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Singlet pair liquid, antiferromagnetism and

superconductivity in a nearly half-filled narrow band

M. Héritier

To cite this version:

M. Héritier. Singlet pair liquid, antiferromagnetism and superconductivity in a nearly half-filled nar- row band. Journal de Physique, 1987, 48 (11), pp.1849-1854. �10.1051/jphys:0198700480110184900�.

�jpa-00210626�

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Singlet pair liquid, antiferromagnetism and superconductivity in a nearly

half-filled narrow band

M. Héritier

Laboratoire de Physique des Solides, Université de Paris-Sud, Centre d’Orsay, 91405 Orsay, France

(Regu le 29 juillet 1987, accepté Ie 21 septembre 1987)

Résumé.2014 L’état de liaisons de valence résonnantes d’Anderson est discuté dans un modèle simple de liquide de paires singulets dans une bande de Hubbard étroite presqu’a moitié remplie. Outre les solitons

de spin, les trous en excès liés à une paire soliton-antisoliton forment un liquide de Fermi d’excitation,

dans lequel le nesting induit une instabilité antiferromagnetique près du demi-remplissage. L’échange

de fluctuations singulets produit entre trous en excès une forte interaction attractive conduisant à une

transition supraconductrice de temperature critique élevée, dont le maximum se trouve à la transition

liquide singulet-paramagnétique. L’application aux nouveaux oxydes supraconducteurs est discutée.

Abstract.- Anderson’s resonating valence bond state is discussed in a simple model of singlet pair liquid, in a nearly half-filled narrow Hubbard band. Besides the spin solitons, the excess holes bound to soliton-antisoliton pairs form an excitation Fermi liquid, in which nesting induces an antiferromagnetic instability near half-filling. A strong attractive interaction between excess holes arises from echange of singlet pairing fluctuations, leading to a superconducting transition with a high critical temperature, maximum at the singlet liquid-paramagnetic transition. Application to the new superconducting oxides

is discussed.

Classification

Physics Abstracts

74.20D - 74.70Y - 75.10J

In the profusion of high T, superconductivity theories, one usually distinguishes conventional

mechanisms, in which electron-phonon cou- pling meets highly favourable circumstances,

from unconventional ones. In the latter cate- gory, the most original and the most widely dis-

cussed theories invoke Coulomb and magnetic

correlation effects, either in the weak correla- tion or in the strong correlation limit. In fact,

weak correlation models, involving exchange of antiferromagnetic fluctuations between itinerant electrons in a wide band [1], have already been proposed to discuss heavy fermion or quasi-

one dimensional superconductors [2]. They im-

ply a maximum of the superconductivity criti-

cal temperature at the antiferromagnetic transi- tion, which is observed in Bechgaard salts [3], but

probably not in the new superconducting copper

oxides [4]. Anderson [5] was the first to pro- pose to describe this new class of materials by

a Hubbard model in the narrow band limit. The

typical example is La2-.,,,, -xsrx CU04-y. Crystal

field splitting leaves an orbitally non-degenerate

copper dx2 -y2 band, strongly hybridizing with

the oxygen p-band half-filled in the "pure com- pound" (x’ = x = y = 0), which is described by a

two-dimensional square lattice Hubbard model :

Precise values of t and U are still unknown, but experimental data seem to indicate intermediate values for the ratio t N 1. Our basic hypothesis

is that we are on the insulating side of the Mott

Article published online by EDP Sciences and available at http://dx.doi.org/10.1051/jphys:0198700480110184900

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1850

transition, as in Anderson et al. [5] and in Cyrot [6], rather than in the itinerant case [1]. In the

following the typical figures t N 0.5 eV, U - 5 eV

will be considered.

Doping and non-stoichiometry introduce a

concentration 6 = x+3x’-2y of excess holes in

the half-filled hand. Note that x’ is generally badly known. A value x’ N 0.02 in the "pure compound" without oxygen vacancies (x = y = 0) gives 6 =0.06, to be compared with the doped

case z = 0.15, x’ = 0, y - 0.04 corresponding

to 6 = 0.07. Therefore similar superconducting properties [7] for x = 0 and x = 0.15 might well

be ascribed to compensating effects of lanthanum and oxygen vacancies.

