• Aucun résultat trouvé

Pressure dependence of Tc and electron phonon interaction in MBa2Cu3O7 systems

N/A
N/A
Protected

Academic year: 2021

Partager "Pressure dependence of Tc and electron phonon interaction in MBa2Cu3O7 systems"

Copied!
12
0
0

Texte intégral

(1)

HAL Id: jpa-00211006

https://hal.archives-ouvertes.fr/jpa-00211006

Submitted on 1 Jan 1989

HAL is a multi-disciplinary open access archive for the deposit and dissemination of sci- entific research documents, whether they are pub- lished or not. The documents may come from teaching and research institutions in France or abroad, or from public or private research centers.

L’archive ouverte pluridisciplinaire HAL, est destinée au dépôt et à la diffusion de documents scientifiques de niveau recherche, publiés ou non, émanant des établissements d’enseignement et de recherche français ou étrangers, des laboratoires publics ou privés.

Pressure dependence of Tc and electron phonon interaction in MBa2Cu3O7 systems

J.M. Besson

To cite this version:

J.M. Besson. Pressure dependence of Tc and electron phonon interaction in MBa2Cu3O7 systems.

Journal de Physique, 1989, 50 (12), pp.1433-1443. �10.1051/jphys:0198900500120143300�. �jpa-

00211006�

(2)

Pressure dependence of Tc and electron phonon interaction in

MBa2Cu3O7 systems

J. M. Besson

Physique des Milieux Condensés (*), Université Pierre et Marie Curie, T. 13, E. 4, 4 Place Jussieu, 75252 Paris, France

(Reçu le 21 mars 1989, accepté le 21 avril 1989)

Résumé.

2014

Les coefficients de pression des températures critiques Tc, dans la série

MBa2Cu3O7-y sont analysés (M

=

yttrium ou un élément des terres rares). En utilisant le modèle BCS à deux dimensions, on peut relier les variations de Tc avec y et avec la pression hydrostatique, la diminution de y étant équivalente à une surpression interne. Les modes de

compression symétrique Ag du barium sont responsables de l’interaction électron-phonon, et leur

variation sous pression est comparée au comportement de modes similaires dans d’autres structures à basse dimensionnalité (1-D et 2-D). Un mécanisme est proposé pour expliquer

l’interaction électron-phonon, mécanisme qui contribuerait au couplage électron-électron.

Abstract.

2014

Existing data for the pressure derivatives of critical temperatures Tc in the

MBa2Cu3O7-y family are analyzed (M

=

Y, or rare earth). Using a two-dimensional BCS model, the electron-phonon coupling parameter is shown to be responsible for the increase of

Tc, which varies with y in the same way as under an equivalent internal pressure. The anharmonic barium symmetrical stretching mode is compared with similar phonons in other 1-D or 2-D quasi-

low-dimensional structures. A possible mechanism for large electron-phonon interaction and electron-electron pairing is proposed.

Classification

Physics Abstracts

74.20F

-

62.50 - 71.38

Introduction.

High pressure measurements have been used since the discovery of high 7c superconductors

to try to understand their mechanism, especially after large pressure coefficients [1] for 7c were shown to occur in those crystals. Attempts to relate the observed pressure

dependence of the critical temperature to existing theories have only been moderately

successful and a very complete discussion of the subject [2] has recently been published.

Here, the available data on the pressure dependence of the critical temperature of the

MBa2CU307 -y series are examined (M

=

Y, Eu, Gd, Sm and Yb). The other series are not

(*) Physique des Milieux Condensés is associated with the C.N.R.S.

Article published online by EDP Sciences and available at http://dx.doi.org/10.1051/jphys:0198900500120143300

(3)

discussed, for lack of enough experimental data. It will thereon be designated as MBCO for brevity, unless otherwise specified.

