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Helimagnons in a chiral ground state of the pyrochlore antiferromagnets PDF

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Helimagnons in a chiral ground state of the pyrochlore antiferromagnets Eunsong Choi,1 Gia-Wei Chern,1,2 and Natalia B. Perkins1 1Department of Physics, University of Wisconsin, Madison, Wisconsin 53706, USA 2Theoretical Division, Los Alamos National Laboratory, Los Alamos, New Mexico 87545, USA (Dated: January 28, 2013) TheGoldstonemodeinahelicalmagneticphase,alsoknownasthehelimagnon,isapropagating mode with a highly anisotropic dispersion relation. Here we study theoretically the helimagnon excitationsinacomplexchiralgroundstateofpyrochloreantiferromagnets suchasspinelCdCr O 2 4 anditinerantmagnetYMn . Weshowthattheeffectivetheoryofthesoftmodesinthehelicalstate 2 3 possesses a symmetry similar to that of smectic liquid crystals. We compute the low-energy spin- 1 wavespectrumbasedonamicroscopicspinHamiltonianandfindadispersionrelationcharacteristic 0 of the helimagnons. By performing dynamics simulations with realistic model parameters, we also 2 obtain an overall agreement between experiment and thenumerical spin-wavespectrum. Ourwork n thusalso clarifies themechanisms that relive themagnetic frustration in thesecompounds. a J Introduction. Therichphenomenologyassociatedwith the scenario predicted in Ref. [7] that the magnetic frus- 5 2 helicalspinorderinghasattractedconsiderableattention tration is relieved by the softening of a q = 0 optical recently. Magneticspiralshavebeenshowntoplayacru- phonon with odd parity. A long-range N´eel order with ] cialroleininducingthespontaneouselectricpolarization ordering wavevector q = 2π(0,0,1) is stabilized by the l e in multiferroic materials [1]. The soft magnetic fluctua- lattice distortion. Moreover, the lack of inversion sym- - r tionsinahelicalspin-density-wavestateofitinerantmag- metry endows the crystalstructure with a chirality. The t s net MnSi also holds the key to its non-Fermi liquid be- collinearstateistransformedintoamagneticspiralasthe t. havior [2]. Contrary to most well known long-rangespin chiralityistransferredtothespinsthroughspin-orbitin- a orders such as ferromagnetism and antiferromagnetism, teraction. The shifted ordering vector q = 2π(0,δ,1) is m spin-wave excitations in a helical magnetic order is de- consistent with the observed magnetic Bragg peaks. - scribed by a theory similar to the elasticity of smectic In this paper we undertake a theoretical calculation d n liquid crystals [3, 4]. In particular, despite the broken of the spin-wave spectrum in the helical ground state o symmetryofthehelicalorderisdescribedbyaO(3)order of pyrochlore antiferromagnet. In particular, our micro- c parameter,thereonlyexistsasingleGoldstonemodesim- scopiccalculationgoesbeyondthephenomenologicalap- [ ilar to the smectic-like phonon mode which emerges on proachesadoptedinmoststudiesofmagneticexcitations 2 scaleslargerthanthehelicalpitch[5,6]. Thislow-energy in helimagnets. Based on a well established microscopic v gapless excitations, dubbed helimagnons in Ref. [5], ex- model for the helical order, we exactly diagonalize the 5 hibit a highly anisotropic dispersion relation. linearized Landau-Lifshitz-Gilbert (LLG) equation with 2 2 The recentdiscoveryofanovelchiralspinstructurein a large unit cell; the size of the unit cell determines the 4 spinel CdCr O has generated much interest both theo- ordering wavevector of the magnetic spiral in the com- 2 4 5. reticallyandexperimentally[7–14]. Averysimilarcopla- mensuratelimit. Bycomparingresultsobtainedfromdif- 0 narhelicalorderhasalsobeenreportedinthe weakitin- ferent helical pitchs, we find a spin-wave spectrum that 2 erantantiferromagnetYMn [15,16]. The magneticions