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3D-Modelling of polycrystalline silicon solar cells
J. Dugas, J. Oualid
To cite this version:
J. Dugas, J. Oualid. 3D-Modelling of polycrystalline silicon solar cells. Revue de Physique Appliquée, Société française de physique / EDP, 1987, 22 (7), pp.677-685. �10.1051/rphysap:01987002207067700�.
�jpa-00245596�
3D-Modelling of polycrystalline silicon solar cells
J.
Dugas
and J. OualidLaboratoire des Matériaux et
Composants Semiconducteurs,
Ecole NationaleSupérieure
dePhysique
de Marseille, Domaine Universitaire deSt-Jérôme,
13397 Marseille Cedex 13, France(Reçu
le 29septembre
1986,accepté
le 8 décembre1986)
Résumé. 2014 Nous nous intéressons à l’influence des
joints
degrains
sur lesprincipaux paramètres qui
caractérisent les
photopiles
en siliciumpolycristallin.
Nous calculons la vitesse de recombinaison effective à l’aide d’une méthode auto-consistantequi
tient compte de la courbure duquasi-niveau
de Fermi des minoritaires dans larégion
decharge d’espace
associée aujoint
et dans larégion quasi
neutre desgrains.
Ennous basant sur cette
étude,
nous avons tracé à l’aide d’un modèle à 3 dimensions une séried’abaques qui
permettent deprévoir
les variations despropriétés photovoltaïques
en fonction desgrandeurs caractéristiques
d’un matériau semiconducteur
polycristallin : dimension g
desgrains, longueur
de diffusionLn
etdopage NA
desgrains
et vitesse derecombinaison
interfaciale S auxjoints
degrains.
Nous montrons que le rendement peut êtreaugmenté
enajustant
ledopage
de la base desphotopiles.
Ledopage optimum
est donné en fonctionde la densité des états d’interface et de la dimension des
grains. Enfin,
nous définissons unelongueur
dediffusion effective dans un matériau
polycristallin
prenant en compte la recombinaison auxjoints
degrains.
Cette
longueur
de diffusion effectivepeut
être mesurée par la méthode de laphototension
de surface(SPV).
Nous en avons déterminé les variations en fonction de
S, Ln
et g. Cettegrandeur
permet deprévoir
une valeurapprochée
despropriétés photovoltaïques.
Abstract. 2014 This work is concerned with the effect of
grain
boundaries(gb)
on the main parameters which characterizepolycrystalline
silicon solar cells. The variation with illumination of thegrain boundary
effectiverecombination
velocity
has been calculatedby
means of a self-consistentprocedure
which takes into account thebending
of theminority
carrierquasi-Fermi
level in thespace-charge region
and in thegb quasi-neutral region.
Abaci have beenplotted
which allow topredict
thephotovoltaic properties
as a function of the characteristicquantities
of apolycrystalline
material:grain
size g, diffusionlength Ln
anddoping
concentration in the
grains
and interfacial recombinationvelocity S
at thegrain
boundaries. It is shownby
means of a 3D-model that the conversion
efficiency
can be enhancedby optimizing
thedoping
concentration of the base of thecells ;
theoptimum doping
level and the relatedefficiency
aregiven
as a function ofgrain
sizefor different interface state densities.
Finally,
an effective diffusionlength taking
into account thegb
recombination is introduced. This effective diffusion
length
can be measuredby
the SurfacePhoto Voltage (SPV)
method. Its variation as a functionof S, Ln and g
have been determined. Thisquantity
allows to forecastapproximate
values of thephotovoltaic properties.
Classification
Physics
Abstracts86.30J - 73.20
Introduction.
Polycrystalline
silicon is different frommonocrystal-
line silicon
essentially
due to the presence ofgrain
boundaries
(gb)
which act as recombination centres for excess carriers[1, 2]
and which contribute to amarked
decrease
of solar cell efficiencies[3-6].
Thegb
recombination of the excess carriers takesplace
via the
gb
interface states which can be due to thedangling bonds,
thedislocations,
or theimpurities segregated
or diffused into thegrain
boundaries.This
gb activity
is well definedby
an interfacial recombinationvelocity.
