ebook img

High-spin polaron in lightly doped CuO$_2$ planes PDF

0.17 MB·English
Save to my drive
Quick download
Download
Most books are stored in the elastic cloud where traffic is expensive. For this reason, we have a limit on daily download.

Preview High-spin polaron in lightly doped CuO$_2$ planes

High-spin polaron in lightly doped CuO planes 2 Bayo Lau, Mona Berciu, and George A. Sawatzky Department of Physics and Astronomy, University of British Columbia, Vancouver, BC, V6T 1Z1 (Dated: January 17, 2011) We derive and investigate numerically a minimal yet detailed spin polaron model that describes lightly doped CuO2 layers. The low-energy physicsof a hole is studied by total-spin-resolved exact diagonalizationonclustersofupto32CuO2unitcells,revealingfeaturesmissedbypreviousstudies. In particular, spin-polaron states with total spin 3/2 are the lowest eigenstates in some regions of theBrillouin zone. In theseregions, and also at other points,thequasiparticle weight is identically 1 zero indicating orthogonal states to those represented in the one electron Green’s function. This 1 highlightstheimportanceofthepropertreatmentofspinfluctuationsinthemany-bodybackground. 0 2 PACSnumbers: 71.10.Fd,75.10.Jm,71.38.-k,74.72.-h n a Introduction: A full understanding of the physics of in models with one [14–17], two [18–20], three [21], or J 4 a CuO2 layer doped with a few holes has still not been more [22, 23] bands. While exact analytical solutions achieved,despitecontinuouseffort[1,2]. Recenthighres- seem to be out of reach, numerical studies are always 1 olutionangularresolvedphotoemission(ARPES)studies carried out with compromises such as the use of small ] [3–5] on the insulating charge-transfer gap parent com- clusters and variational approaches[24]. Given these dif- l e pounds [6]revealmajorpuzzles: do quasiparticlesofone ficultiesandthedrivetofindthesimplestmodel,theone- - electron nature exist and if so what is their energy and band models are unsurprisingly the most studied [14]. r t momentum? Why are the first visible electron removal While certain higher-energy aspects observed by XAS, s . states so broad, of 300 meV at 300K and decreasing lin- EELS and STM [2, 25] cannot be described using one t a early with temperature T, and what causes the very ap- band,thesignificanceofomittingotherbandsinthelow- m parent T-dependent change of line shapes? Is the mo- energy scale cannot be quantified without a comparison - mentum dependence of the lowest energy structure re- to unbiased solutions of more detailed models. d latedtothe pseudo-gapformationathigherholeconcen- n Cuprates exhibit charge-transfer band-gap behavior o trations? Recent neutron experiments performed in the with mobile holes located mainly on anion ligands and c pseudo-gap phase reported magnetic response through- unpaired electrons on cation d-orbitals [6]. One-band [ outthe Brillouinzone,notrestrictedtothe regionofthe models use superexchange [26] and Zhang-Rice singlets 3 muchdiscussedmagnetic resonance[7]. These andother (ZRS)[15]toreducethe(N−n)-electronproblemtoone v issues including the brokenlocal 4-fold symmetry, which of n holes in an AFM background, often modeled as a 7 is taken for granted in single-band models, seen in scan- N´eel background with spin-waves. To reach agreement 6 ning tunneling probe (STM)[8] and X-ray scattering [9] with experiments, such models must be tweaked at least 8 remain either open questions or are controversial. 