0038-1098/88 $3.00 + .OO Pergamon Press plc
Solid State Ccmmunications,Vo1.66,No.12, pp.1231-1235, 1988. Printed in Great Britain
.u
EFFECTS
OF OXYGEN
DEFICIENCY
M. Garriga,
ON THE OPTICAL
J. Humlicek,’
M. Cardona,
SPECTRA
OF YBa&usOr+
E. Schijnherr
Max-Planck-lnstitut fiir Festkijrperforschung, Heisenbergstrasse 1, D-7000 Stuttgart 80, Federal Republic of Germany (Received April 18, 1988 by M. Cardona)
We report on the variation
of ellipsometric
pounds with oxygen content compound
two new, rather
in the semiconducting oxygen content,
spectra of the YBa2Cu30r_x
0 < z 5 1. Beside the structures intense peaks are observed
compound
(z > 0.5).
For the
Cu(3d)
understanding
YBa2Cu307_x tronic
materials
structure
deficiency
z.
Several minor features become significant
conducting
T,
The transport
decreasing
tion of one-electron the material
netic
with
fairly
high
we report
Due to the expected should oxygen
ceramic
tematic
tric function. in ceramic,
thin film
are essentially
dependence
ramics
have already
room temperature
in the spectra
but
spectra
been presented
some sys-
[7].
observed
and annealed
and furnace removal metric
with those
J.E.Purkyne
KotlaFsk6 2, 611 37 Brno, Czechoslovakia
of Solid State University,
to room
sive or diamond
of
atmosphere
temperature.
by heating
The oxygen
the pellets
was determined [9].
pro-
was pressed into
at 950 “C in oxygen
was performed
in argon.
by the thermogravi-
For the optical
measurements
polished
with
alumina
paste dissolved in methanol.
the abra-
For the final
step 0.25 pm abrasive was used. The samples were meaature stat.
after
measurements
polishing.
For the low temper-
the samples were placed in a cryo-
After baking out the cryostat
2 x lo-’
Torr was obtained,
a vacuum
which
better than
is necessary to avoid
condensation. The optical ing analyzer
measurements
~1 + icz
were taken
spectroellipsometer
quantity
light
which,
like the YBa2Cu30r_, plex and differences
reflectance isotropic
the relation
are mainly function;
E=
materials more comthin film
orientations
of
161. Fortunately,
in the absolute the positions
tures remain almost unaffected.
function
is much
axes are observed
pseudodielectric
ratio of s-
of sintered,
due to different
the differences
a rotat-
homogenous
polycrystalline
in the spectra
samples
the crystallographic
for
with
In this system the
related to the dielectric
[ll].For anisotropic
and crystalline
[lo].
is the complex
samples, is directly
several weak features
Department
cooled
method
appropriate
and CuO to 950 “C in pure
The powder obtained
The stoichiometry
measured
we have measured the tem-
of Science,
at 1 atm.
pellets
of high T, ce-
function
BaC03
oxygen
and p-polarized
Our results at
of the pseudodielectric
of Y2O3,
results on the
are enhanced.
Faculty
from Ba(5d)
The samples were made by heating portions
sured immediately
mea-
of YBa2Cu307
Preliminary
* on leave of absence from: Physics,
structures
and single crystals
. At low temperatures
YBa2Cu3Oe
transitions
The 1.75 eV peak is possibly due to Cu(3d)
values of the dielec-
agree in the main features
dependence
of optical
the optical
introduces
the spectral
Further,
upon cooling the samples
involving
samples were mechanically
for z N 1 [S].
on single crystals,
of the optical
of Kelly et al. [8].
Fur-
are most easy to obtain
This fact
the same [6].
oxygen
perature
anisotropy
in the absolute
However,
For
to be antiferromag-
the variation
be performed
samples.
[l].
to the predic-
UV with oxygen concentration.
strong
stoichiometries
inaccuracies
of
is super-
see, e.g., [2,3,4].
