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HAL Id: jpa-00211018

https://hal.archives-ouvertes.fr/jpa-00211018

Submitted on 1 Jan 1989

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A simple model of the Fe/Cu (001) reconstruction

Š. Pick

To cite this version:

Š. Pick. A simple model of the Fe/Cu (001) reconstruction. Journal de Physique, 1989, 50 (13),

pp.1583-1586. �10.1051/jphys:0198900500130158300�. �jpa-00211018�

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1583

LE JOURNAL DE PHYSIQUE

Short Communication

A simple model of the Fe/Cu (001) reconstruction 0160. Pick

J. Heyrovsky Institute of Physical Chemistry and Electrochemistry, Czechoslovak Academy of Sci-

ences, Dolej0161kova 3, 182 23 Prague 8, Czechoslovakia

(Reçu le 24 mars 1989, accepté sous forme définitive le 3 mai 1989)

Résumé.

2014

Afin d’étudier la reconstruction displacive d’un film bicouche de Fe sur du Cu(001),

récemment observée, nous avons analysé un hamiltonien hautement simplifié de liaison forte par la méthode de récurrence. La reconstruction de surface se développe vraisemblablement dans une gamme étroite d’aimantation (probablement ~ par atome).

Abstract

2014

To study the recently observed displacive reconstruction of the two-layer Fe film on Cu(001), a highly simplified tight-binding Hamiltonian is analyzed by the recursion method. In a

narrow range of magnetization (probably ~ per atom), the surface reconstruction is likely to develop.

J. Phys. France 50 (1989) 1583-1586 1er JUILLET 1989,

Classification

Physics Abstracts

68.35 - 73.60 - 75.70

1. Introduction.

Because of their interesting properties, thin layers of ferromagnetic transition metals have been studied extensively during the last years, both experimentally and theoretically. Particularly, much

attention has been paid to iron grown on the (001) face of noble and f.c.c. transition metals [1-6].

For very thin Fe-films, the following properties seem to be established [4-6] : a) the electronic d- states of Fe do not hybridize strongly with the electronic states of the substrate, and b) the iron magnetization is enhanced with respect to the bulk, amounting to about 3 YB per atom.

Recently, a structural transition from (1 x 1) to (2 x 1) phase has been observed for two

Fe-monolayers deposited on Cu (001) when cooled to temperatures below 300 K [2]. For films

4 or 5 monolayers thick, a related phonon softening is detected. Such behaviour may indicate the repulsive stress within the surface (lst) Fe-layer, causing an important change of the surface force constants [2]. It is interesting that softening of an analogous (xi) mode has been predicted

theoretically [7] for the unstable (1 x 1) W (001) surface. According to [8], the repulsion between

the surface tungsten atoms results from the indirect interaction mediated by the subsurface (2nd layer) atoms. T’he explanation of the latter effect is based on the analysis of the 4th-order moment

of the electronic Hamiltonian. However, the generalization of this picture to the Fe/Cu (001)

system is not straightfonvard.

Article published online by EDP Sciences and available at http://dx.doi.org/10.1051/jphys:0198900500130158300

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2. The model.

Below, an attempt is made to study the Fe/Cu (001) instability in the framework of a highly sim- plified one-electron tight-binding approach. Taking the properties mentioned in the introduction into account, we consider the isolated two-layer f.c.c. iron film. As pointed out by the referee, this assumption is less justified for the Cu-substrate than e.g. in the Ag case. The reason is the smaller interatomic distance and the position of the copper d-bands closer to the Fermi energy. In the

light of recent results [6], the very behaviour of thin Fe-films on the (001) faces of noble metals, Pd

and Pt seems to be universal and we believe that the gross qualitative features are not completely

lost in our modeL Besides that, the mean field (rigid band splitting) approximation [9]

is introduced for the electronic energy band dispersion Ea (k). Above, the index "+" ("-") stands

for the majority (minority) spin orientation. The existing theoretical results on ferromagnetic films

seem to support the approximation (1), especially as the flat t2g-bands are concerned.

