(GaAl) As hetero-junctions

(GaAl) As hetero-junctions

Journal of Luminescence 40&41 (1988) 763 764 North-Holland, Amsterdam 763 PHOTOLUMINESCENCE RELATED TO THE INTERFACE OF GaAs/(GaA1)As HETERO—JUNCTIO...

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Journal of Luminescence 40&41 (1988) 763 764 North-Holland, Amsterdam

763

PHOTOLUMINESCENCE RELATED TO THE INTERFACE OF GaAs/(GaA1)As HETERO—JUNCTIONS

W. OSSAU, E. BANGERT, C. LANDWEHR Physikalisches

Institut

der UniversitBt WUrzburg, Ri5ntgenring 8, D—87 Wiirzburg, ERG

W. Forschungsinstitut

der Deutschen Bundespost beim FTZ, D—61 Darmstadt, FRG

We have investigated an unusual new line observed in CaAs/(AlCa)As hetero—junctions, referred to as the H—band, by low—temperature photoluminescence experiments in magnetic fields up to 9.5 T. ‘Ihe direction of the magnetic field was turned from perpendicular to parallel to the interface. From the energetic shift, the splitting—behaviour, the lineshape and the temperature dependence of the luminescence line, we conclude that the H—band is emitted by the recombination of a flat—band electron with a hole confined to an excited subband.

1. Introduction

________________________________________

In the low temperature photolumirsescence spectrum of GaAs/(A1Ga)As heterostructures

an

unusual new line has been observed, referred to 1 which seems to be related to as the H—band, the interface. Up to now, however, there is no



convincing experimental evidence that the line

.-

is connected with the interface. 2. Experimental Results

-

E

The p—type GaAs/(AlGa)As—heterojunctions used



-

— -

*

,r~

-

.4”.

~..

thicknesses (9.5 nm < d < 53 mm), and aluminium concentrations of the (GaA1)As layers (0.5 < x

+5

-‘-

-

,_

in this study were grown by MBE. We investigated samples with different doping levels, space r—

-

+

z

-‘

W

<0.65) in order to observe the dependence of the photoluminescence spectrum on these parameters. The energy difference

B II z

E of the H—band to the

fundamental gap varies between 7 and 15 meV. From our study of 8 p—type samples we conclude that the

E increases with increasing aluminium

0

concentration and decreasing spacer—thickness. In a magnetic field perpendicular to the interface the H—band splits into four components with different polarization. The photon energies of the peak positions are plotted as a function of magnetic field in Fig. 1. We observe a linear

0022 2313/88/$03.50 © Elsevier Science Publishers B.V. (North-Holland Physics Publishing Division)

1

2

3

4

5

6

MAGNETIC FIELD

7

8

9

10

CT)

FIGURE 1 Peak positions of the H—band and the acceptor bound exciton as a represent function of—, magnetic strength. Crosses dots + field polari— zation of the H—band. The squares indicate the shift and splitting of the acceptor bound exci— ton

W~Ossau et al

764

/

Interface of GaAs

(GaA1)As heterojunctions

shift and splitting with magnetic field for the

the lowest electron Landau—level, we conclude

three low energy lines. The fourth component

that the H—band luminescence is caused by the

seems to have another origin. That it behaves

recombination of a free conduction band electron

qualitatively different can be seen by extrapo—

in the flat—band region with a hole confined in

lating the non—linear curve in Fig. To prove the conjecture

1 to B

=

0 T.

that the H—band is

subbands of a two—dimensional hole gas in a

correlated to the interface we have varied the angle

one of the aubbands near the interface. Electric magnetic field have been calculated in the self— 2 If we compare consistent Hartree—approximation.

between magnetic field and sample nor—

mal. The splitting of the H—band is a linear

these

function of the cosine of the angle between

small shift of the Fermi—energy towards the

interface and magnetic field. This means that

valence band, caused by the photoexcitation, we

the splitting is a function of the effective

find that the final state of the H—band recombi—

magnetic field strength normal to the inter—

nation fits well with the second heavy hole

face. When the magnetic fields is parallel to

subband. The three components shifting linearly

the interface the H—band shows no splitting. For

are attributed to the first three Landau—levels

this field direction the shift of the remaining

of this subband. The fourth component visible in

component is still linear with magnetic field

high magnetic fields (Fig. 1) coincides with the

and about 8.4 meV at 10 T. This energy shift is

first

gleater than that of bound exciton lines

and

calculations with the data and consider a

light hole subband only 1 meV apart.

The proposed transition is indirect in real

nearly identical with that of the first Landau—

space. Because the recombination between conduc—

level of GaAs conduction band electrons (8.6

tion band electron and subband hole depends on

meV).

the overlap of the wave functions,

Furthermore, the line shape of the H—band

a transition

can described very well by the product of the

to the highest subband is not probable. The

density of states function of conduction band

calculations show that for the sample discussed

electrons and a Boltzman—factor.

in this paper the wavefunction connected with

For a lattice

temperature of 10 K we obtain from the line

the first excited subband vanishes only at dis—

shape and effective

tances from the interface as large as 50 nm.

electron temperature of

about 24 K. This shows unambiguously that the

Consequently, the assumption of sufficient

the photoexcited

lap of the electron and hole wavefunctions is

carriers

have lost their excess

energy and are cooled via carrier—phonon

not unreasonable.

scattering.

Acknowledgements:

3. Discussion

over—

The work was supported by the Deutsche

From the energy shift in a magnetic field it

Forschungsgemeinschaft.

is obvious that the electron and the hole causing the luminesce are not bound by Coulomb interaction. Excitonic binding would result in a non—linear — diamagnetic — shift, much smaller than the one observed. The angular dependence the line in a magnetic field clearly indicates

two—dimensional behaviour. As the shift in pa— rallel fields corresponds to that expected for

of

References: 1. Y.R. Yuan, M.A.A. Pudensi, G.A. Vawter and J.L. Merz, J. Appl. Phys. 58, 397, 1985

2. E. Bangert and G. Landwehr, Superlattices and Microstructures, 1, 363, 1985.