Journal of the Less-Common
451
Metals, 144 & 165 (1990) 451-457
ION BEAM MIXING OF LA(OH$/CU
and LA(OHI~/SRO/C~ MULTILAVERS
J.P. MATHE"ET*, A. TRAVERSE*, S. MEGTERT+ and J. CHAUMONT* * Centre de Spectrometrie Nucleaire et de Spectrometrie de Masse, INZP3-CNRS, F-91405 Campus Orsay, France + Laboratoire de Physique des Solides, Bat. 510, Universlte Paris XI, F-91405 Orsay Cedex, France
We have submitted bilayers of La(OHls/Cu and multilayers
of La(OH)s/SrO/Cu
to energetic heavy ion irradiation at 300 the possibility of preparing investigate
K and 700 K in order to LaaCuOI and (La1_xSrx)2Cu0 4 through the ion beam mixing technique. For comparison purposes, similar annealed at 700 K. Results are given concerning the samples were modification of the atomic compositions (La, Sr. Cu. 0 and Hl, the atomic depth distributions, the compound formation, induced either by irradiation or by thermal annealing. The specific role of the ion beam mixing process is emphasized.
1. INTRODUCTION The
goal
possibility step,
the
of
experiments
of preparing
using
the
thermodynamical
ion
described
beam
on metallic
mixing
multilayersl,
induced by the irradiation beam
technique.
If
the
target
diffusion
to
investigate
the
This
technique
is
far
from
layers of each component. From results
we know
that
through
elastic
layer interpenetration.
if the heat of mixing of the layer components
temperature
collisions
(scale time 10-13s1, atoms may jump from one
layer to the other, leading to a progressive mixing is enhanced
is
; it consists in sending an energetic (keV to MeVl
equilibrium
ion beam through a stack of alternating obtained
here
thin films of LazCuOl and (La1_xSrx12CuOq in a single
during
irradiation
is
high
Rate of
is negative.
enough
for
atomic
to take place, within lo-" s (a diffusion enhanced by defects due to
irradiation), ordered final systems may build up. The
idea
here
is
to use
11
the amount
of
energy
deposited
in atomic
collisions to induce mixing between La/Sr/Cu layers and ill the possibility of enhanced diffusion usual
ones,
i.e.
(La1_xSrx12CuOl has multilayer
to prepare the final system at a temperature about been
9OO'C'. made
by
Another
two
implanting
steps Sr
in
lower than the
attempt an
to
evaporated
prepare La/Cu
followed by annealing in oxygen at a temperature > 800 K to obtain
superconducting
samples'.
First experiments3 on La/Cu bllayers have already shown that an evaporated La layer even covered with a 40 nm Cu layer evolves
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towards La(OH13 during
0 Elsevier Sequoia, Printed in The Netherlands
452
exposure
to ambiant
Cu instead the
of
initial In
system
this
compared depth
atmosphere.
induces
paper,
to
we
those
under
partial
starting
of
components
shown3 that
results
obtained
on
on La(OH13/Cu bilayers,
La,
Cu, Sr,
Au irradiation
are
La(OHls and
irradiation
at 300 K of
H desorption.
present
obtained
distributions
formed
Hence the
LaaOJ and Cu02. We have also
La(OH13/Sr/Cu
with
0 and H and the
respect
nature
at 300 K and 700 K or under
trilayers
to
of
the atomic
the
thermal
compounds
annealing
at
700 K. A spontaneous samples,
the
boundary
is
initially
mixed
interpenetration
scale thicker
the substrate
irradiation,
thermal
annealing.
identification
the
does
layers
not
evidenced
grains,
being
presence
of
the
layer.
not
increase
there
is
certain, seem
the substrate
is
or
very
only
New compounds,
compounds
with
the
atomic
Hydrogen
partial
possibly are
to
Sr
The
at
the
The
mixed of
irradiation
desorption
some
as-deposited
depth
totally
the
whatever
desorbs
at 700
at 300 K or under
La2CuOI and
formed
display
in
unknown.
much under
or under annealing.
while
being
These
relation
in
layer
of
which,
temperature
K under
ones.
of
(La1 xSrx12CuOa,
expense
of
preferential
the
the
initial
orientation
in
structure.
