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Magnetic Neutron Diffraction for Magnetic Structure Determination. - - PowerPoint PPT Presentation

Magnetic Neutron Diffraction for Magnetic Structure Determination. Instruments and Methods Juan Rodrguez-Carvajal Institut Laue-Langevin, Grenoble, France E-mail: jrc@ill.eu 1 Outline: 1. Impact of magnetic structures in condensed matter


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Magnetic Neutron Diffraction for Magnetic Structure Determination. Instruments and Methods

Juan Rodríguez-Carvajal Institut Laue-Langevin, Grenoble, France E-mail: jrc@ill.eu

1

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Outline:

  • 1. Impact of magnetic structures in condensed

matter physics and chemistry.

  • 2. The basis of Neutron Diffraction for Magnetic
  • structures. Instruments at ILL
  • 3. Magnetic Crystallography: Shubnikov groups

and representations, superspace groups

2

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Impact of Magnetic structures

Search in the Web of Science, TOPIC: (("magnetic structures" or "magnetic structure" or "spin configuration" or "magnetic ordering" or "spin ordering") and ("neutron" or "diffraction" or "refinement" or "determination"))

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Impact of Magnetic structures

Multiferroics Methods and Computing Programs

Superconductors

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Impact of Magnetic structures

Heavy Fermions

Nano particles Multiferroics Manganites, CO, OO Computing Methods

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Impact of Magnetic structures

Search with Topic = “Magnetic structure” or “magnetic structures”

Thin Films

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Impact of Magnetic structures

The impact of the magnetic structures as a field in physics and chemistry of condensed matter is strongly related to (1) the availability of computing tools for handling neutron diffraction data (2) adequate neutron instruments and to (3) the emergence of relevant topics in new materials.

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Impact of Magnetic structures

It is expected an increase of the impact of magnetic structures in the understanding of the electronic structure of materials with important functional properties.

  • Thin films
  • Multiferroics and magnetoelectrics
  • Superconductors
  • Thermoelectrics and magnetocalorics
  • Topological insulators
  • Frustrated magnets
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Outline:

  • 1. Impact of magnetic structures in condensed

matter physics and chemistry.

  • 2. The basis of Neutron Diffraction for Magnetic
  • structures. Instruments at ILL
  • 3. Magnetic Crystallography: Shubnikov groups

and representations, superspace groups

9

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Historical milestones: Halpern et al. (1937-1941): First comprehensive theory of

magnetic neutron scattering (Phys Rev 51 992; 52 52; 55 898; 59 960)

Blume and Maleyev et al. (1963)

Polarisation effects in the magnetic elastic scattering of slow neutrons.

  • Phys. Rev. 130 (1963) 1670
  • Sov. Phys. Solid State 4, 3461

Moon et al. (1969)

Polarisation Analysis of Thermal Neutron scattering

  • Phys. Rev. 181 (1969) 920

10

History: Magnetic neutron scattering

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Magnetic Structures Pictures

How we get the information to construct these kind of pictures?

Thanks to Navid Qureshi for the pictures!

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Magnetic scattering: Fermi’s golden rule

Differential neutron cross-section:

This expression describes all processes in which:

  • The state of the scatterer changes from  to ’
  • The wave vector of the neutron changes from k to k’ where k’

lies within the solid angle d

  • The spin state of the neutron changes from s to s’

2 2 2 ' 2 ' '

' ' ' ' ( ) ' 2 k k

n m s s

m d k s V s E E d dE k

   

      

               Vm = n.B is the potential felt by the neutron due to the magnetic field created by moving electrons. It has an orbital an spin part.