The first section is devoted to a critical selection of experimental values for the pressure variation of Tc. The variation of the electron-phonon interaction in MBCO under pressure is then extracted by use of the 2-D BCS formalism [3-5]. This indicates that the large increase, under pressure, of the interaction of electrons with the Ba2 + symmetric stretching mode along z is expected, and quantitatively fits the observed behavior [6] of corresponding modes (Cs+) in other quasi-low-dimensional systems (CsCdBr3). In the conclusion a coupling

mechanism for electrons is proposed, through the Ba2 + Ag ion vibration, which may induce

large charge transfer in the z direction, âs in other two-dimensional structures [7].

Analysis of high pressure results.

A systematic comparison of dTc/dP has recently been done [2] for the four main classes of high 7c supraconductors :

A clear trend is that dTc/dP is smaller in the high 7c crystals. Below 90 or 100 K nevertheless, data points scatter all over the dTc/dP - 7c plane especially when plotted as

d log Tc/d log V vs. Tc. In the present analysis we will keep to the following rules.

i) Definition of the « critical temperature » Tc : a number of definitions have been

proposed for Tc : zero resistance

-

onset temperature (Tco)

-

midpoint of resistance drop (Tcm)

-

and others. In any case, under pressure, these quantities may well behave in opposite

directions. For instance [8] in YBa2Cu307 - y samples, the zero resistance temperature decreases under pressure, Tco increases and 7cm is almost constant... This flattening out of the resistivity drop under pressure may indeed in some cases be a bona fide physical effect yet to be explained, but could also be related to pressure gradients, crystal inhomogeneities,

internal strain (and stress) variations, etc... The most desirable data (zero resistance) are very few. Onset T co values under pressure are more numerous but subject to uncertainties due to

variable and optimistic definitions of the authors, especially on the high temperature side.

Besides, they are the most sensitive to pressure-induced inhomogeneities. Values for

7cm are comparatively more numerous and are used here as the best compromise. These shall be referred hereafter simply as Te

=

midpoint of resistance drop.

ii) When comparing Tc’s under pressure, only [dTc/dP ]p

=

o shall be used, that is the initial

slope, not the evolution of the slope under pressure, in the few cases when this is known. This restriction is related to the reasons quoted above (i) : Especially in the higher pressure range

(P >_ 10 GPa ) 7c(P) measurements are not done under hydrostatic conditions and have not

yet been shown to be reversible, in the published literature.

iii) Only the MBCO series will be discussed here. Too few data exist over a large 7c range in the La (SrBa) CuO and (TlBi)(CaSr) CuO compounds. Studies on crystals where

Cu is substituted [9] with Fe, Ni or Zn must not be included here. This would be quite

misleading : here, only the dependence of 7c on electron-phonon interaction will be

(4)

discussed, not the electronic contribution which is surely affected by substitution of other elements onto copper sites.

iv) For analogous reasons one data point [10] concerning Yo.4Bao.6Cu03 cannot be retained

for comparison. Barium, there, is not in the same configuration as in MBa2CU307 and this is of

prime importance for the present discussion.

v) The usable data points which are retained after this selection [11-16] are given in the

table I. They are also plotted in figure la. Actually we could have used a few more for the

high 7c region (- 90 K) but they all fall in the same area with small, positive or, in a few cases, negative values and this does not modify the shape of the curve in figure 1. Before proceeding

to the next section, let us note that the low-T, points (n° 5, 6 and 10) are the oxygen-deficient samples (y - 0.5 ). Their pressure coefficient is high and their c-parameter is larger. The dependence of the c-axis and 7c on O-deficiency is well documented [17] and shows strong correlation in both orthorhombic superconducting phases, above and below y

=

0.3.

Table I. - Data points used in this discussion. T, is the critical temperature at 50 % of the

resistance drop. Number of the samples are recalled in figures 1 a and 2 for identification.

COMPARISON WITH 2-D BCS. - These results will now be examined in the light of the 2-D BCS theory [3].

À depends [3, 4], among others, on the electron-phonon interaction, the relevant phonon frequency, and the number [5] of adjacent CU02 sheets in the compound.

To is an ad hoc characteristic temperature which accounts both for the width of the 2-D electronic density of states singularity, and for the equivalent Debye temperature for electron-phonon interaction. To - 600 K is a value that fits well with experiments and was

used for figure 1b. Actually, any To between 400 K and 900 K, may be used without changing

the conclusions.

