
MnWO4 taken with the E vector of the light parallel to the a, b, and
c crystallographic axes and found a small but clear polarization
dependence for MnWO4.
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Figure 1.4: Top panel: experimental and theoretical Mn L2,3 XAS
spectra of MnWO4 with the E vector of the light parallel to the a, b,
and c crystallographic axes. The spectrum of MnO is included as
reference. Bottom panels: a closeup revealing the polarization
dependence of the spectra. [1.23]
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1.2.4 Composite multiferroics (Two-phase systems)
The single-phase multiferroics are not very attractive because
none of the existing materials combine large and robust electric and
magnetic polarizations at room temperature. Composite
multiferroic materials with better design flexibility made by
combining ferroelectric and magnetic substances together in the
form of multilayers or self-organized nanostructures have drawn
significant interest in recent years due to their multifunctionality,
in which the coupling interaction between ferroelectric and
magnetic substances could produce a large ME response. In
composite multiferroics, each phase can be independently
optimized for room temperature performance. In general, two type
of ME coupling between ferroelectric and magnetic subsystems can
be expected: (i) owing to electronic effects at the interface, and (ii)
mediated by strain. This type of multiferroic materials can be
achieved in the form of composites laminates or epitaxial
multilayers. Zheng et al. and Ramesh et al. [1.25, 26] studied the
composite materials consisting of alternating ferroelectric and
ferromagnetic layers of nano-rods embedded in a matrix provide
strong ME coupling effect. Recently, ME properties of CoFe2O4 –
BaTiO3 [1.27] and NiFe2O4 – BaTiO3 [1.28, 29] heterostructures
studied by several groups. Table 1.2 lists some of the known
composite multiferroic materials adapted from Eerenstein et al.
[1.30].
1.2.4.1 Multiferroic CoFe2O4-BaTiO3 nanostructures
Zheng et al. used a different approach to produce multiferroic
thin films. They grew of alternating layers of the ferroelectric
material BaTiO3 and the ferro/ferrimagnetic material CoFe2O4 as
shown in Fig. 1.5 (A) and (B) and heterostructure consisting of
nanopillars of the ferro/ferrimagnetic phase embedded in a
ferroelectric matrix as shown in Fig. 1.5 (C) and (D). Such
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Table 1.2 Example of composite multiferroic materials
Morphology Materials Coupling constant
(mV.Cm-1Oe-1)
Composite BaTiO3 and CoFe2O4 50
Composite Terfenol-D and PZT in
polymer matrix
42
Laminated
composites
Terfenol-D and PZT in
polymer matrix/PZT in
polymer matrix
3000
Laminate Terfenol-D/PZT 4800
Laminate La0.7Sr0.3MnO3/PZT 60
Laminate NiFe2O4/PZT 1400
*PZT (Pb(Zr,Ti)O3) and BaTiO3 are piezoelectric, and terfenol-D
(TbxDy1-xFe2), the maganite and the ferrites are magnetostrictive.
nanostructures are deposited on (100) SrTiO3 (STO) substrates by
the pulsed laser deposition (PLD) technique from a single
0.65BaTiO3–0.35CoFe2O4 target. By using x-ray and electron
diffractions, they found that the films are epitaxial in the plane as
well as out of the plane, with self-assembled hexagonal arrays of
CoFe2O4 nanopillars embedded in a BaTiO3 matrix. In summary,
the CoFe2O4-BaTiO3 ferroelectromagnetic nanocomposite shows a
strong magnetoelectric coupling of the order parameters through
the heteroepitaxy of the two lattices.
1.2.4.2 Multiferroic NiFe2O4-BaTiO3 Heterostructure
Deng et al. [1.28] studied magnetic-electric properties of
epitaxial multiferroic NiFe2O4–BaTiO3 (NFO-BTO) heterostructure.
They found that NFO-BTO heterostructure show strong
ferroelectric and ferromagnetic responses simultaneously at room
temperature. Figures 1.6 (a) and (b) show good coexistence of
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Figure 1.5: (A) Superlattice of a spinel (top) and a perovskite
(middle) on a perovskite substrate (bottom). (B) Schematic
illustration of a multilayer structure on a substrate. (C) Epitaxial
alignment of a spinel (top left) and a perovskite (top right) on a
perovskite substrate (bottom). (D) Schematic illustration of a self
assembled nanostructured thin film formed on the substrate [1.25].
ferroelectric and ferromagnetic behaviors. The ferroelectric loops
show that the saturation polarization Ps and remanent polarization
Pr are about 29 and 10 μC/cm2, respectively. The ferromagnetic
hysteresis loops show that the saturation magnetization Ms is
about 80 emu/cm3. Figure 1.6 (c) show the magnetoelectric (ME)
response of the films. When an in-plane altering magnetic field
signal δH is applied, the single phase BTO and NFO films do not
produce any ME response, while the heterostructured NFO/BTO
film clearly yields the ME output following the magnetic
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Figure 1.6: (a) Ferroelectric hysteresis loops of the NFO/BTO
heterostructured film and the pure BTO film. (b) In-plane magnetic
hysteresis loops of the NFO/BTO film and the pure NFO film. (c)
The ME response of the films when the in-plane magnetic field is
applied. [1.28]
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excitation signal δH. In order to understand the microscopic origin
of the ME coupling at the BTO/NFO interfaces in the BTO/NFO
multilayer thin films, it is necessary to investigate the electronic
and magnetic properties of the Fe and Ni ions at the interfaces. In
the chapter 4, I have studied the origin of magnetoelectric coupling
in BaTiO3/NiFe2O4 heterostructures by XAS and x-ray magnetic
circular dichroism (XMCD).
1.3 Diluted magnetic semiconductors
Ferromagnetic semiconductors have been in the center of
much attention for more than a decade for research due to their
interesting physical properties and potentially useful spintronics
device. One aspect of spintronics of particular interest is the
creation and control of spin-polarized currents in semiconducting
material. The main idea is to combine conventional semiconductor
physics and magnetism to develop novel spin dependent
nanoelectronic devices including devices for quantum information
processing, which have been among the well established areas of
condensed matter physics. In dilute magnetic semiconductors
(DMSs), a fraction of the cations in the lattice are replaced
substitutionally by magnetic ions (Fig. 1.7) and are expected to
have both the properties of magnetic materials and semiconductors.
The coupling between the localized moments and delocalized
band-electrons renders unique properties of DMS, such as a giant
spin-splitting of electronic states and indirect ferromagnetic
exchange interactions between magnetic moments [1.31].
Semiconducting behavior in ferromagnetic material was first
uncovered by the discovery of the europium chalcogenides (EuO)
[1.32]. Eu-rich EuO shows ferromagnetic ordering while O-rich
EuO shows no metal-insulator transition (see Fig. 1.8). In 1986,
Story et al. [1.33] have reported that the alloy between the IV-VI
semiconductor and MnTe [(PbTe)1−x(SnTe)x]1−y[MnTe]y (y = 0.03)
25
shows ferromagnetic ordering when the hole carrier concentration
is above 1021 cm-3, as shown in Fig. 1.9.
Nonmagnetic semiconductor Magnetic semiconductor
Figure 1.7: (a) Semiconductor host doped with magnetic ions (b)
Magnetism in semiconductors: (Left) In normal, nonmagnetic
semiconductors, electronic energy does not depend on the spin
direction. (Right) In magnetic semiconductors, the d electrons of
magnetic ions influence the s and p electrons, and the conduction
band and valence band are split depending on the spin direction
(Zeeman splitting). [1.34]
(a)
(b)
26
Figure 1.8: Early reports on ferromagnetic semiconductors.
Conductivity of Eu-rich and O-rich EuO [1.32].
Figure 1.9: Carrier-concentration dependence of the ferromagnetic
Curie temperatures (TC) of PbSnMnTe [1.33].
Some of the reported DMS materials are summarized in Table
1.3. Most of the early dilute magnetic semiconductors such as
tellurides, selenides and sulfides were based on Mn-doped II-VI
semiconductors. The valence match (i.e. identical charge state) of
27
Table 1.3 Representative dilute magnetic semiconductors.
Material class Material Reference
II-VI p-Cd1-xMnxTe:N 1.40
II-VI p-Zn1-xMnxTe:N 1.38
II-VI Zn1-xCrxSe 1.41
II-VI Zn1-xCrxTe 1.42
II-VI Zn1-xCrxTe:I
Zn1-xCrxTe:N
1.43
IV-VI Pb1-x-ySnyMnxTe 1.44
III-V In1-xMnxAs 1.45
III-V Ga1-xMnxAs 1.46
III-V Ga1-xMnxN 1.47
IV Ge1-xMnx 1.48
Oxide Co-TiO2 1.49
Oxide Mn-ZnO 1.50
Oxide Cu-ZnO 1.51
Oxide Zn1-2xMnxCoxO 1.52
Oxide Co-SnO2 1.53
Oxide Fe-SnO2 1.54
Oxide Cr-In2O3 1.55
the cation of the II-VI host semiconductors to the dopant (Mn),
makes it easy to prepare samples with a large amount of Mn
[1.35-37]. The model materials (i.e. II-VI materials) in which
localized spins and delocalized holes can be introduced and
controlled independently, while dimensional effects can be tested
by using quantum heterostructures [1.38]. Sato and Katayama
Yoshida [1.39] employed first-principles calculation to investigate
ferromagnetism in both semiconductor and oxide spintronics. The
magnetic stability of transition metal-doped ZnO, ZnS, ZnSe, and
ZnTe was calculated using density functional theory (DFT) within
the framework of the local density approximation (LDA). The
28
random distribution of transitional metals impurity over the lattice
was inherently incorporated in the calculations by the coherent
potential approximation (CPA). Magnetic stability was calculated
by comparing the total energy difference between the ferromagnetic
and spin-glass state, the lower of the two representing the ground
state. In the case of Mn doped DMSs, the spin-glass state becomes
most stable while for V-, Cr-doped DMSs, the ferromagnetic states
are more stable than the spin-glass states.
Figure 1.10: Stability of the ferromagnetic states in (a) ZnO-, (b)
ZnS-, (c) ZnSe- and (d) ZnTe-based DMSs. V, Cr, Mn, Fe, Co or Ni is
doped as a magnetic impurity. The vertical axis is the energy
difference per one formula unit between the ferromagnetic state
and the spin-glass state. A positive energy difference indicates that
the ferromagnetic state is more stable than the spin-glass state
[1.39].
29
1.3.1 Transition metal doped CdTe
Galazkaet at el. [1.56] has investigated the magnetic
properties of Mn-doped CdTe single crystals, which could give rise
to paramagnetic, spinglass, and antiferromagnetic phase regions as
functions of temperature and Mn content. Compound or alloy doped
with two kind of transition element has rarely been studied.
Recently, Shen et al. [1.57] doped two transition metals in CdTe
crystal and studied the ferromagnetic behavior of Mn and Cr
co-doped CdTe bulk crystal. Figure 1.11 shows the magnetization
curve of Cr and Mn co-doped CdTe crystal. According to the
magnetic polaron model proposed by Shen et al. [1.57], a small
fraction of Cr atoms incorporated in (Cd,Mn)Te become Cr+ ions
acting as an acceptor and Mn spins are aligned by the holes
residing at this Cr+ acceptor level. The origin of ferromagnetism
and the interaction between Mn and Cr have not been clarified in
Shen et al. [1.57]. In chapter 5, I have studied the electronic
structure and magnetic properties of Mn- and Cr-doped CdTe by
x-ray magnetic circular dichroism, the element specific probe
technique.
Figure 1.11: SQUID magnetization for CdMnCrTe sample with 1%
Cr. Inset: field-cooled and zero-field-cooled temperature
dependences of remanent magnetization measured by SQUID.
[1.57]
30
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35
36
37
Chapter 2
Principles of x-ray magnetic
circular dichroism
X-ray magnetic circular dichroism (XMCD) technique is the
unique tool for an element-specific as well as a symmetry selective
probe of microscopic magnetic properties. XMCD is the difference
between left-handed and right-handed circularly polarized x-ray
absorption spectra (XAS). Nowadays, XAS is easy to measure at
synchrotron radiation facilities with excellent x-ray energy
resolution. This chapter is focusing on the principles of x-ray and
XMCD.
2.1 X-ray absorption spectroscopy
XAS and x-ray photoelectron spectroscopy (XPS) are the two
most widely used core electron spectroscopies. The measurements
of photo-absorption by excitation of a core-level electron into
unoccupied states as a function of photon energy is called x-ray
absorption spectroscopy. We can obtain information about the
valence states and the local environments surrounding each
elements by XAS spectra. The advantage of XAS technique is that it
can probe samples in a surface-sensitive (electron yield detection)
mode or bulk-sensitive (transmission) mode, which is of great
38
importance for artificially made multilayer structures. Figure 2.1
shows the principles of x-ray absorption spectroscopy, using a
one-electron model for the case of L edge absorption in a d band
transition metal. The absorption intensity from the initial state
can be calculated by summing all possible final states :
, (2.1)
where hν is the photon energy of the x-ray, T is the dipole
transition operator. The 2p core-level XAS spectra of transition
metal compounds well reflect the 3d electronic states in the 3d
transition-metal compounds including the symmetry and the
crystal field splitting of the 3d orbitals. Thole et al. [2.1] performed
the calculations of transition-metal 2p XAS spectra of 3d
transition-metal ions in a crystal field.
