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The homogeneous helimagnet and the liquid-solid transition
J. Villain
To cite this version:
J. Villain. The homogeneous helimagnet and the liquid-solid transition. Journal de Physique, 1973,
34 (2-3), pp.211-216. �10.1051/jphys:01973003402-3021100�. �jpa-00207374�
THE HOMOGENEOUS HELIMAGNET AND THE LIQUID-SOLID TRANSITION
J. VILLAIN
Institut
Laue-Langevin,
Grenoble(Reçu
le 26juin 1972)
Résumé. 2014 On examine la
possibilité
d’une transition avec unesusceptibilité
infinie pour q ~ 0 dans un milieuhomogène.
Dans le cadre d’un modèleprécis (§ 2)
on montre(§ 4)
que seule unefaible
singularité
peut exister, etprobablement
pasd’infinité ;
lasingularité
forteapparait à q
= 0et pour une
quantité qui
n’est pas lasusceptibilité (§ 3).
Onprévoit
un résultatanalogue
dans lecas des
liquides (§
1 et5).
Abstract. 2014 The
possibility
of a transition with an infinitesusceptibility
atnon-vanishing q
in an homogeneous medium is
investigated.
In the frame of aprecise
model(§ 2)
it is shown(§
4)that
only
a weaksingularity
can occur, andprobably
noinfinity ;
the strongsingularity
appears at q = 0 for aquantity
which is not thesusceptibility (§ 3).
A similar result isconjectured
for thecompressibility
ofliquids (§
1 and5).
Classification Physics Abstracts
15.00 - 14.80
1. Introduction. - It has been
suggested [1] ]
that the
pair
correlation function of a metastableliquid might
becomelong
range at sometempera-
ture
TL
where theliquid
becomes unstable. Morerecently,
thedynamical aspect
of thisinstability
was
investigated [2], [3] and,
veryrecently, experiments
were
performed
to check thistheory by measuring
the static and
dynamic scattering
factors of neutrons[4].
S(q)
andS(q, w). S(q)
isexpected
to become infinite atTL
for some value qLof q,
andS(qL, w)
isexpected
to have a
vanishing
width atTL (infinite
De Gennesnarrowing).
Experimentally TL
could not be reached[4],
andpossibly
there are fundamental reasons forthat,
at least for a
simple liquid ;
but we do not wish toconsider this
problem :
weonly
mention[5]
thatsymmetry
does not exclude a second order transition for some well-defined pressure at which the 3rd order terms in thethermodynamic potential
vanishaccidentally.
Ourproblem
is thefollowing :
assumethat
TL
can bereached,
then what is thetype
of thesingularity ?
For T N
TL and q N qL
thefollowing approximate
formula has been
suggested [1 ], [2] :
with K2 = A(T - TL). A
and B are constants. The factor K at the numerator islacking
in reference[3],
but is necessary because
S(g)
has to beintegrable [6].
Thus, S(g)
turns out to beproportional
tob(q - gL)
at
T,,
so that thesingularity
ofS(q)
at theinstability temperature
is found to be muchsharper
than inusual transitions
[5],
where1 /S(q)
remainsanalytic
at
TL.
On the otherhand,
there are reasons to believe that on thecontrary, S(q)
is smoother than usual :indeed,
assume that atTL,
theliquid
becomeslocally
solid
like,
inagreement
with the ideas of references[1 ]
and
[2].
For a solidS(q) _ Mft d(q - t),
where tr
are
reciprocal
lattice vectors. For agiven
orientation of the solid germs, oneexpects,
atTL :
by analogy
with the usual Ornstein-Zernikeformula ;
but in the
present
case it is necessary to averageon the orientations of i for a
given 1 I 1
= qL :This
simple
mindedargument
will now beput
into a moresophisticated
form.However,
ratherthan
arguing
on the difhcult case of aliquid,
it isconvenient to define a
precise
modelwhich, although
Article published online by EDP Sciences and available at http://dx.doi.org/10.1051/jphys:01973003402-3021100
212
probably academic,
seems to have features similar to those attributed toliquids
in references[1 ], [2], [3].
2. The
planar helimagnet
withisotropic
interactions in ahomogeneous
médium. - We consider a conti- nuous, 2-dimensional vector field in the 3-dimensional space, with energy :where
J(r)
is a function of r= 1 r only.
It is assumedthat m(r) 1
=1,
so thatm(r)
iscompletely
definedby
itspolar angle cp(r) [7].
In the absence of furtherprescription,
the model has nophase
transition : indeed it is the limit of anincreasing density
ofvanishingly
small moments withvanishingly
smallindividual
susceptibility,
so that there is nophase
transition as can be seen from molecular field appro-
ximation,
which in this case isrigorous
because of thelarge
number ofneighbours [8].
