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Sign change of the c.e.f. parameters in light rare earth compounds in relation with the delocalization of the 4f
shell
P. Lethuillier, J. Chaussy
To cite this version:
P. Lethuillier, J. Chaussy. Sign change of the c.e.f. parameters in light rare earth compounds in relation with the delocalization of the 4f shell. Journal de Physique, 1976, 37 (2), pp.123-127.
�10.1051/jphys:01976003702012300�. �jpa-00208394�
SIGN CHANGE OF THE C.E.F. PARAMETERS IN LIGHT
RARE EARTH COMPOUNDS IN RELATION WITH THE DELOCALIZATION
OF THE 4F SHELL
P. LETHUILLIER
(*)
Laboratoire de
Magnétisme
and J. CHAUSSY
Centre de
Recherches sur les Très BassesTempératures
C.N.R.S.,
BP166,
38042 GrenobleCedex,
France(Reçu
le 10septembre
1975,accepté
le 7 octobre1975)
Résumé. - Le schéma des niveaux de
champ
cristallin decomposés intermétalliques
RX3 (R = Ce, Pr, Nd ; X = In, Pb) a été déterminé par des mesures de susceptibilité et de chaleurspécifique ;
uneexpérience
de diffusioninélastique
de neutrons a été réalisée pour NdIn3. Le para- mètre dechamp
cristallinA04 r4 >
des composés du cérium est positif ; il décroît pour lescomposés
du
praséodyme
et devient négatif pour lescomposés
du néodyme. Leparamètre
dechamp
cristallinA06 r6 >
présente une variation similaire dupraséodyme
aunéodyme.
Cechangement
de signedes paramètres de champ cristallin semble être relié à la faible différence
d’énergie
entre la bandede conduction et les niveaux 4f au début de la
première
série des terres rares.Abstract. 2014 The
crystal
field level scheme of RX3 (R = Ce, Pr, Nd ; X = In, Pb) intermetalliccompounds
has been determined byfitting susceptibility
curves andspecific
heatSchottky
anomalies ;an inelastic neutron diffraction experiment has been
performed
for NdIn3. The fourth order C. E. F.parameter
A04 r4 >
of the cériumcompounds
is positive ; it decreases for thepraseodymium compounds
and becomes negative for theneodymium compounds.
The sixth order C. E. F. para- meterA06 r6 >
exhibits the same trend to negative values frompraseodymium
toneodymium
compounds. Thissign change
of the C. E. F. parameters appears to be related to the small energy difference between the conduction band and the 4f levels at thebeginning
of the first rare earth series.Classification
Physics Abstracts
8.512
1. Introduction. 2014 The
compounds
R(Sn, Pb, In, Tl, Pd)3,
where R is a rareearth,
have the cubicAuCu3 type-structure. They
have beenextensively
studied[1
to11].
It isinteresting
to determine thecrystal
field parameters of these
compounds
so as to under-stand their
physical properties (such
as the super-conducting
transition temperature ofLa1-yPryX3
solutions
[12]
or the electricalresistivity [13])
and alsoin order to understand the interaction between the 4f electrons and the conduction band. These parameters have been
mainly
determinedby
theanalysis
ofsusceptibility
andspecific
heat measurements.In these
compounds,
the rare earth is situated on asite with cubic
symmetry.
Thecrystalline
electric field(C.E.F.) splits
theground multiplet
of the rare earthion and the level scheme is described
by
two C.E.F.parameters
A04 r4>
andA06 r6>
orsimilarly, following
Lea et al.[14], by W and
x.The
magnetic susceptibility
of this ion is thengiven by
the formula :where n is the molecular field coefficient and ~C.F.
is the
crystal
fieldsusceptibility :
| i ~ and |j ~
are theeigen
functions of the hamiltonian defined in reference[14]
and theenergies Ei
are theeigen
values.(*) This work is a part of the thesis of P. Lethuillier.
Article published online by EDP Sciences and available at http://dx.doi.org/10.1051/jphys:01976003702012300
124
The
Schottky-type specific
heat isgiven by
theformula :
where f
is thedegeneracy
of the level of energyE1.
2.
Experimental.
- Thesusceptibility
measure-ments have been
performed
in amagnetic
field of1.7 k0152 between 2 and 300 K. The error bars are
± 0.2 K on the temperature in the whole range; the
precision
on themagnetic susceptibility
is one per cent with a minimum error of ± 0.3 xl0-4 e.m.u./mole.
All these
compounds
meltcongruently.