is characteristicof helimagnons. Our work thus provides 2 1 in these compounds form a three-dimensional network a solid example of helimagnons in frustrated pyrochlore : v of corner-sharing tetrahedra (Fig. 1), known as the py- lattice. We also performed dynamical LLG simulations i rochlore lattice. The geometrically frustrated spin inter- on large finite lattices and found an overall agreement X actions in this lattice gives rise to an extensively degen- with the experimental data on CdCr2O4. r a erate groundstate at the classicallevel [17]. As a result, Model Hamiltonian. Our starting point is a classical magnetic ordering at low temperatures is determined by spin Hamiltonian that includes nearest-neighbor (NN) the dominant residual perturbations in the system. exchangeinteractionsandspin-orbitcouplingmanifested as the Dzyaloshinskii-Moriya (DM) interaction [18, 19] The helical magnetic order in CdCr O is stabilized 2 4 between NN spins: by a combined effect of magnetoelastic coupling and rel- ativistic spin-orbit interactions. Despite a rather high = (J +K )S S +D (S S ) . (1) Curie-Weiss temperature |ΘCW|≈70 K, the spiralmag- H Xhijih ij i· j ij · i× j i netic order sets in only at T =7.8 K, indicating a high N degree of frustration. The magnetic transition at T is The isotropic NN exchange can be recast into N accompanied by a structural distortion which lowers the (J/2) M(r)2 up to a constant, where M(r) denotes r| | crystalsymmetryfromcubictotetragonal[8]. Recentin- thevePctorsumofspinsonatetrahedronatr. Minimiza- frared absorption measurements indicated a broken lat- tion of this term requires the vanishing of total mag- tice inversion symmetry below T [12], consistent with netic moment on every tetrahedron but leaves an exten- N 2 sively degenerate manifold. The lattice distortion intro- duces the exchange anisotropy K through magnetoe- ij lastic coupling. Here we consider tetragonal lattice dis- tortionsthatpreservethelatticetranslationalsymmetry. In particular,the odd-parity distortion breaks the inver- sion symmetry and stabilizes a collinear spin order with wavevector q = 2π(0,0,1) [20, 21]. The DM term is al- lowedontheidealpyrochlorelattice,wherethebondsare not centrosymmetricas requiredby the so-calledMoriya rules[19]. Moreover,thehighsymmetryofthepyrochlore latticecompletelydeterminesthe orientationsofthe DM vectors up to a multiplicative factor. The explicit form of the vectors D can be found in Ref. [22, 23]. ij To understandhow the coplanar helicalorder is stabi- lized, we briefly review the continuum theory basedon a gradientexpansionoftheorderparameters[7]. Theanti- FIG.1: (Coloronline)Coplanarhelicalorderwithspinslying ferromagneticorderonthepyrochlorelatticeischaracter- in the ac plane and rotating about the b axis. The magnetic order corresponds to the solution nˆ = (cosθ(y),0,sinθ(y)), ized by three staggeredorder parametersL (i=1,2,3). 1 i with θ(y) = Qy + const with Q = 2πδ. It produces a For example, L = (S +S S S )/4 describes the staggered spins1on tw0o opp1o−site2[0−11]3and [01¯1] bonds, Bragg peak Q = 2π(0,δ,1) in neutron scattering, consistent with the experimental measurement on CdCr O . The ex- 2 4 herethe subscriptµ=0∼3denotes the four sublattices change anisotropies are K[0,1,±1] = K[′±1,0,1] = −2Ku, and ofthepyrochlorelattice(Fig.1). Theorderparameterfor K[±1,0,1] = K[′0,1,±1] = K[1,±1,0] = K[′1,±1,0] = Ku, where K the collinear order is L1(r)=nˆ1eiq·r, and L2 =L3 =0, andK′ denoteexchangeanisotropyonNNbondsofthegreen where q=2π(0,0,1),andnˆ1 is anarbitraryunit vector. and red tetrahedra, and the subscript indicates the bond di- Assumingaslowvariationofstaggeredmagnetizations rection. in the spiral, we parameterize the order parameters as: L (r) = eiq·rφ (r)nˆ (r), where nˆ are three orthogonal i i i i nˆ (r) = cosθ(ξ)eˆ +sinθ(ξ)cˆ, where ξ r eˆ . Sub- IunnitthveeJctors, φ1lim≈it1, v−an21i(sφh22in+gφof23)t,otaanldmφa2g,nφe3ti≪zatφio1n[o7]n. st1ituting nˆ1(r) inζto Eq. (2) yields an e≡nerg·y ξdensity: →∞ E[θ]= D∂ θ+K (∂ θ)2/4.MinimizationofE givesa tetrahedra requires nˆ3 ∂ynˆ1, and the φ fields can be − ξ u ξ k helical wavenumber analytically expressed in terms of the director fields nˆ . i The effective energy functional in the gradient approxi- Q=2πδ =dθ/dξ =2D/K . (3) mation can be solely expressed in terms of the director u fields nˆ and nˆ ∂ nˆ nˆ [7]: 1 2 k y 1× 1 This rotational symmetry is accidental and is lifted by furtherneighborinteractionsandcubicsymmetryfieldof =D dr nˆ aˆ ∂ nˆ +bˆ ∂ nˆ cˆ ∂ nˆ (2) F Z h 1·(cid:0) × x 1 × y 1− × z 1(cid:1)i the lattice. A similar O(3) symmetry also occurs in the spiral order of MnSi [5]. In addition, all spirals whose +KuZ drh(∂xnˆ1)2+(∂ynˆ1)2+2(∂znˆ1)2−(nˆ2·∂znˆ1)2i. axis lies in the ab plane are also accidentally degenerate withthe spiralinwhichspins rotate aboutthe c axis[7]. Here Ku and D denote the strengths of exchange Theexperimentallyobserved(0,δ,1)spiralisselectedby anisotropy and DM interactions, respectively. The form alargethird-neighborexchangeJ whichfavorscoplanar 3 of the DM terms suggests spiral solutions with nˆ1 ro- spiralsrotatingabouttheaorbaxes. Theexpliciton-site tating about one of the principal axes and staying in magnetizations of a spiral with the pitch vector parallel the plane perpendicular to it. These special solutions to the b-axis are were first obtained in Ref. 7. For example, the solu- tion nˆ1 = (cosQy,0,sinQy) describes a helical order S¯µ(r)=aˆ sin(Q r+ϕµ)+ˆc cos(Q r+ϕµ), (4) · · with coplanar spins lying in the ac plane; see Fig. 1. This spiral magnetic order produces a Bragg scattering where µ=0,1,2,3 is the sublattice index, ϕ =ψ, ϕ = 0 1 atQ=2π(0,δ,1),consistentwiththeexperimentalchar- πδ+ψ, ϕ2 =π+ψ, and ϕ3 =π(1+δ)+ψ, with ψ is an acterization of CdCr O [8]. arbitrary constant related to the U(1) symmetry of the 2 4 The energy functional actually possesses a contin- coplanar spiral, i.e. θ(r)=Q r+ψ. F · uous symmetry related to the O(2) rotational invari- Helimagnons inthecontinuumlimit. Wenextconsider ance of the helical axis. To describe the general copla- aphenomenologicalapproachtolow-energymagneticex- nar spiral solution, we first introduce two orthogonal citations in the helical ground state. For a spiral with a unit vectors eˆ , eˆ which lie in the xy plane. A copla- fixedaxistheobvioussoftmodesaretheU(1)phasefluc- ξ ζ nar spiral rotating about the eˆ direction has the form tuations ψ associatedwith the coplanardirectorfield. A ξ 3 -3 (a) -2 (b) -2 (c) x10 x10 x10 6 3 4 δ=0.2 δ=0.2 δ=0.2 5 δ=0.1 2.5 δ=0.1 3.5 δ=0.1 δ=0.05 δ=0.05 δ=0.05 3 4 2 2.5 εk 3 εk1.5 εk 2 1.5 2 1 1 1 0.5 0.5 0 0 0 0 0.005 0.01 0.015 0 0.005 0.01 0.015 0 0.005 0.01 0.015 (k00) (0k0) (00k) (d) -1 (e) -2 (f) x10 x10 5 1 3.5 (k00) (k00) 3 4 0.8 2.5 3 0.6 α ((000k0k)) α β 2 2 0.4 1.5 1 1 0.2 0.5 0 0 0 0.04 0.08 0.12 0.16 0.04 0.08 0.12 0.16 0.04 0.08 0.12 0.16 δ δ δ FIG. 2: (Color online) Spin-wave dispersions along three principal axes [panels (a)–(c)] obtained from numerical exact diago- nalization ofalargeunitcell. Theresultsarefittedtothephenomenological dispersion ω=pαk2+βk4. Themagnonenergy is measured in unit of JS. Panels (d)–(f) show the dispersion parameters α and β as a function of the helical wavenumber δ. These data are fitted to α=const, α∝δ2, and β ∝δ−2, respectively. naive guess of the effective energy functional of the soft Lifshitz equation [4]: modewouldbe K dr ψ 2,similartothatofpla- u F ∝ |∇ | ∂S (r) δ nar magnets. However,Ra phase variation ψ = αζ corre- µ = γS (r) F , (7) spondingtoarotationofthehelicalaxisisazeromode,a ∂t − µ × δSµ(r) manifestationoftheU(1)symmetry. Yet,itcostsafinite where γ is a constant. Substituting S and into the amount of energy K α2. Consequently, there cannot µ F be any (∂ζψ)2 term∝inuthe effective energy density. The aEnqd. (∂7)myi=eldsγc(oupcle∂d2diffcer∂e2nt+iacl e∂qu4/aQtio2)nψs.