In the present discussion, the variation under pressure of 7c will be related to À through equation (1) and will be shown to depend largely upon the variation of the electron-phonon

interaction. The variation of the phonon frequency will be neglected, since it is a second order

(5)

Fig. 1.

-

a) Left-hand ordinates : dTc/dP vs. T, from the table. Figures correspond to the first column.

Full line is related to the curve in figure 2 by equation (1). b) Right-hand scale : dashed line is A from

equation (1).

contribution (10 to 20 % at most) as compared to the large (over one order of magnitude)

variation of the electron-phonon interaction. Since all compounds studied here have the same

number of adjacent Cu02 sheets, no scaling factor [5] need be taken into account either.

Curve (la) is now plotted in different coordinates in figure 2, that is using À 2 in place of 7c through equation (1), in order to take the square of the electron-phonon interaction as the

appropriate function of pressure. We thus plot :

using :

Integration of (2) gives :

F is any function that goes well through the data points and the inverse of which is readily integrable. It has, for the time being, no physical meaning. Integration can also be done

numerically. This is shown in figure 3, with pressure being defined only within the arbitrary integration constant C.

What does this mathematical procedure mean ? First of all, hydrostatic pressure brings

about a known variation of Tc, that is d7c/dP (experiments). Each observed sample, with its

characteristic Tc (abscissae scale) is then assigned an equivalent intemal pressure. This is caused in the present case by variable oxygen content but should not be related explicitly to

the oxygen deficiency, or, for that matter to the known [17] variation of the crystal axes

through some « experimental » bulk modulus. The reason for this is that long-range forces

(6)

Fig. 2.

-

Function F in equation (2) : obtained from figure 1 with ordinates and abscissae transformed

by equations (3) and (1) respectively. Full line is the slope of the curve in figure 3.

Fig. 3.

-

Variation of the expected electron-phonon interaction with extemal pressure or intemal pressure in MBCO’s, represented by variation of À 2 vs. pressure + integration constant (C in Eq. (4)).

(Coulomb interaction for instance) do bring in an analogue of an intemal pressure but with

tensorial properties which may be quite different from hydrostatic pressure. For example, in

layered compounds, the Coulomb glue is largely a uniaxial stress, not a uniaxial pressure, and

not a purely hydrostatic pressure either, as regards the actual crystal deformation. In the case

(7)

of molecular crystals in the generalized sense, that is 0-D, 1-D or 2-D structures which is the

case here, there are obvious differences in the behavior under pressure of properties linked to

the intramolecular space or intermolecular space. The latter which is more compressible at

low pressures may actually become stiffer than the former under compression [7, 18]. Thus,

other properties of the crystal will not vary in the same way as Tc does under internal pressure.

Notably, the c-axis does decrease in length under increasing internal pressure when y decreases and this variation can be plotted as a function of Te, forgetting the intermediate y variable which actually causes the effect. The decrease of c with increasing Tc is quite smooth

with a slope dTc,/d log c - 6 000 K and shows no strong discontinuity at the orthorhombic orthorhombic phase transition at y

=

0.3. But if one attempts to relate it to an intemal pressure through a bulk modulus of some - 170 GPa which is the average value for this class of compounds, one finds an intemal pressure scale which is different from that derived from

Te. Another consequence of this separate behavior of inter- and intramolecular regions in crystals with two or more kinds of chemical bonds is that the so-called « Grüneisen constants » have little physical significance and are usually not constant. They can be used only for isotropic crystals with one type of chemical bonds (interatomic potentials). Notably a quantity

such as : d log Tc/d log V (V the volume) will not be used here.

In summary, the meaning of the integration done here on À 2, on which Te depends is : The

variation of Te is due to an equivalent intemal pressure which brings about a compression of

some region of the crystal structure which is, at the present stage of the argument, undetermined. This region is responsible for the electron-phonon interaction which is one

step among the steps leading to superconductivity. It need not be the same region where current-carrying regions are located. As a matter of fact, it probably is not here, as will be proposed in the conclusion.

