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Impedance of Soft Magnetic Multilayers:
Application to GHz Thin Film Inductors
ANDREY GROMOV
Department of Physics, Section of Nanostructure Physics
(Stockholm 2001)
Abstract
Transport and magnetic properties of magnetic multilayers have been a topic
of intensive research over the past 10-15 years, owing to such important discov-
eries as the oscillatory interlayer exchange interaction, giant magnetoresistance,
giant perpendicular anisotropy. These phenomena are behind the current un-
precedent growth rates in magnetic and magneto-optical data storage, and are
expected to result in new large scale applications, such as magnetic random ac-
cess memory and spin logic. Recently, the high frequency properties of magnetic
multilayers have been attracting an increasing attention, related to applications
in GHz inductors and sensors. This work is devoted to understanding the high
frequency response of ferromagnetic sandwiches and fabrication of an ecient
magnetic thin lm inductor.
A theoretical approach to calculating impedance of metallic magnetic/conductor
layered structures is developed. The frequency range considered extends to the
ferromagnetic resonance region of soft magnetic lms (of the order of 1 GHz).
The analysis includes the eects of screening of the high frequency elds by
eddy currents as well as the dynamics and relaxation of the magnetization of
the ferromagnetic sub-system. Analytical expressions for the impedance as a
function of frequency and material parameters and geometry of magnetic sand-
wich stripes are obtained. Two main cross-sectional layouts are considered: a
magnetic/conductor/magnetic sandwich stripe with and without ux closure
at the edges along the stripe length - with and without the magnetic lm en-
closing the conductor strip. The importance of good magnetic ux closure for
1
achieving large specic inductance gains and high eciency at GHz frequencies
is emphasized.
The theoretical results obtained were used to design and analyze magnetic
lm inductors produced using iron nitride alloy lms. Patterned sandwiches,
consisting of two Fe-N lms enclosing a conductor lm made of Cu, were fabri-
cated on oxidized Si substrates using lift-o lithography. The inductors exhib-
ited a 2-fold specic inductance enhancement at 1GHz. The magnetic contribu-
tion to the total ux in the narrow devices was less then predicted theoretically,
which was attributed to hardening of the magnetic material at the edges of the
strip leading to incomplete ux closure. Material and design issues important
for further improving the performance of the devices are discussed.
Contents
Outline 4
1 Impedance of ferromagnetic multilayers 4
1.1 Spin dynamics . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 5
1.1.1 Phenomenological theory . . . . . . . . . . . . . . . . . . . . . 5
1.1.2 Spin relaxation . . . . . . . . . . . . . . . . . . . . . . . . . . . 7
1.2 General electrodynamics . . . . . . . . . . . . . . . . . . . . . . . . . . 8
1.2.1 Field and potential representation . . . . . . . . . . . . . . . . 8
1.2.2 Gauge Transformations . . . . . . . . . . . . . . . . . . . . . . 9
1.2.3 Maxwell's equations in a steady state . . . . . . . . . . . . . . 10
1.2.4 Steady state potentials in conductive media . . . . . . . . . . . 12
1.2.5 Solutions for the scalar potential . . . . . . . . . . . . . . . . . 13
1.2.6 Expression for impedance . . . . . . . . . . . . . . . . . . . . . 15
1.3 Sandwich stripe . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 17
1.3.1 Physical aspects of dimensional reduction . . . . . . . . . . . . 18
1.3.2 Approximation of the external ux . . . . . . . . . . . . . . . . 19
1.3.3 Impedance . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 20
2 Materials: soft ferromagnetic lms 24
2.1 Material requirements . . . . . . . . . . . . . . . . . . . . . . . . . . . 24
2.2 Oxides . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 25
2.3 Alloys . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 26
2.4 Instrumentation for magnetic properties measurement . . . . . . . . . 28
2
2.4.1 Loop tracer . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 28
2.4.2 Magnetometry -VSM . . . . . . . . . . . . . . . . . . . . . . . . 30
2.4.3 HF permeameter . . . . . . . . . . . . . . . . . . . . . . . . . . 31
2.5 Fe-X-N lms . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 33
2.5.1 Magnetic properties of Fe-N and Fe-Ta-N . . . . . . . . . . . . 33
2.5.2 Anisotropy due to oblique deposition . . . . . . . . . . . . . . . 36
2.5.3 FMR susceptibility . . . . . . . . . . . . . . . . . . . . . . . . . 39
3 Applications: GHz inductors 41
3.1 Background . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 41
3.2 Design . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 42
3.2.1 Spirals and meanders. . . . . . . . . . . . . . . . . . . . . . . . 42
3.2.2 Planar solenoids . . . . . . . . . . . . . . . . . . . . . . . . . . 44
3.2.3 Sandwiched strip . . . . . . . . . . . . . . . . . . . . . . . . . . 44
3.3 Device fabrication . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 45
3.3.1 Lithography process . . . . . . . . . . . . . . . . . . . . . . . . 45
3.3.2 Film deposition . . . . . . . . . . . . . . . . . . . . . . . . . . . 49
3.3.2.1 UHV system . . . . . . . . . . . . . . . . . . . . . . . 49
3.3.2.2 Reactive magnetron sputtering . . . . . . . . . . . . . 50
3.3.2.3 Electron beam evaporation . . . . . . . . . . . . . . . 51
3.4 GHz inductors . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 52
3.4.1 Impedance measurement: calibration and deembedding . . . . 52
3.4.2 HF performance . . . . . . . . . . . . . . . . . . . . . . . . . . 55
3.4.3 Flux closure at the edges . . . . . . . . . . . . . . . . . . . . . 59
3.5 Prospectives . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 60
4 Appendix 62
References 63
5 Acknowledgments 66
6 Appended papers 67
3
Outline
The thesis consists of three main parts. Part 1 contains an overview of theoretical
modeling of the impedance of soft ferromagnetic multilayers. Maxwell's equations
in the potential form combined with the Landau-Lifshitz equation for the dynamics
and dissipation of the magnetization of the ferromagnetic sub-system are analyzed.
The analysis is applied to a magnetic/conductor/magnetic sandwich, for which the
impedance is obtained analytically. The enhanced magnetic ux due to the mag-
netic lms in the sandwich yields high specic inductance, the property essential for
miniaturization of GHz inductors.
Part 2 contains a brief overview of magnetic materials suitable for use in thin lm
inductors. We discuss the properties required of the material, dictated primarily by
considerations of strong low-loss high frequency magnetic response and compatibility
of the material with integration into various layered structures. A number of recently
developed high moment, high resistivity soft magnetic alloy systems, suitable for use
at GHz frequencies, are briey reviewed. We conclude by describing the preparation
of reactively sputtered Fe(Ta)N lms and discuss the properties important for device
applications.
In Part 3 the status of research on magnetic lm inductors is reviewed. The fab-
rication of FeN/Cu/FeN/ sandwich strips using lift-o lithography is described. The
details of the high frequency impedance measurements are given. The performance
of the devices and the factors aecting it are discussed. We conclude with a view of
the prospects for magnetically enhanced GHz inductors.
This thesis is based on the research work that has been presented in the publica-
tions appended.
1 Impedance of ferromagnetic multilayers
This section is an introduction to the fundamentals of modeling the high frequency
response of metallic magnetic layered systems. The impedance of sandwiches, con-
sisting of soft ferromagnetic and nonmagnetic metal layers, is discussed for various
cross-sectional layouts. The frequency range of interest here extends to the ferromag-
netic resonance (FMR) range of the magnetic sub-system. Therefore, screening of
high frequency elds by eddy currents in the lms is to be considered in combination
with the intrinsic magnetization dynamics and relaxation.
We rst overview the theory of FMR [1], which is used universally to describe
4
the response of ferromagnetic materials at high frequencies. The magnetic response
is expressed through the permeability (or susceptibility) tensor. The dissipation is
treated phenomenologically by introducing a damping parameter, which determines
the rate of decay of the magnetization precession after the excitation is removed.
Next we pose the general electrodynamical problem and dene the impedance for
systems with alternating magnetic and non-magnetic layers, taking into account both
screening and magnetization dynamics.
Finally, we illustrate the theory by discussing the impedance of a thin and long
magnetic/conductor sandwich. This structure is often studied in experiments since it
nds applications in GHz inductors and sensors.
1.1 Spin dynamics
The dynamic magnetization and eddy currents form, in the most general case, a
coupled system described by a set of coupled dynamic equations for the spin preces-
sion/relaxation and Maxwell's equations for elds and currents in the material. Such
systems often are very complex and must be analyzed numerically. If the system
possesses a certain symmetry (excitation vs. the equilibrium magnetization), how-
ever, the spin dynamics and Maxwell's equations can be analyzed independently and
combined in the nal result for the impedance. Here we will deal with such systems
only, keeping the analysis in the analytical domain.
1.1.1 Phenomenological theory
A dynamic equation for the magnetization of a ferromagnetic material,!M , was rst
introduced by Landau and Lifshitz [1], in which they expanded the rate of change of
the magnetization along three orthogonal vectors:
@
@t
!M =
!M
!M !H eff L
!M !M !H eff : (1)
The magnitude of the magnetic moment is a function of temperature only and is
constant for motion at a xed temperature jM j = Ms. Therefore = 0 and the
resulting motion is precession with the gyromagnetic ration and relaxation constant
L. The nature of the relaxation term is clearly seen when (1) is rearranged into
Gilbert's form [2] and is a force proportional to the rate of change of the magnetic
5
moment (magnetization velocity) and opposing the excitation:
@
@t
!M = !M
!H eff
Ms
@
@t
!M
: (2)
The eective magnetic eld in (2) is, in general, a sum of the anisotropy eld, Ha,
externally applied uniform eld H , demagnetizing eld Hd, exchange eld Hex, and
excitation eld h:!H eff =
!Ha +
!H +
!Hd +
!Hex +
!h :
The demagnetizing eld reects the shape of the sample. We omit it for now and
will include it through boundary conditions for multilayer lms discussed later on.
The exchange eld is proportional to the degree of misalignment between neighboring
spins. It is eective for samples of size comparable to the exchange length, which
is typically 106cm. This is much smaller than the structures that we will be
discussing, so Hex is neglected here-forth. Finally, we assume that the anisotropy is
uniaxial in the plane of the lms with the easy axis taken to be along z, and the
external uniform eld (if any) is applied along z, so!Ha +
!H = H0
!ez .In the absence of excitation
!h the magnetic moment is the equilibrium magneti-
zation,!M =
!M0 = M0
!ez . For small excitations we can linearize (2) in the standard
way [3]:
!M =
!M0 +
!mei!t
!H eff =
!H0 +
!h ei!t
!m and!h are small compared to M0 and H0, and have zero z-components. Substi-
tuting these into (2) we obtain:
i!!m = !m !H0 !M0
!h i!
!M0 !m;
!mx + (i H0 + !)my = i hy
!my + (i H0 + !)mx = i hx:
In the matrix form, !m = b!h , where b is the susceptibility tensor. The permeability
6
tensor is
b = b1 + 4b =
0B@ ia 0
ia 0
0 0 1
1CA ; (3)
where b1 is the unit tensor and
=!H (!H + !M ) !2
!2H !2
(4)
a =!M!
!2H !2
(5)
!M = 4Ms ; !H = (H0 +Ha) i!: (6)
For homogeneous materials the components of the permeability tensor are coordinate-
independent. The above result can then be directly substituted into the Maxwell
equations for structures under study.
