J Cuevas, C Katerji, B Sánchez-Rey and A Álvarez Non Linear Physics Group of the University of...

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J Cuevas, C Katerji, B Sánchez-Rey and A Álvarez Non Linear Physics Group of the University of Seville Department of Applied Physics I February 21st, 2003 Influence of moving breathers on vacancies migration

Transcript of J Cuevas, C Katerji, B Sánchez-Rey and A Álvarez Non Linear Physics Group of the University of...

Page 1: J Cuevas, C Katerji, B Sánchez-Rey and A Álvarez Non Linear Physics Group of the University of Seville Department of Applied Physics I February 21st, 2003.

J Cuevas, C Katerji, B Sánchez-Rey and A Álvarez

Non Linear Physics Group of the University of SevilleDepartment of Applied Physics I

February 21st, 2003

Influence of moving breathers on vacancies migration

Page 2: J Cuevas, C Katerji, B Sánchez-Rey and A Álvarez Non Linear Physics Group of the University of Seville Department of Applied Physics I February 21st, 2003.

• Previous: Experimental evidence

• Model

• Vacancy

• MB & vacancy

• Results

Outline

Page 3: J Cuevas, C Katerji, B Sánchez-Rey and A Álvarez Non Linear Physics Group of the University of Seville Department of Applied Physics I February 21st, 2003.

X

X

X

X

X radiation (Ag)

Experimental evidence: defects migrate

sample (Si)

X

X

X

X

X

XX

X

XX

XX

X

XX

layer (Ni)

1

2

43

Page 4: J Cuevas, C Katerji, B Sánchez-Rey and A Álvarez Non Linear Physics Group of the University of Seville Department of Applied Physics I February 21st, 2003.

-1 0 1 2 3 40

0.1

0.2

0.3

0.4

0.5

0.6

0.7

0.8

0.9

1Morse potentials

x

W(x

)

-0.5 0 0.5 1 1.5 2 2.5 3 3.50

0.01

0.02

0.03

0.04

0.05

0.06sine-Gordon potential

x

V(x

)

The model

Frenkel-Kontorova + anharmonic interaction

21)(exp2

1 axbxW

1L 1a

L

xLxV

2cos1

4 2

2

Page 5: J Cuevas, C Katerji, B Sánchez-Rey and A Álvarez Non Linear Physics Group of the University of Seville Department of Applied Physics I February 21st, 2003.

Plane waves (phonons)

The Hamiltonian:

1

'2

2

1 nn

nnn xxWCxVxH

02 11'2 nnnnn xxxCbxx

2sin4 22

02 q

Cph

tqnin

phextx 0

'2CbC

9.0bb

bT2

nnnnn

nn axxbaxxbC

L

xLxH 2

1

2

1

'

2

22 1)(exp

2

11)(exp

2

12cos1

42

1

The linearized equations:

Dispersion relation

2sin4 2'22

02 q

Cbph

Frecuency breather:

,,

1 ,, 0

Page 6: J Cuevas, C Katerji, B Sánchez-Rey and A Álvarez Non Linear Physics Group of the University of Seville Department of Applied Physics I February 21st, 2003.

vn1vn 1vn

The vacancy

Page 7: J Cuevas, C Katerji, B Sánchez-Rey and A Álvarez Non Linear Physics Group of the University of Seville Department of Applied Physics I February 21st, 2003.

nx

nv 22

2

1

2

1 vK

0,,0,

2

1,0,

2

1,0,,00

v

0vv

The moving breather

Energy added to the breather:

Page 8: J Cuevas, C Katerji, B Sánchez-Rey and A Álvarez Non Linear Physics Group of the University of Seville Department of Applied Physics I February 21st, 2003.

0 0.13

03.02

Gaussian distribution

K Forinash, T Cretegny and M Peyrard.

Local modes and localization in a multicomponent nonlinear lattices. Phys. Rev. E, 55:4740, 1997.

