Constraints on possible mechanisms for high-Tc superconductivity
This paper discusses a phenomenological model used to describe various properties of a dx²−y² superconductor in its temperature as well as frequency dependence, namely, the London penetration depth, the optical conductivity, the microwave conductivity, and the electronic thermal conductivity. We ass...
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Інститут фізики конденсованих систем НАН України
1998
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Цитувати: | Constraints on possible mechanisms for high-Tc superconductivity / E. Schachinger, I. Schürrer // Condensed Matter Physics. — 1998. — Т. 1, № 1(13). — С. 69-87. — Бібліогр.: 34 назв. — англ. |
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irk-123456789-1186232017-05-31T03:04:20Z Constraints on possible mechanisms for high-Tc superconductivity Schürrer, I. Schachinger, E. This paper discusses a phenomenological model used to describe various properties of a dx²−y² superconductor in its temperature as well as frequency dependence, namely, the London penetration depth, the optical conductivity, the microwave conductivity, and the electronic thermal conductivity. We assume the CuO₂ planes to be the dominant feature for superconductivity and develop a 2D-formalism in which inelastic scattering is modelled explicitly by a spectral density which describes a fluctuation spectrum responsible for the superconducting transition and also for the large inelastic scattering observed in the normal state above the critical temperature Tc . The feedback effect of superconductivity on the spectral density is modelled by a temperature dependent low frequency cutoff. Theoretical results are compared with the experimental data and the fact that such a model allows a consistent description of a variety of phenomena is then used to formulate constraints on possible mechanisms of superconductivity in oxides. Дана стаття розглядає феноменологічну модель, що використовується для опису різноманітних властивостей dx²−y²–надпровідників в залежності як від температури, так і від частоти, а саме глибини проникнення Лондона, оптичної провідності, мікрохвильової провідності та електронної термічної провідності. Ми вважаємо, що саме площини CuO₂ є основним чинником для виникнення надпровідності, і тому розвиваємо двомірний формалізм, в якому процеси непружного розсіяння моделюються точно через спектральну густину, що описує флуктуаційний спектр, який є відповідальним за виникнення надпровідного переходу, а також за велике непружне розсіяння, що спостерігається в нормальному стані вище критичної температури Tc . Зворотній вплив надпровідності на спектральну густину моделюється температурнозалежним низькочастотним обрізанням. Теоретичні результати порівнюються з експериментальними даними і, виходячи з того, що дана модель дає змогу зробити послідовний опис цілого ряду явищ, формулюються обмеження на можливі механізми виникнення надпровідності в оксидах. 1998 Article Constraints on possible mechanisms for high-Tc superconductivity / E. Schachinger, I. Schürrer // Condensed Matter Physics. — 1998. — Т. 1, № 1(13). — С. 69-87. — Бібліогр.: 34 назв. — англ. 1607-324X PACS: 74.20.Fg, 74.25.Nf, 74.72.-h DOI:10.5488/CMP.1.1.69 http://dspace.nbuv.gov.ua/handle/123456789/118623 en Condensed Matter Physics Інститут фізики конденсованих систем НАН України |
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English |
description |
This paper discusses a phenomenological model used to describe various properties of a dx²−y² superconductor in its temperature as well as frequency dependence, namely, the London penetration depth, the optical conductivity, the microwave conductivity, and the electronic thermal conductivity. We assume the CuO₂ planes to be the dominant feature for superconductivity and develop a 2D-formalism in which inelastic scattering is modelled explicitly by a spectral density which describes a fluctuation spectrum responsible for the superconducting transition and also for the large inelastic scattering observed in the normal state above the critical temperature Tc . The feedback effect of superconductivity on the spectral density is modelled by a temperature dependent low frequency cutoff. Theoretical results are compared with the experimental data and the fact that such a model allows a consistent description of a variety of phenomena is then used to formulate constraints on possible mechanisms of superconductivity in oxides. |
format |
Article |
author |
Schürrer, I. Schachinger, E. |
spellingShingle |
Schürrer, I. Schachinger, E. Constraints on possible mechanisms for high-Tc superconductivity Condensed Matter Physics |
author_facet |
Schürrer, I. Schachinger, E. |
author_sort |
Schürrer, I. |
title |
Constraints on possible mechanisms for high-Tc superconductivity |
title_short |
Constraints on possible mechanisms for high-Tc superconductivity |
title_full |
Constraints on possible mechanisms for high-Tc superconductivity |
title_fullStr |
Constraints on possible mechanisms for high-Tc superconductivity |
title_full_unstemmed |
Constraints on possible mechanisms for high-Tc superconductivity |
title_sort |
constraints on possible mechanisms for high-tc superconductivity |
publisher |
Інститут фізики конденсованих систем НАН України |
publishDate |
1998 |
url |
http://dspace.nbuv.gov.ua/handle/123456789/118623 |
citation_txt |
Constraints on possible mechanisms for high-Tc superconductivity / E. Schachinger, I. Schürrer // Condensed Matter Physics. — 1998. — Т. 1, № 1(13). — С. 69-87. — Бібліогр.: 34 назв. — англ. |
series |
Condensed Matter Physics |
work_keys_str_mv |
AT schurreri constraintsonpossiblemechanismsforhightcsuperconductivity AT schachingere constraintsonpossiblemechanismsforhightcsuperconductivity |
first_indexed |
2025-07-08T14:20:21Z |
last_indexed |
2025-07-08T14:20:21Z |
_version_ |
1837088819079282688 |
fulltext |
Condensed Matter Physics, 1998, Vol. 1, No 1(13), p. 69–87
Constraints on possible mechanisms
for high-T csuperconductivity
E.Schachinger, I.Schürrer
Institut für Theoretische Physik, Technische Universität Graz,
Petersgasse 16, A-8010 Graz, Austria
Received March 23, 1998
This paper discusses a phenomenological model used to describe vari-
ous properties of a dx2
−y2 superconductor in its temperature as well as
frequency dependence, namely, the London penetration depth, the optical
conductivity, the microwave conductivity, and the electronic thermal con-
ductivity. We assume the CuO 2 planes to be the dominant feature for su-
perconductivity and develop a 2D-formalism in which inelastic scattering is
modelled explicitly by a spectral density which describes a fluctuation spec-
trum responsible for the superconducting transition and also for the large
inelastic scattering observed in the normal state above the critical temper-
ature Tc . The feedback effect of superconductivity on the spectral density
is modelled by a temperature dependent low frequency cutoff. Theoretical
results are compared with the experimental data and the fact that such a
model allows a consistent description of a variety of phenomena is then
used to formulate constraints on possible mechanisms of superconductiv-
ity in oxides.