12

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Magnetic scattering: magnetic fields

Magnetic field due to spin and orbital moments of an electron:

2 2

ˆ ˆ 2 4 μ R p R B B B

j j B j jS jL

R R                            

13

O Rj sj j pj R R+Rj

σn μn

Bj Magnetic vector potential

  • f a dipolar field due to

electron spin moment Biot-Savart law for a single electron with linear momentum p

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Magnetic scattering: magnetic fields

Evaluating the spatial part of the transition matrix element for electron j: ˆ ˆ ˆ ' exp( ) ( ) ( ) k k QR Q s Q p Q

j m j j j

i V i Q            ( ') Q k k   Where is the momentum transfer

14

Summing for all unpaired electrons we obtain: ˆ ˆ ˆ ˆ ' ( ( ) ) ( ) ( ( ). ). ( ) k k Q M Q Q M Q M Q Q Q M Q

j m j

V

     

M(Q) is the perpendicular component of the Fourier transform of the magnetisation in the scattering object to the scattering vector. It includes the orbital and spin contributions.

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M(Q) is the perpendicular component of the Fourier transform of the magnetisation in the sample to the scattering vector. Magnetic interaction vector Magnetic structure factor: Neutrons only see the component of the magnetisation that is perpendicular to the scattering vector

M M  Q=Q e

Magnetic scattering

15

 

3

( ) ( )exp M Q M r Q·r r i d  

*

M M I

 

  

    e M e M e (e M M)

1

( ) ( )exp(2 · ) M H m H r

mag

N m m m m

p f H i 

 

2 *

( ) M M d r d   

 

      

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Scattering by a collection of magnetic atoms

16

We will consider in the following only elastic scattering. We suppose the magnetic matter made of atoms with unpaired electrons that remain close to the nuclei. R R r

e lj je

 

( ) exp( · ) exp( · ) exp( · ) M Q s Q R Q R Qr s

j

e e lj je je e lj e

i i i  

  

3 3

( ) exp( · ) ( )exp( · ) ( ) ( )exp( · ) ( ) F Q s Q ρ r Qr r F Q m r Qr r m

j je je j e j j j j j

i r i d i d f Q     

  

( ) ( )exp( · ) M Q m Q R

lj lj lj lj

f Q i  

Vector position of electron e: The Fourier transform of the magnetization can be written in discrete form as

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Scattering by a collection of magnetic atoms

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3 3

( ) exp( · ) ( )exp( · ) ( ) ( )exp( · ) ( ) F Q s Q ρ r Qr r F Q m r Qr r m

j je je j e j j j j j

i r i d i d f Q     

  

If we use the common variable s=sin/, then the expression of the form factor is the following:

0,2,4,6 2 2

( ) ( ) ( ) ( ) (4 )4

l l l l l

f s W j s j s U r j sr r dr  

 

 

 

 

2 2 2 2 2 2 2

( ) exp{ } exp{ } exp{ } 2,4,6 ( ) exp{ } exp{ } exp{ }

l l l l l l l l

j s s A a s B b s C c s D for l j s A a s B b s C c s D               

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Elastic Magnetic Scattering by a crystal (1)

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( ) ( )exp( · ) M Q m Q R

lj lj lj lj

f Q i  

The Fourier transform of the magnetization of atomic discrete

  • bjects can be written in terms of atomic magnetic moments and

a form factor for taking into account the spread of the density around the atoms For a crystal with a commensurate magnetic structure the content

  • f all unit cell is identical, so the expression above becomes

factorised as: ( ) ( )exp( · ) exp( · ) ( )exp(2 · ) M Q m Qr Q R m Hr

j j j l j j j j l j

f Q i i f Q i   

  

The lattice sum is only different from zero when Q=2H, where H is a reciprocal lattice vector of the magnetic lattice. The vector M is then proportional to the magnetic structure factor of the magnetic cell

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Elastic Magnetic Scattering by a crystal (2)

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( ) exp( 2 ) ( )exp(2 · )

k k

M h S kR h R

j l lj lj lj

i f h i    



For a general magnetic structure that can be described as a Fourier series:

( ) ( )exp(2 · ) exp(2 ( )· ) ( ) ( )exp(2 ( )· )

k k k

M h h r S h k R M h S H k r

j j j l j l j j j j

f h i i f Q i       

   

The lattice sum is only different from zero when h-k is a reciprocal lattice vector H of the crystallographic lattice. The vector M is then proportional to the magnetic structure factor of the unit cell that now contains the Fourier coefficients Skj instead of the magnetic moments mj.

