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Pairing in Cu-O models: Joint electron-phonon and electron-electron interactions

Enrico Perfetto and Michele Cini

Istituto Nazionale per la Fisica della Materia, Dipartimento di Fisica, Universita’ di Roma Tor Vergata, Via della Ricerca Scientifica, 1-00133 Roma, Italy

共Received 20 November 2003; revised manuscript received 12 January 2004; published 18 March 2004兲 We discuss a many-electron Hamiltonian with Hubbard-like repulsive interaction and linear coupling to the phonon branches, having the Cu-O plane of the superconducting cuprates as a paradigm. A canonical trans-formation extracts an effective two-body problem from the many-body theory. As a prototype system we study the CuO4cluster, which yields electronic pairing in the Hubbard model; moreover, a standard treatment of the Jahn-Teller effect predicts distortions that destroy electronic pairing. Remarkably, calculations that keep all the electronic spectrum into account show that vibrations are likely to be synergic with electronic pairing, if the coupling to half-breathing modes predominates, as experiments suggest.

DOI: 10.1103/PhysRevB.69.092508 PACS number共s兲: 74.20.Mn, 71.27.⫹a, 73.22.⫺f

The role of electron-phonon 共EP兲 interactions in deter-mining the superconducting correlations in the Cu-O planes of cuprates is a very controversial issue. Possibly, the pairing mechanism has a predominantly electronic origin,1but many high-TCcompounds exhibit a quite noticeable doping depen-dent isotope effect,2suggesting that EP interactions could be important and should be included in the theory. In particular there is experimental evidence3that the half-breathing Cu-O bond stretching mode at k⫽(␲,0),(0,␲) is significantly coupled with the doped holes in the superconducting regime and its contribution may be relevant for the dx2⫺y2

pairing.4 – 6

The simplest way to include both strong electronic corre-lations and EP interactions is the Hubbard-Holstein model, where electrons are coupled to a local Einstein phonon. Much is known7,8about the possibility of a superconducting phase in this model; further evidence for pairing can be ex-tracted by exact numerical diagonalization of small cluster Hamiltonians, calculating the effective pairing interaction defined as ⌬˜(N⫹2)⫽E(N⫹2)⫹E(N)⫺2E(N⫹1), where N is the number of fermions in the system. A negative⌬˜ is interpreted as an effective attraction and suggests the pres-ence of a bound pair in the ground state. Petrov and Egami9 found⌬˜⬍0 in a doped eight-site Hubbard-Holstein ring and showed that the effect disappears once phonons are turned off. Conversely Mazumdar and co-workers10 suggested that pairing in Hubbard clusters reported by some authors11was of doubtful physical interpretation due to the neglect of the lattice degrees of freedom and the Jahn-Teller 共JT兲 effect. Consider even N, such that the (N⫹2)-particle cluster hosts a singlet pair and the (N⫹1)-particle ground state is degen-erate. They argued that JT distortion might cause a larger energy gain of the system with N⫹1 particles, thus reversing the sign of⌬˜. This led to the conjecture that any ⌬˜⬍0 due to an electronic mechanism is just a finite-size effect, which vanishes for large systems as the JT effect does.

Here we further investigate this issue by addressing the question if the recently proposed W⫽0 pairing available in the Hubbard model12–14survives when the lattice degrees of freedom are switched on. In previous works it was shown that a class of C4v-symmetric clusters exhibit the⌬˜⬍0

prop-erty, due to the binding of the so-called W⫽0 pairs. This depends crucially on the symmetry and on the availability of degenerate states. Fermions in strongly correlated systems can avoid the on-site repulsion and possibly form singlet bound states if there is enough symmetry; the fillings and the symmetry channels where the W⫽0 pairing can occur are determined in full generality by the W⫽0 theorem;15 these symmetries achieve the same result as high angular momen-tum and parallel spins in the Kohn-Luttinger16 continuum approach.