Asthey
oxidize
rapidly,
thesamples
are stored under vacuum.3. Results. - The Neel and
paramagnetic
Curietemperatures
and theparamagnetic
moments of thesecompounds
aregiven
in the table I.TABLE I
Neel
and paramagnetic
Curie temperaturesparamagnetic
momentsof RX3 compounds
3.1
CePb3 (Fig. 1 ). - In
thehigh
temperatureregion,
thesusceptibility
follows a Curie-Weiss beha- viour with aparamagnetic
moment very close to the trivalent ion value. Under 30K,
thereciprocal susceptibility
is notlinear;
at 4.2K,
theCurie-constant
is C N 0.36 instead of C = 0.805 for the free ion. The Curie constantcorresponding
to the isolated doublet is C = 0.19 and C = 0.49 for the quartet. We have fitted theexperimental
data with the formula(1).
Unambiguously,
the doublet is the lowest level. The best agreement is obtained with W = 11K,
x = 1.0 and n = 18 e.m.u. The fourth order term is thenpositive : A’ r’ >
= 29 K.3.2
PrPb3 (Fig. 2).
- Thiscompound
is a VanVleck paramagnet
[5, 6], [9].
Thespecific
heat curveof PrPb3
exhibits a lambdatype anomaly
at 0.35 K[6]
which indicates a transition from
antiferromagnetism
to
paramagnetism.
Theentropy
under the lambdaanomaly
is aboutRLn2 showing
that theground
stateis the
non-magnetic
doubletF3-
Moreover it wasFIG. 1. - Reciprocal susceptibility of CePb3 versus temperature.
found
possible
to fit theSchottky anomaly
of thecompound Lao.gPro.,Pb3 [2] by
the two sets ofparameters
W and x :and
The second solution
gives
asusceptibility
minimum(Fig. 2)
which has not been observed. On the contrary, the first solution leads to a calculatedsusceptibility
curve in
perfect
agreement with theexperimental
data :the fourth order term is then
positive.
A similar
analysis
of the results of Bucher et al.[2]
leads to the
following
C.E.F.parameters,
forPrTl3 :
3.3
PrIn3 (Fig. 3).
- For thiscompound,
the ana-lysis
ofsusceptibility
andspecific
heat measure-ments
[3, 4]
has led to : x = - 0.7± 0.1,
the corres-ponding
value of Wbeing
best determinedby
theT = 0
susceptibility
of this Van Vleckparamagnet.
The Curie constant of this
compound
islarger
thanthe free
tripositive
ionvalue, owing
to the matrix contribution(Table I) ;
theparamagnetic
Curie tem-peratures
of theRIn3 compounds, given
in the tableI,
have been determined with theexperimental
datacorrected for the
susceptibility
ofLaln3
measuredby
Toxen et al.
[15].
The correctedsusceptibility
has beenfitted with the formula
(1).
The bestagreement
is obtained with x = - 0.6 + 0.1(Fig. 3) ;
the corres-ponding
value of W is : W = 2.36 K.FIG. 2 ; - Reciprocal susceptibility of PrPb3 versus temperature.
The insert is an expanded scale of the low temperature data.
FIG. 3. - Reciprocal susceptibility of PrIn3 versus temperature.
3.4
Ndln3 (Fig. 4, 5, 6).
- The determination of the C.E.F. parameters of thiscompound
wasperfor-
med with the use of three different
techniques.
An inelastic neutron diffraction
experiment
wasperformed
on thespectrometer
IN7 of the InstitutLaue-Langevin
at Grenoble. Details on theexperi-
mental
technique
aregiven
in reference[10].
Onespectrum was taken at 12
K,
with an incident neutronenergy of 40
meV ;
thecounting
time was twodays.
A broadened
peak
at 6 meV appears on the neutron energy loss side(Fig. 4).
The width of thispeak
isabout 10 channels whereas the
spectrometer
resolution is seven channels(full
width at halfmaximum).
If werefer to the level scheme
given
in reference[14],
thismeans that the value of x is close to x =
0.37,
where the levelsr 6
andr 8 (1)
cross. With an incident neutronenergy of 10
meV,
a smalltransition, corresponding
toan energy of 0.5
meV,
is visible. Wegive (Fig. 4),
forcomparison,
the spectrum of the isostructural com-pound NdSn3, registered
at 10 K. Theoscillating
FIG. 4. - Neutron time of flight spectra of NdIn3.
background
is due toimperfect
calculator correlations.The first transition can be
explained
with the four sets of parameters :The occurence of the second transition excludes the solutions with W 0.
In order to
verify
thisresult,
we havemeasured,
the heat
capacity
ofNdIN3
andLaIn3.