The starting point of our computation is the d-electron nearest-neighbour tight-binding

Hamiltonian based on the canonical f.c.c. parameters of Pettifor taken from the reference [10]

(ddcr = - 0.027784 Ry, dd7r = 0.012535 Ry, ddc5 = - 0.001554 Ry). In the paramagnetic phase (8 = 0), the energy spectrum of the two-layer film is confined between the x2 - y2-like energy levels at -0.106868 Ry and 0.084906 Ry, situated in the surface Brillouin zone points r and M, respectively. Th bring the tight-binding parameters closer to those predicted by Harrison [11] for

iron with the Cu-lattice spacing, we have multiplied the parameters of Pettifor by the factor 1.6.

Any other scaling, as well as a différent choice of the parameter Q introduced below would lead

simply to the linear rescaling of the energy difference curve given in figure 1.

1 If

Fig. 1.- The electronic energy change per atom 6.Eel associated with the deformation with the amplitude

O.Ola. 1be deformation considered is shown in the inset. (The lst and 2nd layer atoms are represented by large and small circles, respectively).

On the ideal two layer sium, the deforinatioii suggested in [2] with the amplitude O.Ola is im-

posed (see Fig. 1 ; the amplitude on the 2n atomic layer is zéro from symmetry reasons). The

corresponding electronic (band) energy change [12, 13] reads

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Above, the indices i, u refer to the type of the orbital and to the spin, respectively, hiiu = 1=8,

and ni, (E) is the partial local density of electronic states. Contribution from both film layers is

included. Due to the approximation (1), the calculation for majority and minority spins can be performed separately. The density of states ni, is evaluated by the recursion method [10,12,13]

including the Hamiltonian moments up to the 10th order, and terminating the continued fraction

by the quadratic terminator fitted to the band limits specified above.

Similar models suffer from the uncertainty in the choice of the parameters [12,13], and the

situation is yet more unfavourable for the pseudomorphic ferromagnetic film, properties of which

are not known in the detaiL Hence, it is more promising to introduce further simplifications into

our model retaining the most essential aspects of the problem at the same time, rather than to insist on a careful fitting procedure. First, we write the perturbation due to the deformation as

AH = Hl = (grad H, ’1) , where q is the deformation. It is this term which is decisive in the stability analysis [14]. On the other hand, we disregard the contribution quadratic in q and containing the 2nd derivatives of H. This term contributes to the repulsive (restoring) forces and

is not sensitive to the détails of the deformation [14]. Hence, it is more convenient to include it into the repulsive force term [12, 13] not considered here. Assuming the r- Q -distance-dependence of

the Hamiltonian matrix elements, the change of the matrix block HAB describing the interaction between atoms A, B is of the form

In equation (3), Aras is the bond length change and w is the infinitesimal rotation generator

associated with the A - B bond rotation by the angle Ao. The choice of Q represents a serious problem : Q = 5 according to canonical theories [11-13], although the recent calculations [12,13j

suggest a reduced value. Here, we adopt the value Q = 3.5. In any case, the first term in the right-

hand side of equation (3) is more important than the second one. Th avoid complications arising

from the Q-dependent interplay between the two terms, we neglect the rotation term completely.

3. Results and discussion.

The electronic energy change per atom, associated with the deformation is shown in figure 1 as

a function of the electronic occupation number N (0 N 5) for électrons with particular (ma- jority or minority) spin orientation. In figure 1, negative values of AEei are favourable for the destabilization. The contribution from the surface and subsurface is comparable, and this is expe-

cially true in the vicinity of the marked minimum at about N = 4.7. The origin of this outstanding

feature can be traced to the flat t2g energy bands. The three t2g orbitals contribute most to the A Eel

curve, whereas the x2 - y2 orbital is almost not involved. For transition metals, the electronic energy gain for deformations with the amplitude 0.01a should be several 10-5 Ry (10-4 eV [15]

to overcome the repulsive forces. That is why the position of the Fermi level EF in the region

close to N = 4.7 for majority spins would be very favourable for the surface softening. We find an essentially smaller energy gain at N N 0.5 and also in the central part of the energy spectrum.

In the latter case, however, the part of the restoring forces due to the second derivatives of the Hamiltonian (which reduce the Hamiltonian second moment m2 and are not considered here)

are maximaL Indeed, according to common, although crude approximation, JE’et is proportional to m2, with the proportionality factor being maximal for roughly half occupied bands. The result- ing guess (which is by no means reliable) indicates that the energy gain is reduced by one third in

this energy region.

