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HAL Id: jpa-00210203

https://hal.archives-ouvertes.fr/jpa-00210203

Submitted on 1 Jan 1986

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Attenuated total reflection from a nonlocal dielectric with an excitonic surface potential

R. Ruppin

To cite this version:

R. Ruppin. Attenuated total reflection from a nonlocal dielectric with an excitonic surface potential.

Journal de Physique, 1986, 47 (2), pp.259-262. �10.1051/jphys:01986004702025900�. �jpa-00210203�

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Attenuated total reflection from a nonlocal dielectric with an excitonic surface potential

R. Ruppin

Soreq Nuclear Research Center, Yavne 70600, Israël (Reçu le 13 aout 1985, accepté le 9 octobre 1985 )

Résumé.

-

Nous présentons une méthode de calcul des spectres de réflexion totale atténuée (ATR) d’un diélec-

trique non-local semi-infini dans lequel l’effet de la surface est décrit par un potentiel de surface continu. Pour des valeurs physiques raisonnables des paramètres du potentiel de surface, les spectres calculés sont indépendants du

choix des conditions aux limites additionnelles (ABC) qui sont appliquées à la surface du diélectrique.

Abstract.

2014

A method for calculating attenuated total reflection (ATR) spectra of a semi-infinite nonlocal dielectric,

in which the effect of the surface is described by

a

continuous surface potential, is presented. For physically reaso-

nable values of the surface potential parameters the calculated spectra are found to be independent of the choice of the additional boundary conditions (ABC) which are applied at the surface of the dielectric.

Classification Physics Abstracts

71.35

Surface exciton-polaritons at planar boundaries

of spatially dispersive dielectrics have been detected

experimentally by attenuated total reflection [1-6].

In this method an electromagnetic wave is incident

on a prism which is separated by a small gap from the surface of the dielectric. For angles of incidence

in the range of total reflection, surface exciton-

polaritons are excited via the evanescent waves.

Although it is known that the exciton parameters near the surface may differ from their bulk values [7-12],

this deviation is usually neglected in ATR calculations.

Sometimes the effect of the surface is described in a

simplified way in terms of an exciton free surface

layer, where the transition from the bulk to the dead

layer is discontinuous [13]. Calculated ATR spectra

are found to depend on the choice of the ABC which

are employed at the surface of the dielectric (or at the bulk-dead layer interface).

We have recently presented a method for calculat-

ing the reflectivity, for both S and P polarizations,

in which the effect of the surface on the excitons is

represented by a continuous surface potential U(z) [14]. We are referring to the geometry of a semi- infinite dielectric at z > 0, having a dielectric constant

I

Here co is the background dielectric constant, Q)T is the frequency of the transverse resonance, cop is a

measure of the oscillator strength, and y is the damp-

ing constant. Spatial dispersion enters through the

term Dq2, with D

=

1iwT/M, where M is the exciton

mass. We have subsequently shown that if the height

of the potential at the boundary, U(o), is not too small, the calculated reflectivity turns out to be inde-

pendent of the choice of the ABC [15J. In the present work we present an analogous method for the cal-

culation of ATR spectra.

We consider the ATR configuration of figure 1.

Fig. 1.

-

Geometry of ATR experiment.

The gap, with a dielectric constant Eg, is bounded by the planes z

=

0 and z

= -

d, and the half space z - d represents the prism and has a dielectric constant ep.

Since only P polarized light interacts with the surface

Article published online by EDP Sciences and available at http://dx.doi.org/10.1051/jphys:01986004702025900

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260

exciton-polaritons, we take the incident field to be of the form

where k2 = k2x

,

+ kz

=

Ep w2/c2. The reflected field in the prism region is

The electric field in the gap

has, of course, the same x dependence as the incident field, and

The excitonic polarization and the electric field

inside the dielectric have to obey the following equa-

tions, which are obtained from Maxwell’s equations

and the exciton equation of motion [14]

Here

and an eitxX x dependence of the fields has been assum-

ed. Again, because of the translational symmetry in the direction parallel to the surface, qx

=

kx.

We know the explicit form of the solutions of

equations (5)-(7) deep inside the dielectric, outside

the range of the surface potential. Thus, for U(z)

=

0

these equations have the three well known solu- tions [16]

The qi of the transverse modes (9) are the two solu-

tions for qz of the bulk dispersion relation

where q2

=

q2x+ q 2, and qL, which appears in the

longitudinal mode (10), is the solution of

We integrate equations (5)-(7) numerically up to the surface z

=

0, starting from some large enough

z

=

zo, where U(z) is negligible. This is done three

times, with the three initial conditions defined by equations (9) and (10). The corresponding initial

electric field values follow from

where TB is the bulk value of r(z), i.e., with U

=

0.

Using the three solutions obtained by this numeri-

cal integration procedure, we write the general solu-

tion as a linear combination

Next, we determine the ratios AJA1 and A21A, from

the ABC, for which we assume the very general form

Applying these ABC at the surface of the dielectric,

z

=

0, we obtain

where all the polarization components and their derivatives are evaluated at z

=

0.

We now apply the Maxwell boundary conditions at the prism-gap interface, z

= -

d, and at the gap- dielectric interface, z

=

0. These require Ex and Hy to be continuous. We have presented above the electric fields in the three regions. The corresponding magnetic fields are readily calculated from the Maxwell equation H

=

-

i(clm) J7 x E. The Maxwell boundary conditions yield the following four equations

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where the field components and their derivatives in (21) and (22) are evaluated at z

=

0. Solving equations (19)- (22) we obtain the ratio of the reflected to incident field amplitudes

Here

where the fields are again evaluated at z

=

0.

