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Yb3+ in RAlO3 (R = Eu, Gd, Tb, Dy, Ho, Er). A 170 Yb Mössbauer effect study of the hyperfine parameters,
magnetic ordering and relaxation
P. Bonville, J.A. Hodges, P. Imbert
To cite this version:
P. Bonville, J.A. Hodges, P. Imbert. Yb3+ in RAlO3 (R = Eu, Gd, Tb, Dy, Ho, Er). A 170 Yb
Mössbauer effect study of the hyperfine parameters, magnetic ordering and relaxation. Journal de
Physique, 1980, 41 (10), pp.1213-1223. �10.1051/jphys:0198000410100121300�. �jpa-00208947�
Yb3+ in RAlO3 (R = Eu, Gd, Tb, Dy, Ho, Er). A 170 Yb Mössbauer effect study
of the hyperfine parameters, magnetic ordering and relaxation
P. Bonville, J. A. Hodges and P. Imbert
DPh-G/PSRM, C.E.N. Saclay, Boîte Postale N° 2, 91190 Gif
surYvette, France.
(Reçu le 23 avril 1980, accepté le 18 juin 1980)
Résumé. 2014 Nous
avonseffectué des
mesurespar effet Mössbauer
sur170Yb dilué dans RAlO3 (R
=Eu, Gd, Tb, Dy, Ho, Er), qui complètent notre étude antérieure
avecR
=Tm, Yb et Y (Phys. Rev. B 18 (1978) 2196).
Dans tous les
casl’ion Yb3+ présente
undoublet fondamental de champ cristallin bien isolé et extrêmement
anisotrope (Ising). Pour la matrice
nonmagnétique EuAlO3
nousdonnons la fonction d’onde du niveau fonda- mental (à partir des
mesurespar effet Mössbauer et par RPE) et
nousexaminons la relaxation de spin due
auxinteractions
avecles phonons. Les autres réseaux présentent des propriétés magnétiques intrinsèques très diffé- rentes, de sorte que l’ion Yb3+ y subit des interactions magnétiques de nature variée. A partir d’une analyse des
formes de raies obtenues à la fois au-dessus et au-dessous de TN,
nousexaminons les interactions magnétiques
entre l’ion Yb3+ et les ions du réseau (influence de l’ordre magnétique et de la relaxation croisée spin-spin). La
contribution du couplage dipole-dipole à la relaxation paramagnétique croisée
aété calculée pour Yb3+ dans les matrices où R est
union de Kramers. Pour Yb3+ dans DyAlO3, l’interaction dipolaire donne la contribution dominante à la fréquence de relaxation mesurée (1,0
x109 s-1), alors que les fréquences mesurées pour Yb3+
dans ErAlO3 et GdAlO3 (3,0 et 4,3
x1010 s-1) sont dues principalement à l’interaction d’échange. Nous
avonsobservé
unedépendance
entempérature des fréquences de relaxation croisée due à l’interaction spin-spin pour Yb3+ dans ErAlO3 2014 causée probablement par
unordre à courte distance
2014et dans le composé
avecdeux sin- gulets fondamentaux HoAlO3, à la suite du dépeuplement thermique du singulet supérieur.
Abstract. 2014 170Yb Mössbauer measurements have been made
onYb3+ substituted in RAlO3 (R
=Eu, Gd,
Tb, Dy, Ho, Er) and complement
ourprevious study
onR
=Tm, Yb and Y (Phys. Rev. B 18 (1978) 2196). In
all
casesthe Yb3+ presents
awell isolated crystal field ground doublet with Ising-like characteristics. For the
nonmagnetic lattice EuAlO3
weestablish the Yb3+ ground state
wavefunction (from Mössbauer and EPR measure- ments) and
wealso examine phonon driven relaxation. The remaining host lattices have widely differing intrinsic magnetic properties
sothat the Yb3+ experiences
anumber of different magnetic environments. By studying the lineshapes both above and below TN
weobtain information concerning the Yb3+-host lattice magnetic interactions (influence of magnetic ordering and spin-spin
crossrelaxation). The contributions of dipole-dipole coupling to
the paramagnetic cross-relaxation rates
werecalculated for Yb3+ in the Kramers ion host lattices. For Yb3+
in DyAlO3 the dipole-dipole interaction accounts for the major part of the measured rate (1.0 x 109 s-1) whereas
the measured rates for Yb3+ in EuAlO3 and GdAlO3 (3.0 and 4.3
x1010 s-1)
arechiefly due to the exchange
interaction. Temperature dependent Yb3+ spin-spin cross-relaxation rates
areobserved both in ErAlO3 2014probably
due to short range ordering
2014and in the two-singlet ground state system HoAlO3 following thermal depopulation
of the upper singlet.
