Concentration of electrons in conduction band formula on n side
Answers
Answer:
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Explanation:
Melissinos, eq.(1.4), gives the formula, valid at thermal equilibrium,
ni = Ns exp
µ
¡
Eg
2kBT
¶
(1)
where,
- ni
is the intrinsic carrier concentration, i.e., the number of electrons in the conduction band
(and also the number of holes in the valence band) per unit volume in a semiconductor
that is completely free of impurities and defects
- Ns is the number per unit volume of effectively available states; its precise value depends
on the material, but it is of order 10
19
cm¡3
at room temperature and increases with
temperature
- Eg is the energy gap (between the bottom of the conduction band and the top of the valence
band)
- kB is Boltzmann's constant, kB = 1:381 ¢ 10
¡23 Joules/Kelvin
- T is the absolute temperature in Kelvin; it is assumed that kBT . Eg=5:
The physical basis of eq. (1) can be understood as follows:
conduction band
The probability of exciting an electron from the top of the
" valence band to the bottom of the conduction band is
Eg proportional to the Boltzmann factor exp
µ
¡
Eg
kBT
¶
:
# This process leaves behind a hole in the valence band and
is called electron-hole pair creation. The total pair creation
valence band rate (see below) is also proportional to this factor.
At thermal equilibrium, the creation of electron-hole pairs is balanced by their recombina-
tion. If n is the concentration of conduction-band electrons and p the concentration of valence-
band holes, the electron-hole recombination rate is proportional to the product np, according
to the general law of mass action of chemical physics. Equating creation to recombination, we
conclude that
np = K exp
µ
¡
Eg
kBT
¶
(2)
where K is a proportionality factor. In an intrinsic semiconductor, by definition, n = p = ni
:
Then eq. (2) is equivalent to eq. (1) with K = N2
s
.
To compute Ns; we must compute the total pair creation rate. We recognize that an electron
can make a transition from any state in the valence band to any state in the conduction band
and we integrate over all these possible transitions, with a weighting factor to account for the