Discussion.

At the present time, no experimental data exist on the evolution of the electron-phonon

interaction in superconducting perovskites under pressure. It is thus necessary to rely on what

is know in other low-dimensionality systems to see if any reasonable physical analogy can be

drawn. In this section a comparison will be made first with the quasi 1-D CsCdBr3 perovskite,

then with a bona fide 2-D layered crystal : GaSe under high pressure.

a) COMPARISON WITH CsCdBr3. - This 1-D structure is made up of rigid ionicovalent chains of (CdBr6 )- octahedra separated by chains of softer Cs+ ions. Under pressure the Cs+ ions do indeed compress [6] as their rare gas analogue, that is xenon, which has the same

closed electronic shells. At ambient, the Coulomb glue between the CdBr6 and the

Cs+ chains is weak enough to leave ample space to the cesium atoms in their rhom- bododecahedral bromine cages : Phonons involving movement of Cs atoms normal to the c- axis, have a large pressure coefficient and weak Raman intensity. Above - 5 GPa, the outer

electrons of Cs+ come into contact with the bromine shells and react in the same way as rare gas atoms do under pressure : they become highly incompressible in the hard sphere regime [19, 20]. Thus, in the low-pressure (van der Waals) regime, Cs vibrations are more or less

harmonic, electron shells and core moving together. Above some 10 GPa, on the contrary, the electronic shell is blocked and the phonon mode induces strong charge transfer, which

means high electron-phonon interaction. This cross-over from the low- to high- pressure

regimes is clearly seen in the pressure dependence of the frequency w of the Ea 29 mode in

CsCdBr3 which involves the motion of Cs : d log w /dP decreases from - 10-1 GPa-1 at ambient down to - 1 x 10- 2 GPa-1 at 10 GPa. At the same time, the Raman intensity of this

mode increases by an order of magnitude relative to the total intensity of all other modes.

(8)

Now the Raman intensity in a transparent crystal is proportional to the Raman cross section

which is :

a, (3 : intermediate states

i, s : incident and scattered photons

HER, HEp : electron-radiation and electron-phonon hamiltonians. Far away from any resonance, which is the case here, the Raman intensity will be proportional to the square of the electron-phonon interaction (HEP ), and thus to À 2, which is the reason why this parameter

was chosen for figure 3.

In figure 4, the calculated values of À 2 of figure 3 for MBa2Cu307 - y are superposed with

the Raman intensity values of the Cs mode (Ea2 g ) in CsCdBr3 taken from figure 9 in reference

[6]. After scaling the ordinate scale by an arbitrary factor, and adjusting C in equation (3) that

is shifting the pressure abscissae, the fit is obvious. Nevertheless the shape of the full line in

figure 2 may be varied by a sizeable amount to still go through the experimental points and

the apparent quality of the fit in figure 4 may be no more than a coincidence. Thus it is

presented here as a semiquantitative trend, not a precise comparison. For this, obviously, experimental values of the Raman tensor and frequency of the Ba vibrations in MBCO under pressure should be used. Experimental data [21] are available on other modes but not on this

low-frequency [22] (~ 120 cm-1 ) phonon. The barium vibration under scrutiny is the Ba(z) symmetrical stretching mode which will compress the Cu(2) 0(3) planes in the same manner as the Ea’ 29 cesium vibrations compress the ionicovalent chains in CsCdBr3. Before pursuing

the discussion, indirect experimental evidence of the possible evolution of this mode under

Fig. 4.

-

Comparison of the variation under pressure of electron-phonon interaction which would accouent for dTc/dP in MBCO from 2-D BCS (full line) with observed electron-phonon interaction in a

1-D crystal under pressure. Circles : experimental points of figure 9 in reference [6] for Raman intensity

of the E2 g mode of Cs in CsCdBr3 (Ir) vs. pressure. Full line : curve No 3, adjusted in ordinates by a

scaling factor to give the best fit with the experimental points.