Analysis:

• b (Morse potential)

The moving breather

Page 9: J Cuevas, C Katerji, B Sánchez-Rey and A Álvarez Non Linear Physics Group of the University of Seville Department of Applied Physics I February 21st, 2003.

Three types of phenomena

i) The vacancy moves backwards.

ii) The vacancy moves forwards.

iii) The vacancy remains at its site.

Page 10: J Cuevas, C Katerji, B Sánchez-Rey and A Álvarez Non Linear Physics Group of the University of Seville Department of Applied Physics I February 21st, 2003.

vn1vn 1vn

MB

vn

i) The most probably is that the vacancy moves backwards

Page 11: J Cuevas, C Katerji, B Sánchez-Rey and A Álvarez Non Linear Physics Group of the University of Seville Department of Applied Physics I February 21st, 2003.

vn1vn 1vn

MB

ii) But the vacancy can move forwards

vn

Page 12: J Cuevas, C Katerji, B Sánchez-Rey and A Álvarez Non Linear Physics Group of the University of Seville Department of Applied Physics I February 21st, 2003.

vn1vn 1vn

MB

iii) And the vacancy can stay motion-less

Page 13: J Cuevas, C Katerji, B Sánchez-Rey and A Álvarez Non Linear Physics Group of the University of Seville Department of Applied Physics I February 21st, 2003.

C=0.4

remainsforwards

backwards

Probability

Probability of the vacancy’s movement

Page 14: J Cuevas, C Katerji, B Sánchez-Rey and A Álvarez Non Linear Physics Group of the University of Seville Department of Applied Physics I February 21st, 2003.

C=0.5

backwards

forwards remains

Probability

Probability of the vacancy’s movement

Page 15: J Cuevas, C Katerji, B Sánchez-Rey and A Álvarez Non Linear Physics Group of the University of Seville Department of Applied Physics I February 21st, 2003.

vn1vn 1vn

b

bMorse potentials

The coupling forces

Page 16: J Cuevas, C Katerji, B Sánchez-Rey and A Álvarez Non Linear Physics Group of the University of Seville Department of Applied Physics I February 21st, 2003.

C=0.5

backwards

forwards remains

Probability

Probability of the vacancy’s movement

Page 17: J Cuevas, C Katerji, B Sánchez-Rey and A Álvarez Non Linear Physics Group of the University of Seville Department of Applied Physics I February 21st, 2003.

C=0.4

remainsforwards

backwards

Probability

Probability of the vacancy’s movement

Page 18: J Cuevas, C Katerji, B Sánchez-Rey and A Álvarez Non Linear Physics Group of the University of Seville Department of Applied Physics I February 21st, 2003.

C=0.4

bifurcation

11 vv nn uu

vn

Page 19: J Cuevas, C Katerji, B Sánchez-Rey and A Álvarez Non Linear Physics Group of the University of Seville Department of Applied Physics I February 21st, 2003.

C=0.5

bifurcation

11 vv nn uu

vn

Page 20: J Cuevas, C Katerji, B Sánchez-Rey and A Álvarez Non Linear Physics Group of the University of Seville Department of Applied Physics I February 21st, 2003.

C=0.4

nx

Amplitude maxima of a vacancy breather

bifurcation

Page 21: J Cuevas, C Katerji, B Sánchez-Rey and A Álvarez Non Linear Physics Group of the University of Seville Department of Applied Physics I February 21st, 2003.

C=0.5

nx

Amplitude maxima of a vacancy breather

bifurcation

Page 22: J Cuevas, C Katerji, B Sánchez-Rey and A Álvarez Non Linear Physics Group of the University of Seville Department of Applied Physics I February 21st, 2003.

Conclusions

• The moving breathers can move vacancies.

• The behaviour is very complex and it depends of the values of the coupling.

• The changes of the probabilities of the different movements of the vacancies are related with the existence of bifurcations.

• Is there a more rich complexity from 1-dim to 2-dim ?

Thank you very much.