∂tAψss=umγrinmg correct energy functional for the soft modes is [3–5] t − − k ξ − z z ⊥ ζ a space-time dependence exp(ik r iωt), we obtain a · − highly anisotropic dispersion relation [5] = 1 dr c (∂ ψ)2+c (∂ ψ)2+c⊥ ∂2ψ 2+rm2 ,(5) F 2Z h z z k ξ Q2(cid:0) ζ (cid:1) i ω(k)=γr1/2 c k2+c k2+c k4/Q2. (8) z z k k ⊥ ⊥ q where c , c K , c J are elastic constants, and k ⊥ u z 3 the true soft m∼ode is a∼generalized phase accompanied For wavevectors parallel to the spiral and the c axes the by arotationofthe directorfield. We havealsoincluded dispersion is linear as in an antiferromagnet, while it is a zero wavevector ferromagnetic mode m which is soft quadratic for wavevectors parallel to the a axis. duetospinconservation. Itisworthnotingthatthefirst Exact diagonalization. At the microscopic level, the term in Eq. (5) is absent in conventional helical order crystal symmetry anisotropy is expected to modify the discussed in Ref. [5]. As discussed above, it originates helimagnon dispersion (8). In addition, the particular from a rather large J3 that gives penalty to variations spiral (0,δ,1) is stabilized by a large J3 which would in- along the z direction. Schematically the coarse-grained creasethe spinstiffness alongthe c axis [7]. To takeinto sublattice magnetizations are accountthese effects,herewe performexactdiagonaliza- tions with a large unit cell to investigate the low-energy S (r) S¯ (r) + m(r)bˆ (6) acoustic-like magnons and compare the results with pre- µ µ ∼ + ψ(r) cos(Q r+ϕ )aˆ sin(Q r+ϕ )ˆc , dictions based on the helimagnon theory. µ µ (cid:2) · − · (cid:3) Tobeginwith,wefirstchooseacommensurateunitcell The spin dynamics is governedby a generalizedLandau- of a size which contains 2 Λ tetrahedra, corresponding × 4 to an ordering wavevector q = 2π(0,δ,1) with δ = 1/Λ. (1k0) 0.6 0.8 1 1.2 1.4 Here the factor of 2 accounts for the staggering of spins 6 (a) along the c axis. The DM constant is then determined 5 according to the expression D = (3/√2)K tanπδ [the u 4 discrete version of Eq. (3)] for a given fixed Ku. Next V) e we introduce small perturbations to spins in the ground m 3 ( state: Si = Sνˆi + σi, where νˆi is a unit vector par- εk 2 allel to the magnetic moment at site r in the ground i state, and σ νˆ denotes transverse deviations. Note 1 i i ⊥ that because of this constraint, there are only two de- 0 grees of freedom associated with σ at each site. As- 6 i (b) suming a time-dependence σi exp(ik ri iωt) for 5 ∼ · − the eigenmodes,the linearizedLLGequationcanbe cast i(nσto,σan,eige,nσva)luiseaprvoebclteomr oTf(dki)mσ~en=si−oniωnk=σ~,2whe2rΛeσ~ =4, meV) 34 1 2 n ( and T i·s·a·n n n matrix. We then numerica×lly dia×go- εk 2 nalize the matr×ix T(k) and obtainthe lowesteigenvalues 1 in the vicinity of k = 0, corresponding to the soft-mode around the ordering vector of the magnetic spiral. 0 0.6 0.8 1 1.2 1.4 The magnon dispersions along the three principal di- (1k0) rections in the vicinity of the ordering wavevector Q = 2π(0,δ,1) are shown in Fig. 2(a)–(c). The number of FIG. 3: (Color online) Simulated spectra of (a) N´eel state spins in the unit cell corresponding to used spiral pitch with q = 2π(0,0,1) and (b) helical order with q shifted to 2π(0,δ,1) where thehelical pitch δ =0.1 dueto a finiteD= δ is N = 40, 80, 160. To incorporate the anisotropy s 0.14 meV. Other parameters used in the simulation are J = due to the cubic symmetry of the lattice, the obtained 1.35 meV, Ku = 0.21 meV, and J3 = 0.28 meV. (b) Fitted spectra are fitted to the phenomenological dispersion: spin wave