Perfect nesting of the U = 0 half-filled tight binding band of equation (1) implies an antiferro- magnetic instability of the Hubbard model either in the small U or in the large U limit. However,

Anderson et al. [5] have proposed that quan-

tum fluctuations stabilize a state of Resonating

Valence Bonds [8] (RVB).

We shall adopt the same hypothesis, con- sidering the RVB state as the reference state in which antiferromagnetic and superconducting in-

stabilities may occur. More precisely, we approx- imate the RVB state by a liquid of singlet pairs

(SPL) defined as follow : consider a partition

of the 2N lattice sites into N nearest neighbour pairs. In the half-filled case, a singlet is created

on each pair (ij)

thus defining a singlet pair configuration. The

SPL is a coherent superposition of all the possible singlet pair configurations corresponding to the possible pair partitions.

Anderson et al. [5] and Kivelson et al. [9]

have dicussed the nature of such a state : it does not possess a broken symmetry and a long range order. However, a topological long-range order

can be defined. Topological excitations are neu-

tral spin solitons (or antisolitons), i.e. dangling

bonds obeying Fermi statistics, formed in pair by breaking a singlet pair, and charged boson

formed by adding an excess hole which bind to a

free spin, leaving a charged soliton, with charge

+e and spin 0.

In the large U limit, the Hubbard Hamilto- nian (1) can be written in the sub-space without

double occupancy of atomic sites :

where J = 4t2/U, 8i+ = c£r Ci, Pi = ErCc,

and H’ describes the kinetic terms :

We define the singlet pair creation operator

The relative phases between neighbouring sin- glet bonds determine the nature of the singlet pairing. In the following, we consider the case

of extended s-wave singlet pairing and of d-wave

singlet pairing described by a gap function

in which A is the mean-field "order parameter"

defined by

..

and 7k = cos kxa + cos kya, where the sign +

stands for the extended s-wave and sign - for the

d-wave.

The Hamiltonian reads

Singlet pairing is favoured by the exchange

term but inhibited by the kinetic term.

The latter is not simple to handle because of the Gutzwiller projection. Up to now, the effects of this projection have not been taken into account properly. This work is the first at-

tempt, as far as we know, to treat them seriouly.

We shall see below that the effects neglected so far, i.e. principally a Nagaoka ferromagnetic ex- change induced by the kinetic energy of the ex- cess holes, have a crucial importance : first, they

influence the RVB long or short range order and the nature of the quasiparticle spectrum ; may be even more importantly, they provide a new mechanism, which has not been considered so far

[13], for Cooper pairing and therefore supercon-

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ducting ordering by exchange of magnetic fluc-

tuations between excess holes in the strong cor- relation limit.

First, we consider the limit Ult » 1, using

the results of Nagaoka [10] in the limit U/t - oo.

The propagation of an excess hole through the

lattice perturbs the spin configuration. Although singlet pairing is preserved [5], the singlet bonds

are displaced by the hole tunnelling, thus de- stroving the wave function phase coherence : the

wave vector is no longer a good quantum num- ber [11]. Using the techniques of Nagaoka [10]

and Brinkman and Rice [11], the self energy of

an excess hole described by H’, localized on site

i for a spin configuration {Q}, can be written :

where the An I s are the weighted number of diagonal n-step walks of the excess hole through

the lattice. A diagonal walk is a walk in which the initial spin configuration (ol is restored when the hole return to the site i. In the ferro-

magnetic configuration, all the walks are diago-

nal : this property minimizes the kinetic energy

[10]. The excess hole density of states has the

full band width 2xt of the non interacting case.

In a random spin configuration, the contribution of the closed loops to the An s are strongly re-

duced, and even more in the antiferromagnetic configuration [11]. In the latter case, to a good approximation, the diagonal walks reduce to the

self-retracing walks [11] : the contribution of the closed loops are almost completely supressed.

This tends to localize the hole, increases its ki- netic energy and narrows the bandwith.