Key words: high- Tc superconductivity, London penetration depth, optical
conductivity, electronic thermal conductivity
PACS: 74.20.Fg, 74.25.Nf, 74.72.-h
1. Introduction
Since the discovery of high-Tc superconductivity in oxide materials by Bednorz
and Müller [1] huge efforts have been made to find a theoretical description of the
pairing mechanism which leads to critical temperatures of the order of 100 K. Nev-
ertheless, it is only recently that a consistent set of experiments performed on high
quality twinned and untwinned single crystals of optimally doped YBa2Cu3O6.95
(YBCO) seem to have resolved the symmetry of the superconducting order param-
eter to be predominantly of the dx2
−y2 symmetry with nodes crossing the Fermi
surface. Most important is the observation of the linear temperature dependence
of the London penetration depth at low temperatures [2] which was discussed ear-
lier by Annett et al. [3]. Such a linear dependence at low temperatures has also
c© E.Schachinger, I.Schürrer 69
E.Schachinger, I.Schürrer
been reported for the spin susceptibility [4]. More evidence was supplied by the
discovery of the existence of the so-called unitary limit in the electronic thermal
conductivity of YBCO single crystals doped with Zn [5], and the c-axis Josephson
tunnelling experiments where the conventional superconductor (Pb) is deposited
across a single twin boundary [6]. This experiment also offers a direct evidence for
a subdominant s-symmetric contribution to the order parameter which is typical
of orthorhombic systems [7].
Modifications in the low-temperature linear dependence of the penetration
depth brought about by the impurity scattering [8] are also naturally understood
from theoretical models with the order parameter having d-wave symmetry [9,10].
Such models, however, tend to predict slopes for the penetration depth near the
critical temperature which are not as steep as those observed. This is true even if
inelastic scattering is incorporated in the calculations through the Eliashberg-type
formalism which represents a first approximate attempt of including self-energy
effects [11].
Another set of experiments which can be used to put constraints on possible
mechanisms of high Tc superconductivity are microwave conductivity measure-
ments as a function of temperature in pure single crystals of optimally doped
YBCO [12,13] which have revealed the existence of a very large peak around 40 K,
whose size and position depend somewhat on the microwave frequency used. A
similar peak can be found in the electronic thermal conductivity, though at much
lower temperatures [14]. This peak in the microwave conductivity has been widely
interpreted to be due to the rapid reduction in the inelastic scattering below Tc and
is generally referred to as the collapse of the low-temperature inelastic scattering
rate. One possible way to describe this experimental result is the introduction of a
temperature dependent inelastic scattering time which can be modelled from the
spin fluctuation theory [15].
Schachinger et al. [16–18] proposed quite a different explanation which not only
allowed a satisfying analysis of the microwave conductivity peak but also described
the temperature dependence of the London penetration depth and of the electronic
thermal conductivity consistently. Their phenomenological model is based first
of all on the observation that a mechanism responsible for superconductivity in
oxides, which also leads to d-wave superconductivity, is most likely to be electronic
in origin. In such a model the collapse of the inelastic scattering rate which causes
a large peak in the microwave conductivity is explained by a gap which opens up in
the fluctuation spectrum responsible for superconductivity [19–21]. Such an effect
is generic to all electronic mechanisms where the fluctuation spectrum causing
superconductivity belongs to the superconducting quasiparticle system itself and
becomes gapped as superconductivity sets in.
The phenomenological model consists in the application of a temperature de-
pendent low frequency cutoff to the fluctuation spectrum to give the correct tem-
perature dependence of the London penetration depth of clean, optimally doped
YBCO single crystals. (It is interesting to note that the temperature dependence
of the low frequency cutoff follows quite closely the temperature dependence of
70
Constraints on HTCS mechanisms
the superconducting gap.) This model is then used (within the framework of
the Eliashberg-type formalism adjusted to allow for d-wave superconductivity)
to calculate optical conductivity, microwave conductivity, and electronic thermal
conductivity of clean superconductors and superconducting systems which also
contain moderate concentrations of impurities.
It is the purpose of this paper to review the recent results and to expand the
application of the model to the calculation of the optical conductivity of a dx2
−y2
superconductor in its normal as well as superconducting state. Section 2 specifies
the basic Eliashberg-like equations and the formulae used to calculate the London
penetration depth, optical conductivity, optical reflectivity, and electronic thermal
conductivity. In Section 3 the results are discussed and, finally, Section 4 presents
our conclusions.
2. Formalism
The simplest description of a d-wave superconductor is obtained within the
BCS formalism assuming a separable model for the pairing interaction. In such a
model the pairing potential depends on the product cos(2θ) cos(2θ′) where θ and
θ′ are the directions of the initial and final momenta on a two-dimensional circular
Fermi surface. To include the dynamics of the fluctuations that are exchanged in
the pairing it is necessary to go beyond the BCS and consider self-energy correc-
tions. We restrict ourselves to the Eliashberg-type formalism which was discussed
by Schachinger and Carbotte [22] and offers at least a first order approximation to
the full self-energy corrections. Such a formalism includes a Bose-exchange spec-
tral density I2F (Ω) which enters both the gap channel for the pairing energy
∆̃(iωn) and the channel for the renormalized Matsubara frequencies ω̃(iωn). This
last quantity exists in the normal state and carries information on the s-wave
part of the interaction. From symmetry considerations, the gap channel involves
the d-wave part of the interaction. In principle, these two projections of the full
boson-exchange interaction need not involve the same weighting of the Bose en-
ergies. In the absence of detailed information on the mechanism we will assume,
for simplicity, that a single I2F (Ω) can, nevertheless, be employed as a first ap-
proximation but with a different weight g in the gap channel as compared to the
renormalization channel. The two nonlinear self-energy equations for ω̃(iωn) and
∆̃(iωn), with iωn = iπT (2n + 1), n = 0,±1,±2, . . ., and temperature T will then
have the following form in the imaginary axis notation [22]:
ω̃(iωn) = ωn + πT
∑
m
λ(m− n)Ω(iωm) + πΓ+
Ω(iωn)
c2 + Ω2(iωn) +D2(iωn)
(1)
∆̃(iωn, θ) = gπT
∑
m
√
2 cos(2θ)λ(m− n)D(iωm) (2)
with Ω(iωn) =
〈
ω̃(iωn)
√
ω̃2(iωn) + ∆̃2(iωn, θ)
〉
θ
(3)
71
E.Schachinger, I.Schürrer
D(iωn) =
〈 √
2 cos(2θ)∆̃(iωn, θ)
√
ω̃2(iωn) + ∆̃2(iωn, θ)
〉
θ
, (4)
and
λ(m− n) = 2
∞
∫
0
d Ω
ΩI2F (Ω)
Ω2 + (ωm + ωn)2
. (5)
Here 〈· · ·〉θ denotes the average over the angle θ, Γ+ = nI/(N(0)π2) with nI being
the concentration of isotropically scattering impurities, N(0) is the normal state
quasiparticle density of states at the Fermi energy, c = cot δ0, and δ0 is the T-matrix
phase shift. For very large values of c (c→ ∞) we are in the Born scattering limit
and for c = 0 in the so-called unitary (resonant) scattering limit. In the weak
scattering (Born) limit the impurity term in equation (1) reduces to πt+Ω(iωn)
with c absorbed into t+ = nIN(0)|V (kF )|2, where V (kF ) is the impurity scattering
potential evaluated at the Fermi momentum kF .
The London penetration depth λL(T ) at any temperature T < Tc follows from
the solution of equations (1) and (2) and is given, within a numerical constant, by
[10]:
1
λ2L(T )
∝ πT
〈
∑
m
∆̃2(iω, θ)
[
ω̃2(iωn) + ∆̃2(iωn, θ)
]3/2
〉
θ
. (6)
The optical conductivity σ(ν) at any temperature T and photon frequency ν is
given by [23,24]:
σ(ν) =
i
ν
e2N(0)v2F
2
×
〈 ∞
∫
0
d Ω tanh
(
Ω
2T
)
1−N(Ω, θ)N(Ω + ν, θ)− P (Ω, θ)P (Ω + ν, θ)
E(Ω, θ) + E(Ω + ν, θ)
+
∞
∫
0
d Ω tanh
(
Ω+ ν
2T
)
1−N(Ω, θ)⋆N(Ω + ν, θ)⋆ − P (Ω, θ)⋆P (Ω + ν, θ)⋆
E(Ω, θ)⋆ +E(Ω + ν, θ)⋆
+
∞
∫
0
d Ω
[
tanh
(
Ω+ ν
2T
)
− tanh
(
Ω
2T
)]
×1 +N(Ω, θ)⋆N(Ω + ν, θ) + P (Ω, θ)⋆P (Ω + ν, θ)
E(Ω + ν, θ)− E(Ω, θ)⋆
+
0
∫
−ν
dΩ tanh
(
Ω+ ν
2T
){
1−N(Ω, θ)⋆N(Ω + ν, θ)⋆ − P (Ω, θ)⋆P (Ω + ν, θ)⋆
E(Ω, θ)⋆ +E(Ω + ν, θ)⋆
+
1 +N(Ω, θ)⋆N(Ω + ν, θ) + P (Ω, θ)⋆P (Ω + ν, θ)
E(Ω + ν, θ)− E(Ω, θ)⋆
}〉
θ
, (7)
72
Constraints on HTCS mechanisms
where the star symbolizes a complex conjugate, e is a charge on the electron, and
vF is the Fermi velocity. Furthermore,
E(ν, θ) =
√
ω̃2(ν)− ∆̃2(ν, θ), (8)
N(ν, θ) =
ω̃(ν)
E(ν, θ)
, (9)
P (ν, θ) =
∆̃(ν, θ)
E(ν, θ)
. (10)
In the normal state equation (7) can be replaced by [23]:
σ(ν) =
ω2
p
4π
1
iν
0
∫
−∞
d Ω tanh
(
ν + Ω
2T
)
S−1(T, ν,Ω)
+
∞
∫
0
d Ω
[
tanh
(
ν + Ω
2T
)
− tanh
(
Ω
2T
)]
S−1(T, ν,Ω)
, (11)
with ωp – the plasma frequency,
S(T, ν,Ω) = ν + Σ(T, ν + Ω)⋆ − Σ(T,Ω)− iπt+, (12)
and
Σ(T, ω) = −
∫
d z I2F (z)
[
ψ
(
1
2
+ i
ω + z
2πT
)
− ψ
(
1
2
+ i
ω − z
2πT
)]
. (13)
Here ψ(z) is a digamma function of complex argument z.
