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Phase diagram of the hexagonal lattice quantum dimer model: order parameters, ground-state energy, and gaps PDF

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Preview Phase diagram of the hexagonal lattice quantum dimer model: order parameters, ground-state energy, and gaps

Phase diagram of the hexagonal lattice quantum dimer model: order parameters, ground-state energy, and gaps Thiago M. Schlittler,1 R´emy Mosseri,1 and Thomas Barthel2 1Laboratoire de Physique Th´eorique de la Mati`ere Condens´ee, UMR CNRS/Universit´e Pierre et Marie Curie/Sorbonne Universit´es, 4 Place Jussieu, 75252 Paris Cedex 05, France 2Laboratoire de Physique Th´eorique et Mod`eles Statistiques, Universit´e Paris-Sud, CNRS UMR 8626, 91405 Orsay Cedex, France (Dated: December 24, 2014) Thephasediagramofthequantumdimermodelonthehexagonal(honeycomb)latticeiscomputed numerically, extending on earlier work by Moessner et al. The different ground state phases are studied in detail using several local and global observables. In addition, we analyze imaginary- time correlation functions to determine ground state energies as well as gaps to the first excited states. This leads in particular to a confirmation that the intermediary so-called plaquette phase is gapped – a point which was previously advocated with general arguments and some data for an order parameter, but required a more direct proof. On the technical side, we describe an efficient world-lineQuantumMonteCarloalgorithmwithimprovedclusterupdatesthatincreaseacceptance 5 probabilitiesbytakingaccountofpotentialtermsoftheHamiltonianduringtheclusterconstruction. 1 The Monte Carlo simulations are supplemented with variational computations. 0 2 PACSnumbers: 75.10.Jm,05.50.+q,05.30.-d,05.30.Rt n a J I. INTRODUCTION the hexagonal lattice, these are ground-state configura- 9 tions of a classical Ising-spin model with antiferromag- Interacting spin systems in two dimensions have been netic interactions on the (dual) triangular lattice, planar ] rhombus tilings, and height models [10, 11]. Topological l widely studied over the last decades, both from experi- e mental and theoretical points of view. Of importance in sectors can be characterized by so-called fluxes (see be- - low). These sectors are invariant under the flips. The r this context is the so-called resonating valence bond ap- t topologicalpropertiesdependforexampleonthebound- s proachputforwardbyP.W.Andersonin1973[1]inorder . to analyze the physics of spin 1/2 Heisenberg antiferro- ary conditions and have consequences on the physics of t a magnets. Thishaslaterbeenadvocatedasawaytostudy the quantum dimer model. m the yet unsolved problem of high-temperature supercon- The quantum version, as proposed by Rokhsar and - ductivity. Following Rokhsar and Kivelson [2], it proves Kivelson, corresponds to considering the set of all dimer d interesting, when studying the low energy properties of coveringsoftheclassicalproblemasanorthonormalbasis n o these phases, to consider a simpler model, called the spanning the Hilbert space. The Hamiltonian contains c quantum dimer model (QDM). In the latter, the SU(2) kinetic terms that correspond precisely to the elemen- [ singlet bonds are replaced by hard core dimers defined tary flips described above and an additional potential on the edges of the lattice. Quantum dimer models have term, proportional to the number of flippable plaque- 1 v been employed to study for example superconductivity ttes. The competition between these kinetic and poten- 2 [2, 3], frustrated magnets [4–8], or hardcore bosons [9]. tial terms leads to a non-trivial phase diagram. For ex- 4 They can feature topological order, spin liquid phases, ample, when the potential term dominates in amplitude 2 and deconfined fractional excitations [7]. andisofnegativesign,thegroundstateisexpectedtobe 2 Before enlarging on the quantum systems, let us say a dominated by configurations which maximize the num- 0 few words about the classical case. Lattice dimer cover- ber of flippable plaquettes; for the opposite sign, one ex- . 1 ings–thebasisstatesoftheHilbertspaceinthequantum pects a ground state dominated by dimer configurations 0 case – represent already a rich mathematical problem without flippable plaquettes. As will be discussed, such 5 with many connections to statistical physics problems. configurations exist and correspond to the so-called star 1 For a graph defined by its vertices and edges (defining andstaggeredphases,respectively. In-betweenthesetwo : v faces, often called plaquettes in the present context), a extremes, the phase diagram can display intermediary Xi dimer covering is a decoration of the bonds, such that phases. The ground state is known exactly for the point every vertex is reached by exactly one dimer. The sim- where kinetic and potential terms are of equal strength. r a plest rearrangement mechanism for dimer coverings is Thephysicsaroundthisso-calledRokhsar-Kivelson(RK) provided by so-called plaquette flips. These are appli- point is expected to be different for bipartite and non- cableforplaquettesaroundwhicheverysecondbondhas bipartite lattices [7]. a dimer and the flip amounts to exchanging covered and In this paper, we provide an extensive study of the