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Magnetic phase transitions and symmetry Laurent C. Chapon Diamond Light Source, UK European School on Magnetism 1 Outline Will discuss exclusively the magnetically ordered state Different type of magnetic structures and how to describe


  1. Magnetic phase transitions and symmetry Laurent C. Chapon Diamond Light Source, UK European School on Magnetism 1

  2. Outline ● Will discuss exclusively the magnetically ordered state ● Different type of magnetic structures and how to describe them ● Magnetic symmetry, representation analysis, and magnetic space groups. ● Landau theory of phase transitions ● Symmetry breaking and types of domains European School on Magnetism 2

  3. Description of magnetic structures Position of atom j in unit-cell l is given by: R lj =R l +r j where R l is a pure m lj lattice translation r j R l Direct lattice European School on Magnetism 3

  4. Formalism of propagation vector For simplicity, in particular for wave-vector inside the BZ, one usually describe magnetic structures with Fourier components: Since m lj is a real vector, one must imposes the condition S -kj *=S kj Here S kj is a complex vector ! European School on Magnetism 4

  5. Formalism of propagation vector -k +k Reciprocal lattice Reciprocal lattice (magnetic superlattices) European School on Magnetism 5

  6. k=0        m S exp 2 i kR S lj k j l k j   k The magnetic structure may be described within the crystallographic unit cell Magnetic symmetry: conventional crystallography plus time reversal operator: crystallographic magnetic groups European School on Magnetism 6

  7. K=1/2 r.l.v       n ( l )    m S exp 2 i kR S -1 lj k j l k j   k REAL Fourier coefficients = magnetic moments The magnetic symmetry may also be described using crystallographic magnetic space groups European School on Magnetism 7

  8. K is inside the Brillouin Zone, amplitude modulation - k interior of the Brillouin zone (pair k, -k) - Real S k , or imaginary component in the same direction as the real one 1 “Longitudinal”     S m u exp( 2 i ) k j j j k j 2     m m u cos2 ( kR ) lj j j l k j European School on Magnetism 8

  9. K is inside the Brillouin Zone, cycloids and spirals Helix Cycloid 1        S m u im v exp( 2 i )   k j uj j vj j k j 2         m m u cos2 ( kR ) m v sin2 ( kR ) lj uj j l k j vj j l k j European School on Magnetism 9

  10. Multi-k structures : Conical structures Multi-k structure with: ● Helical modulation Conical ● Ferromagnetic component European School on Magnetism 10

  11. Multi-k structures : Bunched modulations k=(d,0,0) + k=(3d,0,0) + … + k=((2n+1)d,0,0) European School on Magnetism 11

  12. Wave-vector formalism and centered cells Beware when working with non-primitive unit-cells. If in doubt always think in the primitive setup C k=(1,0,0) or (0,1,0) !!!!! European School on Magnetism 12

  13. Multi-k structures Example of a 4-k structure: the skyrmion lattice k 2 k 1 k 3 ● k 1 +k 2 +k 3 =0, same chirality for k 1, k 2 , k 3 ● Ferromagnetic component European School on Magnetism 13

  14. Multi-k structures “Skyrmion”-type lattice stabilized by energy terms of the type: ik 1 +ϕ 1 .S 2 e ik 2 +ϕ 2 .S 3 e ik 3 +ϕ 3 . M F = ... + S 1 e European School on Magnetism 14

  15. Crystal symmetries So far, we have only considered translation symmetry to describe the different types of magnetic structures. In addition we will need to take into account all the crystallographic symmetries and time-reversal symmetry. Example: Pyrochlore Fd-3m European School on Magnetism 15

  16. Space groups/notations Space group: infinite number of symmetry operations Use the Seitz notation  |t    rotational part (proper or improper)  t  translational part      t  +t  }  European School on Magnetism 16

  17. Isnversion symmetry on vectors and pseudo-vector Axial or 'pseudo' vector Parity even, time-odd - + Polar vector Parity odd, time even - + European School on Magnetism 17

  18. Mirror symmetry on vectors m + + - - m - + + - - European School on Magnetism 18

  19. Mirror symmetry on pseudo-vectors m m European School on Magnetism 19

  20. Magnetic crystallographic symmetry We need to take into account all the “usual” crystallographic symmetries + the time-reversal symmetry (as a linear “classical” operator) Axial or 'pseudo' vector Parity even, time-odd - + Polar vector Parity odd, time even - + Prime symmetry operator , i.e. the combination of a conventional ’ crystallographic symmetry + time reversal will be noted     ( primed) European School on Magnetism 20