When lattice effects are introduced in this scenario, sev-eral questions arise. In the conventional mechanism, phonons overscreen the electron repulsion; what happens if electronic screening already leads to pairing? It is not obvious that the phonons will reinforce the attraction while preserving the symmetry. More generally, some vibrations could be pairing and others pair breaking. To address these problems we use an extension of the Hubbard model in which bond stretch-ings dictate the couplstretch-ings to the normal modes of the C4v-symmetric configuration, generating a long-range 共Fro¨h-lich兲 EP interaction. This is physically more detailed than the Hubbard-Holstein model, and does not restrict to on-site EP couplings that would be impaired by a strong Hubbard repul-sion. A further important drawback of the Holstein EP inter-action in this context is an unphysically large polaron 共and bipolaron兲 mass and low polaron mobility. This problem is avoided using Fro¨hlich-like phonons for modeling the Cu-O planes. It was pointed out recently17–19 that even in the strong EP coupling regime a long-range EP interaction re-moves the problem of polaron self-trapping.

We start from the Hubbard model with on-site interaction U and expand the hopping integrals ti, j(ri,rj) in powers of the displacements ␳i around a C4v-symmetric equilibrium configuration: ti, j共ri,rj兲⯝ti, j 0 共r i,rj兲⫹

ti j共ri,rj兲 ⳵ri

0 ␳i␣ ⫹

ti j共ri,rj兲 ⳵rj

0 ␳j␣, 共1兲 PHYSICAL REVIEW B 69, 092508 共2004兲

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where␣⫽x,y. Below, we write down thei␣ in terms of the normal modes q: ␳i␣⫽兺S(i) q, where ␩ is the label of an irreducible representation共irrep兲 of the symmetry group of the undistorted system and␯ is a phonon branch.

Thus, treating the Cu atoms as fixed, for simplicity, one can justify an electron-lattice Hamiltonian:

Hel-latt⫽H0⫹Vtot. 共2兲 Here H0⫽H0n⫹H0e is given by H0⫽

␩ ប␻␩,␯b␩,␯ † b,␯⫹

i, jti, j0 共ri,rj兲共ci␴ † cj␴⫹H.c兲, 共3兲

where ␻,␯ are normal-mode frequencies. Moreover, let M

denote the O mass, ␰,␯⫽␭␩␯

ប/2M␻␩,␯, with ␭␩␯

num-bers of order unity that modulate the EP coupling strength. Then, Vtot⫽V⫹W reads

Vtot⫽

␩,␯ ␰␩,␯共b␩,␯ † ⫹b ␩,␯兲H␩,␯⫹U

i ni↑ni↓, 共4兲 where the H,␯ operators are given by

H,␯⫽

i, j

␣,␴

S共i兲

ti j共ri,rj兲 ⳵ri

0 ⫹S共 j兲

ti j共ri,rj兲 ⳵rj

0

共ci,␴ † cj,␴⫹H.c.兲. 共5兲

Consider the Hubbard model HH⫽H0e⫹W involving the purely electronic terms of Hel-latt. We recall that W⫽0 pairs are defined as two-body singlet eigenstates of the HHfree of double occupancy; in the many-body problem they interact indirectly and can get bound.12,20Here we wish to derive an effective interaction between the particles in the pair suitable for Hel-latt, by generalizing the canonical transformation ap-proach of Ref. 20.

Denote the phonon vacuum by 兩0

典典

and the N-particle noninteracting Fermi sphere by 兩⌽0(N)

; if we add a W

⫽0 pair to 兩⌽0(N)

丢兩0

典典

, the two extra particles, by

defi-nition, cannot interact directly 共in first order兲. Hence their effective interaction comes out from virtual electron-hole (e-h) excitation and/or phonon exchange and, in principle, can be attractive. To expand the interacting (N⫹2)-fermions ground state兩⌿0(N⫹2)

, we build a complete setS of

con-figurations in the subspace with vanishing z spin component, considering the vacuum state兩⌽0(N)

丢兩0

典典

and the set of excitations over it.

We start by creating W⫽0 pairs of fermions over

兩⌽0(N)

丢兩0

典典

; we denote with 兩m

丢兩0

典典

these states. At weak coupling, we may truncate the Hilbert space to the simplest excitations, i.e., to states involving one e-h pair or one phonon created over the兩m

丢兩0

典典

states. We define the

兩m

兩q

典典

states, obtained by creating a phonon denoted by q⫽(␩,␯) over the兩m

丢兩0

典典

states. Finally we introduce the

兩␣

丢兩0

典典

states, obtained from the兩m

丢兩0

典典

states by

cre-ating one e-h pair. We now expand the interacting ground state in the truncated Hilbert space:

兩⌿0共N⫹2兲

m am兩m

丢兩0

典典

m,q am,q兩m

兩q

典典

a␣兩␣

丢兩0

典典

共6兲

and set up the Schro¨dinger equation with energy eigenvalue E. A canonical transformation21decouples the higher ampli-tudes am,q and a, and the am become expansion coeffi-cients over the W⫽0 pairs of the wave function of the dressed pair 兩␸

. This obeys the Cooper-like equation Hpair兩␸

⫽E兩

with an effective two-body Hamiltonian Hpair:

Hpair⬅共H0⫹W⫹S关E兴兲, 共7兲

where S is the E-dependent effective scattering operator; the pairing problem must be solved self-consistently. It turns out that the effective scattering operator is

S关E兴m,m⬘⫽

Wm,W␣,mE

⫺Em

,q Vm,mq Vmq,m Em

⫹␻q

⫺E. 共8兲 Here the primed quantities in the denominators are the eigenenergies of the 兩m

丢兩0

典典

, 兩m

兩q

典典

, and 兩␣

丢兩0

典典

states; they get renormalized in the decoupling procedure. The pairing criterion involves the properly renormalized Fermi energy ␧FR 共see Ref. 13兲; if the lowest energy eigen-value E is such that E⫽2␧FR⫹⌬ with negative ⌬, the dressed W⫽0 pair gets bound in the many-body interacting problem and the system undergoes a Cooper instability.

As an illustrative application of the above pairing scheme, in this preliminary work we focus on CuO4, the smallest

cluster yielding W⫽0 pairing in the Hubbard model. This requires four holes共total number, not referred to half filling兲; such a doping is somewhat unrealistic, but larger C4v-symmetric clusters and the full CuO2 plane also show W⫽0 pairing in the doping regime relevant for cuprates.12,20 Remarkably, in the pure Hubbard model, one can verify that

⌬⫽⌬˜(4) at least at weak coupling,12

which demonstrates that ⌬˜ has the physical meaning of an effective interaction. CuO4 represents a good test of the interplay between

elec-tronic and phononic pairing mechanisms since we can com-pare exact diagonalization results with the analytic approxi-mations of the canonical transformation. CuO4 allows only

the coupling to phonons at the center or at the edge of the Brillouin Zone; however, phonons near the edge are pre-cisely those which are most involved.3,4

Even in this small system the virtually exact diagonaliza-tions are already hard and the next C4v-symmetric example, the Cu5O4cluster,

22

is much more demanding for the number of vibrations and the size of the electronic Hilbert space. The pure Hubbard CuO4 cluster with O-O hopping tox⫽0 yields12 ⌬˜(4)⬍0, due to a couple of degenerate W⫽0 bound pairs, in the A1and B2irreps of the C4vgroup; there-fore in Eq. 共8兲 we set the m⫽m

labels accordingly.

BRIEF REPORTS PHYSICAL REVIEW B 69, 092508 共2004兲

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Starting with the C4v-symmetric arrangement, any displace-ment of the oxygens in the plane can be analyzed in irreps, A1, A2, B1, B2, E1, E2, see Fig. 1. The EP coupling is

expressed through two parameters ⳵t andtox, defined as the derivatives of t and toxwith respect to the Cu-O and O-O bond lengths. The CuO4cluster is also interesting as a test of

the conjecture of Ref. 10; we checked21 that a standard JT calculation in which the degenerate ground-state wave func-tions interact with the vibrafunc-tions indeed predicts distorfunc-tions that already at moderate EP coupling destroy W⫽0 pairing; here we wish to go beyond this approximation.

According to Eq.共8兲, the phonon-mediated interaction, in the A1 channel is

m,q VA 1,mq Vm,A 1 q Em⫹␻q

⫺E ⫽⫺43tox2

B2 2 2␧A 1⫹␻B2⫺E ⫹ 2␭A 1 2 2␧A 1⫹␻A1⫺E ⫺ ␭E1 2 2␧A1⫹␻E1⫺E ⫺E2 2 2␧A1⫹␻E2⫺E

. 共9兲

In the B2 channels we find

m,q VB 2,mq Vm,B 2 q Em

⫹␻q

⫺E ⫽⫺4⳵tox2 ␭B2 2 2␧A1⫹␻B2⫺E . 共10兲 Thus, the two W⫽0 pairs behave differently: the B2 bind-ing energy is enhanced by phonons, while in the A1 sector

the overall sign depends on ␭ and␻. It turns out that A1

and B2 modes are synergic to the W⫽0 pairing, while both longitudinal and transverse E modes are pair breaking. The half-breathing modes that are deemed most important4,5are A1⫾B1 combinations, but B1 is scarcely relevant. For the sake of argument, in the explicit calculations we took all the normal modes with the same energy␧0⫽ប␻0⫽10⫺1 eV and ␭⫽1. This sets the length scale of lattice effects, ␰0 ⫽

ប/2M␻0⯝10⫺1 Å where we used M⫽2.7⫻10⫺26Kg

for oxygen.