1.1.2 Spin relaxation
The phenomenological relaxation term introduced above (1)-(2) scaled by a constant
represents a number of fundamental dissipative mechanisms in a ferromagnetic ma-
terial. These mechanisms can be roughly divided into direct relaxation to the lattice
(phonons), and indirect relaxation through excitation of non-uniform magnetization
modes (also known as spin-waves or magnons), which in turn decay into the lattice. In
the case where direct ow of energy from the uniform excitation into lattice motions
mediated by magnetoelastic (spin-orbit) coupling dominates, the damping constant
can in general be expressed through the elastic constants of the material [4]. For
samples comparable or larger than the domain wall size (the limit of interest in this
work), decay of the uniform mode into spin-waves needs to be taken into account.
The latter depends on the size as well as the shape of the sample. In the case of
metals an additional loss mechanism is present, namely screening of high frequency
excitations by eddy currents of conduction electrons.
A microscopic treatment, even qualitative, of spin relaxation in magnetically or-
dered media requires an extensive knowledge of the microstructure of the sample, and
is seldom possible for technologically interesting materials. In the case of a ferro-
magnetic metal one can list [5] a large number of elementary microscopic scattering
processes that can play a role in magnetization relaxation. These can be subdivided
into magnon-phonon, magnon-magnon, and magnon-conduction electron scattering.
7
A few examples of the latter would be in order: (i) eddy current damping through in-
duced emf, (ii) exchange in the strong screening regime, (iii) direct dipolar interaction
of a localized magnetic spin with either the spin or orbital moment of an itinerant
conduction electron, and exchange interaction between the same. Although the re-
laxation constant, , is only a qualitative phenomenological representation of many
physical processes, it is found in many cases to provide a satisfactory description of
the experiments.
In what follows we will account explicitly for dissipation due to non-uniform mag-
netization modes and eddy currents by solving the dynamic equations in conductive
multilayered samples in a given and xed geometry as to the interfaces and bound-
aries. The 'intrinsic' damping constant (in the absence of screening and spin waves)
will be assumed to have been determined experimentally (see section 2.5.3 on page 39).
1.2 General electrodynamics
1.2.1 Field and potential representation
The basic laws of electromagnetism in the dierential form are:
Gauss0s law div!D = 4 (7)
Ampere0s law (modified) curl!H =
4
c
!J +
1
c
@!D
@t(8)
Faraday0s law curl!E +
1
c
@!B
@t= 0 (9)
Absence of free magnetic poles div!B = 0: (10)
It required the genius of J. C. Maxwell to see the inconsistency in Amper's law,
and thus modify the set of equations now known as Maxwell's equations. They can
be solved for eld distributions in some simple situations. It is often convenient,
however, to introduce potentials in order to obtain a smaller number of second-order
equations, while satisfying the Maxwell equations identically (see, for example, [6]).
Since div!B = 0, we can dene
!B in terms of a vector potential:
!B = curl
!A: (11)
Then the other homogeneous equation (9), Faraday's law, can be written as
8
curl
!E +
1
c
@!A
@t
!= 0: (12)
This means that the quantity with vanishing curl in (12) can be written as a gradient
of some scalar function, namely, a scalar potential ':
grad' =!E +
1
c
@!A
@t
or
!E = grad'
1
c
@!A
@t: (13)
The denition of!B and
!E in terms of the potentials
!A and ' according to
(11) and (13) satises identically the two homogeneous Maxwell's equations. The
inhomogeneous equations (7-8) can then be written in terms of the potentials as
r2'+1
c
@
@tdiv
!A = 4; (14)
r2!A 1
c2@2!A
@t2 grad
div
!A +
1
c
@'
@t
=
4
c
!J : (15)
We have now reduced the set of four Maxwell's equations to two equations. But they
are still coupled equations. The uncoupling can be accomplished by exploiting the
arbitrariness involved in the denition of the potentials.
1.2.2 Gauge Transformations
When there is a simple or no charge distribution, a useful gauge for the potentials is
the so-called Coulomb, radiation or transverse gauge:
div!A = 0: (16)
From (14) we see that the scalar potential then satises the Poisson equation,
r2' = 4: (17)
The scalar potential is the instantaneous Coulomb potential due to the charge density
(!r ; t) or due to potentials on the boundary. The vector potential satises the
9
inhomogeneous wave equation:
r2!A 1
c2@2!A
@t2=
1
cgrad
@'
@t
4
c
!J : (18)
The term involving the scalar potential can, in principle, be calculated separately
from (17). It is interesting to note a peculiarity of the Coulomb gauge. Electromag-
netic disturbances are well known to propagate with a nite speed. Yet the solution
to (17) indicates that the scalar potential "propagates" instantaneously everywhere
in space. The vector potential, on the other hand, satises the wave equation (18),
with its implied nite speed of propagation, c. At rst glance it is puzzling to see how
this obviously unphysical behavior is avoided. A preliminary remark is that it is the
elds, not the potentials that concern us. Both potentials in this situation play the
role of auxiliary mathematical functions, derivatives of which in combinations return
the real physical quantities.
1.2.3 Maxwell's equations in a steady state
Let us consider a harmonic external power source. The components of the elds are
scalar quantities and therefore their sinusoidal time variations can be represented by
means of complex numbers. The time dependence of!E , for instance, is
!E (t) = Re
!Eei!t
=
1
2
!Eei!t +
!Eei!t
; (19)
where!E is a complex amplitude in the extended 6D space. All the other sinusoidal
eld vectors can be represented similarly in terms of corresponding complex vectors,
and all sinusoidal scalar quantities in terms of corresponding complex scalars.
We must note, however, that, in order for all of the electromagnetic quantities
to be sinusoidal functions of time, the entire electromagnetic system must be linear.
Thus, a sinusoidal steady state can exist only if
!B = b!H (20)!D = "
!E (21)
!J =
!E ; (22)
with the permeattivity, ", conductivity, , and permeability tensor components, ij
(see (3) in section 1.1.1 on page 5), that are independent of time at each point in
10
space. In this case the dierential eld laws (7-10) can be written as linear dierential
equations relating the eld vectors and the free-source densities:
curl(b0
!B ) =
!E + "
@!E
@t(23)
curl!E =
@!B
@t(24)
div!B = 0 (25)
div("!E ) = : (26)
Here 0 = 4 107 is the permeability of free space and b is the inverse tensor,0B@ ia 0
ia 0
0 0 1
1CAwhere =
22a
, a =a
22a
together with (4)-(6). SI units have been used here.
Substitution of the harmonic vectors dened above for!E (19) and
!B into Eq.24
yields
curl!Eei!t + curl
!Eei!t = i!!Bei!t + i!
!Bei!t:
This equation must be satised regardless of the time origin selected, i.e., it must be
satised when an arbitrary constant t0 is added to t [7]. Suppose, for instance, that
t0 =
2!, we obtain then
curl!Eei!t curl
!Eei!t = i!!Bei!t i!
!Bei!t:
Sum of the last two equations yields
2curl!Eei!t = 2i!!Bei!t:
Similarly, for all the equations (23-26) we obtain8>>>><>>>>:curl
!E = i!!B
curl(b!B ) = 0( + i!")!E
div!B = 0
div("!E ) = :
(27)
11
We can conclude then that Eq.27 is equivalent to Eq.23-26 in the sinusoidal steady
state. Clearly, all linear relations between sinusoidal time functions can be trans-
formed into equivalent complex relations by substituting for the time functions the
corresponding complex quantities, and for the dierential operator @
@tthe imaginary
quantity i!.
1.2.4 Steady state potentials in conductive media
We divide our system in to the regions where the media parameters " and can be
approximated by constants in each region, so one can take them outside the space
derivatives: 8>>>><>>>>:curl
!E + i!
!B = 0
curl(b!B ) = 0( + i!")!E
div!B = 0
div!E = 0;
(28)
Assuming no free electric charges.
The following procedure is a transition from unknown eld amplitudes to the
potential amplitudes, rst substituting!B = curl
!A into the rst equation of (28),
and next setting the expression obtained under curl equal to a gradient of some scalar
function. The expression (13) in the sinusoidal steady state becomes:
!E = grad' i!
!A: (29)
Using the dierential Ohm's law, the current density is obtained as
!J =
grad'+ i!
!A: (30)
Next, using (29) and the Coulomb gauge, div!A = 0, the second and forth equations
in (28) become
curlbcurl!A = 0( + i!")(grad'+ i!
!A ); (31)
r2' = 0: (32)
Examples below will be given for soft magnetic alloys, which are technologically
attractive for use in planar devices. The typical conductivity is = 5 105(1m1),
12
the maximum frequency to be considered 10 GHz, and the dielectric constant is
approximately that of vacuum, "0 = 8:854 1012
(faradm1). An estimate of the
complex constant + i!" in (31) gives
(1 + i 1:76 107
):
Obviously, the imaginary part is negligible. By expanding the curl, equation (31)
can be reduced to
r2!A + curl
"1
1
@Ay
@x@Ax
@y
!ez i
a
@!A
@z
#= 0
(grad'+ i!
!A ): (33)
1.2.5 Solutions for the scalar potential
The problem for the scalar potential amplitude can be considered as an electrostatic
problem, with no current living the surface of the structure. This corresponds to the
Neumann boundary condition, @'
@njs= 0, assuming an induced current component
normal to the surface is also zero. We will be considering structures with interfaces
(internal as well as external) that are parallel to the z-axis (Fig. 1), with uniform
potentials applied to the edges along z.
z
y
x
y
dmax
A
A
AA
xz
l
Fig. 1. A cylindrical inductor of arbitrary cross-section dmax `. The
cross-section is constant along z.
The solution to (32) is then gradz' = const = Ed in all regions with dierent
conductivity, and the potential dierence is U = Ed `, where ` is the conductors'
13
length. The projection of (33) onto the z-axis is then
r2Az ia
@
@z
@Ay
@x@Ax
@y
= 0
(grad'+ i!Az):
In the case where the potential dierence is applied to the conductor only, the elec-
tric eld becomes a function of all coordinates due to current redistribution. However,
a numerical solution of (32) shows that the redistribution region is comparable with
the layer thickness and the driving electric eld approaches a constant value expo-
nentially over that distance. The eld map for an axial cylinder with nonuniform
boundary conditions is depicted in Fig. 2. The section shown is along the cylinder
from its center to the outer surface. This short redistribution length allows us to ne-
glect the edge eects and take the driving electric eld to be constant in the volume
of the device.
0 2 4 6 8 10 12 14 16 18 200
2
4
6
8
10
12
14
16
18
20Redistribution
conductor
magnetic
Dis
tanc
e al
ong
radi
us
Distance along z-axis
Fig. 2. Driving electric eld distribution along z-axis of a two-layer cylin-
der. A uniform potential is applied to the conductor region at the left edge.
Conductivity of the magnetic layer is 50 times lower then that of the conductor.
For conductors long compared to the transverse dimensions and short compared to
the signal wavelength,
14
dmax ` ; (34)
the translational symmetry in the z-direction can be used to reduce the problem for
Az to 2D:
r2Az(x; y) = ? [Ed i!Az(x; y) ] : (35)
where
?=
0
= 0
2a
(36)
is the eective transverse permeability in SI units.
For example, conductors of a few micrometers in transverse size and a millimeter
in length operating at 1GHz ( = 0:3m) will satisfy condition (34), as would a
0:1mm-diameter wire of 1 cm in length at 100MHz.