Classification Physics Abstracts 76.80
-71.70C
1. Introduction.
-The Rare Earth orthoaluminates
(RAI03) used as host lattices in this study provide
a range of dif’ering magnetic properties whose cha-
racteristics are generally well known [1-6]. In most
cases data is available concerning the crystal field
levels of the ground multiplet and in addition for those lattices composed of magnetic Rare Earth ions, the ground state g-values, the magnetic ordering
temperatures and the magnetic structures are also known.
We present here an account of the properties of Yb3 + diluted into the heavy Rare Earth ortho- aluminates RAI03 (R
=Eu, Gd, Tb, Dy, Ho, Er)
obtained using 17°Yb Môssbauer Spectroscopy.
Results for the two remaining members of the series R
=Tm and Yb as well as for Yb3 + in YA103
have been published previously [7, 8]. The present results relate to both the one ion properties such
as the g-values and the phonon driven relaxation and also to the magnetic interactions between the
Yb3 + ion and the host lattice ions. These interactions
are examined both through the influence on the Yb 31
ions of magnetic ordering in the host lattice and also
through the influence of the cross relaxation between the Yb3 + ions and the host lattice ions.
There are two advantages for using the Yb3 + ion
Article published online by EDP Sciences and available at http://dx.doi.org/10.1051/jphys:0198000410100121300
(4f ", 2F7/2) as a probe in the present case. First the
lowest Yb3 + crystal field level in all the Rare Earth orthoaluminates is well separated from the excited levels. This means that measurements can be made
over a wide temperature range where however only
the Yb3 + ground doublet is populated. Second, in all cases the Yb3 + ion has Ising-like characteristics
so that to a good approximation it can be taken to
have uniaxial properties. This assumption then facili- tates the relaxation lineshape analysis.
After briefly recalling the crystal structure of the
orthoaluminates and outlining the experimental details
in section 2, we present and discuss the various results in section 3.
The spin-spin cross relaxation data provides a
convenient way of separating the presented results
into three groups depending on the host lattice.
For the first group (section 3.t) EuAI03 (with TmAI03 and Y Al03 [7]), the host lattices are non
magnetic and there is no spin-spin interaction. Any
relaxation present is then driven only by the phonons.
As this phonon driven relaxation is temperature
dependent it is possible by going to low enough temperatures, to suppress any phonon induced line
broadening. In the case of Yb3 + in the orthoalu- minates this means going below about 30 K, where the phonon induced relaxation rates become too low
( N 5 x 1 O8 s -1 ) to broaden the absorption lines.
The second group (section 3.2) GdA103, ErAI03
(with YbAI03 [7]) comprises the three host lattice Kramers ions which give relatively high Yb3 + spin- spin cross relaxation rates at low temperatures.
The third group (section 3. 3) comprises two Van Vleck
ion lattices TbAI03 and HoAI03 and one Kramers
ion lattice DyAI03 all showing low Yb3 + cross
relaxation rates at low temperatures.
Section 4 contains a discussion of the Yb3+ spin- spin cross-relaxation rates in the various lattices in terms of the possible processes driving the relaxa- tion. Section 5 comments on the misfits observed in two cases between the experimental data, and the
relaxation lineshapes.
2. Crystal structure and experimental details.
-In the orthoaluminate lattice, space group D§f Pbnm,
the trivalent Rare Earth ions occupy sites with Cs symmetry. For all the Rare Earth ions considered,
one of the local principal directions of the g-tensor lies along the crystal c axis, the other two lying in
the ab plane. The exact directions in this ab plane depend on the particular Rare Earth ion but are
generally in the neighbourhood of + and - 30°
relative to the crystal a and b directions, the two signs corresponding to the two differently oriented sites which are related by a mirror reflection. For yb3 + the local z-axis (Ising like axis) lies at directions
near + and - 300 from a crystal a axis. For the other Rare Earth ions the directions of the principal
axes in the ab plane, as obtained from Magnetic Structure, Electron Paramagnetic Resonance or Opti-
cal Zeeman studies will be given in the appropriate
sections below. A summary of these properties is given in the table.
The Môssbauer absorption results were obtained
on polycrystalline samples substituted with enriched 17°Yb at concentration levels Yb/Host Rare
Earth - 0.025. Lower levels were not feasible as the
absorption signals became too weak.
3. Results and discussion.
-As mentioned in the introduction, the results are presented in three groups
. corresponding to the three different families of Yb3 + relaxation rates observed in the temperature range where the dominant interaction is spin-spin coupling.
These groups in turn correspond to where the host lattice ion is non magnetic (section 3. 1), magnetic
with low anisotropy (section 3.2) and magnetic
with high anisotropy (section 3.3).