Figure 2.1: Principles of X-ray absorption spectroscopy, using a
one-electron model for the case of L edge absorption in a d band
transition metal. [2.2]
There are two measurement modes for XAS, the
transmission-mode and the total-yield mode. Transition mode is the
most direct measurement mode, in which the intensity of the x-ray
39
is measured before and after the sample and the ratio of the
transmitted x-rays is counted. Transmission-mode experiments are
standard for hard x-rays, though for soft x-rays, they are difficult to
perform because of the strong interaction of soft x-rays with the
sample. The total-yeild method can be classified in two modes, the
total-electron yield (TEY) and the total-fluorescence yield (TFY)
modes. TEY and TFY denote measuring the current flow and the
fluorescence of the sample radiated by x-ray, respectively. TEY
mode is surface sensitive while TFY mode is bulk sensitive and the
probing depth of TEY and TFY modes are ~5 nm and ~100 nm,
respectively. The TFY mode suffers from self-absorption effect
because of its long probing depth. In the present work, TEY and
TFY modes were employed.
2.2 X-ray magnetic circular dichroism
When the relativistic electrons in the storage ring are
deflected by the bending magnets that keep them in a closed
circular orbit, they emit highly intense beams of linearly polarized
x-rays in the plane of the electron orbit (bremsstrahlung). On the
other hand, they emit circularly or elliptically polarized light out of
the plane. Currently, a number of alternative sources for circularly
polarized synchrotron radiation are under development. The most
notable ones are so-called insertion devices like helical wigglers
[2.3] and crossed [2.4] undulators. Both wiggler and undulator are
complex arrays of magnets with which the electrons in a storage
ring are made to oscillate in two directions that are perpendicular
to their propagation direction, with the result that they emit
circularly polarized light.
Figure 2.2 shows schematic diagram of XMCD. Using
circularly polarized light in XAS, the absorption intensity depends
on the helicity of the incident light. When right- and left-handed
circularly-polarized x-rays are irradiated on a sample under applied
40
magnetic fields, differences in the absorption intensity are observed
because of differences of transition matrix elements (or selection
rule). XMCD is defined as the difference in the absorption spectra
when the helicity of the x-rays are parallel and antiparallel to the
magnetization direction of a material. XMCD is an element specific
measurement because of core-level excitation and is sensitive to
magnetically active components. The line shape of XMCD spectra
reflects electronic structure related to the magnetism. In addition,
by applying XMCD sum rules described below, one can estimate
spin and orbital magnetic moments separately from integrated
intensities of XAS and XMCD spectra. Therefore, XMCD is a
powerful tool to investigate magnetic properties of materials.
Figure 2.2 (c) shows the transition probability of 2p → 3d
absorption with circularly polarized x-rays. The transition
probability is proportional to
(2.2)
where is the Gaunt coefficient and mp and md are the
magnetic quantum numbers of the 2p and 3d states with md = mp+1
or md = mp-1. The circular polarization is expressed by , where
and have helicity 1 and -1, respectively. The selection rule is
derived from the equation. The selection rule of the transition
induced by circularly polarized light with helicity is change in the
magnetic quantum number by ±1 while the spin moment is
conserved. The final 2p hole is located at the 2p3/2 and 2p1/2 states,
and two absorption edges related to the 2p3/2 to 3d and 2p1/2 to 3d
transitions, called L3 and L2, respectively. The 2p3/2 and 2p1/2 have
four and two degenerated states, respectively. When we apply
magnetic field on the magnetic material, the final state d orbitals
are split according to the spin and are slightly affected by the
magnetic quantum number. Thus, the final state for both spin
directions can be classified as the states state. For 2p3/2
41
(c)
Figure 2.2: Schematic diagram of x-ray magnetic circular dichroism
(XMCD). (a) Experimental set up for XMCD measurements.
(b) Circularly polarized x-ray absorption spectra. (c) Transition
probability of 2p → 3d absorption with circularly polarized x rays
for less-than-half filled 3d electronic configuration.
42
and positive helicity, the transition probability ratios for each
are 18, 6 and 1. The transition probability ratios for 2p3/2
with opposite helicity are 3, 6 and 6 as shown in figure. Similarly,
the transition probability ratios for 2p1/2 with positive and negative
helicities are 3 and 2, and 3 and 12, respectively. The difference of
the transition probabilities between positive and negative helicities
provides the XMCD.
2.3 XMCD sum rules
XMCD reflects the spin and orbital polarization of local
electronic states. By using integrated intensity of the L2,3-edge XAS
and XMCD spectra of a transition-metal atom, one can separately
estimate the value of orbital and spin magnetic moments. Let us
consider 2p → 3d excitation as an example. Using representation of
hole number of the each 3d states hmd, the orbital and spin moments
are related to hmd as follows:
The relative transition intensity is proportional to product of the
transition matrix element and the hole number, and can be
calculated by using Fermi Golden Rule. Therefore, for less than half
filled 3d states, the difference in the 2p → 3d transition intensity
between the right-handed and left-handed circular polarizations
can be expressed for the for L3 and L2 edges as follows, respectively.
ΔIL3 ∝ 18h+2 + 6h+1 − 2h0 − 6h−1 − 6h−2, (2.5)
ΔIL2 ∝ 3h+1 + 2h0 − 3h−1 − 12h−2, (2.6)
Then, sum of the transition intensities is proportional to the orbital
moment as given below:
43
ΔIL3 + ΔIL3 ∝ 18h+2 + 9h+1 − 9h−1 − 18h−2,
∝ 9(2h+2 + h+1 − h−1 − 2h−2),
∝
∝
As well as the orbital moment, one can estimate the spin moment
from the transition matrix element of circularly polarized x-rays.
Thole et al. [2.5] and Carra et al. [2.6] have derived formulae to
calculate the spin and orbital magnetic moments of the atoms from
the XMCD spectra. For the 2p-3d XMCD analysis, the formulae of
the spin and orbital magnetic moments are given by
(2.8)
where μ+ and μ- are the absorption intensities for the positive- and
negative polarizations, respectively, and Nd is the number of
electrons in the 3d band. MT is the magnetic dipole moment, which
can be neglected in the case of perovskite-type oxide with cubic
symmetry [2.7, 8]. The orbital magnetic moment (Morb) and the spin
magnetic moment (Mspin) both are in units of μB/atom, where μB is
the Bohr magneton.
2.4 Configuration-interaction cluster model
In order to consider the correlation between electrons, we
consider the hybridization between the Slater determinants instead
of a single Slater determinant. The hybridization between the
Slater determinants leads to so called configuration interaction (CI).
In this thesis, core-level and valence-band spectra will be analyzed
using CI calculation. The CI cluster-model analysis has been a
44
useful framework for understanding the electronic structure of
magnetic materials [2.9-11]. According to Tanaka and Jo [2.12], the
Hamiltonian of the cluster is assumed to be
H = H1 + H2 (2.9)
where H1 is the non-multiplet term which describes the valence and
core states and the effective interaction between electrons, which is
adopted from the early stages of analysis of PES and XAS data
[2.13], given by
where denotes the transition metal 3d symmetry group in the
crystal field, e.g., t2g and eg representation in the octahedral (Oh)
configuration, denotes the basis of each representation, and
stands for the orbital and spin state of the core orbit. The energy
difference between the t2g and eg is given by 10Dq for the 3d orbit.
The first, second, third, fourth, fifth and sixth term in equation
(2.10) denote the energy of the 3d orbit of the TM ion, of the ligand
molecular orbit, the core orbit, the effective 3d-3d interaction, the
attractive core hole potential acting on the 3d electron and the
hybridization between the ligand and 3d orbit, respectively. The
charge transfer energy is defined as ∆ = , where
and are the average energies of and
configuration, respectively. Here, denotes a hole in the ligand p
orbitals in the cluster.
45
H2 describes the full-multiplet 3d-3d (Hdd) and 3d-core
interaction (Hdc) is given by
(2.11)
is the spin-orbit interaction in the 3d state with the coupling
constant and is the spin-orbit interaction in core
state.
The wave function of the ground state ψg for N-electron state,
is spanned by linear combinations of charge transfer state as given
by
(2.12)
The final state wave functions of transition-metal 2p core-level ψc
and transition-metal 3d valence-band ψv are also spanned by linear
combinations of charge transfer state as,
(2.13)
(2.14)
where c and L denotes holes in the transition-metal 2p core level
and ligand p orbitals, respectively, and n is the number of d
electrons for the ground state of the transition metal. The
charge-transfer energy for anion-to-3d orbital is defined by Δ≡
E(dn+1)−E(dn), and the 3d-3d Coulomb interaction energy is defined
by U≡E(dn+1)+E(dn-1) − 2E(dn). It is also possible to define the
charge-transfer energy Δeff and the Coulomb interaction energy Ueff
with the lowest term of each multiplet. The multiplet splitting is
expressed using Racah parameters A, B, and C or Kanamori
parameters u, u’, j, and j’ for the multiplet splitting of the dn
configuration due to intra-atomic Coulomb and exchange
46
interactions. There is relationship between these four parameters;
u’=u−2j, j’=j. The charge-transfer energy Δ and Coulomb energy
U as well as the Slater-Koster parameters are adjustable
parameters in the cluster-model calculation.
The Slater parameters which describe the d electrons and the
2p electrons of created the core hole and the spin-orbit coupling
parameter for the d and for the 2p states are also used in the
cluster model calculation. The Slater parameters and the spin-orbit
coupling can be obtained from Hartree-Fock calculations [2.14, 15].
The tetrahedral and octahedral symmetry are shown in figure 2.3.
For Td crystal field symmetry, transfer integrals T(Γi) between the
3d orbitals and ligand p orbitals are given by Slater-Koster
parameters (pdσ) and (pdπ) as
(2.15)
(2.16)
Figure 2.3: Octahedral (a) and tetrahedral (b) crystal symmetry
47
In the case of the Oh crystal field symmetry, one electron transfer
integrals T(Γi) between the 3d orbitals and the anion ligand orbitals
can be expressed in terms of the Slater-Koster parameters (pdσ)
and (pdπ) as follows:
(2.17)
(2.18)
To perform cluster model calculation, I used the program Xtls
8.5 developed by Prof. A. Tanaka. First I set the electronic
configurations of the transition metal ion. In chapter 6, I have
employed three charge-transfer states such as 2p63d5, 2p63d6L, and
2p63d7L2, where, denotes a hole in the ligand p orbitals. Thus the
initial state is expanded by a linear combination of these three
states and the final state is described by a linear combination of
2p53d6, 2p53d7L, and 2p53d8L2.
There are five important adjustable parameters which are
also used to perform the cluster model calculation: the
charge-transfer energy (∆), the Coulomb interaction energy (Udd)
between the 3d electrons, the Coulomb attraction energy (Udc)
between the 2p core hole and 3d electron, the hybridization energy
(Veg) and the crystal field splitting (10Dq).
48
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51
Chapter 3
Experimental Details
One of the most powerful techniques to investigate the
magnetism of magnetic materials is x-ray magnetic circular
dichroism (XMCD). This technique requires circular polarized
x-rays and variation of photon energy which are only fulfilled by
synchrotron radiation at synchrotron facility. Synchrotron
radiation is very popular for scientific applications because it is
available in a large photon energy range and useful for a wide
range of physical, chemical, and biological experiments. The
experiments of the present work were carried out at synchrotron
facilities. We have performed the XAS and XMCD measurements at
beamlines BL-11A (Dragon beamline) of National Synchrotron
Radiation Research Center (NSRRC), Taiwan, BL-16A2 of Photon
Factory (PF), High Energy Accelerator Research Organization
(KEK) and BL-23SU of SPring-8. This chapter describes details of
the experiments.
3.1 NSRRC BL-11A
A Dragon beamline 11A at National Synchrotron Radiation
Research Center (NSRRC) has been designed for x-ray absorption
spectroscopy (XAS), x-ray photoelectron spectroscopy (XPS),
magnetic circular dichroism (MCD) spectroscopy, and magnetic
52
linear dichroism (MLD) spectroscopy. Figure 3.1 shows the
schematic diagram of beamline 11A. The light source is a bending
magnet. There are two mirrors close to each other, the one closest to
the source is the horizontal focusing mirror (HFM), and the other is
the vertical focusing mirror (VFM). Both are spherical mirrors. The
top view shows the HFM focusing the source inside the storage ring,
and the side view shows the VFM focusing the source into the
entrance slit. The optical function of these two mirrors is decoupled.
The advantage of decoupled VFM and HFM is that one can
visualize the possibility of adjusting these two elements to
compensate the drift in the position of the source inside the storage
ring. After the entrance slit there is grating (6m-SGM) which
diffracts and focuses the photon beam vertically into the exit slit.
The exit slit is movable to achieve high resolving power. The
monochromatic light was reflected by toroidal refocusing mirror
(RFM), and introduced to the end station. Two vertical plane
mirrors (VPM) between the gratings and the exit slit to extend the
lowest photon energy to 10 eV. In this beamline, six spherical
gratings are used to cover an energy range from 10 eV to 1700 eV.
In practical measurements, the photon energy was scanned using a
grating which have 1200 lines/mm and covers the photon energy
range 400 − 1200 eV. Photon flux is 1×1010 with the energy
resolution E / ΔE = 10,000. The measurement chamber is located at
the end station of the beamline as shown in Fig. 3.1. The chamber
for XMCD measurements is equipped with an electromagnet with a
water-cooling system and magnetic field up to H = 1 T can be
achieved. The angle between the beam axis and the magnetic field
is 30o. The sample holder can be rotated freely around the vertical
axis by using differentially pumped rotary feedthrough (DPRF).
Both the total electron yield (TEY) and total fluorescence yield
(TFY) measurement modes can be performed. Figure 3.2 (a) show
the experimental geometry of XMCD measurements. For different
elements the resonant energy is different as shown in Fig. 3.2 (b).
53
Figure 3.1: Measurement system in BL-11A. (a) Schematic layout of
beamline [3.1, 2]. (b) Overview of the measurement system at
BL-11A. (c) Data acquisition system.
