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Ultrafast Magnetization Dynamics Ultrafast Magnetization Dynamics

Ultrafast Magnetization Dynamics - PowerPoint Presentation

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Ultrafast Magnetization Dynamics - PPT Presentation

T Ostler 1 Dept of Physics The University of York York United Kingdom December 2013 Increasing demand A few GB to TBs 25TB daily log 100TB storage 25PB 24PB daily 330 EB demand in 2011 ID: 356114

dynamics field demagnetization magnetization field dynamics magnetization demagnetization ostler switching model laser magnetic spin time nature bands calculate exchange heating radu excitation

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Slide1

Ultrafast Magnetization Dynamics

T. Ostler1Dept. of Physics, The University of York, York, United Kingdom.December 2013Slide2

Increasing demand

A few GB to TB’s

25TB daily log

100TB storage

2.5PB

24PB daily

330 EB demand in 2011

Estimated size of the internet 4ZBSlide3

Increasing demand

If all storage demand was met by SSD’s/flash etc, $250 billion in plant construction is required.Faster data access/writing is desirable.

Users [millions]

Months

Now at 175millionSlide4

Write speed challenge

In 1953 IBM launched first commercial HHD with average data access times of just under 1 second!MeIBM 350

A 50KB pdf would take a few days to copy.

How have data rates improved?Slide5

Speed limits in magnetism

Huge increase in speeds since the 80’s.

Rate has been slowing in last 10 years.Slide6

Write times

CD @ 1xEnterprise drivePulsed fields

Faster write times

How fast can we go?Slide7

Magnetic field processes.Atomistic spin dynamics model for magnetization dynamics.

LLGHow we construct such a modelIncluding laser heating + parameterizationLimitations of the modelFinally femtosecond lasers processes.Conclusion: reversal in hundreds of fs using laser without applied field.Mechanism for switching without a field.

Towards femtosecond

processesSlide8

Precession and damping

Landau-

Lifshitz

-Gilbert (LLG) equation

Precession

Damping

NB, if under- damped, many

precesssion

cycles may be necessary in order to reach

equilibrium.

Current HDD has write pole around 1-2T.

Switching around 1ns.Slide9

Ultrafast field switching in 200ps

GaAs photoswitches excited by fs laser pulse creates initial field.Permally thin film, in-plane.High field and low damping causes ringing oscillations in magnetization.

GaAs photoswitches excited by fs laser pulse creates initial field.

Second pulses (at a very specific delay time) can stop magnetization.

Reversal complete in 200 picoseconds.

Figures from :Nature

, 418, 509-512 (2002).Slide10

Control of magnetization dynamics in applied field limited by precession time.

There are a number of other ways to control magnetization:Spin transfer torqueHeat assisted magnetic recordingThe exchange interaction gives rise to magnetic order.The strongest force in magnetism. Can we excite processes on this timescale?

Can we go faster?

Timescale:

10’s -> 100’s

fsSlide11

Femtosecond

laser heating and measurementFast demagnetization of Ni

Beaurepaire et al. PRL, 76, 4250 (1996).

MOKE in transmission.

Using femtosecond laser pulses Beaurepaire

showed fs demagnetization.

Demagnetization in around 1ps. Remagnetization in a few ps.

Can we model this?

E

E

M

θ

F

~M

Z

Faraday

effect

Rotation (

θ

f

) of polarization plane.

χ

: susceptibility tensor

k: wave-vector

n: refractive indexSlide12

Time-scale/Length-scale

10-15 s (fs)10-12 s (ps)10-9 s (ns)

10-6 s (µs)

10

-3 s (ms)

Langevin Dynamics on atomic

level

Kinetic Monte Carlo

10

-0

s (s)+

10

-16

s (<

fs

)

TDFT/

ab

-initio spin dynamics

Time

10

-9

m (nm)

10

-6

m (

μm

)

10

-3

m (mm)

10

-10

m (Å)

Length

Micromagnetics

/LLB

http://www.psi.ch/swissfel/ultrafast-manipulation-of-the-magnetization

http://www.castep.org/

Superdiffusive

spin transportSlide13

The spin

dynamics modelAssume fixed atomic positionsProcesses such as e-e, e-p and p-p scattering are treated phenomenologically (λ).

At each timestep we calculate a field acting on each spin and solve using numerical integration.

To calculate the fields we consider a Hamiltonian (below).

Extended Heisenberg Hamiltonian

Exchange

Anisotropy

Zeeman

Dipole-DipoleSlide14

How do we find J/D/μ?

Jij can be found from DFT. Adiabatic approximation assuming electron motion much faster than spinwaves.Assume frozen magnon pictureSpin spiral for particular q vector.

Integration in q-space gives exchange energy.

Can also assume nearest neighbour interaction and use experimental TC

to determine Jij

Anisotropy can also be calculated from first principles.

Possible to have other anisotropy terms:

Surface

Cubic

Etc.

sc

bcc

fccSlide15

What can we calculate?