uncoveredbonds,yieldingadifferentvaliddimercovering quantumdimermodelonthebipartitehexagonal(honey- (e.g., ←→ forahexagonallattice). Dimercoverings comb) lattice along the lines already followed by Moess- arecloselyrelatedtootherconfigurationalproblems. For ner et al. [12]. In their seminal work, these authors nu- 2 A A A A C C C C B B B B A A C C B B (a) (b) (c) Figure 1: Prototypes of quantum dimer ground states on a honeycomb lattice: (a) star phase, (b) plaquette phase, (c) staggeredphase. Edgeswithahighprobabilityofcarryingadimerareindicatedinblack,andedgeswitha∼50%probability areindicatedingray. The(dual)latticecanbedecomposedintothreetriangularsublatticesA,B,andC asshown. Inthestar state, flippable plaquettes occupy two of the sublattices, while, in the plaquette phase, all plaquettes of one of the sublattices are in a benzene-like resonance state (gray hexagons). merically investigated the phase diagram by studying a II. QUANTUM DIMER MODEL local order parameter which, in addition to the generic RK transition point, shows a first order transition which A. Hilbert space and Hamiltonian separatesthestarphasefromanintermediaryphase,the so-calledplaquettephase. SeeFig.1forasketchofthese Weconsiderthe2Dhexagonallatticeofspins-1/2with twophases. Basedonthedataforthreedifferenttemper- periodic boundary conditions. As described in the intro- atures, Moessner et al. argued that the plaquette phase duction, the quantum dimer models are defined on the shouldbegapped–apointwhichconflictswithanearlier subspace spanned by dimer configurations where every √ analyticalanalysis[13]. InthepresentworkweuseQuan- spin forms a singlet (|↑,↓(cid:105)−|↓,↑(cid:105))/ 2 with one of its tum Monte Carlo simulations to extend the numerical three nearest neighbors. These different dimer configu- work by studying order parameters for different system rations are used as an orthonormal Hilbert space basis. sizes and temperatures as well as ground-state energies Modelsofthistypeareforexampleimportantinthecon- andexcitationgapswhichweobtainfromimaginary-time text of resonating valence bond states and superconduc- correlation functions. This leads to a clear confirmation tivity[2,4,6]. Notethatdifferentdimercoveringsofthe of the gapped nature of the plaquette phase. We shortly lattice(dimerproductstates)arenotorthogonalwithre- explain the reason for conflicting results of Ref. [13] and spect to the conventional inner product for spin-1/2 sys- supplement the Monte Carlo results with a variational tems ((cid:104)σ |σ(cid:48)(cid:105)=δ ). However, as explained in Ref. [2], σσ(cid:48) treatment. the two inner products can be related to one another through additional longer-ranged terms in the Hamilto- nian that turn out to be not essential. The Hamiltonian Hˆ =−t(cid:88)(| (cid:105)(cid:104) |+h.c.) QDM i i i The outline of this paper is the following. In sec- (cid:88) +V (| (cid:105)(cid:104) |+| (cid:105)(cid:104) |) (1) i i i i tion II, the quantum dimer Hamiltonian is detailed and i the nature of the different phases is explained. In sec- tion III, we describe the employed world-line Quantum containsakineticterm∝tthatflipsflippableplaquettes Monte Carlo algorithm which is based on a mapping of (those with three dimers along the six plaquette edges) the two-dimensional (2D) quantum model to a 3D clas- and a potential term ∝ V that counts the number of sical problem, and which we accelerate through suitable flippable plaquettes. The sums in Eq. (1) run over all cluster updates. Section IV introduces the employed ob- plaquettes i of the hexagonal lattice on a torus. The servables. In section V, we present the results of the nu- potential term favors (V < 0) or disfavors (V > 0) flip- mericalsimulations,andcharacterizethedifferentphases pable plaquettes. The only free parameter of this model and phase transitions on the basis of different observ- ishencetheratioV/t. Inthefollowing,aplaquettecarry- ables, ground-state energies, and energy gaps. Supple- ingj dimersiscalledaj-plaquettesuchthat3-plaquettes mentary variational computations are described in sec- are the flippable ones. tion VI. Section VII gives a summary of the results. De- The configuration space of the system is not simply tailed discussions of some technical issues are delegated connected but consists of different topological sectors to the appendices. whicharenotflip-connected. Eachsectorischaracterized 3 by two (flux) quantum numbers, also known as winding the Ising-type quantum model numbers: Call A and B the two triangular sublattices of the hexagonal lattice such that all nearest neighbors HˆQIM =Jz(cid:88)σˆizσˆjz−t(cid:88)σˆix+V (cid:88)δBˆi,0 (2) of any site from A are in B. To compute the flux W (cid:104)i,j(cid:105) i i through a cut C of the lattice, first orient all cut edges, on the triangular lattice, where {σˆx,σˆy,σˆz} denote the say,fromAtoB,weightthemby+2or−1,dependingon i i i Pauli spin matrices for lattice site i. The operator whether they are covered by a dimer or not, and multi- Bˆ := (cid:80) σˆz, with N being the set of the six near- plyeachweightby±1accordingtotheorientationofthe i j∈Ni j i est neighbors of site i, yields for an {σˆz}-eigenstate the edge with respect to C. The flux W is then computed by i value zero, if exactly three of the six bonds starting at