54
Figure 3.2: (a) Experimental geometry of XMCD measurements.
(b) L2,3-edge XAS of Fe, Co, Ni, and Cu transition metals measured
at BL 11A, NSRRC [3.3].
55
3.2 KEK-Photon Factory BL-16A
The beamline BL-16A at the Photon Factory (PF) has been
designed for XMCD, photoemission spectroscopy (PES), and
resonance-soft x-ray scattering measurements. Figure 3.3 shows
the schematic diagram of beamline BL-16. The light source is a
double-array variable polarization undulator of APPLE-II type. The
variation of the phase between the two magnet arrays leads to
change of the polarization of the light. It can generate horizontally
and vertically linear, left- and right-handed circularly-polarized
light. This undulator covers photon energies ranging from hν = 300
eV to 1000 eV in the circular polarization mode by the first
harmonic radiation. The photon energy was scanned using a
varied-line-spacing plane grating (VLSPG) grazing-incidence
monochromator (600 lines/mm) [3.5]. This type of monochromator is
very popular because of its high resolution, high throughput, simple
scanning mechanism and fixed exit slit. The photon flux is better
than 1 × 1011 photons/sec with energy resolution E / ∆E = 8,000. The
degree of circular Pc was evaluated to be Pc = ± 95% ± 4% on BL-16A
of the Photon Factory. The XMCD chamber for measurements [3.7]
is equipped with a superconducting magnet with a coil made of a
NbTi wire, and magnetic field up to H = 5.8 T can be achieved. The
superconducting magnet is designed so that it can be baked to
reach a vacuum as good as ~10–10 Torr. He-gas-flow cryostat is used
to cool the sample and the achievable lowest sample temperature is
5 K. Using a differentially pumped rotary feedthrough (DPRF), the
angle between the sample normal and the magnetic field θ can be
varied in the range of 0o ≤ θ ≤ 60o. Figure 3.4 (a) shows the
experimental geometry of the x-ray magnetic circular dichroism
(XMCD) measurements and the XAS and XMCD spectra measured
at BL 16A are shown in Fig. 3.4 (b). The typical XAS and XMCD
spectra obtained for a Fe/Ni/Cu multilayer, indicating magnetism
56
observed in the top thin Fe layer consisting of only 0.9 times of a
monolayer.
Figure 3.3: Measurement system at BL-16A of Photon Factory.
(a) Schematic layout of the beamline [3.4]. (b) Overview of the
XMCD measurement chamber. (c) Controller of BL-16A2 station.
57
Figure 3.4 (a) Experimental geometry of the x-ray magnetic circular
dichroism (XMCD) measurements [3.6]. (b) Fe L2,3-edge XAS and
XMCD spectra for an Fe(0.9 ML)/Ni(6 ML)/Cu(100 ML) film
measured at BL 16, KEK-PF [3.4].
58
3.3 SPring-8 BL23SU
The beamline BL-23SU at SPring-8 is designed for a wide
variety of scientific research areas such as spectroscopic studies on
actinide compounds, semiconductor surfaces, and biological
materials, etc., in the soft x-ray region [3.8 – 10]. The name of
“SPring-8” comes from Super Photon ring for 8 GeV. A schematic
diagram of the beamline is shown in Fig. 3.5. The light source is a
double-array variable undulator of APPLE-II (advanced planar
polarized light emitter) type. The variation of the phase between
the two magnet arrays leads to change of the polarization of the
light. It generates horizontally and vertically linear, left- and
right-handed circular polarized light. This undulator covers photon
energy range of hν = 500 eV to 3000 eV in the circular polarization
mode. Furthermore, it is possible to switch the direction of circular
polarization periodically at each photon energy [3.11]. This enables
us to measure the XMCD spectra much more precisely than the
conventional measurement mode with fixed polarization. The
photon energy was scanned using a varied-line-spacing plane
grating (VLSPG) grazing-incidence monochromator (600 lines/mm).
This consists of an entrance slit, spherical mirrors,
varied-line-spacing plane gratings, an exit slit, a post-focusing
mirror, and refocusing toroidal mirrors. The photon flux is better
than 1 × 1011 with the energy resolution E /∆E = 10,000. The PES
station and the XAS-MCD station are located at the end station
ST3 shown in Fig. 3.5. At each station, preparation chamber for
sample surface cleaning was connected to the measurement
chamber to enable transfer without breaking the ultra-high
vacuum. In PES measurements, photoelectrons were corrected by a
commercial Scienta SES-2002 analyzer.
59
Figure 3.5: Measurement system in BL-23SU. (a) Schematic layout
of beamline [3.9]. (b) Overview of the measurement system at
BL-23SU [3.12]. (c) Experimental geometry of XMCD
measurements [3.6].
60
References
[3.1]http://140.110.203.42/manage/fck_fileimage/file/bldoc/11ADRA
SGM.htm
[3.2] NSRRC Activity Report 2002/2003,
http://140.110.201.35/djhuang/download/research/XAS_1.pdf
[3.3] http://140.110.201.35/djhuang/research_xas.html
[3.4] KEK annual report 2008, Vol. 1, page 24,
http://ccdb5fs.kek.jp/tiff/2008/0822/0822001.pdf
[3.5] K. Amemiya and T. Ohta, J. Synchrotron Rad. 11, 171 (2004).
[3.6] T. Kataoka, Doctor thesis (2010).
[3.7] T. Koide, T. Shidara, and H. Fukutani, Rev. Sci. Instrum. 63,
1462 (1992).
[3.8] A. Yokoya, T. Sekiguchi, Y. Saitoh, T. Okane, T. Nakatani, T.
Shimada, H. Kobayashi, M. Takao, Y. Teraoka, Y. Hayashi, S.
Sasaki, Y. Miyahira, T. Harami, and T. A. Sasaki, J. Synchrotron
Rad. 5, 10 (1998).
[3.9] Y. Saitoh, T. Nakatani, T. Matsushita, A. Agui, A. Yoshigoe, Y.
Teraoka, and A. Yokoya, Nucl. Inst. Meth. A 474, 253 (2001).
[3.10] J. Okamoto, K. Mamiya, S.-I. Fujimori, T. Okane, Y. Saitoh,
Y. Muramatsu, A. Fujimori, S. Ishikawa, and M. Takano, AIP Conf.
Proc. 705, 1110 (2004).
[3.11] A. Agui, A. Yoshigoe, T. Nakatani, T. Matsuhisa, Y. Saitoh, A.
Yokoya, H. Tanaka, Y. Miyahara, T. Shimada, M. Takeuchi, T.
Bizen, S. Sasaki, M. Takao, H. Aoyagi, T. P. Kudo, K. Satoh, S. Wu,
Y. Hiramatsu, and H. Ohkuma, Rev. Sci. Instrum. 72, 3191 (2001).
61
[3.12]http://www.spring8.or.jp/wkg/BL23SU/instrument/lang-en/IN
S-0000000367/instrument_summary_view
62
63
Chapter 4
Origin of enhanced
magnetoelectric coupling in
BaTiO3/NiFe2O4 multilayers
studied by x-ray magnetic
circular dichroism
NiFe2O4 (NFO)/BaTiO3 (BTO) multilayer heterostructures
grown on (001)-SrTiO3 substrates with alternating ferroelectric
BTO and ferrimagnetic NFO layers exhibit magnetoelectric
coupling which increases with the number of layers, namely, with
the number of interfaces. I have studied the local electronic and
magnetic states of Ni and Fe ions in the NFO/BTO multilayers with
various NFO and BTO thicknesses by x-ray absorption
spectroscopy (XAS) and x-ray magnetic circular dichroism (XMCD)
at room temperature. The measured Ni 2p and Fe 2p spectra
indicate that Ni ions are octahedrally coordinated by oxygen and
that are divalent (Ni2+) and Fe ions are trivalent (Fe3+) and are
tetrahedrally and octahedrally coordinated by oxygen with opposite
spin direction, consistent with the inverse spinel structure of
NiFe2O4. With increasing number of layers, both Ni and Fe
magnetic moment decrease. With decreasing NFO layer thickness,
64
the average magnetic moment of Ni ions decreases while the
average magnetic moment of Fe ions remain unaffected. I found
good correlation between magnetoelectric coupling per interface
(αE/n) and Fe XMCD which means that the Fe magnetic moment at
the interface governs the ME coupling. Specifically, the charge
transfer between the hybridized Fe-TiO2 bonding at the interface
contributes to the density of the trapped electrons, which could
favour the enhancement of the ME coupling.
4.1 Introduction
Multiferroic materials, a class of materials which exhibit
ferroelectric, ferromagnetic, and/or ferroelastic properties
simultaneously have drawn increasing interest due to their
significant potentials for applications as next-generation
multifunctional devices [4.1-4]. If there is magnetoelectric (ME)
coupling in multiferroic materials, by applying an external
magnetic field, the materials will produce electric polarization,
while an external electric field will induce magnetization. ME
coupling in single-phase compounds is, however, generally weak.
On the other hand, it has been demonstrated that Composite
materials consisting of alternating ferroelectric and ferromagnetic
layers [4.5] or ferromagnetic nano-rods embedded in a ferroelectric
matrix [4.6, 7] provide strong ME coupling.
Recently, thin films consisting of alternating NiFe2O4 (NFO)
and the ferroelectric perovskite-type BaTiO3 (BTO) layers
BTO/(NFO/BTO)n were prepared and exhibited the coexistence of
ferroelectric and ferromagnetic ordering with strong ME coupling
between them [4.8, 9]. It was found that the magnetic moment
decreases and ME coupling increases with increasing number of
layers n for a fix total thickness of the sample, and both
observations were attributed to the interfaces since the relative
contributions of the interfaces increases with n. Here, BTO is a well
known ferroelectric oxide. Structural compatibility of perovskites
65
with various magnetic oxides such as those with the spinel
structures allows one to combine thin layers of ferroelectric and
magnetic materials to design multifunctional heterostructures.
NFO is one of the well known inverse spinel-structure oxides,
represented by Fe3+[Ni2+Fe3+]O4. Half of the Fe3+ ions occupy the
tetrahedral sites while Ni2+ ions and the other half of the Fe3+ ions
occupy the octahedral sites. Similar to the Fe ions between the
tetrahedral and octahedral sites in Fe3O4, the Ni2+ and Fe3+ ions at
the tetrahedral sites are coupled antiferromagnetically through
superexchange interaction via oxygen ions as the
Kanamori-Goodenough (KG) rule predicts [4.10, 11].
In order to understand the microscopic origin of the ME
coupling at the BTO/NFO interfaces in the BTO/NFO multilayer
thin films, it is necessary to investigate the electronic and magnetic
properties of the Fe and Ni ions at the interfaces. For that purpose,
X-ray absorption spectroscopy (XAS) and x-ray magnetic circular
dichroism (XMCD) are ideal techniques because they are element
specific probes of the electronic and magnetic properties of
transition-metal ions [4.12]. I have studied the electronic and
magnetic states of the Fe and Ni ions in samples with various BTO
and NFO layer thicknesses. I have found that interfacial Ni atoms
lose ferromagnetic moment while the Fe magnetic moments remain
unaffected at the interface and the loss of the Ni ferromagnetic
moment is well correlated with the enhancement of ME coupling in
the NFO/BTO multilayers. I discuss possible scenarios which lead
to an interfacial structure having both weakened Ni ferromagnetic
moment and strong ME coupling simultaneously.
4.2 Experimental
In this study, two sets of BTO/(NFO/BTO)n (n=1, 2, 3, 4)
heterostructures were prepared on (001)-oriented 0.7% Nb-doped
SrTiO3 (STO) single crystal substrates by using the pulsed laser
66
deposition technique. The structures of the samples are shown in
Fig. 4.1. The total thicknesses of these films were kept about 120
nm. I prepared two sets of samples. In set 1, the volume ratios of
BTO to NFO in the films are kept 4:1 while in set 2, the thicknesses
of the NFO and BTO layers were the same and therefore the
thickness ratio of BTO to NFO varies between samples.
The XAS and XMCD measurements were carried out at the
Dragon monochrometer beamline 11A of National Synchrotron
Radiation Research Center (NSRRC), Taiwan. XAS and XMCD
spectra were collected in the total-fluorescence yield (TFY) mode by
using a photodiode. The probing depth of the fluorescence yield
detection is about 100 nm. The direction of the applied magnetic
field was reversed to obtain XMCD spectra. XAS spectra for
positive and negative magnetic fields μ± with fixed photon helicity
were taken, and XAS and XMCD spectra were obtained by taking
the sum and the difference between μ+ and μ-, respectively. The
samples were positioned with the plane parallel to the magnetic
field. All the measurements were performed at room temperature
with magnetic fields up to 1 T.
FIG. 4.1: Sample structures of BTO/(NFO/BTO)n heterostructures
of sets 1 and 2.
67
4.3 Results and discussion
In Fig. 4.2, the XAS and XMCD spectra of the Ni 2p core level
are shown and compared with reference data. Each absorption
spectrum of Ni shows two groups, the L3 (2p3/2) and L2 (2p1/2) edges,
separated by the spin-orbit splitting of the 2p core level of ~17 eV.
The double peak structure at the L3 edge and a partially resolved
doublet structure at the L2 edge are the characteristic features of
the high-spin (S=1) Ni2+ ion in the octahedral crystal field [4.13, 14].