Once the real (σ1(ν)) and imaginary (σ2(ν)) parts of the conductivity are
known, the optical reflectivity R(ν) can easily be calculated using
R(ν) =
∣
∣
∣
∣
∣
1−
√
ε(ν)
1 +
√
ε(ν)
∣
∣
∣
∣
∣
2
, (14)
with the dielectric function ε(ν) defined as
ε(ν) = ε0 +
4π
ν
iσ(ν), (15)
where ε0 describes the response of quasiparticles in completely filled bands.
Using the above notation we find for the electronic thermal conductivity [25]:
κab,e(T ) =
2N(0)v2F
T 2
∞
∫
0
d ν ν2
cosh2(ν/2T )
×
〈
1 +N2
1 (ν; θ) +N2
2 (ν; θ)− P 2
1 (ν; θ)− P 2
2 (ν; θ)
E2(ν; θ)
〉
θ
. (16)
73
E.Schachinger, I.Schürrer
where indices 1 and 2 refer to the real and imaginary parts, respectively. equations
(7) to (16) require the renormalized gap function ∆̃(ν) and the renormalized fre-
quencies ω̃(ν) on the real axis. These can be found by the analytical continuation
of the results of equations (1) and (2) from the imaginary axis to the real one
employing the method developed by Marsiglio et al. [26].
Most of the parameters of the model have now been specified except for g, the
d- to s-anisotropy of the exchange potential and for the form of the boson-exchange
spectral density I2F (Ω) which describes the fluctuation spectrum. Many choices
could be made for this latter quantity. If we knew the actual mechanism which
leads to pairing in oxides, there would be no choice at all as we would know the
microscopic origin. In the absence of such information we adopt a very simple form
which can be regarded as one guided by the nearly antiferromagnetic Fermi liquid
model [27,28]. We use
I2F (Ω) = I2
Ω/ωsf
1 + (Ω/ωsf)
2
(17)
up to to some convenient high frequency cutoff for the numerical work (400 meV
here). The frequency ωsf sets the energy scale of the fluctuation spectrum and is
not arbitrary because our numerical work has to reflect the observation that above
the critical temperature the inelastic scattering rate is of the order of several times
Tc in value. This requires ωsf = 30 meV and I2 is adjusted to give a clean limit
critical temperature Tc0 = 100 K in solving the linearized equations (1) and (2)
[16]. This results in the strong coupling parameter Tc0/ωlog = 0.31 where ωlog is
defined in the usual way [29]
ωlog = exp
{
2
λ
∫
d Ω
I2F (Ω)
Ω
lnΩ
}
, (18)
and represents the average boson energy in the system. The only parameter left is
g and it has already been shown that the results do not depend qualitatively on
the choice of g [16] and we set g = 0.8 to be definite.
3. Results
3.1. Optical conductivity, normal state
It is the aim of this short subsection to verify the parameters introduced pre-
viously to make the fluctuation spectrum (17) definite, namely, ωsf , and the high
frequency cutoff, by comparing the theoretically obtained normal state conduc-
tivity, equation (11), with the experiment. Figure 1 presents the results of such a
comparison. What is shown here is the real part of the optical conductivity σ1(ν)
(figure 1a) and the inverse of the in-plane optical scattering time
1
τab(ν)
=
ωp
4π
ℜe
[
1
σ(ν)
]
(19)
as a function of frequency ν. The data points are for a clean, twinned, optimally
74
Constraints on HTCS mechanisms
0 200 400 600 800 1000 1200
0
1000
2000
3000
4000
5000
6000
7000
8000
9000
10000
a)
theor. exp. clean
theor. exp. 0.75% Ni
theor. exp. 1.4% Ni
σ 1(
ν)
(
Ω
-1
cm
-1
)
ν (cm-1)
*
0 200 400 600 800 1000 1200 1400 1600
0
200
400
600
800
1000
b)
theor. exp. clean
theor. exp. 0.75% Ni
theor. exp. 1.4% Ni
1/
τ ab
( ν
)
(c
m
-1
)
ν (cm-1)
Figure 1. a) The real part of the normal state optical conductivity σ1(ν) and
b) the inverse optical scattering time 1/τab(ν) as a function of frequency ν. The
data points represent experimental data reported by Homes et al. [30] for a clean,
twinned, optimally doped YBCO single crystal (solid squares), for a similar sam-
ple with 0.75% Ni substitution (solid triangles), and for a sample with 1.4% Ni
(solid down-triangles). Theoretical results obtained from equation (11) are shown
for the clean sample (solid line), the sample with 0.75% Ni (dashed line), and for
the sample with 1.4% Ni (dotted line). The arrows indicate the data points used
to scale theory to experiment. The temperature is 100 K.
doped YBCO single crystal (Tc = 93.2K, solid squares), a similar sample with
0.75% Ni substituted at Cu-sites (Tc = 91K, solid triangles), and a sample with
1.4% Ni substitution (Tc = 89K, solid down-triangles). The normal state conduc-
tivity data have been obtained at a sample temperature of 100 K in all the cases.
Theoretical results are presented for the clean sample (solid line), the sample with
0.75% Ni (dashed line), and the sample with 1.4% Ni (dotted line). The Ni con-
tent was simulated by the value for t+ necessary to decrease the clean sample’s
critical temperature to the required value. The arrows indicate the data points
used to scale theory to experiment. This scaling was necessary as the theoretical
results are on an arbitrary scale because of the factor ωp/4π which was left out
in evaluating equation (11). Theoretically such a scaling should not be necessary
for the inverse scattering time because, according to equation (19), the theoretical
values are free of this material parameter. Nevertheless, Homes et al. [30] point
75
E.Schachinger, I.Schürrer
out in their paper that they were using a value of ωp = 1.6 eV which is somewhat
ambiguous because it depends on the frequency cutoff used in the evaluation of
the experimental data.
The agreement between theory and experiment is excellent for the clean and
the 0.7% Ni sample over the whole frequency range covered by the experiment. We
note some deviations for the 1.4% Ni sample at low frequencies and above 1200
wave numbers. But it is quite obvious that this data set escapes the general trend
established by the other two samples.
