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Reversal mechanism in single domain
Presentation on “Magnetism and magnetic materials (PHY6011)”
to
Dr. Fayyaz Ahmad
By
Muhammad Usama Daud(12987)
Riphah International University Faisalabad
Domain Theory
• A remarkable property of ferrimagnetic materials is
not so much that they have a spontaneous
magnetization, but rather that their magnetization can
be influenced by the application of very low magnetic
fields.
• Even the earth's field (50 T) can cause magnetization
changes even though the inter atomic exchange
forces responsible for the spontaneous magne-
tization are equivalent to a field of about 1000 T,
almost 100 million times greater than the earth's
field.
What allows this to occur?
• It is the fact that the sample is actually
composed of small regions called magnetic
domains.
• Within each of domain the local magnetiza-
tion is saturated but not necessarily parallel.
• Domains are small (1-100's microns), but
much larger than atomic distances.
Existence of domains
• The existence of domains is hinted at by the
observation that some magnetic properties, and in
particular, co-ercivity and remanance vary greatly
with grain size.
• variation of Hc with grain size
Subdivision of magnetic behavior
The magnetic behavior can be subdivided on the basis of
grain size into four ranges
• SPM: super paramagnetic
• SD: single domain
• PSD: pseudo-single domain
• MD: multi domain
Single Domain
• Single domain, in magnetism, refers to the state of
a ferromagnet in which the magnetization does not vary across the
magnet.
• A magnetic particle that stays in a single domain state for all
magnetic fields is called a single domain particle.
• Such particles are very small (generally below a micrometre in
diameter). They are also very important in a lot of applications
because they have a high coercivity.
• They are the main source of hardness in hard magnets, the carriers
of magnetic storage in tape drives, and the best recorders of the
ancient Earth's magnetic field.
• This is the type of particle that is modeled by the Stoner–Wohlfarth
model. However, it might be in a single-domain state except during
reversal. Often particles are considered single-domain if their
saturation remanence is consistent with the single-domain state.
More recently it was realized that a particle's state could be single-
domain for some range of magnetic fields and then change
continuously into a non-uniform state.
Reversal Mechanism
• Magnetization reversal, also known as switching, refers to
the process that leads to a 180° (arc) re-orientation of the
magnetization vector with respect to its initial direction,
from one stable orientation to the opposite one.
• Technologically, this is one of the most important processes
in magnetism that is linked to the magnetic data
storage process such as used in modern hard disk drives. As
it is known today, there are only a few possible ways to
reverse the magnetization of a metallic magnet:
1. an applied magnetic field
2. spin injection via a beam of particles with spin
3. magnetization reversal by circularly polarized
light; i.e., incident electromagnetic radiation that
is circularly polarized
Reversal Mechanism In Single Domain
• In recent years a significant effort has been made to achieve
magnetization reversal in nanostructures, assisted by the low
amplitude ac field in the radio frequency range.
• The dc magnetic field required to reverse the magnetization of a
single-domain magnetic particle, the so-called anisotropy field, is
typically in the range 0.01-0.1T. The field of this strength at the
location of the particle is not easy to develop fast.
• The ac magnetic field that one can typically develop in the radio-
frequency range would be two orders of magnitude weaker.
• Applied in a resonant fashion, it could increase the amplitude of the
precession of the magnetic moment, sometimes leading to its full
reversal, in the same way as weak pushes of a pendulum at the
frequency of its mechanical oscillation can flip the pendulum over
the top.
Points Need to be addressed
• Firstly, a robust magnetization reversal can be effectively
achieved only with a circularly polarized ac field.
• Secondly, the photons are effectively absorbed only when
they are in resonance with the spin levels.
• The latter are not equidistant on the magnetic quantum
number, that is, on the projection of the magnetic moment on
the direction of the effective field.
• As the magnetic moment reverses, the photon frequency that
can be resonantly absorbed by the magnet changes with time,
so that the frequency of the microwave field has to be
adjusted.
• Damping of the precession adds another dimension to this
problem as the power of the ac field that is pumped into the
magnet should exceed the rate of energy dissipation.