As aphase
transition is
desired,
the Fourier transformmq
ofm(r)
will be assumed to vanishfor q greater
thansome cut off qo > QL To sum up, the
prescriptions
are :
In any
physical analogue
of the model(see § 6),
condition
(4b)
expresses the fact that the number ofdegrees
of freedom is of the order of the number of atoms.Conditions
(4a)
and(4b)
arecompatible :
it isindeed sufficient to find
mx(r) satisfying mx(r)
1and relation
(4b),
thenM2 x(r)
satisfies(4b),
thereforem2 y =
1 -mx
also satisfies(4b)
and so does my.2.1 Low TEMPERATURES. - We start with the
assumption (to
bejustified below)
that theground
state is a
helimagnetic
structure :For a
weakly perturbed configuration :
the energy is :
Ô(Pk
and5(k)
are the Fourier transforms ofôg(r)
andJ(r) :
The bracket in the above
expression
ispositive (or
zero for k =0)
and therefore thehelimagnetic
structure is stable at T =
0,
and remains stable at lowtemperature
if(4b)
issatisfied ;
qL is the maximum ofl(k).
2.2 HIGH TEMPERATURES : : MOLECULAR FIELD APPROXIMATION
(MFA). - Let xq
be thestaggered susceptibility
of thenon-interacting system, only
submitted to conditions
(4) :
where
hq
is theqth
Fouriercomponent
of the external field. The effect of Je can be taken into accountby adding
a molecular field 23(q) mq
> toh :
with
The
system
describedby
conditions(4)
isroughly equivalent
to an arrayof cells
of sidellqo
withmagnetization
of order1/qo3 ; thé
individual suscep-tibility
of each cell isgiven by
a Curie law : xo ~f3/qg
and a similar law is
expected
forxq :
It is seen from
(5)
and(6)
that the Néeltemperature
iswhere qL
maximizes3(q). Neglecting
the weakpossible
dependence
ofXo
on q,(5)
reads for T NTN
and so that :where V is the total volume and
mq the
Fouriertransform of
m(r),
and wherevanishes at
TN.
The factor K of eq.(1)
islacking
at the numerator of eq.
(7),
thusviolating
the sumrule
2.3 SPHERICAL MODEL. - The
spherical
model[9], [10]
accounts for eq.(8) (but
not for the moregeneral
condition
m2(r) - 1) by using
thedensity
matrix :where V is the volume and :
where the
Lagrange multiplier y
is determinedby :
The critical
temperature TN
=1 /KB f3N,
determinedby
thecondition Il - 3(q,)
=0,
is found to be zero, in contradiction with what was shownabove,
para-graph
2.1.The best way to describe critical
phenomena
inour model in a consistent
approximation
is to makea
change
ofthermodynamical
variables.3.
Change
ofthermodynamical
variables. - Rather thanm(r),
we wish to introduce the variable :In terms of the
polar angle Q(r)
ofm(r),
eq.(3)
reads :
The cosine can be
expanded
in powers ofu(r)
as follows :
cos 1
After
integration
of thisexpansion,
theexpansion
of the
integral
contains :
a)
A zero-th order termwhich will be
represented by
its Mac Laurinexpansion :
and has a minimum 1
b)
Termscontaining
the derivatives of u,namely :
a term
proportional
to(div U)2
For the sake of
simplicity,
the last 3 terms, whichare of
higher
order in u, will beneglected.
It is relevant to
express
in terms of the Fourier214
transform of
u(r) - VQ(r),
which is a vector withcomponents :
The variable uq =
qqJq
has been introduced because1 Uq 12 >,
and not1 qJq 2
> remains finite for qgoing
to zero in the limit of infinite volume. a,y, 03BE
denote the
coordinates : x,
y, z.Expressing
the terma)
and the first 2 termsb)
asfunctions of
u,,, inserting
into eq.(9),
andintegrating
over r and
r’,
weget :
C, D,
E are constants.If the ordered
phase,
as was said inparagraph 2, corresponds
tou(r)
> =C’,
the constant Eis
expected
to bepositive
and thetransition,
in termsof uq, takes
place at q -
0. This transition is of avery common
type, comparable
for instance to aBose
condensation,
since uo becomesmacroscopic (proportional
to the volumeV)
below the transitiontemperature TN.
Conventional «scaling theory
»[9], [11] ] predicts
aboveTN a
correlation function of thefollowing type :
where q
is a smallpositive
coefficientand f is
a function.In the
appendix,
thethermodynamics
of thesystem
isinvestigated
in the Hartreeapproximation
andeq.
(11)
is derivedmicroscopically with q
= 0.4. Correlation-funetion for
m(r).
- We havegiven
a consistent
description
of thesystem
in terms ofu(r). Unfortunately
the correlation function(11)
is not
easily
accessible toexperiment (in
theliquid-
solid
transition, u(r) represents
a vectorjoining
2
neighbouring
atoms : see nextsection).