In panel (a), the Ni 2p XAS spectrum measured for the
BTO/NFO/BTO sample is compared with the reference data of Ni
metal [4.15], PrNiO3 (Ni3+) [4.16], NiO (Ni2+) [4.17], and a
calculated spectrum of Ni2+ in an octahedral crystal field. The Ni 2p
XAS spectrum of BTO/NFO/BTO is different from those of Ni metal
and PrNiO3 and similar to the spectra of NiO and calculated Ni2+ in
an octahedral crystal field, indicating that the valance of Ni in
BTO/NFO/BTO is 2+ like Ni in NiO. Similarly, as shown in Fig. 2
(b), the Ni 2p XMCD of BTO/NFO/BTO is different from that of Ni
metal and well agrees with the calculated XMCD spectrum of Ni2+
in the octahedral crystal field, indicating that the ionic Ni atoms
with localized 3d electrons contribute to the magnetism in this
sample.
Figure 4.3 shows the Fe 2p XAS and XMCD spectra of the
BTO/(NFO/BTO)1 films. The core–level spin–orbit coupling splits
the XAS into the L3 (2p3/2) and L2 (2p1/2) edges. In Fig. 3(a), the Fe
2p XAS spectrum of the BTO/NFO/BTO is compared with the XAS
spectra of Fe metal [4.18], GaFeO3 [4.19], γ-Fe2O3 [4.20] and
calculated Fe3+ in Oh and Td crystal field. The peak position of Fe3+
is similar to the calculated Fe3+ in Oh and Td peak position. The Fe
valance state in γ-Fe2O3, GaFeO3, and BTO/(NFO/BTO)1 are all
trivalent but the Fe ions are located at sites of different local
symmetries. The line shape of the Fe 2p XAS spectrum of
BTO/NFO/BTO is rather similar to both γ-Fe2O3 and GaFeO3 but is
68
FIG. 4.2: Comparison of the Ni 2p XAS (a) and XMCD (b) spectra of
BTO/NFO/BTO with those of Ni metal [4.15], PrNiO3 (Ni3+) [4.16],
NiO (Ni2+) [4.17], and calculated Ni2+ in octahedral crystal field.
69
FIG. 4.3: Comparison of the Fe 2p XAS (a) and XMCD (b) spectra of
BTO/NFO/BTO with those of Fe metal [4.18], GaFeO3 [4.19],
γ-Fe2O3 [4.20] and calculated Fe3+ in Oh and Td crystal field.
70
quite different from that of Fe metal, indicating that the valence of
the Fe ions in BTO/(NFO/BTO) are in 3+. The difference of the XAS
of BTO/NFO/BTO from those of γ-Fe2O3 and GaFeO3 is the lower
intensities of structures A and C in BTO/NFO/BTO. Because peaks
A and C are due to Fe3+ ions at the octahedral (Oh) sites and peak B
to those at the tetrahedral (Td) site, weaker A and C mean that the
number of Fe3+ at the octahedral positions is smaller. This
corresponds to the facts that the octahedral to tetrahedral ratio
decreases from 5/3 in γ-Fe2O3 to 1 in NiFe2O4, and that all Fe3+ go to
the octahedral sites in GaFeO3. The Fe 2p3/2 XMCD spectra of the
BTO/NFO/BTO samples show three sharp negative, positive, and
negative peaks at hν =708.15, 709.30, and 710.25 eV, denoted by A,
B, and C, respectively, corresponding to the directions of the spins
of the Fe3+ ions at the tetrahedral and octahedral sites which are
coupled antiferromagnetically in NFO. The negative peaks A and C
come from the Fe3+ ions at the octahedral sites and the positive
peak B comes from the Fe3+ ions at the tetrahedral sites. The
XMCD spectrum is also compared with those of γ-Fe2O3, GaFeO3
and Fe metal. The XMCD spectral line shape of the BTO/NFO/BTO
sample is clearly different from that of Fe metal. The positive peak
B due to Fe3+ at the Td sites is absent in GaFeO3 because all the
Fe3+ ions occupy only the octahedral sites in GaFeO3. The peak
positions of A, B, and C coincide with those of γ-Fe2O3 and indicate
that Fe3+ ions are both at the Td and Oh sites. γ-Fe2O3 has the spinel
structure with Fe (Oh) vacancies represented by Fe3+[□1/3Fe3+5/3]O4,
in which the ratio of the octahedral Fe3+ to the tetrahedral Fe3+ is
5/3. NiFe2O4 is represented by Fe3+[Ni2+Fe3+]O4 and the ratio of
octahedral Fe3+ to tetrahedral Fe3+ is 1. Peak C is weaker in NFO
because of the smaller Fe3+(Oh) to Fe3+(Td) ratio than γ-Fe2O3.
Figures 4.4(a) and 4(b) show the Fe 2p and Ni 2p XMCD
spectra of the BTO/NFO/BTO thin film of set 1 measured at various
magnetic fields. Figures 4.4(c) and 4.4(d) show the Fe 2p XMCD
intensity of Oh and Td and comparison of the Ni 2p XMCD intensity
71
FIG. 4.4: Magnetic field dependence of the Ni 2p (a) and Fe (b) 2p
XMCD spectra of the BTO/NFO/BTO thin films of set 1, and
comparison of the SQUID results with the Ni 2p XMCD intensity of
Oh (c), and Fe 2p XMCD Intensity of Td and Oh of BTO/NFO/BTO
(d) of set 1.
with the magnetization measured using a superconducting
quantum interference device (SQUID) magnetometer of the
BTO/NFO/BTO sample of set 1, respectively. Because Ni2+ (Oh) and
Fe3+ (Oh) are antiferromagnetically coupled with Fe3+ (Td), the
difference in the total magnetic moments at the Oh and Td sites
would give rise to ferrimagnetism. In NFO, the magnetic moments
of the Ni2+ ions at the Oh sites are responsible for the macroscopic
net magnetization because the magnetic moments of the Fe3+ ions
at the Td and Oh sites cancel out macroscopically. The Ni 2p XMCD
72
intensities follow the magnetization result. The magnetic field
dependence of XMCD spectra of the BTO/(NFO/BTO)n
heterostructures clearly show ferromagnetism at room
temperature.
Figure 4.5 shows how the XMCD spectra change between the
different samples with different numbers and thicknesses of NFO
and BTO layers. The XMCD spectra of set 1 at the Fe and Ni L2,3
edges of various n’s are shown in Figs. 4.5(a) and 4.5(b). The XMCD
intensity of the Fe and Ni L2, 3 edges decreases with increasing
number of NFO and BTO layers as shown in Figs. 4.5(c) and 4.5(d).
FIG. 4.5: Ni 2p (a) and Fe 2p (b) XMCD spectra of BTO/(NFO/BTO)n
thin films (where n=1, 2, 3) of set 1, and the Ni (c) and Fe (d) 2p
XMCD intensities versus the number of layers of BTO/(NFO/BTO)n
thin films of sets 1 and 2.
73
This observation means that, as we increase the interface-volume
ratio of the NFO layers, the magnetization decreases, which implies
the degradation of the ferromagnetic order at the interfaces. By
changing the layer numbers, not only the interfaces but also the
strain from the BTO layer may influence the magnetization of NFO
because the NFO layers would be in a highly compressively
strained state due to the lattice mismatch between NFO and BTO
layers. Liu et al. [4.9] showed that when the number of layers
increases, the c parameter of NFO increases, which means that the
compressive strain within the ab plane in NFO layers increases. I
also obtained a similar trend of decreasing magnetization in set 2 of
BTO/(NFO/BTO)n multilayer thin films but, set 1 and set 2 behave
differently as functions of the layer (interface) number, which
indeed indicates that the strain itself affects the magnetization in a
complicated way.
In order to see how the Fe and Ni magnetizations are
affected by the number of interface and the NFO thickness, I have
plotted the XMCD intensities of Fe and Ni against NFO thickness
(x-axis) and number of layers (y-axis) in Figs. 4.6 with appropriate
interpolation and extrapolation. In the x-axis (NFO thickness)
direction, the NFO layer thickness increases and the volume ratio
of the interface in the NFO layer decreases. In the y-axis direction,
the number of layers increase which means that number of
interfaces between layers increase. Both Ni and Fe 2p XMCD
intensity decreases with the number of layers because the NFO
layer suffered by compressive strain due to the residual stress
originating from the lattice mismatch and different thermal
expansion coefficients between the NFO and BTO layers. The Fe 2p
XMCD intensity was found to be independent of the NFO thickness
while Ni 2p XMCD intensity depends on the NFO thickness. The Ni
ion is responsible for the net magnetization in the multilayered
films. The gradual reduction in the magnetization of Ni in
BTO/NFO/BTO with decreasing NFO thickness could be
74
understood by considering the negative magnetostriction of NFO
that it contracts when magnetized. The independency of Fe XMCD
intensity on NFO thickness is still unknown. The possible reason
may be that the some of Ni is replaced by Fe with decreasing NFO
thickness and Fe XMCD intensity remains constant (or little
increase) while Ni XMCD intensity decreases. The magnitude of
magnetostriction constant of Fe3O4 (–19×10–6) [4.21] is less than
NiFe2O4 (–45×10–6) [4.22] means that Fe ions less contract in Fe3O4
than Ni ions in NFO when it magnetized. With decreasing NFO
thickness, some of Ni ion in NFO is replaced by Fe and the
magnitude of magnetostriction coefficient reduces, may be the
possible reason of independent of Fe magnetization on NFO
thickness.
As for ME coupling, single-phase films of NFO and BTO
have no obvious ME output but the heterostructure consisting of
NFO and BTO layer clearly yields ME output [4.9]. The interface
therefore should play a crucial role in inducing the ME coupling.
The ME coupling constant increase as the interface density and
number of interface in the heterostructure increases as shown in
Fig. 4.6 (d). Here, the ME voltage coefficient αE is defined by
δV/(δHt), where δV is the induced voltage signal and t is the total
film thickness. From Fig. 4.6 (b) and (d), it is clear that ME
coupling increases with the decrease of Ni ferromagnetism at the
interface. The Ni ferromagnetism is degraded at the interface but
does not degrade the ME coupling. αE/n is a ME coupling constant
per interface and plotted against NFO thickness and number of
layers as shown in Fig. 4.6 (e). I found good correlation between αE/n
and Fe XMCD which means that the Fe magnetic moment at the
interface governs the ME coupling. Recently, microscopic
mechanism of ME coupling at the Fe/BTO interface was studied by
the element specific x-ray magnetic scattering and Ti atoms at the
interface were found to have finite spin polarization [4.23]. The
details about the nature of the ME coupling in the NFO/BTO
75
FIG. 4.6: Fe (Td) (a) Ni (Oh) (b) Fe (Oh) (c) 2p XMCD intensity, ME
coupling coefficient αE (d) and ME coupling coefficient per interface
αE/n (d) plotted against the NFO thickness and the No. of layers.
76
heterostructures are currently unknown, but we may speculate
that strong ME coupling occurs at interfacial defects where Ni
atoms are replaced by Fe atoms and Fe and Ti atoms are located
close to each other at the interface. The Ti and O atoms in the
ferroelectric BTO are sensitive to ferroelectric displacements and
the magnitude of ME coupling constant depends on the interface
termination. The Fe-TiO2 bonding at the interface creates oxygen
vacancies. The oxygen vacancies at the interface may play an
important role in ferroelectric displacement and hence determining
the strength of the ME coupling. In addition, the charge transfer
between the hybridized Fe-TiO2 bonding may possibly contribute to
the density of the trapped electrons, which could favour the
enhancement of the electric polarization by aligning the defect
dipoles and the dynamic exchange interaction of trapped electrons
in the ordered polarons derives the enhancement of the FM. To
improve the ME coupling of the device, to increase the number of
interfaces is important. With increasing n, αE/n decreases rather
than increases. This is probably because the distance between NFO
layers become too short and the surface anisotropy at the interface
increases. Thus, the surface anisotropy contribution increasingly
dominates over the ME contribution and ME coupling decreases.
Finally, with persistently growing demand for strong ME
composites, these materials offer a potential usage as building
blocks for multiferroic materials and can be exploited in
multifunctional devices such as tunable phase shifters, ME sensors,
and resonators. The fast growing research to increase ME coupling
in multiferroic compounds will ultimately tell us much more about
the usefulness of these amazing multiferroic materials. We need
more careful treatment to prepare samples and further
investigations remain in need of investigation for understanding
and designing the ME coupling.
77
4.4 Conclusions
Multilayered heterostructures, BTO/(NFO/BTO)n epitaxially
grown on (001)-STO substrates via pulsed laser deposition
technique were studied by XAS and XMCD. The Ni ions are in the
2+ states at the Oh position while Fe ions are in the 3+ states at Oh
and Td positions. The ferromagnetic moment of Ni2+ is parallel to
Fe3+(Oh) but are antiparallel to Fe3+(Td) following the inverse spinel
structure of NiFe2O4, but the Ni moment is found to decrease at the
interface. With decreasing NFO thickness, some of Ni ion in NFO is
replaced by Fe and the magnitude of magnetostriction coefficient
reduces may be the possible reason of the degradation of Ni
moment. I found clear correlation between the ME coupling
strength and the ferromagnetic moment of Fe. This suggests that
the enhancement of ME coupling occurs at interfacial Fe-TiO2
bonding. The Fe-TiO2 bonding creates oxygen vacancies and the
oxygen vacancies at the interface and the charge transfer between
the hybridized Fe-TiO2 bonding contributes to the density of the
trapped electrons which may play an important role to enhance the
ME coupling.