THE MODEL
• The energy of a single-domain magnetic particle with an uni-
axial anisotropy in a circularly-polarized ac field has the form
K= magnetic anisotropy constant,
V= volume of particle
M=magnetization
,h=amplitude of ac field
Where is phase related to time dependent frequency as:
𝐻 = −𝐾𝑣𝑀𝑧
2
− 𝑉𝑀𝑥 cos 𝜑(𝑡) − 𝑉𝑀𝑦 sin 𝜑(𝑡) (1)
𝜑 𝑡 = 𝜔 𝑡 (2)
Cases
• Case #1: We consider that frequency linearly
changing with time:
• Case#2: We consider a non-linear time
dependence of the frequency that provides the
fastest magnetization reversal.
It is convenient to recast the problem in terms of a
classical spin
where Ms is saturation magnetization.
𝜔 𝑡 = −𝑣𝑡 (2)
Where 𝜑 𝑡 = −
𝑣𝑡2
2
(3)
𝒔 = 𝑴/𝑀𝑠 , 𝑠 = 1
𝑠 = 𝛾 𝑠 × 𝑯 𝑒𝑓𝑓 − 𝛼𝛾 𝑠 × 𝑠 × 𝑯 𝒆𝒇𝒇 (4)
The landau-Lifshitz equation
The landau-lifshitz equation of motion for this spin has the form
of
Where γ is the gyromagnetic ratio and α is
dimensionless damping coefficient, and
Is the effective field. Here d=Ha=KMs is the an-
isotropy field. In the initial state the spin points in the
negative z direction.
𝐻𝑒𝑓𝑓 = −
1
𝑉
𝜕𝐻
𝜕𝑀
= 2𝑑𝑠 𝑧 𝑒 𝑧 + ℎ𝑒 𝑥 𝑐𝑜𝑠𝜑 𝑡 + ℎ𝑒 𝑦 𝑠𝑖𝑛𝜑 𝑡 (5)
Switching the coordinate frame
• It is convenient to switch to the coordinate frame
rotating around the z axis together with the
magnetic field (static).
• In the new frame the spin acquires a rotation
opposite to that of the ac field in initial frame.
• Thus in rotating frame the Landau-Lifshitz has the
form
𝑠 = 𝑠 × 𝛾𝑯 𝒆𝒇𝒇 + 𝛀 𝑡 − 𝛼𝛾 𝑠 × 𝑠 × 𝑯 𝒆𝒇𝒇 𝟔
Where𝑯 𝒆𝒇𝒇 = 2𝑑𝑠𝑧 𝑒𝑧 + ℎ𝑒𝑧 , Ω 𝑡 = 𝜔 𝑡 𝑒𝑧 (7)
GENERAL PROPERTIES
• The ac field at negative times is precessing in the same
direction as the magnetic moment, thus it excites magnetic
resonance and may cause magnetization reversal.
• The resonance condition holds during the whole reversal.
After the magnetic moment overcomes the barrier, sz > 0, it
changes its precession direction, and so does the ac field.
• In the rotating frame, the field ω(t)/γ sweeping at a linear
rate makes the problem resembling that of the Landau-
Zener (LZ) effect that can be formulated in terms of the
evolution of a classical spin described by a Larmor
equation.
Modifications
• There are 3 modifications:
1. Uni-axial anistropy
2. Damping added to model
3. Sweeping w(t) in the negative direction.
• Because of the latter, the initial state of the spin in the
rotating frame is the high energy state with sz opposite
to w.
• To the contrast in the regular LZ effect the initial spin is
the low energy state.
• In the absence of anisotropy and damping, initial
orientation of the spin and sweep direction do not
matter.
GENERAL PROPERTIES (cont.)
• Absence of damping:
Multiply the 1st factor of equation 6 i.e factor of
“γ” by -1 which will make the spin process in
opposite direction but does not effect reversal.
The resulting model is with positive sweep, while
anisotropy becomes easy-plane.
• For a sweep slow enough the system adiabatically
follows the time-dependent lowest energy state.
• In our original model the magnetization reversal
is similar. Only instead of adiabatically following
the lowest energy state, the spin adiabatically
follows the highest energy state.
GENERAL PROPERTIES (cont.)