As the interface states are
generally charged,
aband
bending
appears near agb
characterizedby
abarrier
height Egb
and a spacecharge region (SCR)
of width
Wgb
which lies on each side of thegb (Fig. 1).
Thehigh
electric field in this spacecharge region
drifts theminority
carriers towards thegb
andcontributes to an enhancement of their recombi- nation.
Therefore,
from apractical point
ofview,
itis
interesting
to consider aneffective
recombinationvelocity [7]
which takes into account the presence of thegb
barrierheight.
Thecharge
of thegb
interfacestates
depends
on the level of excitationwhich,
inthe case of a solar
cell,
is related to theintensity
ofArticle published online by EDP Sciences and available at http://dx.doi.org/10.1051/rphysap:01987002207067700
678
wGB
Fig.
1. - Banddiagram
at thevicinity
of agrain boundary
in a p-type illuminated semiconductor. SCR :
gb
spacecharge region ;
QNR :quasi-neutral region ;
NR : neutralregion.
the incident
light.
The excess carriers due to thelight
tend to saturate the
gb
interface states so that thegb
barrier
height [8]
andconsequently
the effective recombinationvelocity [9]
decrease as the excitation level increases.The numerical results
presented
here are con-cerned with interface states distributed with a
density Nt
per unit area on asingle
energy levellying
atmidgap,
which is the most effective for carrier recombination. The model has been extended to different interface state distributions[10].
Thecharge
of states isgiven by
the half-filled band model(HFB) [11]
in which apair
of states is associated with eachdangling bond ;
this model is often used in thecase of undissociated dislocations
[12]
and can beapplied
to lowangle gb
which can be considered as aline of dislocations.
Before
studying
the behaviour of such apolycrys-
talline silicon solar
cell, by
means of a 3D-modeldeveloped
in section2,
we haveestablished,
insection
1,
the variation of thegb
barrierheight Egb
and of thesubsequent
effective recombinationvelocity Seff
under different excitation levels for different interface state densities anddoping
concen-trations. Section 3 is devoted to the definition of an
effective diffusion
length Leff
which takes into ac- count the recombination at thegrain
boundaries.Modelling
this effective diffusionlength
isparticu- larly interesting
since it can be measuredby
theSurface Photo
Voltage
method and is able togive
anestimation of the
photovoltaic performances
of apolycrystalline
material.1. Grain
boundary
under illumination.In the
present work,
thebending
of theminority
carrier
quasi-Fermi
level in thegb
spacecharge
region (L11)
and in thegb quasi-neutral region (03942)
has been taken into account. In contrast to theanalysis given by Seager [9]
basedpartially
on thethermoionic emission
model,
we have usedonly
theShockley-Read-Hall theory
for the self-consistent determination of thegb
barrierheight Egb
and theeffective ’ recombination
velocity Seff.
Figure
1gives
a schematicrepresentation
of thevariation of the energy bands and the
quasi-Fermi
levels with the distance x at a
gb
under illuminated conditions for ap-type
semiconductor. In thismodel,
we assume that :
a)
Under low and medium excitationconditions,
the
quasi-Fermi
level of themajority
carriersEFp
is flateverywhere
but thequasi-Fermi
level ofthe
minority
carriersEFn
is allowed to vary in the spacecharge region (- Wgb
xWgb )
as well as inthe
quasi-neutral region
asproposed by Seager [9].
b)
Theoccupation probability f (under
nonequilibrium conditions)
and the carrier recombi- nation rateUB
aregiven by
theShockley-Read-Hall
expressions [13].
,c)
The excitation is uniform in the base of the solar cell. This isactually
the caseonly
forlong wavelength
illumination for which theabsorption
coefficient is
nearly
constant within the base. The excitation level is characterizedby
the differencebetween the
quasi-Fermi levels, EFn - EFp,
in theneutral
region
of thegrains.
On the basis of these
assumptions,
thegb
barrierheight Egb
and the effective recombinationvelocity
are determined
self-consistently.
The variations of the
bendings 03941
andlà2
as afunction of the excitation level
EFn - EFp
in the bulk of thegrains
are shown infigure
2. Thebending
ofthe
minority
carrierquasi-Fermi
level isalways
muchlarger
in thequasi-neutral region
than in thegb
space
charge region
as obtained alsoby Seager [9].
