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Sébastien Balibar and Ryosuke IshiguroSébastien Balibar and Ryosuke IshiguroLaboratoire de Physique Statistique de l ’Ecole Normale Supérieure,Laboratoire de Physique Statistique de l ’Ecole Normale Supérieure,
associé au CNRS et aux Universités Paris 6 & 7associé au CNRS et aux Universités Paris 6 & 7
Paris, FranceParis, France
critical Casimir forces critical Casimir forces andand
anomalous wetting anomalous wetting
StatPhys Bangalore, july 2004StatPhys Bangalore, july 2004
for references and files, go to for references and files, go to http://www.lps.ens.fr/~balibar/
abstract
a critical introduction to a critical introduction to and discussion ofand discussion of the "critical Casimir effect"the "critical Casimir effect" "critical point wetting", i.e. wetting near a critical point"critical point wetting", i.e. wetting near a critical point 4 experiments:4 experiments:
Garcia and Chan (Cornell, 1999)Garcia and Chan (Cornell, 1999) Ueno et al. (Kyoto, 2000)Ueno et al. (Kyoto, 2000) Ueno et al. (Paris, 2003)Ueno et al. (Paris, 2003) Ishiguro and Balibar (Paris, 2004)Ishiguro and Balibar (Paris, 2004)
the standard Casimir effect : the standard Casimir effect : confinement of the fluctuations of the confinement of the fluctuations of the electromagnetic field electromagnetic field the two electrodes attract each otherthe two electrodes attract each other
the "critical Casimir effect"the "critical Casimir effect"
confined fluctuations2 plates2 plates
the critical Casimir effect (Fisher and de Gennes, 1978):the critical Casimir effect (Fisher and de Gennes, 1978):near a critical point, near a critical point, confinement of the fluctuations of the order parameterconfinement of the fluctuations of the order parameter
a singular contribution to the free energy E ~ ka singular contribution to the free energy E ~ kBBT /LT /L2 2
a force between the two plates Fa force between the two plates FCasCas = - dE/dL ~ 2 k = - dE/dL ~ 2 kBBT /LT /L33
LL
the universal scaling functions the universal scaling functions and and
Further work Further work ((Nightingale and J. Indekeu 1985, M.Krech Nightingale and J. Indekeu 1985, M.Krech and S. Dietrich 1991-92) shows that and S. Dietrich 1991-92) shows that
E = kE = kBBT/LT/L22 (L/ (L/))
where where the "universal scaling function"the "universal scaling function" depends on depends on the bulk correlation function the bulk correlation function ~ t ~ t -- which diverges near the critical temperature Twhich diverges near the critical temperature Tc c . .
At TAt Tc c , i.e. t = 0, , i.e. t = 0, , the "Casimir amplitude". , the "Casimir amplitude".
a similar scaling function is introduced for the forcea similar scaling function is introduced for the force
FFCasCas = k = kBBT/LT/L33 (L/ (L/))
UniversalityUniversality
the scaling functions only depend onthe scaling functions only depend on- the dimension of spacethe dimension of space- the dimension of the order parameterthe dimension of the order parameter- the type of boundary conditions :the type of boundary conditions :
- periodic or antiperiodicperiodic or antiperiodic- DirichletDirichlet- von Neumann von Neumann
the 5 different values the 5 different values = = (T(Tcc) have been calculated, ) have been calculated,
but not but not at any T nor with any boundary conditions at any T nor with any boundary conditionsfor example Dirichlet-Dirichlet below Tfor example Dirichlet-Dirichlet below Tcc
the sign of the forcethe sign of the force
attractiveattractive if symmetric boundary conditions ( if symmetric boundary conditions ( < 0) < 0)repulsiverepulsive if antisymmetric ( if antisymmetric ( > 0) > 0)
the Casimir amplitude the Casimir amplitude = = (L/ (L/ = 0) = 0)
~ 0.2 to 0.3 for periodic boundary conditions~ 0.2 to 0.3 for periodic boundary conditionsproportional to the dimension N of the order parameterproportional to the dimension N of the order parameter10 times smaller if the order parameter vanishes at the 10 times smaller if the order parameter vanishes at the wall (Dirichlet-Dirichlet)wall (Dirichlet-Dirichlet) twice as large if tri-critical instead of criticaltwice as large if tri-critical instead of critical