1 by adding longer-range hopping [20, 27]. One trade-off . It is widely believed that a complete description of a fortheireleganceistheuseofmomentum-independentef- 0 1 single hole in a spin-1 2D antiferromagnet (AFM) with fectiveparameters,eventhoughitiswellknownthatthe 2 0 full quantum fluctuations could provide the answers to ZRSstatehasastrongk-dependentrenormalization[15]. 1 these questions, as well as clues for understanding the The impact of such approximations must be verified for v: originofthenon-Fermi-liquidbehaviorandthesupercon- allkwithmodelsthatdistinguishanionandcationsites. i ducting ground-state in the higher hole density region. X In this Letter we study a single hole in a model that Of course, consideration of exotic many-body scenarios includes the O 2p orbitals explicitly and full quantum r a [10], or of coupling to lattice vibrations [11] are excit- fluctuations of the AFM background. This results in ing developments; however, a detailed modeling of the spin-polaron solutions absent from other models or ap- hole+AFM is a crucial first step to understand the sig- proximations used to date. The energy dispersion of the nificanceofsuchadditions. Thisproblemisverydifficult lowest energy electron removal state is similar to that of because of the complicated nature of the 2D AFM back- the ZRS, which effectively locks the O hole in a singlet ground, whose quantum fluctuations in the presence of with one of the two adjacent copper sites. Without such doped holes were never fully captured for a large CuO 2 restrictions, our resulting wavefunction features the hole lattice. Recent technical developments [12] allow us to forming a stable S = 1 three-spin polaron (3SP) with 2 present the first such results for samples with up to 32 its two neighbour copper sites. In some regions of the Cuand64O,inthisLetter. Ourworkalsorevealsimpor- Brillouinzone,aS =1quantumfluctuationbindstothe tant failings of the single-band models used extensively S = 1 polaronyieldingalow-energyS = 3 stateinvisible 2 2 in the literature, and which we briefly review below [13]. at T = 0 to ARPES. For all momenta, the S = 3 states 2 Microscopic hole-AFM interactions have been studied are found to be within <∼J/2 of the S = 21 band. These 2 O(a(cid:0)(cid:0)(cid:0)(cid:0)(cid:0)(cid:1)(cid:1)(cid:1)(cid:1)(cid:1)(cid:0)(cid:0)(cid:0)(cid:0)(cid:0)(cid:1)(cid:1)(cid:1)(cid:1)(cid:1)(cid:0)(cid:0)(cid:0)(cid:0)(cid:0)(cid:1)(cid:1)(cid:1)(cid:1)(cid:1))(cid:0)(cid:0)(cid:0)(cid:0)(cid:0)(cid:1)(cid:1)(cid:1)(cid:1)(cid:1)(cid:0)(cid:0)(cid:0)(cid:0)(cid:0)(cid:1)(cid:1)(cid:1)(cid:1)(cid:1)(cid:0)(cid:0)(cid:0)(cid:0)(cid:0)(cid:1)(cid:1)(cid:1)(cid:1)(cid:1) (cid:0)(cid:0)(cid:0)(cid:1)(cid:1)(cid:1)(cid:0)(cid:0)(cid:0)(cid:1)(cid:1)(cid:1)(cid:0)(cid:0)(cid:0)(cid:1)(cid:1)(cid:1) δ (cid:0)(cid:0)(cid:0)(cid:0)(cid:0)(cid:1)(cid:1)(cid:1)(cid:1)(cid:1)(cid:0)(cid:0)(cid:0)(cid:0)(cid:0)(cid:0)(cid:1)(cid:1)(cid:1)(cid:1)(cid:1)(cid:1)(cid:0)(cid:0)(cid:0)(cid:0)(cid:0)(cid:1)(cid:1)(cid:1)(cid:1)(cid:1)(cid:0)(cid:0)(cid:0)(cid:0)(cid:0)(cid:1)(cid:1)(cid:1)(cid:1)(cid:1)(cid:0)(cid:0)(cid:0)(cid:0)(cid:0)(cid:0)(cid:1)(cid:1)(cid:1)(cid:1)(cid:1)(cid:1)(cid:0)(cid:0)(cid:0)(cid:0)(cid:0)(cid:1)(cid:1)(cid:1)(cid:1)(cid:1) (cid:0)(cid:0)(cid:0)(cid:1)(cid:1)(cid:1)(cid:0)(cid:0)(cid:0)(cid:1)(cid:1)(cid:1)(cid:0)(cid:0)(cid:0)(cid:1)(cid:1)(cid:1)(cid:0)(cid:0)(cid:0)(cid:1)(cid:1)(cid:1) (cid:0)(cid:0)(cid:0)(cid:0)(cid:0)(cid:0)(cid:1)(cid:1)(cid:1)(cid:1)(cid:1)(cid:1)(cid:0)(cid:0)(cid:0)(cid:0)(cid:0)(cid:1)(cid:1)(cid:1)(cid:1)(cid:1)(cid:0)(cid:0)(cid:0)(cid:0)(cid:0)(cid:1)(cid:1)(cid:1)(cid:1)(cid:1)(cid:0)(cid:0)(cid:0)(cid:0)(cid:0)(cid:0)(cid:1)(cid:1)(cid:1)(cid:1)(cid:1)(cid:1)(cid:0)(cid:0)(cid:0)(cid:0)(cid:0)(cid:1)(cid:1)(cid:1)(cid:1)(cid:1)(cid:0)(cid:0)(cid:0)(cid:0)(cid:0)(cid:1)(cid:1)(cid:1)(cid:1)(cid:1) (b) tpd Cu O tpd E(--k44)23 a) (cid:0)(cid:0)(cid:0)(cid:0)(cid:0)(cid:1)(cid:1)(cid:1)(cid:1)(cid:1)(cid:0)(cid:0)(cid:0)(cid:0)(cid:0)(cid:1)(cid:1)(cid:1)(cid:1)(cid:1)(cid:0)(cid:0)(cid:0)(cid:0)(cid:0)(cid:1)(cid:1)(cid:1)(cid:1)(cid:1)(cid:0)(cid:0)(cid:0)(cid:0)(cid:0)(cid:1)(cid:1)(cid:1)(cid:1)(cid:1)Cεu(cid:0)(cid:0)(cid:0)(cid:0)(cid:1)(cid:1)(cid:1)(cid:1)(cid:0)(cid:0)(cid:0)(cid:0)(cid:1)(cid:1)(cid:1)(cid:1)O(cid:0)(cid:0)(cid:0)(cid:0)(cid:1)(cid:1)(cid:1)(cid:1) (cid:0)(cid:0)(cid:0)(cid:0)(cid:0)(cid:0)(cid:1)(cid:1)(cid:1)(cid:1)(cid:1)(cid:1)(cid:0)(cid:0)(cid:0)(cid:0)(cid:0)(cid:1)(cid:1)(cid:1)(cid:1)(cid:1)(cid:0)(cid:0)(cid:0)(cid:0)(cid:0)(cid:0)(cid:1)(cid:1)(cid:1)(cid:1)(cid:1)(cid:1)(cid:0)(cid:0)(cid:0)(cid:0)(cid:0)(cid:1)(cid:1)(cid:1)(cid:1)(cid:1) (cid:0)(cid:0)(cid:0)(cid:0)(cid:1)(cid:1)(cid:1)(cid:1)(cid:0)(cid:0)(cid:0)(cid:0)(cid:1)(cid:1)(cid:1)(cid:1)(cid:0)(cid:0)(cid:0)(cid:0)(cid:1)(cid:1)(cid:1)(cid:1)(cid:0)(cid:0)(cid:0)(cid:0)(cid:1)(cid:1)(cid:1)(cid:1) (cid:0)(cid:0)(cid:0)(cid:0)(cid:0)(cid:0)(cid:1)(cid:1)(cid:1)(cid:1)(cid:1)(cid:1)(cid:0)(cid:0)(cid:0)(cid:0)(cid:0)(cid:1)(cid:1)(cid:1)(cid:1)(cid:1)(cid:0)(cid:0)(cid:0)(cid:0)(cid:0)(cid:0)(cid:1)(cid:1)(cid:1)(cid:1)(cid:1)(cid:1)(cid:0)(cid:0)(cid:0)(cid:0)(cid:0)(cid:1)(cid:1)(cid:1)(cid:1)(cid:1) Cu O tsw Cu O Z-(4k4) b) SSSTTT===131///222 331226AAB 0.3 S=3/2 16B T FIG. 1. (a) Two adjacent unit cells of the CuO2 plane. The 0.2 t-t’-t’’-J 32A orbitals keptin the3-band model of Eq. (1) are shown, with white/shaded for positive/negative signs. The two ǫ vectors 0.1 (solid arrow) and the four δ vectors (dashed arrow) are also 0 (0,1) (0,0) (1/2,1/2) (1,1) (0,1) (1/2,1/2) (1,0) shown. (b) Sketchof a virtualprocess of Tswap. (k,k)/π x y FIG. 2. a) Energy and b) quasiparticle weight (bottom) for andotherresultsinconsistentwithone-bandmodels,and the lowest