HAL Id: jpa-00210292
https://hal.archives-ouvertes.fr/jpa-00210292
Submitted on 1 Jan 1986
HAL is a multi-disciplinary open access archive for the deposit and dissemination of sci- entific research documents, whether they are pub- lished or not. The documents may come from teaching and research institutions in France or abroad, or from public or private research centers.
L’archive ouverte pluridisciplinaire HAL, est destinée au dépôt et à la diffusion de documents scientifiques de niveau recherche, publiés ou non, émanant des établissements d’enseignement et de recherche français ou étrangers, des laboratoires publics ou privés.
Zero temperature magnetization of the random axis chain
B. Derrida, A. Zippelius
To cite this version:
B. Derrida, A. Zippelius. Zero temperature magnetization of the random axis chain. Journal de
Physique, 1986, 47 (6), pp.955-958. �10.1051/jphys:01986004706095500�. �jpa-00210292�
Zero temperature magnetization of the random axis chain
B. Derrida
Service de
Physique Théorique,
CENSaclay,
91191 Gif surYvette,
Franceand A. Zippelius
Institut für
Festkörperforschung der Kernforschungsanlage Jülich,
Postfach1913,
5170Jülich,
F.R.G.(Reçu
le 12dgcembre 1985, accepté
le 5février 1986)
Résumé. 2014 Nous
calculons
l’aimantation àtempérature
nulle du modèle d’axesaléatoires
à une dimension dans la limite d’une forteanisotropie
et d’unfaible champ magnétique
h. Pour unedistribution
uniforme des axesaléa- toires,
nousobtenons m
=Ch1/03B4
oùl’exposant critique
03B4 = 3 comme pour un verre despin d’Ising à
unedimension
avec une
distribution gaussienne
des interactions.Abstract. 2014 We have
calculated
the zerotemperature magnetization
of the random axischain
in the limitof strong anisotropy
andsmall magnetic
field h. For the uniform distribution of random axes weobtain m
=Ch1/03B4
withthe
same critical
exponent
03B4 = 3 as in the onedimensional Ising spinglass
with a Gaussiandistribution
ofbonds.
Classification Physics
Abstracts75.10201375.30K201375.30G201375.40D
The random anisotropy axis model (RAM)
wasintroduced by Harris et al. [ 1]
todescribe amorphous
intermetallic compounds. The possibility of both
-
ferromagnetic and spinglass like behaviour
-has stimulated much theoretical work. In the
meanfield limit the model is always ferromagnetic [2],
no matterhow strong the random anisotropy. Below four dimensions the ferromagnetic order is destroyed,
ascan
be shown with
adomain wall argument [3]
aswell
aswith
arenormalization group analysis [4].
Whether
or notthe model has
aspinglass phase is
still
a matterof controversy. Furthermore, if
aspin- glass phase exists, it is
notclear whether its critical
properties
arerelated
tothose of the
more conven-tional spinglass model of Edwards and Anderson [5].
Recently Bray and Moore [6] have studied the RAM numerically in
twodimensions, using
alarge
cell renormalization group method. They interpret
their results in
termsof
a zerotemperature phase
transition in the universality class of the Ising spin- glass.
The RAM in
onedimension and
zeroapplied field
has been considered by Thomas [7], who showed
that the ground
stateis nonferromagnetic. He also
discussed the effect of
amagnetic field in
termsof
domain wall argument : weak bonds of strength I Jij I Jo divide the chain into segments of length
L - 1/Jo. A magnetic field h
canflip the magnetic
moment
of such
asegment M L ’" J L, provided the
energy gain ML h compensates the bond energy Jo.
This yields m
=ML/L
=Ch1/3’.
In this
note wepresent
an exactcalculation of the
zero
temperature magnetization for the random axis chain (RAC). The result agrees with the domain wall argument of Thomas and furthermore yields
anexplicit expression for the amplitude C.
The RAM is defined by the Hamiltonian
for d component spins S, of fixed length Si - Si = 1.
Nearest neighbours
arecoupled by
auniform exchange
interaction J
>0. The direction ni (0; = 1) of the
local anisotropy varies randomly from site
tosite, whereas the strength of the anisotropy D and the applied magnetic field H
arethe
samefor all sites.
We restrict
ourdiscussion
tothe
caseof large aniso-
tropy, D >> J and D > I H 1, such that the spins point
either parallel
orantiparallel
tothe local axis ni
In
termsof these
newvariables the Hamiltonian
Article published online by EDP Sciences and available at http://dx.doi.org/10.1051/jphys:01986004706095500
956
reduces
to anIsing model
with random bonds Jij
=J(ni - OJ) and random fields
H; = (H - ni). Note that the fluctuations in the bonds and in the fields
arecorrelated.