• Adiabatic Solution:
The adiabatic solution corresponds to the maximum of the energy in the rotating
frame
𝐻
𝑉𝑀𝑠
= −𝑑𝑠𝑧
2
− 𝑠 𝑥 ℎ −
𝜔
𝛾
𝑠𝑧 8
The maximal energy corresponds to 𝑠 𝑦 =0
Using 𝑠 𝑥 = − 1 − 𝑠𝑧
2 and requiring
𝑑𝐻
𝑑 𝑠 𝑧
=0
We obtain 2𝑑𝑠𝑧 +
ℎ 𝑠 𝑧
1−𝑠 𝑧
2
+
𝜔
𝛾
= 0 9
Since in practical conditions ℎ ≪ 𝑑, an approximate solution of this 4th
order
algebraic equation for the adiabatic spin value reads
𝑠𝑧 =
−1 𝜔 > 2𝛾𝑑
−
𝜔
2𝛾𝑑
𝜔 ≤ 2𝛾𝑑
1 𝜔 < −2𝛾𝑑
(10)
GENERAL PROPERTIES (cont.)
• Note that this solution is independent of h.
• Nonzero values of h cause rounding at the borders of the central region
|ω| ≤ 2γd where the reversal occurs.
• In the laboratory frame, the spin is precessing during adiabatic reversal
being phase-locked to the ac field.
• For α = 0 the magnetization reversal can be achieved for whatever small ac
field h.
• In the case of a nonzero damping, there is a dissipative torque acting
towards the energy minima, and the ac field h has to exceed a threshold
value to overcome this torque.
• Below we will see that the magnetization reversal requires
h > αd (11)
that is much easier to fulfill than h > 2d in the case of a static field. As the
torque due to the transverse field is maximal when the magnetic moment
is perpendicular to it, in the presence of damping the magnetic moment
goes out of the x-z plane during the reversal.
Numerical- Magnetization reversal by The time
linear frequency sweep
• A. Time Dependence of reversing magnetization.
The results of numerical solution of Eq. (6) in the un-damped case α = 0 for a small
frequency sweep rate are shown in Fig. 1. Magnetization reversal in this case is
almost adiabatic and sz(t) is well described by Eq. (10) with rounding at the
borders of the reversal interval due to a small value of h/d. The reversal is
practically confined to the z-x plane and sy is small.
Conti….
• Numerical results for a faster sweep rate are shown in Fig. 2. Here there is still
magnetization reversal but it is not adiabatic and the final value of sz is smaller than one.
Because of this, the magnetic moment is precessing around the z axis, as manifested by sx
and sy. During reversal the magnetization is substantially deviating from the z-x plane. For
larger sweep rates the reversal quickly becomes impossible.
Conti….
• Fig. 3 shows that in the damped case the magnetic moment substantially
deviates from the z-x plane. Still, overall the reversal in this case is close
to adiabatic.
ANALYTICAL
• Analytical investigation of the magnetization
reversal is more convenient in spherical coordinates
𝑠𝑧 = 𝑐𝑜𝑠𝜃 , 𝑠𝑥 = 𝑠𝑖𝑛𝜃𝑐𝑜𝑠𝜑, 𝑠𝑦 = 𝑠𝑖𝑛𝜃𝑠𝑖𝑛𝜑 (12)
After neglecting ac field the dissipation term of equation 6 becomes
𝜃 = 𝛾ℎ𝑠𝑖𝑛𝜑 − 𝛼𝛾𝑠𝑖𝑛2𝜃 (13)
𝜑 = −2𝛾𝑑𝑐𝑜𝑠𝜃 − 𝜔 𝑡 + 𝛾ℎ𝑐𝑜𝑠𝜑𝑐𝑜𝑡𝜃 (14)
A. Linear frequency Sweep
• In case of linear frequency sweep, eq.3, we can rewrite this equation of
motion for the spin in terms of dimensionless time variable
𝜏 =
𝑣𝑡
2𝛾𝑑
(15)
The resulting equation
𝑑𝜃
𝑑𝜏
= 𝑏𝑠𝑖𝑛𝜑 − 𝛼𝑎𝑠𝑖𝑛2𝜃 16
𝑑𝜑
𝑑𝜏
= −2𝑎 𝑐𝑜𝑠𝜃 − 𝜏 + 𝑏𝑐𝑜𝑠𝜑𝑐𝑜𝑡𝜃 17
𝑤ℎ𝑒𝑟𝑒 𝑎 =
2𝛾2
𝑑2
𝑣
, 𝑎𝑛𝑑 𝑏 =
2𝛾2
𝑑ℎ
𝑣
18
𝑐ℎ𝑎𝑟𝑎𝑐𝑡𝑒𝑟𝑖𝑠𝑒 𝑡ℎ𝑒 𝑠𝑤𝑒𝑒𝑝 𝑟𝑎𝑡𝑒.