78
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80
81
Chapter 5
Cr-doping induced
ferromagnetism in the
antiferromagnetic spin glass
Cd1-xMnxTe
The prototypical diluted magnetic semiconductor Cd1-xMnxTe
is a spin-glass (x<0.6) or antiferromagentic (x>0.6), but becomes
ferromagnetic upon doping a small amount of Cr ions. In this
chapter, in order to investigate the origin of the ferromagnetism in
Cd1-x-yMnxCryTe, I have studied the element specific magnetic
properties of its thin films by x-ray absorption spectroscopy (XAS)
and x-ray magnetic circular dichroism (XMCD). I have studied thin
films with a fixed Mn content x ~ 0.2 and varied Cr contents in the
range of y = 0 ~ 0.04 grown by molecular beam epitaxy. The
measured Cr 2p and Mn 2p spectra indicate that both Cr and Mn
ions are divalent and that the spins alignment of Cr and Mn are
aligned in the parallel directions. The ferromagnetic moment of Mn
increases with increasing Cr concentration. These results suggest
that in the presence of Cr ions in Cd1-x-yMnxCryTe, the interaction
between Mn spins changes from antiferromagnetic to ferromagnetic
mediated by the Cr ions and possible mechanism of ferromagnetic
ordering between Mn and Cr ions is due to the double exchange
82
interaction.
5.1 Introduction
II-VI semiconductor compounds based diluted magnetic
semiconductors (DMS’s) [5.1-3] have attracted much attention
because of their relevance to spintronic applications by utilizing
both charge and spin of electrons [5.4, 5]. In II-VI DMS such as
ZnTe, ZnSe, CdSe, and CdTe, magnetic ions with valency 2+ can
easily be incorporated at the II-cation sites of the host lattice [5.6-8].
The replacement of a fraction of the lattice of the nonmagnetic
semiconductor compounds by magnetic ions, paticularly Mn, brings
about interesting magnetic and optical properties such as giant
Faraday rotation, spin glass behavior, formation of magnetic
polarons and so on, which arise from sp–d interaction of the
magnetic ions with band electrons, and/or from interaction between
the magnetic ions themselves, which makes DMS’s as a CdMnTe for
fabricating magneto-optical devices. Galazka et al. [5.9] and Nagata
et al. [5.10] have investigated the magnetic properties of Mn-doped
CdTe and Mn-doped HgTe single crystals, respectively, which could
give rise to paramagnetic, spinglass, and antiferromagnetic phase
regions as functions of temperature and Mn content. Cr is also an
interesting 3d transition element to be incorporated in II-VI
compounds. Cr-based magnetic semiconductors were theoretically
investigated by Sato et al. [5.11] and Blinowski et al. [5.12]. The
ground state of the Cr2+ ion has the 3d4 (e2↑t2
↑e0↓t0
↓) configuration,
which opens the possibility of hopping of both spin-down and
spin-up valence band electrons. Sato and Blinowski et al. predicted
that the p-d exchange between the valence band p holes and the d
electrons of the Cr ions become ferromagnetic. Recently, Shen et al.
[5.13] found that Cr doping into Cd1-xMnxTe turns the system from
the antiferromagnetic spin glass to a ferromagnet. They studied the
ferromagnetic behavior of Cd1-x-yMnxCryTe bulk crystals using a
superconducting quantum interference device (SQUID), but the
83
magnetization measured by a SQUID does not provide the element
specific information about the interaction between Mn and Cr,
which is necessary to elucidate the origin of ferromagnetism have
not been clarified yet. To clarify the current issue, x-ray absorption
spectroscopy (XAS) and x-ray magnetic circular dichroism (XMCD)
are ideal techniques because they are element specific magnetic
probes of the electronic and magnetic properties of transition-metal
ions. In this chapter, I have studied the electronic structure and
magnetic properties of Mn and Cr ions embedded in the lattice of
Cd1-x-yMnxCryTe thin films by XAS and XMCD experiments.
5.2 Experimental
The samples studied here are thin films of Cd1-x-yMnxCryTe
with Cr contents y varied from 0 to 0.04 while keeping Mn content x
fixed around 0.20. The thin films were fabricated on GaAs (001)
substrates by the molecular beam epitaxy (MBE) technique. First, a
buffer layer of CdTe of thickness ~ 700 nm was grown on a GaAs
(001) substrate and after that a Cd1-x-yMnxCryTe layer of thickness
~ 300 nm was successively grown on the CdTe buffer layer. The
sample surface was capped with a 2 nm thick Al layer to avoid
oxidization when the sample was exposed to air. X-ray diffraction
(XRD) studies confirmed that the thin films of Cd1-x-yMnxCryTe were
grown epitaxially without formation of any secondary phases.
Mn and Cr 2p core-level XAS and XMCD measurements were
done at BL-16 of KEK-Photon Factory (PF), Japan. XAS and XMCD
spectra were collected in the total-fluorescence yield (TFY) mode
using a photodiode. The probing depth of the fluorescence yield
detection is about 100 nm. A fixed magnetic field is used to obtain
the XAS spectra and the direction of the photon helicity was
reversed to obtain XMCD spectra. The samples were positioned
with the plane perpendicular to the magnetic field. All the
measurements were performed at 15 K with magnetic fields up to 5
T.
84
5.3 Results and discussion
Figure 5.1 shows the Mn 2p-3d XAS and the XMCD spectra
for Cd1-x-yMnxCryTe thin films, taken in the TFY mode at T = 15K.
The main two groups of the peaks shown in the XAS spectra are
due to the Mn 2p3/2 (L3 edge) and 2p1/2 (L2 edge) spin-orbit
components and are in good agreement with the Mn XAS of
Ga1-xMnxN reported by Hwang et al. [5.14]. From this finding, I
conclude that the doped Mn ions in the Cd1-x-yMnxCryTe thin films
are in the Mn2+ state. Figure 5.1(b) shows the Mn 2p3d XMCD
spectra of the Cd1-x-yMnxCryTe sample measured at various
magnetic fields at T=15 K. It is shown that the peak intensity of the
XMCD spectra is dependent on the magnetic field.
Figure 5.2 shows the Cr 2p XAS and XMCD spectra of the
Cd1-x-yMnxCryTe thin films taken in the TFY mode at T = 15K. Here,
μ+ and μ- indicate absorption spectra for photon helicity parallel and
antiparallel to the Cr 3d spin, respectively. The major two peaks in
the spectrum structures around hν = 579.4 and 589.1 eV are due to
absorption from the Cr 2p3/2 and Cr 2p1/2 core levels, respectively.
The XAS and XMCD spectra at the Cr 2p edge show multiplet
structures, indicating the localized nature of the Cr 3d electrons in
a crystal field. The Cr 2p absorption overlaps with the tail of the
broad absorption due to Te 3d Te 5p transition. Therefore, one
can assume that the Te 3d core absorption spectrum behaves as a
background in Cr 2p XAS and that Te does not show magnetization
so that XMCD is unaffected by the Te core-level absorption. It is
found that the intensity of μ- is larger than that of μ+ in the 2p3/2
core absorption region, whereas the intensity of μ- is smaller than
that of μ+ in the 2p1/2 region. The difference of μ+ and μ- XAS derives
the XMCD (μ+-μ-) structures as shown in Fig. 5.2(b). Figures 5.1(b)
and 5.2(b) reveal the features that the polarity of Mn 2p XMCD is
the same to that of the Cr 2p XMCD, which indicates the parallel
alignment of the spin moments between the Mn and Cr ions.
85
FIG. 5.1: Mn 2p XAS spectra of Cd0.76Mn0.2Cr0.04Te compared with
GaMnN (Mn2+) [5.14] (a) and XMCD spectra at various magnetic
fields (b) of the Cd1-x-yMnxCryTe thin film.
86
FIG. 5.2: Cr 2p XAS spectra (a) and XMCD spectra at various
magnetic fields (b) of the Cd1-x-yMnxCryTe thin film.
87
The energy integral of Mn and Cr 2p XMCD are shown in Fig.
5.3 (a) and (b). Although the application of XMCD sum rules [5.15,
16] to TFY data does not give accurate results because of the
self-absorption effect, I have attempted to deduce the magnetic
moments of the Mn and Cr ions by applying the XMCD sum rules to
the TFY data. Following the orbital sum rule [5.16], the orbital
moment of the Mn ion is almost quenched and consistent with the
expectation while the orbital moment of the Cr ion has large
negative XMCD integral. We can understand the orbital moment by
the electronic configuration of Mn and Cr. Mn2+ has 5 electrons in
3d states and all t2g levels are filled, results the quenching of Mn
orbital magnetic moments. For Cr2+ (3d4), one level of t2g is vacant,
provides the orbital magnetic moment.
Figure 5.4 (a) shows the XMCD intensity of the Cr and Mn 2p
core-levels of Cd1-x-yMnxCryTe thin film versus magnetic field. The
Cr and Mn XMCD intensities show finite slope and can be
extrapolated to a finite value at zero field. This means that the Cr
and Mn XMCD intensities contain both the paramagnetic (PM) and
ferromagnetic (FM) components. I assume that the PM component
is linear in the magnetic field, and obtain the FM components by
subtracting the PM components from the XMCD spectra as shown
in Fig. 5.4 (b). From the line shapes, I conclude that both the FM
and PM components of Cr and Mn are originated from the Cr2+ and
Mn2+ ions, respectively, and that the ferromagentic moment is
larger for the Cr ions than the Mn ions. This suggests that the Cr
ions drive the ferromagnetic ordering of both Cr and Mn ions in the
present system.
88
FIG. 5.3: Mn (a) Cr (b) 2p XMCD of Cd0.76Mn0.2Cr0.04Te and its
energy integral at 5T. (c) Single-electron energy levels in a Td for
Mn2+ (3d5) and Cr2+ (3d4).
89
FIG. 5.4: Cr and Mn 2p XMCD intensity (a) and FM and PM
component of Cr and Mn (b) versus magnetic field of the
Cd1-x-yMnxCryTe thin film.
90
The magnetic field dependences of the Cr and Mn spins are
decomposed into the paramagnetic (PM) component and the
ferromagnetic (FM) component as shown in Fig. 5.4 (b). The slope of
the PM component of Mn is larger than the slope of the PM
component of Cr, indicating that the PM contribution of Mn in
magnetism is larger than the Cr. From the paramagnetic magnetic
susceptibility formula, χ=(gμB)2S(S+1)/3kBT, I calculated the
theoretical susceptibility (χThe.) for Mn2+ (S=5/2) and Cr2+ (S=2),
where g is the lande factor and kB is the Boltzmann constant. I
found that the χThe. for Mn2+ and Cr2+ are 0.52 and 0.35 μB.T-1/ion,
respectively, and are larger than the experimental susceptibility
(χexp.), which suggests the antiferromagnetically (AFM) coupling of
Mn2+ and Cr2+ ions in the Cr-doped CdMnTe. (χThe./ χexp.)Mn > (χThe./
χexp.)Cr indicates that the antiferromagnetic (AFM) coupling of Mn
ions is larger than the Cr ions.
Figure 5.5(a) shows the Mn 2p XMCD spectra of the
Cd1-x-yMnxCryTe sample with various Cr concentration. The figure
indicates that the Mn2+ XMCD intensity depends on the Cr
concentration. Figure 5.5 (b) shows the magnetic moments of the
Mn ions versus magnetic field for various Cr concentrations. From
Fig. 5.5 (b), it is clear that Mn ions without Cr show paramagnetic
behavior as reported by Galazkaet at el. [5.9] and Nagata et al.
[5.10]. After incorporating a small concentration of Cr ions in
Mn-doped CdTe, the dramatically change in the Mn magnetic
moment are observed. The magnetic moment of Mn increases with
the increase of Cr ions in the thin films. A similar trend has also
been observed by Shen et al. [5.13] and Ishikawa et al. [5.17] and
they measured magnetization by using a SQUID. Ishikawa et al.
[5.17] observed a negative Curie-Weiss temperature ΘP in
Cd1-xMnxTe and the ΘP turns to be positive after incorporating only
0.46 % of Cr. Therefore, small content of the Cr present in thin
films changes ΘP from negative to positive value indicating that the
magnetic interaction between Mn spins becomes dominating by
91
FIG. 5.5: Mn 2p XMCD spectra (a) and magnetic moment of Mn (b)
with various Cr content of Cd1-x-yMnxCryTe thin film.
92
ferromagnetic interaction, in contrast to the predominantly
antiferromagnetic Mn-Mn interaction in Cd1-xMnxTe. In the
presence of Cr ions, there should be some mechanism by which the
interaction between Mn becomes ferromagnetic mediated by Cr.
According to Shen et al. [5.13], a small fraction of Cr + ions are
present and the hole bound to the Cr+ acceptor can mediate FM
ordering between the magnetic ions contained within the Bohr orbit
of the hole and this orbit would include both the Cr and the nearby
Mn ions (bound magnetic polaron mechanism). However, the
energy level of the Cr+ charge state is located 1.34 eV above Ev
[5.18], which is too deeply located within the band gap. Another
possible mechanism of the ferromagnetic ordering DMSs doped
with two kind of transition metal atoms is proposed by Akai et al.
[5.19]. They proposed a model for the case of co-doped transition
metals in ΙΙ–ΙV compound semiconductors that the
antiferromagnetic interaction between different kinds of transition
metals results in ferrimagnetic ordering, due to a mechanism
similar to the double-exchange interaction. However, it is not
certain whether this mechanism would be really effective in the
present case where the contents of Mn and Cr are much different
because in Akai et al. [5.19], equal amount of transition metals are
doped. Furthermore, magnetic interaction between Mn and Cr in
the present case is ferromagnetic and not antiferromagnetic which
could lead to ferrimagnetism in Akai et al's model.
Figure 5.6 shows a possible mechanism and a schematic
picture of magnetic interaction between Mn-Mn in Mn-doped CdTe
and Mn-Cr in Cr-doped CdMnTe. In Mn-doped CdTe, the Mn spins
are antiferromagnetically coupled as shown in Fig. 5.6 (a) but after
small amount of Cr doping the interaction between Mn ions near a
Cr ions are changed and aligned parallel with a net magnetic
moment. I calculated the number of ions aligned parallel in samples.
