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Theory
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Theory

• Isotropic Thermal Expansion

• Phase Transitions

• Lagrange Strain Tensor

• Anisotropic Thermal Expansion

• Magnetostriction

• Matteucci effect

• Villari Effect

• Wiedemann Effect

• Saturation Magnetostriction

• (Phenomenological Description, Symmetry Considerations)

• Band Magnetostriction

• Local Moment Magnetostriction (Crystal Field & Exchange Striction)









M.Rotter „Magnetostriction“ Course Lorena 2007 1

Isotropic Thermal Expansion

 ln V T , P 

Thermal expansion Coefficients 

T P







 ln V T , P  PT , V  PT , V 

    T

P T T V T V



Helmholtz free Energy dF  SdT  PdV



1

1 V T , P  1   F T ,V  

2



Compressibility T     

V P T V   V

2

T





M.Rotter „Magnetostriction“ Course Lorena 2007 2

 2 F T ,V  S T ,V 

   T  T

TV V T



Approximation: compressibility is T independent

(dominated by electrostatic part of binding energy)



S r T , V 

 (T )    r   T 

r r V T





Subsystem r ..... phonons, electrons,

magnetic moments









M.Rotter „Magnetostriction“ Course Lorena 2007 3

Phase

Transitions









M.Rotter „Magnetostriction“ Course Lorena 2007 4

   

x'  x  u ( x)

Mechanics of Solids - i=1,2,3

Kinematics





Inf. Translation





Inf. Rotation Inf. Strain

(antisymmetric matrix) (symmetric matrix)

 0 3  2 

     

dx '    dx    3 0 1 dx

  1 0 

 2 







Volume Strain





M.Rotter „Magnetostriction“ Course Lorena 2007 5

Lagrange Strain Tensor

The strain tensor, ε, is a symmetric tensor used to quantify the strain of an object

undergoing a small 3-dimensional deformation:

• the diagonal coefficients εii are the relative change in length in the direction

of the i direction (along the xi-axis) ;

• the other terms εij = 1/2 γij (i ≠ j) are the shear strains, i.e. half the variation

of the right angle (assuming a small cube of matter before deformation).

The deformation of an object is defined by a tensor field, i.e., this strain tensor is

defined for every point of the object. In case of small deformations, the strain



tensor is the Green tensor or Cauchy's infinitesimal strain tensor, defined by

the equation:







Where u represents the displacement field of the object's

configuration (i.e., the difference between the object's

configuration and its natural state). This is the 'symmetric

part' of the Jacobian matrix. The 'antisymmetric part' is

called the small rotation tensor.

M.Rotter „Magnetostriction“ Course Lorena 2007 6

T stress tensor is defined by:







where the dFi are the components of the

resultant force vector acting on a small

area dA which can be represented by a

vector dAj perpendicular to the area

element, facing outwards and with

length equal to the area of the element.

In elementary mechanics, the subscripts

are often denoted x,y,z rather than 1,2,3.





Stress tensor is symmetric, otherwise the volume element would

rotate (to seet this look at zy and yz component in figure)

6



Hookes Law     c  

 1



(Voigt) notation 1 = 11, 2 = 22 3 = 33 4 = 23 5 = 31 6 = 12

M.Rotter „Magnetostriction“ Course Lorena 2007 7

Anisotropic Thermal Expansion

dF  SdT  V  d 

1 6

Elastic Energy density    d    c    

2  1

1 F (T ,  )

.... strain can be written as   

V  

   T ,  

Thermal expansion Coefficients  

T

 

Elastic Constants c 

  6



 c s    

    1

Elastic Compliances s 



M.Rotter „Magnetostriction“ Course Lorena 2007 8

  T ,   6

  T ,    6

s   2 F 6

s  S

      

 

T  1  T  1 V T  1 V 









.... this can (as in the isotropic case) be written as

sum of contributions of subsystems r = phonons,

electrons, magnetic moments



  r T ,   6

s  S r

  

 

r    

r r T r  1 V 









s  Fr

6

     r  

r r  1 V   T , 0







M.Rotter „Magnetostriction“ Course Lorena 2007 9

Grueneisens Approximation



S r



   cV

r r





• Specific heat of subsystem r

• Grueneisen Parameter of

subsystem r ... Is in many

simple model cases

temperature independent



s  r r

6

  (T )     r     c V (T )

r r  1 V



M.Rotter „Magnetostriction“ Course Lorena 2007 10

Normal thermal Expansion

Anharmonicity of C

u

Y

.0

0

10 2

lattice dynamics

.9

9

09

a

anharmonic .8

9

09

Potential

.7

9

09





c







Giterpametr,normiertauf30K

.6

9

09

b

.5

9

09



Harmonic

potential 0 0 5 0 5 0

0 0 0 0 0

0 5 1 1 2 2 3

[

K

T]

l

    el   phon  K1T 2  K 2TD( D / T )

+ Small l

contribution of z 3

3 x dx

z3  e x 1

band electrons with Debye function D( z ) 

0

Magnetostriction



Magnetostriction is a property of magnetic materials that

causes them to change their shape when subjected to a magnetic

field. The effect was first identified in 1842 by James Joule

when observing a sample of nickel.









