Langevin Molecular Dynamics of Driven Magnetic Flux Lines Ulrich - - PowerPoint PPT Presentation

langevin molecular dynamics of driven magnetic flux lines
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Langevin Molecular Dynamics of Driven Magnetic Flux Lines Ulrich - - PowerPoint PPT Presentation

Langevin Molecular Dynamics of Driven Magnetic Flux Lines Ulrich Dobramysl, Michel Pleimling and Uwe C. T auber Department of Physics, Virginia Tech, Blacksburg, VA, USA SESAPS Meeting, Roanoke, VA, October 22, 2011 Motivation Type II


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SLIDE 1

Langevin Molecular Dynamics of Driven Magnetic Flux Lines

Ulrich Dobramysl, Michel Pleimling and Uwe C. T¨ auber

Department of Physics, Virginia Tech, Blacksburg, VA, USA

SESAPS Meeting, Roanoke, VA, October 22, 2011

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SLIDE 2

Motivation

◮ Type II superconductors exhibit a

second order phase transition from superconducting to normal state

◮ Magnetic flux penetrates above

critical field Hc1 through vortex lines - each one carries a flux quantum

◮ Vortex lines movement generates dissipation ◮ Pinning by (artificially introduced) defect sites - optimization ◮ Complex and rich system that is accessible in experiments ◮ High TC SC - interesting for technology and applications

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SLIDE 3

Elastic Line Model

After coarse graining: Vortex lines are interacting elastic lines† Fel =

N

  • j=1

L dz  ǫ1 2

  • d

r dz

  • 2

+ 1 2

N

  • i=j

VI(| rij|) + VD( rj)  

◮ Elastic energy ǫ1 (stiffness) ◮ Line interaction energy VI(|

rij|) ∝ K0(| rij|)

◮ Defects potential VD(

r) due to pin sites

◮ This work: only random point defects

Discretize lines into connected particles → simulations

†D.R. Nelson and VM Vinokur PRB 48 13060 (1993), T.

Klongcheongsan, TJ Bullard, and UC T¨ auber, Supercond Sci Tech 23 025023 (2010)

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SLIDE 4

Visualization

LMD simulation of interacting vortex lines in clean system → form hexagonal lattice t = 0

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SLIDE 5

Methods

Monte Carlo Find steady state by performing a biased random walk on the energy landscape

◮ Problem: external drive enters energy - not well defined for

relaxation into non-equilibrium steady-state Langevin Molecular Dynamics Algorithm Solve the system of coupled Langevin equations ¨

  • ri = −ζ ˙
  • ri +

F({ rj}) +

  • 2ζkBT

R(t)

◮ Additional random force term

η describing fast degrees of freedom - temperature bath

◮ Gaussian white noise Ri(t)Rj(t′) = δijδ(t − t′) ◮ Problem: also not well defined for non-equilibrium (driven)

systems

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SLIDE 6

Time regimes

Transient regime

◮ Dependent on inital

conditions

◮ Dynamical scaling - aging ◮ Time translation invariance

broken

◮ Need two-time quantities to

characterize Steady state

◮ Time translation invariance

recovered

◮ No dependence on initial

conditions

◮ All quantities stationary in

thermodynamic limit

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SLIDE 7

Driven system results

0.4 0.5 0.6 0.7 0.8 0.9 1.0 1.1

Driving force Fd

0.00 0.25 0.50 0.75 1.00

Normalized velocity v/v0

16 lines 32 lines 64 lines LMD MC

0.4 0.5 0.6 0.7 0.8 0.9 1.0 1.1

Driving force Fd

2 4 6 8 10

Gyration radius rg

16 lines 32 lines 64 lines LMD MC

◮ 16, 32 or 64 initially straight lines placed at random positions ◮ 34200 randomly distributed point defects ◮ Driven system, allowed to relax into steady state ◮ Agreement between MC and LMD good

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SLIDE 8

Two-time height-height autocorrelation

LMD yields similar results as previously performed MC simulations† No defect sites

10-1 100 101 102 103 104

t−s

10-3 10-2 10-1 100

C(t,s)

4 8 16 32 64

0.0 0.5 1.0 1.5 2.0

ln(t/s)

7.0 6.5 6.0 5.5

ln(s−0.5 C(t,s))

128 256 512 1024

◮ Dynamical scaling - aging

exponent ≈ 0.5 Disordered system

10-1 100 101 102 103 104

t−s

0.3 0.4 0.5 0.6 0.7 0.8 0.9 1.0 1.1

C(t,s)/C(s,s) ◮ Disorder leads to glass-like

relaxation

†M. Pleimling and U.C. T¨

auber, arXiv:1106.1130 (2011)

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SLIDE 9

Summary

Conclusion

◮ Complex out-of-equilibrium system ◮ Important to understand vortex dynamics to optimize

technological applications

◮ Both methods yield comparable results - complementary to

each other

◮ LMD is much more efficient

Outlook

◮ Aging regime – universality/scaling ◮ Correlated defects ◮ Thin films ◮ Relaxation of driven systems

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SLIDE 10

Thank you for your attention!

References

◮ D.R. Nelson and VM Vinokur PRB 48 13060 (1993) ◮ T. Klongcheongsan, TJ Bullard, and UC T¨

auber, Supercond Sci Tech 23 025023 (2010)

◮ M. Pleimling and U.C. T¨

auber, arXiv:1106.1130 (2011) This research was funded by the Department of Energy, grant number BES DE-FG02-09ER46613.