We have calculated the groundstate energy of the model (3) in the limit of small magnetic field. Our method of calculation is
ageneralization
tothe RAC
of
amethod already used for the onedimensional
spinglass [8]. Hence
wekeep
ourdiscussion brief and refer the reader
toreference [8] for any details.
One first derives
arecursion relation for the ground-
state
energy of
achain with L spins. If the spin UL
= +1(UL
= -1) then its groundstate energy is denoted
by - FL(- GL). These quantities obey the following coupled recursion relations
with
A single, closed equation is obtained for the diffe-
rence
2 CL
=(GL - FL)IJ
CL remains finite
asL -+
ooand obeys
astationary probability distribution P(CL, nL) which depends
onthe local random axis nL. It satisfies the integral equation :
with h
=H/J.
Here
wehave assumed that the ni
areindependent variables, which all have the
samedistribution p(n).
Once the distribution P(C, n) is known,
one cancal- culate the groundstate energy - E, via
where the average ... > is taken
over n,n’ and C’.
In this section
wepresent the solution of the integral equation for P(C, n). As
afirst step
webreak up the
integration
overC’ and work
outthe various contributions explicitly :
To solve this equation, it is useful
tolook
atthe
momentsof the distribution function
In the following
wespecialize
tothe isotropic distribution p(n) and consider the limit of
aweak magnetic field only. In that
casethe angular dependence of the integral kernel (9) allows
one toderive
aclosed
setof equa- tions for the low order
moments.For
zeromagnetic field
onehas the solution Qo(C, h
=0)
=ð(C). For fmite
but small magnetic field
weexpect Qo(C, h)
tobe concentrated in
asmall region around C
=0. We multiply
equation (9) by (h - n)m, integrate
over nand expand for small C. The first three equation (m
=0, 1, 2) read :
with
Let
uslook for
asolution which has the following properties :
a) Qo and Q2
areeven in C and Ql is odd in C.
b) For small C and h, Qm(C, h) have
ascaling form
We shall
usethis
ansatz tosimplify the equations and
then show explicitly that this
ansatzdoes indeed solve the equations.
To leading order in C and h equations (12, 13) imply
and
Therefore
our ansatzis only consistent if
wechoose
and
With these results, equation (11) reads
where
Hence
one musthave
With the substitution
we can
reduce equation (18)
to anordinary differential
equation
This equation is solved by
with
and K 1/3
aBessel function.
The groundstate energy is
aweighted integral of the stationary probability distribution (Eq. (8)). In par-
ticular for the isotropic distribution p(n), it is given by
For small h
wehave
seen,that P(C, n) is concentrated in
asmall region around C
=0. Hence
we canexpand
around C
=0 and obtain
This integral
canbe further transformed with help of
958
the substitutions
asdefined above
We differentiate with respect
toH,
toobtain
ourfinal result for the magnetization
where Ad is given in equation (14). This implies
m =
0.9050 (H/J)1/3 for xy spins (d
=2) and
m ‘
0.6123 (H/J)1/3 for Heisenberg spins (d
=3).
To conclude : the
exactcalculation agrees with the result
- m =Chl/3
-of
adomain wall argument
and explicitely yields the amplitude C. The critical exponent 6 is the
same asfor the onedimensional
Ising spin glass with
a nonzeroprobability of
zerobonds [8]. A domain wall argument exists also for the Ising spin glass [9] with
anarbitrary distribution of bonds. In that
casethe exponent 6
wasshown
todepend
onthe density of bonds
atJij
=0 [8, 9]. It
would certainly be interesting
togeneralize
ourcal-
culation for the RAC
to anarbitrary distribution of random
axes[10]. Our method of solution, using the
moments
Qm of the distribution function P(C, n),
relies
onthe isotropy of p(n). So far
wehave
notbeen
able
togeneralize it
to anarbitrary distribution p(n).
Acknowledgments.
One of
us(A.Z.) would like
tothank P. Rujan for
avery useful discussion and the CEN Saclay for its hospitality.
References
[1] HARRIS, R., PLISCHKE,
M. andZUCKERMANN, M., Phys.
Rev. Lett. 31(1973)
160.[2] DERRIDA,
B. andVANNIMENUS, J.,
J.Phys.
C 13(1980)
3261.
[3] JAYAPRAKASH,
C. andKIRKPATRICK, S., Phys.
Rev. B 21(1980)
4072.[4] AHARONY, A., Phys.
Rev. B 12(1975)
1038.[5] EDWARDS,
S. F. andANDERSON,
P.W.,
J.Phys.
F 5(1975)
1965.[6] BRAY,
A. andMOORE, M.,
J.Phys.
C 18(1985)
L139.[7] THOMAS, H.,
inOrdering
inStrongly Fluctuating
Con-densed Matter
Systems,
Ed. T. Riste(Plenum,
New
York)
1980.[8] GARDNER,
E. andDERRIDA, B.,
J. Stat.Phys.
39(1985)
367.