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Crystal fields and magnetic properties of NdSn3, NdPb 3 and Ndin3

P. Lethuillier, J. Pierre, K. Knorr, W. Drexel

To cite this version:

P. Lethuillier, J. Pierre, K. Knorr, W. Drexel. Crystal fields and magnetic properties of NdSn3, NdPb 3 and Ndin3. Journal de Physique, 1975, 36 (4), pp.329-333. �10.1051/jphys:01975003604032900�.

�jpa-00208258�

(2)

CRYSTAL FIELDS AND MAGNETIC PROPERTIES OF NdSn3, NdPb3 AND Ndin3 (*)

P. LETHUILLIER and J. PIERRE

Laboratoire de

Magnétisme, C.N.R.S.,

BP

166,

38042

Grenoble, Cedex,

France and

K. KNORR

(**)

and W. DREXEL Institut Max-von

Laüe-Paul-Langevin,

BP

156,

38042

Grenoble, Cedex,

France

(Reçu

le 9 décembre

1974, accepté

le 23 décembre

1974)

Résumé. 2014 Nous avons réalisé des expériences de diffusion inélastique des neutrons sur les composés intermétalliques

NdPb3

et NdSn3. Nous avons observé des transitions bien résolues entre niveaux de champ cristallin à différentes températures. Deux schémas de champ cristallin

sont possibles pour chaque composé. Des mesures magnétiques et des

expériences

de diffraction

neutronique permettent de lever cette indétermination. Les paramètres de champ cristallin obtenus diffèrent beaucoup des

prévisions

d’un modèle de charges

ponctuelles.

Abstract. 2014 Inelastic neutron scattering experiments have been performed on the intermetallic

compounds NdPb3

and NdSn3. Well resolved transitions between crystal field levels were observed at different temperatures and for each compound, two level schemes were possible. Magnetic measure-

ments and elastic neutron scattering experiments were performed to remove this uncertainty. The

experimental

crystal field parameters deviate considerably from

point charge

estimates.

Classification Physics Abstracts 8.524 - 8.537 - 8.512

1. Introduction. - The cubic

compounds RX3

with

CU3Au

structure between rare earths

(R)

and different metals

(X)

such as

In,

Sn and Pb have been studied from different

points

of view :

magnetic

structure,

crystalline field, superconducting properties

and elec-

tronic structure. In

particular,

a great deal of work has been spent to determine the

crystalline

electric

field

(CEF)

levels : the direction and the values of the ordered moments have been determined in the

RIn3 [1-3]

and the

RSn3 [3] compounds. Schottky

anomalies have been observed and

analyzed

in

specific

heat measurements on

Celn3, Prln3 [4]

and

Lao.9Pro.1Pb3 [5]. Susceptibility

studies have led to the determination of the

ground

state levels

in

praseodymium compounds [6, 7].

However,

the most

straightforward

method to

determine the level scheme is inelastic neutron

scattering.

We have thus undertaken

experiments

on the two

neodymium compounds, NdSn3

and

NdPb3,

which were

complemented by magnetization

measurements in

pulsed fields, susceptibility

and

magnetic

structure determinations. All these

experi-

ments were

performed

with

polycrystalline samples.

(*) This work is part of the thesis of P. Lethuillier.

(**) Present address : Physikalisches Institut, Frankfurt/M, Germany.

2. Neutron

spectroscopy.

- In cubic symmetry, the J =

2 multiplet

of the Nd3+ ion is

split

into

one doublet

r6

and two quartets

T8(1)

and

T8(2).

The level scheme can be described

by

two CEF-

parameters A4 r 4 >

and

A6 r6 >

or

equivalently, following Lea,

Leask and Wolf

[8],

W and x. The

transition

probabilities

are

given by Birgeneau [9].

Inelastic neutron

scattering

is a very direct method for the determination of

crystal

field levels.

Magnetic dipole

transitions between

crystal

field levels occur

with

matching

neutron energy transfers. The

resulting peaks

in the neutron energy spectrum are propor- tional to the square of the

magnetic dipole

matrix

elements and to the thermal

population

of the initial CEF-level.

The inelastic neutron

scattering experiments

were

performed

on the statistical

chopper

time of

flight

spectrometer IN 7 of the Institut

Laüe-Langevin

at Grenoble. An array of 10 detectors was located at

scattering angles

between 150 and 200. Several incident neutron

energies

were

used,

from 10 meV

up to 56 meV. The

samples weighed

about 100 g ;

a

typical counting

time was one

day.

The resolution

of the instrument was seven time of

flight

channels

(full

width at half

maximum).

All spectra were domi- nated

by

the elastic line. The error bars were estimated from the scatter of data

points

between

peaks.