eigenstates with S = 1 and 3 vs. momentum. their experimental implications, are discussed below. T 2 2 Different sets are shifted so as to havethesame GS energy. We start with the three-band p−d model which ex- hibits the basic physics of a hole doped charge transfer gap and insulating spin 1/2 antiferromagnet [21]: unitsofJ tofindtheirdimensionlessvaluestobet = dd pp 4.13, t =2.98, and J =2.83. H3B =Tpd+Tpp+∆pdXnl+ǫ,σ sw pd While we find thatthe 3-spinpolaron(3SP) [19]plays +UppXnl+ǫ,↑nl+ǫ,↓+UddXnl,↑nl,↓ (1) an important role, our approach is different from previ- ous work[18] by recognizing(i) T ’s role as a coherence where n = d† d , n = p† p count holes pp l,σ l,σ l,σ l+ǫ,σ l+ǫ,σ l+ǫ,σ facilitator rather than a mere correction; (ii) its comple- in Cu 3dx2−y2, respectively O 2px/y orbitals (see Fig. menting processT , illustrated in Fig. 1(b), (iii) sup- swap 1) and U > U > ∆ describe Hubbard and charge dd pp pd pression of superexchange along the bond inhabited by transfer interactions. Nearest neighbor (NN) Cu-O hop- the hole, see Eq. (5) [13], and iv) total-spin (S ) eigen- pingT =t [(p† −p† )d +h.c.]isincluded,as T pd pdP l+ǫ,σ l−ǫ,σ l,σ states arestudied explicitly. We pushthe computational is hopping T =t s p† p −t′ (p† + limit to perform S -resolved exact diagonalization (ED) pp ppP δ l+ǫ+δ,σ l+ǫ,σ ppP l−ǫ,σ T p†l+3ǫ,σ)pl+ǫ,σ betweenNNandcertainNNN Osites. For of a topologically superior [28] cluster of N = 32 CuO2 NN hopping by δ =(δ ,δ ), s =δ δ /|δ δ |. unit cells, treating the AFM background exactly. ED x y δ x y x y In a half-filled, large-U system with no hopping, the provides the transparency, flexibility, and neutrality to ground-state(GS)hasaholeateachCusite: d† |0i= supportnewresults. The priceforasystematicmapping |σ i, with the usual 2N spin degeneracy. QAn le,σlelctron of the excited states is the limited k resolution. N =16 l Q results are provided to check for size dependence. removal adds a hole in an O orbital, so the doped GS is p† |σ i, with 2N ×2N+1 degeneracy. We study We find that all low-energy eigenstates have a total thel+bǫe,hσaQviorlof such anion holes when the hopping is spin of either ST = 21 or 32. The z-projections for each turned on, in the frameworkof superexchange. The idea ST are degenerate. The ST = 21 subspace is due to the is reminiscent of studies such as Refs. [18, 19, 22]; how- s= 21 holemixingwithvariousS =0backgroundstates, ever, these also used further approximations. A detailed including the AFM GS, or mixing with the S = 1 back- comparisonofourHamiltonianversusthoseusedinthese groundstates,includingthe“single-magnon”states. The referencesisprovidedintheSupplementaryMaterial[13]. s = 21 carrier can also mix with S = 1 or 2 background Model: Noting that all Tpd processes increase energy states to yield the ST = 23 subspace; we explicitly con- byeitherU and/or∆ ,wederivetheeffectivemodelfor sider such states here for the first time. The partition of pd the states p† |σ i to be [13]: the STz subspace into separate ST sectors was managed l+ǫ,σQ l by the optimizations of Ref. [12]. Unlike