goal: the density of electrons (n o ) can be found precisely if we know 1. the number of allowed...
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![Page 1: GOAL: The density of electrons (n o ) can be found precisely if we know 1. the number of allowed energy states in a small energy range, dE: S(E)dE “the](https://reader036.vdocument.in/reader036/viewer/2022071709/56649cd95503460f949a1e5a/html5/thumbnails/1.jpg)
GOAL:
• The density of electrons (no) can be found precisely if we know1. the number of allowed energy states in a small energy
range, dE: S(E)dE “the density of states”
2. the probability that a given energy state will be occupied by an electron: f(E)
“the distribution function”
no = bandS(E)f(E)dE
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Energy Band Diagram
conduction band
valence band
EC
EV
x
E(x)
S(E)
Eelectron
Ehole
note: increasing electron energy is ‘up’, but increasing hole energy is ‘down’.
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Reminder of our GOAL:
•The density of electrons (no) can be found precisely if we know
1. the number of allowed energy states in a small energy range, dE: S(E)dE
“the density of states”
2. the probability that a given energy state will be occupied by an electron: f(E)
“the distribution function”
no = bandS(E)f(E)dE
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Fermi-Dirac Distribution
The probability that an electron occupies an energy level, E, is
f(E) = 1/{1+exp[(E-EF)/kT]}
– where T is the temperature (Kelvin)– k is the Boltzmann constant (k=8.62x10-5 eV/K)– EF is the Fermi Energy (in eV)
– (Can derive this – statistical mechanics.)
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f(E) = 1/{1+exp[(E-EF)/kT]}
All energy levels are filled with e-’s below the Fermi Energy at 0
oK
f(E)
1
0
EF
E
T=0 o
K
T1>0
T2>T1
0.5
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Fermi-Dirac Distribution for holes
Remember, a hole is an energy state that is NOT occupied by an electron.
Therefore, the probability that a state is occupied by a hole
is the probability that a state is NOT occupied by an electron:
fp(E) = 1 – f(E) = 1 - 1/{1+exp[(E-EF)/kT]}
={1+exp[(E-EF)/kT]}/{1+exp[(E-EF)/kT]} -
1/{1+exp[(E-EF)/kT]}
= {exp[(E-EF)/kT]}/{1+exp[(E-EF)/kT]}
=1/{exp[(EF - E)/kT] + 1}
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The Boltzmann ApproximationIf (E-EF)>kT such that exp[(E-EF)/kT] >> 1 then,
f(E) = {1+exp[(E-EF)/kT]}-1
{exp[(E-EF)/kT]}-1
exp[-(E-EF)/kT] …the Boltzmann approx.
similarly, fp(E) is small when exp[(EF - E)/kT]>>1:
fp(E) = {1+exp[(EF - E)/kT]}-1
{exp[(EF - E)/kT]}-1
exp[-(EF - E)/kT]
If the Boltz. approx. is valid, we say the semiconductor is non-degenerate.
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Putting the pieces together:for electrons, n(E)
f(E)
1
0
EF
E
T=0 o
K
T1>0
T2>T1
0.5
EV EC
S(E)
E
n(E)=S(E)f(E)
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Putting the pieces together: for holes, p(E)
fp(E)
1
0
EF
E
T=0 o
K
T1>0
T2>T1
0.5
EV EC
S(E)
p(E)=S(E)f(E)
hole energy
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Energy Band Diagramintrinisic semiconductor: no=po=ni
conduction band
valence band
EC
EV
x
E(x)
n(E)
p(E)EF=Ei
where Ei is the intrinsic Fermi level
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Energy Band Diagramn-type semiconductor: no>po
conduction band
valence band
EC
EV
x
E(x)
n(E)
p(E)
EF
]/)(exp[0 kTEENn FCC
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Energy Band Diagramp-type semiconductor: po>no
conduction band
valence band
EC
EV
x
E(x)
n(E)
p(E) EF
]/)(exp[0 kTEENp VFV
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The intrinsic carrier density
kTEVCi
ikTE
VC
g
g
eNNn
neNNpn2/
2/00
is sensitive to the energy bandgap, temperature, and m*
2/3
2
*
22
kTm
N dseC