the experiment by R. Garcia and M. Chan
a non-saturated film of pure 4He (200 à 500 angströms)in the vicinity of the superfluid transition (a critical point at 2.17 K),
the film gets thinner : evidence for long range attractive forcesevidence for long range attractive forcescomparison with predictions :
assume a critical Casimir force assume a critical Casimir force (x)(x)//l l 33 measure [x = (L/)], the function"of this
force
comparison with theory
below Tbelow Tcc : :
no theoryno theorythe magnitude of the experimental the magnitude of the experimental depends on L (not universal ??) depends on L (not universal ??)it is also surprisingly large (1.5 to 2, no theoretical result larger than it is also surprisingly large (1.5 to 2, no theoretical result larger than ~ 0.5)~ 0.5)
above Tabove Tcc : :
agreement with Krech and Dietrich agreement with Krech and Dietrich [Phys. Rev. A 46, 1886 (1992)][Phys. Rev. A 46, 1886 (1992)]
far below Tfar below Tcc::
a finite value of a finite value of ? ?confinement of Godstone modes confinement of Godstone modes (Ajdari et al. 1991, Ziherl et al. 2000, Kardar et al. 1991-2004,(Ajdari et al. 1991, Ziherl et al. 2000, Kardar et al. 1991-2004, Dantchev and Krech 2004)Dantchev and Krech 2004)
Phys. Rev.
E 2004
periodic boundary conditionsperiodic boundary conditionsthe Casimir amplitude is larger by a factor ~2 for the XY model (N = 2)the Casimir amplitude is larger by a factor ~2 for the XY model (N = 2)the scaling function does not vanish as T tends to 0 for the XY model the scaling function does not vanish as T tends to 0 for the XY model
the magnitude of the effect of Godstone modes
for Dirichlet-Dirichlet boundary conditions, for Dirichlet-Dirichlet boundary conditions, Kardar and Golestanian (Rev. Mod. Phys. 1999) predict Kardar and Golestanian (Rev. Mod. Phys. 1999) predict a very small amplitude a very small amplitude ~ - 0.05 ~ - 0.05Garcia's measurement : Garcia's measurement : ~ - 0.3 ~ - 0.3 in agreement with Dantchev (but with periodic boundary conditions) in agreement with Dantchev (but with periodic boundary conditions) at the 2004 APS march meeting,at the 2004 APS march meeting,R.Zandi, J. Rudnick and M. Kardar invoke the surface fluctuations R.Zandi, J. Rudnick and M. Kardar invoke the surface fluctuations of the film which would enhance the Goldstone mode contribution, of the film which would enhance the Goldstone mode contribution, but the sign of this last effect is somewhat controversial.but the sign of this last effect is somewhat controversial.In fact the situation is not settled: In fact the situation is not settled: better experiments, better experiments, and calculations with the right boundary conditions and calculations with the right boundary conditions are neededare needed
substrate
12
12
12
"critical point wetting ":"critical point wetting ":wetting near a critical pointwetting near a critical point
Young - Dupré :Young - Dupré :
cos cos = (= (22 - - 11)/)/1212
Tc
Xc
1 2
X1 X2
Moldover and Cahn (1980) :Moldover and Cahn (1980) :near the critical point at Tnear the critical point at Tcc
12 12 0 as T --> T 0 as T --> Tcc
((22 - - 11) ) 0 also , but usually with 0 also , but usually with
a smaller critical exponent, a smaller critical exponent, especially ifespecially if((22 - - 11) ~ X) ~ X22 - X - X11
cos cos increases with T up to Tincreases with T up to Tww
where cos where cos = 1 and = 1 and = 0 = 0
TcTw
cos
Tc
1
Tw
the contact angle usually decreasesthe contact angle usually decreasesto zero at Tto zero at Tww < T < Tcc
Moldover and Cahn 1980:Moldover and Cahn 1980:a wetting transition takes place at a wetting transition takes place at TTww < T< Tcc
P.G. de Gennes (1981) + Nightingale and Indekeu (1985):P.G. de Gennes (1981) + Nightingale and Indekeu (1985):not necessarily true in the presence of long range forcesnot necessarily true in the presence of long range forces