spectrum to the neutron scattering measurement ω(k) = αk2+βk4. The dispersion along the b and c (whitecircles)[8]. ThefiniteDMinteractionsplitseachband axescanpbewellapproximatedbyalinearrelation,while into three as shown in panel (b). The vertical peaks at the the spectrum along the a-axis exhibits a predominant ordering wavevectors are numerical artifacts. quadratic behavior at small δ similar to that of a fer- romagnet. The dispersion parameters α and β obtained fromthefittingareshowninFig.2(d)–(f)asafunctionof using inelastic neutron scattering in Ref. [8]. Here we the helical wavenumber δ. The large spin-wave velocity present our numerical calculations and compare the re- along the c axis can be attributed to a large J , consis- sultswiththe experimentalfindings. The measuredheli- 3 tent with the analysis of gradient expansion [7]. More calpitchδ 0.1canbeusedtofixtheratiooftheDMin- ≈ importantly, the δ-dependence of parameters for disper- teractiontotheexchangeanisotropyK . Thentheabso- u sion along the a-axis exhibits a scaling relation α δ2 lutevalueofK canbeestimatedbythemagnonenergies u ∼ and β 1/δ2, reminiscent of that of a helimagnon [5]. atthezonecenter. Asforfurther-neighborexchanges,ab ∼ Magnons in CdCr O . Although the exact diagonal- initio calculations find a negligible J and a quite large 2 4 2 ization method discussed above provides a rather accu- J with antiferromagnetic sign [7, 25]. Using the follow- 3 ratemagnonspectrum,thecomplicatedband-foldingdue ing set of parameters: J = 1.35 meV, K = 0.21 meV, u tolargeunitcellmakesitdifficulttocomparetheresults D = 0.14 meV, and J = 0.28 meV, we obtained very 3 with experiment. Instead, here we employ a less accu- good agreementwith the experimentally measuredspec- rate but more direct approach based on simulating the trum, as shown in Fig. 3(b). real-time LLG equations in a large finite lattice [24]: Concluding discussions. We have studied the spin- wave excitations in a complex helical magnetic order on ∂S ∂ α ∂S i =S H + GS i, (9) the pyrochlore lattice. Our exact diagonalization calcu- ∂t i× ∂S S i× ∂t i lation of the low-energy dispersion in the commensurate where α is the dimensionless Gilbert-damping coeffi- limit of the long-period spiral clearly demonstrates the G cient. The dynamics simulation is initiated by a short existence of helimagnonexcitations in the frustrated py- pulse localizedatr =0. Since the systemis drivenby a rochloreantiferromagnet. Thisnovelmagneticexcitation i white source with flat spectrum, we expect magnetic ex- canbeobservedinspinelCdCr O anditinerantmagnet 2 4 citationsofvariousenergyandmomentumaregenerated YMn . We have performed dynamical LLG simulations 2 in our simulations. The spin-wave spectrum is then ob- withparametersinferredfromstructuraldataandabini- tained via the Fourier transform of the simulation data. tiocalculations. The numericalmagnonspectrumagrees ThemagnonspectrumofCdCr O hasbeenmeasured wellwiththemeasureddispersioninCdCr O . Ourwork 2 4 2 4 5 thus helps clarify the underlying mechanisms that stabi- J. Wosnitza, R. Moessner, M. E. Zhitomirsky, P. Lem- lizetheobservedhelicalorderandprovidesaquantitative mens,V.Tsurkan,andA.Loidl,Phys.Rev.B83,184421 description of the model Hamiltonian. (2011). [11] R. Valdes Aguilar, A. B. Sushkov, Y. J. Choi, S.- Acknowledgements. We thank J. Deisenhofer, O. W. Cheong, and H. D. Drew, Phys. Rev. B 77, 092412 Sushkov, O. Tchernyshyov for stimulating discussions. (2008). N.P. and E.C. acknowledge the support from NSF grant [12] Ch.Kant,J.Deisenhofer,T.Rudolf,F.Mayr,F.Schret- DMR-1005932. G.W.C. is supportedby ICAM and NSF tle, A.Loidl, V.Gnezdilov,D. Wulferding,P. Lemmens, Grant DMR-0844115. N.P. and G.W.C. also thank the and V.Tsurkan, Phys. 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