𝑜𝑛𝑒 𝑖𝑚𝑝𝑜𝑟𝑡𝑎𝑛𝑡 𝑝𝑎𝑟𝑎𝑚𝑒𝑡𝑒𝑟 𝑖𝑠 𝐴 =
𝑎𝑑
ℎ
(19)
A. Linear frequency Sweep(cont.)
• Since a is a large parameter, phase locking of the magnetic moment to the
ac field and thus efficient reversal requires cosθ = τ in the reversal region
|τ| < 1. If cosθ only slightly deviates from this form, this causes strong
oscillations of ϕ and thus the breakdown of the phase locking. Setting
cosθ = τ, from Eq. (16) one obtains the phase-locking condition for ϕ in the
form
• The term on the left of this formula is proportional to the torque acting on
the spin from the ac field. This torque has to ensure temporal change of θ
(i.e., reversal) and compensate for the dissipative torque that is acting
toward potential wells.
sin 𝜑 =
1
𝑏
𝑑𝜃
𝑑𝜏
+ 𝐴𝑠𝑖𝑛2𝜃 (20)
A. Linear frequency Sweep(cont.)
• One can see that damping hampers climbing the barrier by the magnetic
moment. The maximal damping torque is realized at θ = 3π/4, where sin2θ
= −1. Since the reversal implies dθ/dτ < 0, it is clear that for A > 1 the ac
torque cannot overcome the damping torque. Thus, the necessary
condition for the magnetization reversal is
A<1 (21)
• while the more restricting sufficient condition requires that the right-hand
side of Eq. (20) does not drop below -1 for all τ. The latter requires the
frequency sweep rate to be not too fast. Using cosθ = τ, one can rewrite
this condition in the form
max 𝑓 𝜏 < 1, 𝑓 𝜏 ≡ −2𝐴 𝜏 1 − 𝜏2 +
1
𝑏 1 − 𝜏2
(22)
A. Linear frequency Sweep(cont.)
F(t) graph of equation equation 22
Discussion and conclusions
• We conclude from our studies that a circularly polarized ac
field that has specific time dependence of the frequency
can be an effective tool for switching the magnetization.
• The corresponding physical mechanism consists of the
resonant absorbtion of photons of the spin projection that
ensures the consistent change in the projection of the
magnetic moment.
• Emission of excitations by the magnetic moment inhibits
this process. In the micromagnetic theory it is described by
the phenomenological dimensionless small parameter α
that can be independently measured.
• In single-domain particles this parameter is usually greater
than in bulk materials and is typically of order 0.01−0.1.
Conti….
• The condition on the power of the ac field needed to
overcome damping and reverse the magnetization is h
> αd. For, e,g., the anisotropy field d of order 0.01T and
α of order 0.01, one obtains h of order 0.0001T for the
amplitude of the ac field, which is a reasonable value
from the practical point of view.
• It has been demonstrated that the linear case, ω = −vt,
resembles the Landau-Zener problem. Magnetization
reversal has been demonstrated numerically and the
phase diagrams have been obtained that show the
range of v, h, d, and α that provide the reversal.
• They show that for the reversal to occur, the frequency
sweep must be sufficiently slow, but not too slow when
the damping is finite.
Conti….
• It has been demonstrated that, besides ensuring the fasted
magnetization switch, it also pumps less energy into the system as
compared to the linear sweep. In both cases the injected energy is
proportional to α.
• Circularly polarized ac field can be generated by coupling a single-
domain particle electromagnetically to two weak superconducting
links whose phases are displaced by π/2 with respect to each other.
• One advantage of such a system is that the time dependence of the
frequency of the ac field generated by the links can be controlled by
voltage. This problem has been studied by us with account of the
back effect of the magnetic moment on the links.
• Magnetization reversal has been demonstrated numerically and
analytical expressions have been derived for the time dependence
of the voltages across the links that provide the fasted
magnetization reversal.
• One remarkable property of this system is weak dependence of the
reversal dynamics on the voltage noise.