a possible exception to critical point a possible exception to critical point wetting wetting
T
10
3He concentration
superfluid
normal
0.87 K
0.675
tri-criticalpointa tri-critical point:a tri-critical point:
superfluidity + phase separation superfluidity + phase separation
at Tat Tt t = 0.87 K= 0.87 K
the example of helium 3 - helium 4 the example of helium 3 - helium 4 liquid mixturesliquid mixtures
a a 44He-rich superfluid filmHe-rich superfluid film
T
3He concentration
10
Teq
superfluid
normal
tri-criticalpoint
Romagnan, Laheurte and Sornette (1978 - 86):Romagnan, Laheurte and Sornette (1978 - 86): van der Waals attractive fieldvan der Waals attractive field
a a 44He-rich film grows on the substrateHe-rich film grows on the substrate
substrateleq
4He-rich superfluid film
lleqeq ~ (T - T ~ (T - Teqeq))-1/3-1/3 up to 60 Angstömsup to 60 Angstöms
two possibilities:two possibilities:- van der Waals only,van der Waals only, lleqeq tends to a macroscopic value: tends to a macroscopic value:
complete wetting (complete wetting (= 0)= 0)- vdW + an attractive force (Casimir),vdW + an attractive force (Casimir), lleqeq saturates at some mesoscopic value: saturates at some mesoscopic value:
partial wetting (partial wetting ( ≠ 0) ≠ 0)
substrate
superfluid film
leq
4He-richbulk phase
ΠH(l)=3πσi2l
exp−2πσil
2
3kBT
⎛
⎝ ⎜ ⎞
⎠ ⎟
ΠCas(l)=Ttl3 ×θ(l /ξ)
ΠvdW(l)=
1000×(1/Vd−1/Vc)l3(1+l/193)
in K.A−3o
the contact angle the contact angle is obtained from the is obtained from the "disjoining pressure" "disjoining pressure" (l)(l) (see Ueno, (see Ueno, Balibar et al. PRL 90, 116102, 2003 and Ross, Bonn and Meunier, Nature 1999):Balibar et al. PRL 90, 116102, 2003 and Ross, Bonn and Meunier, Nature 1999):
3 contributions to 3 contributions to (l) from long range forces:(l) from long range forces:
van der Waals van der Waals
(repulsive on the film surface) (repulsive on the film surface)
Casimir (attractive)Casimir (attractive)(l/(l/) < 0 is the scaling function ) < 0 is the scaling function
which can be estimated from Garcia and Chanwhich can be estimated from Garcia and Chan
the entropic or "Helfrich" repulsionthe entropic or "Helfrich" repulsion
due to the limitation of the fluctuations of the film surfacedue to the limitation of the fluctuations of the film surface
an approximate calculation an approximate calculation
cosθ=1−Π(l)dl
∞
leq
∫σi
optical interferometryoptical interferometry
copper
mixing chamber
10 mmHe-Ne laser
opticalinterferometric
cavity(sapphire treated for 15% reflection)
vapor
3He-rich liquid
4He-rich liquid
coppercopper
Images at 0.852 KT. Ueno et al. 2003
the empty cell:stress on windows
fringe bending
liquid-gas interface
vapor
3He-rich "c-phase"
3He- 4He interface
4He-rich "d-phase
zone to be analyzed
the contact angle the contact angle and the interfacial tension and the interfacial tension ii
fringe patternfringe pattern --> --> profile of the meniscusprofile of the meniscus --> --> and and ii
typical resolution : 5 typical resolution : 5 mmcapillary length: from 33 capillary length: from 33 m (at 0.86K) to 84 m (at 0.86K) to 84 m (at 0.81K)m (at 0.81K)
zoom at 0.841 K
d-phase
c-phase
the interface profile at 0.841K
c-phase
d-phase
sapp
hire
experimental experimental
resultsresults the interfacial tensionthe interfacial tension
agreement with Leiderer et al. agreement with Leiderer et al. (J. Low Temp. Phys. 28, 167, 1977):(J. Low Temp. Phys. 28, 167, 1977):
ii = 0.076 t = 0.076 t22
where t = 1 - T/Twhere t = 1 - T/Tt t and Tand Tt t = 0.87 K= 0.87 K
the contact anglethe contact angle is non-zero is non-zero
it it increasesincreases with T with T
the disjoining pressure at 0.86K (i.e. t = 10the disjoining pressure at 0.86K (i.e. t = 10 -2-2))
-40
-20
0
20
40
0 200 400 600 800 1000 1200
disjoining pressure
( )(l
-9
.K A
-3)
( )film thickness l Angström
Helfrich
van der Waals
total pressure
+van der Waals Casimir
Casimir