Since in (35) the driving eld amplitude, Ed, is constant, it is convenient to work
with a normalized vector potential, eA =Az
Ed, and transform (35) to
r2 eA(x; y) = ?h1 i! eA(x; y)i ; (37)
which has to be solved separately in each conductive region. eA describes the properties
of the device, independent of the external source.
1.2.6 Expression for impedance
Assume a potential dierence is applied to the conductor only. Performing averaging
in (30) over the cross-section of the conductor,
1
S
ZS
!J @!s =
1
S
ZS
!r' @!s i!1
S
ZS
!A @!s ;
and then integrating along the cylinder,Z`
0
SI @z =
Z`
0
@ h'is
@z@z i!
1
S
Z`
0
ZS
Az @s @z;
`
SI + i!
`
V
ZV
Az @V = h'(0)is h'(`)i
s; (38)
we obtain
15
R0I + i!` hAziV = U0;`; (39)
where R0 is the DC resistance and the angle brackets mean averaging over the volume.
The impedance is the proportionality coecient between the voltage and the current,
and from (39) it is
Z = R0 + i!` hAziV
I: (40)
If we assume bias conditions such that the current amplitude I is xed, then the
z-component of the vector potential completely describes the impedance.
In the literature [8] one can nd reactance denition as a ratio of magnetic ux
linkage to the total current. Thus in (40) the ux linkage is
link = ` hAziV =1
S
Z`
0
ZS
Az @s @z =1
S
ZS
@s
Ic
!A @!l =
=1
S
ZS
@s
ZS0
!B @
!s0 = h(x; y)i
s: (41)
Where we have extended the integration path from line a to contour c closed through
innity, where!A1
= 0 (Fig. 3). c is chosen such that tangent vectors !n b, !n0
bare
normal to!A . Therefore the ux linkage is a ux averaged over all possible contours
crossing the volume of the conductor. Expression (39) represents a macroscopic Ohm's
law for harmonic signals taking into account a nite thickness of the device. For such
structures, circuit parameters must be derived directly from the eld distribution.
z
x
y
l/2
-l/2
A
A
c
a
b´
b
→nb
→nb´
Fig. 3. One of the integration contours, c, extended to innity. The magnetic
ux through this contour is equal to the vector potential integrated along the
line parallel to the z-axis.
16
If the bias conditions are such that a xed voltage amplitude is applied to areas with
dierent conductive properties, the simplest approach for the impedance calculation is
to nd the total current, and take the potential dierence averaged over the edges (as
in (38)). Then, the current density distribution completely describes the impedance.
Let us assume that the scalar potential gradient has only one component, gradz' =
Ed = Const, in conductive media. We can then drag the constant eld outside the
integral and normalize by it the current density:
Z =U
I=
Ed`RS
!J @!s
=`P
k
RSk
(Jzk=Ed) @s=
`PkkRSk
1 i! eAk
@s
; (42)
k denotes the regions connected to the voltage source and tilde means normalization
on driving eld. In order to get the impedance, one needs to solve only the equation
for the normalized vector potential.
1.3 Sandwich stripe
Here we illustrate the model with a generic structure of rectangular cross-section. A
schematic of the planar inductor structure is shown in Fig. 4. A voltage is applied to
a magnetic/conductor/magnetic strip along the z-direction, which is also taken to be
the easy axis direction for the magnetization.
y
x“0”
“1”
“2”
w/2z
M→l
Jd1=σ1E
Jd0=σ0E
t1
t0
Fig. 4. A schematic (x > 0) of a magnetically enclosed stripe inductor. Regions
0, 1 and 2 denote the conductor, magnetic lm and air, 0 and 1 are the
permeabilities of the conductor and the magnetic lm, respectively.
17
There are three regions 0, 1 and 2 denoting the conductor, the magnetic lm and
air. In what follows t0, 0 and 0 are the thickness, conductivity and permeability of
the conductor, and t1, 1 and 1 = r0 are those of the magnetic lm. The conductor
width is w, and the length of the structure is `. Equation (33) for the vector potential
has to be solved in every region and the solutions joined at the regions boundaries.
1.3.1 Physical aspects of dimensional reduction
In section 1.2.5 we have shown that accuracy is not compromised by limiting the
driving electric eld to one non-zero component, Ez(t), which results in one non-
zero component of the vector potential, Az(t). For long stripes, with ` w, we
can therefore use the two-dimensional equation (35). For the given geometry, with
t0; t1 w and ux closure at the edges of the stripe, the magnetic moment has a
preferred direction in the plain, which reduces the demagnetizing energy. Since in
practice r 1, the y-component of the magnetic induction is small, By = @A
@x
Bx, which further reduces the problem to 1D. For the sake of clarity, in what follows
A will denote the amplitude of the z-component of the vector potential, with the
subscript k denoting the region:
@2
@y2Ak(y) = 2
kAk(y) kkEd; (43)
where k =1+i
Æk, and Æk = (!kk)
12 is the skin depth in every region. The general
solutions to (43) are
Ak = Ck cosh(ky) +Dk sinh(ky) iEd
!: (44)
The symmetry along y, A0(y) = A0(y), yields D0 = 0.
Since we have By 0, the boundary condition on the normal component of the
induction is satised automatically. We have to require that the vector potential be
continuous across the boundary. The conditions at the two boundaries become8>>>><>>>>:A0(
t0
2) = A1(
t0
2)
1@
@yA0(
t0
2) = 0
@
@yA1(
t0
2)
A1(t0
2+ t1) = A2(
t0
2+ t1)
0@
@yA1(
t0
2+ t1) = 1
@
@yA2(
t0
2+ t1)
(45)
18
1.3.2 Approximation of the external ux
If the external ux constitutes an appreciable portion of the total ux, then A2 must
be taken into account. The diculty in calculating the external ux in idealized
systems (assumed innite in at least one dimension) is the divergence of the vector
potential at innity. The standard approach to avoid this problem is to use a cut-o
distance for the vector potential of the order of the characteristic size of the device,
the length of the stripe in our case.
z
x
y
y=t0/2+t1
l/2
-l/2
Isurf
Fig. 5. A stripe of length ` with surface current density Isurf .
We performed a direct calculation of the 3D vector potential of an innitesimally thin
stripe conductor (Fig. 5):
A3D(x; y; z) =
Z w
2
w
2
@z0Z1
1
@y0Z `
2
`
2
@z0Jsurf Æ(y
0
)p(x x0)2 + (y y0)2 + (z z0)2
:
We can use the 3D vector potential of a current carrying stripe at (x = 0; z = 0),
taking it to represent the functional form of A2(y).
A2 = Cf(y) (46)
= C
"`
2wln
R+ w
R w
2y
warctan
w`
2yR
+ ln
`+ Rpw2 + 4y2
!#;
R =
pw2 + 4y2 + `2;
19
with f yw!0 ! 1 + ln
2`
w
;@f
@y
y
w!0
!
w.
The error in the external ux introduced by this procedure is <10%, which results
in an even smaller error in the total ux. This expression correctly reproduces the
magnetic eld at innity and results in a non-diverging vector potential for a nite
length stripe.
1.3.3 Impedance
Using (44) and (46), the vector potential becomes
A0 = iE
![C0 cosh(0y) 1] ; (47)
A1 = iE
![C1 cosh(1r) +D1 sinh(1r) 1] ; (48)
A2 = iE
!C2f(y): (49)
After substituting (47-49) into the boundary conditions (45), together with approxi-
mation (46) we obtain for the coecients
C0 = D1;
C1 = D1
cosh(0
t0
2) cosh(1
t0
2)
r01
10sinh(0
t0
2) sinh(1
t0
2)
;
D1 = D1
r01
10sinh(0
t0
2) cosh(1
t0
2) cosh(0
t0
2) sinh(1
t0
2)
;
where
D =
coth
0
t0
2
coth (1t1) +
r01
10+w01
1
1 + ln
2`
w
coth
0
t0
2
+
r01
10coth (1t1)
sinh (1t1) sinh
0
t0
2
The coecients are numbered with respect to the region (C0; C1; D1; C2). Coecient
C2 is not given above, since it will not be used in the following discussion.
From (30) the complex amplitude of the total current density is
J0 = E0 cosh (0y) (50)
J1 = E1 [C1 cosh(1y) +D1 sinh(1y)] : (51)
20
Figure 6 shows the current density (50-51) normalized to the driving electric eld as
a function of y.
0.0 0.2 0.4 0.6 0.8 1.00
2
4
6
8
MagneticConductor
Distance from centre, y (µ m)
Nor
mal
ised
cu
rren
t d
ensi
ty |J
/E| (
S)
(a)
0.0 0.2 0.4 0.6 0.8 1.0-2.0
-1.5
-1.0
-0.5
0.0
MagneticConductor
Distance from centre, y (µ m)
Ph
ase
(rad
)
(b)
Fig. 6. Magnitude (a) and phase (b) of the normalized current density jJ=Ej
as a function of y at 500MHz (w = 10m, ` = 1mm, t0 = 1m, t1 = 0:5m,
0 = 5 107S, 1 = 5 10
6S, r = 100).
21
The current in the magnetic lm is a sum of the eddy currents and the driving current,
and is increasingly concentrated at the magnetic/air interface as the frequency is
increased. A signicant portion of this current is in phase with the driving electric
eld. The external magnetic ux can contribute appreciably to the total magnetic
ux in the structure.
Since the magnitude of the driving electric eld is constant, the impedance can
be obtained as the proportionality factor between the voltage and the total current
in the device:
Z =`1
2w1
1 +
q01
10tanh
0
t0
2
tanh (1t1)q
01
10tanh
0
t0
2
+ tanh (1t1)
+ i!`0
2
1 + ln
2`
w
: (52)
This expression includes the DC resistance, reactance, the skin eect and FMR
contributions. 1 = ?
is dened by (36) with Ms=21000 kG, Ha =50 Oe, and
=0.01. The inductance, L = Im(Z)=!, resistance, R = Re(Z), and quality fac-
tor, Q = Im(Z)=Re(Z), are plotted in Fig. 7 as a function of frequency for typical
parameters.
10M 100M 1G0.1
1
10
100
L
R
Q
Qu
ali
ty f
act
or,
Res
ista
nce
(Ω
)
Frequency (Hz)
-1
0
1
2
3
4
5
Ind
ucta
nce (n
H)
Fig. 7. Impedance characteristics of a magnetically enclosed inductor from
(52), with w = 20m, ` = 1mm, t0 = 1m, t1 = 0:1m, 0 = 5 107S,
1 = 106S, 4Ms = 21000G, Ha = 50Oe, = 0:01.
22
The impedance exhibits a resonance at approximately 3 GHz, the FMR frequency of
the ferromagnetic sub-system. The specic inductance is enhanced three-fold over the
air-core value of the bare conductor ( 1 nH/mm), a great advantage in miniaturizing
planar magnetic ux devices.
23
2 Materials: soft ferromagnetic lms
The impedance of magnetic sandwiches has recently become of interest because of
new applications in magnetic ux devices operating at frequencies up to the GHz
range. High frequency operation and compatibility issues impose certain requirements
on the magnetic materials to be used, which are summarized below. With these
requirements in mind, we briey discuss the two main material groups, magnetic
oxides and metallic lms. We conclude the section by describing the preparation and
magnetic characterization of our Fe-based nitrogen containing lms, which are then
used to fabricate planar devices.
