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Photocurrent spectroscopy of self assembled InAs/GaInAsP/InP(113)B quantum dots

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HAL Id: hal-00727159

https://hal.archives-ouvertes.fr/hal-00727159

Submitted on 3 Sep 2012

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Photocurrent spectroscopy of self assembled InAs/GaInAsP/InP(113)B quantum dots

Abdallah Sakri, Patrice Miska, Charly Platz, Daniel Lemoine, Jacky Even, Olivier Dehaese, Karine Tavernier

To cite this version:

Abdallah Sakri, Patrice Miska, Charly Platz, Daniel Lemoine, Jacky Even, et al.. Photocurrent spec- troscopy of self assembled InAs/GaInAsP/InP(113)B quantum dots. GDR Nanoélectronique Journées Scientifiques, Jan 2003, Grenoble, France. �hal-00727159�

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GDR Nanoélectronique – Journées Scientifiques – 28/31 Janvier 2003

Photocurrent spectroscopy of self assembled InAs/GaInAsP/InP(113)B quantum dots.

A. Sakri, P. Miska, C. Platz, D. Lemoine, J. Even, O. Dehaese, K. Tavernier

Laboratoire d’Etude des Nanostructures Semiconductrices (LENS), INSA-Rennes, 20 avenue des Buttes de Coesmes 35043 Rennes Cedex, France [email protected]

1- Introduction

In this paper we present photocurrent (PC) spectroscopy of InAs/InP(113)B quantum dots (QD) as a function of bias and temperature. The PC spectra reflect the optical absorption of the QDs layers and reveal the QD electronic structure. A simple model, used to determine the energy levels into the QDs, gives results consistent with the PC spectra. Morever, the PC signal is governed by a competition between recombinaison and escape processes (themal and tunneling escape) of photogenerated carriers.

2- Experiments

We have investigated InAs/GaInAsP/InP(331)B QDs bureid in a p-i-n laser jonction. The growth on InP(113)B substrate yields smaller QDs with higer density than on InP (100) substart [1]. Morever, the QDs are performed with the double cap (DC) grouth technique which enables us to control their average heigth at 3nm. Lasing emission has been observed on laser structure respectively at 1.4µm and 1.5µ m at room temperature on the ground (GS) and the first excited states of such QDs[2].

As shown in figure 1, the QDs PC signal obtained at 4K rise with increasing the reverse bias. Evolution spectra shows saturation effects for bias below –3V.

This value is in agreement with C(V) mesurements.

The QD energy states redshift weakly with increasing reverse bias. This shift may be do to a size selective tunneling effects [3] and a quntum confined Stark effect (QCSE) [4, 5].

We show(figure 2) the dependence temperature PC spectra. We observed that carriers extraction from QDs to the barrier is gouverned by faster thermal escape at high temperatures and by tunneling escape process at low temperatures.

3- Simulation

Simple calculations of the electronic levels have also been performed by solving the single particle Schodinger equation in cylindrical coordinates [4]. A one band model with effective masses taking into account strain effects in the dots gives results consistent with PC experiments. It allows us to identify the 1s-1s (GS) and 1p-1p (ES) transitions occuring.

Figure 1 : photocurrent (PC) spectra mesurement as function of reverse bias at T=4K for bias (V=0.1V ; 0V ; -0.25V ; -0.5V ; -1V ; -2V ; -3V).

Figure 2 : The temperature dependence PC spectra at bias Vp=-1V.

References

[1]C.Paranthoen, N.Bertru, O.Dehaese, A.Le Corre,

S.Loualiche,B.Lambert "

Appl. Phys. Lett., 78 (2001) 1751.

[2] (65) C. Platz, O. Dehaese, A. Le Corre, C. Paranthoen, J. Even, G.Moreau, N. Bertru, H.Folliot, P. Miska, C. Labbé, S. Loualiche Proceeding of the International Conference on the Physics of semiconductors (ICPS) IOP Publishing

[3]W. H. Chang, T. M. Hsu, C. C. Huang, S. L. Hsu and C. Y. Lai, Phy. Rev B 62 6959 (2000)

[4]P.Miska, C. Paranthoen, J. Even, N. Bertru, A. Le Corre, O.

Dehaese

J. Phys. C : Condens. Matter, 14, 12301 (2002)

[5]A. Patanè, A A. Levin, A. Polimeni, F. Schindler, P. C. Main, L.

Eaves, and M. Hini,

Appl. Phys. Lett. 77 2979 (2000).

0.8 0.9 1.0 1.1

GSQ1.18 WL ES GS

4K

Photocurrent (arb. units)

Energy (eV)

-3V -2V -1V -0.5V -0.25V 0V +0.1V

0.80 0.85 0.90 0.95 1.00

WL

ES GS

VP = -1V 300K

200K 150K 110K 90K 77K 4K

Photocurrent (arb. units)

Energy (eV)

Références

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