(9)

pressure may be found in its variation with y, as regards : i) Raman cross section and

ii) frequency variation.

i) Raman cross section. - Only the Raman intensity of this mode is given in reference [23]

for y

=

0. For y

=

0.75 which is

-

unfortunately

-

tetragonal, it disappears. Thus, the fact that the Ba 118 cm-1 line is indeed not seen in the latter, as expected from the previous

discussion does not give very strong support to it. All that can be said is : it does not contradict it.

ii) Raman frequency variation.

-

Here again the y-dependence has to be used. The phonon density of states from neutron scattering experiments [24] shows a positive shift of the

phonon frequencies, of about 20 % for y decreasing from 1 to 0 in the region of

-

14 meV, at (120 cm-1 ) which corresponds to the w (k) branch of the Ba (z ) mode. Here again, the expected shift would be of - 20 % by reference to the pressure behavior of

E2a g in CsCdBr3 which is the right order of magnitude, but the existence of the tetragonal-->

orthorhombic transition again casts some doubt upon the validity of this comparison.

To conclude this part of the discussion :

i) the increase under pressure of the electron phonon interaction which is required by 2-D

BCS theory to account for the dTc/dP values in MBCO, and for the y-induced overpressure effect on Tc is quantitatively identical to the observed increase under pressure in CsCdBr3 of

the interaction of electrons with the Cs mode which compress the chains normal to the c-axis ; ii) the effect of barium Ag vibrations on the Cu(2) 0(2,3) plane in MBCO could be

analogous to that of Cs atoms on CdBr6 octahedra in compressed CsCdBr3. Both involve motions of rigid filled shells, analogous to those of xenon under the simplifying assumption

that Cs and Ba be fully ionized which, admittedly, is only an approximation. Under high

pressure for CsCdBr3, or for MBa2CU307 (y

=

0), at ambient, these shells are blocked and the motion of the Ba or Cs atoms induces large charge transfer to and from the (CdBr6)

chains in the first case, to and from the CU02 planes in the second ;

iii) indirect indication that this behavior is indeed similar to that of MBCO can be derived from the fact that the Ba mode is absent for y

=

1, and that the frequency shift of this mode between y

=

0 and y

=

1 is that which would be expected for the corresponding equivalent

pressure, but it is not possible to be more specific because of the orthorhombic-tetragonal phase transition which occurs around y - 0.6.

b) COMPARISON WITH OTHER 2-D STRUCTURES. - We noted before, that the Ag mode of

the Ba 2, ion should induce large charge transfer when its outer electronic shells were pushed against the CU02 planes and thus cause large interaction of electrons with this phonon. Now

the eigenvectors pattern of this mode is analogous to the homopolar layer breathing modes

which occur in layered crystals with two sheets per layer, in indium or gallium chalcogenides.

These vibrations alternatively involve symmetrical compression (dilation) of the van der

Waals gap and dilation (compression) of the layers.

An analogous situation occurs in MBCO where, in each layer, two Cu(2) 0(3) sheets are

linked by the Ba2 + and Cu(l) 0(1,4) chains. The interlayer van der Waals gap in GaSe

corresponds to the quasi-empty rare earth planes in MBCO.

In GaSe, a remarkable electron-phonon interaction occurs between the carriers at the energy gap level and this particular phonon. This interaction is large enough to completely

dominate that of all other modes for electrons and holes at the gap energy. This is well documented in a number of papers and for instance, the temperature dependence of the

energy gap [25], or of the exciton linewidth [26] can be entirely explained by the interaction of

charge carriers, only with the layer breathing mode which causes large charge transfer

(10)

between the intra- and interlayer spaces and thus large electron-phonon interaction.

Although there is no direct relation between the band structures of GaSe and MBCO, the

same dominant role must also be played in the latter by the barium Ag mode which must indeed induce symmetrical breathing of the layers.

