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HAL Id: jpa-00218974

https://hal.archives-ouvertes.fr/jpa-00218974

Submitted on 1 Jan 1979

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The specific heat of TbPd3 and ErPd3 at low temperatures

J.M. Machado da Silva

To cite this version:

J.M. Machado da Silva. The specific heat of TbPd3 and ErPd3 at low temperatures. Journal de

Physique Colloques, 1979, 40 (C5), pp.C5-152-C5-153. �10.1051/jphyscol:1979557�. �jpa-00218974�

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JOURNAL DE PHYSIQUE Colloque C5, supplément au n° 5, Tome 40, Mai 1979, page C5-152

The specific heat of TbPd 3 and ErPd 3 at low temperatures

J. M. Machado da Silva (*)

Clarendon Laboratory, Oxford, England

Résumé. — Nous avons mesuré les chaleurs spécifiques de TbPd

3

et de ErPd

3

de 2,1 à 8,6 K et de 0,2 à 0,9 K respectivement. La chaleur spécifique de TbPd

3

présente un pic au voisinage de la température 3,75 K. La cha- leur spécifique du ErPd

3

ressemble à une anomalie de Schottky avec un maximum C

v

/R ~ 0,74 qui apparaît aux environs de la température 0,75 K.

Abstract. — The specific heats of TbPd

3

and ErPd

3

have been measured from 2.1 to 8.6 K and from 0.2 to 0.9 K respectively. The specific heat of TbPd

3

shows a magnetic ordering with a typical X shape at 3.75 K. The specific heat of ErPd

3

resembles a Schottky anomaly with a maximum at about 0.75 K with C

v

/R ~ 0.74.

In the REM

3

phases the strength of the exchange interaction, as shown by the transition temperatures, varies widely. The magnitude of the crystal field shows also substantial variations due to the different charge on the M ion. The symmetry of the crystal field is cubic and its effect can therefore be calculated from the results of Lea et al. [1]. We attempt here to calculate the energy levels of the low lying states for the TbPd

3

and ErPd

3

compounds.

The calorimeter where the experiments were per- formed, as well as the method of measurement, have been described elsewhere [2].

The samples used in the measurements were pre- pared by I. R. Harris [3] by arc melting stoichiometric quantities of the pure metals in an argon atmosphere.

The heat capacity of TbPd

3

(figure 1) clearly shows a magnetic transition with a typical X shape at 3.75 K.

The heat capacity up to 8.6 K is always larger than that of LaPd

3

[4] (figure 1), revealing that above 3.75 K there is a contribution from the exchange interaction and from the crystal field. We expect that above 5 K the contribution to the heat capacity due to the exchange interaction is negligible and that the extra heat capacity above the heat capacity of LaPd

3

must be explained in terms of the crystal field splittings.

A point charge model calculation with Z

T b

= 3, Z

Pd

= 0 predicts that a non-magnetic doublet ( r

3

) will be the ground state with a triplet OT^) at 2.2 K, and a singlet (r

2

) at 9 K. The other excited states, having much higher energy, need not be considered in the temperature range of this measurement. In the absence of an exchange interaction a Schottky ano- maly would occur, and considering simply the two lowest states, (C

v

AR)

m3X

will be ~ 0.61 and r

m a x

~ 0.87 K. Comparing these values with the

(*) Present address : Centre de Fisica, University of Porto, Portugal.

1 r - i — i n 1 1 P 1 1

C

v

/R I C

v

/R

a- - 08

7 - \ -07

" Ink.

5 - / X - 05

>• I J - - •»

2 - / 7 - 0 2

? - / / I ^ - < o ,

/' ,** **•*•

U

TOO

" - - ' I - . 1 T I I I '

0 1 2 3 4 5 6 7 8 9 10 Fig. 1. — The heat capacity of TbPd

3

. • lhs y axis, o rhs y axis.

Schottky anomaly for a 0, 8, 60 K crystalline energy levels + lattice heat capacity of LaPd

3

.

results above 5 K, we conclude that the point charge model predictions must be rejected. A fitting of the Schottky type above 5 K is very sensitive to the two low lying states and we can only achieve a good fit if T

3

is the ground state and the energy of r

(51}

is 8 + 0.5 K. Some uncertainty about the energy of f

2

remains because the lattice heat capacity is not accurately known. If we assume that the lattice heat capacity of TbPd

3

is the same as that of LaPd

3

, the energy of T

2

will be 60 + 10 K : however a value of 33 ± 5 K for F

2

will give a good fit provided a lattice heat capacity similar to that of PrPd

3

[4] is adopted.

The inelastic neutron scattering results on TbPd

3

[5]

exhibit a transition peak at ~ 6 meV. This might well suggest that the energy of r

2

is indeed ~ 60 K as predicted above.

