Theo Rasing Radboud University Nijmegen Institute for Molecules and Materials
(including pump-probe techniques)
All-optical Control of Magnetism I
HFML - FELIX (THzFEL)
1
All-optical Control of Magnetism I (including pump-probe techniques) - - PowerPoint PPT Presentation
All-optical Control of Magnetism I (including pump-probe techniques) Theo Rasing Radboud University Nijmegen Institute for Molecules and Materials HFML - FELIX (THzFEL) 1 1681 : ship to Boston 2 Controlling magnetism by lightning 3
Theo Rasing Radboud University Nijmegen Institute for Molecules and Materials
(including pump-probe techniques)
HFML - FELIX (THzFEL)
1
1681: ship to Boston
2
3
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Lecture topics:
b.Nonthermal opto-magnetic effects
b.AOS of Ferromagnets
b.Neuromorphic applications
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Lecture topics:
a.Faraday/Kerr effects b.XMCD
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Time scales
Time [seconds]
One second
Fundamental Physical/Chemical processes
Electronics Camera flash
10-15 10-12 10-9 100 10-6 10-3 ps ns fs μs ms s
30 fs = 0.00000000000003 seconds (shortest man-made event)
Ultrashort laser pulse
Blink
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1 ns 1 ps 1 fs 100 ps 10 ps 100 fs 10 fs
Stimulus
Thermodynamics Adiabatic approximation
phonons
Magnons
electrons
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1 ns 1 ps 1 fs 100 ps 10 ps 100 fs 10 fs
Stimulus
Thermodynamics Adiabatic approximation
Laser Pulse
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NUCLEATION OF MAGNETIC ORDER
COHERENT ROTATION OF MAGNETIZATION
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Leland Stanford
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Edward Muybridge: The Horse in Motion
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Magnet
All-optical pump-probe technique
100fs pulses 20J/pulse 1kHz rep. rate
Ti:Sapphire laser & amplifier system
Experimental fs-pump-probe technique
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Revealing ultrafast dynamics with fs flashes
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240fs 3ps C.V. Shank et al, Phys.Rev.Lett.51, 900 (1983)
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~ 0.01 ps – 0.1 ps Exchange interaction 1 ns 1 ps 1 fs 100 ps 10 ps 100 fs 10 fs Homogeneous spin motion (precession) ~ 1 ps - 1 ns via precessional motion 1 s Domain-wall motion Switching via domain-wall motion
H
?
H H M
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S
𝐟𝐠𝐠
𝒋 𝒋 𝐟𝐠𝐠 eff
Hi
𝑗
Li+JijSj
100 T 10 T 1 T 0.1 T Exchange interaction Spin
interaction
Superconducting Magnet
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Current creates a magnetic field
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10 ps rise time 400 ps decay time
short magnetic field pulses!
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Magnetic fieldpuls
F
Th.Gerrits et al, Nature 418, 509 (2002)
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2 .0 1 .5 1 .0 .5 .0
Switching: pulse length=half a precessional period!
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Th.Gerrits et al, Nature 418, 2002 Switching within 200 ps !
II
pulse 1 pulse 223
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The Nobel Prize in Physics 1902
"in recognition of the extraordinary service they rendered by their researches into
the influence of magnetism upon radiation phenomena“ (together with Lorentz)
Zeeman effect
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The Nobel Prize in Physics 1902
"in recognition of the extraordinary service they rendered by their researches into
the influence of magnetism upon radiation phenomena“ (together with Lorentz)
Zeeman effect
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dM dM
s(-) s(+)
inverse? Faraday effect
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Free-electron bath (Te) Lattice (TL=300 K)
Model assumes two heat baths for electrons and phonons:
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Coupled diffusion equations for Tel and Tph note that Cel << Cph – this is why electrons get so hot!
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Coupled diffusion equations for Tel and Tph note that Cel << Cph – this is why electrons get so hot!
.
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.
33
.
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200 400 600 800 1000 1200
Delay (ps)
250 Oe 500 Oe 750 Oe 1000 Oe 1250 Oe
300 600 900 1200 1 2 3 4
Frequency (GHz) Magnetic field (Oe)
anisotropy field
H HA
thin film of magnetic garnet (~Y3Fe5O12)
~GHz
35
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10 20 30
20
20
20
50
[100] [010] [110] (b) Rotation Angle [millidegree]
= 40 Oe H = 240 Oe H = 400 Oe H
= 4 ns Δt x [m]
M
20
20
20 10 5 Time delay [ns] y [m] (c) Radium [m]
LMEW TMEW = 15°
Propagation Dynamics of Optically-excited Spin Waves
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Spin-wave Tomography
2 1 2 1 2 1 2 1
H = 240 Oe H = 400 Oe
(d)
M k
= 15° H = 40 Oe 2000 1000 Amplitude [a. u.]