2.1 Material requirements
There are two basic requirements to physical properties of the magnetic materials
for use in GHZ inductive devices: high loss-free permeability and compatibility with
under/over-layers in multi-layered device designs. For achieving a high permeability
at high frequencies the following properties are desirable:
high saturation magnetization,Ms. This is a precondition for high permeability.
The permeability employed in most of the designs is the transverse permeabil-
ity (?, hard axis response) in lms of uniaxial anisotropy, which is directly
proportional to Ms;
controllable anisotropy, Hk, in the range 10 50 Oe. At low frequencies ?
Ms=Hk, so high Hk results in too low a permeability. For low Hk the FMR
frequency is decreased: fFMR ' p4MsHk. At FMR the permeability is
mostly imaginary producing high losses;
small FMR line-width. This is commonly dened as the full-width at half-
maximum in the bell-shaped imaginary part of the permeability. In a system
without dissipation the FMR line is innitely narrow. In a real system it can
be rather broad due to various dissipation processes (see section 1.1.2);
high resistivity. Eddy currents are one of the many dissipation channels. How-
ever, in widely used soft magnetic alloys screening often dominates as a magnetic
loss mechanism;
single domain state, for low magnetic loss as well as for reproducibility. Varia-
tions in inductance caused by changes in the domain pattern of the (soft) lms
will most likely be unacceptable for applications;
24
low magnetostriction is preferable, since the fabrication process may result in
stress in the lms leading to stress-induced anisotropy, which limits the perme-
ability.
It is important that the magnetic material should be compatible with the under/over-
layers in multi-layered device designs. The highest impact for integrated inductors, for
example, is seen in scaling down CMOS or BICMOS RF ICs. Process compatibility
in this respect would mean the ability to fabricate the material on various 'imperfect'
substrates (polycrystalline or amorphous insulation or metallization layers, SiO, Al,
etc.), and a restricted process temperature required for other on-chip components.
2.2 Oxides
Ferrites and other oxides are attractive for one reason, their high resistivity. Other
properties of ferrites are disadvantageous compared with those of soft magnetic al-
loys. The saturation magnetization is a factor of 5 lower. Generally, the anisotropy
in oxides is much more sensitive to growth conditions and is harder to control. There
is no simple and robust method of growing soft uniaxial ferrite lms in a biasing eld.
Epitaxial garnets are known to have the smallest FMR linewidths among the magnetic
materials. However, their low saturation magnetization (10 times lower than that of
alloys) and especially the need for single-crystalline lattice-matched substrates, make
garnet lms uninteresting for use in integrated inductors. Polycrystalline ferrite lms
prepared at relatively low temperature have relatively large FMR linewidths. Ex-
change biasing of ferrite lms to achieve a single-domain remnant state has been
demonstrated, but is less straightforward than with alloy lms. However, the high
resistivity of ferrite lms warrants research on integrating them into Si-based tech-
nology.
A common method to prepare ferrite cores for power inductors and transformers
is to use a prefabricated ferrite powder, mix it with a polymer by ball mill rotation,
spin cast or screen print it on a substrate, and nally cure the resulting paste at a
few hundred ÆC [9] up to 800ÆC [10]. The typical relative permeability obtained by
this method is r = 20 30, which is sustainable up to 10MHz [9].
NiZn-ferrite lms produced on glass substrates by a low-temperature (T < 100ÆC)
plating technique, having 4Ms 6 kG and a large anisotropy perpendicular to the
plane, for use in microwave non-reciprocal devices have been reported [11]. This
technique is very promising and it would be interesting to see if the method can be
25
used to produce ferrite lms with properties required in a GHz inductor (see previous
subsection).
Sputtering and pulsed laser deposition have been used to fabricate ferrite lms.
Typically, sputtered as-deposited lms are highly disordered or amorphous [12], and
have undesirable magnetic properties, even spin-glass behavior [13]. The lms often
require a post-deposition annealing at up to 1000ÆC. Pulsed laser deposition of high-
quality (Mn,Zn)-ferrite lms, having bulk magnetic properties, was achieved at 400600
ÆC by a careful selection of buer layers [14]. Also exchange biasing has been
demonstrated in ferrite bilayers [15].
At present, however, there appears to be no readily available techniques for fabrica-
tion of ferrites having the desired properties for use in GHz inductors and compatible
with the Si-based integration. In this respect the situation is quite dierent with soft
magnetic alloys.
2.3 Alloys
Soft magnetic alloy lms can be prepared by a variety of deposition techniques practi-
cally on any surface in various multilayer congurations at low temperature. Permal-
loy as the core material has dominated the eld of planar inductive devices for decades.
Its relatively low saturation magnetization ( 10 kG) and resistivity ( 20 cm),
however, make the material too lossy to be used at above 100MHz. Recent suc-
cess in fabrication of a number of alloy systems with high saturation magnetization
( 20 kG) and high resistivity ( 100 cm and higher) gives a large choice in
designing HF devices. A rigorous classication or a complete survey of the enormous
eld of soft magnetic alloys is beyond the scope of this introduction. We will limit
ourselves to mentioning a few illustrative examples of soft alloy lms developed for
high frequency applications.
The general approach is to start with an intrinsically high moment material, such
as Fe, Co or FeCo and modify, by alloying in additional elements, the structure on the
atomic or nanometer scale in order to achieve the desired soft magnetic properties,
high resistivity, low magnetostriction, high thermal stability etc. Amorphous alloys
have been particularly popular as materials for high frequency inductive applications
([16, 17] and references therein). In these Si, B, C, P, Zr, Nb, etc., are added (at 10-30
atomic %) to promote a glass-like structure with no long range order. The result is
a magnetically soft material (Hc; Hk 1 Oe, Ms 10 15 kG), with a vanishing
crystal anisotropy and magnetostriction and increased resistivity (100 200 cm).
26
Amorphous lms are typically prepared by 'quenching' the material on cold substrates.
They are often annealed at 400600ÆC to ne tune the magnetic properties (see [18],
and references therein). The annealing induces crystallization of nano-sized Fe(Co)-
rich grains embedded in an amorphous ferromagnetic matrix - a morphology known
as nanocrystalline.
The combination of high magnetization( 20 kG), high resistivity (50 100 cm), and excellent soft magnetic properties (Hc; Hk 1Oe) has made nanocrystalline
Fe-X-N compositions (with the alloying element X=Ta, Hf, Si, Zr, Al, Cr, Ti, etc.)
one of the most promising systems for high frequency inductive applications (see, e.
g., [16, 19, 20] and the extensive literature cited therein). Nitrogen atoms intersti-
tially incorporated into the iron lattice promote ne crystalline Fe-rich grains, 10nm in diameter, embedded in a disordered N-rich phase. The size of the grains is
smaller than the exchange length in the material, which can explain the soft magnetic
properties as resulting from vanishing (averaged over the grains) magnetocrystalline
anisotropy. It is essential for achieving soft magnetic properties that the inter-grain
material is ferromagnetic and provides a suciently strong exchange coupling be-
tween the grains. For this reason incorporation of large amounts of nitrogen, leading
to weakening of the inter-grain couplings, is not desirable. Adding various alloying
elements into FeN can improve magnetic softness, thermal stability, etc.
Another member of the nanocrystalline family of magnetic lms is known as gran-
ular lms. These consist of ne Fe(Co)-rich grains mixed with an insulating non-
magnetic phase, typically Al2O3 (see, e. g., [21]). The relative volume of the insulat-
ing phase is critical since Al2O3 breaks the magnetic coupling at the grain boundaries.
When the volume fraction of the magnetic metallic phase is bellow the percolation
threshold, the grains couple through dipolar interactions only and the lms exhibit
hard magnetic properties or even a super-paramagnetic behavior (if the magnetic en-
ergy of a single grain, proportional to the volume, is smaller than kT). Good soft mag-
netic properties in combination with very high resistivity values (500 1000 cm)
can be obtained.
Finally, we would like to mention two more systems, ultra-high moment Fe16N2
lms and high moment high resistivity electrodeposited lms.
High moment materials, being intrinsically the best magnetic ux ampliers, have
traditionally been of great interest. Among these, a delicate (metastable) phase
Fe16N2, rst found in 1972 by Kim and Takahashi [22], has been attracting an increas-
ing attention. Epitaxial Fe16N2 lms obtained using ultra-high vacuum evaporation
have been reported [23]. Single crystal substrates of In0:2Ga0:8As (100) were used
27
to provide a good lattice match. A thin underlayer of pure Fe was rst deposited,
on which Fe16N2 was grown at an extremely low rate, 0.006-0.03 Å/s. Record high
saturation magnetization values were reported, 4Ms=28-29 kG, with the resistivity
30 40cm at room temperature [24]. Deposition of the same phase (4Ms=26-
27 kG) by sputtering under carefully optimized deposition conditions has recently
been reported [25], [26]. The high sensitivity of this phase to preparation conditions
is due to the presence of a number of phases with competing formation energies. The
high magnetic moment is a great advantage in inductive applications. It remains to
be seen, however, whether Fe16N2 can be produced in a way that is technologically
compatible with incorporation in planar device structures.
Electro-deposition is often preferred to sputtering for soft lms because of its low
capital cost, good control of the lms' properties, and most importantly because in
many cases it oers high exibility in fabrication of various patterned structures.
Recently, soft Co-Fe-Ni alloy lms with very high saturation magnetization (20-21
kG) and resistivity (>100 cm) have been obtained by using electrolytes containing
various additives, such as S, C, Mo (see the recent review by T. Osaka, [27]). These
results are very promising and are likely to warrant a conversion from sputter-based
fabrication processes to electro-deposition.
In this work FeN and (Fe90Ta10)N are used as the magnetic layers in mag-
netic/conductor/magnetic sandwiches. Our interest was in the material aspects of
incorporating the lms in a multilayer device rather than in optimizing the properties
of single layer lms. These aspects include variations in the magnetic anisotropy for
deposition on various surfaces, such as SiO and Cu, with various hight gradients.
2.4 Instrumentation for magnetic properties measurement
The experimental techniques and instrumentation used to magnetically characterize
lms in this study are described in this section. These instruments were designed and
built from scratch at Nanostructure Physics (KTH). Setting up and maintaining the
instrumentation was part of this Ph. D. project.
2.4.1 Loop tracer
The function of this instrument is based on Faraday's eect, where an EMF is in-
duced by a magnetic ux change (see dierential form in (9) on page 8). A low
frequency magnetic eld changes the magnetization of the specimen periodically; the
corresponding ux change is picked up by a coil, the output voltage of which is inte-
28
grated and displayed as a function of the driving eld. We have developed a thin lm
loop tracer and optimized it specically for studies of in-plane anisotropy.
Our implementation was inspired by the single-wire-pickup loop tracer with near
monolayer sensitivity described by H. Oguey in 1960 [28]. The changes introduced
in our design exploit advances since the 1960's in low noise amplier electronics and
signal enhancement by a lithographic patterning of the planar pick-up loop. The block
diagram of the instrument is shown in Fig. 8. A sinusoidal driving eld is supplied
by a Helmholtz coil. The pick-up voltage is amplied, integrated and applied to the
Y-input of a real time digital oscilloscope. The signal for the phase compensation
and X-input of the oscilloscope is taken directly from 1 resistor in series with the
driving coil.