there, no basis H =T +T +H +H (2) truncation was employed here for rigorous results. The eff pp swap Jpd Jdd (k,S = 3,Sz = 1) sector contains ∼0.44×109 states. where the O-O hopping of the hole is supplemented by: T 2 T 2 Results: Fig. 2(a) shows the lowest eigenenergies. The Tswap =−tswXsηp†l+ǫ+η,σpl+ǫ,σ′|σl′ǫ,ηihσlǫ,η| (3) GS has k = (π2,π2) and ST = 21, is consistent with the 3SP but can also be thought of in terms of ZRS [13]. H =J S ·S (4) Jpd pdX l l±ǫ Remarkably,wefindsimilardispersionalong(0,0)→(π,π) and(0,π)→(π,0)withouthavingtoaddlongerrangehop- H =J S ·S Π (1−n ) (5) Jdd ddX l±2ǫ l σ l±ǫ,σ ping or fine-tune parameters as is needed in one band Using t = 1.3eV, t = 0.65eV, t′ = 0.58t , ∆ = models. The biggest surprise, though, are the low-lying pd pp pp pp pd 3.6eV, and U = 4eV [14], we scale the parameters in S = 3 states which go below the 1 states near (0,0) pp T 2 2 3 (a−0.26) −−00..2390−0.05+−00..1236−0.22−−00..3239−0.31 (b−0.23) −−00..2281−0.07+−00..1174−0.07−−00..2281−0.23 Σ(−−10).2ly4hp†l−+0ǫ.1x,9σ|σ−,0l.i2x4+p†l+ǫy,σ|σ,liyi −0.28−−00.2.049−0.26−−0.02.409−0.28 −0.31−0.33−0.22−0.26−0.05−0.30−0.26 −0.23−0.21−0.07−0.14−0.07−0.21−0.23 −0.23−0.29−0.10+0.16−0.10−0.29−0.23 −0.19−0.09+0.15−0.09−0.19 −0.23 −0.10 −0.10 −0.23 0.28 0.26 0.28 FIG. 3. hC (δ,a)i for the lowest energy state at (a) (π,π) −0.24 −0.19 −0.24 −−0.24 −−0.24− x 2 2 with S = 1, and (b) at (π,π) with S = 3. The darkly- T 2 T 2 FIG.4. hC (δ,a)iforloweststateatk=(0,π)withS =1/2. shaded bullet denotes the oxygen position at l+e . Each x/y T x bulletshowsthecorrelation valuebetweenthetwosandwich- ing Cu sites. The central 12 Cu sites are shown; the corre- lations between the other 20 Cu spins converge fast towards hence constructive interference if kx = ky. In contrast, theAFM valueof ∼-0.33. hCy(δ,a)i is thePˆx↔y reflection. hopping in the upper-right/lower-left direction yields a phase shift of eikx/e−iky, and the interference is scaled down by cos(k ). In the GS, having a mixture of sin- x/y and (π,π). Finite-size analysis, discussed in the Supple- glets and triplets upper-left/lower-right to the O hole mentary Material, reveals that the ST = 23 states are lowers energy with the least disturbance to AFM order. stable polarons at least in the regions marked by thick Thus, the two outside zigzag bonds are triplet ”distur- solid lines in Fig. 2(a). Thus, a ST = 21 quasiparti- bancetails”pointingorthogonaltothemomentumdirec- cle cannot describe the low-energy states throughout the tion. ThisisverydifferentfromtheZRS,whichfreezesa BZ.Tocomparethelowestenergystatesonbothsidesof CuspinbyintraplaquettecoherencewithitsfourOsites. thhaevecroodsdsinpga,riwtye nuoptoentahaPˆtxt↔hey lroewfleescttikoxn=(Fkigy.1eaig)esnosttahteeys poFlairgo.n3bbeschoomwesstthheecloorwreelsattieonnervgaylusetsawteheant t(hπe,πS).T T=h23e canbe expressedas 2−1/2(1+Pˆ ) eiklp† |σ,li . results look similar at (0,0). hH i remains ∼ −0.9J , x↔y P l+ex,σ x Jpd pd Theband-crossingresultsinnoticeablechangeinthe ex- but there are now four more heavily disturbed bonds. pectation values of the correlation function: This further supports this being a stable polaron with an extra magnon bound locally close to the O hole. We Cˆ (δ,a)=2 S ·S n (6) stress here that this 3 polaron is formed by a spin dis- x X l+δ l+δ+a l+ex,σ 2 l,σ turbance around the 3SP. This is very different from the S = 3 excitation local to H with energy +Jpd [22]. 