In this
figure,
it is exhibitedthat 2l
may beneglected
at very low or very
high excitation,
but’à2
isalways quite significant. So,
theminority
carrierquasi-
Fermi level can be assumed to be flat in the
gb
spacecharge region
and with a lessdegree
ofvalidity
in thequasi-neutral region only
in theselimiting
cases. Theflat
minority
carrierquasi-Fermi
levelapproximation
may be
adopted only
at very low excitation due to the smallminority
carrier flux or athigh
excitationdue to the decrease of the
gb
effective recombinationvelocity. 03941
andlà2
are maximum for a critical excitation level whichdepends
on thegb
interfacestate distribution and on the
doping
concentration in thegrains.
The variation of the effective recombination vel-
ocity Seff
as a function of the excitation level is shown infigure
3 for different interface state densitiesNt
and for differentdoping
levelsNA.
For agiven
Fig.
2. -Bendings
of theminority
carrierquasi-Fermi
level in the
gb
spacecharge region (03941)
and in thequasi-
neutral
region
of theadjacent grain (’à2) vs
the excitation level.Doping
concentrationNA
=1016 cm-3 ;
diffusionlength Ln
= 50 03BCm.excitation, Seff (and. Egb)
increasesalways
withNt (Fig. 3a)
whereasSeff (and Egb)
decreases as thedoping
level becomessufficiently large (Fig. 3b).
Wehave
demonstrated
that the recombinationvelocity Seff
cannot exceed alimiting
value which is about the half of the thermalvelocity
vth[13].
Theasymptotic
behaviour of
Seff
towardsvth/2
when thedensity
ofstates is
large
is obvious infigure
3. It is worthnoting
Fig.
3. - Variation of the effective recombinationvelocity Seff
with the excitation levela)
for different interface state densities.1) Nt = 4 1011 cm-2 ; 2) Nt = 6 1011 cm-2 ; 3) Nt = 8 1011 cm- 2 ; 4) Nt
=1012 cm- 2 ; 5) Nt = 5 1012
cm-2.
b)
for differentdoping
concentrations.1) NA = 1015
cm-3 ; 2) NA
= 3 x 1015cm-3 ; 3) NA = 1016 cm- 3 ; 4) NA = 3 x 1016 cm- 3 ; 5) NA = 1017 cm-3.
REVUE DE PHYSIQUE APPLIQUÉE. - T. 22, N° 7, JUILLET 1987
680
that
Seff
remains constant up to an excitation levelEfn - Efp
= 0.5 eVcorresponding
to about the maxi-mum power
point
of a solar cell under AM1 illumination. This result allows tosimplify signifi- cantly
theanalysis developed
in the next section.2. Solar cell 3D-model.
2.1 HYPOTHESES. - The
grains
have been assumedto have
homogeneous properties (doping
concen-tration, minority
carriermobility,
recombination lifetime and difusionlength),
and to befibrously oriented,
i.e. all thegrain
boundaries are perpen- dicular to the front and back surfaces and conse-quently
to thejunction.
For the sake ofsimplicity,
we have assumed a square cross section
(side g)
forthe
grains (Fig. 4).
Theanalysis
can beeasily
ex-tended
to arectangular grain shape [14],
e.g. in thecase of ribbons.
Fig.
4. - Model of a squaregrain (side g). We
andWb
are the widths of the emitter and the base of thecell, respectively.
Theorigin
of the axes is in thejunction plane,
the x- and y-axes areperpendicular
to thegrain boundaries,
the z-axis isperpendicular
to thejunction.
As the emitter
region is heavily doped, Seff
is very small in thisregion
as shown above and thegb
recombination in the emitter is therefore
negligible [15].
We have alsoneglected
thegb
recombination in thejunction
spacecharge region
since we haveshown in a
previous
work[16]
that thegb
barrierheight
isstrongly
reduced in thisregion,
in agree- ment with the results of Green[17]. Therefore,
thecontributions of these two
regions
have been calcu-lated
using
the classical one-dimensional model[18].