summing the contributions of all cut edges. Such fluxes site i are frustrated. A bond is called frustrated if the W are invariant under plaquette flips. As fluxes through corresponding two spins are parallel. closed contractible curves C are zero, one has two flux Atthecenterofeachtriangleliesavertexofthehexag- quantumnumbersW andW ,correspondingtothetwo x y onal lattice. For a given dimer covering, one dimer is topologically distinct closed non-contractible curves on shared by this vertex and the dimer crosses exactly one the torus. Notice that these two fluxes characterize an of the three edges of the triangle at an angle of 90°. See averageslopeintheheightrepresentation[10]ofthesys- Fig. 2. For sufficiently strong J , the physics of the tem. z quantum Ising model (2) is restricted to the subspace Let us briefly recall the phase diagram obtained in spanned by the classical ground states. Those have ex- Ref. [12]. Three phases belonging to two different topo- actly one frustrated bond per triangle (all other configu- logical sectors have been described. The ground states rations have higher energy). The identification of dimer for the so-called star phase (−∞ < V/t < (V/t) ) and C basisstatesandIsingbasisstatesisthenstraightforward. the plaquette phase ((V/t) < V/t < 1) are found in C Given a certaindimer configuration, put aspin up onan the zero flux sector, while the staggered phase ground arbitrary site. Associating frustrated Ising bonds with states (1<V/t<∞) are in the highest flux sector. See those that are crossed by a dimer in the given state, we Fig. 1. The ground states in the zero flux sector can be canworkinward-out,assigningfurtherIsingspinstillthe distinguished using sublattice dimer densities. For that triangular lattice is filled. The state, up or down, for a purpose, we recall that the plaquettes of the hexagonal newsitedependsonthespinstateofanalreadyassigned lattice can be separated into three subsets – triangular neighboring site and on whether the corresponding bond sublatticesA,B andC ofdisjointplaquettes,asdepicted is frustrated or not. in Fig. 1, such that every hexagon of a set shares bonds This mapping of dimer configurations on the hexago- with three hexagons of the two other sets each. nal lattice to spin-1/2 configurations on the triangular lattice implies that, for the quantum Ising model, we employ the conventional inner product (cid:104)σ |σ(cid:48)(cid:105) = δ σσ(cid:48) III. QUANTUM-CLASSICAL MAPPING AND that makes different {σˆz}-eigenstates orthonormal. In MONTE CARLO SIMULATION i the Hamiltonian (2), the spin-flip terms ∝ t correspond tothekineticterminthequantumdimermodel(1). Due AsdonebyMoessner,Sondhi,andChandra[5,12,14], totheenergeticconstraintimposedbyJ →∞,theyare z the 2D quantum dimer model on a hexagonal lattice can onlyeffectiveforsiteswherethespinflipdoesnotchange be studied by mapping it first to a 2D quantum Ising the number of of frustrated bonds, corresponding to the model on the (dual) triangular lattice. The resulting flippable plaquettes in the dimer model. The term ∝ V Ising-typequantummodelcanbestudiedefficientlyusing corresponds exactly to the potential term in the dimer world-line Quantum Monte Carlo [15] by approximating model. its partition function and observables by those of a clas- sical 3D Ising-type model (CIM) on a stack of triangu- lar2Dlattices(quantum-classicalmapping)asdescribed in the following sub-sections. We accelerate the Monte Carlo simulation of the classical 3D model through suit- Flip able cluster updates. A. Equivalence to a quantum Ising model on the dual lattice As shown in Fig. 2, the dual of the hexagonal lattice Figure 2: Equivalence of dimer coverings of the hexagonal is the triangular lattice whose vertices are located at the lattice and Ising-spin configurations on the (dual) triangular hexagoncenters. Weassignaspin-1/2(σ =±1)toeach lattice. Every dimer corresponds to a frustrated bond (↑−↑ i of the vertices and, as explained in the following, the or ↓ − ↓). Flipping a plaquette in the hexagonal lattice is quantum dimer model (1) maps for the limit J →∞ to equivalent to flipping a spin in the dual lattice. z 4 The equivalence of the two models is slightly compli- As shown in appendix B, the parameters Kz and Kτ cated by two issues. First, as we are free to choose the of the classical Ising model (3) are given by orientationofthefirstassignedspin,agivendimerconfig- urationcorrespondstotwospinconfigurationsthatdiffer Kz =∆β and e−2Kτ =tanh(∆βt). (6) by a global spin-flip. Second, periodic boundary condi- tions correspond, for certain topological sectors of dimer configurations, to anti-periodic boundary conditions in C. Monte Carlo algorithm with cluster updates the Ising model. The representation (5c) of expectation values (5b) of quantum observables as expectation values of classical B. Approximation by a classical 3D Ising model observables is of great value, as it can be evaluated effi- cientlywithaMonteCarloalgorithmbysamplingclassi- To apply world-line Quantum Monte Carlo [15], we cal states σ. Specifically, one generates a Markov chain can approximate the partition function and observables of classical states σ with probabilities e−ECIM(σ)/ZCIM of the quantum Ising model (2) on the 2D triangular and averages O(σ) over these