The expected FM component of Cr2+ (3d4) and Mn2+ (3d5) are 4μB/ion
and 5μB/ion, respectively. I found the FM component of Cr and Mn
93
~0.4μB/ion and 0.1μB/ion at 5 T, respectively (see Fig. 5.4 b). It
means only 10% of Cr and 2% of Mn ions are aligned parallel and
the concentration of ferromagnetic Cr and Mn ions in
Cd0.76Mn0.2Cr0.04Te sample aligned parallel is 0.004 ions. The equal
number for Mn and Cr indicates that possible mechanism of
ferromagnetic ordering is due to the double exchange interaction
between Mn and Cr ions as shown in Fig. 5.6 (b). This situation is
similar to doubly and equally doped DMS in Akai et al. [5.19] where
an electron may be exchanged between two species of transition
metal. The double exchange process is mediated by the conduction
band of the host crystal via a resonance state that mixes same spin
d orbitals of the Cr and Mn ions and extended conduction band
states. The wave functions of the state of Cr2+ and Mn2+ ions
coupled with the same spin direction because the d orbitals of the
Cr2+ and Mn2+ ions are less than half filled and half filled,
respectively, and provide the ferromagnetic interaction between Cr
and Mn ions.
FIG. 5.6: Schematic picture of magnetic interaction between (a)
Mn-Mn in Mn-doped CdTe and (b) Mn-Cr in Cr-doped CdMnTe.
94
5.4 Conclusion
I have performed an XAS and XMCD study on
Cd1-x-yMnxCryTe thin films with a fixed Mn content x ~ 0.2 and
varied Cr contents in the range of y = 0 ~ 0.04. From the XAS and
XMCD measurements, the valence of Cr and Mn ions were found to
be in the 2+ state and the spin alignment between Cr and Mn ions
are parallel. From the sum rule analysis, the orbital moment of the
Mn ion is almost quenched while the Cr ion has a large value. The
magnetic moment of Mn depends on Cr concentration in the film
and it increases with increasing the Cr concentration. In the
presence of Cr ions, the interaction between Mn ions becomes
ferromagnetic which is mediated by Cr ions. I found the equal
concentration of ferromagnetic Cr and Mn ions in
Cd0.76Mn0.2Cr0.04Te sample. The equal number for Mn and Cr
indicates that possible mechanism of ferromagnetic ordering is due
to the double exchange interaction between Mn and Cr ions similar
to doubly and equally doped DMS in Akai et al. [5.19].
95
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98
99
Chapter 6
Orbital magnetic moment in
multiferroic MnWO4 studied
by x-ray magnetic circular
dichroism
In this chapter, I have investigated the existence of orbital
magnetic moment in the multiferroic MnWO4 using the Mn
L2;3-edge x-ray magnetic circular dichroism (XMCD) in the
paramagnetic state. I confirmed that the Mn ions in MnWO4 are in
the 2+ states and that the Mn site has lowered symmetry. By
applying the orbital sum rule to the XMCD spectrum, despite the d5
configuration of Mn ion in MnWO4, a finite large orbital magnetic
moment was deduced: Morb/Mspin ~ 0.057. The large value of
Morb/Mspin is due to lower symmetry of Mn sites in the distorted
[MnO6]10- octahedron of MnWO4.
6.1 Introduction
Recently there have been intensive studies on multiferroic
materials due to their intriguing magnetoelectric properties and
potential applications for storage devices, sensors, traducers,
100
actuators, etc [6.1−4]. Very few multiferroic material exist in nature
because in most ferroelectrics such as BaTiO3 ferroelectricity is
driven by the hybridization of empty d orbitals with the occupied p
orbitals of the octahedrally coordinated oxygen ions while
ferromagnetism arises from the partially filled d shell of transition
elements [6.5]. Also ferroelectricity can be induced if the
spin-lattice interaction is large enough to displace the nuclei
cooperatively in particular direction giving rise to a macroscopic
electric polarization. Recently, a new type of multiferroics such as
rare-earth perovskite RMnO3 (R = Y, Tb, Gd, Dy) [6.6−8], in which
magnetic ions are directly involved in a spontaneous electrical
polarization and show a strong interplay between electric
polarization and magnetic order, have been investigated in detail.
Manganese tungstate (MnWO4) is a special compound among the
multiferroic manganates which does not contain a rare-earth ion. It
has already been proved that ferroelectricity can appear in the
cycloidal-spiral spin phase without centrosymmetry [6.9, 10].
Multiferroicity in which electrical polarization is caused by the
spiral order of magnetic moments is explained by the spin-current
model [6.11, 12]. If the spin-rotation axis ê is not parallel to the
magnetic propagation vector Q, nonvanishing spontaneous
polarization P α ê ×Q develop. In these spiral magnets, correlation
between the ferroelectric polarization and cycloidal-spiral spin
structure is suggested to be associated with the antisymmetric part
of exchange coupling, known as Dzyaloshinskii-Moriya interaction
(DMI) [6.12−14].
The multiferroic compounds TbMnO3 [6.15], Ni3V2O8 [6.16],
and MnWO4 [6.17] are prominent examples for inversion symmetry
breaking magnetic ordering. In these multiferroic oxides,
non-collinear spiral spin structure without centro-symmetry may
induce macroscopic spontaneous electric polarization. Among the
spin-spiral multiferroics, MnWO4 is one of the prototypical
multiferroic oxide that exhibits ferroelectricity which is induced by
101
its spiral spin structure, and has been studied by several groups
[6.17, 18]. Taniguchi et al. [6.17] and Arkenbout et al. [6.18] have
reported that the noncollinear spin configuration of the sample is
caused by the electric polarization. Moreover, the electric
polarization induced by the magnetic field flops from the b to the a
axis of the crystal structure. MnWO4 is crystallized in a wolframite
structure (Fig. 1.2), which belongs to the monoclinic space group
P2/c and the MnO6 and WO6 octahedra in the crystal structure
share their edges to form zigzag chains along the c direction. This
compound exhibits three different magnetic phase transitions at T1
= 7.6 K, T2 = 12.7 K and TN = 13.5 K [6.19] to three long wavelength
antiferromagnetic (AF) ordering states. According to neutron
diffraction results, AF1 (T < T1), AF2 (T1 < T < T2), and AF3 (T2 < T
< TN) are a commensurate collinear antiferromagnetic phase, an
incommensurate cycloidal spiral-spin phase, and an
incommensurate collinear antiferromagnetic phase, respectively.
The magnetic structure of the AF1 state is commensurate with the
propagation vector (−1/4, 1/2, 1/2), while that of the AF3 and AF2
states are incommensurate with the propagation vector (−0.214, 1/2,
0.457), while other wolframite FeWO4, CoWO4, and NiWO4 show
only one magnetic transition to the commensurate magnetic state
with a propagation vector (1/2, 0, 0).
The valence state of Mn ions in MnWO4 is 2+ and the orbital
magnetic moment of the Mn2+ ion with the half filled 3d5
configuration is supposed to be quenched. Recently K. V.
Shanavas et al. [6.20] reported a finite orbital magnetic moment
and the origin of ferroelectricity using ab initio electronic-structure
calculations in MnWO4. In this chapter, I report on Mn L2,3 x-ray
absorption spectra (XAS) and x-ray magnetic circular dichroism
(XMCD) experiments of MnWO4 polycrystalline sample in order to
study the electronic structure and magnetic properties of Mn in
MnWO4.
102
6.2 Experimental
Polycrystalline MnWO4, which is expected to have higher
conductivity than the single crystals and good for the measurement
of XAS and XMCD in the TEY mode. Polycrystalline MnWO4
pellets sintered under anisotropic pressures in pure Ar atmosphere.
The sample was then arc melted to create an oxygen vacancies and
to make the sample less resistive.
The XAS and XMCD measurements were carried out at the
undulator beam line BL23-SU of SPring-8, Japan. XAS and XMCD
spectra were collected in the TEY mode. The probing depth of the
total electron yield detection was about 5 nm. In order to avoid
charging effect, the measurements were performed at room
temperature in an applied magnetic field of 8 Tesla. XAS and
XMCD spectra were obtained by taking the sum and the difference
between the spectra taken with different helicities μ+ and μ−,
respectively. The monochromator resolution was E /ΔE > 10000.
The base pressure of the measuremet chamber was about 10−9 Torr.
The sample was cleaved in-situ in the vacuum to obtain a clean
surface.
6.3 Results and Discussion
In Fig. 1, the XAS and XMCD spectra of the Mn 2p core level
are shown and compared with data of reference compounds. Each
absorption spectrum of Mn shows two groups, the L3 (2p3/2) and L2
(2p1/2) edges separated by the spin-orbit splitting of the core level of
~ 11 eV. In Fig. 1, the Mn 2p XAS spectrum measured for the
MnWO4 sample is compared with the Mn 2p XAS data of SrMnO3
(Mn4+, Oh) [6.22], LaMnO3 (Mn3+, Oh) [6.23], Ga1-xMnxN (Mn2+, Td)
[6.24], MnO (Mn2+, Oh) [6.23], and MnWO4 (Mn2+, Oh) [6.25]. The
Mn 2p XAS spectrum of MnWO4 is distinctly different from those of
SrMnO3, and LaMnO3. However, the line shape of the Mn 2p XAS
103
FIG. 1. Mn 2p XAS spectra of MnWO4 compared with those of
SrMnO3 (Mn4+, Oh) [6.22], LaMnO3 (Mn3+, Oh) [6.23], Ga1-xMnxN
(Mn2+, Td) [6.24], MnO (Mn2+, Oh) [6.23], and MnWO4 (Mn2+, Oh)
[6.25].
104
spectrum of MnWO4 is somewhat similar to Ga1-xMnxN. The
difference of XAS of MnWO4 from Ga1-xMnxN is the peak at
structure A. Peak A in MnWO4 is due to the Mn2+ ions at octahedral
site. On the other hand, the spectral features of the Mn 2p XAS of
MnWO4 and MnO are similar to each other with the L3 main peaks
at identical energies. This clearly indicates that the Mn ions in
MnWO4 are also in the high-spin state of the d5 electronic
configuration as the Mn ions in MnO, and the valence of Mn ions in
MnWO4 are in 2+ state at the octahedral position. The clear
differences between the spectra of MnWO4 and MnO are the
shoulder height at low and high energies of the L3 edge. The
differences of peak height suggest that the crystal field in the
MnWO4 system has a lower symmetry than octahedral.
Figure 2 shows the Mn L2,3-edge XAS and XMCD spectra of
the MnWO4 polycrystal. We evaluated the orbital magnetic moment,
morb (Mn), and the spin magnetic moment, mspin (Mn), of the Mn2+
ion using the XMCD sum rules [6.26, 27],
(6.2)
where μ+ and μ− stand for the absorption coefficients for the photon
helicity, parallel and antiparallel to the Mn 3d majority spin
direction, respectively, Nd is the number of electrons in the 3d band,
and MT is the magnetic dipole moment. The orbital magnetic
moment (Morb) and the spin magnetic moment (Mspin) both are in
units of μB/atom, where μB is the Bohr magneton. The spin and
orbital magnetic moments of the Mn ion are thus found to be
0.07±0.01 and 0.004±0.001 μB/ion. Thus the ratio between the
orbital and spin magnetic moments becomes Morb/Mspin = 0.057. The
105
orbital magnetic moment is found to be large and in the same
direction of the spin magnetic moment, indicating that Mn 3d
states are more than half-filled [6.28].
FIG. 2. Mn L2,3-edge XAS and XMCD of MnWO4. (a) XAS
spectrum (sum of μ+ and μ− XAS spectra) and its energy integral (b)
XMCD spectrum and its energy integral. Here, μ+ and μ− stand for
the absorption coefficients with photon helicity parallel (↑↑) and
antiparallel (↑↓) to the Mn 3d majority-spin direction.
106
The large orbital magnetic moment obtained from the
experiment is due to the distortion of [MnO6]10- octahedra. I have
carried out configuration interaction (CI) calculations for MnO6
cluster with the Mn2+ ion in a D3d symmetry crystal field in the
magnetic field of 8 T at a temperature of 300 K. The D3d crystal
field is nothing but the distortion of the [MnO6]10- octahedron.
Under the trigonal distortion, the local symmetry group around the
Mn site changes from the cubic Oh to D3d. The calculated XAS and
XMCD spectra are shown in Fig. 3, where they are compared with
the experimental XAS and XMCD spectra of the Mn2+ ion. The line
shape of the experimental Mn L2,3 XAS is reproduced very well by
the calculated spectrum in the D3d crystal field with Udd = 4.0 eV,
Udc = 4.4, ∆ = 7.0 eV, 10Dq = 0.4 eV, and Veg = 2.0 eV. Here, ∆ is the
charge-transfer energy, Udd is the on-site Coulomb interaction
energy between two 3d electrons, Udc is the Coulomb energy
between the 2p core hole and 3d electron, 10Dq is the octahedral
crystal field splitting, and Veg is the p-d hybridization energy for
the eg electrons of the Mn2+ ion. The charge-transfer energy
between the O 2p and Mn 3d orb i tals i s def ined as
∆=E(dn+1L1)−E(dn), where E(dn) is the multiplet averaged energy of
the Mn 3dn configuration and E(dn+1L1) denotes the same for a
configuration obtained by transferring one electron from one of the
O 2p orbitals to a Mn 3d level having n electrons. I have also
calculated the spin and orbital magnetic moment from the
calculated XAS and XMCD spectra using the sum rules (Equ. 6.1
and 6.2) and found that Mspin=0.07 and Morb=0.002 μB/ion,
respectively, and the ratio of Morb/Mspin=0.029. The experimental
value of Morb/Mspin is large than the calculated Morb/Mspin. One of the
possible reason for the large experimental value of Morb/Mspin may
be the distorted [MnO6]10- octahedron forms lower symmetry than
the D3d. Second possible reason for the large experimental value of
Morb/Mspin is the hybridization between Mn 3d and W 5d orbitals
through the oxygen atoms. The spin and magnetic moments are in
107
the same direction. From the calculation, I found the average 3d
occupancy, n3d, to be 5.09 with 89.10 % d5 character, 10.58% d6L1
character, and 0.32% d7L2 character. These values are in good
agreement with the values obtained by Shanavas et al. [6.20], the
average occupancy of 3d state is 5.14, with 86.48% d5 character,
FIG. 2. Comparison of the experimental and calculated XAS and
XMCD spectra at the Mn L2,3-edge of Mn2+. Experimental and
calculated XAS (a) and XMCD (b) spectra.