With this choice, pairing is enhanced in the A1 sector as

well, albeit less than in B2, see Fig. 2, where the pairing

energy without phonons is ⌬⯝⫺20 meV for both the W

⫽0 pairs. In other terms, the vibrations split the degeneracy

of the electronic ground state, effectively lowering the sym-metry like a nonvanishing tox. Here again we stress that ⌬

⫽⌬˜(4) for both symmetries, generalizing the Hubbard

model result. To go beyond the weak-coupling case, we di-agonalized Hel-latt numerically in the truncated Hilbert space

FIG. 2. Analytical results of the canonical transformation: pair binding energy in the A1and B2sectors as a function of⳵tox. Here

we used␭⫽1 for every mode, t⫽1 eV, tox⫽0, U⫽1 eV;⳵toxis

in units of␧0/␰0⫽1 eV Å⫺1, ⌬ is in eV.

FIG. 3. ⌬˜(4) as a function of ⳵tox for different values of⳵t.

␭␩⫽1 for all the vibrations, except ␭␩⫽0 for␩⫽E1共a兲; ␭␩⫽0 for

⫽E2 共b兲. nv⫽3 for each active mode;⳵t⫽⫺0.2 共diamonds兲; ⳵t

⫽⫺0.5 共triangles兲;⳵t⫽⫺1 共crosses兲. Here we used t⫽1 eV, tox

⫽0, U⫽1 eV, ⳵toxand⳵t are in units of ␧0/␰0⫽1 eV Å⫺1,⌬˜ is

in eV. FIG. 1. Pictorial representation of the ionic displacements in the

eight normal modes of the CuO4cluster, labeled according to the

irreps of the C4vGroup.

BRIEF REPORTS PHYSICAL REVIEW B 69, 092508 共2004兲

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with up to five modes at a time having vibrational quantum numbers nv⭐3. In Fig. 3共a兲 we included all vibrations ex-cept E1; with increasing the EP coupling, the pair binding

energy steadily increases, in agreement with the trend in Fig. 2; the unbinding mode E2 is dominated by the pairing ones.

Note that the binding energy increases with⳵toxas predicted by the weak-coupling theory, but also with 兩⳵t兩, suggesting that at strong coupling the Cu-O bond stretching grows in importance.

In Fig. 3共b兲 we included all vibrations except E2. The E1

vibrations are strongly pair breaking, and ⌬˜(4) is much smaller in magnitude than in Fig. 3共a兲; it becomes positive at intermediate coupling. It is likely that the couplings to the pair-breaking E modes are somewhat underestimated by the choice of␭ parameters in Fig. 3共a兲 and overestimated in Fig. 3共b兲. Interestingly, however, at stronger coupling the pairing modes prevail again driving the system to pairing共bipolaron formation兲. This resembles the trend found in Ref. 9, al-though there a Hubbard-Holstein framework is used and since the system is one-dimensional the electronic pairing does not occur.

These results yield several indications. First, the cata-strophic distortions predicted by the JT approximation are not borne out by more complete approaches involving a

broader spectrum of electronic states. This interesting result arises since the electronic ground state belongs to a narrow multiplet; the standard treatment of the JT effect singles out the lowest level, which is justified only at weak EP coupling. Pairing prevails also at strong coupling in part of the param-eter space in the symmetry channels where W⫽0 pairs oc-cur. The correct trend is predicted by the canonical transfor-mation approach, which also explains the pairing or pair-breaking character of the modes. In particular it is found that the half-breathing modes give a synergic contribution to the purely electronic pairing; since they are believed to be mainly involved in optimally doped cuprates, our findings suggest a joint mechanism, with the Hubbard model that cap-tures a crucial part of the physics. This scenario was also drawn in the context of an extended t-J model, where the half-breathing mode was found to enhance electronic pairing.6,23Finally, experimental data on nanopowders24also indicate that one should not be overly pessimistic about clus-ter calculations. YBa2Cu3O6⫹xpowders consisting of 0.7 nm

thick grains with an 11 nm radius show the same TC as the bulk, indicating that going to the thermodynamic limit could not be essential to understand pairing. Cluster calculations can be relevant and physically insightful concerning the in-terplay of various degrees of freedom on pair structure and formation.