states. latticebythoseofa3DclassicalIsingmodelonastackof The most simple scheme would be to choose in every 2DtriangularlatticesbyaTrotter-Suzukidecomposition iteration of the algorithm one of the flippable spins (a [16, 17]. To this purpose, we separate the Hamiltonian spin on site j of time slice n is flippable, iff (cid:80) σn = (2) into two parts 0), compute the energy difference E (σ(cid:48))−i∈ENj i(σ) CIM CIM thattheflippingofthespinwouldcause, andflipitwith HˆQIM =Hˆz+Hˆx with Hˆx :=−t(cid:88)σˆix and a probability that is given by the so-called Metropolis i rule as detailed in appendix C. Hˆz :=Hz({σˆz}):=J (cid:88)σˆzσˆz+V (cid:88)δ . However, as one increases the accuracy by reducing i z i j Bˆi,0 ∆β (for a fixed inverse temperature β =N∆β), the cou- (cid:104)i,j(cid:105) i pling Kτ between the time slices increases with Kτ ∝ AsdetailedinappendixB,onecanusetheTrotter-Suzuki log(1/∆β) and the classical Ising model, hence, becomes decomposition stiff with respect to the time direction. In the generated states σ, there will occur larger and larger 1D clusters (cid:16) (cid:17)N e−βHˆQIM = e−∆2βHˆze−∆βHˆxe−∆2βHˆz +O(∆β3) of spins along the time-direction that have the same ori- entation, σm = σm+1 = ··· = σm+n. Flipping one of i i i of the density operator with imaginary-time step ∆β ≡ the spins inside such a cluster becomes less and less fre- β/N to determine the parameters Kz and Kτ for the quent as the associated energy change increases with the classical Ising model increasing coupling Kτ. This would result in an ineffi- cient Monte Carlo sampling with high rejection rates for (cid:88) (cid:88) E (σ)=Kz Hz(σn)−Kτ σnσn+1 (3) spin-flips. We avoid this effect by doing 1D cluster up- CIM i i dates instead of single-spin updates: In every iteration n n,i of the algorithm an initial flippable spin is selected and, suchthatthepartitionfunctionsZQIM ≡Tre−βHˆQIM and in an intermediate phase, a 1D cluster is grown in the ZCIM =(cid:80)σe−ECIM(σ) of the two models coincide (up to icmluasgteinraarsy-atimwehodleir.ecWtioenfubrethfoerredseucgregaessetinrgejetcotioflniprattheiss a known constant A), by taking account of changes in the number of flippable Z =A·Z +O(∆β3) (4a) spinsduringtheclusterconstruction. SeeappendixCfor QIM CIM details. with A=[sinh(2∆βt)/2]LN/2, (4b) Besides computing in this way expectation values of diagonal operators Oˆ = O({σˆz}), one can also evalu- aswellasexpectationvaluesofobservablesOˆ =O({σˆz}) i i ate expectation values of non-diagonal operators such as that are diagonal in the in the {σˆz}-eigenbasis, i certain correlation functions or, for example, the energy (cid:104)Oˆ(cid:105) =(cid:104)O(cid:105) +O(∆β3), where (5a) expectation value as described in appendix D. QIM CIM 1 (cid:104)Oˆ(cid:105) ≡ Tr(e−βHˆOˆ) and (5b) QIM ZQIM IV. STUDIED OBSERVABLES 1 (cid:88) (cid:104)O(cid:105) ≡ e−ECIM(σ)O(σn) ∀ . (5c) CIM Z n In the next section, section V, we numerically charac- CIM σ terize the phase diagram of the quantum dimer model In these equations, σ = (σn|n = 1,...,N) is a vector using several observables: the magnetization of the as- of classical spin configurations σn = (σn|i ∈ T) on the sociated Ising model, dimer densities, the ground-state i triangular lattice T for each of the imaginary-time slices energy, and the energy gap to the first excited state. Let n=1,...,N, and L is the number of lattice sites i in T. us briefly describe them in the following. 5 A. Magnetization of this possible problem in analyzing the data. Specifi- callyforthesublatticedimerdensities,duringthecourse We compute the root mean square (RMS) magnetiza- of the Monte Carlo simulation, we have rearranged the tion (cid:104)mˆ2(cid:105)1/2 := (cid:104)((cid:80) σˆz/L)2(cid:105)1/2 for the quantum Ising three sublattice labels according to the dimer occupan- i i QIM cies, instead of keeping the ordering constant. model (2) with L sites as an order parameter to distin- guishthestarandplaquettephasesandtofacilitatecom- parison to earlier work [12]. D. Ground state energy B. Local and global dimer observables To study the phase diagram, it is certainly of high interest to access the ground-state energy which directly decideswhatphaseprevailsforgivenvaluesoftheHamil- The simulations give access to dimer densities (cid:104)nˆ (cid:105), i tonian parameters. For sufficiently low temperatures the average number of dimers on plaquette i. Two- in the simulation, the expectation value (cid:104)Hˆ (cid:105) of the dimensional (contrast) plots of these densities nicely il- QIM quantum Ising model Hamiltonian corresponds to the lustrate the ground-state structure, even when its peri- ground-state energy. But Hˆ is not a diagonal op- odicity has to be understood in a probabilistic way. QIM erator, and hence Eq. (5) cannot be used. As detailed in We also evaluate the normalized total numbers of j- appendixD,itcanneverthelessbeevaluatedonthebasis plaquettes ((cid:104)ρˆ (cid:105),(cid:104)ρˆ (cid:105),(cid:104)ρˆ (cid:105),(cid:104)ρˆ (cid:105)). Specifically, with j- 0 1 2 3 of imaginary-time correlators (cid:104)σnσn+1(cid:105) . plaquettes being the plaquettes carrying j dimers and i i CIM (cid:80) L being the system size, ρˆ ≡ δ /L. As described j i nˆi,j inappendixA,theplaquettenumbers(cid:104)ρˆ (cid:105)obeythesum j rule E. Energy gap (cid:104)ρˆ3(cid:105)−(cid:104)ρˆ1(cid:105)−2(cid:104)ρˆ0(cid:105)=0. (7) It is important to determine whether a given phase has gapless excitations or not. As explained in ap- Notice that (cid:104)ρˆ (cid:105) does not enter in the sum rule, while 2 pendix E, we can estimate the energy gap to the first changes in the number of 3-plaquettes, which enter both excited state by fitting imaginary-time correlation func- thekineticandpotentialenergyterms,mustbecompen- tions (cid:104)Aˆ(0)Aˆ†(iτ)(cid:105). In the classical Ising model (3) they sated by plaquettes with zero dimers or one dimer. (cid:104)ρˆ (cid:105) 2 correspond to inter-layer correlators with layer distance is nevertheless constrained by the fact the total number of plaquettes is of course constant, i.e., (cid:80)3 (cid:104)ρˆ (cid:105)=1. j=0 j C. Sublattice dimer densities Star Plaquette Stagerred RK point AsdescribedaboveandindicatedinFig.1,thehexago- nalplaquettescanbeseparatedintothreesets(A,B,C), 0.35 eachformingatriangularlattice,suchthateveryhexagon 0.3 in a set shares a bond with three hexagons of the two other sublattices each. The “prototype” states of the 0.25 star and the plaquette phases (Fig. 1) can be charac- terized qualitatively in terms of dimer densities in the 1/2 0.2 three sublattices. To this purpose, we can analyze av- > 2 eraged dimer densities on each sublattice and call them m 0.15 L (cid:104)nˆA,B,C(cid:105), i.e., nˆA ≡ L3 (cid:80)i∈Anˆi etc. < 14346 Itshouldbestressedthatthesystemsunderstudymay 0.1 324 576 have degenerate (or nearly degenerate) ground states. 1296 0.05 The star crystal (ground state for V/t = −∞) and the 3600 ideal plaquette state (not a ground state, see below) are Staggered 0 both 3-fold degenerate. For sufficiently large systems, -3 -2 -1 0 1 2 it is expected that this symmetry is kinetically broken V/t in the Monte Carlo simulation. However, one cannot fully prevent the system from translating from one typ- Figure 3: The root-mean square magnetization (cid:104)mˆ2(cid:105)1/2, as ical ground-state configuration to another (even at the defined in Section IVA, for the quantum dimer model. The levelofmedium-sizepatches), smearingouttheinforma- different curves correspond to different system sizes L and tion carried by these local parameters. This possibility are obtained from Monte-Carlo simulations for V/t≤1 with β =19.2and∆β =0.02. ForallV/t>1,thestaggeredstate, was minimized here by choosing large system sizes and depictedinFig.1c,isthegroundstateandhence(cid:104)mˆ2(cid:105)1/2 =0. low temperatures. We nevertheless carefully kept track 6 0.16 L 0.14 36 4.8 144 9.6 0.12 324 19.2 V/t 576 38.4 1/2 0.1 13269060 -0-.02.73 2> 0.08 6561 -0.24 m 11664 -0.23 < 0.06 -0.226 -0.22 0.04 -0.21 -0.15 0.02 -0.1 0 0 -0.3 -0.25 -0.2 -0.15 -0.1 -0.05 0 0 0.03 0.06 0.09 0.12 0.15 0.18 -0.3-0.25-0.2-0.15-0.1-0.05 0 0.05 0.1 V/t 1/l V/t (a) (b) (c) Figure4: Locatingthetransitionbetweenthestarandplaquettephases. (a)Theroot-meansquaremagnetization(cid:104)mˆ2(cid:105)1/2 for different lattice sizes L as a function of V/t for β = 19.2 and ∆β = 0.02. (b) For the same temperature, (cid:104)mˆ2(cid:105)1/2 is plotted for different values of V/t as a function of the inverse linear system size 1/(cid:96). (c) (cid:104)mˆ2(cid:105)1/2 as a function of V/t for different temperatures, ∆β =0.02, and L=81×81. ∆n = τ/∆β. For sufficiently low temperatures, and τ third sublattice (C) are dimer-free. and β−τ big compared to the gap to the second excited (cid:79) (cid:79) state,theleadingtermsinthecorrelationfunctionareof |ψstar(cid:105)= | i(cid:105) | j(cid:105) (8) the form a+b·cosh((β/2−τ)∆E), allowing to fit the i∈A j∈B upper bound ∆E of the gap. Changing from the dimer to the Ising-spin represen- tation, A and B carry spins of equal orientation, say σ =+1, and all spins on sublattice C have the oppo- A,B V. SIMULATION RESULTS siteorientation(σ =−1)suchthattheRMSmagnetiza- C tion reaches its maximum possible value (cid:104)mˆ2(cid:105)1/2 = 1/3. In the following, let us study in detail the phase dia- It will decrease as V/t is increased – a behavior which is gram of the quantum dimer model, starting from large clearlyseeninFig.3. Noticethat,forV/t=−3,(cid:104)mˆ2(cid:105)1/2 negative V/t, i.e., in the star phase. The observables is still very close to the maximum value 1/3. described in the previous section are evaluated in simu- TounderstandhowincreasingV/taffectstheidealstar lations for patches of linear size (cid:96) with a 60◦ rhombus state, one can do perturbation theory in t/V. The cal- shape,periodicboundaryconditions,andL=(cid:96)2 plaque- culation, done up to second order in t/V, is given in ttes. In order to be able to separate the lattice into the appendix F. The result for the ground-state energy is three sublattices A, B, and C (Section IVC), (cid:96) needs to plotted in Fig. 8. It compares well with the simulation be a multiple of three. results up to V/t∼−1. The first correction to the ideal star state amounts to mixing in configurations with one flipped plaquette. The ground state for small negative t/V is the ideal A. The star phase (−∞<V/t<(V/t) ) C star state dressed with flipped plaquettes in both A and B,and,atsomepointalsoinC,whenthreeormoreflips This phase has previously been called the “columnar