We conclude that the simple model fluctuation spectrum (17) with ωsf =
30meV and a high frequency cutoff of 400 meV allow an excellent description
of the frequency dependence of the normal state optical conductivity and thus,
establishes a valid basis for further investigations into the superconducting state.
3.2. In-plane London penetration depth
Our results for the temperature dependence of the in-plane London penetration
depth given on evaluation of equation (6) which requires only the solutions of the
self-energy equations (1) and (2) on the imaginary axis are displayed in figure 2.
What is presented is the inverse square of the normalized in-plane penetration
0.0 0.2 0.4 0.6 0.8 1.0
0.0
0.2
0.4
0.6
0.8
1.0
Experiment
d-wave, ω
c
= 0
d-wave, ω
c
= 2.1 T
c0
s-wave
[ λ
L(
0)
/ λ
L(
t)
]2
t = T/T
c
Figure 2. The inverse square of the normalized in-plane London penetration
depth [λL(0)/λL(t)]
2 as a function of the reduced temperature t = T/Tc. The solid
curve is for a dx2
−y2 superconductor and without a low frequency cutoff in the
fluctuation spectrum. The dashed curve is for a low frequency cutoff ωc = 2.1Tc
in the fluctuation spectrum. The solid squares indicate the data by Bonn et al.
[31]. Finally, the dotted line gives the results one would get for a classical s-wave
superconductor like Pb.
76
Constraints on HTCS mechanisms
depth [λL(0)/λL(t)]
2 as a function of the reduced temperature t = T/Tc. The ex-
perimental data by Bonn et al. [31] are indicated by solid squares. It is obvious
from the figure that these data cannot be described by an s-wave superconductor
(dotted line). On the other hand, the low temperature results for a dx2
−y2 super-
conductor (solid line) seem to agree rather well with the experiment in the region
0 6 t 6 0.2 but for t > 0.2 very pronounced deviations are noted. In particular,
as in the previous work [11], the slope of the penetration depth near Tc is not so
steep as compared with the experiment.
0 100 200 300 400
0.0
0.1
0.2
0.3
0.4
0.5
0.6
0.7
T/T
c
= 1
T/T
c
= 0.9
T/T
c
= 0.8
T/T
c
= 0.7
I2 F
( Ω
)
Ω (meV)
0 10 20 30 40
0.0
0.2
0.4
0.6
Ω (meV)
I2 F
( Ω
)
Figure 3. The fluctuation spectrum I2F (Ω) according to equation (17). We
present spectra for four different temperatures, namely, T/Tc = 1 (dotted line),
T/Tc = 0.9 (dashed line), T/Tc = 0.8 (dash-dotted line), and T/Tc = 0.7 (solid
line). At T/Tc = 0.7 the full low frequency cutoff ωc = 2.1Tc is in effect. The
insert shows the low frequency part of the fluctuation spectrum on an extended
frequency scale.
In order to develop a theoretical model able to remove this discrepancy be-
tween theoretical predictions and the experiment we recall the result well known
from functional derivative methods and applied to conventional anisotropic s-wave
superconductors, namely, that very low frequency phonons have the same effect
as static impurities and reduce Tc, i.e., they are pair breaking [32]. Similar con-
siderations apply to a d-wave superconductor in which case it has been shown
that the functional derivative of Tc with the fluctuation spectral density is nega-
tive at low frequencies [33]. If, at low temperatures, such low-energy excitations
are removed because of the feedback effect superconductivity has on the fluctua-
tion spectrum, one would expect that the superconducting gap itself will be larger
than it would otherwise be for the associated value of Tc. With the increase of
77
E.Schachinger, I.Schürrer
temperature the amount of pair breaking increases, because the low frequency
part of the fluctuation spectrum is restored as the superconducting gap closes up.
This should affect the temperature dependence of the penetration depth. In fact,
the experimental data of Bonn et al. [31] can be used to model the temperature
dependence of such a low frequency cutoff to make the theoretical results follow
quantitatively the experiment. If we apply a low frequency cutoff ωc = 2.1Tc0 at
t = 0 to the fluctuation spectrum and model the temperature dependence of ωc
closely to that of the superconducting gap, we achieve, after minor adjustments,
optimal agreement between theory and experiment (dashed line, figure 2). This
fluctuation spectrum, which will also be used in all further calculations, is pre-
sented in figure 3 where the temperature dependence of the low frequency cutoff
is emphasized in the insert which shows the low frequency part of the fluctua-
tion spectrum on an extended frequency scale for various reduced temperatures.
Obviously, what pushes up [λL(0)/λL(t)]
2 at intermediate temperatures and, cor-
respondingly, increases the slope near Tc, is the pair breaking effect associated with
the introduction of lower frequency fluctuations as T increases towards Tc.
3.3. Microwave conductivity
In discussing the microwave conductivity we concentrate on the case ν =
34.8GHz ≃ 0.144meV studied by Bonn et al. [12] using a clean, twinned, and opti-
mally doped YBCO single crystal. It has already been pointed out by Schachinger
et al. [16,17] that the peak in the microwave conductivity of a dx2
−y2 supercon-
ductor falls too low in temperature and is not large enough to agree with the
experiment if equations (1) and (2) are solved in a clean limit employing an un-
modified fluctuation spectrum (17) before equation (15) is solved to calculate opti-
cal conductivity. But applying a low frequency cutoff to (17) according to figure 3
moves the microwave peak towards higher temperatures and increases its mag-
nitude considerably bringing the theoretical predictions into better but still not
satisfying agreement with the experiment.
