Growth of third ferromagnetic solid 3He layer on graphite with and without 4He pre-plating
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Transcript of Growth of third ferromagnetic solid 3He layer on graphite with and without 4He pre-plating
Growth of third ferromagnetic solid 3He layer on graphite
with and without 4He pre-plating
Akira Yamaguchi*, Takamichi Watanuki, Ryuichi Masutomi1, Hidehiko Ishimoto
The Institute for Solid State Physics, The University of Tokyo, 5-1-5 Kashiwanoha, Kashiwa, Chiba 277-8581, Japan
Abstract
We have measured the nuclear susceptibility of 3He in Grafoil filled with pure liquid 3He over the pressure region between 0.6 and
31.38 bar and at temperatures down to 0.5 mK with a cw NMR method. The nuclear magnetization corresponding to the adsorbed 3He layers
on the Grafoil surface shows a strong ferromagnetic tendency with a periodic behavior as a function of liquid pressure. This observation is
attributable to the growth of third and fourth solid 3He layer with the liquid pressure increase. The pressure dependence of the Weiss
temperature indicates that the third layer is completed at 19 bar and the fourth probably at 28 bar. The results for Grafoil pre-plated by 2.5 and
3.5 layers of 4He are consistent with this scenario.
q 2005 Elsevier Ltd. All rights reserved.
Keywords: A. Surfaces; B. Epitaxial growth; D. Magnetic properties
1. Introduction
3He atoms bounded on the surface of various materials
form a unique system to study two-dimensional magnetism.
In particular, 3He films adsorbed on graphite have been
extensively studied owing to the atomically flat surface and
large surface area of graphite [1]. The previous investi-
gations on the film have revealed that the first and the
second atomic layer solidify on the graphite surface, while
the upper layers above the second one exist as liquid [1].
The second solid layer displays a spectacular evolution from
antiferromagnetism to ferromagnetism as a function of the
areal density. The behavior is understood as a consequence
of competing multiple spin exchange (MSE) interactions in
the solid layer. In addition to the intra layer interactions,
there is a long-standing controversy on a possible indirect
interaction mediated by 3He quasi-particles in the
over-layer liquid. Theoretically various models are
proposed and most of the models predict the existence of
RKKY (Ruderman–Kittel–Kasuya–Yoshida) type indirect
0022-3697/$ - see front matter q 2005 Elsevier Ltd. All rights reserved.
doi:10.1016/j.jpcs.2005.05.038
* Corresponding author.
E-mail address: [email protected] (A. Yamaguchi).1 Present address: Department of Physics, Tokyo Institute of Technology,
2-12-1 Ookayama, Meguro-Ku, Tokyo 152-8550, Japan.
exchange interaction [1]. In this paper, we present the
systematic study with a cw NMR technique for the solid 3He
layer on graphite covered with bulk liquid 3He as a function
of liquid pressure.
2. Experimental
The experimental setup is described in our previous work
[2]. The substrate used is an exfoliated graphite (Grafoil
GTY grade dZ76 mm) [3], which consists of partially
aligned microcrystals of graphite. Six Grafoil sheets
(8 mm!8 mm) are stacked in a sample chamber made of
epoxy (Stycast 1266). They are dipped into pure liquid 3He,
which is cooled through a sintered powder heat exchanger,
the mixture of Ag and Pt powder with the surface area of
24 m2. It has a good thermal contact with the copper nuclear
stage. The pre-plated samples with 4He were prepared with
the procedure described previously [4]. 4He gas was
introduced at 4.2 K while monitoring isothermal adsorption
pressure. NMR measurements were made with a continuous
wave method at 698 kHz. A static field of 21.5 mT was
applied in parallel to the Grafoil sheets and swept to cover
the whole NMR line. A saddle type rf coil wound around the
sample chamber (145 mH) produces an rf field paralleled to
the Grafoil sheets. Magnetization (M) was obtained from
numerical integration of the whole absorption line. The
temperature was measured with a 3He melting curve
Journal of Physics and Chemistry of Solids 66 (2005) 1482–1485
www.elsevier.com/locate/jpcs
A. Yamaguchi et al. / Journal of Physics and Chemistry of Solids 66 (2005) 1482–1485 1483
thermometer (MCT) and a Pt NMR thermometer both of
which are mounted on the nuclear stage.
3. Results
Total 3He magnetization consists of liquid magnetiza-
tion, which is due to the bulk liquid in the cell and solid
contribution from the layered spin (not shown). The liquid
contribution increases with increasing liquid pressure.
Based on the expression for a three-dimensional Fermi gas
[5] with the known Fermi temperature ðT��F Þ [6], the
calculated pressure dependence well reproduces the
observed behavior above 70 mK.
Subtracting the estimated liquid contribution, the
magnetization for the localized spins is obtained for various
pressures as shown in Fig. 1. Here, the change of the liquid
magnetization due to a superfluid transition is negligible
because of much smaller liquid magnetization itself below
the superfluid temperatures than the solid magnetization.
