model for spin-wave chaos in the coincidence regime of nonlinear ferromagnetic resonance a....
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Model for spin-wave chaos in the Model for spin-wave chaos in the coincidence regime of nonlinear coincidence regime of nonlinear
ferromagnetic resonanceferromagnetic resonance
A. Krawiecki , A. SukiennickiA. Krawiecki , A. Sukiennicki11 1,21,2
Faculty of Physics, Warsaw University of Technology,Faculty of Physics, Warsaw University of Technology,Koszykowa 75, 00-662 Warsaw, PolandKoszykowa 75, 00-662 Warsaw, Poland
11
Department of Solid State Physics, University of Łódź,Department of Solid State Physics, University of Łódź,Pomorska 149/153, 90-283 Łódź, PolandPomorska 149/153, 90-283 Łódź, Poland
22
Nonlinear ferromagnetic resonance
• Ferromagnetic sample is placed in perpendicular dc and rf (with frequencies in the GHz range) magnetic fields.
• The uniform precession of magnetization (uniform mode) is excited in the sample by the rf field. In the coincidence regime the rf field frequency p is close to the uniform mode frequency o.
• If the rf field amplitude hT exceeds a certain threshold hthr, the uniform mode decays into spin-wave pairs.
• The measured quantity is usually absorption in the sample, which is proportional to the uniform mode amplitude.
• As the rf field amplitude is increased, periodic (with frequencies in the range of kHz) and then chaotic oscillations of absorption appear.
The 1st-order Suhl instability (coincidence regime)
Decay of the uniform mode (pumped in resonance)
into spin-wave pairs with half the pumping
frequency and opposite wave vectors
Theoretical description
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ion;magnetizatsaturation
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The magnetic HamiltonianThe magnetic Hamiltonian
The Hamiltonian contains the Zeeman energy, the energy of magnetic dipolarinteractions, and the exchange energy; all magnetizations and fields are
normalized to the saturation magnetization.
The Holstein-Primakoff canonical transformationThe Holstein-Primakoff canonical transformation
ratioicgyromagnetthe;
4122
0
0
210
2120
ssMM
ssM
sMssMsiMMM
z
yx
The Fourier expansionThe Fourier expansionrki
kk
rki
kk esVsesVs
2121 ;
The Bogolyubov transformationThe Bogolyubov transformation
.ts,coefficienationdemagnetiz2,
,sin444
,214
,214
,2,2where
,
20
200
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kkkkkkkkkk
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ikkkNNNN
MDkMNHDkMNH
kkNMB
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aas
The Hamiltonian in the canonical formThe Hamiltonian in the canonical form
.tscoefficienninteractio,,
....
.,intermsorderhigher..cos
321321
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,,,,
,,,,,,3
3
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kkk k
kkkkkpT
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aaHaaccaIthH
The above Hamiltonian contains non-resonant three-mode interaction terms,e.g., . Such terms should be removed by another canonical transformation, which, however, should leave the resonant terms (e.g., ) intact. The removal of all non-resonant terms from H3 influences the higher-order terms in the Hamiltonian. However, since the basic nonlinear process in the case under study is the 1st-order Suhl instability (the resonant three-mode process), the higher-order terms in the Hamiltonian can be subsequently neglected.
00,, aaaV kkkk
00,, 2121aaaU kkkk
The second quasi-canonical transformationThe second quasi-canonical transformation
0,0,0,,,,,
0,0,0,,,
,
,,,,,,,,,,,,
12
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2121
21 21
21212121
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1111 kkkkkk
kkkkkkkkkkk
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kkk
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aaVVaaV
aaUUUaaVVaaVa
Let us assume that only the uniform mode (denoted by zero) is directly excited by the rf field and has frequencyclose to p, and the spin-wave pairs have frequencies close to p/2. Then the following transformation removes the non-resonant terms from H3:
[ A similar transformation is well known in the case of parallel pumping:[ A similar transformation is well known in the case of parallel pumping:V.S. Zakharov et al., V.S. Zakharov et al., Usp. Fiz. NaukUsp. Fiz. Nauk 114114, 609 (1974)], 609 (1974)]
Equations of motion for the spin-wave amplitudesThe Hamiltonian and canonical equations (with damping)The Hamiltonian and canonical equations (with damping)
kkk
kkkkkpT ccVccIthH ...).)(cos( 0,000
kkk
k Hi
t
kkk
k Hi
t
I0 - interaction coefficient between the uniform mode and the rf field,
k- complex amplitudes of the uniform mode and spin waves,
kphenomenological damping of the uniform mode and spin waves,V0,k - coefficients of nonlinear interactions between the uniform mode and spin-wave pairs.