2. EXPERIMENTAL Bilayers thick
of
La/Cu and trilayers
and Sr layers
by electron
gun evaporation,
0.15
As
rim/s..
of
20 nm thick)
already
induces
an evolution
despite
the 40 nm Cu coverage,
(La and Cu layers
on
bilayer3,
about
lo-’
exposure
La to La(OH13. We found although
were
at 300 K on carbon
under a vacuum of
shown
of
La/Sr/Cu
were deposited
that
a definite
Pa at a rate
to
ambiant
Sr also
40 I-MI
substrates around
atmosphere
trapped
identification
oxygen,
between
SrO
or Sr(OH12 is not possible. Irradiations’ f luence before
of
and after
He particles’ atoms, “N
were
8~10’~
ii)
irradiation
to measure using
the
on H to measure
diffraction identify
performed
with
energetic
Au ions
: i) by Rutherford
the amount and depth
resonant
(XRBl patterns compounds present
The thicknesses
nuclear
were
recorded
on a 8-28
evaporated
here
are
not
those
Although we use
by RBS to detect
6.385 in
the
powder
a
2 MeV
Cu Sr and 0 MeV incident
target.
X ray
diffractometer
to
in the stack.
in RBS experiments. possible
(FlNRl of
La,
to
in situ
(RBSl of of
distribution
; however they were chosen
substrates,
backscattering
reaction’
the H amount and depth
MeV) up
were analyzed
distributions
La2CuOl composition
on carbon
(3.65
ions. cms2, at 300 K and 700 K. Samples
not
high
required to
Tc superconducting thanks
only
components
to
their of
reach
well
films
them because, the heavy
to
provide
are
the
defined not
deposited
low mass, the
target
final peaks
it
is
such as
453
La, Sr, Cu but also the light one such as 0. A precise characterization samples
is a prerequisite
for the understanding
of the processes
of our
involved
in
trilayer before irradiation
is
ion beam mixing.
3. RESULTS A typical RBS spectrum recorded on La/Sr/Cu shown in Fig.
1 (dotted line). By comparison
between
experimental
in the target. The numbers of La, Sr and Cu correspond
to those expected from
within 5%. while the number of 0 is approximately
the evaporation
peak area
it is possible to deduce the amount of each component
and those of standards,
equal to 3
times the number of La plus the number of Sr. The RNR spectrum detected on the same trilayer, plotted in Fig. 2 (square before irradiation),
indicates that a
layer, about 30 nm thick just below the surface remains free of hydrogen. Part of the Cu layer and rest of the sample contain an H amount, H/La a 3. These two results are in favour of an initial stack formed of La(OHls/SrO/Cu.
Au
I
FIGURE 2
FIGURE 1 Number of MeV "N on (crosses) versus the
RBS spectrum of a trilayer before (dotted line) and after (full line) Au irradiation at 700 K.
Part of an experimental showing Fig.
La and Cu peaks
3.
A
good
interpenetration the bottom,
fit
RBS spectrum detected
is compared requires
the
layer. Approximately boundary.
about
30%
of
on a La(OHls/Cu bilayer
to a simulation assumption
with
of
a
and
the RUMP' code in
spontaneous
partial
on the initial layers. The stack is made of a pure La(OHls at
then a layer containing
mixed
7 due to the RNR of 6.385 H before (square) and after Au irradiation at 700 K N energy.
When the
Cu, La, 0 and H atoms,
13% of the La and Cu atoms a Sr
total
layer
number
is present, of
heavy
are
the
(La, Sr
then a pure Cu
in this
spontaneously
interpenetration and
Cul
atoms.
concerns Through
454
RBS, it is not possible to determine if it is at the atomic or at the grain scale that this interpenetrationtakes place.
300
320
310
Channel FIGURE 3 Simulation (dotted line) and experimentalLa and Cu peaks (full line) of a RBS spectrum recorded on a bilayer. An XRD spectrum,Fig. 4 a, recordedbefore irradiation,displays the (1001, (2001, (3001 lines of the La(OH)s phase. The wide peaks are the (0021, (IOO), (0041, (110) lines of the badly crystallizedcarbon substrate.The absence of other
La(OHls peaks
indicates a
preferential orientation along
the
crystallographica axis. Signals coming from SrO or Cu are too weak to be detected, due to the thin layer thicknesses and low linear absorption coefficientwith respect to the incidentwavelength (Cu Kcrradiation).
b
FIGURE 4. X Ray spectrum recordedbefore (al and after (bl Au irradiationat 300 K. The evolution of a trilayer under Au iradiationat 700 K is shown Fig. 1 (full line). The Au peak correspondsto the irradiatingAu ions stopped at a
455
depth
of
900
nm
redistribution displacement
below
the
the
of
substrate
species
surface.
(widening
and
Although
there
lowering
of
of the La peak). it is obvious that an homogeneous
reached. Such an homogeneous the experimental
distribution
is
the
a
depth
Sr
peak,
mixing is not
is simulated Fig. 5 and compared to
spectrum. Increasing the irradiation fluence does not lead to
more in depth homogeneity. Results obtained after irradiation at 300 K are
FIGURE 5 Comparison between the experimental RBS spectrum taken after Au irradiation of (dotted line) of a a trilayer at 700 K (full line) and the simulation homogeneously mixed system containing the same amount of La, Cu, Sr and 0 atoms. similar.