108
12.99% d6L1 character, and 0.52% d7L2 character. The significant
population of Mn 3d level more than half-filled in MnWO4 might
provide a way to understand the presence appreciable orbital
moment in MnWO4.
Shanavas et al. [6.20] calculated orbital magnetic moment for
the MnWO4 system in the magnetically ordered state and found
0.001 μB with the same direction as the spin magnetic moment by
using ab initio electronic-structure calculations. This orbital
moment is several times smaller than the observed one. Similar to
the present case of the MnWO4 system, Kim et al. [6.29] also found
large orbital moment for the FeO6 octahedra in the GaFeO3 system.
In GaFeO3, the Fe ion shifts along a certain direction from the
center of the FeO6 octahedron, the parity symmetry of the orbitals
becomes broken for axes orthogonal to the direction and creates
orbital moment according to Kim et al. [6.29]. In the MnWO4
system too, the Mn sites are surrounded by oxygen octahedra and
each oxygen octahedron is significantly distorted and the distorted
octahedra give rise to inequivalent bond lengths. Due to the
distortion, the three different bond lengths of Mn-O in [MnO6]10- are
2.285 Å, 2.160 Å, and 2.104 Å, respectively. The distorted
arrangement of oxygens leads to the distortion of Mn positions and
forms a noncentrosymmetric structure for each individual
octahedron, which is considered to be responsible for the apparently
orbital magnetic moment and electric polarization. Alternatively,
the broken inversion symmetry induce hybridization between Mn
3d and Mn 4p orbitals, which may distort the L2,3 edge XAS and
XMCD in a subtle way, and the orbital sum rule may become
inaccurate.
6.4 Conclusion
In order to investigate the orbital magnetic configuration of
MnWO4, I carried out XAS and XMCD measurements at the Mn
L2,3 edges. The spectral features of Mn 2p XAS indicate that Mn
109
ions are in the high-spin electronic configuration in the 2+ states.
From the sum rule analysis, the spin and orbital magnetic
moments of the Mn ion are found to be 0.07±0.01 and 0.004±0.001
μB/ion, respectively. The orbital magnetic moment is in the same
direction as the spin magnetic moment, indicating that Mn 3d
states are more than half-filled. Using the CI cluster-model
analysis, I found that the average 3d occupancy, n3d, is equal to 5.09.
The distorted (MnO6)10- octrahedra play an important role in giving
rise to the apparently large orbital magnetic and electric
polarization in MnWO4. Further investigation of large orbital
moment in MnWO4 system is needed due to the complex nature of
the coupling between structural and electronic degrees of freedom.
110
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113
114
115
Chapter 7
Summary and Outlook
In the preceding chapters, I have presented the x-ray
absorption spectroscopy (XAS) and x-ray magnetic circular
dichroism (XMCD) studies on the NiFe2O4 (NFO)/BaTiO3 (BTO)
multilayer thin films, Cr-doped CdMnTe thin films, and MnWO4
crystal, in order to obtain the understanding of these materials
from the electronic structure points of view. XMCD is a powerful
technique to study transition metal ions of the magnetic structure
of complex systems and the spin-orbit splitting of L2,3 absorption
edges enables the determination of the spin and orbital magnetic
moments by using sum rules. XMCD technique also enables to
study the electronic structure and the orientation of spin direction.
In Chapter 4, I have performed the Ni and Fe 2p XMCD
measurements on the multiferroic BTO/(NFO/BTO)n multilayer
thin films grown on (001)-SrTiO3 substrates using pulsed laser
deposition with various NFO and BTO thicknesses to understand
the microscopic origin of the magnetoelectric (ME) coupling at the
BTO/NFO interfaces. The XAS and XMCD of the Ni and Fe ion of
the NFO/BTO heterostructures were recorded in the bulk-sensitive
total-fluorescence yield (TFY) mode at room temperature. I found
that the Ni ions are in the 2+ states at the octahedral (Oh) position
116
while Fe ions are in the 3+ states at both Oh and Tetrahedral (Td)
positions. The ferromagnetic moment of Ni2+ is parallel to Fe3+(Oh)
but are antiparallel to Fe3+(Td) following the inverse spinel
structure of NiFe2O4. With decreasing NFO layer thickness, the
average magnetic moment of the Ni ions decreases while the
average magnetic moment of the Fe ions remains unaffected. The
strong ME coupling occurs at interfacial defects where Ni atoms are
replaced by Fe atoms and Fe and Ti atoms are located close to each
other at the interface. The Ti and O atoms in the ferroelectric
BaTiO3 are sensitive to ferroelectric displacements and the
magnitude of ME coupling constant depends on the interface
termination. The Fe-TiO2 bonding at the interface creates oxygen
vacancies. The oxygen vacancies at the interface may play an
important role in ferroelectric displacement and hence determining
the strength of the ME coupling. To improve the ME coupling of the
device, to increase the number of interfaces is important. With
increasing n, αE/n decreases rather than increases. This is probably
because the distance between NFO layers become too short.
meaning that Ni ions at the interface lose ferromagnetic ordering. I
found clear correlation between the ME coupling strength and
decreases of the ferromagnetic moment of Ni. This suggests that
the enhancement of ME coupling occurs at interfacial Ni atoms
whose ferromagnetic behavior is weakened and hybridization with
the BTO electronic states are enhanced.
In Chapter 5, I have studied the XAS and the XMCD of
Cd1-x-yMnxCryTe thin films with Cr content y varied from 0 to 0.04
while keeping the Mn content x fixed around 0.20 grown on GaAs
(001) substrates by the molecular beam epitaxy (MBE) technique to
clarify the origin of the ferromagnetism in the thin films. From the
XAS and XMCD measurements, the valence of Cr and Mn ions were
found to be in the 2+ state and the spin alignment between Cr and
Mn ions are parallel. From the XMCD spectra, I obtained the
ferromagnetic (FM) and paramagnetic (PM) component and found
117
that both the FM and PM components of Cr and Mn are originated
from the Cr2+ and Mn2+ ions, respectively, and that the
ferromagentic moment is larger for the Cr ions than the Mn ions.
From the sum rule analysis, the orbital moment of the Mn ion is
almost quenched while the Cr ion has large value. The magnetic
moment of Mn depends on Cr concentration in the film and it
increases with increasing the Cr concentration. In the presence of
Cr ions, the interaction between Mn ions becomes ferromagnetic
which is mediated by Cr ions.
In Chapter 6, I investigated the possible existence of orbital
magnetic moment in multiferroic MnWO4 using the Mn L2;3-edge
XMCD. The XAS and XMCD of the Mn L2;3-edge was measured in
total-electron yield (TEY) mode at room temperature. From the
spectral features of Mn 2p XAS, I conclude that Mn ions are in the
high-spin electronic configuration in the 2+ states. By applying the
sum rule to the XMCD spectrum, despite the d5 configuration of
Mn2+ ion, a significantly large orbital magnetic moments was
deduced and the orbital magnetic moment is in the same direction
as the spin magnetic moment, indicating that Mn 3d states are
more than half-filled. The distorted (MnO6)10- octrahedra play an
important role in giving rise to the apparently large orbital
magnetic and electric polarization in MnWO4.
Finally, prospects on possible future spintronics research are
mentioned. In this thesis, I studied the magnetoelectric coupling of
NFO/BTO heterostructures. Since BTO is a strong ferroelectric
material, we may consider heterostructure of other ferromagnetic
ferrites such as MnFe2O4, CoFe2O4, and MnCr2O4, etc., with the
ferroelectric BTO to understand the microscopic origin of the ME
coupling at the interfaces. I also studied the Cr and Mn interaction
in Cr and Mn co-doped CdTe. DMS materials doped with two kinds
of magnetic elements have rarely been studied and little has been
known about the interaction between different kinds of magnetic
elements. The present work will highlight new development in
118
doubly doped DMSs in the spintronics. In this thesis, I have also
demonstrated the orbital magnetic moment studies on MnWO4 and
hope that this work will capture some of exciting new developments
in the field of spintronics at a rapid pace, throwing further light
onto the details of these materials. Overall, we have demonstrated
that soft x-ray spectroscopic studies on spintronics materials
provide rich information about the electronic and magnetic
structures. In particular, the present XAS and XMCD studies show
that the interplay between the two transition-metal ions (Ni and Fe,
Mn and Cr, Mn and W) is very rich and is important to create new
spintronics functionalities with significant spin dependent
electronic and magnetic properties. I hope that the present work
will promote soft x-ray spectroscopy on multiferroic and dilute
magnetic semiconductors, leads to further understandings of
physics of spintronics material and could help researcher in the
next generation of smaller, more affordable and more power
efficient devices from spintronics materials.
119
120
121
Appendix
Orbital magnetic moment in
FeCr2S4 studied by x-ray
magnetic circular dichroism
A.1 Introduction
Transition metal-based spinel compounds (AB2X4) have been
a hot topic of experimental and theoretical studies for researchers
[A.1-3]. Within the last decade, a number of new physical
phenomena were discovered in these compounds such as colossal
magneto-resistance [A.4], complex spin order and spin dimerization
[A.5, 6], spin-orbital liquids [A.7], and orbital glasses [A.8], colossal
magneto-capacitive coupling [A.9], and multiferroic behavior [A.10].
These novel phenomena in transition metal-based spinel
compounds present an increased interest for spintronic and
advanced multifunctional device applications. Among them,
FeCr2S4 is a ferromagnetic semiconductor with TC ~ 170 K, and
shows large negative magnetoresistance near the Curie
temperature [A.4]. Due to the strong coupling among spin, charge,
orbital and lattice degrees of freedom, FeCr2S4 displays abnormal
low-field magnetic behavior [A.11] and fascinating physical effects,
e.g., colossal magnetoresistance [A.4] and gigantic Kerr rotation
[A.12]. Park et al. [A.13] reported a band-structure calculation for
FeCr2S4 in which each sublattice of the Fe and Cr transition metals
122
orders ferromagnetically, while the two sublattices are coupled
antiferromagnetically to each other. Recently, the electronic
structure of FeCr2S4 has been studied by density functional
calculation [A.14]. Sarkar et al. [A.14] found small orbital moment
of Cr ion while Fe ion shows large orbital moment. In previous
years, there have been several theoretical and experimental studies
on this compound except for the orbital magnetic moment in
FeCr2S4 by element-specific XMCD technique. To study the orbital
magnetic moment, it is necessary to elucidate the electronic and
magnetic structure of FeCr2S4 by microscopic element-specific
measurement technique that provides the direct information on
valence states, spin and orbital magnetic moments of each
transition-metal element. Here, I report on Fe and Cr L2,3 x-ray
absorption spectroscopy (XAS) and x-ray magnetic circular
dichroism (XMCD) measurements of FeCr2S4 single crystal in order
to study the electronic structure and magnetic properties of Fe and
Cr ions and I find that the Fe ions show a large orbital magnetic
moment at 80K.
A.2 Experimental
The sample studied here is a single crystal of FeCr2S4. The
crystal was grown by a chemical vapor transport method with CrCl3
as a transport agent. The octahedral-shaped crystals were
characterized by powder x-ray diffraction and inductively coupled
plasma spectrometry, which confirms that the obtained crystals are
single phase with expected chemical formula. The sample was
cleaved in-situ to obtain a clean surface. Fe and Cr 2p core-level
XAS and XMCD measurements were done at BL-16 of KEK-Photon
Factory (PF), Japan. XAS and XMCD spectra were collected in the
total-electron yield (TEY) mode (probing depth ~5 nm) at T = 80K
by measuring the sample current and normalizing it with the
mirror current. A fixed magnetic field is used and the direction of
the photon helicity was reversed to obtain XMCD spectra. The base
123
pressure of the measurement chamber was about 10−9 Torr and the
energy resolution was E / ∆E = 8,000.
A.3 Results and Discussion
Figure A.1 (a) shows comparison of the Fe 2p XAS spectrum of
FeCr2S4 with those of FeO (Fe2+) [A.15], Fe metal [A.16], and
γ-Fe2O3 (Fe3+) [A.17]. It is clearly seen that the the Fe 2p XAS
spectra of FeCr2S4 are different from that of γ-Fe2O3 and somewhat
similar to that of FeO. However, in contrast to FeO, no (or very
weak) multiplet structures are observed in FeCr2S4 in both the L3
and L2 peaks, resulting in the line shape which is very similar to
that of Fe metal. The absence of multiplet structures in FeCr2S4
indicates that the Fe 3d electrons are strongly hybridized with the
valence electrons of the S p electrons. The Fe 2p XAS spectrum of
Fe metal is more broadened than the Fe 2p XAS spectra of FeO and
FeCr2S4. Figure A.1 (b) shows comparison of the Fe 2p XMCD
spectra of FeCr2S4 and Fe metal [A.16]. The Fe 2p XMCD spectrum
of FeCr2S4 shows some multiplet features indicated by arrows in
Fig. A.1 (b) while the multiplet features are absent in Fe metal.