The series
resistance
due to the basematerial,
whichvaries as the
doping
concentration isvaried,
hasbeen taken into account but limitations which
might
be introduced
by
the series resistances due to theemitter,
thegrid
or the back ohmic contact have notbeen taken into account since
they depend strongly
on the process involved.
Therefore,
the resultsgiven
in this paper must be considered as an upper limit of what can be
expected
frompolycrystalline
siliconsolar cells.
The
photocurrent,
for agiven
illumination and for short-circuitconditions,
is derived from the excessminority
carrier concentration àn in agrain
whichcan be written as an infinite series
[14].
Similarexpressions
are used for the darkminority
carrierconcentration needed to
compute
the dark saturationcurrent
[10].
2.2 PHOTOVOLTAIC QUANTITIES. - The
photovol-
taic
quantities
understudy,
short-circuitphotocur-
rent, dark saturation current, open circuit
voltage,
fill factor and
efficiency,
have beencomputed
andplotted
as a function of one of thefollowing
macro-scopic quantities [10] :
- the effective recombination
velocity Seff
de-fined in the
previous section,
which characterizes the electronicactivity
of thegrain boundaries ;
- the diffusion
length Ln,
which characterises the recombination of theminority
carriers in thegrains ;
- the
grain size g
which isobviously
the funda-mental
parameter
forpolycrystalline
materials.It has been found that the
degradation
of thephotovoltaic properties,
withrespect
to a monocrys-talline silicon
cell,
is small as the effective recombi- nationvelocity
is less than103
cm/s whereas astrong
variation is observed in the range103 Seff 105 cm/s, particularly
a drastic increase of the dark saturation current.Larger
effective recombination velocities do not affectsignificantly
more thephoto-
voltaic
properties.
Increasing
the bulk diffusionlength Ln provides
an enhancement of the
photovoltaic properties
up toa saturation value which
depends
on thegrain
size.As an
example,
the conversionefficiency
has beenplotted
infigure
5 as a function of the ratiog/2 Ln
for different values of the bulk diffusionlength Ln.
It can be seen thatincreasing
thegrain
size more than ten times the bulk diffusion
length
does not
improve significantly
the conversion ef-ficiency.
In the case of a diffusionlength Ln
=100 03BCm, which is
usually
measured inpolycrystalline
silicon wafers like Silso-Wacker or
CGE-Polyx,
conversion efficiencies
greater
than 14 % can beexpected
if thegrain
size isgreater
than 2 mm.These results confirm
that,
in agettering
process,preference
must begiven
to the reduction of thegb activity
for « small »grain
materials and to thepassivation
ofintragrain
defects for« large » grain
Fig.
5. - Variation of the conversionefficiency
vs. thescaled
grain
size.NA
=1016 cm-3 ; S = 106 cmls ;
basethickness : 500 Fim. Bulk diffusion
length :
1) Ln
= 25 03BCm;2) Ln
= 50 03BCm ;3) Ln
= 75 03BCm ;4) Ln
= 100 ktm ;5) Ln
= 150 f.Lm.materials,
« small » and «large » being
defined withrespect
to thé diffusionlength.
2.3 BASE DOPING CONCENTRATION INFLUENCE. - Since an increase in the
doping
concentration level involves a reduction of thegb
effective recombi-nation
velocity [15],
it appearspossible
to achievebetter
photovoltaic performances by increasing
thedoping
level in thegrains. However,
themobility
and lifetime and
consequently
the diffusionlength
ofthe
minority
carriers decrease as thedoping
level isincreased.
So,
anoptimum doping
concentration canbe found which must result from a
compromise
between the
degradation
of the bulk electronicproperties
and the reduction of thegb activity
as thedoping
level is enhanced.Intragrain
defects(deep
levels introduced
by
dislocations orimpurities)
havenot been taken into account but
only
the unavoidable effects due to thehigh doping level, scattering
andAuger
effect inparticular. So,
theminority
carriermobility
can berepresented by
the relation :derived from the curves
given by
Adler et al.[19]
forsingle-crystal
silicon. Theminority
carrier lifetimehas been calculated from the relation
given by
Fossum
[20] :
As the base
doping
levelNA is
increased from1014 cm-3
to1018
cm-3, the
dark saturation current decreasesmonotonically
from some10-6 mA/cm2
to some10-10 mA/cm2 [21], joining
the value of asingle-crystal
cell for thisdoping
level. Due to thelessening
of the carrier diffusionlength,
the short-circuit
photocurrent Jph decreases, except
in a range ofdoping
concentration whereSeff
decreasesstrongly. Jph
is maximum for adoping
concentration whichdepends
on thegrain size
and on the interfacestate
density [21].
The variation of the conversion
efficiency
as afunction of the
doping
concentration isplotted
infigure
6 for differentgrain
sizes and for alarge density
of interface states. Themaximum
of theconversion
efficiency
is obtained for smallerdoping
concentrations and its
amplitude
is enhanced as thegrain
size is increased.Fig.
6. - Variation of the conversionefficiency
as afunction of the base
doping level,
for differentgrain
sizes :1) g
= 50 03BCm ;2) g
= 100 03BCm ;3) g
= 200 03BCm ;4)
g = 500 03BCm ;
5) single-crystal
cell.Base width :
Wb
= 370 f.Lm.Figure
7gives
the variation of theoptimum doping
concentration
NA opt
as a function of thegrain size,
for different interface state densities. The compu- tation has been limited tograin
sizes in the range 35itm-2 000
03BCm : forgreater grain sizes,
the efficien-cy passes
through
a broad maximum so that its determination is very inaccurate and has no interest whereas for smallergrain
sizes thepresent
model is lessadequate.
2022 the
optimum doping
concentrationNA opt
is allthe
greater
that thegrain size g
issmaller,
whateverthe interface state
density Nt.
2022 for a
given grain size, NA opt
increases withNt.
682
Fig.
7. -Optimum
basedoping
concentration as afunction of the
grain size,
for different interface statedensities :
1) Nt
= 3 x1011 cm-2 ; 2) Nt
= 5 x1011 cm-2 ; 3) Nt
=6 x
1011 cm-2 ; 4) Nt
= 8 x1011 cm-2 ;
Base width :
Wb
= 370 f.Lm.Emitter : n-type,
No
= 5 x 1019cm-3, We
= 0.2 f.Lm.Fig.
8. - Maximum conversionefficiency
as a function of thegrain
size when the basedoping
concentration isoptimized,
for different interface state densities :1) Nt
= 3 x1011 cm- 2 ; 2) Nt
= 5 x1011 cm- 2 ; 3) Nt
=6 x
1011 cm-2 ; 4) Nt
= 8 x1011 cm- 2 ;
Base width :
Wb
= 370 03BCm.Emitter :
n-type, ND
= 5 x 1019cm- 3, We
= 0.2 f.Lm.2022 as g increases or
Nt decreases, NA opt
tends tothe
optimum doping
concentration of asingle-crystal cell,
i.e. 3 x1015 cm- 3
for theparameters given
inthe
caption.
2022 linear and
parallel graphs
arefound,
forg 1 mm, in the
log-log diagram
offigure
7 so thata very
simple
numericalexpression
can begiven
tocalculate
Np
opt in so far as thegrain size g
and theinterface state
density Nt
are known :NA opt
= 10N1.4t g-
0.35(CGS units). (3)
The variation of the
corresponding
maximum ef-ficiency
isplotted
infigure
8. It can be noticed thatgood efficiency
levels(q
> 12%)
can beobtained,
even with small
grain
materials(g
= 3503BCm)
andvery active
grain
boundaries(Nt
= 8 x1011 cm- 2)
on condition that the base of the cell be
doped
at theoptimum
level.The relation between the
optimum doping
levelNA
opt, thegrain
size g and the interface statedensity Nt
can beparticularly
useful toengineers
who wantto
improve
theperformances
of solarcells
realizedon a
given polycrystalline
silicon on condition that :i)
theshape
and the dimensions of thegrains
arenot too different from one
another,
which allows to define asignificant
« meangrain
sizeg»
to be usedinstead of g.
ii)
an average valueNt representative
of thedifferent
gb
interface state densities can be intro-duced.
So, despite
therecombining activity
ofgrain
boundaries, good efficiency
levels can be obtainedwith
polycrystalline
silicon solar cells in so far as the basedoping
level isoptimized.