Similarly as in [12, 13], the exact d-electron count per atom is not known, although it is un-

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1586

doubtedly higher than 6 (cf. Ref. [16]). Accepting the value Nd+ 4.7 for majority spin electrons,

the magnetic moment per atom will be > 3 PB, in accord with thé values quoted above.

It would be nice to offer a simple picture of the surface destabilization, e.g. in the following

form : let us consider (x a y) z orbitals interacting predominantly along the atomic chains in the

[1, 1] direction. (The situation is the very same for (x - y) z orbitals and the [1, -1] direction).

Ileating the chains as one-dimensional arrays of alternating lst and 2nd layer atoms, the deforma- tion studied in the present paper has formally period 4 along the chain. (Note that the glide-plane symmetry operation, interchanging the lst and the 2nd layer, behaves in most respects as a "com-

mon" translation along the chain). Consequently, two Peierls gaps open in the upper and in the lower part of the density of states, respectively [17]. The minima at about N = 0.5 and N = 4.7 in

figure 1, together with the proof of the importance of t2g orbitals, may give some credit to the above

idea. Nevertheless, the model of the quasi-one-dimensionai chains is probably too simplified to be

taken literally.

Tb summarize, our simple tight-binding model indicates that the two-layer iron film on Cu(001) can reconstruct providing that the Fermi level falls into a narrow range of energies cor- responding probably to the magnetic moment value > 3 UB per atom. The cause of the instability

is the indirect repulsive interaction between surface atoms, mediated by the 2nd layer. For this interaction, t2g orbitals are important.

Acknowledgement.

The author is indebted to Professor Dr. Harald Ibach for drawing his attention to the problem.

References

[1] PESCIA D., STRAMPANONI M., BONA G.L., VATERLAUS A., WILLIS R.F. and MEIER F., Phys. Rev.

Lett. 58 (1987) 2126.

[2] DAUM W., STUHLMANN C. and IBACH H., Phys. Rev. Lett. 60 (1988) 2741.

[3] DÜRR W., TABORELLI M., PAUL O., GEMAR R., GUDAT W., PESCIA D. and LANDOLT M., Phys.

Rev. Lett. 62 (1989) 206, and references given therein.

[4] FU C.L., FREEMAN A.J. and OGUCHI T., Phys. Rev. Lett. 54 (1985) 2700.

[5] RICHTER R., GAY J.G. and SMITH J.R., Phys. Rev. Lett. 54 (1985) 2704.

[6] BLÜGEL S., WEINERT M. and DEDERICHS P.H., Phys. Rev. Lett. 60 (1988) 1077.

[7] SINGH D. and KRAKAUER H., Phys. Rev. B 37 (1988) 3999.

[8] TOMÁ0160EK M., PICK 0160. and LUCHINI M.U., Surf. Sci. 209 (1989) L 99 ;

PICK 0160., TOMÁ0160EK M. and LUCHINI M.U., to appear.

[9] ZIMAN J., Principles of the Theory of Solids (University Press, Cambridge) 1964.

[10] HAYDOCK R. and KELLY M.J., Surf. Sci. 38 (1973) 139.

[11] HARRISON W.A., Electronic Structure and the Properties of Solids (W.H. Freeman, San Francisco)

1980.

[12] TERAKURA I., TERAKURA K. and HAMADA N., Surf. Sci. 111 (1981) 479.

[13] LEGRAND B., TRÉGLIA G., DESJONQUÈRES M.C. and SPANJAARD D., J. Phys. C 19 (1986) 4463.

[14] PEARSON R.G., Symmetry Rules for Chemical Reactions: Orbital Topology and Elementary Processes (J. Wiley, New York) 1976.

[15] PICK 0160. and TOMÁ0160EK M., Surf. Sci. 165 (1986) L 85.

[16] OHNISHI S., FREEMAN A.J. and WEINERT M., Phys. Rev. B 28 (1983) 6741.

[17] TURCHI P., DUCASTELLE F and TRÉGLIA G., J. Phys. C 15 (1982) 2891.

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