In the SPL configuration, in the case of a

"bare" excess hole or of a "charged boson", the

contribution of the closed loops are negative [12] :

the hole return to the origin with a phase shift

x. The result is a destructive interference effect,

which tends to localize the hole and increases its kinetic energy compared to the antiferromag-

netic case. For example, the smallest closed loop

on the square lattice (this could be extended to any alternate lattice), the 4-step square, has a

weight - 2 in the SPL. However, creating an ex-

cess hole in a perfect SPL necessarily breaks a singlet pair, forming a soliton-antisoliton pair.

The "charged boson" is a soliton-hole bound sta- te. It is also possible, without spending any more magnetic energy to bind the charged boson to

the anti-soliton, i.e. to the dangling bond. This is very efficient in suppressing the closed loops

available for the hole propagation [12]. Then,

the excess hole bound to the soliton-antisoliton

pair has a kinetic energy comparable to the bare

hole in the antiferromagnetic lattice. Using the

moment technique of Brinkman and Rice [11],

we have calculated the lower band edge energy of the excess hole in the square lattice, for var-

ious spin configurations. The results are : -4 t in the ferromagnetic case, -3.5 t in the antifer-

romagnetic case, -3.3 t for the charged boson

in the SPL and -3.5 t for the hole bound to the soliton-antisoliton pair in the SPL. There- fore, the latter quasiparticle should be stable at

temperature lower than a binding energy - 0.2 t

(-1000-2000K) and should behave as a "charged

fermion" .

The picture discussed by Anderson et al.

[5] and by Kivelson et al. [9] was the follow-

ing : introducing excess holes in the half-filled band by doping does not change the spin soli-

ton Fermi surface but creates charged boson ex-

citations which can undergo a Bose-Einstein con-

densation leading to superfluidity. Our point of

view is different. We recover the more intuitive

picture in which doping introduces excess holes which behave as charged fermions strongly cou- pled to magnetic fluctuations by many body ef-

fects.

The results show the importance of the cou- pling between the excess hole and the singlet pairing correlation, which can be described by

an interaction Hamiltonian of the form :

in which akq is a numerical factor of order unity.

First, consider the half-filled case 6 = 0. The Hamiltonian (6) is easily solved in the mean-field

approximation. A mean field critical tempera-

ture for SPL formation kBTe(6 = 0) =t2/U is

found for extended s-wave as well as for d-wave

pairing.

As shown by Anderson et al. [5] and by

Kivelson et al. [9], the quasi-particles in the half- filled case 6 = 0 are spin soliton fermions, with

a dispersion Eo(k) = J d I lie I exhibiting perfect

nesting for the wave vector Q = (E, E) . These

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1852

quasiparticles can be described by a Fermi liq-

uid theory for kBT J. As noted by Anderson

et at. [5], perfect Fermi surface nesting implies

an antiferromagnetic instability, if one takes into

account the quasiparticle interactions, neglected

in the Hartree-Fock Hamiltonian but of course

present. If A is the molecular field constant for these interactions, the Neel temperature is of the

form :

where Ao = 1 £k 1-yk I is the low temperature SPL order parameter. This picture is only valid

for Tun « Tel’ which requires A « J, a condition

which might not be fulfilled. Nevertheless, we be-

lieve that perfect nesting would imply an insta- bility in any case, even though the correct treat- ment would be much less simple.

Adding a concentration 6 « t/U of excess

holes, they form ferromagnetic spin polarons, as

a result of the balance between kinetic energy and magnetic free energy, propagating in the an- tiferromagnetic medium. The SPL energy spec- trum may be approximated by

where Ep is the spin polaron energy. The pres-

ence of excess holes rapidly spoils the Fermi

surface nesting, and antiferromagnetism is de- stroyed by a small value of 6. In fact, in real systems, a small violation of perfect nesting ex-

ists even at half-filling. Best nesting, and, thus,

maximum of TN might occur slightly away from

half-filling. In some cases, nesting may be too

imperfect to induce an instability and antiferro-

magnetism may not occur at all. This might be

the case of the YBa2Cu307-y compounds.