It istherefore of interest to
investigate
the suscep-tibility m(o) . m(r)
>. It cannot be deduced fromu(O). uer)
> without additionalassumptions,
be-cause
strictly speaking,
theknowledge
ofhigher
order
correlations,
uuuu>,
etc., isrequired.
Toapproximate
these correlationsby
a factorization is notsatisfactory,
as shown in theappendix.
It seems
preferable
toapply
the ideas of the «droplet
model »
[11]
and to assume that atTN
thesystem
is constituted of «droplets »
which look somewhat like the condensedphase. Quantitatively,
this ideais
expressed by
thefollowing assumption :
P(r)
isroughly
theprobability
that rbelongs
tothe same «
droplet
» as theorigin. m(r)
andu(r)
are mean values
corresponding
togiven
values ofm(0)
andu(O). Comparison
of eq.(11)
and(12b) yields :
The case T >
TN
will not be treated forbrevity.
At T
TN, P(r)
has a finite limit forlarge
r.For a
given
value ofu(O) =
u, the average valueof
m(O).m(r)
is from(12a)
and(13) :
and
averaging
over the orientations of uyields :
The Fourier transform of this function is not infinite
at q
= qL,except if il
=0,
where theloga-
rithmic
singularity
ofparagraph
1 is recovered.5.
Liquids.
- Our model can betransposed
toliquids :
the functiong(r),
instead ofbeing
thepolar angle
ofm(r),
now defines « reticular surfaces »by
theequation
cosqJ(r) =
1. It is alsopossible
todefine 3 families of reticular surfaces
corresponding
to 3 variables
qJa(r) (a
=1, 2, 3).
The atoms wouldbe located at the intersections of 3 surfaces. A
possible
hamiltonian is :
The hamiltonian
(3)
is asimplified
version withonly
one functionQ(r).
The orderedphase
describedin
paragraph
2.1clearly pictures
a solid since thereticular surfaces are
parallel planes.
The
description
of theliquid phase
is very poor, due to the absence ofdynamics
and to the presence of elasticproperties
that aliquid
hasprobably
not.It is not clear whether a more realistic
description
ofa
liquid
wouldgive
rise to aninstability
of thetype investigated
in this paper, but if itdoes,
there isprobably
nosingularity
at finite q in thecompressi- bility,
or a weak one, as discussed inparagraphs
1and 3.
Acknowledgments.
- The author isespecially grateful
to Pr. P. G. DeGennes,
B.Jancovici,
P. C.Martin and L. Verlet for their valuable comments and
suggestions. Acknowledgments
are also madeto Dr. Kleban and
Kugler,
and to Pr. Schofield.Appendix :
The Hartreeapproximation
The hamiltonian
(10)
will now be treated in the Hartreeapproximation, namely :
In this
approximation,
the correlation functionis,
from(10)
and standard fluctuationtheory [5] :
The Néel
temperature TN
is definedby
thefollowing
relation :
Below
TN,
uo isgiven by
the minimization of(10)
after insertion of
(A.1) :
where Ox is the direction of uo.
Inserting (A. 4)
into(A. 2) yields :
where ç
is definedby
thefollowing integral equation :
When ç
increases from 0 to00, j (ç)
decreasesfrom a
positive
value to0, except
for uo -0,
thenf(ç)
= 0.Therefore ç
> 0 for TTN,
so that thestability
conditionu _ q uq > > 0 is fulfilled,
inagreement
with Section 2.1.Remarks. -
a)
The rotational invariancerequires ôu-L. ôu-L
> = oo, wherebuô
is the fluctuationof uo
perpendicular
to uo >. On the otherhand, u_q.uq
> does not go to zero in the directionperpendicular
to uo >. Thisdiscontinuity
islikely
aspurious
result of the Hartreeapproximation,
as it would show up in a similar treatment of an
ordinary, crystalline ferromagnet,
as well.b)
Athigh temperature
thepresent approximation predicts u _ q uq
> ~T¥2.
This result should not be taken tooseriously
because it is notlegitimate
toneglect
terms ofhigher degree
in u in eq.(10).
If the factorization
(A.l)
is made in formula(10),
it is
possible
to calculatem(O). m(r)
>[7] :
The
integrand
ispositive,
so that theexponent
decreases when r increases andm(o) . m(r)
> is adecreasing
function of r. This result cannot beaccepted
because the same treatment
yields
ananalogous
result for a
crystalline helimagnet,
whereasm(o). m(r)
> is known tobe,
atTN,
anoscillating
function of r in this case. This is the reason
why
the
droplet
model was used in section 4 rather than the Hartreeapproximation.
216
References
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SCHNEIDER T., BROUT R., THOMAS H., FEDER J.,Phys.
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