Reversal mechanism in single domain

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Reversal mechanism in single domain

  • 1. Reversal mechanism in single domain Presentation on “Magnetism and magnetic materials (PHY6011)” to Dr. Fayyaz Ahmad By Muhammad Usama Daud(12987) Riphah International University Faisalabad
  • 2. Domain Theory • A remarkable property of ferrimagnetic materials is not so much that they have a spontaneous magnetization, but rather that their magnetization can be influenced by the application of very low magnetic fields. • Even the earth's field (50 T) can cause magnetization changes even though the inter atomic exchange forces responsible for the spontaneous magne- tization are equivalent to a field of about 1000 T, almost 100 million times greater than the earth's field.
  • 3. What allows this to occur? • It is the fact that the sample is actually composed of small regions called magnetic domains. • Within each of domain the local magnetiza- tion is saturated but not necessarily parallel. • Domains are small (1-100's microns), but much larger than atomic distances.
  • 4. Existence of domains • The existence of domains is hinted at by the observation that some magnetic properties, and in particular, co-ercivity and remanance vary greatly with grain size. • variation of Hc with grain size
  • 5. Subdivision of magnetic behavior The magnetic behavior can be subdivided on the basis of grain size into four ranges • SPM: super paramagnetic • SD: single domain • PSD: pseudo-single domain • MD: multi domain
  • 6. Single Domain • Single domain, in magnetism, refers to the state of a ferromagnet in which the magnetization does not vary across the magnet. • A magnetic particle that stays in a single domain state for all magnetic fields is called a single domain particle. • Such particles are very small (generally below a micrometre in diameter). They are also very important in a lot of applications because they have a high coercivity. • They are the main source of hardness in hard magnets, the carriers of magnetic storage in tape drives, and the best recorders of the ancient Earth's magnetic field. • This is the type of particle that is modeled by the Stoner–Wohlfarth model. However, it might be in a single-domain state except during reversal. Often particles are considered single-domain if their saturation remanence is consistent with the single-domain state. More recently it was realized that a particle's state could be single- domain for some range of magnetic fields and then change continuously into a non-uniform state.
  • 7. Reversal Mechanism • Magnetization reversal, also known as switching, refers to the process that leads to a 180° (arc) re-orientation of the magnetization vector with respect to its initial direction, from one stable orientation to the opposite one. • Technologically, this is one of the most important processes in magnetism that is linked to the magnetic data storage process such as used in modern hard disk drives. As it is known today, there are only a few possible ways to reverse the magnetization of a metallic magnet: 1. an applied magnetic field 2. spin injection via a beam of particles with spin 3. magnetization reversal by circularly polarized light; i.e., incident electromagnetic radiation that is circularly polarized
  • 8. Reversal Mechanism In Single Domain • In recent years a significant effort has been made to achieve magnetization reversal in nanostructures, assisted by the low amplitude ac field in the radio frequency range. • The dc magnetic field required to reverse the magnetization of a single-domain magnetic particle, the so-called anisotropy field, is typically in the range 0.01-0.1T. The field of this strength at the location of the particle is not easy to develop fast. • The ac magnetic field that one can typically develop in the radio- frequency range would be two orders of magnitude weaker. • Applied in a resonant fashion, it could increase the amplitude of the precession of the magnetic moment, sometimes leading to its full reversal, in the same way as weak pushes of a pendulum at the frequency of its mechanical oscillation can flip the pendulum over the top.
  • 9. Points Need to be addressed • Firstly, a robust magnetization reversal can be effectively achieved only with a circularly polarized ac field. • Secondly, the photons are effectively absorbed only when they are in resonance with the spin levels. • The latter are not equidistant on the magnetic quantum number, that is, on the projection of the magnetic moment on the direction of the effective field. • As the magnetic moment reverses, the photon frequency that can be resonantly absorbed by the magnet changes with time, so that the frequency of the microwave field has to be adjusted. • Damping of the precession adds another dimension to this problem as the power of the ac field that is pumped into the magnet should exceed the rate of energy dissipation.