James Prescott Joule, (1818 – 1889)



M.Rotter „Magnetostriction“ Course Lorena 2007 12

 



 





  T , H

Thermal expansion Coefficients  T, H 

T

 



 





  T , H

Magnetostriction Coefficients  T, H 

H

H









 

 

 



 



 

l||   T , H || e

l   T , H || e





 

 

 

l   T , H  e



Material Crystal axis Saturation magnetostriction

l|| (x 10-5)

Fe 100 +(1.1-2.0)

Fe 111 -(1.3-2.0)

Fe polycristal -0.8

Terfenol-D 111 200

M.Rotter „Magnetostriction“ Course Lorena 2007 13

Villari Effect the change of the susceptibility of a material

when subjected to a mechanical stress

Matteucci effect creation of a helical anisotropy of the

susceptibility of a magnetostrictive material

when subjected to a torque

Wiedemann Effect twisting of materials when an helical magnetic

field is applied to them









M.Rotter „Magnetostriction“ Course Lorena 2007 14

Domain Effects

rotation of the domains.

T>TC TTN

kT >>cf kT TN

kT >>cf kT TN





…spontaneous

magnetostriction T matrix elements

M   g  B tanh( g  B ( H  lM ) /( 2kT ))

P. Svoboda et al. JMMM 104 (1992) 1329

  a, b, c

g a / g J   J y   2.1

g b / g J   J z   2.8

g c / g J   J x   1.5









M.Rotter „Magnetostriction“ Course Lorena 2007 47

How to start analysis – the story

of NdCu2

• Neutron TOF spectroscopy – CF levels

... Blm Gratz et. al., J. Phys.: Cond. Mat. 3 (1991) 9297









B20=1.35 K

B22=1.56 K

B40=0.0223 K

B42=0.0101 K

B44=0.0196 K

B60=4.89x10-4 K

B62=1.35x10-4 K

B64=4.89x10-4 K

B66=4.25 x10-3 K

M.Rotter „Magnetostriction“ Course Lorena 2007 48

The story of NdCu2

• Thermal expansion – cf influence

... Magnetoelastic parameters (A=dB20/dε, B=dB22/dε)









E. Gratz et al., J. Phys.: Condens. Matter 5, 567 (1993)





M.Rotter „Magnetostriction“ Course Lorena 2007 49

The story of NdCu2

• Neutron diffraction+ magnetization:

magstruc, phasediag H||b-> model

... Jbb

M. Loewenhaupt et al., Z. Phys. B:

Condens. Matter 101, 499 (1996)





n(k)=sum of Jbb(ij) with ij being of bc plane k

f(B) [arb.units] T=0K

BcAF1F3 B

Bc1  AF1





Bc2

 Bc3



F1



F2



F3

NdCu2 Magnetic Phase Diagram

F1   



F3 

c



F1 

b

a



AF1 

lines=experiment









M.Rotter „Magnetostriction“ Course Lorena 2007 51

The story of NdCu2

Jaa=Jcc(R)

• Neutron spectroscopy on single crystals in H||b=3T

... Anisotropy of J(ij) - determination of Jaa=Jcc







F3 









M. Rotter et al., Eur. Phys. J. B 14, 29 (2000)





M.Rotter „Magnetostriction“ Course Lorena 2007 52

F3  NdCu2









F1 









AF1

M. Rotter, et al. Applied Phys. A 74 (2002) s751 

How to start analysis – the story

of NdCu2

• Magnetostriction ... Confirmation of phasediagram model for H||a,b,c, and

determination of dJ(ij)/dε









M. Rotter, et al. J. of Appl. Physics 91 10(2002) 8885

M.Rotter „Magnetostriction“ Course Lorena 2007 55

McPhase - the World of Rare Earth Magnetism

McPhase is a program package for the calculation of

magnetic properties of rare earth based systems.

Magnetization Magnetic Phasediagrams









Magnetic Structures Elastic/Inelastic/Diffuse

Neutron Scattering

Cross Section









M.Rotter „Magnetostriction“ Course Lorena 2007 56

Crystal Field/Magnetic/Orbital Excitations









Magnetostriction









and much more....





M.Rotter „Magnetostriction“ Course Lorena 2007 57

Epilog

McPhase runs on Linux and Windows and is available as freeware.

www.mcphase.de



McPhase is being developed by

M. Rotter, Institut für Physikalische Chemie, Universität Wien, Austria

M. Doerr, R. Schedler, Institut für Festkörperphysik,

Technische Universität Dresden, Germany

P. Fabi né Hoffmann, Forschungszentrum Jülich, Germany

S. Rotter, Wien, Austria

M.Banks, Max Planck Institute Stuttgart, Germany



Important Publications referencing McPhase:

• M. Rotter, S. Kramp, M. Loewenhaupt, E. Gratz, W. Schmidt, N. M. Pyka, B.

Hennion, R. v.d.Kamp Magnetic Excitations in the antiferromagnetic phase of

NdCu2 Appl. Phys. A74 (2002) S751

• M. Rotter, M. Doerr, M. Loewenhaupt, P. Svoboda, Modeling Magnetostriction

in RCu2 Compounds using McPhase J. of Applied Physics 91 (2002) 8885

• M. Rotter Using McPhase to calculate Magnetic Phase Diagrams of Rare Earth

Compounds J. Magn. Magn. Mat. 272-276 (2004) 481



M.Rotter „Magnetostriction“ Course Lorena 2007 58


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