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SOLAR CELL FUNDAMENTALS 91<br />

The solutions to the minority-carrier diffusion equation, equations (3.106)<br />

and (3.107), can be used to evaluate the minority-carrier current densities, equations<br />

(3.110) and (3.111). These can then be substituted into equation (3.116), which,<br />

with some algebraic manipulation, yields<br />

I = I SC − I o1 (e qV/kT − 1) − I o2 (e qV/2kT − 1) (3.118)<br />

where I SC is the short-circuit current and is the sum of the contributions from each of<br />

the three regions: the n-type region (I SCN ), the depletion region (I SCD = AJ D ), and the<br />

p-type region (I SCP )<br />

I SC = I SCN + I SCD + I SCP (3.119)<br />

where<br />

⎡<br />

p ′ (−x N )T p1 − S F,eff p ′ dp ′<br />

(−W N ) + D p<br />

∣<br />

dx<br />

I SCN = qAD p ⎢<br />

⎣<br />

L p T p2<br />

∣<br />

x=−WN<br />

− dp′<br />

dx<br />

⎤<br />

∣ ⎥<br />

x=−xN ⎦<br />

(3.120)<br />

with<br />

T p1 = D p /L p sinh[(W N − x N /L p ] + S F,eff cosh[(W N − x N /L p ] (3.121)<br />

T p2 = D p /L p cosh[(W N − x N )/L p ] + S F,eff sinh[(W N − x N )/L p ] (3.122)<br />

and<br />

⎡<br />

n ′ (x P )T n1 − S BSF n ′ dn ′<br />

(W P ) + D n<br />

∣<br />

dx<br />

I SCP = qAD n ⎢<br />

⎣<br />

L n T n2<br />

∣<br />

x=WP<br />

+ dn′<br />

dx<br />

⎤<br />

∣ ⎥<br />

x=xP<br />

⎦<br />

with<br />

(3.123)<br />

T n1 = D n /L n sinh[(W P − x P )/L n ] + S BSF cosh[(W P − x P )/L n ] (3.124)<br />

T n2 = D n /L n cosh[(W P − x P )/L n ] + S BSF sinh[(W P − x P )/L n ] (3.125)<br />

I o1 is the dark saturation current due to recombination in the quasi-neutral regions,<br />

I o1 = I o1,p + I o1,n (3.126)<br />

with<br />

{ }<br />

I o1,p = qA n2 i<br />

D p Dp /L p sinh[(W N − x N )/L p ] + S F,eff cosh[(W N − x N /L p ]<br />

N D L p D p /L p cosh[(W N − x N )/L p ] + S F,eff sinh[(W N − x N )/L p ]<br />

(3.127)

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