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Quantum and conversion ef fi ciencies optimization of superstrate CIGS thin- fi lms solar cells using In 2 Se 3 buffer layer

Idris Bouchama

a

, Samah Boudour

a,b,c

, Nadir Bouarissa

d,*

, Zahir Rouabah

e

aElectronic Department, Faculty of Technology, University M. Boudiaf, 28000, Msila, Algeria

bResearch Centre in Industrial Technologies CRTI, P.O. Box 64, Cheraga, 16014, Algiers, Algeria

cThin Films and Applications Unit (UDCMA), Setif, Algeria

dLaboratory of Materials Physics and its Applications, University of M'sila, 28000, M'sila, Algeria

eMaterials and Electronic Systems Laboratory, University of Bordj-Bou-Arreridj, 34000, Bord-Bou-Arreridj, Algeria

a r t i c l e i n f o

Article history:

Received 27 March 2017 Received in revised form 26 May 2017

Accepted 30 May 2017

Keywords:

Cu(In,Ga)Se2material Superstrate solar cells Transparent conducting oxides Barrier height

AMPS-1D

a b s t r a c t

In this present contribution, AMPS-1D device simulator is employed to study the performances of superstrate SLG/TCO/p-Cu(In,Ga)Se2(CIGS)/n-ODC/n-In2Se3/Metal thinfilm solar cells. The impact of the TCO and Metal work functions on the cell performance has been investigated. The combination of optical transparency and electrical property for TCO front contact layer is found to yield high efficiency. The obtained results show that the TCO work function should be large enough to achieve high conversion efficiency for superstrate CIGS solar cell. Nevertheless, it is desirable for Metal back contact layer to have low work function to prevent the effect of band bending in the n-In2Se3/Metal interface. Several TCOs materials and metals have been tested respectively as a front and back contact layers for superstrate CIGS solar cells. An efficiency of 20.18%, withVocz0.71 V,Jscz35.36 mA/cm2andFFz80.42%, has been achieved with ZnSn2O3-based as TCO front contact layer. In the case of SnO2:F front contact and indium back contact layers, an efficiency of 16.31%, withVocz0.64 V,Jscz31.4 mA/cm2andFFz79.4%, has been obtained. The present results of simulation suggest an improvement of superstrate CIGS solar cells efficiency for feasible fabrication.

©2017 Elsevier B.V. All rights reserved.

1. Introduction

CuIn1-xGaxSe2(CIGS) has a major potential as a semiconductor material for thinfilm photovoltaic devices. This is due to its high optical absorption coefficient, appropriate band gap and outstanding electro-optical properties[1e3]. CIGS-based solar cells with x¼0.3 corresponds to a bandgap energy range of 1.1e1.2 eV yields the best efficiency both in laboratory and commercial solar cells [4,5]. Recently CIGS thin film solar cells approached effi- ciencies of 22.8% for substrate configuration [6]. The superstrate configuration is an alternate design, where the deposition sequence is reversed, the absorber is grown on glass coated with the trans- parent front contact (TFC), followed by an evaporated CdS or In2Se3

buffer layers andfinished by a sputtered metallic back contact layer [7e9]. Further improvements of the superstrate CIGS solar cells performance require an accurate knowledge of the electronic loss

mechanisms.

The properties of Transparent conducting oxide (TCO)films, such as resistivity, band-gap energy and work function, affect obviously the performance of solar device because they affect both the energy barrier height at the heterojunction interfaces and the electronfield emission [10]. TCOfilms are n-type degenerated semiconductors (metallic oxides), they are formed from binary oxides, such as In2O3, SnO2and ZnO; ternary oxides, such as Zn2In2O5, Zn2SnO4, CdSb2O6, MgIn2O4, ZnSnO3, GaInO3, and In4Sn3O12 and multi-component oxides composed of combinations of these binary or ternary ox- ides[11]. The work function of the TCOfilms (WTCO) has a critical importance in optoelectronic device performance, the change in work function and electron/hole injection barrier is related to the band alignment[12e14]. Ritzau et al.[15]have reported the role of the work function and back contact barrier height on the perfor- mance of a-Si:H solar cells. Besides, Belfar et al.[16]investigated the effect of WTCOfor the performance of neiepþand neiepepþsolar cells based on hydrogenated amorphous silicon (a-Si:H) and hy- drogenated nanocrystalline silicon (nc-Si:H) absorber layers using AMPS-1D simulation tools. Furthermore, Hussain et al.[17]reported

*Corresponding author.

E-mail address:n_bouarissa@yahoo.fr(N. Bouarissa).

Contents lists available atScienceDirect

Optical Materials

j o u r n a l h o m e p a g e : w w w . e l s e v i e r . c o m/ l o ca t e / o p t m a t

http://dx.doi.org/10.1016/j.optmat.2017.05.056 0925-3467/©2017 Elsevier B.V. All rights reserved.

Optical Materials 72 (2017) 177e182

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