Neel temperature
spectra in the visible-near
with
properties
as x increases
band theory,
elec-
on the oxygen
in contrast
has been found
In this Communication
states.
in the
of their
For 0 < z < 0.5 the compound
ther,
different
knowledge
show a strong dependence
with
surements
states to O(2p)
of superconductivity
2: 2 0.5, it is semiconducting
depends on the
states.
good
is needed.
these materials
strongly
whereas the energy shows a weak dependence both on oxygen content
and temperature.
and O(2p)
at N 1.75 eV and N 4.1 eV
Their intensity
to 7 K. We associate the 4.1 eV peak to excitations and/or
high Z’, com-
observed in the z = 0
values of the
of spectral
struc-
Spectra between 1.6 and
5.3 eV were taken on a large number of samples of different oxygen deficiency
1231
x, both with Y and Tm as trivalent
THE OPTICAL SPECTRA OF YBa2Cu307-x
1232 ions. In the semiconducting
compound
eral rare earth ions were substituted spectral
structures
main features
in our ellipsometric
with other optical
transmission
and reflection
tron
loss spectroscopy
energy
metric
measurements
features,
YBa2Cu30s
observed
measurements, [14],
structure
including
[7,12,13],
A similar
structure
at -2.7
[13,15].
to transitions
eV has been reported
Therefore,
within
ellipso-
dominate
we found
weaker
weak features appear
at low temperatures.
the spectra
we attribute
the Cu-0
are present in both materials. Two strong absorption bands
elec-
and recent
In addition
mainly
[7].
for La2_,SrxCuO4
results agree in the
spectroscopy
[S].
sev-
for Y. The strongest
Vol. 66, No. 12
planes,
at 1.75 and 4.08 eV
; further,
of YBa2Cu30rj
and three low energy satellites
as oxygen
content
this which
several
(they
dis-
increases in the same way as
the main peak) of the 4.08 eV band, can be resolved in The pseudodielectric exhibits
function
substantially
YBa2Cu307
more
structure
the superconducting
behavior. material
increasing
range, but centered oxygen deficiency
eV for z =
the temperature appreciable There
spectral
of
spectrum
or its first derivative
Fig. 1).
positions
of all the observed
The energy
tures for different
semiconducting
pendence
on the oxygen
dependence trivalent
eV in YBa2Cu307
ion.
are shown
end of the
strong
With
deficiency.
Spectra
for different
in Fig. 2.
The
results
and their
When
is however
a red shift with
with
is observed increasing
ion M in the MBa2Cu307
(Fig.
concerning
at 4.08 eV is the strongest
spectra of the z = 1 materials.
ionic radius
Gd or Sm no significant
compounds
can therefore
change is observed
b .: : _....
:
. . ..
. ....
.. . .../
4
2
1
2
3
Energy
4
5
6
I’
1”’
1
2
(eV1
electric
I”’ 4
3
Energy
Fig. 1. Left: Real and imaginary function
< ~1 >
samples of YBazCusOrj and 300K derivative
(dotted of < q
to the energy, ted line).
< ~2 > of ceramic
measured at 7 K (solid line)
line).
Right:
> of YBa2Cu306
at 7 K (solid
numerical with
first
respect
line) and 300 K (dot-
The arrows indicate
resolved structures.
(eV I
parts of the pseudodi+i
for Tm,
(Fig. 3). We
discard the rare earth ion as being responsi-
.:’
,“5
one in the
When replacingy
Y Ba2cU3ofj
(El)
the two
et al. 181. We
of these two structures
10
;
this
z in TmBa2Cq07_,
7K . . . . . . . 300 K
A
in de-
possible origin.
The structure
no 1).
r Y 6a2cu306
8
a strong
decreasing
to 7 K only a slight sharpening of this structure
are listed
We investigated
bands are similar to those of Kelly
shall discuss the characteristics
of Q down
(see struc-
in two series of samples, with Y and Tm as
of the maximum
1 (see Fig. 2).
samples
Table I. The 1.75 and 4.08 eV peaks exhibit
of
of the two
at lower energies.
the low temperature
z this band shows a progres-
shift
of the trivalent
feature
at the semiconducting
sive decrease in the position to -2.6
that
has been discussed in detail
is the broad band at -2.8
is also present
composition
than
The spectral structure
in Ref. [6]. The only common materials
(Fig. 1)
which shows few broad bands and a low en-
ergy onset of metallic
which
of YBa2Cu306
the position
of the
I 5
6
THE OPTICAL SPECTRA OF YBa2C~30~_~
Vol. 66, No. 12
1233
Table I. Energy positions (in eV) of the maxima in the spectra of ~2 in MBa2Cu& ent trivalent
materials, for differ-
ions M.
