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Preview Wave function statistics at the symplectic 2D Anderson transition: bulk properties

2D-sp-AM/INT Wave function statistics at the symplectic 2D Anderson transition: bulk properties A. Mildenberger1 and F. Evers2,3 1Fakult¨at fu¨r Physik, Universit¨at Karlsruhe, 76128 Karlsruhe, Germany 2Institut fu¨r Nanotechnologie, Forschungszentrum Karlsruhe, 76021 Karlsruhe, Germany 3Institut fu¨r Theorie der Kondensierten Materie, Universit¨at Karlsruhe, 76128 Karlsruhe, Germany 7 (Dated: February 6, 2008) 0 The wave function statistics at the Anderson transition in a two-dimensional disordered elec- 0 tron gas with spin-orbit coupling is studied numerically. In addition to highly accurate exponents 2 (α0=2.172±0.002,τ2=1.642±0.004), wereportthreequalitativeresults. (i)Theanomalousdimen- n sions areinvariant under q→(1−q) which is in agreement with a recent analytical prediction and a supports the universality hypothesis. (ii) The multifractal spectrum is not parabolic and therefore J differs from behavior suspected, e.g., for (integer) quantum Hall transitions in a fundamental way. 8 (iii) The critical fixed point satisfies conformal invariance. ] PACSnumbers: 72.15.Rn,05.45.Df l l a h Disordered electron systems that are confined to two scrutinize the nature of τ more closely. For one thing, - q s spatial dimensions (2D) cannot support a true metallic thewavefunctionstatisticscanbemeasured,inprinciple, e state because of Anderson localization.1 The underlying andpromisingsteps inthis directionweremade notlong m physics relates to an interference-enhanced return prob- ago.6 . t ability of quantum mechanical particles due to repeated But also important questions concerning our con- a backscattering of the same (quenched) disorder configu- ceptual understanding of the localization-delocalization m ration. There are exceptions to the rule, however. For transitionarecloselyrelatedtomultifractality. First,the - instance, if spin-orbit scattering exists, the return prob- analytic structure of τ is a specific characteristic of the d q n ability is not enhancedbut evendepleted andthe metal- criticalfieldtheoryofthe transitiondescribingscalingof o lic state survives.2 Universal properties of such metals the localdensity of states. For example,it has been pro- c are described by the symplectic symmetry class of Gaus- posedthatthe(integer)quantumHalltransitionexhibits [ sian random matrix theories. By increasing the disorder reduced anomalous dimensions δ , q 2 strength W, a metal-insulator (i.e. Anderson transition) v canbe driveninthese materials. Its universalproperties τq =d(q−1)+δqq(1−q), (2) 0 have been studied intensively in the last two decades. 6 One of the controversial questions in the late 1990s with a special property: δq does not depend on q, such 5 concerningthesymplectictransitionin2Dwasaboutthe that τq is parabolic and also invariant under q → 1−q. 8 numerical value of the critical exponent ν that describes Very recently, it has been predicted7 – based on exact 0 the divergence of the localization length when the disor- results for the nonlinear σ model and invoking the uni- 6 0 der approaches its critical value: ξ ∼ |W −Wc|−ν. In versalityhypothesis–thatthislastsymmetryisageneral / recent work, Asada et al. have made a very convincing property of all transitions belonging to the conventional at case in favor of ν=2.75 (overview in Table I) employing Wigner-Dyson classes. That is m the SU(2) model.3 A work by Markos and Schweitzer4 δ =δ (3) - comes to a similar conclusion, ν ≈2.8±0.04,within the q 1−q d Ando model and the debate is now settled. n should hold. A numerical verificationbeyond the frame- However,this