 

 

 

k k

kR S m

l j lj

i exp  2

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  • Diff. Patterns of magnetic structures

Magnetic reflections: indexed by a set of propagation vectors {k} h is the scattering vector indexing a magnetic reflection H is a reciprocal vector of the crystallographic structure k is one of the propagation vectors of the magnetic structure ( k is reduced to the Brillouin zone) Portion of reciprocal space Magnetic reflections Nuclear reflections h = H+k

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Blume-Maleyev equations

Cross-section (Equation 1):

   

* * * * * h h h h h h h h h h h

M M M M P M M P

i i

I N N N N i

     

      

Final polarisation (Equation 2):

   

 

   

* * * * * * * * * h h h h h h h h h h h h h h h h h h h

P P M M P P M M P M M M M P M M M M

f i i i i i

I N N i N N N N i

           

            

Polarized Neutrons

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Blume-Maleyev equations

Simplified notation for the Cross-section

   

* * * * *

MM M M P M M P

i i

I NN N N i       

Simplified notation for the Final polarisation

   

 

   

* * * * * * * * *

P P M M P P M M P M M M M P M M M M

f i i i i i

I NN i N N N N i            

Most common case

Polarized Neutrons

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Blume-Maleyev equations

* *

M M I NN

 

 

The simplest case: the major part of experiments using neutron diffraction for determining magnetic structures use non-polarised neutrons The intensity of a Bragg reflection may contains contribution from nuclear and magnetic scattering Nuclear: proportional to the square of the structure factor Magnetic: proportional to the square of the magnetic interaction vector

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Powder diffractometers for magnetic structure determination @ILL:

D20, D1B (CRG-CNRS-CSIC), D2B

Polarised cold neutrons, diffuse scattering: D7

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D1B … the most productive instrument at ILL

High Flux Powder diffractometers @ ILL

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D20 … the most versatile and highest flux

High Flux Powder diffractometers @ ILL

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Single Crystal magnetic diffraction at ILL:

High resolution, magnetism:

D10, D23 (polarised neutrons, CRG-CEA)

High-Q, hot neutrons: D9, D3 (polarised neutrons)

Laue diffractometer: CYCLOPS

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D10 …thermal neutrons, triple axis single crystal diffractometer.

Single Xtal diffractometers at ILL

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Single Crystal Diffractometers

D10

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Projects of the diffraction group @ILL: XtremeD: A diffractometer for extreme

conditions: small samples, high-pressure and magnetic field, powders and single crystals. Upgrade of D10, increase the flux (x 10) for small samples and thin films

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D10: upgrade (single crystals and thin films)

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XtremeD: new diffractometer for magnetism and extreme conditions

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XtremeD: new diffractometer for magnetism

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CryoPAD: instrument to exploit B-M equations

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Polarised neutrons (D3)

Two configurations: High field: Measurement of flipping ratios Output: magnetisation densities Zero field: CryoPAD 3D-Polarimetry Measurement of polarisation tensor Output: Precise magnetic structures

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Blume-Maleyev equations

Matrix form for the scattered polarization.

P P +P

f i

P   

* * *

M M M M W T P

R

N N i I I      

With We have defined the vector W= 2 NM*= WR+i WI that we shall call the nuclear-magnetic interference vector. The vector M* M is purely imaginary, so that T = i(M* M) is a real vector that we shall call the chiral vector.

   

 

   

* * * * * * * * *

P P M M P P M M P M M M M P M M M M

f i i i i i

I NN i N N N N i           

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37

Blume-Maleyev equations

P P +P

f i

P 

The polarization “tensor” is the matrix

 

 

* * * * * *

1 M M M M + M M M M

D S A

P NN i N N I                    

* * * * * *

M M M M M M

N M N M N M

NN I I D NN I I NN I I                            

Diagonal

   