Between 20and 300
K,
thesamples
used for theexperiment
werecylinders
of about 20 g. Our resultconcerning LaIn3
is in
perfect
agreement withpreviously reported
measurements
[4].
Between 20 and 30K,
thespecific
heat of
NdIn3 slightly
exceeds that ofLaln3 owing
to the
Schottky
contribution(Fig. 5).
Above 30K,
theopposite
behaviour is observed because theDebye
temperature is lower in
LaIn3
than inNdln3.
At 20K,
the difference between the heatcapacities
ofNdln3
and
Laln3
is about 1.5J/mole.K.
TheSchottky-type specific heat,
calculated at this temperature with the formula(2)
for the parameters determinedabove,
is
Cp N
1.7J/mole.K
with W > 0 andCp N
3 withW 0. In this
experiment also,
the agreement is better with W > 0.126
FIG. 5. - Heat capacities of Laln3 and Ndln3 versus temperature.
The insert is an expanded scale of the low temperature data.
FIG. 6. - Reciprocal susceptibilities of NdIn3 and Lao.75 Ndo,zsIn3 (corrected and calculated values).
The
susceptibility
measurements ofNdln3
andLao.7sNdo.2sIn3 (Fig. 6)
confirm thepreceding
results. In
particular,
between 2 and 5K,
the Curieconstant of
Lao.75Ndo.25In3
is C = 1.3 inagreement
with the calculated values with W > 0(with
W0,
the calculated Curie constant would be C =1.1 ).
Only
two sets ofparameters
arepossible, namely :
Thus the fourth and sixth order terms are
negative
as inNdPb3
andNdSn3 (10)-
4. Discussion. - We have
reported
in the table IIthe values of
W, x, A 0 r 4 >
andA6 r’ >
forRX3 compounds (X
=In, Pb, Sn)
taken from references[3, 4], [10]
and[ 11 ]
or determined in this work. InCelni [4], specific
heat measurements have shown that the doublet is the lowest state(A ’ r’ >
> 0 asin
CePb3),
in agreement with our conclusions frommagnetic susceptibility
data. The variation ofA4 ( r4>
andA6 ( r 6 >
withtfie
rare earth ion has beenrepresented
on thefigures
7 and 8 forRX3 compounds (X
=In, Pb, Sn).
The C.E.F. parameters of theheavy
rare earthcompounds RIn3
have beenfound
negative [8]
as those of theneodymium
com-pounds NdX3.
TABLE II
C.E.F. parameters
of
theRX3 compounds
It is well known
that,
for ceriumcompounds,
thedegree
of localization of the 4f shell is smaller than forheavy
rare earthcompounds [16].
Forinstance, CeSn3
becomes
non-magnetic
at lowtemperature [1]
andCeln3
exhibits a Kondo effect[17].
For the praseo-dymium compounds,
there are fewpublished
expe- rimental data. We have shownrecently, by resistivity
measurements
[13],
thatPrSn3
exhibits a Kondoeffect.
Moreover,
theexchange integral
r between the 4f shell and the conductionband,
as determined from thedepression
of thesuperconducting
transition tem-perature,
has been found muchlarger
inLa1-’pryX3
solutions
[2], [11, 12]
than inLal _yGdySn3 [18]. Thus,
we may think that the observed
sign
reversal of theFIG. 7. - Variation of the fourth order C.E.F. parameters of the RX3 compounds with the rare earth ion.
C.E.F.
parameters
is related to the delocalization of the 4f shell at thebeginning
of the rare earth series.Chow
[19]
has shownthat,
in dilutealloys
ofheavy
rare earths in
Ag
andAu,
the 4f-5d interaction leads to anexchange
correction to the direct Coulomb fourth order term, which reaches 85%
of its value and is ofopposite sign.
In ceriumcompounds,
as the 4f shell is not very far from the Fermilevel,
the 4f-5doverlap
may lead to an
exchange
termlarger
than the Cou- lomb term,inducing
thesign change
of the fourth order term. It isinteresting
to observe that the caseof
praseodymium
is intermediate between those of cerium andneodymium (Fig.
7 and8).
FIG. 8. - Variation of the sixth order C.E.F. parameters of the RX3 compounds with the rare earth ion.
Finally,
it is remarkable thatA 4 0 r’ >
andA’ ,6 >
varysimilarly
for the isoelectronic com-pounds RSn3
andRPb3 ;
the variation of the fourth and sixth order terms of theRIn3 compounds
islarger
than that of the
RPb3
andRSn3 compounds.
Acknowledgments.
- We thank Dr. J. Pierre for hishelp
and Dr. E. Bucher forcommunicating unpublished
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