The magnetic ordering of TbPd

3

raises the question whether the exchange energy is sufficient to cause the

Article published online by EDP Sciences and available at http://dx.doi.org/10.1051/jphyscol:1979557

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THE SPECIFIC HEAT OF TbPd3 AND ErPd, AT LOW TEMPERATURES C5-153

states r, and Ti') to cross or it merely induces a moment in the T3 state through its second order term.

The crystal field energies suggest that the second possibility is the likely answer.

Calculations of the energies of the levels T, and r i l l , within a molecular field model, show that for the direction ( 100 ) no magnetic field will make these levels cross, and that r, magnetises in second order due to the mixing in the ( 100 ) direction. In the ( 1 1 1 ) direction the r, state remains degenerate to second order and again the exchange field cannot cause r , and ril) to cross: thus we deduce [ti] that ordering will occur in the ( 100 ) direction from the

r, state.

The specific heat of ErPd, from 0.2 to 0.9 K (figure 2) resembles a Schottky anomaly with a maximum CvIR - 0.74 at about T,,, = 0.75 K , revealing that magnetic ordering does not occur in ErPd, above 0.2 K. We can therefore use the point charge model to interpret the experimental results. If we take Z,, = 3, Z,, = 0, the point charge model predicts that a magnetic doublet T6 will be the ground state with the four-fold degenerate level rh3) at 0.9 K and the doublet T, at 17 K. The two four-fold degenerate levels

ri2) and rhl) have energies still higher than T,. It can be seen from the energy level diagram [l] that r?)

and r6 cross at x - 0.85, where x is one of the para- meters of the crystal field.

We compare the observed data with the predictions for a two level system, with gllgo = 2, where g, and go are the degeneracies of ri3) and T6 respectively. We obtain (CV/R),,, = 0.74, which agrees reasonably well with the experiments. This indicates that T, is the ground state, since if rA3) and T6 had crossed, g,!g, would be 0.5 and (CV!R),,, would become 0.24, which would have been too small. On the other hand from T,,, = 0.75 K we can derive a value of 2.0 K for the energy of the ri3) state.

The agreement between the experimental and theoretical values (figure 2) is reasonable above 0.35 K, especially as the experimental points show a lot of scatter above 0.7 K. Below 0.35 K there is a significant

Fig. 2. - The heat capacity of ErPd,. - - - - Schottky curve for

gl/gO =

2 and E(ri3)) - E(r,)

=

2.0 K.

deviation from the theoretical curve. This additional contribution to the heat capacity could well be asso- ciated with the short range interactions present above a magnetic ordering temperature.

Values of x - - 0.8 and of the second crystal field parameter [I] W - 0.65 K for TbPd,, and of x - 0.9

and W - 0.12 K for ErPd,, would be compatible with our experimental results. In both TbPd, and ErPd,, the reduced fourth-order crystal field para- meter B4 as/( r4 ) fi [5] is - 0.30 f 0.05 peV.cm.

Here a is the lattice constant [3], B4 = W . x , fi is a reduced matrix element [7] and ( r4 ) is a relativistic radial function tabulated by Lewis [8]. The value of this parameter in TbPd, and ErPd, agree quite well with those in PrPd,, NdPd, [5] and YbPd, [5,9] suggesting, as pointed out by Furrer et al. [5], that the reduced fourth-order parameter (together with the less reliable reduced sixth-order parameter), can be used to esti- mate the crystal field splittings in the REPd, com- pounds.

We are grateful for the help of Drs. R. W. Hill, W. E. Gardner and I. R. Harris. This research was supported by a grant from the S.R.C.

References

[I] LEA, K. R., LEASK, M. J. M. and WOLF, W. P., J. Phys. Chem. [6] TRAMMELL, G. T., Phys. Rev. 131 (1963) 932.

Solids 23 (1962) 1381. [q STEVENS, K. W. H., PYOC. Phys. Soc. A 65 (1952) 209.

[2] MACHADO

DA

SILVA, . I M., MCDERMOTT, . J. M. and HILL, R. W., [8] LEWIS, W. B., Proc. XVIth Congress Ampere, Bucharest 1970,

J . Phys. C 5 (1972) 1573. ed. I. Ursu (Publishing House of the Academy of Romania,

[3] GARDNER, W. E., PENFOLD, J., SMITH, T. F. and HARRIS, I. R., Bucharest).

J. Phys. P 2 (1972) 133. [9] NOWIK, I., DUNLAP, B. D. and KALVIUS, C. M., Phys. Rev. B 6 [4] MACHAW

DA

SILVA, J. M., submitted to Solid State Commun. (1972) 1048.

[5] FURRER, A. and PURWINS, H.-G., J. Phys. C 9 (1976) 1491.

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