latter worknotonly has helped to fixν, o workofthe powerlawrandombandedmatrix modelhas it also has reemphasizedthat another important topic is c not been reported yet. This would be an interesting test : still unresolved. Recall that the critical wave functions, v Ψ(x) atthe boundary between insulator and metal obey of universality, since it does not only rely on compar- i ing quantitative values for some few exponents – which X a multifractal statistics.5 This implies that the moments has been the usual procedure – but rather refers to the r a hh|Ψ(x)|2qii∼L−d−τq, q ∈R (1) analytic structure of an exponent spectrum. Note that Eq. (3) does not generally hold outside the conventional scale with system size L, introducing the exponent spec- symmetry classes. The spin quantum Hall effect is an trum τ . (The angular brackets denote a combined spa- example for a transition in a nonstandard universality q tialandensembleaverage.) Aprecisenumericaldetermi- class, where Eq. (3) is manifestly violated.8,9 nationofτ hasnotbeenundertakenyet. Thenumerical Second, lately it has become clear that near bound- q work presented in this letter is an attempt to close this aries multifractality differs from the bulk: flat interfaces gap. supporttheirown“surface”spectrumτs;inthepresence q There are several good reasons why one would like to of corners yet another spectrum is superimposed, etc.10 2 model method Wc Λc α0 =2+δ0 δq ν reference SU(2) TM 5.953±0.001 1.843±0.0013 2.746±0.009 3 AM TM 5.838±0.007 1.87±0.02 2.8±0.04 4 MAt 5.838±0.007 2.107±0.005 δ1=0.111 4 AM MAt 5.86±0.04 δ2 =0.19±0.005 2.41±0.24 23 AM wave-packet propagation 5.74 δ2=0.15±0.02 24 AM MAt 5.74 2.19±0.03 δ2=0.17±0.025 15 EZM MAa δ1=0.16±0.02 25 δ2=0.185±0.01 26 network model 1.83±0.03 2.51±0.18 27 TABLE I: Overview of results for the symplectic transition in two dimensions. AM: Ando model16; EZM: Evangelou-Ziman- model28; MAt (MAa): multifractal analysis based on scaling of typical (average) amplitudes; TM: transfer matrix; SU(2): SU(2) model18; δ : reduced anomalous dimension, see Eq. (2). Entriesfor thesame model are in chronological order, starting q with thelatest work. Also, in principle, an edge could break a bulk symmetry and the earlier result3 Λ =1.843 we arrive at πΛ δ = c c 0 andthuswouldnotevensharethebulkuniversalityclass. 0.996±0.012. Thus numerical evidence is provided that In fact, the unraveling of surface multifractality could the symplectic fixed point obeys CI, in agreement with leadtoaparadigmaticshiftofourpresentunderstanding general expectations. ofcriticalwavefunctionstatistics. Clearly,aprerequisite Models: We consider a tight-binding Hamiltonian on for all this is a detailed knowledge of bulk properties. a two dimensional square lattice with nearest neighbor Third, finally, a relation between δ and the ratio Λ coupling 0 c ofwidthandlocalizationlengthofquasi-1Dstripsexists: H = ǫ c† c + V c† c , (5) X i i,σ i,σ X i,σ;j,σ′ i,σ j,σ′ Λc =1/πδ0, (4) i,σ hi,ji,σ,σ′ whichisexactifthecritical2Dfixedpointisconformally where c† (c ) denotes a creation (annihilation) opera- invariant.11 It is believed thatconformalinvariance(CI) i,σ i,σ tor of an electron with spin σ on site i. is a generic property of localization-delocalization tran- In the Ando model16, the on-site energies ǫ are taken i sitions in 2D. For instance, it has been demonstrated to independently fromthe interval[−W/2,W/2] with a ho- hold at the integer quantum Hall transition.12,13 Excep- mogenous distribution. The hopping matrix Vi,σ;j,σ′ re- tions are not known so far, but Eq. (4) can be used flecting the spin-orbit coupling is chosen as as a test of CI. In this respect, recent numerical results are alarming. It is reported4 