Thepresent
limita- tions of theefficiency
of cast or ribbon silicon solar cellsmight
be due tointragrain
defects which reducethe
grain
diffusionlength
or to theintergranular
diffusion of
impurities
which enhancesleakage
cur-rents.
As the
optimum doping
level ishigh,
the substratethickness can be reduced since the diffusion
length
issmaller ;
so, the cost of thephotocells
may be lowered.Moreover,
as a consequence of bothhigh doping
concentration and thinsubstrate,
the seriesresistance is
reduced,
which isfavourable
forhigh
excitation
(greater
than onesun)
inparticular.
3. Effective diffusion
length
andphotovoltaic
proper- ties.In
polycrystalline silicon,
an « effective diffusionlength »
is often defined in order to take intoaccount the
grain boundary
recombination.By
means of this
concept
of effectivequantities,
an« equivalent monocrystalline
cell »(EMC)
can bedefined as a cell whose diffusion
length
would beequal
to this theoretical effective diffusionlength
orto a measured one
[22, 23].
Thephotovoltaic
proper- ties of thepolycrystalline
cell are then assumed to be the same as those of the EMC.The purpose of the
present
section is to determineto what extent the EMC model can be used in order to calculate the
photovoltaic properties
from themeasurement of an effective diffusion
length Leff
inpolycrystalline
silicon[3, 5] by
means of the SurfacePhotoVoltage (SPV)
method[24].
This forecast is veryimportant
since this measurement isrelatively
easy and does not need the full realization of a solar cell which is arduous and
expensive.
It can be seen in
figure
9 that theplot
of thereverse of the
quantum efficiency Q
as a function ofthe reverse of the
absorption
coefficient acomputed
with our model is linear for
polycrystalline silicon
aswell as for
monocrystalline
silicon. Under this con-dition,
an effective diffusionlength Leff
can bedefined as the
intercept
with the x-axis of thestraight
line
1 / Q
=f(1/03B1). Leff depends
on thegrain size,
in
particular.
Fig.
9. - Variation of the inverse of the quantumefficiency
as a function of the inverse of theabsorption
coefficient.
Base : p-type,
NA
=1016 cm-3, Wb
= 500 )JLm.Emitter : n-type,
N,
= 5 x1019 cm-3, We
= 0.2 f.Lm.G.b.
effective
recombinationvelocity S =106
cmls.Bulk diffusion
length Ln
= 100 jim.Grain size and effective diffusion
length :
1) g
= 100 03BCm ;Leff
= 19.9 jim.2) g
= 200 03BCm ;Leff =
35.7 lim.
3) g
= 500 03BCm ;Leff
= 63.6 ktm.4) g
= 2 mm ;Lcff
= 92.4 ktm.The relation between this effective diffusion
length
and thephotovoltaic properties
has beencomputed
for different values of the material par- ameters(grain size,
bulk diffusionlength,
effectivegrain boundary
recombinationvelocity, doping level) [25].
The influence ofgrain
boundaries onLeff
when thegrain
size is small withrespect
to the bulk diffusionlength
is obvious infigure
10 whereLeff
isplotted
as a function of the ratiog/2 Ln
fordifferent bulk diffusion
lengths.
Figue
11 shows the variation of the conversionefficiency
as a function of the effective diffusionFig.
10. - Effective diffusionlength vs
the ratiograin
size/bulk diffusion
length. NA = 1016 cm-3 ; Wb
=500 03BCm ;
Wc
= 0.2 03BCm ;Seff = 106
cm/s.1) L,,
= 25 03BCm ;2) Ln
= 50 03BCm ;3) Ln
= 75 03BCm ;4) Ln
= 100 03BCm.Fig.
11. - Variation of the conversionefficiency
as afunction of the effective difusion
length,
for differentgrain
sizes :
1) g
= 100 iim2) g
= 200 itm ;3)’g
= 500 03BCm ;4)
g = 2 mm ;
5) equivalent monocrystalline
cell(EMC).