For each of the different hosts in turn the various results concerning the hyperfine parameters and the influence of magnetic ordering are presented and
discussed. The Yb3 + relaxation results are also
presented in this section however the discussion of the relaxation data is defered to section 4.
Table 1.
-S0l11e characteristics of the orthoaluminate lattices studied. The references to the various data are
giren in the appropriate .sections of the main text.
3.1 Yb3 + IN EuA’03 (AND TmA’03, YAl03).
-This section concerns results for Yb3 + ions substituted into matrices which are truly diamagnetic (YA103)
or behave as if they are diamagnetic (EuA103, TmAI03) at low temperatures due to the presence of well isolated singlet ground states. At sufficiently
low temperatures (below about 30 K) the slow relaxa- tion limit spectrum is visible in each of the three
cases. The results concerning YA103 and TmAl03
have been presented previously [7] and are recalled briefly here in order to relate them to the case of
EuAI03 which forms the main part of this section.
In addition to the Môssbauer measurements, EPR data was obtained for single crystals containing 0.5
and 3.0 % of Yb having natural isotopic abundance.
3.1.1 Parameters at 4.2 K.
-The EPR g-values
of the Yb3 + ion were found to be the same, to within
experimental error, for the two concentrations but could be obtained with better precision in the 0.5 % sample due to the lower linewidths. One of the princi- pal g-values lies along the crystal c-axis, the two
others lying in the ab plane. The values are
ga z b = 6.45 :t 0.01, g;b = 0.6 +0.1 and g’ x = 0.5+0.1.
Any contribution to these values arising from the
second order coupling between the Yb 31 ion and the Zeeman field induced Van Vleck moment on the EU3 1 ions (exchange g-shift) is expected to be lower than
Fig. 1.
-170Yb Môssbauer Absorption for EuAI03 + 2.5 % Yb". 83 % of the total absorption is due to isolated ions giving
a
slow relaxation lineshape (curve A). The remaining 17 % is mainly due to Yb" ions which
arespin-spin coupled to other Yb" ions, giving
alineshape influenced by relaxation (curve B).
The total fit corresponds to the
curveC.
the quoted errors and so can be disregarded. The
dominant value g"’ lies at angles + and - 30.50 1: 0.5 relative to a crystal a axis. This angle is to be compared
with the local anisotropy axes for pure EuAI03,
where one of the principal axes for the Eu3+ ion
was found to lie at angles of + and - 38° from the
a axis in the ab plane [1].
The Môssbauer absorption spectrum at 4.2 K is shown in figure 1. From a previous study of the
influence of Yb3 + ion concentration on the Môssbauer
absorption in the orthoaluminate lattice [7] we expect that for a concentration of 2.5 % Yb as used then
near 90 % of the Yb3 + ions present will not interact with other Yb3 + ions and will show the slow relaxation limit spectrum whereas the remaining 10 % will be spin-spin coupled to Yb neighbours giving an absorp-
tion lineshape influenced by relaxation effects. The fits to the data show that 80 to 85 % of the total absorption is associated with isolated Yb3 + ions in
EuAI03. The difference between this value and the value 90 %, can be associated with impurities containing Yb. An X-ray analysis shows in fact that the impurity level is in the neighbourhood of 5 %.
In the ground Kramers doublet of the Yb3 + ions in the C, sites the energy levels of the ’7’oYb I = 2 excited state can be described by the Hamiltonian
where the magnetic hyperfine « tensor » A and the
electric field gradient (EFG) tensor are supposed to
have identical local principal axes, both tensors having
their largest values along the local z axis. This assump- tion stems from the fact that because of symmetry
reasons (mirror plan 1 c), the two tensors will both have the c axis as a principal axis and that the large principal g-value along Oz in the ab plane implies a ground doublet chiefly made up of ± 7/2 ) which in
tum induces a large ionic contribution to the EFG
along this same z-direction.
For the Yb3 + ion, the lowest multiplet J
=7/2
is well separated from the excited J
=5/2 multiplet
so that J remains a good quantum number. In this
case the A and g «tensors» are proportional to
within a few percent and
so that A (MHz)
=266 g.
From the slow relaxation limit spectrum of figure 1 we find that A,,
=25.4 ± 0.3 mm/s (1.72 x 103 MHz)
which corresponds to gZ
=6.50 ± 0.07 in agreement with the EPR result. From the Môssbauer analysis
alone it was not possible to obtain accurate values for
the small hyperfine parameters A x and Ay but these
are available from the EPR data.