Amplifier
Phase compensation
Integrator
R61Ω
Audio amplifier
Function generator
dM/dt
M
H
Scope
Film
Fig. 8. Block diagram of at-coil-pickup M-H loop tracer.
The central part of the instrument is a at two-section pickup coil (g. 9). The
coil plane is oriented along the external magnetic eld, which signicantly reduces
the direct pickup. The two coil sections, with windings in opposition, compensate
any remaining o-axis eld, while summing up the fringing ux from the sample.
When produced lithogracally, this sensitive part of the instrument has two main
advantages. First is the increased sensitivity due to numerous nely dened turns
(2x10 in our case), which simplies design of the amplication circuit and removes
the need for a voltage boosting transformer used in the original design [28]. Secondly,
the ability to use high precision lithography to dene two copper spirals of essentially
29
identical geometry greatly reduces the unwanted pickup.
H
Iind
Fig. 9. Layout of pickup coil.
The phase compensation unit has no mechanical parts or varyometers found in [28].
0Æ 180
Æ phase adjustment is done electronically. No DC restorers have been used
since the integrator, built on an active band-pass lter, is very ecient with respect
to icker noise. Any remaining ham (50 or 60 Hz) was removed using the digital
oscilloscope averaging. The schematic and description of the amplier/integrator are
given in the Appendix.
An additional major advantage of the loop tracer developed here is the free access
to the back surface of the sample. The back side of the substrate is placed on a non-
magnetic rod using a double-sided tape. The rod is then placed through an opening
transverse to the Helmholtz axis with the lm facing the at pickup coil. Thus, a
free in-plane rotation is achieved, allowing a 'real time' evaluation of the angular
dependence of the magnetization loop. With driving frequencies of typically 200-400
Hz, digital trace averaging for less than one second was sucient for good signal
to noise ratio, and the entire in-plane magnetization map could be obtained within
seconds.
2.4.2 Magnetometry -VSM
A home built Vibrating Sample Magnetometer (VSM) was used for characterization of
magnetic lms (Fig. 10). The VSM consist of room temperature eld coils(Hmax<220
Oe), a pair of counter-wound pick-up coils, and a vibrator mechanically connected to
the sample. Following Foner, the inventor of the VSM, we have used a loud speaker
30
for producing the vibrations. A lock-in amplier, a function generator and a DC
power supply complete a magnetometer.
PC
Lock-in Amplifier Vibrator
Pick-up coilsDC field coil
IDC
Power Supply
osc.
Fig. 10. Block diagram of the VSM.
The function generator output is used to drive the loud speaker. A magnetic sample
xed on a non-magnetic vibrating rod induces voltage in a pair of pick-up coils. The
induced voltage depends on the geometry of the coils, amplitude and frequency of
the vibration, and is directly proportional to the magnetic moment of the sample.
This voltage is then phase-sensitively measured using the lock-in, and read in to a
computer along with the DC-eld (solenoid current) value. The instrument is well
suited for studies of soft magnetic lms, and allows sensitive measurements down to
10nm in lm thickness.
2.4.3 HF permeameter
This apparatus is based on a Vector Network Analyzer and a strip-loop xture, and
is used to measure the complex magnetic permeability of lms [29]. The complex per-
meability data contain information about the inductive properties of the lms as well
as dissipation (also known as magnetization relaxation or Ferromagnetic Resonance
loss).
Fig. 11 shows a schematic of the measurement setup. A computer-controlled
3GHz impedance analyzer HP8714C is used to measure the complex reection coef-
cient of the xture containing the sample under test. The xture consists of a copper
strip loop mounted directly on an SMA connector and a standard N to SMA
31
adapter, which is then connected to the impedance analyzer reection port. A
Helmholtz coil is used to apply an external DC magnetic eld. The same loop is
used both to generate the excitation eld and to detect the sample's response. The
loop impedance, obtained from the reection coecient, is recorded with and without
the sample in the loop as a function of frequency. The recorded change in the loop
impedance is then converted into complex susceptibility or permeability spectra.
HP8714C
N-JACK SMA-PLUGN-PLUG toSMA-JACK
adapter
Helmholtz coil
Sample
Striploop
Hdc
I
Film
w
h
Loop section
Hdc
Fig. 11. Schematic of the setup.
The magnetic eld in the center of a strip loop of width w carrying current I (see
inset to Fig. 11) is H = kHI
w; where a geometrical factor, kH =
2
arctan
w
h
for
innitely long loop of width w and height h (w = 6:5mm; h = 1:2mm; kH = 0:88 in
our case). The total length of the measuring loop was kept below 10 mm to ensure
that the loop is a lumped element even at the highest frequencies used.
The principle of the method can be understood by considering the following. The
ux due to a magnetic lm enclosed by a strip loop is [28]
= 0HV
w;
where 0 is the permeability of free space, is the susceptibility of the lm, V is the
volume of the lm and 1 is a geometrical correction term, which, in general, is
32
a function of the lm-coil geometry. Once the value is computed for given loop
dimensions, it does not vary appreciably (within 3%) with the size of the lm. We
can write for the impedance induced by the ux :
Z =V
I=
1
I
@
@t= i!0
V
w2kH
or separating real and imaginary parts:
L = 00tmk
R = !000tmk
where k =Sm
w2 kH is a geometrical factor of the order of unity, Sm and tm are the
area and thickness of the magnetic lm, respectively. Thus, the change in inductance
and resistance of the loop when the sample is inserted is proportional to the real
and imaginary parts of susceptibility, respectively, scaled by the lm thickness. Since
= 1 and 1, the real and imaginary parts of the impedance are similarly
related to the permeability, Z = R+ i!L = k!0tm(00+ 0).
2.5 Fe-X-N lms
In this section we discuss the preparation and properties of Fe-based nitrogen con-
taining lms, illustrating the issues relevant for their incorporation in planar devices,
such as anisotropy and dissipation.
2.5.1 Magnetic properties of Fe-N and Fe-Ta-N
As was discussed above the magnetic properties of nanocrystalline Fe N (Fe X N) are sensitive to the shape and size of the grains, and to the nature of the
grain boundary material. The microstructure is inuenced by the reactive sputtering
process parameters, such as the substrate temperature (T ), nitrogen partial pressure
(pN2), total gas pressure (p), output power of the magnetron (P ), as evidenced by
many detailed studies on the subject (see section 2.3). Fig. 12 illustrates the variation
of the coercivity and resistivity of our reactively sputtered FeN lms with the nitrogen
partial pressure in an Ar +N2 gas mixture, pN =pN2
pAr+N2
100%. The coercivity along
two orthogonal in-plane directions are denoted Hce (easy-axis) and Hch (hard-axis),
and both show a rapid decrease already at pN 1% and a steady rise at high nitrogen
concentrations.
33
0 2 4 6 8 10 12 140
20
40
60
80
ρ
ρ (
µΩ
cm
)
pN (% )
0
10
20
30
40
50
Hc
Hce
Hch
Fig. 12. The coercivity and resistivity of FeN lms versus nitrogen partial
pressure.
The incorporation of nitrogen into iron lms can generally be divided in two stages.
Below the interstitial nitrogen solubility limit of the single Fe(Ta) crystalline phase
(pN ' 1%), N acts as a 'grain rener'. The softening of the lms in this regime can
be explained in terms of a vanishing local magnetocrystalline anisotropy. At high
nitrogen concentrations the soft magnetic behavior is lost progressively in spite of the
ne nanostructure. This is due to weakening of the inter-granular exchange coupling
often attributed to a transformation of the amorphous matrix into a lower Tc phase
with addition of excess N [19].
The resistivity of the lms increases almost linearly with increasing pN . Such an
increase may reect two main indirect contributions to the scattering of the conduction
electrons: one being grain boundary scattering due to a decrease in the grain size and
increase of the volume fraction of the inter-granular amorphous-like phase; the other
being a lattice distortion scattering in the grains, due to the nitrogen incorporation.
The coercivity of FeTaN (Fig. 13) has a similar broad minimum. However, the
absolute minimum is shifted to higher pN .
34
0 2 4 6 8 10 12 140
20
40
60
80
ρ
ρ (
µΩ
cm
)
pN (% )
0
10
20
30
40
50
Hc
Hce
Hch
Fig. 13. The coercivity and resistivity of FeTaN lms with 10w=o of Ta versus
nitrogen partial pressure.
FeN lms sputtered at pN = 7% exhibit similar properties to FeTaN lms prepared
at pN = 11%. Both systems show a weak in-plane anisotropy in this range of pN .
The resistivity of FeTaN is larger than that of FeN for low pN (due to the Ta
alloying), but the two become comparable by pN 5%. Thus, we nd no signicant
dierences in properties between the two systems in the range pN = 4 12%. The
choice of high N contents (10 12%) may seem obvious in view of high frequency
applications. We nd, however, that high pN makes the material more sensitive to
deposition conditions, such as the angle of incidence (see next section).
Both FeN and FeTaN are found to become softer with lowering the total sputtering
gas pressure and with increasing the magnetron output power. The lowest pressure
needed to maintain a stable plasma in our deposition system was 2:5 103Torr.
High magnetron power can lead to an increase of the substrate temperature [30] during
deposition, sometimes causing hardening of the material or melting of the mask when
devices are made using the lift-o technique. We therefore limited the magnetron
power to 300W (15W=cm2).
35
2.5.2 Anisotropy due to oblique deposition
Magnetic lms deposited on tilted substrates possess properties dierent from those
of normally (on-axis) deposited lms. The incidence angle, , at a given point is
dened as the angle between the normal to the substrate and the line connecting
the point with the center of the target (g. 14). Films thus deposited are found to
posses a uniaxial in-plane anisotropy with the easy axis directed perpendicular to the
deposition plane (containing the substrate normal and the target center).
Averageatom fluxdirection
Ha
θ
Fig. 14. The angle of incident atom ux to the normal and corresponding
anisotropy direction.
M H traces for magnetic lms sputtered at pN = 1% are shown in Fig. 15a for
three dierent incidence angles. The normal incidence lms ( = 0) show no preferred
in-plane orientation of the magnetization. The lms deposited at 20Æ develop a
weak in-plane anisotropy. The easy-axis coercivity, Hce, increases while that for the
hard axis, Hch, decreases, and a uniaxial anisotropy with Hk 10Oe develops. The
lms sputtered at = 60Æ show Hce 200Oe and Hk 400Oe (the hard axis loop
for 21Æ incidence is shown for comparison, Fig. 15b). This growth induced anisotropy
leads to more than an order of magnitude reduction in the transverse permeability,
which is responsible for the inductive response of the lm.
36
-50 -40 -30 -20 -10 0 10 20 30 40 50
-1.0
-0.5
0.0
0.5
1.0
M/M
S
H (Oe)
e h
00
210
(a)
-400 -300 -200 -100 0 100 200 300 400
-1.0
-0.5
0.0
0.5
1.0
M/M
S
H (Oe)
e h
210
600
(b)
Fig. 15. M-H curves for Fe-N (1%) lms deposited at (a) = 0Æ, 21Æ, and (b)
21Æ, 60Æ incidence angles.
Two potential mechanisms of this anisotropy are discussed in the literature (see, e.g.,
[17]). The rst is the shape anisotropy of magnetic columns, which are typically
37
present in lms deposited at oblique angles due to the self-shadowing eect [31, 32].