k [10
4
cm
]
BVMSW LMEW 100
Frequency [GHz]
TMEW
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Coherent-energy Transfer from Elastic waves to Spin Waves
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Phonon Spin
400 nm (3.1 eV) 800 nm (1.6 eV)
Linear Square
Optical charge transfer transition near 400 nm (3.1 eV)
800 nm 400 nm Single photon Two photon
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THz excitation of spin waves in TmFeO3
excitation via change in anisotropy
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Faraday rotation (norm.) Delay time (ps)
Ferromagnetic mode softens at magnetic phase transitions
30 40 50 60 70 80 90 100 150 200 250 0.0 0.1 0.2 0.3 0.8 0.9 Temperature, T (K) Frequency, (THz) d q-FM mode q-AFM mode
24 4 2
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Theo Rasing Radboud University Nijmegen Institute for Molecules and Materials
(including pump-probe techniques)
HFML - FELIX (THzFEL)
44
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counterintuitive?
𝑻𝒋
𝐟𝐠𝐠
S H
Intuitive estimate:
If 100 fs pulse reverses the magnetization, it should act as an effective magnetic field
Simple single spin problem Light acts as a magnetic field, which is either strong (>>1 Tesla)
Why?
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Inverse Faraday effect
*
E E W
M
E E M W H
*
1
*
E E H
Pitaevskii, Sov. Phys. JETP 12, 1008 (1961). van der Ziel Phys. Rev. Lett. 15, 190 (1965).
s
s
dH
dH
2
ˆ M
i M i
zz yy xx
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(see further lecture on Magneto Optics by Prof. Schaefer)
E H
Magneto-optics
Magneto-optics
E E qF ~Mz Mz Faraday effect
Opto-magnetism
dH dH
s(-)
Inverse Faraday effect
) ( ) ( ) (
*
E E Heff
both result from spin-orbit interaction!
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Ultrafast excitation of spins via IFE in DyFeO3
(all-optical spin resonance)
A.V. Kimel, A. Kirilyuk, P.A. Usachev, R.V. Pisarev, A.M. Balbashov, and Th. Rasing, Nature 435, 655-657 (2005) photons L L 0.1 ps 0.1 ps
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Ultrafast excitation of spins via IFE in DyFeO3
(all-optical spin resonance)
DyFeO T = 95 K
3s
s
+
Faraday rotation (deg)
s
s
dH
15 30 45 60 0.0 0.1 0.2
Time delay (ps)
dH
A.V. Kimel, A. Kirilyuk, P.A. Usachev, R.V. Pisarev, A.M. Balbashov, and Th. Rasing, Nature 435, 655-657 (2005) photons L L 0.1 ps 0.1 ps
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25 50 75 0.0 0.5 1.0
Amplitude (arb. units) Pulse fluence (mJ/cm2)
) ( ) ( ) (
*
E E H eff
Inverse Faraday effect
Fields up to 5 T! (even up to 20 T!)
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20 40 60 80 100 120 140
Faraday rotation Delay time (ps)
20 40 60 80 100 120 140
Delay time (ps) DyFeO3 10 K DyFeO3 10 K
First pump Second pump First pump Second pump
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Femtosecond laser reversal of magnetization?
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Polarization microscope + pulsed laser
Circularly polarized 40fs laser pulses
Magneto-Optical microscope 20 nm GdFeCo film
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s s
Hext = 0
GdFeCo
40 fs pulses, 1 kHz
Reversal by 40fs laser pulsen!
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Sweeping the pulsed laser beam at high speed across the sample
C.D. Stanciu et al., PRL 99,047601 (2007)
switching of magnetization by single pulse!
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Femtosecond Magnetic Recording in GdFeCo!
C.D. Stanciu et al., patent #P77323PC00,
PRL 99, 047601 (2007)
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Pulse intensity
All-optical reversal Multidomain state
σ+ σ-
Helicity- independent reversal
Helicity dependent AOS in narrow (~few%) intensity range
+M
50 μm
Pulse profile:
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Switching No Switching
Size of window is 1.5%. Exactly equal to difference in absorption!
Excitation wavelength: 700nm
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Gd Fe Gd Fe
Femtosecond laser reversal: role of exchange? JFe-Gd ~ 30-50T
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Gd Fe Fe Free-electron bath (Te) Lattice (TL=300 K)
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40 fs
Bloch relaxation
Dynamics scales with magnetic moment
Distinct dynamics of sublattices!
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S2 S1 ?
Ground state AFM, transient FM! Conservation total angular momentum
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?
X-rays 400-1400 eV 10-50 ps (FWHM)
BESSY II
fs-Laser pump – X-ray probe
775 780 785 790 795 800 805 L2 L3 Photon energy (eV) TEY (a.u.)
k
Fe
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(for more details: see lecture Prof. Luning)
BESSY II
fs-Laser pump – X-ray probe X-rays 400-1400 eV 100 fs (FWHM)
FEMTO-SLICING!
