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Ultrafast Magnetization Dynamics. T. Ostler 1 Dept . of Physics, The University of York, York, United Kingdom . December 2013. Increasing demand. 100TB storage. 25TB daily log. A few GB to TB’s. 2.5PB. 24PB daily. 330 EB demand in 2011. Estimated size of the internet 4ZB.

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ultrafast magnetization dynamics

Ultrafast Magnetization Dynamics

T. Ostler1

Dept. of Physics, The University of York, York, United Kingdom.

December 2013

slide2
Increasing demand

100TB storage

25TB daily log

A few GB to TB’s

2.5PB

24PB daily

330 EB demand in 2011

Estimated size of the internet 4ZB

slide3
Increasing demand

Now at 175million

Users [millions]

Months

  • If all storage demand was met by SSD’s/flash etc, $250 billion in plant construction is required.
  • Faster data access/writing is desirable.
slide4
Write speed challenge
  • In 1953 IBM launched first commercial HHD with average data access times of just under 1 second!

Me

IBM 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

Enterprise drive

CD @ 1x

How fast can we go?

Faster write times

Pulsed fields

slide7
Towards femtosecond processes
  • Magnetic field processes.
  • Atomistic spin dynamics model for magnetization dynamics.
    • LLG
    • How we construct such a model
    • Including laser heating + parameterization
    • Limitations of the model
  • Finally femtosecond lasers processes.
  • Conclusion: reversal in hundreds of fs using laser without applied field.
  • Mechanism for switching without a field.
precession and damping
Precession and 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.

Landau-Lifshitz-Gilbert (LLG) equation

Precession

Damping

ultrafast field switching in 200ps
Ultrafast field switching in 200ps
  • GaAsphotoswitches excited by fs laser pulse creates initial field.
  • Permally thin film, in-plane.
  • High field and low damping causes ringing oscillations in magnetization.

Figures from :Nature, 418, 509-512 (2002).

  • GaAsphotoswitches excited by fs laser pulse creates initial field.
  • Second pulses (at a very specific delay time) can stop magnetization.
  • Reversal complete in 200 picoseconds.
slide10
Can we go faster?
  • Control of magnetization dynamics in applied field limited by precession time.
  • There are a number of other ways to control magnetization:
    • Spin transfer torque
    • Heat assisted magnetic recording
  • The exchange interaction gives rise to magnetic order.
  • The strongest force in magnetism. Can we excite processes on this timescale?

Timescale:

10’s -> 100’s fs

slide11
Femtosecond laser heating and measurement

E

E

  • Rotation (θf) of polarization plane.
  • χ: susceptibility tensor
  • k: wave-vector
  • n: refractive index

θF~MZ

M

Faradayeffect

Fast demagnetization of Ni

  • MOKE in transmission.
  • Using femtosecond laser pulses Beaurepaire showed fs demagnetization.
  • Demagnetization in around 1ps. Remagnetization in a few ps.
  • Can we model this?

Beaurepaireet al. PRL, 76, 4250 (1996).

time scale length scale
Time-scale/Length-scale

Length

10-10 m (Å)

10-9 m (nm)

10-6 m (μm)

10-3 m (mm)

TDFT/ab-initio spin dynamics

10-16 s (

10-15 s (fs)

Superdiffusive spin transport

10-12 s (ps)

Langevin Dynamics on atomiclevel

Micromagnetics/LLB

Time

10-9 s (ns)

10-6 s (µs)

Kinetic Monte Carlo

10-3 s (ms)

10-0 s (s)+

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

http://www.castep.org/

slide13
The spin dynamics model
  • Assume fixed atomic positions
  • Processes 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-Dipole

slide14
How do we find J/D/μ?
  • Anisotropy can also be calculated from first principles.
  • Possible to have other anisotropy terms:
    • Surface
    • Cubic
    • Etc.
  • Jij can be found from DFT. Adiabatic approximation assuming electron motion much faster than spinwaves.
  • Assume frozen magnon picture
  • Spin 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

sc

bcc

fcc

slide15
Magnetization dynamics

Static properties: M(T), hysteresis

What can we calculate?

Distribution of spinwave energies

Spinwave dispersion

slide16
The spin dynamics model

Heat bath

  • Damping is phenomenological.
  • Energy exchange is to/from bath and magnon-magnon interactions.

Spinwaves

slide17
Modelling temperature effects

Damping

Precession

Noise

slide18
Laser heating

Chen et al. Int. Journ. Heat and Mass Transfer.49, 307-316 (2006)

slide19
How can the electron temperature be determined?

Usually known from literature

Fitting initial decay to an exponential

Final temperature determines

Figure from Atxitiaet al. Phys. Rev. B. 81, 174401 (2010).

slide20
Laser heating

Experiment

Theory

  • What governs the time-scale for demagnetization?
  • Can we control it?
  • What happens if we have multiple species?
slide21
Two sublattices

Jij>0

Jij<0

Model calculations

Two sublattice ferromagnet

Two sublattice ferrimagnet

  • 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
  • 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.

Radu, Ostler et al. submitted.

More details arXiv:1308.0993

slide25
Can we actually do something useful?
  • Controlling demagnetization is interesting but can we actually do something with it?

Element-resolved dynamics.

  • Switching in a magnetic field
  • Some interesting behaviour

Experiment

Model results

Transient ferromagnetic-like state

Reversal of the sublattices

Different demagnetization times

Initial State

Raduet al. Nature, 472, 205-208 (2011).

slide26
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).

experimental verification gdfeco microstructures
Experimental Verification: GdFeCo Microstructures

Initial state

- two microstructures with opposite magnetisation

- Seperated by distance larger than radius (no coupling)

2mm

XMCD

Experimental observation of magnetisation after each pulse.

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
Intermediate structure factor (ISF)
  • To obtain information on the distribution of modes in the Brillouin zone we calculate the intermediate structure factor:

3D FFT

1.0

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

0.8

0.6

Normalized Amplitude

0.4

0.2

0.0

Χ

Γ

Μ

slide30
Intermediate structure factor (ISF)
  • ISF  distribution of modes even out of equilibrium.

975K

Above switching threshold

Below switching threshold

X/2

FeCo

1090K

Gd

M/2

X/2

M/2

No significant change in the ISF

Excited region during switching

2 bands excited

  • J. Barker, T. Ostler et al. Nature Scientific Reports, 3, 3262 (2013).
slide31
Dynamic structure factor (DSF)
  • To calculate the spinwave dispersion from the atomistic model we calculate the DSF.

Relative Band Amplitude

FeCo

1090K

Gd

X/2

M/2

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

Overlapping bands allows for efficient transfer of energy.

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

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).
summary
Summary
  • 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.

Slides available at:

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

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