From Figs. A.1 (a) and (b), one can conclude that the Fe ions are
mainly in divalent (2+) states in FeCr2S4. The valence state of Fe2+
in FeCr2S4 crystal is also confirmed by the Mossbauer spectroscopy
measurements performed by Chen et al. [A.18].
Figure A.2 shows comparison of the Cr 2p XAS spectrum of
FeCr2S4 with those of Cr2O3 (Cr3+) [A.19] and Cr metal [A.20]. The
Cr 2p XAS spectra of FeCr2S4 are qualitatively similar to that of
Cr2O3, but very different from that of Cr metal, indicating that the
Cr ions in FeCr2S4 are mainly trivalent (3+). On the other hand, the
multiplet structures in FeCr2S4 are not so sharp compared to the
Cr3+ XAS of Cr2O3. These differences in multiplet structures reflect
that the character of the Cr–S bonding is not a simple ionic bonding,
but rather close to a covalent bonding as compared to the more ionic
Cr–O bonding in Cr2O3. This is probably due to the weaker
124
electronegativity of S ions than the O ions.
Figure A.1: (a) Comparison of the Fe 2p XAS spectra of FeCr2S4
with those of FeO (Fe2+) [A.15], Fe-metal [A.16], and γ-Fe2O3 (Fe3+)
[A.17]. (b) XMCD spectrum of FeCr2S4 compared with Fe metal
[A.16].
125
Figure A.2: Comparison of the Cr 2p XAS spectra of FeCr2S4 with
those of Cr2O3 (Cr3+) [A.19] and Cr metal [A.20].
The Fe 2p XAS spectra of FeCr2S4 for incident radiation with
both positive and negative helicities (μ+ and μ-) taken in the TEY
mode are shown in Fig. A.3 (a). The major two peaks in the spectral
structures around hν = 707.9 and 720.6 eV are due to absorption
from the Fe 2p3/2 and 2p1/2 core levels, respectively. The intensity of
μ+ is larger than that of μ- in the 2p3/2 (L3-edge) core absorption
region, whereas the intensity of μ+ is smaller than that of μ_ in the
2p1/2 (L2-edge) region. The difference between the μ+ and μ- XAS
derives the XMCD (μ+-μ-) structures as shown in Fig. A.3 (b). The Fe
2p3d XMCD spectra of the FeCr2S4 crystal measured at various
magnetic fields are shown in Fig. A.3 (b). The inset of the Fig. A.3
(b) shows the enlarge Fe 2p XMCD of FeCr2S4 at 0 T. The XMCD
126
intensity down to H = 0 T clearly indicates the ferromagnetism by
Fe ions of the sample.
Figure A.4 (a) shows Cr 2p XAS spectra of FeCr2S4 for
incident radiation with photon helicity parallel (μ+) and antiparallel
(μ-) to the Cr 3d spin, respectively, taken in the TEY mode. The
major two peaks in the spectrum structures around hν = 579.6 and
587.9 eV are due to absorption from the Cr 2p3/2 and Cr 2p1/2 core
levels, respectively. It is found that the XAS spectrum with positive
helicity (μ+) is more broadened than that of negative helicity (μ-). In
addition, the spectral weight of μ+ is shifted to higher energy
compared to μ- both in the 2p3/2 and 2p1/2 regions. This derives the
complicated XMCD (μ+-μ-) structures. The Cr 2p XMCD spectra of
the FeCr2S4 measured at various magnetic fields are shown in Fig.
A.4 (b). The inset of Fig. A.4 (b) shows an enlarged Cr 2p XMCD of
FeCr2S4 at 0 T. The XMCD intensity of Cr 2p down to H = 0 T
clearly indicates ferromagnetism by Cr ions in the sample. From
Figs. A.3 and A.4, one can see the polarity of Fe 2p XMCD is
opposite to that of Cr 2p XMCD, which indicates the antiparallel
alignment of the spin moments between the Fe and Cr ions, which
is consistent with the band-structure calculation for FeCr2S4
reported by Park et al. [A.13].
Figures A.5 and A.6 show the Fe and Cr 2p XAS and XMCD
spectra with its energy integral. The black dotted lines in Figs. A.5
(a) and A.6 (a) show arctangent background to subtract [A.21]. A
determination of the spin magnetic moment using XMCD sum rules
for lighter transition metal elements such as Cr is questionable
because the 2p3/2 and 2p1/2 edges are not well separated and overlap
each other. Here, I have evaluated the orbital magnetic moments of
Fe and Cr ions using the XMCD sum rules [A.22, 23]
127
Figure A.3: Fe 2p XAS spectra at 1T (a) and XMCD spectra at
various magnetic field (b) of FeCr2S4. Inset shows an enlarged
spectrum of Fe 2p XMCD at 0 T in the inset of Fig. A.3 (b).
128
Figure A.4: Cr 2p XAS spectra at 1T (a) and XMCD spectra at
various magnetic field (b) of FeCr2S4. Inset shows an enlarged
spectrum of Cr 2p XMCD at 0 T in the inset of A.4 (b).
129
where Nd is the number of electrons in the 3d band. The orbital
magnetic moment (Morb) is given in units of μB/atom, where μB is
Bohr magneton. From the sum rule analysis, the orbital magnetic
moments of Fe and Cr ions are found to be 0.225 and 0.016 μB/ion,
respectively. In the Fe ions, the spin and orbital moments have the
same sign, whereas opposite sign is found for the Cr ions. This is
because the d states of Fe2+ are more than half filled while those
Cr3+ is less than half filled. The orbital moment of the Cr ions is
found to be small due to the d3 configuration of Cr. However, the
large orbital moment of the Fe ions is remarkable since the
spin-orbit interaction within e levels of Fe should be small. A
possible reason is that the crystal-field splitting is small in FeCr2S4.
According to first-principles calculation by Sarkar et al. [A.14], the
orbital magnetic moments of Fe and Cr ions are 0.077 and 0.024 for
GGA+SO calculation, and 0.134 and 0.026 for GGA+U+SO
calculation, respectively. Here, GGA, U, and SO stands generalized
gradient approximation, Hubbard, and spin-orbit interaction,
respectively. Our experimental orbital moment of the Fe ion is a
little larger while the orbital moment of the Cr ion is a little smaller
than the theoretical value given by Sarkar et al. [A.14].
Han et al. [A.24] performed XAS and XMCD measurements of
Fe0.5Cu0.5Cr2S4 and found that the spin and orbital magnetic
moment of Cr3+ (d3 system) are aligned in the same direction (Fig.
A.7). According to Hund's third rule, the spin and orbital moment
should be antiparallel for systems with less than a half-filled shell,
and parallel for systems with more than a half-filled shell. I found
that the spin and orbital magnetic moments are aligned in the
opposite direction in Cr3+ (d3 system), in disagreement with to the
result in Han et al. and in agreement with Hund’s third rule. Park
et al. and Sarkar et al. also found that the opposite alignment of the
spin and orbital moments of Cr ions from band structure
calculations for FeCr2S4.
130
Figure A.5: Fe 2p (μ++μ-) XAS spectrum of FeCr2S4 and its energy
integral (a) and XMCD (μ+-μ-) spectrum and its energy integral (b)
at a magnetic field of 1T. Black dotted line in Fig (a) shows the
arctangent background subtraction.
131
Figure A.6: Cr 2p (μ++μ-) XAS spectrum of FeCr2S4 and its energy
integral (a) and XMCD (μ+-μ-) spectrum and its energy integral (b)
at a magnetic field of 1T. Black dotted line in Fig (a) shows the
arctangent background subtraction.
132
Figure A.7: Cr 2p XAS and XMCD spectra of Fe0.5Cu0.5Cr2S4 [A.24].
A.4 Conclusion
FeCr2S4 crystal grown by a chemical vapor transport method
with CrCl3 as a transport agent was studied by an XAS and XMCD.
The valence states of Cr and Fe ions are nearly trivalent (Cr3+) and
divalent (Fe2+), respectively. On the other hand, the Fe 2p XAS
spectra of FeCr2S4 do not exhibit the multiplet structures,
indicating the strong hybridization between the Fe 3d and S p
electrons. From the magnetic field dependence XMCD
measurement of Fe and Cr ions, I can conclude that the Fe and Cr
ions ordered ferromagnetically in FeCr2S4. From the sum rule
analysis, the two sublattices in FeCr2S4 are coupled
antiferromagnetically to each other and agree with the Hund’s
third rule and the orbital magnetic moments of Fe and Cr ions were
0.225 and 0.016 μB/ion, respectively.
133
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137
Acknowledgments
It is my great pleasure to express my deep regards and special
gratitude to the following people for their help concerning my
doctor thesis.
First, my special cordial gratitude goes to Prof. Atsushi Fujimori,
for his advice, encouragement, as well as for always making himself
available for discussion and guidance whenever it was needed
throughout the whole project. My Ph. D. thesis would not have been
possible without his excellent supervision. I have appreciated his
clear advice, which comes from his deep knowledge and insight in
the field of condensed matter physics.
I would also like to express my deeply thanks to Dr. Teppei
Yoshida. His valuable advice were indispensable to this work. I
have learned a lot from his energetic action and thoughtfulness. I
would like to say my special thanks to Dr. Takashi Kataoka and Dr.
Vijay Raj Singh who have introduced me the enchanted world of
DMS and multiferroic materials and their enthusiasm and effort
took me step into the field of synchrotron radiation spectroscopy in
the very beginning. I also thank Dr. Toshiharu Kadono, Mr. Keisuke
Ishigami, Mr. Yo Yamazaki, Mr. Goro Shibata, and Mr. Takayuki
Harano for their great help during beamtime and the fruitful
discussion we had together. I have spent great time with all of them
during our study.
The experiments at NSRRC, Photon Factory, and SPring-8 were
supported by a number of people. I am particularly grateful for
members of NSRRC: Mr. Fan-Hsiu Chang, Dr. Hong-Ji Lin, Prof.
Di-Jing Huang and Prof. C. T. Chen for their helpful technical
138
support during the beamtimes at NSRRC. The experiments at
Photon Factory BL-16A2 were supported by Prof. Tsuneharu Koide,
who has given me a lot of educative advice about experimental
technique and XMCD measurements. I would like to thank for their
valuable technical support during the beamtime. I am deeply
thankful to SPring8 members: Dr. Yukiharu Takeda, Dr. Tetsuo
Okane, Dr. Yuji Saito, and Prof. Hiroshi Yamagami for their kind
support during the beamtimes at SPring8.
I have to express my great thanks to Prof. Yuanhua Lin, Prof.
Ce-Wen Nan, Dr. Yi Zhang, and Dr. Jing Liu for providing us with
the high-quality samples of the BTO/(NFO/BTO)n multilayer thin
films and warm encouragement. I am very thankful to Prof. Shinji
Kuroda and Mr. Kôichirô Ishikawa for providing us with the
interesting samples Cr-doped CdMnTe thin films and valuable
discussions. I would also like to thank Prof. Sugata Ray and Mr.
Somnath Jana for providing excellent MnWO4 crystal and their
kind support. I would like to thank Prof. Kenya Ohgushi and Prof.
Yoshinori Tokura for the high-quality FeCr2S4 crystal and valuable
discussions.
I express my special thanks to Prof. Arata Tanaka for his
theoretical support about CI cluster-model analysis of the x-ray
absorption spectra, teaching me his codes of cluster model
calculation, and enlightening discussions.
My warmest thanks go to all the former and current members of
Fujimori group for useful advice and supporting my daily research
life: Dr. Shin-ichiro Ideta, Dr. Kohei Yoshimatsu, Mr. Leo Cristobal
C. Ambolode II, Mr. Shin-ichi Aizaki, Mr. Ichiro Nishi, Mr. Wataru
Uemura, Mr. Hakuto Suzuki, Mr. Fumio Takahashi, and Mr.
Masafumi Horio. I have spent great time with all of them during
our study and in many other additional activities. Also I thank
them all for being ready to help me all the time. I would like to
thank Ms. Emiko Murayama, Ms. Yuko Shimazaki, Ms. Ami Ito,
and Ms. Miki Ueda for dealing with a lot of business stuff and
139
giving me encouragement.
I express my thanks to Ms. Emiko Gosho and other staffs of
International Liaison Office (ILO) for dealing with matters such as
admission & enrollment registration for International Research
Students, an arrival orientation, arrangements of scholarships,
housing, visas and organizing various intercultural events.
My stay in Tokyo makes a lot of friends who shared with me
everything and a lot of discussions. List is very long, in no
particular order Dr. Kirpa Ram, Dr. Md. Rizwan, Dr. Md. Waseem
Akhtar, Dr. Zainul aabdin Khan, Dr. Gautam Singh, Mr. Saurabh
Sharma, Mr. Raghavendra Jain, Mr. Akki Reddy, Mrs. Alka Gupta
and Mr. Deepu. I would also like to thank the family members of
University of Tokyo-Indian Students Association (UTISA) who
made my days at University of Tokyo really enjoyable and cheerful.
My great thanks are also to the Japanese Embassy in India and
the Japanese Ministry of Education, Culture, Sports, Science and
Technology (MEXT) for choosing me to come to Japan and receive
the Monbukagakusho scholarship and continue my PhD study at
The University of Tokyo. I would also like to thank Department of
Physics's special program (Yusen Haichi Waku in Japanese) for
inviting me for Ph. D. course.
I would like to thank the whole University of Tokyo family which
made my stay in University and Tokyo a memorable one.
Finally, I express my best regards and thanks to my father Sri.
Ram Anuj Verma, mother Smt. Gyanmati Verma, brother Mr. Jai
Prakash Verma, sister Sarita Verma, and other family members
Smt. Poonam, Neha, Anisha, Utkarsh and Divyansu for their love,
understanding, support and encouragement.
University of Tokyo Virendra Kumar Verma
July 2012