Neutron

Article published online by EDP Sciences and available at http://dx.doi.org/10.1051/jphys:01975003604032900

(3)

330

detected in channels to the left of the elastic

peak gained

energy

by

the de-excitation of upper states,

neutrons

inducing upward

transitions were counted in channels on the

right

hand side.

The first measurement was taken on

NdPb3

at

6,5 K with incident neutrons of 56 meV. A

peak at

10 to 11 meV

appeared

on the neutron energy loss side

(Fig. 1).

A measurement on

LaPb3

at 80 K but

otherwise under the same conditions did not show any structure other than the elastic line. Thus we

explain

the

peak

observed for

NdPb3

as a transition

from the

ground

state to an excited state at about

11 meV. The second spectrum was measured at 120 K in order to observe new transitions from this excited level

(Fig. 1).

The

original peak

was

changed

into a shoulder

indicating

a new, not yet

resolved,

transition in the energy range from about 4 to 9 meV.

Fm. 1. - Neutron time of flight spectra of NdPb3 at 6.5 and 120 K.

The incident energy is E. = 56.0 meV.

A

corresponding

shoulder

appeared

on the de-excita- tion

side,

too. Since this new transition was absent at 6

K,

it must connect the two excited CEF levels of

Nd3+.

To increase the resolution and to ascertain the

transition,

a third spectrum was measured at 51 K with the incident neutron energy lowered to 40.0 meV

(Fig. 2a).

The two transitions were now

FIG. 2. - Neutron time of flight spectra. The incident energy is Eo = 40.0 meV. a) NdPb3 : T = 51 K. b) NdSn3 : T = 10 K.

c) NdSn3 : T = 51 K.

resolved,

with

energies

of

(10.6

±

0.2)

meV and

(7.6

±

0.2)

meV. A

hint

of the reverse transitions can

be seen on the de-excitation side of the spectrum.

The fact that the 7.6 meV transition was

already

visible at 51 K where the level at 10.6 meV is still not

substantially populated

demands a sequence of levels as follows :

We searched for the transition between the

ground

state and the first excited level at 3.0 meV. A spectrum taken at low

temperature

with an incident energy of 14.0 meV did not show more than a

slight

indication

of a

peak

around 3 meV. One has to conclude that the

probability

for this third transition is

significantly

lower than for the other two.

Refering

to the level scheme

given

in ref.

[8]

for

Nd3+,

one finds that five sets of CEF parameters

can

reproduce

the observed

splitting, namely :

(4)

The decision between these cases has to be based on

the transition

probabilities [9]. Quite clearly,

the

solutions

c) d) e)

can be ruled out because

they

demand a very intense transition at 3 meV. The distinction between case

a)

and

b)

is more difficult.

The situation is best described

by

a calculation of the theoretical spectra

[13, 14]

for both cases

(Fig. 3).

Both spectra fit the

experimental

results within the statistical error. There is a small

preference

for case

a),

where the

ground

state is the

r 6

doublet.

FIG. 3. - Theoretical spectra of NdPb3 and NdSn3 at 51 K, with Eo = 40.0 meV.

The results on

NdSn3

are very similar and the

interpretation

follows the same scheme. At 10

K,

an excitation

peak

at 10.2 meV can be observed

(Fig. 2b).

At 51

K,

a broad maximum

ranging

from 7

to 12 meV is visible

(Fig. 2c).

It is

explained by

a

second transition at 8.2 meV of about the same

intensity as

the first one. We conclude that the sequence of levels is 0

meV, (10.2 - 8.2)

= 2

meV,

10.2 meV.

The transition at 2.0 meV could not be detected.

These results exclude all but two sets of CEF para- meters,

namely x = 0.24,

W = 0.123 meV and

x = 0.48,

W = 0.166

meV,

which

again

fit the

experimental

data with about the same

quality (Fig. 3b).

For both

compounds,

the

question

remains

as to whether the sequence of levels is

r 6’ T8(1), rà2)

or

râ1), r 6’ râ2).

In order to remove this

uncertainty,

we

performed magnetic

measurements and elastic neutron diffraction studies.

3.

Magnetic susceptibility (Fig. 4).

- We have

studied the

magnetic susceptibility

of these

compounds using

a translation balance in a

magnetic

field of

7

kOe,

over the temperature range from 1.6 K to 300 K. Above 50

K,

a Curie-Weiss behaviour is observed for both

compounds,

the effective moments

FIG. 4. - Reciprocal susceptibility versus temperature for NdSn3

and NdPb3. The continuous curves have been calculated for respec-

tively : W = 1.43 ; x = 0.24 and W = 1.26 ; x = 0.13.

are in close agreement with that of the free

tripositive

Nd ion.