Distribution of spinwave energiesMagnetization dynamics

Static properties: M(T), hysteresis

Spinwave dispersionSlide16

The spin

dynamics model

Spinwaves

Heat bath

Damping is phenomenological.

Energy exchange is to/from bath and

magnon-magnon

interactions.Slide17

Modelling temperature effects

Precession

Damping

NoiseSlide18

Laser heating

Chen

et al

.

Int.

Journ

. Heat and Mass Transfer.

49

, 307-316 (2006)Slide19

How can the electron temperature be determined?

Figure from

Atxitia

et al. Phys. Rev. B.

81

, 174401 (2010).

Usually known from literature

Fitting initial decay to an exponential

Final temperature determinesSlide20

Laser heating

Theory

Experiment

What governs the time-scale for demagnetization?

Can we control it?

What happens if we have multiple species?Slide21

Two

sublattices

Model calculations

J

ij

>0

J

ij

<

0

Two sublattice

f

erromagnet

Two sublattice

f

errimagnet

Strongly exchange coupled.

But

decoupled dynamics.

Fine in theory, what do we see experimentally?

Radu

, Ostler

et al.

submitted.Slide22

X-ray Magnetic Circular

Dichroism

(XMCD)

XMCD used to measure individual magnetic elements.

Excite core electrons from spin-split valance bands.

Circularly polarized photons (+

ħ

,

-

ħ

) give rise to different absorptions.

Radu

, Ostler

et al. Nature

,

472

, 205-208 (2011).Slide23

Two

sublattices

Experiments of dynamics (via XMCD) shows qualitatively similar results.

What determines the rate of demagnetization?

Radu

, Ostler

et al.

submitted.Slide24

Time-scales of elements in different materials

Radu

, Ostler

et al.

submitted.

More details

arXiv

:1308.0993

Measured demagnetization time to 50% demagnetization by tuning pump

fluence

.

Plot the above data against the magnetic moment.

Seems to scale with the magnetic moment.

Deviation due to exchange. Slide25

Can we actually do something useful?

Controlling demagnetization is interesting but can we actually do something with it?

Element-resolved dynamics.

Initial State

Different demagnetization times

Transient ferromagnetic-like state

Reversal of the

sublattices

Radu

et al. Nature

,

472

, 205-208 (2011).

Switching in a magnetic field

Some interesting

behaviour

Experiment

Model resultsSlide26

Switching without a field

What role is the magnetic field playing?

Model calculations show field playing almost no role!

Sequence of pulses without a field

Do we see the same experimentally?

Ostler

et al. Nat.

Commun

.

3

, 666 (2012).Slide27

Experimental Verification: GdFeCo Microstructures

XMCD

2

m

m

Experimental observation of magnetisation after each pulse.

Initial state

- two microstructures with opposite magnetisation

-

Seperated

by distance larger than radius (no coupling)

Ostler

et al. Nat.

Commun

.

3

, 666 (2012).Slide28

Beyond magnetization

How can we explain the observed effects in GdFeCo?

Suggests something is occurring on microscopic level

No symmetry breaking external source.Slide29

To obtain information on the distribution of modes in the Brillouin zone we calculate the intermediate structure factor:

For each time-step we obtain S(q). We then apply Gaussian smoothing.0.00.2

0.40.6

0.8

1.0

Γ

Χ

Μ

3D FFT

Intermediate structure factor (ISF)

Normalized AmplitudeSlide30

Below switching threshold

No significant change in the ISFAbove switching thresholdExcited region during switching2 bands excited

975K

M/2

X

/2

1090K

FeCo

Gd

M/2

X

/2

Intermediate structure factor (ISF)

ISF

distribution of modes even out of equilibrium.

J. Barker, T. Ostler

et al. Nature Scientific Reports,

3

,

3262 (2013).Slide31

Relative Band Amplitude

Dynamic structure factor (DSF)

To calculate the spinwave dispersion from the atomistic model we calculate the DSF.

The point (in k-space) at which both bands are excited corresponds to the spinwave excitation (ISF).

1090K

FeCo

Gd

M/2

X

/2

J. Barker, T. Ostler

et al. Nature Scientific Reports,

3

,

3262 (2013).Slide32

Frequency gap

By knowing at which point in k-space the excitation occurs, we can determine a frequency (energy) gap.

This can help us understand why we do not get switching at certain concentrations of Gd.

Overlapping bands allows for efficient transfer of energy.

Large band gap precludes efficient energy transfer.

J. Barker, T. Ostler

et al. Nature Scientific Reports,

3

,

3262 (2013).Slide33

What is the significance of the excitation of both bands?

Excitation of only one band leads to demagnetization.Excitation of both bands simultaneously leads to the transient ferromagnetic-like state.

J. Barker, T. Ostler

et al. Nature Scientific Reports,

3

,

3262 (2013).Slide34

Summary

Slides available at:http://tomostler.co.uk/list-of-publications/conference-presentations/

Field limit of magnetization switching.

The atomistic spin dynamics model of ultrafast magnetization dynamics.

How we model femtosecond laser heating.

Demagnetization and switching experiments and theory.

How we switch without a field.