1For an overview, see E. Dagotto, Rev. Mod. Phys. 66, 763共1994兲, and references therein.

2M.K. Crawford, M.N. Kunchur, W.E. Farneth, E.M. McCarron, and S.J. Poon, Phys. Rev. B 41, 282共1990兲; Science 250, 1390 共1990兲; J.P. Franck, et al., Physica C 185-189, 1379 共1991兲; Phys. Rev. Lett. 71, 283共1993兲; J.P. Franck, Physica C 235-240, 1503共1994兲.

3R.J. McQueeney, Y. Petrov, T. Egami, M. Yethiraj, G. Shirane, and Y. Endoh, Phys. Rev. Lett. 82, 628共1999兲.

4Z.X. Shen, A. Lanzara, S. Ishihara, and N. Nagaosa, cond-mat/0108381共unpublished兲.

5O. Ro¨sh and O. Gunnarsson, cond-mat/0308035共unpublished兲. 6S. Ishihara and N. Nagaosa, cond-mat/0311200共unpublished兲. 7C.H. Pao and H.B. Schuttler, Phys. Rev. B 57, 5051共1998兲; ibid.

60, 1283共1999兲.

8A.S. Alexandrov, Phys. Rev. B 46, 2838共1992兲; G. Wellein, H. Roder, and H. Fehske, ibid. 53, 9666 共1996兲; J. Bonca, T. Katrasnik, and S.A. Trugman, Phys. Rev. Lett. 84, 3153共2000兲. 9Y. Petrov and T. Egami, APS, Annual March Meeting Y 20, 003

共2000兲.

10S. Mazumdar, F. Guo, D. Guo, K.C. Ung, and J.T. Gammel, cond-mat/9303003共unpublished兲; J.T. Gammel and D.K. Camp-bell, cond-mat/9209025共unpublished兲.

11S.R. White, S. Chakravarty, M.P. Gelfand, and S.A. Kivelson, Phys. Rev. B 45, 5062 共1992兲; A. Parola, S. Sorella, M. Par-rinello, and E. Tosatti ibid. 43, 6190共1991兲.

12M. Cini and A. Balzarotti, Phys. Rev. B 56, 14 711共1997兲. 13E. Perfetto, G. Stefanucci, and M. Cini, Phys. Rev. B 66, 165434

共2002兲.

14A. Callegari, M. Cini, E. Perfetto, and G. Stefanucci, Phys. Rev. B 68, 153103共2003兲.

15

M. Cini, A. Balzarotti, R. Brunetti, M. Gimelli, and G. Stefanucci, Int. J. Mod. Phys. B 14, 2994共2000兲.

16W. Kohn and J.M. Luttinger, Phys. Rev. Lett. 15, 524共1965兲. 17J. Bonca and S.A. Trugman, Phys. Rev. B 64, 094507共2001兲. 18A.S. Alexandrov and P.E. Kornilovitch, J. Phys. C 14, 5337

共2002兲.

19A.S. Alexandrov, Int. J. Mod. Phys. B 17, 3315共2003兲.

20M. Cini, G. Stefanucci, and A. Balzarotti, Eur. Phys. J. B 10, 293 共1999兲.

21E. Perfetto and M. Cini共unpublished兲.

22M. Cini, A. Balzarotti, and G. Stefanucci, Eur. Phys. J. B 14, 269 共2000兲.

23T. Sakai, D. Poilblanc, and D.J. Scalapino, Phys. Rev. B 55, 8445 共1997兲.

24P. Paturi, J. Raittila, H. Huhtinen, V.-P. Huhtala, and R. Laiho, J. Phys.: Condens. Matter B 15, 2103共2003兲.

BRIEF REPORTS PHYSICAL REVIEW B 69, 092508 共2004兲

Figura

FIG. 3. ⌬˜(4) as a function of ⳵t ox for different values of ⳵t.

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