The solid magnetization shows a ferromagnetic tendency
over the whole pressures range. The magnetization at
0.62 bar shows the weakest temperature dependence. Below
7.7 bar, the data exhibit a rapidly rising magnetization
around 3 mK and the temperature corresponding to the rapid
rise shifts to lower temperature with increasing pressure.
This shift continues to exist up to 19.35 bar, where the
temperature dependence is week and close to that of
0.62 bar again. The evolution above 19.35–27.62 bar
resembles that in the lower pressure region. The pressure
dependence above 27.62 bar is much weaker than in the
low-pressure regions.
What causes such a periodic behavior of the magnetiza-
tion? It is difficult to explain by RKKY interaction through3He quasi-particles, because the Fermi momentum is a
monotonically and weakly increasing function of the
pressure. The other possibility is solidification of the third
and the fourth layer with increasing the liquid pressure,
analogous to the liquid pressure dependent epitaxial
adsorption of solid 4He up to seven layers [7]. The adsorbed
atoms feel the pressure from the graphite substrate given as
12
Tempera
(b)
.5 .7
500
400
300
200
100
0
Solid
Mag
netiz
atio
n [a
rb. u
nits
]
12 3 4 5 6
10
0.61bar3.39bar7.35bar
12.30bar16.67bar18.14bar
(a)
.5 .7
Temperature [mK]
Fig. 1. Temperature dependence of the solid magnetization at (a) low pressures, 0.6
28.54–31.38 bar. The bar lines are guides to the eye.
follows
pðrÞ Z pL Cns
h
C3
r3C
C4
r4
� �: (1)
Here, r is the distance from the graphite surface and pL is the
pressure of bulk liquid. The second term arises from van der
Waals potential from the graphite surface where C3 (Z2.53!10K23 J nm3) and C4 (Z1.42!10K22 J nm4) are the
coefficients of van der Waals potential determined
experimentally [8]. h is a monolayer thickness and ns is
areal density which is assumed constant here. According to
Franchetti model [9], the liquid layer solidifies in the region
p(r)Ops where ps is the melting pressure of bulk liquid
(w34 bar). If we assume the monolayer thickness is 0.3 nm
and ns is equal to the maximum value for the second layer
(Z8.7 atoms nmK2), the solidification at the third and the
fourth layer position are expected to be completed at 19 and
28 bar, respectively. Thus, the present scenario seems to
reproduce the observed behavior, although it is believed
from the adsorbed film experiments that the only two layers
exist as a solid. Above 28 bar, the pressure dependence of
the magnetization is weak, and it is not clear whether the
fifth or more solid layers exist or not from the present
observation.
Based on the above-described model, the data are
analyzed at high temperatures where the Curie–Weiss
approximation is valid. In the low-pressure region below
19.35 bar, a three solid layers model is employed
MsolidðTÞ Z Cn1st
T Kq1
Cn2nd
T Kq2
Cn3rd
T Kq3
� �; (2)
where C is a Curie constant for each spin, n1st, n2nd, n3rd
are the amount of 3He atoms, and q1, q2, q3 are the Weiss
temperature for the first, the second, and the third solid
layer, respectively. According to the film experiment, he
first layer is highly compressed [1], being consistent with
the calculated pressure from Eq. (1) (p(r)O750 bar) at the
first layer position. Therefore, we assume n1stZ11.4 atoms nmK2, a maximum density observed in the
film experiment, and q1Z0 mK, independent of the liquid
pressure. In the same way, the parameters for the second
3 4 5 610
ture [mK]
19.35 bar19.61 bar24.03 bar27.62 bar
12 3 4 5 6
10Temperature [mK]
28.54 bar30.40 bar31.38 bar
(c)
.5 .7
4–18.14 bar; (b) middle pressures, 19.35–27.62 bar; and (c) high pressures,
60
50
40
30
20
10
0
n solid
[at
oms/
nm2 ]
302520151050P [bar]
n1st+n2nd+n3rd
n1st+n2nd+n3rd+n4th
n1st+n2nd
n1st+n2nd+n3rd
3rd layer
4th layer
Fig. 2. The total amount of solid 3He layer, (B) ntotalZn1stCn2ndCn3rd and
(6) ntotalZn1stCn2ndCn3rdCn4th. Vertical lines correspond to the third
and fourth layer completion. The horizontal dotted and dashed lines
indicate the amount of solid 3He corresponding to the second and third layer
completion.
5
4
3
2
1
θ [m
K]
302520151050P [bar]
θ3 θ4
3rd layer
4th layer
Fig. 3. Pressure dependence of the Weiss temperature, (B) q3 for the third
layer and (:) q4 for the fourth layer.