  • 10. THE MODEL • The energy of a single-domain magnetic particle with an uni- axial anisotropy in a circularly-polarized ac field has the form K= magnetic anisotropy constant, V= volume of particle M=magnetization ,h=amplitude of ac field Where is phase related to time dependent frequency as: 𝐻 = −𝐾𝑣𝑀𝑧 2 − 𝑉𝑀𝑥 cos 𝜑(𝑡) − 𝑉𝑀𝑦 sin 𝜑(𝑡) (1) 𝜑 𝑡 = 𝜔 𝑡 (2)
  • 11. Cases • Case #1: We consider that frequency linearly changing with time: • Case#2: We consider a non-linear time dependence of the frequency that provides the fastest magnetization reversal. It is convenient to recast the problem in terms of a classical spin where Ms is saturation magnetization. 𝜔 𝑡 = −𝑣𝑡 (2) Where 𝜑 𝑡 = − 𝑣𝑡2 2 (3) 𝒔 = 𝑴/𝑀𝑠 , 𝑠 = 1
  • 12. 𝑠 = 𝛾 𝑠 × 𝑯 𝑒𝑓𝑓 − 𝛼𝛾 𝑠 × 𝑠 × 𝑯 𝒆𝒇𝒇 (4) The landau-Lifshitz equation The landau-lifshitz equation of motion for this spin has the form of Where γ is the gyromagnetic ratio and α is dimensionless damping coefficient, and Is the effective field. Here d=Ha=KMs is the an- isotropy field. In the initial state the spin points in the negative z direction. 𝐻𝑒𝑓𝑓 = − 1 𝑉 𝜕𝐻 𝜕𝑀 = 2𝑑𝑠 𝑧 𝑒 𝑧 + ℎ𝑒 𝑥 𝑐𝑜𝑠𝜑 𝑡 + ℎ𝑒 𝑦 𝑠𝑖𝑛𝜑 𝑡 (5)
  • 13. Switching the coordinate frame • It is convenient to switch to the coordinate frame rotating around the z axis together with the magnetic field (static). • In the new frame the spin acquires a rotation opposite to that of the ac field in initial frame. • Thus in rotating frame the Landau-Lifshitz has the form 𝑠 = 𝑠 × 𝛾𝑯 𝒆𝒇𝒇 + 𝛀 𝑡 − 𝛼𝛾 𝑠 × 𝑠 × 𝑯 𝒆𝒇𝒇 𝟔 Where𝑯 𝒆𝒇𝒇 = 2𝑑𝑠𝑧 𝑒𝑧 + ℎ𝑒𝑧 , Ω 𝑡 = 𝜔 𝑡 𝑒𝑧 (7)
  • 14. GENERAL PROPERTIES • The ac field at negative times is precessing in the same direction as the magnetic moment, thus it excites magnetic resonance and may cause magnetization reversal. • The resonance condition holds during the whole reversal. After the magnetic moment overcomes the barrier, sz > 0, it changes its precession direction, and so does the ac field. • In the rotating frame, the field ω(t)/γ sweeping at a linear rate makes the problem resembling that of the Landau- Zener (LZ) effect that can be formulated in terms of the evolution of a classical spin described by a Larmor equation.
  • 15. Modifications • There are 3 modifications: 1. Uni-axial anistropy 2. Damping added to model 3. Sweeping w(t) in the negative direction. • Because of the latter, the initial state of the spin in the rotating frame is the high energy state with sz opposite to w. • To the contrast in the regular LZ effect the initial spin is the low energy state. • In the absence of anisotropy and damping, initial orientation of the spin and sweep direction do not matter.
  • 16. GENERAL PROPERTIES (cont.) • Absence of damping: Multiply the 1st factor of equation 6 i.e factor of “γ” by -1 which will make the spin process in opposite direction but does not effect reversal. The resulting model is with positive sweep, while anisotropy becomes easy-plane. • For a sweep slow enough the system adiabatically follows the time-dependent lowest energy state. • In our original model the magnetization reversal is similar. Only instead of adiabatically following the lowest energy state, the spin adiabatically follows the highest energy state.