The reflectivity is given by R = ) 1 ER/ Eo 12 and can

be calculated using the last three equations together

with (17) and (18).

We have performed numerical ATR calculations

using a surface potential of the form

This was done for ZnSe, using the bulk parameters 1imT

=

2.8022 eV, 1iwL

=

2.8034 eV, y

=

0.8 meV, so

=

8.1 [3]. In order to estimate physically reasonable

values for the surface potential parameters o-)B and a,

we first performed some calculations of normal inci- dence reflectivity for various choices of these para-

meters and compared the results with an experimental spectrum due to Lagois [5]. We have found that with a-)B

=

0.015 roT and a

=

3.5 nm the experimental

behaviour is satisfactorily reproduced, as shown in figure 2. We note that with this value of a%, U(0)

is large enough so that the calculated reflectivity is independent of the choice of the ABC [15].

Fig. 2.

-

Normal incidence reflectivity of ZnSe. The full

curve was calculated with the surface potential parameters COB

=

0.015 coy and a

=

3.5 nm. The broken curve shows the experimental results of Lagois.

A calculated ATR spectrum is shown in figure 3.

Fig. 3.

-

ATR spectrum of ZnSe calculated for d

=

70 nm, 0

=

550, ag

=

1, ap

=

2.18 and the surface potential para- meters COB

=

0.015 WT and

a =

3.5 nm.

This is again independent of the choice of the ABC.

Thus, in figure 4 we compare ATR spectra calculated for two choices of the ABC. One is the Pekar ABC

[17], defined by (16) with Px = pz:

=

0, and the other

is the Fuchs-Kliewer (FK) ABC [18], defined by

ax = pz: = 0. Without a surface potential, figure 4a,

there exists a considerable difference between the

two spectra. With a surface potential of height coB

=

0.005 wT, figure 4b, the difference is small. When me

is increased to 0.01 coT, figure 4c, the ATR spectra obtained with the two different ABC choices coalesce.

We note that this coalescence of the ATR spectra holds for any ABC of the general form (16). The FK and

Pekar ABC results shown here are just two examples.

These two ABC have been chosen because they are

known to yield the most diverging results in standard

reflectivity calculations (without a surface potential).

The exponential form for the surface potential was

used because of its simplicity. Numerical calculations

show that the ABC independence of the ATR spectra

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262

holds for other forms of U(z) as well, again providing

that U(O) is not too small.

In conclusion, we have presented a method for calculating ATR spectra of a nonlocal dielectric in which the effect of the surface is represented by a

continuous surface potential. As was also the case for S

and P reflectivities [15], for barrier heights which are

not too small the calculated ATR spectra turn out

to be independent of the choice of the ABC. This suggests that the importance of the ABC problem

has been overrated in the literature and that it is

more important to develop reliable quantum mecha- nical models for the evaluation of the surface potential.

Acknowledgments.

Helpful discussions with Professor R. Englman are gratefully acknowledged.

Fig. 4.

-

Comparison of ATR spectra of ZnSe calculated 1 with Pekar ABC (full curves) and FK ABC (broken curves).

(a) Without

a

surface potential; (b) with wB

=

0.005 COT,

a =

3.5 nm; (c) with wB

=

0.01 wT, a

=

3.5 nm. The other parameters as in figure 3.

References

[1] LAGOIS, J. and FISCHER, B., Phys. Rev. Lett. 36 (1976)

680.

[2] HIRABAYASHI, I., KODA, T., TOKURA, Y., MURATA, J.

and KANEKO, Y., J. Phys. Soc. Japan 43 (1977) 173.

[3] TOKURA, Y., KODA, T., HIRABAYASHI, I. and NAKADA, S., J. Phys. Soc. Japan 50 (1981) 145.

[4] LAGOIS, J., Solid State Commun. 39 (1981) 563.

[5] LAGOIS, J., Phys. Rev. B 23 (1981) 5511.

[6] SCHULTHEIS, L. and LAGOIS, J., Solid State Commun.

44 (1982) 1557.

[7] DAVYDOVA, N. A., MYASNIKOV, E. N. and STRASHNI- KOVA, M. I., Fiz. Tverd. Tela 15 (1973) 3332 [Sov. Phys. Solid State 15 (1974) 2217].

[8] SAKODA, S., J. Phys. Soc. Japan 40 (1976) 152.

[9] BALSLEV, I., Phys. Status Solidi (b) 88 (1978) 155.

[10] STAHL, A., Phys. Status Solidi (b) 106 (1981) 575.

[11] BALSLEV, I., Phys. Rev. B 23 (1981) 3977.

[12] SCHULTHEIS, L. and BALSLEV, I., Phys. Rev. B 28 (1983) 2292.

[13] HOPFIELD, J. J. and THOMAS, D. G., Phys. Rev. 132 (1963) 563.

[14] RUPPIN, R., Phys. Rev. B 29 (1984) 2232.

[15] ENGLMAN, R. and RUPPIN, R., Bull. Israel Phys. Soc.

30 (1984) 42;

RUPPIN, R. and ENGLMAN, R., Phys. Rev. Lett. 52

(1984) 1688.

[16] MARADUDIN, A. A. and MILLS, D. L., Phys. Rev. B 7 (1973) 2787.

[17] PEKAR, S. I., Zh. Eksp. Teor. Fiz. 33 (1957) 1022 [Sov. Phys. JETP 6 (1958) 785].

[18] FUCHS, R. and KLIEWER. K. L., Phys. Rev. B 3 (1971)

2270.

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