A. Yamaguchi et al. / Journal of Physics and Chemistry of Solids 66 (2005) 1482–14851484
layer at SVP are estimated from those of the previous film
experiments to be n2ndZ8.7 atoms nmK2 and q2w1.5 mK
[1]. The liquid pressure dependence of these values is
unknown, but seems to be negligible. Because the first and
the second layer feel strong pressures much higher than
Sol
id M
agne
tizat
ion
[ arb
.uni
ts]
200
150
100
50
0
Sol
id M
agne
tizat
ion
[arb
.uni
ts]
121086420Temperature [mK]
pure3He
2.5 layers of4He pre-plated
3.5 layers of4He pre-plated
(a)
Fig. 4. (a) Magnetization at saturated vapor pressure for the sample with no p
magnetization for the 3.5 layers of 4He pre-plated sample under various pressure
34 bar from the graphite substrate and therefore their
densities should not be affected seriously by the liquid
pressure. Consequently, n3rd and q3 are two free
parameters which should be determined by fitting the
data between 0 and 19.35 bar to Eq. (2). Pressure
dependence of n3rd is shown in Fig. 2 as a total solid
contribution ntotalZn1stCn2ndCn3rd and the corresponding
q3 is shown in Fig. 3.
A relatively rapid increase of ntotal and the weak
dependence of q3 with a large value between 0 and 10 bar
should be attributed to the growth of the low-density third
layer, while a weak dependence of ntotal and a rapid drop of
q3 between 10 and 18.35 bar is possibly due to the
compression of the third layer.
In the higher-pressure region than 19.35 bar, a similar
analysis is made by assuming the growth of the fourth layer
and adding the term n4th/(TKq4) to Eq. (2). The first and
second layer parameters are assumed to be the same as in the
above analysis. As for the third layer parameters, the values
obtained at 19 bar are employed, n3rd of 8.1 atoms nmK2
and q3 of 1.6 mK. The results for n4th and q4 are shown in
Figs. 2 and 3. The increase of ntotal is similar to the third
layer region. The difference of ntotal between 0 and 28 bar is
almost the same with the ntotal at 0 bar, supporting our
assumption that the third and the fourth layer are added to
the two original solid layers. q4 does not show any particular
pressure dependence, being nearly constant, in contrast to
the large pressure dependence of q3 near the third layer
completion. Moreover, the value of q4 is large and
independent of the fourth layer completion. A possible
cause of this behavior is weaker adsorption potential at the
fourth layer position than at the third layer. Therefore, the
normal motion of 3He atoms to the substrate is enhanced
between the solid layer and the liquid. This situation is
favorable for investigating a liquid mediated RKKY type
interaction.
350
300
250
200
150
100
50
05 6 7 8 9
12 3 4 5 6 7 8 9
10Temperature [mK]
0.22 bar8.21 bar
10.03 bar19.85 bar
(b)
re-plating and those pre-plated with 2.5 and 3.5 layers of 4He. (b) Solid
s.
A. Yamaguchi et al. / Journal of Physics and Chemistry of Solids 66 (2005) 1482–1485 1485
What happens for the 4He pre-plated samples? Fig. 4(a)
shows the temperature dependence of magnetization for
pure 3He, 2.5 and 3.5 layers of 4He pre-plated samples at
saturated vapor pressure, where the magnetization arising
from the bulk 3He liquid is already subtracted. The
magnetization are reduced by substitution of 3He in the
first and second layer with solid 4He. The 2.5 layers of 4He
is not sufficient to suppress the formation of solid 3He layer
probably in the third layer [10]. The 3.5 layers of pre-plating
eliminates most of surface magnetization except for very
small amount of solid-like magnetization, which is probably
due to 3He atoms trapped at the heterogeneities with much
deeper absorption potential than the flat area. Fig. 4(b)
shows the magnetization data for the 3.5 layers of 4He pre-
plate sample under various pressures. With increasing liquid
pressure a magnetization obeying a Curie–Weiss law
gradually grows in the same way as for pure liquid 3He.
The pressure-induced magnetization is attributable to the
formation of solid 3He layer in the fourth layer. The fitting
the high temperature data to a Curie–Weiss law gives the
Weiss temperature, qw3 mK. Both the Weiss temperature
and the simultaneously obtained Curie constant correspond-
ing to the number of 3He atoms have relatively weak
dependence on the liquid pressure, which is similar to that
for the fourth layer of pure sample.
In summary, the third and the fourth layer grow as a solid
with increasing liquid pressure. In our knowledge, it is
the first experimental evidence that more than two 3He
layers solidify on graphite surface. The upper solid layers
show a strong ferromagnetic tendency that depends on
liquid pressure.
Acknowledgements
This work was partly supported by a grant-in-aid
Scientific Research from Ministry of Education, Science,
Sports, and Culture of Japan.
References
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[2] A. Yamaguchi, et al., J. Low Temp. Phys. 134 (2004) 67 Phys. Rev.
Lett. 93 (2004) 165301.
[3] Grafoils is a product of GrafTech Int. Ltd.
[4] A. Yamaguchi, et al., J. Low Temp. Phys. 138 (2005) 307.
[5] D.P. Grimmer, et al., J. Low Temp. Phys. 26 (1997) 19.
[6] H. Ramm, et al., J. Low Temp. Phys. 2 (1970) 539.
[7] S. Ramesh, et al., Phys. Rev. Lett. 49 (1982) 47.
[8] F. Joly, et al., Surf. Sci. 264 (1992) 419.
[9] S. Franchetti, Nuovo Cimento 4 (1956) 1540.
[10] M. Neuman, et al., in: The Proceedings of QFS2004 Conference
(2004).