Investigation into Efficiency-Limiting Defects in mc-Si Solar Cells
Oras A. Al-Ani
1 ,a*
, Ahmed M. A. Sabaawi
1,b
, J. P. Goss
1 ,c
, N. E. B. Cowern
1,d
,
P. R. Briddon
1 ,e
and M. J. Rayson
2,f
1
School of Electrical and Electronic Engineering, Newcastle University, UK.
2
Department of Chemistry, University of Surrey, UK.
a
o.a.s.al-ani@ncl.ac.uk,
b
a.m.a.sabaawi@ncl.ac.uk,
c
jonathan.goss@ncl.ac.uk,
d
nick.cowern@ncl.ac.uk,
e
patrick.briddon@ncl.ac.uk,
f
m.j.rayson@surrey.ac.uk
Keywords: silicon; solar cells, interstitial iron; gettering; extended defects
Abstract. First-principles quantum-chemical simulations are combined with TCAD device modelling
to examine the impact of the intrinsic stacking faults and Σ
5
-(001) twist grain-boundaries on the per-
formance of solar cell efficiency. We find from the combination of these computational methods, the
optical properties of ideal stacking faults are similar to those of pure Si, whereas the optimised grain-
boundary leads to a clear change in the real and imaginary parts of refractive index, increasing the
solar-cell current density, and thus the solar cell efficiency. The impact at a device level is dependent
upon the areal density of such material. So far as the optically absorption and carrier generation is
concerned, segregation of diffusing iron at these planar defects has a negligible impact on device
characteristics, but non-radiative recombination processes and carrier traps due to iron are expected
to significantly affect efficiency in these regions.
Introduction
Cost reduction of photovoltaic (PV) material is an important issue in the development of future eco-
nomic fabrication of solar cells. Currently, relatively expensive waferbased crystalline-Si represents
the majority (more than 80%) of the PV market [1], but multicrystalline silicon (mc-Si) can offer a
more cost-effective option to gain reasonable cell efficiency compared with crystalline Si [2]. The
main problem with mc-Si is that it generally contains high concentrations of extended defects (EDs)
and transition elements present during module fabrication [3], with iron arguably the most important
impurity in lower-grade silicon [4, 5]. Interstitial iron (Fe
i
) is understood to be an active recombina-
tion centre, lowering device efficiency even at less than 1 ppb [6]. Furthermore, recombination, mo-
bility reduction and minority carrier lifetime effects are directly associated with the both impurity and
structural imperfections in the crystal structure, and hence, degrade the solar cell performance [6, 7].
However, the deleterious effects of EDs and Fe may be mitegated by gettering Fe in the form of
precipitates at EDs [8, 9]. Despite numerous theoretical [10, 11] and experimental [8, 12, 13] studies
reflecting the interest in the properties of EDs in Si, there is relatively limited understanding of the
mechanisms for iron gettering at GBs at an atomistic level. Thus, it is crucial to develop a fundamental
understanding of the mechanism of the attractive interaction (segregation) between EDs in mc-Si and
diffusing Fe, and the subsequent impact upon PV efficiency. A recent study investigated the electronic
and optical properties of different GBs structures on the PV performance [7], and here we present the
results of a similar study to resolve the likely impact of intrinsic stacking faults (ISF) and Σ
5
-(001)
twist grain-boundaries (GBs), including some reflection upon the effects of Fe
i
at these EDs.
Methodology
Different structures of doped and un-doped planar defects were modelled using density-functional the-
ory, under the local-density approximation, as implemented in Ab Initio Modelling Program (AIM-
PRO) [14]. Details of the simulation systems, their optimisation and energetics are provided else-
where [15].
Solid State Phenomena Submitted: 2015-05-27
ISSN: 1662-9779, Vol. 242, pp 96-101 Accepted: 2015-05-28
doi:10.4028/www.scientific.net/SSP.242.96 Online: 2015-10-23
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