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HAL Id: jpa-00228881

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Submitted on 1 Jan 1988

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EFFECT OF A FIELD ON THE

THERMODYNAMICS OF THE RANDOMLY DILUTE

1D HEISENBERG FERROMAGNET

A. Rettori, M. Pini

To cite this version:

(2)

JOURNAL DE PHYSIQUE

Colloque C8, Suppl6ment au no 12, Tome 49, decembre 1988

EFFECT OF A

FIELD ON THE THERMODYNAMICS OF THE RANDOMLY

DILUTE

1D

HEISENBERG FERROMAGNET

A. Rettori (I) and M. G . Pini (2)

(I) Istituto di Fisica del17UniversitiL di Siena, 53100 Siena, ed Unit& del GNSM-CISM, 50125 Firenze, Italy (2) Istituto Elettronica Quantistica CNR, 50127 Firenze, Italy

Abstract.

-

The thermodynamics of the dilute 1D Heisenberg ferromagnet in a field is investigated. The quantum free spin-wave theory is used to calculate the specific heat and analytical results are obtained for low temperatures and low concentration of impurities. The bulk, surface and size contributions t o the free energy are evaluated by the classical

transfer matrix method and analytical results for the surface one are given at low and high temperatures.

Impure 1D magnetic systems have ~eceived con- for h = 0. Any thermodynamic property of the dilute siderable interest in recent years [l-lo]. If the non- system is obtained summing over all the segments: e.g. magnetic impurities are distributed randomly, divid- the specific heat per site is C/N = (1

-

c ) ~ CcTC,, ing the chain into non-interacting segments, the free

energy of the dilute system can be evaluated summing

cT

= CK, [(PEK, 12) cosech (PEK, /2)12

.

(4)

In the quantum case, the Si are spin operators. At low temperatures one can transform to Bose operators and diagonalize the quadratic Hamiltonian [2, 81. In this free spin-wave theory the free energy of a segment with T

2

2 spins is (KB= 1,

P

= 1/T, j = J S ~ , h =

~ ~ B H S ) :

over all the segments: F = ~ T ~ F T ( r = 17%

...,

N) In figure 1 we report the numerical results for the tem- weighted by their probability of occurrence PT = perature dependence of C/N. At very low and c + 1,

N (1

-

c ) ~ cT, where N is the total number of sites and c the concentration of magnetic ones. For high c, the

1

Fig. 1. - Quantum free spin-wave contribution to the spe- cific heat per site of the dilute Heisenberg FM versus T* =

T / J S for c = 0.9. Full line: h = 0; dashed-double-dotted:

h = 0.5; dashea-dotted: h = 1. Insert: comparison with analytical expression (5a, b) (full lines).

classical Heisenberg model was found to explain the zero-field properties of the real quasi-lD compound

it can be evaluated in closed form using the method of steepest descents [2, 41.

c=O 9

C/N = exp (-PhlS) { A -t

(CD3),NMnCCul-,CIS [8-91, but not those of high-

-

- .

dilution samples of CsMn,Mg,-,Br3 [lo], for which quantum effects dominate.

In this paper we study the effect of a magnetic field

on the thermodynamic properties of the dilute 1D

5

/

U

Heisenberg ferromagnet (FM). We consider both the quantum case at low temperatures and the classical

one, for a single segment with T spins the Hamiltonian o o I

is ( J

>

0) :

0 1 2

where EK, are the energies of the harmonic modes

+B ( T ~ / T ) ~ / ~ exp (-To/T)lI3

K T =7rp,,.;p=O,1

,...,

T - 1 ) : x [I+ 2 ( ~ o / x ) ~ (h/j)2

+

( T O / X ) ~ (h/jI4]

)

( 5 4 EK,/JS = 2 (1

-

cos KT)

+

(h/j) (3)

In order t o ensure the convergency of F,, any zero- B = 27r1I2 (1

-

c ) ~

/

(27

In

(l/c))

,

energy mode must be excluded from the summation in To = (2714) x2 ln2 (llc) (j/S)

.

(2). This implies that for a segment of length T one (5b)

has t o sum over T modes for h

#

0, i.e. one more than TO = [27r2/1n (llc) ( ~ j l ~ ) ] 'I3

(3)

C8 - 1418 JOURNAL DE PHYSIQUE

In the classical spin approximation, the transfer ma- trix method [6, 7, ll] can be applied to calculate the partition function of a segment of length r :

where

An are the eigenvalues of the transfer integral

equation. For the Heisenderg chain [ll], y5, (2) are the eigenfunctions and

We devote particular care to the separation of bulk (B), surface (SF) and size (SZ) effects on the free en- 'ergy of the dilute chain.

Analytical expressions for the surface contribution f s ~ can be obtained using for Xo the low and high expan- sions and for a$ :

x [(sinh (a

+

ph/2))

/

(a

+

ph/2)I2

.

(9) The latter is obtained using for the lowest eigenfunc- tion the trial form y5T (x) =

A

eux [ll]. Analytic ap- proximations for a in the low and high T limits are:

where L (2) is the Langevin function

The finite-size contribution to the free energy has to be calculated numerically. Note that fsz= 0 for h = 0

since an+ = 0 owing t o the symmetry of the eigen- functions.

In figure 2 we report the different contributions to the susceptibility as a function of temperature for c = 0.9. For this high value of c, the three contributions are of the same order. The more rapid increase of X S F with

respect t o X B at low

T

is due t o the greater freedom

Fig. 2.

-

Full lines: ciassical transfer mittrix results for the total (T), bulk (B), surface (SF) and size (SZ) contribu- tions to the susceptibility per site verstis T* = T / J S ~ for

j = 1, h = 0.01 and c = 0.9. Dashed lines: low and high temperature expansions (Eq. (lla, b)) for X S F .

in the fluctuations of the surface spins. The low and. high T expansions for X S F

correctly reproduce the numerical da-ta. The size con- tribution Xsz presents a behaviour si.milar to that ob- served for the dilute classical planar model in a field

[GI.

[l] Thorpe, M. F., J. Phys. 36 (1975) 1177.

[2] Mc Gurn, A. R. and Thorpe, M. F., J. Phys. C 16

(1983) 1255.

[3] Maccio, M., Rettori, A. and Pini, M. G., Phys. Rev. B 31 (1985) 4183.

[4] Maccio, M., Rettori, A. and Pini, M. G., Phys. Rev. Lett. 55 (1985) 1630.

[5] Hu, G. Q. and Mc Gurn, A. R., Phys. Rev. B 34

(1986) 7836.

[6] Pini, M. G. and Rettori, A., Pf,bys. Lett. A 127

(1988) 70.

[7] Dong, X. Y. and Mc Gurn, A. R., J. Phys. C 21

(1988) 1571.

[8] Endoh, Y., Heilmann, I. U., Birgeneau, R. J., Shi- rane, G., Mc Gurn, A. R. and Thorpe, M. F., Phys. Rev. B 23 (1981) 4582.

[9] Boucher, J. P., Mezei, F., Reginault, L. T. and Renard, J. P., Phys. Rev. Lett. 55 (1985) 1778, 2370 (E).

[lo] Folk, U., Furrer, A., Furer, N., Oiidel, H. U. and Kjems, J. K., Phys. Rev. B 35 (1987) 4893. [Ill Blume, M., Heller, P. and Lurie, 13. A., Phys. Rev.

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