2 Jpd 2 which measuresthe correlationbetween two neighboring Fig.2bshowsthequasiparticleweightZ(k)forthefirst Cu spins at a distance δ from the hole. hCi ranges from electron removal state. The major difference from other -3/4forsinglet,to∼-0.33for2DAFM,to1/4fortriplet. models is that Z(k) = 0 in three regions: a) Z(0,0) = Fig. 3a shows hCˆxi when the hole is located at the Z(π,π)=0 because here the lowest eigenstate has ST = darkly shaded bullet, in the GS: k = (π2,π2), ST = 21 23 which due to spin-conservation is not in the Krylov (hCˆ i is a reflection with Pˆ for k = k ). The hole space of any S = 1 state [13], and b) Z(0,π)=0 even y x↔y x y T 2 affects the AFM order in its vicinity. Because of the though this is a S = 1 state (see below). The t-t’- T 2 hole-spin exchange H and the blocked superexchange t”-J model treatment does not conserve S , resulting in Jpd T between the two Cu spins neighboring the hole, these Z(0,0)∼0.1andafiniteZ(π,π)[16]. OurZ(k)issmaller “central” spins have triplet correlations, of ∼0.13. Also, everywhere than that of the t-t’-t”-J model, suggesting hH i ∼ -0.9J , showing that locally this is consistent less ”free particle” nature of the polaron. Jpd pd with the 3SP solution [13]. More interesting are the cor- The lowest energy state at k=(0,π) has S = 1, but T 2 relationswith the other 3 neighborsofeachofthese cen- its Z = 0 because the state is not in the Krylov space tral Cu spins: with two of them, there are robust AFM of an electron removal [13]. This seems to be due to correlations of ∼ −0.22, while with the third the cor- symmetry, althoughwe do not yet fully understand this. relation nearly vanishes (lightly shaded bullet). This is States with finite but small Z are at least 0.006J higher counterintuitive if one views the system as a fluctuat- in energy. Their close existence above the Z = 0 lowest ing Ne´elbackground,where a spin-flip wouldchange the state may be related to pseudogap phenomena in this spin-spin correlationto all four neighbors. Although the region; however, this needs to be investigated in more two central Cu spins have 2 weight in triplet configu- detail. Fig. 4 shows the correlationfor this Z =0 lowest 3 ration which is hardly bi-partite, long-range AFM order state. Compared to the GS (see Fig. 3a), there are 2 cannotbeautomaticallydiscounted[29]. Indeed,thecor- moredisturbedbondsasrequiredbythereflectionparity relations we find are consistent with such order, except about k. This larger disturbance range is accompanied for the zigzag of 3 bonds shown by shaded bullets. This by more negative (AFM) correlation values. strangeshapeisdictatedbythehoppingmechanism. For Although we are restricted to rather low momentum a Blochwave,O-Ohole