haveoccurredlocally. Theseschangesinthegroundsate phase”, in analogy with a corresponding phase of the canbequantifiedbythenumbersofj-plaquettesasdone square lattice quantum dimer model, where dimers are in Fig. 5. In the ideal star state (V/t → −∞), one has aligned along columns. For the hexagonal lattice, this ((cid:104)ρˆ (cid:105),(cid:104)ρˆ (cid:105),(cid:104)ρˆ (cid:105),(cid:104)ρˆ (cid:105)) = (1/3,0,0,2/3). Say, sublattices 0 1 2 3 denomination is a bit misleading, and we follow Ref. [18] A and B contain the flippable plaquettes in this limit. in calling it the “star phase” [27]. For large negative AfterflippingaplaquetteinA,thethreeneighboringpla- V, the potential term dominates the kinetic term and quettes in sublattice B carry two instead of three dimers the ground state is dominated by dimer configurations and the three neighboring plaquettes in C are no more that maximize the number of flippable plaquettes. In dimer free, but carry one dimer each. The numbers of 0- the limit V → −∞, there are three degenerate ground and 3-plaquettes are hence reduced by three and those states given by ideal star states as depicted in Fig. 1a, of 1- and 2-plaquettes are increased by 3. This explains where all plaquettes from two of the three sublattices, why the curves for (cid:104)ρˆ (cid:105) and (cid:104)ρˆ (cid:105) in Fig. 5 are almost 0 3 say A and B, are flippable, while all plaquettes of the parallel up to V/t∼−1 and why those for (cid:104)ρˆ (cid:105) and (cid:104)ρˆ (cid:105) 1 2 7 our simulations The transition can also be observed in the dimer ob- 0 1 servables. The normalized j-plaquette numbers (cid:104)ρˆ (cid:105) all 1 j 2 show a small discontinuity at (V/t)C (Fig. 5). The dis- 3 continuityof(cid:104)ρˆ (cid:105)(seeFig7b)atteststhefirstorderchar- 3 acter of the transition, since (cid:104)ρˆ (cid:105) is the derivative of the 0.8 3 energy with respect to V. But the discontinuity is quite small leading to a barely visible slope change for the en- ergy (Fig. 7a). 0.6 > At least as spectacular as the magnetization drop is i < the sudden shift in sublattices dimer densities seen in Fig. 6b. It nicely agrees with the qualitative properties 0.4 oftheidealplaquettestate,depictedinFig1b,wherethe resonating 3-plaquettes are located on one of the three sublattices. 0.2 C. The plaquette phase ((V/t) <V/t<1) C 0 -3 -2.5 -2 -1.5 -1 -0.5 0 0.5 1 1.5 The plaquette phase is certainly more complex to de- scribe than the star phase. The features of the ground V/t state in this phase are to some extent captured by the “ideal”resonatingplaquettestate,asimpleproductstate Figure 5: Normalized numbers of j-plaquettes, (cid:104)ρˆ (cid:105), for the such that all plaquettes of one of the three sublattices, j zero flux sector, system size L = 81×81, β = 19.2, and say A, are in a benzene-type resonance state such that ∆β =0.02. Around(V/t) ,afinergridofpointswasusedto C √ (cid:79) resolve the jumps in the densities at the transition. In that |ψ (cid:105) = (| (cid:105)+| (cid:105))/ 2, (9) plaq dimer i i region,datapointsarenotmarkedbysymbols. Althoughthe i∈A global ground state is not in the zero flux sector for V/t>1, data obtained for the zero flux sector is also shown for that This would in principle lead to a three-fold degeneracy region and is discussed in the text. (theresonating3-plaquettescouldjustaswellbelocated onsublatticesBorC). Incontrasttothestarphasecase, the ideal plaquette state is not an exact ground state for increase correspondingly and are on top of each other. any V/t. The actual ground states can be viewed as The contrast plots of the dimer density (cid:104)nˆ (cid:105) in Fig. 6a i the ideal plaquette state, dressed by a variable amount andtheplotofthesublatticedimerdensities(cid:104)nˆ (cid:105)in A,B,C of flip excitations in the other two plaquette sublattices. Fig.6bshowthatthedifferencesbetweendimerdensities For convenience, we use the Ising-spin notation. In this on sublattices A and B on one hand and those on sub- representation, the ideal plaquette state |ψ (cid:105) can be plaq lattice C on the other hand are reduced before reaching denoted as a critical point (V/t) . C (cid:79) (cid:79) (cid:79) |ψ (cid:105)= |→(cid:105) |↑(cid:105) |↓(cid:105) , (10) plaq i j k i∈A j∈B k∈C B. The star to plaquette phase transition at √ (V/t)C =−0.228±0.002 where |→(cid:105) denotes the σˆx-eigenstate (|↑(cid:105) +|↓(cid:105) )/ 2. i i i i The spins in sublattices B and C must be anti-parallel A first order transition occurring between the star with respect to each other. In accordance with the nu- phase and the the so-called plaquette phase is found at mericalresults,theRMSmagnetization(cid:104)mˆ2(cid:105)1/2alsovan- (V/t)C = −0.228±0.002. This critical value is consis- ishes for the ideal plaquette state |ψplaq(cid:105) in the thermo- tent, but more precise than that given in Ref. [12]. At dynamical limit. As (cid:80) σˆz|ψ (cid:105)=(cid:80) σˆz|ψ (cid:105), we (V/t)C, the RMS magnetization (cid:104)mˆ2(cid:105)1/2 suddenly drops have that i i plaq i∈A i plaq to a much smaller value which goes to zero in the ther- modynamic limit. Fig. 3 displays the RMS magnetiza- (cid:16)(cid:88) (cid:17)2 (cid:104)ψ |mˆ2|ψ (cid:105)=(cid:104)ψ | σˆz |ψ (cid:105)/L2 tion for the whole phase diagram, while Fig. 4a provides plaq plaq plaq i plaq a zoom close to the transition. We determined (V/t) i∈A C by plotting (cid:104)mˆ2(cid:105)1/2 as a function of the inverse (linear) =(cid:88)(cid:104)ψ |(σˆz)2|ψ (cid:105)/L2 = 1 →0. (11) size of system (Fig. 4b). The temperature dependence plaq i plaq 3L i∈A shown in Fig. 4c indicates that using a larger β should not substantially modify the numerical results. Consid- Theenergydensityfor|ψ (cid:105)canbecomputedeasilyand plaq ering this, we set β = 19.2 and ∆β = 0.02 for most of yields an upper bound to the exact ground state energy. 