that δ0=0.107±0.005 and Vi,σ;i+k,σ′ =(V0exp(iθkσk))σ,σ′, k =x,y, (6) Λ =1.87±0.02; thus the product πΛ δ =0.629±0.036 c c 0 would signal a strong violation of Eq. (4) and therefore with σ ,σ denoting Pauli matrices and the parameters x y absence of CI.14 V = 1 and θ = π/6. We have determined the critical 0 k In this Rapid Communication,we present a numerical disorder strength independently via analysis of the crit- high-precision study of δ at the 2D-symplectic transi- ical level statistis.17 Our finding W =5.85±0.025 agrees q c tion. Our particular aim is to answer three qualitative well with earlier work.4 questions. (i) Is δ a constant, so τ is parabolic? (ii) If The second model, the SU(2) model, has been intro- q q not,doesitobeythesymmetryrelationEq. (3)confirm- duced by Asada, Slevin, and Ohtsuki18. In addition ing the universality hypothesis? (iii) Is the fixed point to the on-site energies ǫ , now also the hopping matrix i conformally invariant? Vi,σ;j,σ′ israndom. Itistakentobeuniformlydistributed Most earlier works analyzed typical moments in small over the entire group SU(2) using the group invariant ensembles, where finite-size effects make it difficult to (Haar) measure.18 obtainreliableerrorbars. Bycontrast,weemployscaling H is implemented on square L×L-size lattices with of typical and average moments in very large ensembles periodic boundary conditions. For our numerical diag- with big system sizes. Errors can thus be reduced by onalization of the resulting 2L2 ×2L2 matrices we use almost an order of magnitude. In order to cross-check, an inverse iteration routine coupled with direct sparse we analyze the two most important microscopic models. solversin orderto obtainthe eigenvaluesandwavefunc- Results thus obtained agree very well. Specifically, we tions with energies closest to zero.19 (Cf. Ref. 20.) find that δ is not a constant and the symmetry relation Multifractal analysis: Our multifractal analysis pro- q (3) is satisfied. ceeds by analyzing the scaling behavior of the average On a quantitative level, we obtain δ =0.180±0.002 moments of wave function amplitudes, Eq. (1). 2 (both models), δ =0.173±0.003 (Ando model), and In order to analyze the critical behavior we take the 0 δ =0.172±0.002 (SU(2) model). Together with Eq. (4) disorder value W =5.84 (for states at energy zero being 0 c 3 0.2 0.18 SU(2)-model Ando-model 0.176 q 1-q 0.174 0.16 ) 0.19 (L W=5.84, q=1.5, 0.0042 0.172 Ωq W=5.84, q=2.0, 0.0087 n 0.14 q=1.5, 0.0040 W=5.86, q=1.5, 0.0042 ) l q=2.0, 0.0083 W=5.86, q=2.0, 0.0087 q 0.17 δ( -0.5 0 0.5 1 1.5 0.18 0.12 3 4 5 3 4 5 ln L ln L FIG.2: TestfunctionΩ (L)highlightingvariabilityofδ with q q 0.17 q for two q values. Solid lines represent power law fits, with a slope representing δ −δ ; for values, see legend. Slight 0 1 2 3 q 1/2 q deviations between models are due to larger errors in finite- sizeextrapolationofAndomodel. Forthatmodel,resultsfor two values of W are given to illustrate that the uncertainty FIG. 1: Reduced anomalous dimension δ as defined in Eq. q in W is not a precision-limiting factor. Note that δ −δ c 3/2 1/2 (3) for the Ando model (dashed, Wc=5.84) and the SU(2) agrees well with curvature δ′′ seen in Fig. 1. model (solid, W =5.953). Additionally, anomalous dimen- 1/2 c sionsδ˜ obtainedfromtypicalinverseparticipation ratiosare q shown (⋄) for the latter model. Dashed lines indicate the require a coarse graining in order to overcomethe diver- estimated error (2σ) in δ0. Inset: blowup of the solid line gence of the moments (1) related to zeros of the wave behavior near q=0.5 now represented by ◦. Data near q=0 and q=1 suffer from noise amplification (dividing by q(1−q) functions.) A symmetric shape of the curve