hoppingin the upper-left/lower- resolution, more can be said about the E3 − E1 = 0 right direction yields a phase shift of ei0/ei(kx−ky) and band crossings in the nodal direction by lo2oking2at the 4 k points between which the difference switch signs. The in the anti-nodal region is still being investigated. observationinFig.2aisthat,goingawayfromthe(π,π) Acknowledgement: We thank G. Khaliullin for discus- 2 2 GS,E3 −E1 islargertowards(0,0)thantowards(π,π). sions, B. Keimer for providing x-ray data, I. Elfimov 2 2 The 1 → 3 bandcrossingwouldinduceanabrupt change and Westgrid for tech support, and CFI, CIfAR, CRC, 2 2 in Z(k) from non-zero to exactly zero, irrespective of the NSERC and Sloan Foundation for funding. Z(k)valueonthefiniteside. ThelargerE3−E1 towards 2 2 k =(0,0)suggeststhatthenon-zeroregionextendsmore towards k = (0,0) than towards k = (π,π). Fig. 2a also showsthatthe 3 statesgetpushedfurtherdownasN → 2 [1] D.Bonn,NaturePhysics2,159(2006; )S.Hufneretal., ∞sothecrossingisexpectedtobeclosertothe(π2,π2)GS. Rep. Prog. Phys. 71, 062501 (2008); D. M. Newns and ThisisconsistentwithARPESwhichindeedobservedan D. Tsui, Nature Physics 3, 184 (2007); G. Sangiovanni abruptpeaksuppressioninthenodaldirectionaswellas et al.,Phys.Rev.Lett.97, 046404 (2006); C. Webberet the peaks surviving longer towards k=(0,0) [5]. al., Phys.Rev.Lett. 102, 017005 (2009). Evenwhenthe S = 3 states arenotlowestinenergy, [2] M. Vojta, Advancesin Physics 58, 699 (2009). they hug the ST =T21 ba2nd. This provides a <∼Jdd/2 en- [[43]] KA..DMa.mSahsecnelleiteatl.a,l.P,hRyesv..RMeovd..LPethty.s9735,,24677300(220(0230)0.4); ergy scale for spin excitations. At finite T, as magnons K. M. Shen et al., PhysRev B 75, 075115 (2007). becomethermallyactivated,these 32 statesbecome“visi- [5] F. Ronning et al., Phys. Rev. B 67, 035113 (2003); F. ble”toARPES.ThissuggestsaT-dependentbroadening Ronning et al.,Phys. Rev.B 71, 094518 (2005). mechanismof<∼Jdd/2scale,which,coincidentally,isthe [6] J. Zaanen, et al,Phys. Rev.Lett. 55, 418 (1985). same energyscale recentlylinkedto phonons,asanother [7] G.Yuetal.,Phys.Rev.B81,064518(2010).Y.Lietal. possible source for this broadening [4, 11]. Nature 468 283 (2010) [8] M. J. Lawler, et. al. Nature466 347 (2010) Recentneutronexperimentsonsamplesathigherdop- [9] P. Abbamonte,et. al. NaturePhys. 1 155 (2005) ing reveal ∼50meV magnetic response centered at q=0, [10] C. Varma, Nature468 184 (2010). awaythe AFMresonancemomentum[7]. Thebottomof [11] V. Cataudella et al.,Phys.Rev.Lett 99, 226402 (2007). the single-particle band structure in Fig 2a) indeed has [12] B. Lau et al.,PhysRev B 81, 172401 (2010). a q=0 1/2-to-3/2excitationof this energy scale. Our re- [13] See SupplementaryMaterial for more details. sultssofararerestrictedtoasinglehole;nevertheless,it [14] M.OgataandH.Fukuyama,Rep.Prog.Phys.71,036501 has been pointed out that the q=0 magnetic excitation (2008); P.A. Lee, Rep. Prog. Phys.71, 012501 (2008). [15] F.C. Zhang et al, Phys. Rev.B 37, 3759 (1988). can be explained by involving spins on oxygensites [30], [16] P. W. Leung