A second effect of this particular mode can be proposed. In the previous paragraph, we

discussed the oscillatory charge transfer and/or induced dipole of the Ag mode. We will now

show that it might also induce a static local strain in the lattice along the z-axis. It has been noted before [27] that the Ba 2, ions move inside the CuO cages in a double well or symmetry- breaking potential and have large amplitudes. Due to the local asymmetry of the site, the restoring force when Ba moves towards the rigid Cu(2) 0(2,3) planes will be larger than when

it moves in the other direction which is less densely settled. This means that the amplitudes

would be asymmetrical which will be compensated by an average movement of the center of

gravity away from the Cu(l) planes. This is only the classical rectification effect in the response of a non-linear systems to a sine wave. The two Ba atoms in the unit cell will thus on

the average come closer together under the eigenvectors of the Ag phonon. What happens

then to the Cu(l) planes under the motion of this phonon is not clear. On the average they might as well be pushed out into the Y-R.E. gap by the Ba2 + electronic shells, or be pulled in, by the decrease of the Ba-Ba distance. In any case the important point is that the

Ag barium mode decreases the Ba-Ba distance and is thus analogous to hydrostatic pressure in that is squeezes electrons out of the inner part of the layer. This is a general case in molecular

crystals, that is solids where different chemical bond speciés coexist : pressure transfers

charge density from the strongest to the weakest bonds. Thus, as regards charge transfer, this

mode is similar to a static compression, irrespective of its frequency or wave vector. Now in

other 2-D structures, such as GaSe, we have recently shown [7] that high pressure, through charge transfer out of the intralayer space, brings about a very large increase (dell /dP - 1 GPa-1 ) of the component of the static dielectric constant tensor ( Ep ) parallel to

the c-axis. This increase is due to depletion of the intralayer charge density which in the case

of GaSe, spills out into the vdW gap leaving B 1. about constant. In the case of MBCO, this

would mean that the Ba mode propagating - for argument’s sake

-

perpendicular to z would

be accompanied by a static local overpressure and thus a larger value of the component of the dielectric constant parallel to c. This would decrease the Coulomb repulsion for electrons in adjacent layers, with similar x, y coordinates, which interact through ell. This Coulomb

repulsion minimum will of course occur at the same location as the charge density maximum brought about in or close to the Cu(2) planes by expulsion of electrons from the inner part of the layer and both singularities will, of necessity, follow the barium phonon k-vector.

Conclusion.

The last section of the discussion is obviously highly speculative and the hand-waving

arguments presented there should be verified by more quantitative calculations. Nevertheless,

it is interesting, in conclusion, to check a few of the consequences of the proposed scheme against experimental evidence.

i) The proposed mechanisms are specific to the crystal structures of MBCO compounds,

not of La1 _ x (BaSr )xCu204 crystals. The only common point is the succession of La 3+ double

layers with 2-D CuO octahedra. This justifies the fact that they were not compared with the

MBCO’s. They are similar but not identical. Among others, they could not be compared with

the same A(P) scale.

ii) With the present model and reference [17] an increase of 7c from 50 to 90 K through

oxygen concentration variation would correspond (Figs. 2 and 3) to about 15 GPa equivalent

(11)

pressure, whereas by varying y, a compression of the c-axis of less than 1 % is observed for this 7c variation. Even with an isotropic bulk modulus of 200 GPa, this corresponds to only

6 GPa, not 15 GPa. This illustrates what we said at the beginning : oxygen concentration is

important in a small region around the chains where it locally increases the internal

overpressure over the Ba 21 ions but on the whole does not much increase in the Y-Re gap or in the Cu(2) layers where conduction presumably takes place, but not the pressure-dependent coupling mechanism which is proposed here.

iii) We have here drawn an analogy between MBCO and two-dimensional crystals with two

atoms (or molecular subunits) in the layer. The structural analogy was utilized only to discuss

its impact on the Ba Ag mode, and intra- to inter- charge transfer. A variety of other phenomena are predictable of course, in relation to this, in particular on the 0 and Cu vibrations. Among others, the intralayer shear modes should have either a small

dw /dP or even a negative one, through charge depletion. Interestingly enough such a mode

has been observed [21] in YBa2CU307 but not yet explained. It is tempting to assign is to a