  • 17. GENERAL PROPERTIES (cont.) • Adiabatic Solution: The adiabatic solution corresponds to the maximum of the energy in the rotating frame 𝐻 𝑉𝑀𝑠 = −𝑑𝑠𝑧 2 − 𝑠 𝑥 ℎ − 𝜔 𝛾 𝑠𝑧 8 The maximal energy corresponds to 𝑠 𝑦 =0 Using 𝑠 𝑥 = − 1 − 𝑠𝑧 2 and requiring 𝑑𝐻 𝑑 𝑠 𝑧 =0 We obtain 2𝑑𝑠𝑧 + ℎ 𝑠 𝑧 1−𝑠 𝑧 2 + 𝜔 𝛾 = 0 9 Since in practical conditions ℎ ≪ 𝑑, an approximate solution of this 4th order algebraic equation for the adiabatic spin value reads 𝑠𝑧 = −1 𝜔 > 2𝛾𝑑 − 𝜔 2𝛾𝑑 𝜔 ≤ 2𝛾𝑑 1 𝜔 < −2𝛾𝑑 (10)
  • 18. GENERAL PROPERTIES (cont.) • Note that this solution is independent of h. • Nonzero values of h cause rounding at the borders of the central region |ω| ≤ 2γd where the reversal occurs. • In the laboratory frame, the spin is precessing during adiabatic reversal being phase-locked to the ac field. • For α = 0 the magnetization reversal can be achieved for whatever small ac field h. • In the case of a nonzero damping, there is a dissipative torque acting towards the energy minima, and the ac field h has to exceed a threshold value to overcome this torque. • Below we will see that the magnetization reversal requires h > αd (11) that is much easier to fulfill than h > 2d in the case of a static field. As the torque due to the transverse field is maximal when the magnetic moment is perpendicular to it, in the presence of damping the magnetic moment goes out of the x-z plane during the reversal.
  • 19. Numerical- Magnetization reversal by The time linear frequency sweep • A. Time Dependence of reversing magnetization. The results of numerical solution of Eq. (6) in the un-damped case α = 0 for a small frequency sweep rate are shown in Fig. 1. Magnetization reversal in this case is almost adiabatic and sz(t) is well described by Eq. (10) with rounding at the borders of the reversal interval due to a small value of h/d. The reversal is practically confined to the z-x plane and sy is small.
  • 20. Conti…. • Numerical results for a faster sweep rate are shown in Fig. 2. Here there is still magnetization reversal but it is not adiabatic and the final value of sz is smaller than one. Because of this, the magnetic moment is precessing around the z axis, as manifested by sx and sy. During reversal the magnetization is substantially deviating from the z-x plane. For larger sweep rates the reversal quickly becomes impossible.
  • 21. Conti…. • Fig. 3 shows that in the damped case the magnetic moment substantially deviates from the z-x plane. Still, overall the reversal in this case is close to adiabatic.
  • 22. ANALYTICAL • Analytical investigation of the magnetization reversal is more convenient in spherical coordinates 𝑠𝑧 = 𝑐𝑜𝑠𝜃 , 𝑠𝑥 = 𝑠𝑖𝑛𝜃𝑐𝑜𝑠𝜑, 𝑠𝑦 = 𝑠𝑖𝑛𝜃𝑠𝑖𝑛𝜑 (12) After neglecting ac field the dissipation term of equation 6 becomes 𝜃 = 𝛾ℎ𝑠𝑖𝑛𝜑 − 𝛼𝛾𝑠𝑖𝑛2𝜃 (13) 𝜑 = −2𝛾𝑑𝑐𝑜𝑠𝜃 − 𝜔 𝑡 + 𝛾ℎ𝑐𝑜𝑠𝜑𝑐𝑜𝑡𝜃 (14)
  • 23. A. Linear frequency Sweep • In case of linear frequency sweep, eq.3, we can rewrite this equation of motion for the spin in terms of dimensionless time variable 𝜏 = 𝑣𝑡 2𝛾𝑑 (15) The resulting equation 𝑑𝜃 𝑑𝜏 = 𝑏𝑠𝑖𝑛𝜑 − 𝛼𝑎𝑠𝑖𝑛2𝜃 16 𝑑𝜑 𝑑𝜏 = −2𝑎 𝑐𝑜𝑠𝜃 − 𝜏 + 𝑏𝑐𝑜𝑠𝜑𝑐𝑜𝑡𝜃 17 𝑤ℎ𝑒𝑟𝑒 𝑎 = 2𝛾2 𝑑2 𝑣 , 𝑎𝑛𝑑 𝑏 = 2𝛾2 𝑑ℎ 𝑣 18 𝑐ℎ𝑎𝑟𝑎𝑐𝑡𝑒𝑟𝑖𝑠𝑒 𝑡ℎ𝑒 𝑠𝑤𝑒𝑒𝑝 𝑟𝑎𝑡𝑒. 𝑜𝑛𝑒 𝑖𝑚𝑝𝑜𝑟𝑡𝑎𝑛𝑡 𝑝𝑎𝑟𝑎𝑚𝑒𝑡𝑒𝑟 𝑖𝑠 𝐴 = 𝑎𝑑 ℎ (19)
  • 24. A. Linear frequency Sweep(cont.) • Since a is a large parameter, phase locking of the magnetic moment to the ac field and thus efficient reversal requires cosθ = τ in the reversal region |τ| < 1. If cosθ only slightly deviates from this form, this causes strong oscillations of ϕ and thus the breakdown of the phase locking. Setting cosθ = τ, from Eq. (16) one obtains the phase-locking condition for ϕ in the form • The term on the left of this formula is proportional to the torque acting on the spin from the ac field. This torque has to ensure temporal change of θ (i.e., reversal) and compensate for the dissipative torque that is acting toward potential wells. sin 𝜑 = 1 𝑏 𝑑𝜃 𝑑𝜏 + 𝐴𝑠𝑖𝑛2𝜃 (20)