* * * * * * x x y x y z y x y z z z

M M S M M M M M M M M M M                      

Symmetric

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38

Blume-Maleyev equations

P P +P

f i

P 

The polarization “tensor” is the matrix Symmetric

* * * * * * * * * * * * * * *

2 2 2

x x x y x y x z x z x y x y y y y z y z x z x z y z y z z z

M M M M M M M M M M S M M M M M M M M M M M M M M M M M M M M                 

 

 

* * * * * *

1 M M M M + M M M M

D S A

P NN i N N I                    

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39

Blume-Maleyev equations

P P +P

f i

P 

The polarization “tensor” is the matrix

 

 

* * * * * *

1 M M M M + M M M M

D S A

P NN i N N I                    

Anti-Symmetric

* * * * * * * * * * * *

( ) ( ) ( ) ( ) ( ) ( )

z z y y Iz Iy z z x x Iz Ix y y x x Iy Ix

i NM N M i NM N M W W A i NM N M i NM N M W W i NM N M i NM N M W W                                  

Coming from the vectorial product:

 

* *

M M P

i

i N N   

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40

Blume-Maleyev equations

In practice, the scattered polarisation is measured by putting the incident polarisation successively along x, y and z and measuring the components x, y, z of the scattered polarisation for each setting of Pi . The list of the calculated polarisations, to be compared with observations, are gathered in the columns of the following matrix:

( , , )

P

y z Iy x N M M x Iz x x y z y z Iz Ry N M M Ry mix Ry x y z f x y z y z Rz Iy mix Rz N M M Rz x y z

W T I I I T W T I I I W W I I I W M W I I I W W M W I I I W I I I                                     

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41

Blume-Maleyev equations

The terms of the polarization matrix have to be calculated taking into account all kind of possible domains existing in the crystal.

( , , )

P

y z Iy x N M M x Iz x x y z y z Iz Ry N M M Ry mix Ry x y z f x y z y z Rz Iy mix Rz N M M Rz x y z

W T I I I T W T I I I W W I I I W M W I I I W W M W I I I W I I I                                     

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Diffractometers for magnetism in pulsed sources

Currently available: WISH @ ISIS superHRPD @ J-Park Project of Single crystal diffractometer: MAGIC @ ESS

42

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Outline:

  • 1. Impact of magnetic structures in condensed

matter physics and chemistry.

  • 2. The basis of Neutron Diffraction for Magnetic
  • structures. Instruments at ILL
  • 3. Magnetic Crystallography: Shubnikov groups

and representations, superspace groups

  • 4. Computing tools

43

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44

1968: Describing 3-dimensional Periodic Magnetic Structures by Shubnikov Groups Koptsik, V.A. Soviet Physics Crystallography, 12 (5) , 723 (1968) 2001: Daniel B. Litvin provides for the first time the full description of all Shubnikov (Magnetic Space) Groups. Acta Cryst. A57, 729-730

Magnetic Structure Description and Determination

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The magnetic moment (shortly called “spin”) of an atom can be considered as an “axial vector”. It may be associated to a “current loop”. The behaviour of elementary current loops under symmetry operators can be deduced from the behaviour of the “velocity” vector that is a “polar” vector. A new operator can be introduced and noted as 1′, it flips the magnetic moment. This operator is called “spin reversal”

  • perator or classical “time reversal” operator

Time reversal = spin reversal (change the sense of the current)

1′

Magnetic moments as axial vectors

45

' { | } r r t n r r t n=r a

j j h j j h i gj

g h h       

' det( ) m m m

j j j

g h h   

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46

One obtains a total of 1651 Shubnikov groups or four different types. T1: 230 are of the form M0=G (“monochrome” groups) T2: 230 of the form P=G+G1′ (“paramagnetic” or “grey” groups) 1191 of the form M= H + (G  H)1′ (“black-white”, BW, groups). T3: Among the BW group there are 674 in which the subgroup H  G is an equi-translation group: H has the same translation group as G (first kind, BW1). Magnetic cell = Xtal cell T4: The rest of black-white groups, 517, are equi-class group (second kind, BW2). In this last family the translation subgroup contains “anti-translations” => Magnetic cell bigger than Xtal cell

Shubnikov Magnetic Space Groups

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Magnetic structure factor:

Magnetic structure factor

47

*

M M I

 

1

( ) ( )exp(2 · ) M H m H r

mag

N m m m m

p f H i 

 

M e M e M e (e M)

  

   

 

1

( ) det( ) {2 [( { } ]} M H m H t r

n j j j s s s j s j j s

p O f H T h h exp i h

 

 

n independent magnetic sites labelled with the index j The index s labels the representative symmetry operators of the Shubnikov group: is the magnetic moment

  • f the atom sited at the sublattice s of site j.

det( ) m m

js s s s j

h h  

The use of Shubnikov groups implies the use of the magnetic unit cell for indexing the Bragg reflections

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48

Magnetic Structure Description and Determination

Only recently the magnetic space groups are available in a computer database Magnetic Space Groups Compiled by Harold T. Stokes and Branton J. Campbell Brigham Young University, Provo, Utah, USA June 2010 These data are based on data from: Daniel Litvin, Magnetic Space Group Types, Acta Cryst. A57 (2001) 729-730. http://www.bk.psu.edu/faculty/litvin/Download.html

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49

Magnetic Structure Description and Determination

Bertaut is the principal developer of the method base in irreps Representation analysis of magnetic structures E.F. Bertaut, Acta Cryst. (1968). A24, 217-231

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50

Magnetic Structure Description and Determination

Symmetry Analysis in Neutron Diffraction Studies of Magnetic Structures, JMMM 1979-1980 Yurii Alexandrovich Izyumov (1933-2010) He published a series of 5 articles in Journal of Magnetism and Magnetic Materials on representation analysis and magnetic structure description and determination, giving explicit and general formulae for deducing the basis functions

  • f irreps.
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51

Formalism of propagation vectors

A magnetic structure is fully described by: i) Wave-vector(s) or propagation vector(s) {k}. ii) Fourier components Skj for each magnetic atom j and wave-vector k, Skj is a complex vector (6 components) !!!

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52

 

{ 2 }

k k

m S kR

ljs js l

exp i   

js js k k

  • S

S

Necessary condition for real moments mljs  l : index of a direct lattice point (origin of an arbitrary unit cell) j : index for a Wyckoff site (orbit) s: index of a sublattice of the j site General expression of the Fourier coefficients (complex vectors) for an arbitrary site (drop of js indices ) when k and –k are not equivalent:

1 ( )exp{ 2 } 2

k k k k

S R I i i     

Only six parameters are independent. The writing above is convenient when relations between the vectors R and I are established (e.g. when |R|=|I|, or R . I =0)

Formalism of propagation vectors

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53

Magnetic Structure Factor

1

( ) ( ) {2 [( ){ } ]}

k

M h h S H k t r

n j j j js s j j s

p O f T exp i S 

 

 

j : index running for all magnetic atom sites in the magnetic asymmetric unit (j =1,…n ) s : index running for all atoms of the orbit corresponding to the magnetic site j (s=1,… pj). Total number of atoms: N = Σ pj

{ } t s S

Symmetry operators of the propagation vector group or a subgroup

If no symmetry constraints are applied to Sk, the maximum number of parameters for a general incommensurate structure is 6N (In practice 6N-1, because a global phase factor is irrelevant)

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54

Fourier coefficients and basis functions

 

k k

S S

js n n n

C js

    



     

 

1

2

k

M h h S h r

n j j j n n s j j n s

p O f T C js exp i

    

 

 

The fundamental hypothesis of the Representation Analysis of magnetic structures is that the Fourier coefficients of a magnetic structure are linear combinations of the basis functions of the irreducible representation of the propagation vector group Gk , the “extended little group” Gk,-k or the full space group G.

Basis vectors Fourier coeff.

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55

Seminal papers on superspace approach Wolff, P. M. de (1974). Acta

  • Cryst. A30, 777-785.

Wolff, P. M. de (1977). Acta

  • Cryst. A33, 493-497.

Wolff, P. M. de, Janssen, T. & Janner, A. (1981). Acta

  • Cryst. A37, 625-636.