et al.,Phys. Rev.B 56, 6320 (1997). which certainly are present in our results. [17] A.F.Barabanov et al.,JETPLetters75(2),107(2002). In addition to the low-energy 3/2 polaron band, there [18] J.ZaanenandA.M.Oles,Phys.Rev.B37,9423(1988); are internal energy scales of the local 3SP since HJPD D.M.Frenkelet al.,ibid41,350(1990); J.L.Shenetal, also has a S = 1 doublet and a S = 3 quartet separated ibid 41, 1969 (1990); H. Q. Ding et al., ibid 46, 14317 2 2 inenergybyJ and3J /2fromthelowestenergystate. (1992); Y.Petrov and T. Egami, ibid 58, 9485 (1998). pd pd Magneticexcitationsoftheseenergyscaleshavebeenob- [19] V.J.EmeryandG.Reiter,Phys.Rev.B38,4547(1988). [20] A.Macridin et al.,Phys.Rev.B71, 134527 (2005); J.F. served via inelastic resonant X ray scattering even for AnnettandR.M.Martin Phys.Rev.B42,3929(1990); doped samples without long-range AFM order [31]. R. Eder and K. W.Becker, Z.Phys. B. 79, 333 (1990); Summary: We solved a detailed model which includes [21] V.J. Emery,Phys.Rev.Lett.58, 2794 (1987); H.Eskes the O sites and takes full account of the AFM quantum and G. A.Sawatzky, Phys.Rev.Lett. 61, 1415 (1988). fluctuations, for large N = 32 clusters. The phases of [22] L. Klein and A. Aharony Phys.Rev.B 45, 9915 (1992). the p and d orbitals lead to phase coherence via T + [23] D. F. Digor et al., Theor. and Math. Phys. 149, 1382 pp T [13]. This is re-enforced by H and the blocking (2006). L. Hozoi et al., Phys. Rev. B 75, 024517 (2007); swap Jpd C. H. Patterson, Phys. Rev. B 77, 094523 (2008); L. of the AFM superexchange, making corrections such as Hozoi et al.,Phys. Rev.B 78, 165107 (2008). T negligible. Whilethe dispersionissimilartothat Kondo [24] T. Yanagisawa et al.,Phys.Rev.B64 184509 (2001); J. measuredbyARPESwithoutanyfine-tuning, the lifting Bonca et al., Phys. Rev. B 76, 035121 (2007); F. Tan of Cu-O singlet restriction present in ZRS-based models and Q.H. Wang, Phys.Rev. Lett.100, 117004 (2008). leads to wavefunctions of different nature, i.e. the 3SP [25] M. Merz, Phys. Rev. Lett. 80 5192 (1998); R. Schuster, where the O hole correlates with both its neighbour Cu Phys. Rev.B 79, 214517 (2009). sites. This model also provides low-energy channels for [26] P. W. Anderson,Phys. Rev.115, 2 (1959). [27] J.H. Jefferson et al., Phys. Rev. B. 45, 7959 (1992); O. S =1 excitations. Z(k) was found to be identically zero P. Sushkovet al.,Phys.Rev.B. 56, 11769 (1997). in certain regionsof the BZ for two reasons: 1) the spin- [28] D.D. Betts et al., Can. J. Phys.77, 353 (1999). 32 of the lowest energy state close to (0,0) and (π,π); [29] S.Liangetal.,Phys.Rev.Lett.61,365(1988);R.Eder, and2)aroundthe antinodalregionbecauseofthelowest Phys. Rev.B. 59, 13810 (1999). energy state there being exactly orthogonalto the single [30] B. Fauque,et al, Phys. Rev.Lett. 96 197001 (2006) electron removal state. The detailed nature of the state [31] B. Keimer, unpublished.

See more

The list of books you might like

Most books are stored in the elastic cloud where traffic is expensive. For this reason, we have a limit on daily download.