0,0
,000000 )cos(2
kkkkkk
kkkkp
T
iVi
Viith
iI
Separation of the fast time dependenceSeparation of the fast time dependence
).2exp(),exp(
;),exp(
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uViuih
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p
The 1st-order Suhl instability thresholdThe 1st-order Suhl instability threshold
k
kk
kthr VI
iih
,00
002min
Just above the threshold only one (critical) spin-wave pair is excited; if hT
exceeds much the threshold, other pairs with frequency close to p/2 can be excited. However, experimental results (low correlation dimension of chaotic attractors, etc.) suggest that even deeply in the chaotic regime the oscillations of absorption appear due to interactions of a small number of spin-wave pairs
with the uniform mode.
Model with two spin-wave pairsModel with two spin-wave pairs
• The model with one spin-wave pair ( with a2=0) shows transition to chaos via period-doubling,•Inclusion of a second spin-wave pair, with higher Suhl instability threshold, can lead to quasiperiodicity, Pomeau-Maneville type-III intermittency, etc.•The chaotic behavior of the models with one or two spin-wave pairs is in qualitative agreement with experiments on spin-wave chaos in the coincidence regime.
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where
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Equations of motion in a dimensionless formEquations of motion in a dimensionless form
Example: route to chaos via period-doubling
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;84.1),(;75.1),(
,0.3;0.1;5.1;0.1
:Parameters
1100
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Model with one spin-wave pair,Model with one spin-wave pair,left column: time series of absorption,left column: time series of absorption,right column: chaotic attractor.right column: chaotic attractor.
Example: route to chaos via quasiperiodicity
.motionchaotic,34.1),(
motion,dicquasiperio,32.1),(
motion,periodic,3.1),(
.952.0;0.3;0.1
,0.3;0.1;0.1;0.1
:Parameters
22
1100
fe
dc
ba
V
Model with two spin-wave pairs,Model with two spin-wave pairs,left column: time series of absorption,left column: time series of absorption,right column: power spectrum of right column: power spectrum of absorption.absorption.
Example: type-III Pomeau-Maneville intermittency
.5.152.1slope
haslinestraightthe,992.7)(
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haslinestraightthe,9908.7)(
,03.8)(
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:Parameters
22
1100
c
b
a
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c
Model with two spin-wave pairs,Model with two spin-wave pairs,(a) time series of absorption,(a) time series of absorption,(b) mean duration of laminar phases(b) mean duration of laminar phasesvs. the control parameter,vs. the control parameter,(c) probability distribution of (c) probability distribution of durations of laminar phases.durations of laminar phases.
Conclusions
• Systematic derivation of the equations of motion for spin-Systematic derivation of the equations of motion for spin-wave amplitudes in the coincidence regime of nonlinear wave amplitudes in the coincidence regime of nonlinear ferromagnetic resonance above the 1-st order Suhl instability ferromagnetic resonance above the 1-st order Suhl instability threshold was presented,threshold was presented,
• The non-resonant three-mode interaction terms can be The non-resonant three-mode interaction terms can be removed by means of the quasi-canonical transformation, removed by means of the quasi-canonical transformation, which leaves only resonant three-mode terms in the which leaves only resonant three-mode terms in the Hamiltonian, and the higher-order terms can be neglected,Hamiltonian, and the higher-order terms can be neglected,
• The model equations with one or two parametric spin-wave The model equations with one or two parametric spin-wave pairs show transition to chaos via, e.g., period doubling, pairs show transition to chaos via, e.g., period doubling, quasi-periodicity, Pomeau-Maneville intermittency, etc., and quasi-periodicity, Pomeau-Maneville intermittency, etc., and the results of simulations are in qualitative agreement with the results of simulations are in qualitative agreement with experimental results.experimental results.
Thank you for your
attention
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