Y
Y
Tm
Gd
Sm
6
7 K
300 K
300 K
300 K
300 K
1.78
1.75
1.76
1.71
1.74
2.12
2.12
2.12
2.06
2.08
2.59
2.61
2.58
2.51
2.58
3.16
-
-
-
-
3.73
3.74
3.75
3.74
3.72
3.86
3.90
3.90
3.90
3.92
3.95
-
-
-
-
4.08
4.08
4.08
4.08
4.08
4.59
4.60
4.58
4.58
4.60
5.2
5.3
5.3
5.3
5.3
A\\
-
089
1
ble for that feature; see also Ref. [8]. On the other hand the intensity of the satellites in the low energy side of the structure depends on the trivalent
ion substituted for Y:
whereas for Gd the satellites can be clearly resolved even at room temperature
(see real part of < E >,Fig.
3)
for
Y they become clear only upon cooling to 7 K, or in the differentiated
room temperature
spectrum (Fig. 1). The
4.08 eV band shows a rather small temperature
I I.
depen-
I
I
I
2
1
dence. No significant shift in energy or increase in intenWhen decreasing the oxygen
I
4
Energy
sity is observed between 300 K and 7 K, the broadening decreasing by about 20%.
I
1
3
I
I
5
6
(eV)
deficiency 2: the structure exhibits a rapid decrease in intensity and a considerable shift to higher energies (right side of Fig. 4)
remain unchanged, In the complete
Fig. 2. Imaginary part < ~2 > of the pseudodielectric function of TmBa2Cu#_x
whereas the broadening and lineshape in agreement
with Kelly et al.
as a function of oxy-
gen deficiency 2.
[8].
range of z a shift of 160 meV and a
linear decrease in intensity is observed.
In some of the
intensity fall with increasing oxygen content would be re-
one-electron
[3,4] there is a
lated to the diminution
band structure calculations
group of rather flat conduction
bands at -4
eV above
the Fermi level that could be a good candidate for the fi-
In the Ba-0
of the number of 0-Cu-0
units.
case, the oxygen content dependence of the
structure could be understood as due to changes in the
nal states of the observed peak. Those bands are mainly
Ba-0
of Ba(5d) character.
of excitonic interaction by the free carriers. The best way
Therefore one tentative assignment
of the 4.1 eV structure is that corresponds to Ba-0 transitions. ported
This interpretation
would be further
by the fact that the optical spectrum
like sup-
of BaO,
which crystallizes in the sodium chloride structure with a lattice constant of 5.52
A,exhibits
two strong excitonic
peaks at 4.06 and 4.30 eV, accompanied features at 3.88 and 3.95 eV [16]. of YBa2Cus07_,
by two small
In the Ba-0
planes
, the atomic arrangement is similar to
that of the sodium chloride structure with a distance of 2.753
A
between Ba and 0 atoms which corresponds to a
lattice constant of 5.45
A.On
the other hand Kelly et al.
[8] concluded that Ba does not participate because substitution
in the peak
of Sr for Ba does not change sub-
stantially the observed structure.
They attribute
the 4.1
distance, accompanied
to decide between both possibilities would be a measurement of the different components of the dielectric tensor in the 4 eV region.
within the Ba-0 that should be
observed preferentially with the electric field of light perpendicular to the c axis. to 0-Cu-0
Similarly,
if the band is_due
units, it should appear mainly for the E I] c
configuration. The absorption peak at -1.75 onset of strong optical ing compounds.
eV corresponds to the
absorption in the semiconduct-
It lies far above the effective gap of
0.2 eV given by temperature
dependent
resistivity mea-
surements [18]. The strong dependence of this structure on oxygen deficiency z is shown in Figs. 2 and 4. pronounced maximum
isolated linear 0-Cu-0
seen up to 2 N 0.5.