Bg mode involving for instance 0(1) which should decrease in frequency with pressure and

possibly increase in intensity because of the Ba2 + ions displacement, which is the reported

behavior [21].

iv) For mathematical simplicity only, the curve of figure 2 was restricted to positive values

at high À 2. Actually, above 90 K it goes to slightly negative values which means that the A 2(P ) curve in figures 3 and 4 decreases slowly above 7c - 90 K. Thus the observed maximum [2] of Te with pressure in MBCO can very easily be reconciled with the present scheme : The pressure-induced charge transfer towards the 0(2) layers will at a given point

start pushing the Fermi level away from the logarithmic maximum of the 2-D density of states,

and thus decrease Tc, as actually observed. Nevertheless, this is a second order effect in the analysis presented here : The largest contributions to the shift of Tc with pressure and oxygen content can be assigned solely to variable electron-phonon interaction.

v) The model used here also shows antiferroelectric order to be a natural consequence of the structure of 2-D perovskites, but this will not be discussed here [28]. For the present, let

us note that for large electron-phonon interaction, the mirror symmetry of the Ag mode

eigenvectors is not compatible with the inversion symmetry of perfect antiferroelectric order.

At most, antiferroelectric fluctuations would be allowed to remain in material with electron-

phonon interaction large enough to lead to superconductivity. Interestingly enough, the same

conclusion has been reached, recently [29], by a different argument, that is by showing the supraconducting and antiferroelectric instabilities to be mutually excluded by symmetry.

Here, it is the interaction mediator (Ag phonon) which breaks antiferromagnetic order. The important point to note is that the ln2 parquet equations used in reference [29] for their 2-D

model, are exactly equivalent to equation 1 for the interaction.

Acknowledgments

This paper heavily relies on the data, references, and discussions of reference [2]. 1 thank

Rinke J. Winjgaarden for early communications of his manuscript which actually was the

basis for this note. It is a pleasure to acknowledge the help of Julien Bok for fruitful

discussions and suggestions on this subject, and of Jacques Friedel for pointing out the shift of

the Fermi level under pressure.

(12)

References

[1] CH C. W., HOR P. H., MENG R. L., AO L. G., HUANG Z. J. and WANG Y. Q., Phys. Rev. Lett. 58 (1987) 405.

[2] WIJNGAARDEN R. J. and GRIESSEN R., High pressure studies in Studies of High Temperature Superconductors, Ed. A. V. Narlikar (Nova Science Publishers Inc 2014 New York) 1989.

[3] LABBE J. and BOK J., Europhys. Lett. 3 (1987) 1225.

[4] LABBE J. and BOK J., Phys. Scr. 37 (1988) 940.

[5] BOK J., Solid State Commun. 67 (1988) 251.

[6] CHERVIN J. C., ANDRAUD C., TERCIER N., BLANZAT B., CAZZANELLI E. and BESSON J. M., Phys. Rev. 38 (1988) 12310.

[7] GAUTHIER M., Thesis, Paris VI (1983) ;

GAUTHIER M. , POLIAN A., BESSON J. M., CHEVY A., High pressure optical properties of GaSe, to

be published in Phys. Rev. B 15-2 (1989).

[8] DIETRICH M. R., FIETZ W. M., ECKE J., OBEST B. and POLITIS C., Z. Phys. B 66 (1987) 283.

[9] KURISA M. , KUMAGAI K. , MAENO Y. and FUJITA T., Physica C 152 (1988) 339.

[10] MURATA K., IHARA H., TOKUMOTO M., HIRABAYASHI M., TERADA N., SENZAKI K. and KIMURA Y., Japn J. Appl. Phys. 26 (1987) L 471.

[11] KAMARAD J., ARNOLD Z. and POLLERT E., Phys. Status Solidi B 144 (1987) K 39.

[12] BORGES H. A., KWOK R., THOMPSON J. D. , WELLS G. L. , SMITH J. L. , FISK Z. and PETERSON D. E., Phys. Rev. B 36 (1987) 2404.

