The structure of the high temperature superconducting
cuprates has proven to be a complex subject, but
nonetheless rewarding because of the wealth of structural
and physical phenomena which can be observed within
these systems. From the basic components of covalent
CuO
and ionic metal-oxygen planes, a rich and varied
family has been constructed since the first discovery in
1986 of superconductivity in the La
Ba
CuO
system [4]. The challenge to achieve a detailed
understanding of the nature and properties of these cuprate
structures is motivated by a fundamental desire to
understand their, as yet unexplained, superconducting
mechanism, and novel normal state properties. It is further
motivated by the technological need to optimise their
performance for applications, and the continuing possibility of
designing new materials with still higher values of T
.
Although, with their extraordinary properties, they are
usually treated as a class of materials unique to themselves,
the high-T
cuprates can be most effectively considered
as being members, or at least close relations, of a number of
pre-existing groups of materials which are well understood.
Crystallographically, the ideal structures of all the cuprate
systems have much in common with the perovskite ABO
structure type. In this system, a metal atom B sits at the centre of
an oxygen octahedra, and a large metal atom A occupies the
spaces formed when these octahedra link into a corner-sharing
network. A huge array of perovskite-based systems are known,
and have been of special interest for their magnetic and
ferroelectric properties long before the advent of high-T
superconductivity [5]. The systems can all be developed
from the ABO
structure by considering the various possibilities
of stacking the two constituent layers, AO and BO
. The
system A
BO
is, for example, such a combination of
layers with a stacking sequence AO-BO
-AO; with A=La
and B=Cu this is essentially the structure of the cuprate
La
CuO
. Although the basic perovskite structure
is cubic and truly three-dimensional, it is through a combination
of layer stacking, intergrowths, and ordered vacancies, that
the strongly two-dimensional nature of the cuprates derive.
A complete scheme of classification for the cuprates based
upon the perovskite description has been
advanced [6].
Listed in Table 1.1 are some of the most commonly
studied cuprate structural families, along with their respective
stacking sequences, and transition temperatures. In the text that
follows each cuprate system will be identified by its principal cation,
and a particular phase by its layer sequence (so that
YBa
Cu
O
becomes Y-123 for example). There
are many more systems than can be listed here, and comprehensive
structural surveys are available [7,8].
An important factor for superconductivity is the number,
, of adjacent CuO
layers, the value of T
increases
with
up to a maximum for
. In single layer structures
the Cu atoms are octahedrally coordinated, but for
the
layers are formed of Cu-O tetrahedra, with each adjacent layer
separated by an oxygen-deficient layer of an A atom.
It is within these planes of copper oxide that superconductivity
takes place, and it is the mixed valence state of the Cu which
appears to be the crucial factor governing superconductivity
in this. Each of the perovskite A
Cu
O
blocks is separated by
further layers, which can be of a variety of compositions
and structures, but which fulfill the common role of acting
as a charge reservoir for the doping of carriers to the CuO
planes. It is the oxidation of the average Cu valence above 2+
by this mechanism of charge transfer from the AO reservoir
layers which is responsible for the metallic, and ultimately the
superconducting behaviour, of the CuO
layers.
The orderly picture of the cuprates presented by Table
1.1 is only a starting point, for their real structures
are far from those of the crystallographic ideal. In his review
[7], Sleight states the pervasive themes of the
oxide superconductors to be defects, disorder, inhomogeneity
and thermodynamic instability: `It is highly doubtful that
a good understanding of the high-T
superconductors
can be obtained unless we learn to model the inhomogeneities
that abound.'. The inhomogeneities include point defects
due to mixed cation substitutions, oxygen vacancies and
interstitials, as well as extended defects, dislocations, distortions
due to the strain between layers, and twinning as
a response to the relief of strain. In addition, the compositions
given in Table 1.1 are only to be considered as
nominal values; the true stoichiometries are always different
from these, and may vary over a considerable range. These
intrinsic structural complexities are a characteristic of
metastable multi-atom structures, and they are, it would seem,
intimately linked to the exciting novel properties of these
systems. Indeed, if the ideal structures were to be
actualised (and some of the ideal compositions are too
unstable to even prepare) then in the main, they would
result in anti-ferromagnetic insulators. The metallic states
of the real systems, which are essential for superconductivity,
are the result of oxidation or cation doping, and the deliberate
introduction of such defects can be employed to control the
doping of carriers to the CuO
planes, and hence control
the superconducting properties. The intentional application
of defects to increasing the magnetic flux pinning properties
is also a vital means of increasing values of critical current,
a factor so important for technological applications.
Inevitably, the non-ideal crystalline nature presents very
difficult problems for reliable synthesis and characterisation
of samples, and differentiating the effectiveness of specific
defects is likewise problematic. X-ray scattering is now
well established as an essential tool in the determination
of crystal structures, and in the case of diffuse scattering
as a means of observing deviations from the ideal structure
due to both structural fluctuations and defect structures
[9]. The advantages of x-rays for studying
relatively small samples, and the ability to investigate bulk
properties, means the technique can provide an invaluable
complement to the other probes of atomic structure such as
high-resolution electron microscopy (HREM), electron diffraction,
neutron diffraction, EXAFS, positron annihilation, etc. It is certainly an
important tool for characterising the high-T
cuprates,
and it is the aim of this thesis to apply x-ray scattering
techniques to the study of one of the structurally most
involved, and consequently least well understood, of the
cuprates, the system
(or Bi-2212).
