662
Journal of Non-Crystalline Solids 117/118 (1990) 662-665 North-Holland
STRUCTURES OF LIQUID METAL SURFACES AND THE SPECULAR REFLECTION OF FAST ELECTRONS* Masayuki HASEGAWA+ and Toshihiro ICHIKAWA§ +School of Mathematics, Faculty of Engineering, lwate University, Morioka 020, Japan §Institue for Materials Research, Tohoku University, Sendai 980, Japan# In this contribution we seek f o r the p o s s i b i l i t y of deducing the atomic density p r o f i l e s of l i q u i d metal surfaces from the r e f l e c t i o n high energy electron d i f f r a c t i o n (RHEED) experiments. For this purpose, we have calculated the glancing angle dependence of the specularly reflected i n t e n s i t y of f a s t electrons f o r assumed atomic density p r o f i l e s . Comparisons of these results with the RHEED experiments suggest that monotone density p r o f i l e s are plausible f o r both In and Sn in cont r a s t to the previous results for other metals obtained by the Monte Carlo simulations and the X-ray r e f l e c t i o n experiments. I t is also found that the surface width of Sn is much larger than that of In. I . INTRODUCTION
tions are i n e v i t a b l y involved in the calcula-
Over the l a s t two decades increasing attention has been paid to the microscopic theory of
tions of the e f f e c t i v e Hamiltonian which determines the energetics of the ions.
We also note
l i q u i d metal surfaces and various type of theo-
that a s t r a t i f i e d structure, i f any, of the
ries have been developed I ,
density p r o f i l e is reflected as a small struc-
These theories are
generally successful in predicting the surface
ture in the angle dependence of the X-ray re-
tension of the l i q u i d simple metals such as the
flectance and making analysis of such data
a l k a l i metals.
without ambiguity is not easy.
However, these theories are too
much complicated or too crude to be used for calculating surface density p r o f i l e s .
Recently, one of the authors (T. I . ) has
Rice and
performed the r e f l e c t i o n high energy electron
co-workers have p r i m a r i l y been concerned with
d i f f r a c t i o n (RHEED) experiments in an attempt
t h i s problem and performed Monte Carlo simula-
to determine the surface structures of l i q u i d
tions for l i q u i d Na, Cs and Hg2.
In and Sn.
The atomic
Electron beams couple much more
density p r o f i l e s obtained by these studies show
strongly with the atoms than the X-rays and, in
o s c i l l a t o r y or s t r a t i f i e d structures near the
a sense, are more adequate for studying surface
surface.
structures.
The X-ray r e f l e c t i o n experiments on
l i q u i d Cs and Hg also support the existence of such structures in the density p r o f i l e s 3. Unfortunately, the results of these studies for the atomic density p r o f i l e s are not very conclusive because of various d i f f i c u l t i e s .
density p r o f i l e s of l i q u i d metal surfaces from the RHEED experiments.
We
f i r s t note that the numerical simulations f o r l i q u i d metal surfaces are f a r from exact in the sense that crude and u n j u s t i f i a b l e approxima-
The purpose of this contribution is to seek for the p o s s i b i l i t y of deducing the atomic For this purpose, we
calculate I ( 0 ) , the glancing angle dependence of the specularly reflected i n t e n s i t y of f a s t electrons, for assumed atomic density p r o f i l e s . Then, we look f o r the plausible density p r o f i l e
*This work is supported in part by the research grant of I n s t i t u t e for Materials Research, Tohoku U n i v e r s i t y , through No. 880168. #Present address: Department of Applied Physics, Faculty of Engineering, Meiji University, Kawasaki 214, Japan 0022-3093/90/$03.50 (~) Elsevier Science Publishers B.V. (North-Holland)
M.Hasegawa,T. Ichikawa/ Struetures of liquid metal surfaces
663
by comparing these results with experiments.
e ik-r
2. SPECULAR REFLECTION OF FAST ELECTRONS I f the dynamical e f f e c t of the atomic d i s t r i -
ei(k,q).r
9
VAPOUR ,
~
bution ( i . e . the energy of phonon-like excita-
\/"
tion) can be ignored, we may consider that the external electrons in l i q u i d metals are scattered by the s t a t i c superposition of the atomic potentials.
LIQUID~
Then, the potential f e l t by an exter-
eik°.r
nal f a s t electron may be given by V(r) = ~ Vatom(l~ - r i l )
(I)
1
where Vatom(r ) is the atomic p o t e n t i a l , i . e . the
FIGURE 1 Specular r e f l e c t i o n of f a s t electrons from the l i q u i d metal surface.
e l e c t r o s t a t i c potential due to the nucleus and atomic electrons.