NdSn3

shows a maximum of the suscep-

tibility

at 4.6

K,

in

good

agreement with Tsuchida and Wallace

[10], indicating

the onset of antiferro-

magnetism ;

this

compound

shows a minimum of the

susceptibility

at 3 K. Below 50

K,

in the

paramagnetic domain,

the

susceptibility

x deviates

slightly

from

Curie-Weiss behaviour.

NdPb3

orders antiferroma-

gnetically

at 2.6 K and as for

NdSn3,

x deviates

slightly

from a Curie-Weiss behaviour at low tempe-

rature. We have calculated the

crystal

field

suscepti- bility

for the three

crystallographic ’axes 100 j, 111 >, 110 >

and found it

weakly anisotropic.

For both

compounds,

the agreement between the calculated and measured values of the

susceptibility

is

good

for the different sets of W and x : it is

slightly

better when

r 6

is the lowest level.

(5)

332

4. Elastic neutron diffraction. - In a

previous study,

we had

performed

a neutron diffraction

experiment

on

NdSn3 [3].

The

magnetic

cell was found

quadratic (a,

a, 2

a)

and the

magnetic

moment, which is in the basal

plane,

reaches 1.5 +

0.311B

at 1.3 K. We

performed

similar work on

NdPb3

at the reactor

Siloe

(Neutron

Diffraction

Laboratory, C.E.N.,

Gre-

noble).

This

compound

has the same

magnetic

struc-

ture as

NdSn3

and the

magnetic

moment reaches

1.4 ±

0.411B

at 1.3 K

[11].

In order to account for these neutron diffraction

results,

we have calculated the

magnetic

moment at 1.3 K. For this purpose we

diagonalize

the Hamiltonian

where the

exchange

field

Hm

is taken from

Jz)

is the thermal average of the

magnetization

and C is the Curie constant at low temperature. The

magnetization

and

ground

state energy are found

by

a self-consistent method. The

anisotropy

energy between the

principal

axes is weak

(AE

1

K)

for

the different sets of W and x. For

NdSn3,

the solution

W = 0.123 meV

(1.43 K),

x = 0.24

(r6 lowest) gives

a moment Il =

1.62,u,

close to the

experimental

value

(1.5

± 0.3

I1B).

The other solution will lead to a moment Il = 2.47 IUB-

For

NdPb3,

Ilexp = 1.4 +

0.4’UB.

The solution W = 0.109 meV

(1.26 K),

x = 0.13

(r6 lowest) gives

a moment p =

1.39 ,uB.

The other solution

gives

a moment Il =

2.26 y/a. Quite clearly,

for both

compounds,

the

r 6

level is lowest and the CEF

parameters

are : for

NdSn3 : W

= 1.43

K ;

x = 0.24 and for

NdPb3 : W

= 1.26

K ; x

= 0.13 .

We

give

the level scheme in

figure

5.

5.

Magnetization

measurements

(Fig. 6).

-

Finally, experiments

on the three

compounds NdIn3, NdPb3

and

NdSn3

were

performed

at 1.35 K in

pulsed

fields

up to 260 kOe in order to overcome the antiferroma-

gnetic exchange

field and

align

the moments. The

samples

are

powders,

and the

eddy

currents do not

significantly perturb

the measurements. The magne- tization of

Ndln3

increases

slowly

and

linearly

above

160

kOe,

where its value is about 1.55 ,uB, close to the moment of the

r 6

level. The

magnetization

of

NdPb3

and

NdSn3

do not saturate. For the three

compounds,

the

magnetization

in the

highest

field

is below

2,uB,

far from the free ion value

(gJ

=

3.27 IUB)’

This is in

qualitative

agreement with the behaviour of a

r 6 ground

level in a field.

FIG. 5. - Crystal field level scheme for NdSn3 and NdPb3’

FIG. 6. - Magnetization curves of Ndln3, NdSn3 and NdPb3.

6. Discussion. - In the

following,

we will

analyze

the CEF parameters for these

neodymium compounds.

In the two isoelectronic

compounds NdSn3

and

NdPb3,

the two parameters

A2 r4 )

and

Ag ( r6 ) keep

the same

negative sign (Table I).

In a

point charge model,

where all the

neighbouring

atoms

are taken into account, the CEF parameters can be written as :

(6)

TABLE 1

CEF parameters determined

experimentally

If we first

analyze

the fourth order term

alone,

the

experimental

values lead to a small or

negative charge

on Sn or

Pb,

if we assume a trivalent rare earth ion

(Table II).

This is in agreement with the

assumptions

of Bucher et al.

[12]

who

analyze

the effective

charges

in relation to

electronegativity. However,

with such

charges,

the calculated sixth order term is smaller than observed

by

one order of

magnitude.