Using the absolute magnitudes of the 3 principal
g-values and the normalization condition we can
derive the Yb3 + wave functions if we make the
approximation that the local symmetry has the form
C2v as then the wave function involves only four
constants. (For the actual symmetry present the wave functions would involve eight constants.)
For Yb3+ in EuAI03 we obtain
which compares with Yb3 + in Y AI03 [8]
and compares with Yb3 + in TmAI03 for which the coefficient of 1 ± 7/2 ) is also near 0.935.
The quadrupole splitting parameter x was obtained from the Môssbauer data by blocking the A-values
at their EPR values. In fact two slightly different
values for x are found depending on the signs assumed
for the A-values. If the product of the three A-values is taken to be positive a - 4.1 mm/s (279 MHz)
whereas if the same product is taken to be negative
then a - 3.8 mm/s (258 MHz). Now our measure- ments in the ordered region of Yb3 + in GdAI03 unambiguously show that oc is near 3.85 mm/s (262 MHz) whereas for Yb3 + in TmAl03 (X is unambi- guously near 4.05 mm/s (275 MHz). As EuAI03
has crystallographic parameters which are much closer to those of GdAI03 than to those of TmAI03
it seems that for EuAI03 OC - 3.85 mm/s (262 MHz)
is a more plausible choice. Also favouring this choice
are the calculated values of the dominant 4f part of the quadrupole splitting obtained from the above
wave functions which is 0.4 mm/s higher for both Yb 31 in YAl03 and Yb3 + in TmAI03 than for Yb 31
in EuAl03. In tum these results show that the product
of the 3 principal A (or g) values has a negative sign
in EuAI03.
The parameter 11 is expected to be small following
the highly uniaxial character of the ground doublet.
This is confirmed by the fits of the high temperature almost pure quadrupole spectra. The fits to the slow relaxation spectra at 4.2 K are in fact insensitive to
the value ouf 1.
3.1.2 Phonon induced relaxation and crystal field splittings.
-Above about 35 K the absorption lineshapes show the influence of electronic spin
relaxation effects. These spectra have been fitted to the relaxation lineshape for extreme anisotropy given by equation (79) of reference [9] which involves only
one relaxation parameter W -1. The lineshape expres- sions used strictly apply if only the ground Kramers
doublet of the Yb3 + ion is populated. An experi-
mental verification of this population criterion can
be obtained by following the thermal variation
Fig. 2.
-The quadrupole splitting parameter
xfor Yb’* in
YAI03 (0), TmA103 (e) and EuAI03 (D). With increasing tempe-
rature
ain EuAI03 falls
morerapidly than in YA103 and TmA103.
of the quadrupole parameter. Namely, if this para- meter varies as a function of temperature then states other than the ground doublet are populated in the
considered temperature range. However we make here what seems to be a reasonable approximation
that even in the range where the quadrupole splitting parameter varies slightly with temperature the same
lineshape expressions can be used. We thus obtain both the relaxation rate W and the quadrupole splitting x as functions of temperature. The quadru- pole splitting results together with those for Yb3 +
in YAl03 and Yb 31 in TmAI03 are given in figure 2
and the relaxation data in figure 3. Both figures
Fig. 3.
-Electronic relaxation rates for Yb3+ in Y A 10
3(0), TmAI03 (8) and EuA103 (0)
as afunction of temperature. The results for YAI03 and TmAI03 have been decomposed into Raman
and Orbach contributions
asshown by the lines.
show differences between the results for Yb" in
EuAI03 and those for Yb 31 in Y Al03 or in TmAI03.
For YAl03 and TmAI03 the quadrupole splitting
remains constant up to about 70 K whereas for
EuAI03 it begins to drop at much lower temperatures.
As the lattice contribution to the electric field gradient
is small and almost temperature independent, the
decrease of the quadrupole splitting with increasing temperatures for EuAI03 arises chiefly from the 4f electron contribution. Despite the large error bars
this clearly shows that Yb3 + states other than ground
state are significantly populated at temperatures where the phonon driven relaxation begins to modify
the Môssbauer lineshape.
Thus in EuAI03 the excited Yb3 + levels are at lower energies than in YAI03 and TmAI03. This
in tum suggests that the fitted values for W in Yb3 +
in EuAI03 towards the higher temperatures examined where the Yb 3 ’ excited levels are appreciably popu- lated are in fact not exact. This interpretation is supported by the observation that the relaxation data for Yb3 + in EuAI03 cannot be decomposed
into meaningfull Orbach and Raman contributions
as was done for YAl03 and TmAI01.
Yb34- in EuAI03 thus has a slightly less anisotropic ground state and lower lying excited levels than Yb3 + in Y AI03 or TmAI03.
3.2 Yb 3+ IN GdAI03, ErAl03 (AND YbAI03 [7]).
-