In this quasi-elastic approx-
where E =~2k2/2m is the energy of the incident
imation, the e f f e c t of the thermal diffuse scat-
electrons and the wave function ~(r) is subject
tering (phonon-like e x c i t a t i o n ) which dominates
to the asymptotic conditions in Fig. I .
the e l a s t i c scattering is i m p l i c i t l y taken into
convenient to rewrite eq. (2) as
I t is
account through the s t a t i c d i s t r i b u t i o n of the [-(~2/2m)~2 + Vs(z) + AV(~)]~(r) = E~(r) (3)
atoms. In metals, i t is desirable to t r e a t the va-
where Vs(Z) is the potential averaged over the
lence electrons as the extended conduction elec-
d~rections p a r a l l e l to the surface and AV(r) =
trons.
V(r) - Vs(Z ).
In heavy metals, however, the electro-
The specular r e f l e c t i o n of a
s t a t i c potential due to the core electrons domi-
s u f f i c i e n t l y extended plane wave is e s s e n t i a l l y
nates the electronic potential and any d i f f e r -
determined by Vs(Z), whereas AV(r) may be
ence arising from d i f f e r e n t treatments of the
treated as giving r i s e to the damping of the
valence electrons is i n s i g n i f i c a n t .
incident, reflected and refracted waves.
We consider the specular r e f l e c t i o n of fast electrons in the above approximation.
We take
Fur-
thermore, we may expect that the electrons incident with small 0 are reflected before any
the z axis to be perpendicular to the l i q u i d
damping e f f e c t becomes important.
surface and assume that the incident electrons
in the f i r s t approximation, the problem may be
can be treated as a plane wave.
reduced to the one-dimensional scattering prob-
Let e be the
glancing angle of the incident electrons with wave-vector k = (k x, O, kz), where kx : kcos8 and kz= -ksine (see Fig. I ) . Then, the asymp-
Therefore,
lem represented by the Sch~dinger equation -(~2/2m)d2w(z)/dz2 + Vs(Z)W(Z) : (~2k~/2m)w(z)
t o t i c form of the specularly reflected wave may
(4)
be given by the plane wave with wave-vector k +
The wave function w(z) in eq. (4) s a t i s f i e s the
q, where q : (0, O, q) and q = 2ksine.
asymptotic condition
A practical method of calculating l ( e ) may be to solve the scattering problem represented by the Sch~6dinger equation [-(~2/2m)V 2 + V(~)]~(r) : E~(~)
(2)
w(z)
f
aeikz z + be-ikz z
I eikr z
(z + ~)
(z ÷ -~)
where kr = kz[l - Vs(_=)/Esin2e]I/2
(s)
664
M. Hasegawa, T. Ichikawa/ Structures of liquid metal surfaces
Then, the r e f l e c t i v i t y
is given by
1.6
l ( e ) = Ib/al 2
(6)
We note that the approximate treatment in the
~(z)
/
/'\D \
1.2 i"
~\
it/ /t
above is v a l i d only f o r small 0 and the damping e f f e c t may become important as 8 increases.
0.8
3. APPLICATIONS TO LIQUID In AND Sn
0.4
i,
"~
---,I
\
STEP
I,
The RHEED experiments have been made f o r In and Sn near above t h e i r melting temperatures.
0
These metals have been chosen f o r practical reasons, i . e .
-3
I
I
-2
-1
0
z/R s
1
low melting temperatures, low vapour
pressures and s t a b i l i t y
against oxidations.
The
energy of the electron beams adopted in these experiments is 20keV.
The experimental d e t a i l s
FIGURE 2 Atomic density p r o f i l e s assumed f o r c a l c u l a t i n g the surface potential Vs(Z). p(z) = p(z)/p b.
w i l l appear elsewhere. In order to deduce the atomic density prof i l e s of In and Sn from these experiments, we have applied the formalism in §2 to these metals.
0
Vs(z)
The surface potential Vs(Z ) may be most -0.5
conveniently taken to be the average of V(r) over the atomic d i s t r i b u t i o n , i . e .
'~...__. , . I I ~
Vs(Z ) : < ~ Vatom(Ir - r i l ) ) a v I
":S ' TEP
-1.0
= fdr'vatom(Ir - r'I)p(z')
,,__iD
(7)
where p(z) is the atomic number density.
1.5
To calculate Vs(Z ) we assume parametrized
I -2
I -1
I
z/R s
0
I 1
density p r o f i l e s of the form p(z)
:
{
Pb[l - cexp(81x)cos6x]
(x < O)
Pb(l - c)exp(-B2x)
(x > O)
(8)
where Pb is the atomic number density of the
FIGURE 3 Surface p o t e n t i a l s of In calculated by using p(z) in Fig. 2. The results of Sn are almost i n d i s t i n g u i s h a b l e from those of In in t h i s scale. Vs(Z ) = Vs(Z)/IVs(-~) I.
bulk l i q u i d metal and x = z/Rs, Rs being the atomic-sphere radius defined by (4~/3)R~ = pb -1
steep potential b a r r i e r ( f o r the atoms) near
Two of the four parameters c, BI, 62 and 6 can
the surface.