The amount
incident
Au beam,
remains
of Cu is slightly
since
identical within
The amount
the Cu
layer
the experimental
of 0 is lowered by about
about 50% after
decreased,
irradiation
due
to sputtering
is the overlayer uncertainties,
10% after
at 700 K. Hydrogen
by
the
; the amount of La La being
irradiation
below Cu.
at 300 K and by
totally diffuses
out of the
sample when it is irradiated at 700 K as shown on Fig. 2 (crosses), by going either outside or in the carbon substrate. Annealing at 700 K during the same time as irradiation previously substrate
noted,
temperature,
the La(OH1s lines LazCuOl or allow
leads to a partial H desorption only
a
partial
is
only
(75%). At 300 K, as
measured.
XRD spectra taken after irradiation
Whatever
phase
The
identification
lack of
supplementary
(other systems
such
peaks
as LaCue
cannot be excluded). However, this is in favour of a preferential growth.
the
no longer display
; new peaks are present whose 26 values may correspond to
(LaX_XSrXlaCuOo peaks.
a unique
desorption
does
not
or LazOs
orientation
456
4. DISCUSSION AND CONCLUSION To build up LazCuOl or (La,_xSrxlzCuOl thin films, we have chosen an unusual starting high
technique,
materials,
Tc
the ion beam
of multilayers
La(OHla, SrO and Cu. The carbon
superconducting
atomic
irradiation
films
characterization.
epitaxial
The
growth,
as-deposited
sustrate,
was
used
interpenetration
of the layers, which has not been explained
interpenetration
being
mixing
increase
does
whatever
favoured
the temperature,
collisions density,
not
very
the Sr under
although
is on the average
metallic
by much
This
a
precise
up to now, the
initial
ion beam
spontaneous irradiation, in atomic
In such a range of deposited
are usually
mixed
over
for
spontaneous
the amount of energy deposited
300 eV/i.
multilayers
layer.
energetic
unusual
not good
to allow
display
stack
to check
and
several
energy
nm depth.
The
absence of mixing in these experiments could be due to the fact that we try to mix
oxide-metal
layers
instead
of
mixing
metallic
However
layers.
leave the sample (partially or totally depending on the substrate under irradiationl. it increases
are
the H
locally
compounds.
temperature
Irradiation is more efficient than thermal annealing since loss. As a result
atomic bonds between atoms
the
: hydrogen and oxygen
composition of the spontaneously mixed layer is modified
of
irradiation
La and 0 or H and between
present,
The saturation
new
atomic
bonds
or thermal
treatment,
Sr and 0 are broken. may
form
to
build
of ion beam mixing may be understood
As Cu
up
other
in the sense
that once the spontaneously mixed layer has evolved under irradiation
towards
a new compound, the latter is stable against further ion beam treatment. It is
interesting
to note
systems formed under
that either
the La(OHls
irradiation display a preferential
on the carbon substrate
compound
or
the new
orientational
as indicated by the absence of conventional
intensity peaks seen in a powder X ray diffraction have recently been observed"
pattern.
growth highest
Similar
effects
in implanted systems.
What can we expect concerning the formation of LazCuOl and (Lal_xSrx12Cu04, after
these results
multilayers
? The
concerning starting
instead of 2 required) temperature possibly
higher
irradiation
system
of La(OHls/Cu
is already
rich
and La(OHls/SrO/Cu
in oxygen
(3 0
per
La
: no further oxygen charging may be needed. Instead of
than 800 K as in Ref. 4, a temperature
lower, no intermediate
of only 700 K (or
temperature having been checked)
is necessary
for a total H loss accompanied with formation of new compounds. This indicates the specific role of energy deposition under ion beam treatment. The structure of the substrate
seems important
in building
was observed even on the badly crystallized
up oriented
phases,
since this
carbon substrate. This encourages
us to use substrates such as MgO or SrTiOs since they are known to favour good epitaxial
growth9
of
the
superconducting
phase.
Moreover,
as
they
are
insulating materials, they should be helpful for measuring the conducting properties of
our
samples, a
supplementary and
necessary too1
for
characterizationof our final systems.
ACKNOWLEDGEMENT The SEMIRAMIS group of the Centre de Spectrometrie Nucleaire et de Spectrometriede Masse is gratefullyacknowledgedfor its constant and helpful assistanceduring the irradiationand characterizationexperiments.
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