This eect has recently been analyzed in detail for Co lms on underlayers deposited
at oblique angles [33] and was found to result in up to 1 kOe of anisotropy. Another
possible origin of the oblique-growth induced anisotropy in magnetic lms discussed
in the literature is due to magnetostriction. The later is less likely to result in such
high anisotropy values (Hk 1 kOe).
Films containing dierent amounts of nitrogen have dierent sensitivity to oblique
deposition. This is illustrated in Fig. 16 by xing at 21Æ and varying the nitrogen
partial pressure. The hard axis loops, measured for lms corresponding to pN =
1; 2; 4; 8% demonstrate an increase in anisotropy from 10Oe to 100Oe. The easy
axis coercivity, Hce, showed a slight increase from 5Oe to 15Oe on increasing pN .
-150 -100 -50 0 50 100 150-1.5
-1.0
-0.5
0.0
0.5
1.0p
N = 1% 2% 4% 8%
Incident angle 21o
M/M
S
H (Oe)
Fig. 16. Hard axis loops for FeN lms, sputtered at 21Æ and dierent pN .
The increase in Hce and Hk with pN is dramatic for large incidence angles. The data
for = 60Æ are shown in Fig. 17.
38
0 1 2 3 4 5 6 7 8 9 10 11 120
100
200
300
400
500
600
700
800
PN / P
tot (% )
HC
Hk Hce
Fig. 17. Hce and Ha for FeN deposited at = 60Æ versus nitrogen partial
pressure.
Here we see a rapid hardening of the lms for nitrogen partial pressure 0-2%, with
the coercivity approaching 200Oe and the anisotropy eld 600Oe. Further increase
of pN does not inuence Hce and leads to a gradual increase in Hk. This trend is
opposite to that of the normal incidence lm. Thus, the soft properties of normal
incidence lms is in no way a guarantee of magnetic eciency of the material used in
a device, where deposition on tilted surfaces (microstrip edges) is required.
2.5.3 FMR susceptibility
We have measured the high frequency magnetic response of the lms using the tech-
niques described above (see section 2.4.3). To illustrate the variation in the response
of the lms, we show in Fig. 18 the complex susceptibility of two FeN lms deposited
at approximately 10Æ and 15Æ, represented with open and closed symbols, respectively
(squares - real component, circles - imaginary component).
39
0.4 0.5 0.6 0.7 0.8 0.9 1 2 3 4-600
-300
0
300
600
900
1200
1500
Fe-N(4.5%) 4πMS=21kG
Su
scep
tib
ilit
y
frequency (GHz)
Fig. 18. Complex susceptibility versus frequency for FeN(4.5%), =10Æ (open
symbols) and 15Æ (closed symbols).
The measured values of the initial permeability are 600 (10Æ) and 360 (15Æ). The real
part of the permeability goes through zero at the FMR frequency, 2.2 GHz and 2.8
GHz, respectively. Theoretical tting of the susceptibility spectra using (36) yields
the following parameters of the material: Hk=33 Oe, 4Ms=21 kG and =0.018 for
=10Æ and Hk = 55Oe, 4Ms = 20 kG and = 0:012 for =15Æ.
40
3 Applications: GHz inductors
Electronic products continue to undergo a rapid reduction in size and weight. An in-
creasing demand for communication products has been motivating research on mono-
lithic integration of radio components and systems. The fundamental electronic com-
ponent least compatible with silicon integration is the inductor, which is required for
implementation of lters, oscillators and matching networks. The dominating inte-
grated inductor design is an air-core spiral. Spirals are inecient magnetically, rela-
tively large, and often perform poorly in silicon integrated circuits. Use of magnetic
lms as ux-amplifying components allows for smaller inductors. Magnetic inductor
designs exist with most of the ux contained within the magnetic lms, which reduces
stray elds and the associated losses. After summarizing the current state of research
in the eld, we discuss the material and design issues involved in developing ecient
magnetic lm inductors. We then continue by analyzing one specic implementation
- a magnetic sandwich strip inductor.
3.1 Background
Saleh and Qureshi [34] proposed a magnetic thin lm inductor consisting of a square
spiral deposited between two Permalloy lms, 0.3 m thick on a glass substrate.
The inductor operated at 10 MHz and had a quality factor Q '18 with a 15%inductance enhancement over the free space value. In spite of the small gain in the
specic inductance, this work is still relevant for high-frequency magnetic inductor
design because of the use of the transverse permeability (AC eld transverse to the
equilibrium magnetization), as well as the segmentation of the magnetic lm to reduce
displacement currents due to the distributed conductor-to-lm capacitance. Soohoo
[35] gave a basic magnetic analysis for a magnetically sandwiched spiral and a mag-
netic lm core solenoid. He also presented a prototype inductor with copper lm
winding 'wrapped' around a Permalloy lm/glass(Si) substrate, which showed a 700-
fold enhancement in the specic inductance (no frequency or quality factor data were
provided).
Over the last 10-15 years there have been numerous eorts to fabricate an ecient
IC-compatible magnetic inductor and extend its operating frequency range from 1-
10 MHz to 100-1000 MHz. Shirae and coworkers have implemented a number of
structures, starting with planar coils embedded in SiO and sandwiched between two
Permalloy lms [36]. This design did not yield an ecient inductor (Q 1) and
41
the resonances at a few tens of MHz were attributed to the distributed coil/SiO/lm
capacitance in the structure. Going from magnetically sandwiched planar coils to
magnetically sandwiched conductor strips (Py/Cu/Py trilayers) patterned into planar
coils was found to improve the high-frequency characteristics of the devices: Q 3
at 100 MHz. The gain in the specic inductance due to the magnetic cladding was
however 'too small' [37]. In this regard the importance of magnetic material at the
edges of the conductor (anges) to achieve ux closure was pointed out [38]. A
gain in inductance up to a factor of 4 with Q2-3 at 100 MHz was obtained by
Yamaguchi et al. [39],[40] for Permalloy-coated conductor strips, with and without
magnetic closures at the edges, formed into meanders and spirals. Korenivski and
van Dover [41] have studied Cu strips sandwiched with Permalloy and Co-Nb-Zr,
with and without anges at the edges. Up to 7-fold inductance enhancements over
the air-core value (100 nH/cm linear inductance density) with Q 2 at f 250 MHz
were observed for 10-50 m strips. Another geometry, a solenoid, was studied by
Shirakawa and coworkers, who have demonstrated 10-fold inductance gains with Q
= 10-15 at f = 10-100 MHz for planar solenoids with laminated amorphous magnetic
cores [42],[43]. Two recent papers discuss the use of high moment, high resistivity Fe-
Ta-N and Fe-Al-0 lms (rather than Permalloy) in planar inductors, the trend that
will certainly continue. The design, however, was chosen such that in one case the
frequency range was limited to about 20 MHz [44] and in the other case the gain in
inductance was below 15% [45, 46].
3.2 Design
There is a number of ways one can incorporate a magnetic lm into a magnetic
ux device. These will vary in eciency, frequency range of operation, and ease of
fabrication. Here we briey argue advantages and disadvantages with the common
inductor designs for the GHz frequency range. We conclude the section by discussing
why a magnetic/conductor sandwich is a promising system for this application.
3.2.1 Spirals and meanders.
As mentioned above, there have been numerous attempts to minituarize a spiral
inductor by sandwiching it with magnetic lms. The main advantage of this structure
is that a well developed integrated fabrication process exists. However, there are
numerous disadvantages with this design:
42
the spiral is a compromise between the need for a planar layout and a solenoid,
and it is not very ecient magnetically. An extra metallization level is required;
insulation is required when coils are sandwiched between metallic magnetic
lms. This introduces a distributed coil-to-lm capacitance, which is strongly
geometry dependent and is recognized to be a limitation for operation at 1GHz;
the structure contains relatively large air gaps, which is undesirable from the
basic magnetic analysis point of view;
planar coils produce large out-of-plane elds, which in turn produce in-plane
eddy currents in the magnetic lms and Si substrate (Fig. 19). In-plane sec-
tioning of the magnetic lms can be used to reduce eddy currents in the magnetic
lms, but this may cause additional demagnetizing problems.
hard-axis (rotational, fast) permeability is preferred over easy-axis (switching,
domain wall motion, slow) permeability. In this regard biasing the magnetic
lms is not straightforward since the eld of a spiral is biaxial. A solution to
magnetically cover one-half of the coil [34] is available, though at the expense
of reducing the magnetic volume by 50%.
H
J
J
Jind
Si
Fig. 19. Large z-component of the magnetic eld of a spiral induces in-plane
eddy currents in metallic ferromagnetic lms.
43
3.2.2 Planar solenoids
A planar solenoid can be formed by plating the patterned lower conductor layer,
covering it with polyamide or SiO, depositing the magnetic core of desired geometry
with another layer of polyamide/SiO, arranging for metal via contacts and nally
plating the patterned top conductor layer. The advantages with this geometry are:
a well-developed fabrication process;
magnetically most ecient;
biasing the magnetic core is straightforward;
most of the eld produced by the solenoid is in the plane of the core, so eddy
currents can be controlled by varying the thickness of the core (lamination if
necessary).
The disadvantages are:
large distributed capacitance in the structure;
relatively complex structure with multiple via contacts, which may add up to
a high resistance of the coil and lead to low Q. It is important to note that
the inductors used at 1GHz are often of only several nH, a value that can
be realized with a magnetic core solenoid having a single turn. A single-turn
solenoid is essentially equivalent to a magnetic sandwich strip inductor.
3.2.3 Sandwiched strip
A sandwich strip inductor is a thin lm multilayer having a conductor strip, typically
made of Al or Cu, 0:1 1m thick, 10 20m wide and 1mm long, sandwiched
between two magnetic lms, with optional insulation layers between the conductor
and the magnetic lms. In addition, ux closure can be achieved by incorporating
magnetic anges at the edges of the strip, ux-linking the magnetic lms. A magnetic
sandwich strip with a 5 10-fold inductance enhancement over the air-core value can
substitute a typical RF spiral, and thus make free a lot of chip area. If needed, longer
strips can assume a spiral or a meander layout to achieve large inductances. The
structure has the following advantages:
simple in fabrication;
44
biasing the magnetic lms is straightforward;
the external magnetic ux is a small part of the total ux. The external eld is
in the plane of the substrate, therefore a reduced dissipation in Si is expected;
the excitation eld produced by a current in the conductor is mostly in the
plane of the magnetic lms, so eddy currents can be controlled by varying the
thickness of the lms;
no insulation is required, since the dierence in the conductivity between the
conductor (Al, Cu) and currently available high-resistivity soft alloys is 100.
This eliminates the unwanted capacitance.
Disadvantages:
anges are desirable for magnetic eciency. Incorporating anges adds addi-
tional fabrication steps and is typically done by making the top magnetic lm
somewhat wider to cover the conductor strip. The process can result in some
additional stress in the magnetic lm at the edges and, hence, anisotropy. This
problem, however, is routinely dealt with in making writing heads in magnetic
recording. The latest advances in electrodeposition of high moment high re-
sistivity lms (see section 2.3) are promising, since the technique is known to
be eective in achieving magnetic ux closures in micro-devices (such as write
heads in magnetic recording).
3.3 Device fabrication
In this section we describe the fabrication and characterization of magnetic sandwich
inductors. We conclude by discussing the circuit characteristics of the devices and
the issues limiting their high frequency performance.