However, this picture corresponds to the li-

mit U/t » 1, while the real situation seems

rather U/zt £5 1. As Ult decreases, the polaron

energy increases, and eventually, for a critical ra-

tio (Ult)c - the polaron state merges with the

band of diffusive motion of the bare hole. The

precise determination of this critical value de-

pends very much on the details of the variational treatment, but the Cu oxide situation seems to

correspond to this limit in which the polaron

state is no longer stable : the excess hole is no

longer surrounded by a long life-time ferromag-

netic bubble, but it is strongly coupled to large amplitude local spin fluctuations. The complete description of such a system is very difficult, but

the simplest approximation is a mean field ap-

proach in which the spin fluctuations are, first, neglected. In this sheme, because of the coupling

(8), we replace the kinetic term Hr in (2) by an

effective kinetic Hamiltonian for the excess hole

f, I :

in which wo (A) is the Brinkman-Rice bandwidth

narrowing factor [11] and ek is the dispersion

relation for non-interacting electrons (U = 0).

Moreover, the kinetic energy dependence on A is responsible for a molecular field for singlet pair- ing, which we write in the form :

in which a is a numerical factor of order unity,

and p is the mean field average (ct cj) on nearest

neighbour bond (ij). We must emphasize that

this is only a rough approximation because the

wave vector is not a good quantum number. The

excess hole should be described, in principle, by

a broad wave packet.

Using (9) and (10) our Hartree-Fock Hamil- tonian for the SPL transition reads :

in which p is the chemical potential.

The Bogolubov transformation gives the quasiparticle energy :

The gap and the chemical potential are given by

the self-consistence equations :

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As 6 increases from zero, Te decreases rapidly. It

is given by :

,

where ek = 6wo (A)ek - p.

The decrease is much larger for extended s-wave

pairing, where -y2 vanishes on the Fermi surface

ek = 0, than for d-wave pairing where the aver-

age of i£ on the Fermi surface is 1. In the latter case, for 8 « t

where a’ is a numerical factor of order unity.

At larger values of 6, Tc decreases very rapidly

and vanishes for 6c given, still in the d-wave, ap-

proximately by the equation

with

so that 6, til t

-

u .

Therefore, in this picture, we expect a d-wave SPL. However, this result depends heavily on the approximation made in (9), which describes the

excess hole by a well defined wave vector. The

wave packet broadening should strongly reduce

the energy difference between s-wave and d-wave

pairing. In fact, a mixing of these two states, as allowed by the symmetry of the orthorhombic or

tetragonal lattice, seems plausible.

As discussed above, this simple treatment neglects the large spin fluctuations which sur-

round each excess hole. As in any intermedi- ate coupling problem, it seems difficult to give

a precise treatment of these fluctuations, but they probably destroy the small energy gap -

61, which, itself, requires the presence of ex- cess holes. Therefore the SPL long range order is probably destroyed, but short range magnetic

correlations still persist as long as 6 « (t/U)1/2.

As above, a small concentrations of excess holes

spoils the nesting and rapidly destroys antifer-

romagnetism. We are left with a short range SPL order below the mean field SPL "transition line". It does not seem possible to invoke a Bose-

Einstein condensation of the "charged bosons",

since they are trapped by spin antisolitons.

However, a Cooper pairing of the charged

fermions can be induced by the strong coupling

to the singlet fluctuations described by equation (8). Exchange of singlet pairing fluctuations gi-

ves rise to an effective interaction between fer-

mions, the low frequency behaviour of which is attractive. Keeping only the terms in which

the Cooper pairs have zero momentum, the hole interaction takes the forms :

where wm (q) is the singlet pairing fluctuation en-

ergy, and A(k, k’) is a numerical factor. The or-

der of magnitude of this attractive coupling, is

the low frequency limit, is - J - -U, and of

the cut-off energy beyond which the interaction becomes repulsive J. One can replace the attrac-

tive potential by a constant at frequency lower

than J, as in BCS. The dimension-less coupling

parameter is g - I - T 81/2. For 6 « (If) 2 , t the

weak coupling limit gives a BCS ordering tem- perature

However, this approximation breaks down when

one approaches the SPL mean field transition.