is clearly in Eq. (2)) and have therefore been omitted. Filled symbols displayedinthe regimeofbestaccuracy,−0.5>q >1.5. (•) show original trace after reflection at q=0.5. Dot-dashed line indicates parabolic fit (offset: 10−3) with δ1/2=0.1705 (iii) The set of exponents δq does not reduce to a con- and curvatureδ1′′/2=0.0043. stant, e.g., δq has a small but nonzero curvature δ1′′/2. Detecting δ′′ requires high-precision data, because the 1/2 numericalwindowislimited toq >2.0. Atlargervalues, critical) in the Ando model. For the SU(2) model we (a)finite-Leffectsproliferate(inAndomodelfasterthan employW =5.953inordertohaveamobilityedgeaten- c in SU(2)), so deviations between solid and dashed lines ergy ǫ=1.3 The average (1) has been performed over an increase. And(b)momentshh|Ψ|2qiiforlargeq probethe ensemble of wave functions that have been calculated in tails of the distribution function, so that typical values systemsofsizesL=16,24,32,48,64,96,128,192,256(the and averages differ from each other. Then, error bars last two values were not used in all cases). For each dis- tend to become large due to undersampling.20 The part- order realization64 wave functions closestto the critical ing of the three curves at q ? 2 visible in Fig. 1 is a energy have been taken into account; all together the consequence of these effects. number of wave functions in the ensemble is typically As a sensitive test for variability of δ we investigate 4×107 (L=16) to 3×105 (L=256). q in Fig. 2 the ratio The exponents τ are readily extracted from a power- q law fit as suggested by Eq. (1).21 In Fig. 1 we plot the 1/q(1−q) 4 reduceddimensionsδq definedin(2)asobtainedforboth Ωq(L)=hhh|Ψ|2qiiLdqi /hhh|Ψ|iiLd/2i (7) models. It incorporates our three main results. (i)We determine δ =0.172±0.002. The valuesatisfies encompassing only unprocessed data. It scales as 0 Eq. (4) and thus the consistencycheck on CI is positive. Ωq(L)∼L−δq+δ1/2 and therefore any slope in lnΩ signal- Thegoodaccuracystemsmainlyfromlargestatisticsand izes that δ deviates from δ =0.1705±0.001. Data for q 1/2 the fact, that finite-size corrections in the SU(2) model Ω at q=1.5,2.0 are shown in Fig. 2. It clearly exhibits q turnouttobeextremelysmallatq >1.5. Ascanalsobe a linear trace with the nonzero slope indicative of curva- seen from Fig. 1, the Ando model gives a similar result. ture in δ . Note that finite-size effects are very small, so q (ii)Thefunctionδ satisfiesthesymmetryrelationEq. that δ −δ can be extracted with good accuracy. q q 1/2 (3). Thus the universality postulate is confirmed. The A more conventional object than δ to characterize q inset of Fig. 1 shows that part of the full curve δ , for the wave function statistics is the Legendre transformed q which numericaldata areavailable at both points, q and f(α) = qα−τ , α =∂τ/∂q, displayed in Fig. 3. Even q q its image 1−q. (The numerical procedure that we work thoughwe haveobtainedτ onlyfor q?−1/2andthere- q with is limited to q?−1; more negative values would fore are restricted to α>α , the spectrum can be re- 1/2 4 constructed also at values α?α by making use of Eq. 2 1/2 (3).7 Then deviations from parabolicity obtrude. Summary: The multifractal spectrum of wave func- 1 tions at the 2D symplectic Andersontransitionhas been α) calculatedin the Ando andSU(2) models with high pre- ( f cision. On a qualitative level, our results demonstrate 0 thatthe criticalfixedpointis conformallyinvariantwith a nonparabolic spectrum τ . Furthermore, δ =δ , as q q 1−q predictedfromcalculationswithinthenonlinearσ model -1 parabolic approx., δ =0.1715 0 and thus supports the universality hypothesis. 