3.3.1 Lithography process
The inductor is a strip of width 2-100 m and length 1250 m (center-pad separation)
xed at the pitch of the RF probe. A scanning electron microscope (SEM) image in
Fig. 20 shows a set of stripe inductors with widths 5-20 m.
45
Fig. 20. SEM image of an inductor set.
The sandwich consists of three layers. The bottom and top magnetic lms have the
same thickness (typically 100-200 nm). The conductor layer is 400-1000 nm thick.
The substrate is silicon with a 1 m thermal oxide layer.
Normally, a sandwich with ux closure (with an overlap of the magnetic lms at
the edges) is produced using three mask steps as illustrated in Fig. 21 (left to right).
Mask N1 Mask N2 Mask N1
Fig. 21. Fabrication of a sandwich strip with ux closure using three mask
steps.
We have fabricated inductors with ux closure using only one lift-o mask.A two-layer
resist system is used, with a PMGI low contrast resist as the bottom layer and a high
contrast resist, ZEP, as the top layer. The mask after development had an undercut
46
of 0.5-1.5 m as schematically shown in Fig. 22. We made use of the dierence in the
shadow depth for evaporation and sputtering. An e-beam evaporation source placed
at a distance of 20 cm from the substrate was used to produce a sharp edge mapping
of the top resist layer (solid arrows in Fig. 22). Sputtering, on the other hand, results
in material deposition in the open as well as the undercut regions (dashed arrows in
Fig. 22).
Fig. 22. Schematic of the lift-o process.
The following sequence was used:
1. spin the two-layer resist (PMGI SF71, ZEP5202 diluted 1:2), expose3 and de-
velop4 the pattern. The development time for the bottom resist layer5 is slightly
longer, in order to create 1 m undercut;
2. sputter 100-200 nm thick FeN or FeTaN lm, evaporate 400-500 nm thick Cu
lm, sputter FeN or FeTaN (see section on page 51 for details);
3. lift-o6.
The pattern was dened using an e-beam writer. Test patterns written with the dose
of 100 C=cm2 and dose modulation 50-150% were used to determine the proximity
correction. An optical image of a typical mask with a large undercut is shown in Fig.
23.
1At 1000 rpm it gives 600nm thickness; (soft bake 200ÆC 10 min on hot plate is needed).2At 3000 rpm it forms 90 nm thickness; (soft bake is 160ÆC 10 min on hot plate).3At 30 kV dose is in the range 80-100 C=cm2; 60 m and 120 m e-beam apertures give
reasonable exposure time.4Develop top layer 35s in P-xylene; blow dry.5Develop bottom layer 4.5min in 60%MF322 + 40%H2O; rinse with Distill water; blow dry.6with the Shipley 1165 Remover in a water bath of 55-60ÆC; rinse with Distill water; blow dry.
47
Fig. 23. Optical microscope image (top view) of a two-layer mask for 2m
width inductor. The dark area is SiO, the top resist layer is transparent (red
lter used).
An optical image in Fig. 24a shows a Cu/FeTaN sandwich with a FeTaN ange
produced using the above mask. The cross-section of a FeTaN/Cu/FeTaN sandwich
produced using a mask with a small (0.5 m) undercut is shown in Fig. 24b. Ap-
preciable sputter deposition on the bottom resist wall in this case can result in the
ange wrapping up during the lift-o. Fig. 24b demonstrates that a thin magnetic
lm can wrap up on the edges. This can be as a result of either too small undercut
and remaining resist on the substrate or strong penetration of the sputtering.
In order to avoid edge curling deeper undercuts have to be used. These, however,
should not be too deep as that would lead to weak top-layer resist bridges (see section
3.3.2).
48
(a)
(b)
Fig. 24. (a) Optical microscope image (top view) of Cu/FeTaN; (b) SEM cross-
section of FeTaN/Cu/FeTaN produced with 0:5 m undercut depth.
3.3.2 Film deposition
In this section our deposition system is described, in setting up and maintaining/upgrading
which I took an active part. Evaporation and sputtering steps in the lift-o process
are discussed.
3.3.2.1 UHV system The system we use for making lms has a UHV design
with a load lock, bakable to 200ÆC (Fig. 25). It is turbo/TSP pumped and has a
built in manipulator for doing angle depositions. The pressure is measured at dierent
locations: in the load lock (thermocouple gauge), at the chamber bottom (ion gauge)
and top (combined ion/thermocouple gauge). A pirani gauge is used for oxidation
inside the chamber.
49
MDX 500HVpowersupply
O2
-+
-
+
N2
Ar
~
DepositionmonitorXTM2
SKY945
Load lock
Piranigauge
Thermo-couplegauge
Combigauge
Iongauge
Air inlet
Fig. 25. Schematic of UHV system with standard graphic symbols used in
vacuum technology.
There is one ve-pocket e-Gun and two 2 inch sputter sources (one regular magnetron
source and one specialized for magnetic targets). The system is set up for doing in-situ
oxidation and reactive sputtering (O2; Ar;N2). The gas ow is controlled manually
with leakage valves and a turbo pump shutter.
3.3.2.2 Reactive magnetron sputtering Reactive sputtering is a method of
depositing lms of composition dierent from that of the target, and consists of adding
to the sputter gas (typically Ar) a reactive gas (typicallyN2 or O2). Nitrogen (oxygen)
in the plasma reacts with the target material (say Fe) and is incorporated in the
50
deposited lm. The amount of nitrogen in the lm is controlled by varying the partial
pressure of N2 in N2Ar plasma. We have used AJA A300 series magnetron sources
with Advanced Energy MDX500 magnetron drives.
Fe and Fe9Ta1 targets have been used. The total pressure was kept at 3mTorr
with 0 12% partial pressure of nitrogen. Depositions were made at ambient tem-
perature. During sputtering (typically 7 min for a 200 nm lm) the temperature is a
function of magnetron power and can increase to 100ÆC, which can result in melting
of the mask. Therefore, the power was restricted to 300W , corresponding to maxi-
mum deposition rate of 5 Å/s. Sputter deposition in the (large) undercut region is
demonstrated in Fig. 26 for a thicker (500 nm) sputtered Al lm (Al allowed for
clean cross sections, sputtered iron lms had a similar prole in the undercut region).
Fig. 26. Cross-section of a mask with an Al lm sputtered at 300W .
3.3.2.3 Electron beam evaporation Electron beam heated sources dier from
resistance heated sources in two ways: the heating energy is supplied to the top
of the evaporant by the kinetic energy of a high current electron beam, and the
evaporant is contained in a water cooled cavity or hearth. As a result the source
of evaporated material can be conned to a small spot. The small spot combined
with the line-of-sight directional deposition makes e-beam evaporation suitable for
producing patterned structures with boundaries well dened by the edges of the lift-
o mask.
We have used a Thermionics ve pocket e-Gun system (Model 100-0050) for
depositing (through mask) the conductor lm (Cu, typically 3 108 Torr base
pressure, 7-10 Å/s rate). The Cu layer thus deposited maps exactly the mask layout
(Fig. 27).
51
Fig. 27. Cross-section of a mask with evaporated Cu. Thickness of the bridge
is 90 nm, the undercut is 0:5 m.
A gradual buildup of the material at the edge of the mask leads to a gradual reduction
in width of the lm during deposition, resulting in an edge slope of about 80Æ.
A 5nm thick capping layer of gold was evaporated on the top of the magnetic
layer to ensure a good electrical contact for impedance measurements.
3.4 GHz inductors
In this section we describe the measurements and discuss the performance of magnetic
sandwich inductors.
3.4.1 Impedance measurement: calibration and deembedding
A four-point technique was used for DC resistivity measurements of the lms. The
resistivity of FeN lms was in the range 20 80 cm, that of Cu 2.4 cm.
For impedance measurements we have set up a xture with an XYZmicro-positioning
stage, a Cascade 12GHz xed-pitch probe, a stereo-scope for sample positioning
and an HP8714C network analyzer (Fig. 28). The real and imaginary parts of the
impedance were obtained from measurements of the reection coecient, = x+ iy,
in the 30MHz 3GHz frequency range:
Re (Z) =100y
(1 x)2+ y2
52
Im (Z) =50
1 x2 y2
(1 x)
2+ y2
:
Fig. 28. The experimental setup for HF impedance measurements: XYZ micro-
positioning stage with the sample holder, 12GHz probe, stereo-scope, HP8714C
network analyzer, PC.
The measurements are controlled by a PC using LabView. The external magnetic
eld is applied using a Helmholtz coil positioned around the xture (not shown).
The following deembedding procedure was used. The network analyzer was cali-
brated to the probe plane (PP in g. 28). A correction was made for the electrical
53
delay corresponding to the probe length. The measured impedance was modeled as a
sum of the probe, contact (probe to pads), xture (coupling to Si),and Device Under
Test (DUT) impedances (see Fig. 29).
ZDUTRcontZprobe
Zfixture
Fig. 29. Schematic of the xture impedance.
The contact resistance was evaluated from the low frequency limit using a set of
strips of varying width. The DC-limit resistance scaled linearly vs. the inverse strip
width with a 0:2 0:5 oset, which was attributed to the contact resistance of the
probe/pads (Fig. 30).
0.05 0.10 0.15 0.200
2
4
6
8
10
12
14
Rcont
= 0.24ρ l/t =59
Rexp
Rcont
+ρ l/tw
1/w (µ m-1)
R (
Ω)
Fig. 30. DC resistance of a set of strips.
54
The Cascade probe introduces a series impedance, which was determined using Cu
test strips. The impedance of the strips of varying width could be accurately modeled
and compared with the measurements. The correction for parallel xture impedance,
Zfixture, due to the measurement conguration was found to be negligible for strips
5m and wider (see Fig. 31).
0.1 1-6
-4
-2
0
2
0.1 1
100µm
5µm
5µm
w=2µm
f (GHz)
∆R
(Ω
)
-1.0
-0.5
0.0
0.5
1.0
100µm
w=2µm
∆L
(n
H)
Fig. 31. The measured impedance of Cu test stripes with the series impedance
and the calculated impedance of the stripes subtracted.
3.4.2 HF performance
The measured inductance, L = Im(Z)=!, is plotted in Fig. 32 as a function of
frequency for dierent inductor widths, unbiased and in an externally applied eld of
35 Oe.
55
0.1 10
1
2
3
4
5 µ m
10 µ m
20 µ m
50 µ m
100 µ m
L (
nH
)
f (GHz)
H ~ 35 Oe H = 0
Fig. 32. Inductance as a function of frequency for 5, 10, 20, 50, and 100 m
wide strips, unbiased (dashed lines) and biased in 35Oe (solid lines).
The contribution of the anges to the magnetic inductance becomes smaller as the
width of the strip is increased. The measured inductance of the 50m strip is essen-
tially the value expected for a sandwich with perfect ux closure, hence the model for
the impedance of a closed magnetic structure should apply (see (52) on page 22 and
equivalent circuit approximation in appended paper V). The inductance and quality
factor for the 50m width strip measured in three biasing elds are shown as func-
tions of frequency in Fig. 33a and 33b, respectively, along with the theoretically tted
curves. Fixing the geometrical parameters at the measured values, a good t can be
obtained by varying the permeability and damping parameter.
If we use the same parameters to t the impedance of the 10m strip, the deviation
from the predicted performance is signicant (see Fig. 34). In order to obtain a good
t not only the permeability has to be signicantly reduced (by roughly a factor of
two) but the dissipation constant has to be signicantly increased: from =0.028
(consistent with values 0.020-0.025 measured on similar test lms using the technique
56
of 2.5.3) to 0.06.