This

excessive value of the sixth order term has been

TABLE II

CEF parameters Ag r4 ), Ag r6 ) (K)

calculated

for NdSn3 from a point charge model, assuming

trivalent

neodymium

and

given charges ZM for

the

Sn atoms.

observed in a number of intermetallic

compounds :

in the cubic Laves

phases TbAl2

and

NdAl2

com-

pounds [13],

in the cubic CsCI

type phases

between

Ho and Er and the different metals

Cu, Ag,

Zn and

Rh

[14, 15]

and in the cubic

AuCu3 type TmAl3 compound [16].

In all these

compounds,

a

point charge model,

where the rare earth has a

positive charge

and the

alloyed

metal has no

charge, gives

the correct

sign

for

A2 ,4)

and

Ag r6 )

but the

calculated order of

magnitude

for

Ag ,6 )

is then

generally

much smaller than the

experimental

value.

Dixon and

Dupree [17, 18] analyze

the results

obtained

by

Williams et al.

[19]

in solid solutions of

heavy

rare earths in a f.c.c. matrix

(Ag, Au) by taking

into account the d- and f-like character of the conduc- tion electrons. In the

LaSn3 compound,

band calcula- tions

[20, 21]

have shown that conduction electrons have a

large

d character in the

vicinity

of the Fermi

level. It is

possible

that the influence of the d-electrons

aspherical

distribution may

explain

the

negative sign

of

A04 r4 >

encountered in

NdSn3

and

NdPb3 ;

the

large

value of

A06 ,6 )

may then arise from an

exchange-type

interaction with the conduction band.

A

peculiar

case is that of some

compounds

with

praseodymium :

in

Prln3 [6], PrSn3

and

PrPb3 [7],

the fourth order term is

positive;

on the contrary,

a

study

of the

magnetic properties

of the

RIn3

com-

pounds

with

heavy

rare earths

[22]

has shown

that,

most

probably,

the

A04 ( r4 >

parameter is

negative,

as in

NdPb3

and

NdSn3.

The case of

Ndln3

is still

uncertain and must await a new determination.

References

[1] ARNOLD, G. and NERESON, N., J. Chem. Phys. 51 (1969) 1495.

[2] NERESON, N. and ARNOLD, G., J. Chem. Phys. 53 (1970) 2818.

[3] LETHUILLIER, P., PIERRE, J., FILLION, G. and BARBARA, B., Phys. Stat. Sol. (a) 15 (1973) 613.

[4] VAN DIEPEN, A. M., CRAIG, R. S. and WALLACE, W. E., J. Phys.

& Chem. Solids 32 (1971) 1867.

[5] BUCHER, E., ANDRES, K., MAITA, J. P. and HULL, G. W., Jr., Helv. Phys. Acta 41 (1968) 723.

[6] BUSCHOW, K. H. J., DE WIJN, H. W., VAN DIEPEN, A. M., J. Chem. Phys. 50 (1969) 137.

[7] LETHUILLIER, P., CHAUSSY, J., To be published.

[8] LEA, K. R., LEASK, M. J. M. and WOLF, W. P., J. Phys. & Chem.

Solids 23 (1962) 1381.

[9] BIRGENEAU, R. J., J. Phys. & Chem. Solids 33 (1972) 59.

[10] TSUCHIDA, T. and WALLACE, W. E., J. Chem. Phys. 43 (1969)

3811.

[11] LETHUILLIER, P., To be published.

[12] BUCHER, E. and MAITA, J. P., Solid State Commun. 13 (1973) 215.

[13] BARBARA, B., ROSSIGNOL, M. F., PURWINS, H. G. and WALKER, E., Phys. Stat. Sol. 22 (1974) 553.

[14] MORIN, P., PIERRE, J., ROSSAT-MIGNOD, J., KNORR, K. and DREXEL, W., Phys. Rev. B 9 (1974) 4932.

[15] CHAMARD-BOIS, R., ROSSAT-MIGNOD, J., KNORR, K. and DREXEL, W., Solid State Commun. 13 (1973) 1549.

[16] DE WIJN, H. W., VAN DIEPEN, A. M. and BUSCHOW, K. H. J., Phys. Rev. B 1 (1970) 4203.

[17] DIXON, J. M., Solid State Commun. 12 (1973) 789.

[18] DIXON, J. M. and DUPREE, R., J. Phys. F 3 (1973) 118.

[19] WILLIAMS, G. and HIRST, L. L., Phys. Rev. B 185 (1969) 407.

[20] GRAY, D. M., MEISEL, L. V., Phys. Rev. B 5 (1972) 1299.

[21] FREEMAN, A. J., KOEHLING, D. D., J. Physique Colloq. 33 (1972) C 3-57.

[22] LETHUILLIER, P., Thesis, University of Grenoble, 1972, unpu- blished.

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