Adding impurity scattering in the Born approximation affects the size and
width of the microwave peak with the position of the peak in temperature re-
maining relatively unchanged. If, instead, the impurity scattering is treated in the
unitary limit, the attenuation of the microwave peak is much more pronounced
and shifts to higher temperatures [17]. While in the best untwinned single crystal
samples of YBCO the residual scattering is believed to be rather small, we have
to assume for twinned crystals some residual scattering which can be modelled by
adding some Born limit impurity scattering to achieve the best possible agreement
between theory and experiment. Figure 4 shows the result of such a fitting process
in which the impurity parameter t+ = 0.822meV has been chosen which reduces
the clean limit critical temperature by 5 K to Tc = 95K. (The solid squares in
figure 4 correspond to the experimental data reported by Bonn et al. [12] and
the solid curve gives our best theoretical result.) The scale in our theoretical data
is arbitrary and was fitted to agree with the data at the temperature indicated
by the arrow. For comparison we also show in figure 4 the theoretical result one
78
Constraints on HTCS mechanisms
would get if the system’s critical temperature were lowered to 95 K by adding
the resonant impurity scattering (the dotted line). While for the Born scattering
excellent agreement is obtained, the unitary impurity scattering results certainly
provide an unacceptable description of the data.
0.0 0.2 0.4 0.6 0.8 1.0
0
2
4
6
8
10
12
T
c
= 95 K, Born scattering
T
c
= 95 K, resonant scattering
Bonn et al., clean sample
σ 1(
ν
=
0
.1
44
m
eV
)
(1
016
s
-1
)
T/T
c
Figure 4. The real part of the microwave conductivity, σ1, for the frequency
ν = 34.6GHz ≃ 0.144meV as a function of the reduced temperature T/Tc. The
solid line represents the theoretical results for a model system having Tc of 95 K as
a result of the additional Born impurity scattering. The dotted line corresponds to
a model system with the additional resonant impurity scattering having the same
Tc as the former system. In both systems a low frequency cutoff of ωc = 2.1Tc
at zero temperature has been applied to the fluctuation spectrum I2F (Ω). The
solid squares correspond to experimental data reported by Bonn et al. [8] for a
clean, twinned, optimally doped YBCO single crystal. The arrow indicates the
data point which has been used to scale theory to experiment.
This establishes the theoretical equivalent of a clean and twinned YBCO single
crystal and completely defines the phenomenological model by the temperature
dependence of the low-frequency cutoff in the fluctuation spectrum responsible
for superconductivity and by a certain amount of the Born impurity scattering to
compensate for the residual scattering in a clean, twinned sample. If this model
is to be used to define additional constraints on possible theoretical explanations
of high Tc superconductivity, predictions of this model are to be compared with
other properties of clean and twinned YBCO single crystals which do not need
additional theoretical parameters and do not depend linearly on the properties
investigated so far.
79
E.Schachinger, I.Schürrer
3.4. Electronic thermal conductivity
A candidate, for which experimental data are readily available, is the electronic
thermal conductivity. While the normal state electronic thermal conductivity is lin-
early related to the d.c. conductivity (ν = 0) via the Wiedemann-Franz law, there
is certainly no linear relation between the microwave conductivity (ν 6= 0) and the
electronic thermal conductivity, as a close inspection of equations (7) or (15) and
(16) reveals immediately. It has already been pointed out in the introduction that
the in-plane electronic thermal conductivity, κab,e(T ), of clean, twinned YBCO sin-
gle crystals develops a very pronounced low temperature peak in its temperature
dependence. This feature can now be used to check on the consistency of the model
developed so far.
0.0 0.2 0.4 0.6 0.8 1.0
0
20
40
60
80
100
120
140
ω
c
/T
c0
= 0, T
c
= 95K
ω
c
/T
c0
= 2.1, T
c
= 95K
Matsukawa et al., YBCO Sample No. 3
κ ab
,e
(
m
W
/c
m
K
)
T/T
c
Figure 5. The in-plane electronic thermal conductivity κab,e(T ) in units of
mW/cm K as a function of the reduced temperature T/Tc. The solid curve is
the result of model calculations using a temperature dependent low frequency
cutoff in the fluctuation spectrum. The solid squares are the data of Matsukawa
et al. [14] and seem to agree well with theory. The scale of the theoretical κab,e(T )
was adjusted to fit the point indicated by the arrow. The dotted line is a theo-
retical calculation without a low frequency cutoff on the fluctuation spectrum. It
disagrees strongly with the data.
Schachinger and Carbotte [18] demonstrated in an extensive study that κab,e(T )
does not show in the clean limit of equations (1) and (2) a very pronounced peak
around t = 0.15 if the unmodified fluctuation spectrum (17) is applied. This peak
is then enhanced by at least one order of magnitude if the temperature dependent
low frequency cutoff of the fluctuation spectrum is included. No significant shift
80
Constraints on HTCS mechanisms
of the peak in temperature occurs. Adding impurities attenuates the peak and it
becomes shifted towards higher temperatures. In this, again, the Born impurity
scattering is less effective than resonant scattering impurities.
Without the introduction of any new parameters, the theoretical results of
calculations within the phenomenological model are scaled to meet the in-plane
electronic thermal conductivity measured by Matsukawa et al. [14], as shown in fig-
ure 5 (the solid line). (This scaling is still necessary because in order to set the scale
theoretically the value N(0)v2F of equation (16) is needed but it is not known. Thus,
a fit to one data point, indicated by the arrow in figure 5, is essential.) Without
the low frequency cutoff the dashed curve is obtained which shows no agreement
with the experiment at all. Thus, the in-plane electronic thermal conductivity is
an equally sensitive probe of the feedback effect which superconductivity has on
the fluctuation spectrum.