The trace over the singlet pairing operators in- volves the correlation function for singlet pairing

The attractive potential between fermions can be written

which diverges on the SPL transition line, where, therefore, we expect the maximum superconduc- ting critical temperature. Of course, the same

mechanism applies in the paramagnetic phase,

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1854

with the same orders of magnitude. The qualita-

tive origin of this strong attrative interaction be- tween excess holes is easy to understand : an ex- cess hole destroys the singlet correlation around itself to lower its kinetic energy. This is energet- ically favourable to the second excess hole reab-

sorbing the magnetic fluctuations.

The expected phase diagram is schematized in figure 1.

The main features are the following :

i) antiferomagnetism appears near half-filling for good enough nesting and is rapidly destroyed by doping. Antiferromagnetic order is not necessary for the occurrence of superconductivity and may be absent if nesting is not good enough.

ii) The superconductivity transition temperature

is maximum on the SPL transition line for 6

b, away from the antiferromagnetic transition.

Such a model seems to well describe the main properties of the new superconduct- ing oxides L82-:.cSr:.cCu04-y, but also YBa2Cu3 07-y, in which less good nesting might not

allow antiferromagnetism.

I gratefully thank G. Collin, J. Joffrin, G.

Montambaux, C. Noguera and J.-P. Pouget for helpful discussions.

Fig.l.- Phase diagram of the Hubbard model for a

concentration 6 of excess holes. Antiferromagnetic instability of the singlet pair liquid occurs very near

half-filling. The shaded area represents the supercon-

ducting phase, with a maximum of the critical tem-

perature on the SPL transition line.

References

[1] EMERY, V.J., Synth. Metals 13 (1986) ;

MIYAKE, K., SCHMITT-RINK, S. and VAR-

MA, C.M., Phys. Rev. 334 (1986) 6554 ; SCALAPINO, D.J., LOH, E. and HIRSCH, J.E., Phys. Rev. B34 (1986) 8190 ; SCHULZ, H., to be published, BEAL-MONOD, to be published.

[2] EMERY, V.J., J. Physique Colloq. 44 (1983)

C3-977 ; BEAL-MONOD, M.T , BOURBON-

NAIS, C. and EMERY, V.J., Phys. Rev. B34

(1986) 7716.

[3] JÉROME, D. and SCHULZ, H., Adv. Phys.

31 (1982) 299.

[4] BEDNORZ, J.G. and MÜLLER, K.A., Z.

Phys. B64 (1986) 188 ; UCHIDA et al., to

be published, CHU, P. et al., Phys. Rev.

Lett. 58 (1987) 405 ; ZHAO, Z. et al., KE

XUE TONGBAO, to be published.

[5] ANDERSON, P.W., Science 235 (1987)

1196 ; BASKARAN, G., ZOU, Z. and ANDERSON, P.W. to be published ;

ANDERSON, P.W., BASKARAN, G., ZOU, Z.

and Hsu, T., Phys. Rev. Lett. 58 (1987)

2790.

[6] CYROT, M., to be published.

[7] BEILLE, J., CABANEL, R., CHAILLOUT, C., CHEVALLIER, B., DEMAZEAU, G., DESLAN-

DES, F., ETOURNEAU, J., LEJAY, P., MI-

CHEL, C., PROVOST, J., SULPICE, A., THOLENCE, J.L., TOURNIER, R.C., Hebd.

Scean. Acad. Sci. 304 II (1987) 1087.

[8] ANDERSON, P.W., Mat. Res. Bull. 8 (1973)

153 ; FAZEKAS, P. and ANDERSON, P.W.,

Philos. Mag. 30 (1974) 432.

[9] KILVELSON, S., ROKHSAR, D. and SETHNA,

J. Phys. Rev. B35 (1987) 8865.

[10] NAGAOKA, Y., Phys. Rev. 147 (1966) 392.

[11] BRINKMAN, W.F. and RICE, T.M., Phys.

Rev. B2 (1970) 1324.

[12] HÉRITIER, M., to be published.

[13] see DE GENNES, P.G., to appear in C.R.

Hebd. Scéan. Acad. Sci. for a similar mech-

anism caused by double exchange.

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