in K2CuCl3
If the transitions
planes are responsible for the structure,
eV band to localized excitations which take place in the units, arguing that
by an increasing screening
The
in the < Q > spectra is clearly For larger x values the band tends
where the Cu is bonded in a similar linear complex [17],
to disappear in the background of metallic-like
also a strong absorption peak is observed at 4.4 eV. We
tion, but it is still observed as a weak shoulder in the
feel that both interpretations, them, are possible.
or even a combination
In the case of Cu-0
of
excitations the
derivative spectra (Fig. 4). temperature
absorp-
The peak has the strongest
dependence of all the observed structures:
THE OPTICAL SPECTRA OF YBa2C~30~_~
1234
I
1
2
3
4
Energy
5
1
6
I
I
2
Vol. 66, No. 12
I
I
3
Energy
(eV 1
Fig. 3. Real (left)
and imaginary
pseudodielectric
functions
(right)
parts
of sintered
.
I
4
II
5
I
6
(eV) of the
samples
of
, for M = Tm, Y, Gd, and Sm.
YBa2Cu306
lb
-
0mY
_
ooTm
3
d 0
0
2
/:
O0
Q1
0
x Y
JE
al
00 l
1.85
_
s -? sl 1.80 -
a
.=
l
a5
a
8
l
iii c 1.75 -
*
0.2
0.4
0.6
8
l
I
0.8
0
1.0
0.2
0.4
0.6 X
X
Fig. 4. Left: Energy position and intensity eV structure
as a function
in YBa$u307_x (circles). the -4.1 deficiency
Right:
of oxygen
(squares) Energy
eV structure
(circles).
deficiency
z
and TmBa$u307_,
position
as a function
z in YBa2Cu307_,
TmBa2Cu307_x
of the -1.75
and intensity of oxygen
(squares) and
of
4.20
-415
l
8
W
0.0
-
m
l
l
0 0.8
z
E
G - 4.10 t I 5 1.0
1235
THE OPTICAL SE'ECTRAOF YBa Cu 0 2 3 7-x
Vol. 66, No. 12 linear interpolation
of its position between 300 K and 7
K gives a temperature
coefficient of -8
x
10e5eV K-‘.
structures at 1.75, 2.61, and 4.08 eV and several weaker transitions that can be better resolved at low tempera-
Its intensity increases by a factor of two, whereas the
tures.
spectral width decreases by about 10% in that tempera-
has been measured. The 2.6 eV band is nearly indepen-
ture range. The changes with temperature
dent of the oxygen deficiency and is probably related to
become even
The temperature
larger when the samples are heated up to 700 K [19]. On
transitions
the other hand, the peak shows a very weak pressure de-
have a rather strong dependence on oxygen deficiency
pendence 114. The transition seems to be not consistent Since the proposed in-
z. The 4.08 eV peak progressively decreases as z decreases from 1 to 0. This peak could be due to transi-
[12] should be rather weak, an
tions in the Ba-0 planes although fairly strong arguments
with band structure calculations. traionic
d-d excitations
alternative
explanation
in terms of charge transfer tran-
sitions within Cu(3d)-O(2p)
states is also possible [13,7].
in the Cu-0
dependence of the main bands
[8] support a 0-Cu-0
planes.
origin.
The other two features
The 1.75 eV band is ob-
served as a strong peak for z < 0.5.
For larger z values
A coherent explanation of the structure should give a cor-
only weak shoulders in the metallic-like
rect interpretation
been found. The most plausible explanation for this band
of the temperature
in the present work, together
changes observed
with the pressure depen-
are charge transfer excitations within Cu-0
dence reported in Ref. [13]. Again, determination of the optical anisotropy can contrrbute to the assignment of
experiments,
the structure.
cidate the origin of these bands.
materials on oxy-
gen deficiency. At x N 1, the spectra show three strong
in particular,
determination
planes. New
of polarization
dependence of the last two structures would help to elu-
We thank K. Syassen and U. Venkateswaran
In conclusion, we have measured the dependence of the optical spectra of MBa2Cus07_,
absorption have
ful discussions, the crystall preparation
for help-
group, H. Hirt,
M. Siemers, and P. Wurster for expert technical help.
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