the equilibrium the equilibrium thickness of the thickness of the superfluid film:superfluid film:
lleqeq = 400 = 400 ÅÅ~ about 4~ about 4,,
where where (l) = 0(l) = 0
the calculated contact angle the calculated contact angle
at T = 0.86 K, i.e. t = 1 - T/Tat T = 0.86 K, i.e. t = 1 - T/Tt t = 10= 10 -2 -2
lleqeq = 400 Å = 400 Å , 4 times the correlation length , 4 times the correlation length
By integrating the disjoining pressure from lBy integrating the disjoining pressure from leqeq to infinity, to infinity,
we find we find = 45 ° = 45 °
near a tri-critical point, the Casimir amplitude should be near a tri-critical point, the Casimir amplitude should be larger by a factor 2larger by a factor 2
this would lead to this would lead to = 66 °, in even better agreement with our = 66 °, in even better agreement with our experimentexperiment
At lower temperature (away from TAt lower temperature (away from Tt t ):):
ii and van der Waals are larger, Casimir is smaller, and van der Waals are larger, Casimir is smaller,
so that so that should also be smaller should also be smaller
the contact angle increases with T, the contact angle increases with T,
as found experimentallyas found experimentally
In 2003, our exp. resultsIn 2003, our exp. results (Ueno et al. , JLTP 130, 543, (Ueno et al. , JLTP 130, 543,
2003)2003) agreed with our approximate calculation agreed with our approximate calculation (Ueno et al. PRL 60, 116102, 2003)(Ueno et al. PRL 60, 116102, 2003)
new setup for new setup for experiments at lower Texperiments at lower T
(R. Ishiguro and S. (R. Ishiguro and S. Balibar, in progress)Balibar, in progress)
laser beamlaser beam
closer to normal incidencecloser to normal incidenceless distortion due to refraction less distortion due to refraction effects, better control of the effects, better control of the fringe patternfringe patternmeasurements at lower T:measurements at lower T:is the contact angle ≠ 0 ?is the contact angle ≠ 0 ?Goldstone modes ? amplitude ?Goldstone modes ? amplitude ?
(sapphire treated for 15% reflection)
dilution refrigeratordilution refrigerator
copper framecopper frame
optical cavity3He-rich liquid
4He-rich liquid
Ishiguro's profiles
the contact angle is zero at low T (237 mK) and near Tthe contact angle is zero at low T (237 mK) and near Ttt (840 mK) (840 mK)
the contact angle
Ishiguro and Balibar (2004) find Ishiguro and Balibar (2004) find = 0 = 0in contradiction with previous measurementsin contradiction with previous measurements
could the Casimir force be 5 times smaller than measured by Garcia and Chan ?
the disjoining pressure would the disjoining pressure would be dominated by the van der be dominated by the van der Waals field, Waals field, always positive, always positive, implying complete wetting implying complete wetting ((= 0)= 0)
-40
-20
0
20
40
0 200 400 600 800 1000 1200
( )film thickness l Angström
Helfrich
van der Waals
total pressure
+van der Waals Casimir
Casimir
-40
-20
0
20
40
0 200 400 600 800 1000 1200
( )film thickness l Angström
Helfrich
van der Waals
/5total pressure with GC
+ ( /5)van der Waals Casimir GC
( /5)Casimir GC
summary
the exception found by Ueno et al. to "critical point wetting"the exception found by Ueno et al. to "critical point wetting"is not confirmed by our more careful, and more recent experimentis not confirmed by our more careful, and more recent experiment
still possible if the substrate exerted a weaker van der waals field ?still possible if the substrate exerted a weaker van der waals field ?
the amplitude of the critical Casimir force measured bythe amplitude of the critical Casimir force measured byGarcia and Chan is not really universal and its amplitude looks Garcia and Chan is not really universal and its amplitude looks largelargebut there is no available calculation with the right boundary but there is no available calculation with the right boundary conditions below Tc where it is large.conditions below Tc where it is large.
more work ...more work ...