Superspace Symmetry

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56

Magnetic superspace groups

The future of Magnetic Crystallography is clearly an unified approach of symmetry invariance and representations

Journal of Physics: Condensed Matter 24, 163201 (2012)

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57

Superspace operations

4 4 ,0 , 4 , 4

( ) [ sin(2 ) cos(2 )] ( , | ) 1( ) 1( ) r r kr M M M M t

l l ns nc n b

x x nx nx time reversal

  • therwise

         

      

     l R

The application of (R, | t) operation to the modulated structure change the structure to another one with the modulation functions changed by a translation in the fourth coordinate The original structure can be recovered by a translation in the internal space and one can introduce a symmetry operator

' 4

( ) M M x  

 

 ( , | , ) t   R

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58

k k H

I

R   

R

R

HR is a reciprocal lattice vector of the basic structure and is different of zero only if k contains a commensurate component. If in the basic structure their atomic modulation functions are not independent and should verify

( | ) t r r  

 

R l

4 4 4 4

( ) det( ) ( ) ( ) ( ) M H r M u H r u kt

I I

R x x R x x        

     

    

R R

R R R

If belongs to the (3+1)-dim superspace group of an incommensurate magnetic phase, the action of R on its propagation vector k necessarily transforms this vector into a vector equivalent to either k (RI = +1) or -k (RI = -1).

( , | , ) t   R

Superspace operations

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( , 1| , ) t k t   1

The operators of the form: constitute the lattice

  • f the (3+1)-dim superspace group

Using the above basis the we can define 3+1 symmetry

  • perators of the form:

( , 1|100, ),( , 1| 010, ),( , 1| 001, ),( , 1| 000,1)

x y z

k k k        1 1 1 1

The basic lattice translations are:

1 2 3 11 12 13 21 22 23 1 2 3 31 32 33 1 2 3

( , | , ) ( , | ) ( , , ) ( , , , ) t t t kt t

S S S S R R R I

t t t R R R R R R t t t R R R H H H R                         R R R

The operators of the magnetic superspace groups are the same a those

  • f superspace groups just extended with the time inversion label 

Superspace operations

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Simplified Seitz symbols for 3+1 symmetry operators

1 2 3 1 2 3 0 1 2 3 0 1 2 3 0

( , | , ) ( , | ) ( , , , ) ( , | , ) { , | } { | } { '| } 1 1 1 1 1 ( , | 00 , ) { , | 00 } * 2 2 2 2 2 t t t kt t k c

S S S

t t t t t t t t t

  • r

t t t with                          R R R R R R R R

Simple example

1 2 3 4 1 2 3 4 1 2 3 4 1 2 3 4

1 1'( )0 {1| 0000} , , , , 1 {1| 0000} , , , , 1 {1'| 0001/ 2} , , , 1/ 2, 1 {1'| 0001/ 2} , , , 1/ 2, 1 P s x x x x x x x x x x x x x x x x               

Superspace operations

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61

4 4 ,0 , 4 , 4

( ) [ sin(2 ) cos(2 )] r r kr M M M M

l l ns nc n

x x nx nx      

      

  l

 

, , 1

( ) | | ( ) {2 } 2 M M F H k H k H k Hr

n mc ms mag

i m p f m T m exp i

    

    

Simplified magnetic structure factor in the superspace description with the notation used in JANA-2006

Magnetic Structure Factor

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   

{ 2 } { 2 }

k k k k

M S k M kr

l l

exp i exp i    

 

   

  l

, ,

1 1 ( )exp{ 2 } ( )exp{ 2 } 2 2

k k k k k k

S R I M M kr

c s

i i i i      

     

  

   

1 , , 1

( ) {2 ( ) } 1 ( ) ( ) {2 } 2

k k k

M h S H k r M h M M Hr

n n c s

p f h T exp i p f h T i exp i

 

   

 

          

 

Simplified magnetic structure factor in the description used in FullProf (with notations adapted to those used in superspace approach)

Magnetic Structure Factor

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Magnetic Structure Factor

Superspace formalism computing modules are being prepared to be used within FullProf Thank you for your attention