  • 25. A. Linear frequency Sweep(cont.) • One can see that damping hampers climbing the barrier by the magnetic moment. The maximal damping torque is realized at θ = 3π/4, where sin2θ = −1. Since the reversal implies dθ/dτ < 0, it is clear that for A > 1 the ac torque cannot overcome the damping torque. Thus, the necessary condition for the magnetization reversal is A<1 (21) • while the more restricting sufficient condition requires that the right-hand side of Eq. (20) does not drop below -1 for all τ. The latter requires the frequency sweep rate to be not too fast. Using cosθ = τ, one can rewrite this condition in the form max 𝑓 𝜏 < 1, 𝑓 𝜏 ≡ −2𝐴 𝜏 1 − 𝜏2 + 1 𝑏 1 − 𝜏2 (22)
  • 26. A. Linear frequency Sweep(cont.) F(t) graph of equation equation 22
  • 27. Discussion and conclusions • We conclude from our studies that a circularly polarized ac field that has specific time dependence of the frequency can be an effective tool for switching the magnetization. • The corresponding physical mechanism consists of the resonant absorbtion of photons of the spin projection that ensures the consistent change in the projection of the magnetic moment. • Emission of excitations by the magnetic moment inhibits this process. In the micromagnetic theory it is described by the phenomenological dimensionless small parameter α that can be independently measured. • In single-domain particles this parameter is usually greater than in bulk materials and is typically of order 0.01−0.1.
  • 28. Conti…. • The condition on the power of the ac field needed to overcome damping and reverse the magnetization is h > αd. For, e,g., the anisotropy field d of order 0.01T and α of order 0.01, one obtains h of order 0.0001T for the amplitude of the ac field, which is a reasonable value from the practical point of view. • It has been demonstrated that the linear case, ω = −vt, resembles the Landau-Zener problem. Magnetization reversal has been demonstrated numerically and the phase diagrams have been obtained that show the range of v, h, d, and α that provide the reversal. • They show that for the reversal to occur, the frequency sweep must be sufficiently slow, but not too slow when the damping is finite.
  • 29. Conti…. • It has been demonstrated that, besides ensuring the fasted magnetization switch, it also pumps less energy into the system as compared to the linear sweep. In both cases the injected energy is proportional to α. • Circularly polarized ac field can be generated by coupling a single- domain particle electromagnetically to two weak superconducting links whose phases are displaced by π/2 with respect to each other. • One advantage of such a system is that the time dependence of the frequency of the ac field generated by the links can be controlled by voltage. This problem has been studied by us with account of the back effect of the magnetic moment on the links. • Magnetization reversal has been demonstrated numerically and analytical expressions have been derived for the time dependence of the voltages across the links that provide the fasted magnetization reversal. • One remarkable property of this system is weak dependence of the reversal dynamics on the voltage noise.

Editor's Notes

  1. The Stoner–Wohlfarth model is a widely used model for the magnetization of single-domain ferromagnets. It is a simple example of magnetic hysteresis and is useful for modeling small magnetic particles in magnetic storage, biomagnetism, rock magnetism and paleomagnetism
  2. photons of circular polarization have a definite orientation of their spin projection, while photons with linear polarization are in a superposition of spin states. Consequently, photons with the right circular polarization, when absorbed by the magnet, drive the magnetization in one direction towards the reversal, while linearly polarized photons can be both absorbed and emitted and, therefore, do not necessarily reverse the magnetization.