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86 THE PHYSICS OF THE SOLAR CELL<br />

Thus, in 1D, utilizing the Einstein relationship, the electric field can be written as<br />

⃗E = kT q<br />

1 dp o<br />

p o dx<br />

(3.92)<br />

Rewriting equation (3.85) and substituting equation (3.92) yields<br />

V bi =<br />

∫ xP<br />

−x N<br />

∫ xP<br />

Edx ⃗<br />

kT<br />

=<br />

−x N<br />

q<br />

1<br />

p o<br />

dp o<br />

dx dx = kT q<br />

∫ po (x P )<br />

p o (−x N )<br />

dp o<br />

= kT [ ]<br />

p o q ln po (x P )<br />

p o (−x N )<br />

(3.93)<br />

Since we have assumed nondegeneracy, p o (x P ) = N A and p o (−x N ) = n 2 i /N D. Therefore,<br />

V bi = kT [ ]<br />

q ln ND N A<br />

n 2 . (3.94)<br />

i<br />

Figure 3.14 shows the equilibrium energy band diagram, electric field, and charge density<br />

for a simple abrupt pn-junction silicon diode in the vicinity of the depletion region.<br />

The conduction bandedge is given by E C (x) = E 0 − qφ(x) − χ, the valence bandedge<br />

qf(x)<br />

c<br />

E 0<br />

E<br />

E C<br />

(a)<br />

qV bi<br />

E i<br />

E F<br />

E V<br />

E →<br />

(b)<br />

qN D<br />

0<br />

r<br />

(c)<br />

0<br />

−qN A<br />

x = −x N x = 0<br />

x = x P<br />

Figure 3.14 Equilibrium conditions in a solar cell: (a) energy bands; (b) electric field; and<br />

(c) charge density

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