(a)
0.1 10.8
1.0
1.2
1.4
1.6
H3=160 Oe
H2=84 Oe
H1=42 Oe
L (
nH
)
f (GHz)
experiment theory
(b)
0.1 1.0
1
10
H1
H2
H3
Q
f (GHz)
experiment theory
Fig. 33. L (a) and Q (b) versus frequency for a 50 m wide inductor in three
biasing elds. Solid lines are theoretical ts using (52).
The reduction in the eective permeability for narrow strips can be attributed to
the increasing inuence of the incomplete ux closures at the edges. However, the
57
increase in the damping constant is not expected to directly depend on the width of
the strip.
(a)
0.1 10
1
2
3
4
5
H1=42 Oe
H3=160 Oe
72 Oe
260 Oe
L (
nH
)
f (GHz)
experiment theory theory
(b)
0.1 1.00.1
1
H3
H1
260 Oe
72 Oe
Q
f (GHz)
experiment theory theory
Fig. 34. L (a) and Q (b) versus frequency for a 10m wide inductor in two
biasing elds. Solid lines are theoretical ts using (52) with the parameters
from Fig. 8. Dashed lines are ts with assuming a reduced permeability and
increased damping constant (see text).
58
A probable cause of the increased dissipation is that an increasing portion of the
magnetic ux leaks through the conductor near the ange, causing screening currents
in the conductor. This dissipation mechanism is not accounted for in the 'closed-ux'
model (52) but known to be the dominating loss mechanism in sandwiches without
ux closure [appended paper IV]. The performance of the inductors at 1 GHz is
summarized in Fig. 35. A 2-fold inductance gain with Q 3 was obtained with the
20m width inductor. By varying the width of the device the inductance gain can
be compromised for higher quality factor.
0 20 40 60 80 1000
1
2
3
4
5
6
7
L (
nH
), Q
w idth (µ m )
L Q
Fig. 35. Inductance and quality factor at 1 GHz versus inductor width.
3.4.3 Flux closure at the edges
From the low frequency limit of the inductance (Fig. 32, solid lines) one can determine
the magnetic lm contribution, which excludes any dissipation or resonance eects
at high frequencies. The total inductance in this limit, L = L0 + Lm, is the sum of
the air-core inductance of the strip, L0, and the contribution due to the magnetic
lm, Lm. In Fig. 36, Lm is plotted versus the strip width. The experimental data
deviate from the ideal 1=width (dash-dotted line) behavior expected when there is
perfect magnetic ux closure at the edges. The observed magnetic contribution to the
59
inductance is below the theoretical value for narrow strips, while it approaches the
expected values for wide strips. This behavior indicates an incomplete ux closure at
the edges, which plays a progressively larger role as the width of the strip is reduced
[41].
10 100
0.1
0.2
0.3
0.4
0.5
0.60.70.80.9
1
2
3
4
5
100
50
20
105
2
L
m (
nH
)
w idth (µ m )
FeN(4%) exp. models, µ
r=390:
g=44nm, wf=0.1µ m
g=0 g=t
c
Fig. 36. The magnetic contribution to inductance, Lm. The expected in-
ductance of a 'closed' magnetic structure (dash-dot line) and 'open' structure
(dashed line).
3.5 Prospectives
We have demonstrated a signicant inductance gain at 1 GHz by using magnetic/conductor
sandwiches. Several issues should be addressed in the future. The use of soft lms
with resistivities of 100 -cm and higher should allow thicker magnetic layers in
the sandwich, hence larger magnetic ux and inductance. Use of thicker conductor
layers, provided the edge ux closures are not thereby degraded, should yield higher
quality factors. Control of the properties of the magnetic lms at the strip edges
needed for ecient ux closure is crucial for both improving the inductance gain and
performance in the GHz range.
60
We see no principal limit on the inductance gain one can achieve in a magnetic
sandwich, even with the currently manufacturable materials. The magnetic volume
can be increased, and screening controlled, by using laminated magnetic lms. E-
cient magnetic closure must of course be maintained.
When the 'extrinsic' dissipation issues of screening and incomplete ux closure
are solved by using optimum device parameters, the 'intrinsic' dissipation in the fer-
romagnetic material (usually described by a phenomenological damping constant) is
seen as the main factor limiting the device performance. Although magnetic relax-
ation is a long established area of solid state physics, the understanding of relaxation
in the technologically attractive lms we have discussed is in its early stages. Ulti-
mately, one would like to know the microscopic and microstructural mechanisms of
the magnetization dissipation and, more importantly, be able to control it.
61
4 Appendix
Combined preampleer and integrator circuit
The two stage preampleer is built on very low noise, low oset, low drift Precision
Dual Operational Amplier, OPA2107. It has a xed gain of 1000.
In the compensation block we have an instrumentation amplier, which compares
the voltage between two middle points of R3=R4 and C2=P1 circuits. Varying the
resistance of P1(P2) in 0 1 range, one can shift input phase in 0 range,
while keeping the constant amplitude. The input voltage, taken over the 1 resistor,
is equal to the driving current in Helmholtz coil. In the next stage we subtract the
compensation signal (divided with P3 and P4) from amplied signal. The second
instrumentation amplier, INA111, is AC coupled (U4B) and has two additional
gains for dierent volumes of the samples.
The nal stage is the band-pass lter, optimized for attenuation of the low fre-
quency noise below 100Hz and possessing the dispersion function f(!) = 1
!above
0:5 kHz.
+12V
R4 4.43k2
3
6
74
1
8
5
U2
INA111
2
3
6
74
1
8
5
U3
INA111
11
3
A1 A2 A3
50 k50 k
50 k
50 k
1000pF 1000pF
11478
12
139 10
¾ U4A
UAF42
2
3
4
1
½ U1A
OPA21075
6
8
7
½ U1B
OPA2107
VSS
5
46
¼ U4B
UAF42
VCC
R9 33k
R2
10 k
R1
10
R8 6.8k
C1 100pF
IN
VCC
VCC
VCC
P3
1 k
P4
100
R7
1.5 k
R5
50k
VSS
R3
4.43 k
R61 Ω
C2
0.22
P1
10 k
P2
1 k& COIL
R101 M
R11
22 k
C3
0.1
VSS
VSS
R121 k
C4
0.01
C5
0.01
R13
150 k
R14
220 k
M
OUT
dM/dt
OUT
-12V
HOUT
VSS
VCC
Ω
Ω
S1
"GAIN"
from
SINsource
pick-up coil
"PHASE"
"FINE"
"AMPLITUDE"
"FINE"
× 8.3
× 2.5
× 1000
S2
Preamplifier
Compensation block
Integrator
Fig. 37. Schematic of analog integrator based on band-pass lter.
62
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65
5 Acknowledgments
I gratefully acknowledge nancial support from the Swedish funding agencies SI and TFR,
and Bell Laboratories, Lucent Technologies.
During my work at the department of Nanostructure Physics and, previously, at the Con-
densed Matter Physics department I have had the pleasure to work with several people,
whom I wish to acknowledge.
Professor David Haviland, head of Nanostructure Physics department, for giving me the op-
portunity to work in his group and for excellently organizing the work in a newly established
department.
Docent Vladislav Korenivski, my supervisor and friend, for motivating me to work on mag-
netic devices and for the stimulating discussions in a broad area of magnetism. Tatjana
Korenivski (absolute record in friendship: almost 20 years) for her life guidance.
Docent Anders Liljeborg for careful management of Nanofabrication Laboratory, so that we
PhD students have scientic results in spite of capricious E-beam lithography system.
Professor Alexander Sukstanskii, who has shown me the real meaning of theoretician and
teacher.
Karin Andersson and Mattias Urech, my colleagues and friends, for shearing our oce on a
high spiritual level. Special credit goes to Mattias for ideas on perfect phase compensation
in Loop-Tracer electronics.
Peter Ågren, Jan Johansson, Jonas Rundqvist and Jochen Walter, Doctor Michio Watanabe
and Doctor Volker Schöllmann, my colleagues and friends, for the shearing knowledge of
dierent elds in physics and for the humorous atmosphere in the nano-group.
Professor K. V. Rao, for inviting me to Sweden and introducing me to experimental physics.
Professor Alex Grishin for discussion of many subtle points, which lead me to the deeper
understanding the problems in physics.
Doctor Sergey Khartsev for much useful advice in experimental work.
Björn Rodell, Jesper Wittborn, Valter Ström, my colleagues at CMP-KTH for being such a
nice company when I rst arrived in Stockholm.
Andrius and Egle Miniotas, my close friends who made me feel at home in our student
housing in Kungshamra.
My family, Olga and Arina for their love and encouragement.
66
6 Appended papers
I. A Model for Impedance of Planar RF Inductors Based on Magnetic Films, A.
Gromov, V. Korenivski, K. V. Rao, R. B. van Dover, P. M. Mankiewich, IEEE
Transactions on Magnetics, 34 (1998) 1246.
Maxwell's equations are solved analytically for a magnetic/conductor/magnetic sand-
wich strip with ux closure at the edges and no driving current in the magnetic lm. The
nal result is the impedance of the sandwich as a function of frequency and geometrical
parameters. My contribution was all of the calculations and the rst draft.
II. Analysis of Current Distribution in Magnetic Film Inductors, A. Gromov, V.
Korenivski, D. Haviland, and R. B. van Dover, Journal of Applied Physics, 85 (1999)
5202.
This paper is an extension of the above model to account for driving current redistribution
across the interface between the conductor and the magnetic lm. The obtained impedance
is valid for long and thin strips (large length-to-width and width-to-thickness ratios). My
contribution was all of the calculations and the rst draft.
III. Electromagnetic Analysis of Layered Magnetic/Conductor Structures, A. Gro-
mov and V. Korenivski, Journal of Physics D: Applied Physics, 33 (2000) 773.
A method for calculating the impedance of layered magnetic/conductor structures of
arbitrary cross section is presented. The method is exemplied on a conductor of axial
symmetry (wire) coated with a high permeability lm. The dependence of the impedance
on an external magnetic eld is analyzed in relation to the eect known as Giant Magneto-
Impedance, which is promising for sensor applications. My contribution is the calculations
and rst draft.
IV. Impedance of a Ferromagnetic Sandwich, A. Sukstanskii, V. Korenivski, and
A. Gromov, Journal of Applied Physics, 89 (2001) 775.
Maxwell's equations coupled with the Landau-Lifshitz equation for the magnetization
dynamics are solved for a three-layer sandwich, consisting of two ferromagnetic layers sep-
arated by a non-magnetic conductive layer. A 2D problem is analyzed, with and without
magnetic ux closure at the edges of the stripe. The impedance of the magnetically closed
structure is demonstrated to be more ecient then open structure. My contribution was in
discussing the boundary conditions and solutions for the external region, and commenting
on the manuscript.
V. GHz sandwich strip inductors based on FeN lms, A. Gromov, V. Korenivski
and D. Haviland, submitted to Journal of Physics D: Applied Physics (2001).
67
Planar strip inductors based on Fe-N and Cu lms have been fabricated on oxidized Si
substrates. The impedance measurements were carried at frequencies up to 3 GHz, and
revealed a substantial inductance enhancement compared to the air-core values of the strips.
Magnetic characterization of the structures was used to analyze the factors determining their
impedance. My contribution was all experimental aspects as well as the rst draft.
68