3.5. Microwave conductivity in systems with impurities
After the phenomenological model has been defined and verified against the in-
plane electronic thermal conductivity, it is certainly of some interest to test it even
further using experimental results reported by Bonn et al. [8] for the microwave
conductivity of twinned YBCO single crystals which have been doped with small
concentrations of Zn and Ni. In particular, one sample with 0.3% Zn substitution
at the Cu-sites showed a critical temperature of 89.5 K (about 4 K down from
the clean sample’s Tc) and the other sample with 0.71% Ni substitution had Tc of
90.47 K (about 3 K down). This alone establishes Zn as a more powerful dopant.
The experiments also revealed that both types of impurities had about the same
effect on the peak in the microwave conductivity (a substantial reduction to less
than half the height of the clean sample and only a little shift towards higher
temperatures). On the other hand, the in-plane penetration depth followed a T 2
law in its low temperature dependence in the Zn doped sample (typical of the
resonant impurity scattering) while the Ni doped sample developed a linear low
temperature dependence which is typical of the Born scattering [3,10]. This is the
reason why Ni impurities have been regarded to be of the Born type.
The experimental situation can be simulated theoretically by either increasing
t+ beyond its clean sample value of 0.822 meV until the observed decrease in Tc by
about 3.5 K on the average is achieved or by adding nonzero values of Γ+ to de-
scribe additional resonant scattering impurities. It was pointed out by Schachinger
and Carbotte [17] that only resonant scattering impurities have the observed ef-
fect on the peak of the microwave conductivity. As Ni does not show the required
T 2 law in the low temperature variation of the in-plane penetration depth, these
authors concluded that Ni impurities must be at least of intermediate scattering
strength and setting c = 0.5 in equation (1) results in excellent agreement between
the experimental and theoretical microwave conductivity data even for Ni doped
YBCO. This is demonstrated in figure 6a. Schachinger and Carbotte [17] were also
able to prove that the T 2 to T law crossover in the low temperature variation of
the in-plane penetration depth occurs in the region 0.3 < c < 0.4 and this explains
81
E.Schachinger, I.Schürrer
why the theoretical predictions for the low temperature variation of the in-plane
penetration depth agree so well with the experiment, as it is shown in figure 6b.
0.0 0.2 0.4 0.6 0.8 1.0
1
2
3
4
5
a)
ω
c
/T
c0
= 2.1 res. scattering, c = 0
ω
c
/T
c0
= 2.1, res. scattering, c = 0.5
Bonn et al. 0.31% Zn
Bonn et al. 0.75% Ni
σ 1(
ν
=
0
.1
44
m
eV
)
(1
016
s
-1
)
T/T
c
0.0 0.1 0.2 0.3
0
20
40
60
80
100
120
b)
ω
c
/T
c0
= 2.1, res. scattering, c = 0
Bonn et al., YBCO+0.31% Zn
ω
c
/T
c0
= 2.1 res. scattering, c = 0.5
Bonn et al., YBCO+0.75% Ni
λ L(
T
)
-
λ L(
1.
3
K
)
(Å
)
T/T
c
Figure 6. a) The real part of the microwave conductivity, σ1, for the frequency
of ν = 34.8GHz = 0.144meV; b) the difference in the London penetration depth
λL(T )− λL(1.3K) as a function of the reduced temperature T/Tc. The solid line
represents the theoretical results for a model system the critical temperature of
which has been lowered from 95 K to 91.5 K by the resonant impurity scattering
(c = 0). The dashed line corresponds to a model system of the same Tc = 91.5
K but with the intermediate strength impurity scattering (c = 0.5). In both
systems a low frequency cutoff ωc = 2.1Tc0 at zero temperature had been applied
to the fluctuation spectrum. The solid squares represent the experimental data
for a YBCO sample with 0.31% Zn substitution, while the open triangles describe
the experimental data for a YBCO sample with Ni substitution [8]. The arrows
indicate the data points which have been used to scale theory to experiment.
All this proves that a phenomenological model which describes the feedback
the superconductivity has on a fluctuation spectrum belonging to the same system
of quasiparticles which condense is capable of a consistent description of the tem-
perature dependence of various properties of optimally doped samples of YBCO
with and without additional doping with Zn or Ni impurities. In the next sub-
section we would like to investigate how the frequency dependence of the optical
conductivity is affected by the model assumptions and how this agrees with the
experiment.
82
Constraints on HTCS mechanisms
3.6. Optical conductivity, superconducting state
In figure 7a we compare the optical reflectivity R(ν) and the real part of the
optical conductivity σ1(ν) with the data reported by Wang et al. [34] for an un-
twinned, optimally doped, clean YBCO single crystal (T = 8K) and with the data
measured by Homes et al. [30] for a similar sample (T = 12K). These authors also
0 200 400 600 800 1000
0.84
0.86
0.88
0.90
0.92
0.94
0.96
0.98
1.00 a)
ν (cm-1)
R
( ν
)
ω
c
= 0, T = 9.5 K
ω
c
= 2.1 T
c0
, T = 9.5 K
exp. untwinned, E||a
exp. untwinned, E||b
Wang et al. T = 8 K
exp. twinned,
exp. untwinned, E||a
exp. untwinned, E||b
Homes et al. T = 12 K
0 200 400 600 800 1000 1200
0
1000
2000
3000
4000
5000
b)
ν (cm-1)
σ 1(
ν)
(
Ω
-1
c
m
-1
)
exp. twinned,
exp. untwinned, E||a
Homes et al. T = 12 K
exp. untwinned, E||a
Wang et al. T = 8 K
theor. ω
c
= 0, T = 9.5 K
theor. ω
c
= 2.1 T
c0
, T = 9.5 K
Figure 7. a) The reflectivity R(ν) and b) the real part of the optical conduc-
tivity σ1(ν) as a function of frequency ν. Theoretical data are presented for the
theoretical equivalent of a clean sample with (solid lines) and without (dotted
lines) a low frequency cutoff in the fluctuation spectrum. The temperature is 9.5
K. Included are the experimental data reported by Wang et al. [34] for a clean,
untwinned, optimally doped YBCO single crystal. The sample temperature is 8
K, the solid triangles correspond to the light polarized along the a axis (E||a)
while the open circles are for E||b. The other data are from the experiments by
Homes et al. [30] and are for a clean, untwinned, optimally doped YBCO single
crystal and a sample temperature 12 K. The solid down-triangles correspond to
E||a and the open squares to E||b. Finally, data for a clean, twinned, optimally
doped YBCO single crystal are also included (solid squares).
