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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�
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.
2014Les 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.
2014Existing 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
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
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
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
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
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.
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.
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
-