8 3 2.5 > 2 C n < >, B 1.5 n < >, A n < 1 0.5 L = 144 L = 3600, Sub. A Sub. B Sub. C 0 -1 -0.5 0 0.5 1 V/t (a) (b) Figure 6: (a) Local dimer density (cid:104)nˆ (cid:105) for different values of V/t with L=60×60 plaquettes, β =19.2, and ∆β =0.02. (b) i Sublatticedimerdensities(cid:104)nˆ (cid:105)asfunctionsofV/tforL=60×60(solidlines)andL=12×12plaquettes(dashedlines), A,B,C respectively. See section VI. At V =0, it takes for example the value lowering the temperature, observables should converge, −1/3 which is clearly above the numerically determined once the temperature is sufficiently below the gap. This value of ≈−0.38 (Fig. 7a). One can improve |ψ (cid:105) as a is confirmed in Fig. 4c. plaq variational state by adding flip excitations in sublattices Incontrast, anearlieranalyticaltreatmentinRef.[13] B and C. This is possible due the fact that 3-plaquettes suggests that the plaquette phase should be gapless. We occur in B and C with density 1/8. believe that this is due to a mistake in that derivation. In Ref. [13], the model for V = 0 and a hexagonal lat- A finite energy gap for the plaquette phase was advo- tice with mixed boundary conditions is mapped to a cated in Ref. [4] with an indirect numerical confirmation model of vertically fluctuating non-intersecting strings based on the magnetization for three different tempera- on a square lattice. First, one can obtain the ground tures. As a matter of fact, it is possible to estimate ex- state of a single string which corresponds to the ground citation gaps on the basis of imaginary-time correlation state of the XX chain (energy E(1) → −2(cid:96)t/π) and functions. The computation is described in appendix E. 0 that of the quantum dimer model in a high-flux sec- OurresultsarepresentedinFig9: Startingfromthestar tor. One can now add further strings, each reducing the phase, the gap estimate decreases in a marked behavior flux by one. To construct an N-string ground state, in around the first order phase transition at (V/t) . Then, C Ref. [13], the product of vertically shifted single-string it increases again in the plaquette phase, and eventually ground state wavefunctions is considered. To take ac- goes to zero as we approach the RK point at V/t = 1. count of the no-intersection constraint for the strings, This is clear evidence for a finite gap in the plaque- this wavefunction is anti-symmetrized with respect to tte phase with a maximal value of roughly 0.7t around the string positions, first with respect to all variables V/t≈0.1. InthevicinityoftheRKpoint,thecurvesfor gap estimates in Fig 9, computed at different β, are not y1(n), then with respect to all y2(n), etc., where (x,yx(n)) convergedwithrespecttothetemperatureanymore. The are the coordinates of string n. In analogy to the reason is simply that, as the gap vanishes, temperatures anti-symmetrization for fermions, it is being assumed in would have to be reduced more and more to obtain the Ref.[13]thattheresultingstatehasenergyNE(1) andis 0 actualgapfromtheimaginary-timecorrelators. Also,fit- hence the N-string ground state. Generalizing the pro- ting the correlation functions becomes more difficult as cedure to excited states, gapless excitations are found they ultimately change from an exponential to an alge- which simply correspond to gapless excitations of a sin- braic decay. Further evidence for the finite gap is given gle string. The described anti-symmetrization, also em- by the temperature dependence of observables. When ployed in Refs. [19, 20], appears to be flawed. Different 9 -0.38 0.46 L 36 144 -0.4 0.45 1296 11664 -0.42 0.44 > / L -0.44 > M 3 0.43 QI < <H -0.46 0.42 -0.48 -0.5 L = 36 sites 0.41 144 sites 1296 sites 11664 sites -0.52 0.4 -0.3 -0.25 -0.2 -0.15 -0.1 -0.05 0 -0.3 -0.25 -0.2 -0.15 -0.1 -0.05 0 V/t V/t (a) (b) Figure 7: Zoom near the first order phase transition at (V/t) for different lattice sizes with β = 19.2 and ∆β = 0.02: (a) C While the ground-state energy density, (cid:104)Hˆ (cid:105)/L, is continuous near (V/t) , (b), the density of flippable 3-plaquettes, (cid:104)ρˆ (cid:105), QDM C 3 displays a small but evident jump. from the conventional anti-symmetrization for fermions, and sublattice dimer densities in Fig 6b show large fluc- theresultingN-stringwavefunctionisnotasumofprod- tuations in the interval 0.7<(V/t) <1. C uct states but contains also entangled states. Hence, the The most natural explanation for this behavior are fi- resulting state is not an energy eigenstate. [28] nitesizeeffects,andthevanishingofthegapinthevicin- Let us look at further observables to better under- ity of the RK point which leads to an enhancement of stand the plaquette phase. The normalized j-plaquette fluctuations, the divergence of dimer-dimer correlation numbers (cid:104)ρˆ(cid:105) are shown in Fig 5. They appear to be i lengths, and a critical slowing down of the Monte Carlo much more sensitive to variations in V/t than the RMS simulation. More precisely, the observed effects can be magnetization. As V/t increases, (cid:104)ρˆ (cid:105) and (cid:104)ρˆ (cid:105) contin- 3 0 attributedtoacrystallineregimewithapproximateU(1) uously decreases while (cid:104)ρˆ (cid:105) increases, and (cid:104)ρˆ (cid:105) stays al- 2 1 symmetryinthevicinityoftheRKpoint. Thecontinuum most constant, assuming its maximal value in the phase version of the height representation [10] of the quantum diagram. Theconstantandmaximalvalueof(cid:104)ρˆ (cid:105)≈0.25 1 dimermodelhasU(1)symmetryandalgebraicallydecay- seems to be a characteristic signature for the plaquette ing correlations at the RK point V/t = 1. For V/t < 1, phase. For the ideal plaquette state |ψ (cid:105), one ob- plaq close to the RK point, there are two length scales, one tains ((cid:104)ρˆ (cid:105),(cid:104)ρˆ (cid:105),(cid:104)ρˆ (cid:105),(cid:104)ρˆ (cid:105)) = (1/12,1/4,1/4,5/12). For 0 1 2 3 beyond which dimer-dimer correlators show exponential no value of V/t do we find agreement with these values, decay signaling crystalline order, and one beyond which showing once again the difference between the ideal and one can observe the breaking of the U(1) symmetry. A realplaquettestates. Thediscussionabouttheapproach linearsystemsizein-betweenthesetwolengthscalescor- to the RK point is postponed to section VD. responds to the crystalline U(1) regime [21]. D. From the plaquette phase to the RK point The current belief is that, for bipartite lattices, there occurs a continuous transition from the plaquette phase E. The Rokhsar-Kivelson point (V/t=1) to the RK point, the latter being an isolated critical point. Some of our measured parameters, like the dimer densities (Fig 5), show indeed the expected smooth be- The Rokhsar-Kivelson point is the only point of the havior. Nevertheless, the magnetization curves, dis- phase diagram where the system does not display local playedinFig.3,showasmallbumpbeforetheRKpoint, order. At this point, the Hamiltonian Hˆ becomes a QDM 10 0.25 1.2 E(0)Star 19.2 0 EEVa(2Er,) PS6ltaxa6qr 1 1537386...648 81x81 -0.25 0.8 -0.5 Lt) >/(M -0.75 E/t 0.6 D Q H < -1 0.4 -1.25 0.2 -1.5 -1.75 0 -2.5 -2 -1.5 -1 -0.5 0 0.5 1 -0.4 -0.2 0 0.2 0.4 0.6 0.8 1 V/t V/t Figure 8: Numerically computed energy density (cid:104)Hˆ (cid:105)/L Figure 9: Estimates for the energy gap ∆E/t to the first QDM for β =19.2, ∆β =0.02, and L=81×81, compared to vari- excited state for different temperatures. The gaps were ob- ationalandperturbativeestimatesasdescribedinsectionVI tained from fits of imaginary-time auto-correlation functions and appendix F, respectively. (cid:104)σˆ (0)σˆ (iτ)(cid:105) , for a system with L = 36×36 sites. The i i QIM resultsshouldbeinterpretedasupperboundstotherealgap, whichareclosetheactualgapafterconvergenceinβ. Theer- rorbarsonlyindicatethequalityofthefit,notthestatistical sum of projectors Monte-Carlo error. Hˆ =−V (cid:88)(| (cid:105)(cid:104) |+h.c.) QDM,RK i i i (cid:88) sum of projectors with positive coefficients, +V (| (cid:105)(cid:104) |+| (cid:105)(cid:104) |) i i i i i (cid:88) Hˆ =t(cid:88)(| (cid:105)−| (cid:105))·((cid:104) |−(cid:104) |) =V (| (cid:105)−| (cid:105))·((cid:104) |−(cid:104) |). QDM i i i i i i i i i i (cid:88) +(V −t) (| (cid:105)(cid:104) |+| (cid:105)(cid:104) |), (12) i i i i Therefore, the ground-state energy vanishes. For each i topological sector, and for each flip-connected sub-space in a topological sector, one can build a zero-energy state the ground state energy is non-negative. The ground as an equal-amplitude superposition of all dimer cover- states are isolated states, corresponding to dimer cover- ings in the corresponding basis set. ings without any flippable plaquettes, for which the en- AttheRKpoint,manyphysicalproperties,likedimer- ergy vanishes and which are generally called staggered dimer correlations, can be derived from the behavior of configurations. These states belong to the topological the classical dimer problem. See for instance Ref. [22], sectors with highest flux, one of which being displayed wheretherelationbetweenquantumdimermodelsatthe in Fig. 1c. Notice that such states are zero-energy eigen- RKpointandtheirclassicalcounterpartsisdiscussed. In states of Hˆ for all values of V/t and become ground QDM particular, diagonal operator expectation values amount statesforV/t≥1. ThetransitionontherightoftheRK to doing classical enumerations. We used such computa- point is abrupt. At the RK point, all topological sectors tions to benchmark the QMC simulations. sectors contain (at least one) state of vanishing energy, whileonlytheisolatedgroundstatesinthemaximalflux sector persist for V/t>1. F. Staggered phase (1<V/t<∞) In the zero flux sector, the RK point corresponds to a first order transition to states with a large majority of In the parameter region 1 < V/t < ∞, flippable pla- 2-plaquettes ((cid:104)ρˆ (cid:105) > 0.8), vanishing (cid:104)ρˆ (cid:105), and finite but 2 0 quettes are disfavored. As the Hamiltonian becomes a small values of (cid:104)ρˆ (cid:105)=(cid:104)ρˆ (cid:105). See Fig. 5. 1 3

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