1 α2 3 We thank L.Schweitzer andK. Yakubo for useful cor- respondence and A. D. Mirlin for valuable discussions FIG. 3: f(α) spectrum from data of Fig. 1, SU(2) model. and suggestions on the manuscript. While finalizing the f(α) is slightly asymmetric and not a parabolic function, manuscript, we learned about a closely related project, which would havemeant f(α)=2−(α−2−δ0)2/4δ0. with partly overlapping results.22 1 P. Anderson,Phys. Rev. 109, 1492 (1958). fields is J(L,W) = J˜ (φL1/ν) + χL−yJ˜(φL1/ν) + ... R I 2 P.LeeandT.V.Ramakrishnan,Rev.Mod.Phys.57,287 with φ(W)=|W−W |/W (χ(W)) being the relevant (ir- c c (1985). relevant) variables. Results of the scaling analysis are 3 Y. Asada, K. Slevin, and T. Ohtsuki, Phys. Rev. B 70, W =5.85±0.025,ν=2.74±0.12, andy=1.5±0.5.Thelarge c 035115 (2004). error of theexponentsresult from the uncertaintyin W . c 4 P. Markos and L. Schweitzer, J. Phys. A: Math. Gen. 39, 18 Y.Asada,K.Slevin,andT.Ohtsuki,Phys.Rev.Lett.89, 3221 (2006). 256601 (2002). 5 A. D.Mirlin, Phys. Rep. 326, 259 (2000). 19 R.B. Lehoucq, D. Sorensen, and C. Yang, ARPACK 6 M.Morgenstern,J.Klijn,C.Meyer,andR.Wiesendanger, Users Guide (SIAM, Philadelphia, 1998); A. Gupta, M. Phys. Rev.Lett. 90, 056804 (2003), Joshi, and V. Kumar, IBM report RC 22038 (98932), 7 A.D.Mirlin,Y.V.Fyodorov,A.Mildenberger,andF.Ev- (2001); P. R. Amestoy, I. S. Duff, and J.-Y. L’Excellent, ers, Phys.Rev.Lett. 97, 046803 (2006), Comput. Methods Appl. Mech. Engrg. 184, 501 (2000); 8 F. Evers, A. Mildenberger, and A. D. Mirlin, Phys. Rev. P.R.Amestoy,I.S.Duff,J.Koster,andJ.-Y.L’Excellent, B 67, 041303(R) (2003), SIAMJ. Matrix Anal.Appl., 23, 15 (2001). 9 A. D. Mirlin, F. Evers, and A. Mildenberger, J. Phys. A: 20 F. Evers, A. 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Lett. 86, 2094 Indeed,thepublisheddata([29],Fig.6)areconsistentwith (2001). aslow, logarithmic flowof σ(L)tozeroin agreement with 14 The cited value for δ0 is inconsistent with an earlier one, the self averaging nature of the multifractal exponents τq 0.19±0.03 (Table I), which would appear to give a much and in contrast to earlier claims made in the literature31. betterfit,1/πδ0=1.68±0.3 (Ref.15).However,errorbars 22 H.Obuse,A.R.Subramaniam,A.Furusaki,I.A.Gruzberg, on the earlier estimate are somewhat unclear, because it A.W.W. Ludwig, cond-mat/0609161. was obtained with a value W =5.74 that is considerably 23 K. Yakuboand M. Ono, Phys.Rev.B 58, 9767 (1998). c below more recent findings (Ref. 4), W =5.84±0.007. In 24 T.Kawarabayashi andT.Ohtsuki,Phys.Rev.B53, 6975 c fact,laterresultsbySchweitzerandZharakeshevforlarger (1996). systemsizestogetherwithaccountingforirrelevantscaling 25 S. N.Evangelou, Physica A 167, 199 (1990). terms are compatible with W from Ref. 4.(L. Schweitzer 26 J. T. Chalker, G. J. Daniell, S. N. Evangelou, and I. H. c and I.Zharakeshev (unpublished).) Nahm, J. Phys.: Condens. Matter 5, 485 (1993) (index 15 L. Schweitzer, J. Phys.C 7, L281 (1995). in Table I should be shifted: q→q+1; J. Chalker, private 16 T. Ando,Phys.Rev. B 40, 5325 (1989). communication). 17 Weemployastandardprocedure15,30andconsiderthescal- 27 R. Merkt, M. Janssen, and B. Huckestein, Phys. Rev. B ing of the second moment of the normalized level spac- 58, 4394 (1998). ing distribution J(L,W) = 21R0∞ds s2PL,W(s), where 28 S.N.EvangelouandT.Ziman,J.Phys.C20,L235(1987). P (s) denotes the probability to find an energy differ- 29 H.ObuseandK.Yakubo,Phys.Rev.B69,125301(2004); L,W ence s between two consecutive eigenvalues. Our renor- ibid. 71, 035102 (2005). malization group ansatz incorporating irrelevant scaling 30 I. K. Zharekeshev and B. Kramer, Japan J. Appl. Phys. 5 34, 4361 (1995). (1999). 31 D. Parshin and H. Schober, Phys. Rev. Lett. 83, 4590

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