[13] BORGES H. A., WELLS G. L., CHEONG S. W., KWOK R. S., THOMPSON J. D., FISK Z., SMITH J. L. and OSEROFF S. B., Physica 148 B + C (1987) 411.

[14] CHU C. W., HUANG Z. J., MENG R. L. , GAO L. and HOR P. H., Phys. Rev. B 37 (1988) 9730.

[15] YOMO S., MURAYAMA C., UTSUMI W., TAKAHASHI T., YAGI T., MORI N., TAMEGAI T., WATANABE A. and IGE Y., Japn. J. Appl. Phys. 26 (1987) 1107.

[16] MARCUS J., ESCRIBE-FILIPPINI C., REYDER P. L. , BOUJIDA M., DEVENYI J., SCHLENKER C.,

BEILLE J. and GUNDLACH K. M., J. Phys. France 49 (1988) 111.

[17] IHARA H. , OYANAGI H., SUGISE R. , OHNO E. , MAKUBARA T., OHASHI S. , TERADA N., JO M., MIRABAYASHI M., MURATA K., NEGISHI A., KIMURA Y., AKIBA E., HAYAKAMA M. and SHIN S. , Physica C 153-155 (1988) 948.

[18] POLIAN A., BESSON J. M. , GRIMSDITCH M. and VOGT H. , Phys. Rev. B 25 (1982) 2767.

[19] ZISMAN A. N., ALEKSANDROV A. V. and STISHOV S. M., JETP. Lett. 40 (1984) 1029.

[20] POLIAN A. , BESSON J. M., GRIMSDITCH M. and GROSSHANS W. C. , Phys. Rev. B 39 (1989) 1332.

[21] SYASSEN K. , HANFLAND M. , STROESSNER K. , HOLTZ M., KRESS W., CARDONA M., SCHRODER U., PRADE J., KULKARNI A. D. and DE WETTE F. W., Physica C 153-155 (1988) 264.

[22] THOMSEN C., CARDONA M. , GEGENHEIMER B. and LIV R., Physica C 153-155 (1988) 262.

[23] HADJIEV V. G. , ILIEV M. N. and VASSILEV P. G., Physica C 153-155 (1988) 290.

[24] RIETSCHEL M., FINK J. , GERING E. , GOMPF F. , NUECKER N., PINTSCHOvius L., RENKER B., REICHARDT W., SCHMIDT M. and WEBER W., Physica C 153-155 (1988) 1067.

[25] BESSON J. M., Il Nuovo Cimento 38 B (1977) 478 and references therein.

[26] PICCIOLI N., Ph. D. Thesis, Paris (1987).

[27] KELLER J., Physica C 153-155 (1988) 1321.

[28] BESSON J. M., in preparation.

[29] DZYALOSHINSKII I. E. and YAKOVENKO V. M., J. Molec. Electronics 4 (1988) 193.

Références

Documents relatifs

This in- terpretation can be extended to the variation in C deduced for Pb-TI /l/, i.e., we interpret the in- crease in C with the percentage of TI as due to the removal

a result of the change of the EFS connectivity at P = Pc. Solid line is the calculation of g,, on the basis of McClu- re's model with corrections taking into conside-

the strain response.of the Fermi surface (FS) of Therefore the shear response can be calculated from transition metals to homogeneous volume conserving a using zero-pressure for

L’archive ouverte pluridisciplinaire HAL, est destinée au dépôt et à la diffusion de documents scientifiques de niveau recherche, publiés ou non, émanant des

is the nature of the structural phase transition taking place at about 260 K This transition has been detected [I] recently by differential scanning calorimetry (DSC), and

This surprising result has been explained by Engelsberg and Simpson /3/ who showed that the in- fluence of the electron-phonon interaction on the dHvA effect is rather subtle

Since the orbital functions of the spin singlet and the spin triplet states may differ, six parameters are needed to describe the electron- lattice interaction in

High symmetry points in the Brillouin zone allow for an unambiguous identification of the contributions of specific deformabilities to the phonon self-energy in the correspon-