  21. Note about time-reversal operator In QM, one needs to introduce the time reversal operator Q as defined by Wigner,sometimes noted T*. This operator comes about in QM, from the time-dependent Schrodinger equation: « Whenever the Hamiltonian of the problem is real, the complex conjugate of any eigenfunction is also an eigenfunction with the same energy ». The operator Q is the combimation of T (t -> -t) and complex conjugation (K). In the rest of the lecture, I will use time-reversal as a unitary linear operator, also called the “prime” operator. European School on Magnetism 21

  22. Why symmetry is important ? ● Neumann’s principle: If a crystal is invariant under a symmetry operation, its physical properties must also be invariant under the same symmetry operation (and generally under all the symmetry operations of the point group) ● Symmetry dictates what is allowed and what is forbidden/constrained ● Unless there is a “phase transition”, what is forbidden/restricted by symmetry is “protected”, i.e. it will remain forbidden unless the symmetry changes. [Neumann, F. E. (1885), Vorlesungen über die Theorie der Elastizität der festen Körper und des Lichtäthers, edited by O. E. Meyer. Leipzig, B. G. Teubner-Verlag] European School on Magnetism 22

  23. Why symmetry is important ? Example 1 DM interaction 2 1 European School on Magnetism 23

  24. Why symmetry is important ? Example 2 Linear ME effect Which of these two AFM structures support a linear magnetoelectric effect? European School on Magnetism 24

  25. Ordered magnetic state In some crystals, some of the atoms/ions have unpaired electrons (transition metals, J ij rare-earths). S i  0 The intra-atomic electron correlation, Hund's rule, favors a state with maximum S/J, the ions posses a localized magnetic moment    E J S S ij ij i j core Ni 2+ S i  0 Exchange interactions (direct, superexchange, J double exchange, RKKY,dipolar ….) often stabilizes a long range magnetic order. ij Time-reversal symmetry is a valid symmetry operator of the paramagnetic phase, but is broken in the ordered phase. European School on Magnetism 25

  26. Paramagnetic group Example: Monoclinic SG P2/m1’ Magnetic atom in general position x,y,z Paramagnetic group is what is called a grey group P2/m1’ European School on Magnetism 26

  27. Transitions to magnetically ordered phases with k=0 Example: Monoclinic SG P2/m1’ Magnetic atom in general position x,y,z Perez-Mato, JM; Gallego, SV; Elcoro, L; Tasci, E and Aroyo, MI J. of Phys.: Condens Matter (2016), 28:28601 European School on Magnetism 27

  28. Symmetry descent Pnma1’ Perez-Mato, JM; Gallego, SV; Elcoro, L; Tasci, E and Aroyo, MI J. of Phys.: Condens Matter (2016), 28:28601 European School on Magnetism 28

  29. Representation theory Vector space V that contains all the possible degrees of freedom of my system. Group GL n (V) Group G Group properties: Every group element is Closure represented by a nxn matrix Mapping Associative and group composition Identity rule is mapped into Inverse matrix multiplication European School on Magnetism 29

  30. Representation theory g 1 g 2 g 3 g n ... nxn matrices Similarity transformation European School on Magnetism 30

  31. Group of pure translations { 1 ∣ 000 }{ 1 ∣ 100 }{ 1 ∣ 010 }{ 1 ∣ t }{ 1 ∣ 200 } . .. .. .. .  …… e -ikt  K ………………………….....…... ● Infinite abelian group ● Infinite number of irreducible representations, and consists of the complex root of unity. ● Basis are Bloch functions. European School on Magnetism 31

  32. Space group Consider a symmetry element g={h|t} and a Bloch-function ’:  k=(k x ,0,0) F ’ is a Block-function with index (hk) European School on Magnetism 32

  33. Little group G K • By applying the rotational part of the symmetry elements of the paramagnetic group, one founds a set of k vectors, known as the “star of k” • Two vectors k 1 and k 2 are equivalent if they equal or related by a reciprocal lattice vector. • In the general case, all vectors k 1 , k 2 ,……k i in the star are not equivalent • The group generated from the point group operations that leave k invariant elements + translations is called the group of the propagation vector k or little group and noted G k .. European School on Magnetism 33

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