The bismuth-based family
is closely related to both thallium
and mercury
families, and
together the n=3
phases of these rank amongst the highest T
values yet achieved;
110K, 128K, and 135K respectively. The charge reservoir AO
layers have a rocksalt-type structure, but in all three systems
they are strongly distorted. In the case of the Bi-systems, the
distortions are so strong that the whole structure is modulated,
and this modulation has long-range order with a well-defined
periodicity which is incommensurate with that of the ideal
structure. Such incommensurate structures are also observed
with only short-range ordering in the Tl-systems. The incommensurate
nature of the structure has compounded greatly the difficulties of
determining the structural characteristics of an already complex
system, and many uncertainties remain. The potential implications
of the incommensurate modulation for the superconducting
properties, perhaps through control of charge transfer has,
for instance, led to much inconclusive debate.
The incommensurate modulation of the Bi-systems
are the most dramatic response to a structural frustration which is
common to all of the cuprates: the mismatch in lattice dimensions
between the covalently bonded perovskite CuO
planes and
the rocksalt-type structure of the charge reservoir layers. Frustration
is a characteristic of all layered structures to some degree and as
such the modulation of the Bi-systems forms part of a wider field
of interest which is associated with the general properties of
incommensurate structures. In this field, the interest is focused on
the mechanisms which drive the incommensurate phenomena, and
the factors which determine amplitudes, wavevectors, and other
characteristics of the modulation.
The aim of the experiments which make up this thesis attempt
to study the structure of Bi-2212 with reference to
its dual properties as both a high-T
cuprate and an
incommensurate structure. As such, Chapter 2 first sets out to place the
cuprate systems in this wider context. It starts by introducing the
general concepts of incommensurate structures with particular
reference to the class of two dimensional layered misfit structures
with which the cuprates are most closely associated, and examples
of systems which share features of relevance are discussed.
The formalism of basic x-ray scattering theory and the extension
necessary for its application to incommensurate systems will
also be set out in this chapter.
In the field of high-T
a tremendous amount of literature
has been published since 1986, and the portions relating to the
structure and properties of Bi-2212 have occupied a considerable
share. The relevant parts of the literature will therefore be reviewed,
where necessary, at the most appropriate points throughout
the thesis. Chapter 3 starts with an extensive review of studies
concerned with determining the structure of Bi-2212, and emphasises
the many still unresolved differences between proposed models,
and the contradictions of some experimental observations. An
attempt to resolve some of these questions, is then described, by
a comparative
study of x-ray scattering measurements obtained from a variety of
Bi-2212 single crystals grown by four different research groups.
The results are successful in clarifying precisely which features are
fundamental to the structure, and which are sample-dependent. Extra
features not accounted for by current models are also identified, and
high-resolution measurements of these show them to be characteristic
of defects in the incommensurate modulation.
In Chapter 4 the properties of the incommensurate modulation are
investigated by studying its temperature response in situ
up to 450
C. The results reveal the invariance of the
incommensurability due to pinning, and the fundamental control
exerted by oxygen diffusion above 300
C is also characterised.
A possible new oxygen-deficient high-temperature phase is
tentatively identified.
The important role of oxygen in the high-T
cuprates is now
beyond doubt, and the experiments in Chapter 5 attempt to
distinguish changes in diffuse scattering associated with changes
in oxygen content or ordering. The specific case of Bi-2212 is
reviewed at the start of this chapter, for which there have been
many investigations of the transport properties as a function of
oxygen content, but remarkably few into the possible associated
changes of microstructure.
The final question relating to the Bi-2212 structure regards the
possible existence of low temperature structural changes which
could be associated with the superconducting transition. There
have been a variety of reports from other structural probes
for evidence of changes in the buckling of the CuO
layers,
and an anomaly in the temperature dependence of the O(apical)
Debye-Waller factor. Chapter 6, therefore, presents the most
detailed x-ray measurements to date made over the temperature
range T=200-10K of the variation in intensity of fundamental and
satellite reflections. It is found that the results follow well the
expected Debye-Waller behaviour, and show no evidence for
any changes in either the period or amplitude of the modulation.
The results thus place an upper limit upon the magnitude, or the
lengthscale, of any possible structural involvement.
The thesis is completed by Chapter 7 which describes the development of a method to simulate the diffuse scattering from a computer model of the Bi-2212 structure, with the aim of aiding the interpretation of the experimental observations from previous chapters. The approach involves large scale numerical calculations of the scattered intensity which are designed to exploit the parallel architecture of a Connection Machine 200. The preliminary results which are presented show the method to be well capable of accommodating the incommensurate features of Bi-2212, and to be suitable for more detailed studies in the future.