report data for a twinned, optimally doped, clean YBCO single crystal. Theoreti-
cal results are presented for the theoretical equivalent of the clean sample without
(the dotted line) and with (the solid line) a low frequency cutoff ωc = 2.1Tc0 at
zero temperature. We also used ε0 = 3.5, ωp = 1.6 eV, and T = 9.5K. Obviously,
the theoretical data for a system with the low frequency cutoff in the fluctuation
spectrum are in better agreement with the experiment. It is also interesting to
83
E.Schachinger, I.Schürrer
note that the best agreement can be found for the E||a data of untwinned samples
(the solid triangles and the solid down-triangles). This is not surprising as the light
polarized along the a-axis probes just the CuO2 planes and the theory presented
here is developed to describe superconductivity in two-dimensional copper-oxygen
planes. The worst agreement between theory and experiment is found for the
twinned sample (the solid squares). This shows that our theoretical equivalent of
the twinned clean sample is not sufficient to describe completely the influence the
background scattering has on the optical conductivity at higher frequencies.
A similar comparison can be found in figure 7b for the real part of the optical
conductivity σ1(ν) as a function of frequency ν. The theoretical results for the
system with the low frequency cutoff in the fluctuation spectrum have been scaled
to fit the data point indicated by the arrow. Using a slightly different scaling would
have provided an almost equally good agreement with the data reported by Homes
et al. (the solid down-triangles). The same scaling was then applied to the system
with the full fluctuation spectrum. The main feature of these results is that the low
frequency cutoff in the fluctuation spectrum suppresses the real part of the optical
conductivity to higher frequencies, thus indicating a bigger gap than one would
find without such a low frequency cutoff. This is in very good agreement with the
E||a data for the untwinned sample in the region of 200 < ν < 1000 wave numbers
which is quite remarkable. Again, no agreement at all is found for the twinned
sample developing a frequency dependence of σ1(ν) which would correspond to a
much higher impurity content as it is required by the critical temperature.
4. Conclusion
Experimental evidence is very much in favour of a superconducting order pa-
rameter which is predominantly of a d-wave symmetry. In orthorhombic systems
a subdominant component of a s-wave symmetry can be expected. A mechanism
which is responsible for the superconductivity in oxides and which also results in
a d-wave symmetry of the superconducting order parameter is most likely to be
electronic in origin (no phonons).
In this paper a phenomenological model developed by Schachinger et al. [16–18]
has been discussed and proved to be able to describe consistently the tempera-
ture dependence of the in-plane penetration depth, the temperature dependence
of the microwave conductivity and of the electronic thermal conductivity of clean,
twinned and optimally doped YBCO single crystals. Moreover, calculations per-
formed within the framework of this model revealed that the influence of impurities
of various kinds on the temperature dependence of the microwave conductivity and
of the in-plane penetration depth can also be explained consistently. Finally, it was
possible to demonstrate in this paper that the model is also capable to predict a
frequency dependence of the low temperature optical conductivity which is in very
good agreement with the experimental data found for the light polarized along the
a-axis of untwinned, clean, optimally doped YBCO single crystals.
These results will now be used to put additional constraints on possible mecha-
84
Constraints on HTCS mechanisms
nisms of superconductivity in oxides: it is not only most likely that the mechanism
is electronic in origin leading to a d-wave superconductivity. Moreover, it seems
necessary for the fluctuation spectrum which causes superconductivity to belong
to the superconducting quasiparticle system because it becomes gapped as the
superconductivity sets in. This has been demonstrated quite clearly by the phe-
nomenological model discussed here.
Acknowledgements
The authors are greatly indebted to Prof. Dr. J.P.Carbotte for his intensive
collaboration and support. They would also like to thank Dr. C.C.Homes and
Prof. Dr. T.Timusk for the access to their data prior to publication. This research
was supported in part by Fonds zur Förderung der wissenschaftlichen Forschung
(FWF), Vienna, Austria under contract No. P11890-NAW.
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Обмеження на можливі механізми
високотемпературної надпровідності
Е.Шахінґер, І.Шюррер
Інститут теоретичної фізики, Технічний університет м.Ґрац,
Петерсґассе 16, А-8010 Ґрац, Австрія
Отримано 23 березня 1998 р.
Дана стаття розглядає феноменологічну модель, що використовуєть-
ся для опису різноманітних властивостей dx2
−y2 –надпровідників в за-
лежності як від температури, так і від частоти, а саме глибини про-
никнення Лондона, оптичної провідності, мікрохвильової провідності
та електронної термічної провідності. Ми вважаємо, що саме площи-
ни CuO 2 є основним чинником для виникнення надпровідності, і то-
му розвиваємо двомірний формалізм, в якому процеси непружного
розсіяння моделюються точно через спектральну густину, що описує
флуктуаційний спектр, який є відповідальним за виникнення надпровід-
ного переходу, а також за велике непружне розсіяння, що спостері-
гається в нормальному стані вище критичної температури Tc . Зво-
ротній вплив надпровідності на спектральну густину моделюється тем-
пературнозалежним низькочастотним обрізанням.
Теоретичні результати порівнюються з експериментальними даними
і, виходячи з того, що дана модель дає змогу зробити послідовний
опис цілого ряду явищ, формулюються обмеження на можливі меха-
нізми виникнення надпровідності в оксидах.
Ключові слова: високотемпературна надпровідність, глибина
проникнення Лондона, оптична провідність, електронна
теплопровідність
PACS: 74.20.Fg, 74.25.Nf, 74.72.-h
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