Such a behaviour may be s i m i l a r
be eliminated by requiring that p(z) and dp/dz
to that of the radial d i s t r i b u t i o n function of
are continuos at z = O.
the bulk l i q u i d metal.
Figure 2 shows p(z) used in our calculations. The parameters of each curve in Fig. 2 are A; 61 : 6.5, ~ = 0
C; 61 : 2.0, ~ = 3.8
The value of 6 = 3.8
(curves C and D in Fig. 2) has been chosen f o r t h i s reason.
Other p o s s i b i l i t i e s , of course,
cannot be excluded but d i f f i c u l t
B; B1 = 2.0, ~ = 0 D; BI : 0.7, 6 : 3.8 O s c i l l a t o r y behaviours of p(z), i f any, may be
on physical basis.
considered as a r i s i n g from the presence of a
lated by using p(z) in Fig. 2.
to i n t e r p r e t e
Figure 3 shows the surface potentials calcu-
M. Hasegawa, T. Iehikawa / Structures of liquid metal surfaces The results of calculations f o r l ( e ) are
665
1
compared with experiments in Fig. 4. The experimental results are normalized so that the
ItS}
smooth extrapolations of the reflected i n t e n s i t i e s ( f o r small e) to e = 0 is unity.
This
i 0 -~
normalization is almost unique for In, but
"'"'"-,. STEP
there is some ambiguity for Sn since the reflected i n t e n s i t i e s are not smooth probably be-
10-2
\\
cause of the experimental errors.
""
We see from Fig. 4 that monotone density p r o f i l e s are plausible for both In and Sn and that the surface with of Sn is about three times larger than that of In.
10 -3 _
We find that the behav-
iour of l ( e ) in the range of small e is essentially
determined by the steepness of Vs(Z) near
the surface.
Once we allow for the physically
10 -& 0
5
10
15
20
GLANCINGANGLE9 Lmrod)
acceptable o s c i l l a t i o n s in p(z), the steepness of Vs(Z ) near the surface is almost uniquely determined. Such a Vs(Z) is too soft ( f o r In) or too steep ( f o r Sn) to reproduce experimental
l(e).
FIGURE 4 Glancing angle dependence of the specular ref l e c t i v i t y of fast electrons (E = 20keV). F i l l ed and open c i r c l e s are observed results for In and Sn respectively and curves are results calculated by using p(z) in Fig. 2.
4. DISCUSSIONS We f i r s t note that the atomic density prof i l e s p(z) of l i q u i d In and Sn which reproduce
ondly, we have considered only the l i m i t e d type of p(z), but other p o s s i b i l i t i e s cannot be ex-
RHEED experiments are quite d i f f e r e n t from the
cluded.
previous results for other l i q u i d metals: p(z)
analysis of the X-ray reflectance data.
of l i q u i d Na, Cs and Hg obtained by Monte Carlo
This statement also applies to the
In conclusion, the present analyses of the
simulations or X-ray r e f l e c t i o n experiments show o s c i l l a t o r y behaviours near the surface.2'3 I t
RHEED experiments for l i q u i d In and Sn cast a
is not clear at this stage i f this difference is
density p r o f i l e s of l i q u i d metal surfaces.
doubt on the previous results for the atomic
due to the inadequateness of the present or previous studies or to the d i f f e r e n t natures of the individual metals. There remain some problems in the present anslyses.
F i r s t l y , we have ignored the damping
e f f e c t which would become important f o r large e. I t is e a s i l y understood that, i f we take into account this e f f e c t , 1(e) would decrease more rapidly than otherwise. In f a c t , the observed l ( e ) decrease more r a p i d l y at large e than the calculated l ( e ) and t h i s difference may be understood in terms of the damping e f f e c t .
Sec-
REFERENCES I . M. Hasegawa, J. Phys. F 18 (1988) 1449 and references therein. 2. M.P. D'Evelyn and S.A. Rice, J. Chem. Phys. 78 (1983) 5225; J. Gryko and S.A. Rice, J. Chem. Phys. 80 (1984) 6318; J. Harris, J. Gryko and S.A. Rice, J. Chem. Phys. 86 (1987) 1067. 3. B.C. Lu and S.A. Rice, J. Chem. Phys. 68 (1978) 5558; D. Sluis and S.A. Rice, J. Chem. Phys. 79 (1983) 5658; L. Bosio and M. Qumezine, J. Chem. Phys. 80 (1984) 959.