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reversal of magnetization driven by exchange!!!
S2 S1
J.H. Mentink et al., PRL 057202, 2012
Radu et al, Nature 472, 205-208 (2011)
Fs-XMCD, BESSY
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10 ps laser (heat) pulse
No hot, spin polarized
Ultrafast electrical pulse reverses magnetization!
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[Co/Pt]n
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0.1 ps 1.6 ps 2.2 ps Pt2.0 nm Pt 0.7 nm Co0.4 nm Pt5.0 nm Ta5.0 nm Glass Substrate x3
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0.1 ps 1.6 ps 2.2 ps Pt2.0 nm Pt 0.7 nm Co0.4 nm Pt5.0 nm Ta5.0 nm Glass Substrate x3
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1) No single shot switching 2) Stochastic + deterministic 3) ~100 pulses
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1 ms 35 μm No pulse 10 30 50 5
Stochastic nucleation & growth!!!
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2 nm/pulse @ 0.4mJ/cm2 takes many pulses!
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Magnetic recording in Co/Pt requires multiple pulses. The first pulses form (stochastically) domains with reversed magnetization. The following pulses cause helicity dependent domain wall motion.
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Photo-magnetism of Co-substituted iron garnet
(Y2CaFe3.9Co0.1GeO12 / GGG (001))
laser CW:
EII[110] EII[1-10]
Light-induced slow (~m/sec) motion of domain wall
A.Chizhik et al. PRB, 57 (1998). A.Stupakiewicz et al. PRB, 64 (2001).
Y3+ Co2
+
Co2
+ Fe3 +
Fe3
+
Co3
+
Co3
+
Recording? Heating? Speed?
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Y2CaFe3.9Co0.1GeO12 on GGG (001) thickness d=7.5 μm) 50 fs pulse 50 fs pulse
200×200 m2
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single pulse repeatable switching zero applied field room temperature
Nature 542, 71 (2017).
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Femtosecond magnetic recording Present magnetic recording
10 micron 100 nanometer! 100 x smaller
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PEEM experiment SLS; L. Le Guyader et al, APL 2012, Nature Comm. 2015
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PEEM experiment SLS; L. Le Guyader et al, APL 2012, Nature Comm. 2015
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Nanoscale switching with plasmonic antennas
(with Bert Hecht, Wuerzburg)
Tian-Min Liu et al, Nano Letters, 2015
(10 ns/bit) 0,05 $/GB (2 ns/bit) 0,65 $/GB (>pJ/bit) (>nJ/bit) (~fJ/bit) (~ ps/bit) ?? $/GB
(20x20nm)
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19.928 17.337 15.663 12.953 Fluence(mJ/cm2) 34.036 30.968 25.308 22.558 Fluence(mJ/cm2)
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Single pulse illumination ( = 800 nm) through microscope objective (NA = 0.4) Read-out with Near-field microscopy ( = 532 nm, Resolution 80 nm)
+ =
Sample: Tb22Fe69Co9
Finazzi, et al. Phys. Rev. Lett. 110, 177205 (2013)
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Low fluence High fluence
FeTb
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Minimizing the energy we obtain the Skyrmion radius Single Skyrmion Skyrmionium: Sk+ + Sk- Exchange Energy Anisotropy Energy Dipolar Energy Zeeman Energy
From the model, R0/R1 is sample & fluence independent at Hz = 0: R0/R1 = 1.87 Experimentally R0/R1 2
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Create a new paradigm, beyond von Neumann
0101010 101010
I. End of “Moore”: too much heat
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Processing and storage Separated and serial and 2D Processing and storage Integrated and parallel and 3D!
Processing and storage Separated and serial and 2D Processing and storage Integrated and parallel and 3D!
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Neuromorphic Computing with Magneto-Optics?
102
see: A. Chakravarty et al, Supervised learning of an opto- magnetic neural network with ultrashort laser pulses,
To conclude:
pump/probe magnetism on timescale of exchange interaction
b.Nonthermal opto-magnetic effects
antiferromagnets, metals, dielectrics
Neuromorphic applications
103
DyFeO T = 95 K 3s
s
+ Faraday rotation (deg) s s dH 15 30 45 60 0.0 0.1 0.2 Time delay (ps) dH Radboud Nijmegen A.V. Kimel A.Kirilyuk
D.Stanciu A.v.Etteger
K.Vahaplar
with many thanks to:
STW, NWO, EU, NanoNed, UltraMagnetron, FANTOMAS, IFOX Bessy
T.Kachel N.Pontius L.Le Guyader (Hamburg) Stanford Herman Durr (Uppsala) A.Reid C.Graves University of York
T.A. Ostler (Sheffield) J.Barker R.Evans Ioffe Institute R.V. Pisarev
Nihon University
Kiev
Yassine Quessab Sheena K.K. Patel Eric E. Fullerton UC San Diego
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