Base : p-type,
NA
=1016 cm-3 , Wb
= 500 03BCm.Emitter : n-type,
No
= 5 x1019 cm-3, We
= 0.2 jim.G.b. effective recombination
velocity S = 106
cm/s.length, in
the case of very activegrain
boundariescharacterized
by
an effective recombinationvelocity
S
= 106
cm/s. In order toget
a variation in the effective diffusionlength,
the « bulk » diffusionlength
has been varied from 10 p,m to 150 03BCm, for different values of thegrain size g (g = 100, 200,
500 ktmand g
= 2mm).
Curve 5 has been calculated in the case of theequivalent monocrystalline
cell(EMC),
i.e. whose diffusionlength
isequal
toLeff-
684
Note that the curves 1-3 cannot be
extrapolated
togreater
effective diffusionlengths
sinceLeff
is limitedfor a
given grain
size[25].
The most
important
remark is that there is not a one to one relation between the effective diffusionlength
and thephotovoltaic quantities.
The relationbetween these
quantities depends
on all the par-ameters
introduced in thisstudy,
i.e. thegrain size,
the bulk diffusion
length,
theg.b.
recombinationvelocity,
thegrain doping level...
Thedispersion
ofthe
experimental
resultsconcerning
the measure-ments of the short-circuit
photocurrent
as a functionof the effective diffusion
length [3, 6]
must not beonly
ascribed toexperiment
errors ; it can be at leastpartly explained by
this theoretical result.The
values
of the EMCphotovoltaic quantities
arealways
moreoptimistic
than thecorresponding
values
computed by
means of the 3D-model. The EMC short-circuitphotocurrent
can begreater
than thecomputed photocurrent by about
7%,
whereasthe EMC dark saturation current can be smaller
by
afactor of 2
[22].
The shift in the open circuitvoltages
is
relatively
small because of thelogarithmic depen-
dence of
Voc
on thecurrents,
but the EMC conver-sion
efficiency
can be overestimatedby
about1.5
point
if thegrain
size is small withrespect
to the bulk diffusionlength Ln (Fig. 10).
For agiven
effective diffusion
length Leff,
the shift is all the moresmaller that the
grain
size islarger
and the bulk diffusionlength
issmaller,
i.e. as the ratiog/Ln
isgreater.
Note that small
effective
diffusionlengths
can bedue either to small bulk diffusion
lengths
or to smallgrain
sizes. In the firstcase,
the EMC-model is able togive
agood approximation
of,the photovoltaic properties
whereas in the second case the EMC- modelgives only
a coarseestimation.
So,
it follows from thisstudy
that the EMC modelcan be useful for the
metallurgist
as a first test of theingots, particularly
forlarge grain
materials like Silso-Wacker silicon orCGE-Polyx silicon,
forwhich the
grain
size istypically greater
than 1 or 2 mm and bulkdiffusion lengths
are close to 100 03BCm.Conclusion.
A
self-consistentformulation
of thegb
barrierheight
and the
subsequent gb
effective recombination vel-ocity
versus the excitation level has beenestablished, using
theShockley-Read-Hall theory
of carrier re-combination-generation phenomena.
The variationof the
quasi-Fermi
level of theminority
carriershas
been determinated and taken into account and it has been
analytically demonstrated
that the effective recombinationvelocity
is limited tonearly Uth/2.
The
computation
of thephotovoltaic properties
ofpolycrystalline
silicon solarcells
withfibrously
oriented
grains
has been doneby
means of a 3D-model. It has been shown that
grain
boundaries are not aninsuperable
obstacle to the realization ofgood efficiency
cells on condition that thedoping
level ofthe base be
optimized
in terms ofgrain
size andinterface state
density.
The variation of theoptimum doping
level as a function ofgrain
size has beengiven
for different interface state densities. A nu-merical relation is
proposed
in order tocompute
thisoptimum doping
leveleasily.
It has been demonstrated that an effective dif- fusion
length taking
into account the recombinationat the
grain
boundaries can be defined inpolycrystal-
line silicon. The measurement of this effective diffusion
length by
the SurfacePhotoVoltage
method is able to
give easily
an upper limit of theperformances
one canexpect
from apolycrystalline
material. This limit can be
approached
when theratio
g/Ln (grain
size/bulk diffusionlength)
isgreater
than 10. When this ratio issmaller, achieving
agood accuracy requires
the use of a 3D-model as devel-oped
here.References
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