Solution Manual for Semiconductor Devices--Physics and Technology [Sze, S. M] Solution
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1
Solutions Manual to Accompany
SEMICONDUCTOR DEVICESPhysics and Technology
2nd Edition
S. M. SZEUMC Chair Professor
National Chiao Tung UniversityNational Nano Device Laboratories
Hsinchu, Taiwan
John Wiley and Sons, IncNew York. Chicester / Weinheim / Brisband / Singapore / Toronto
0
ContentsCh.1 Introduction--------------------------------------------------------------------- 0Ch.2 Energy Bands and Carrier Concentration -------------------------------------- 1Ch.3 Carrier Transport Phenomena -------------------------------------------------- 7Ch.4 p-n Junction -------------------------------------------------------------------- 16Ch.5 Bipolar Transistor and Related Devices---------------------------------------- 32Ch.6 MOSFET and Related Devices------------------------------------------------- 48Ch.7 MESFET and Related Devices ------------------------------------------------- 60Ch.8 Microwave Diode, Quantum-Effect and Hot-Electron Devices --------------- 68Ch.9 Photonic Devices ------------------------------------------------------------- 73Ch.10 Crystal Growth and Epitaxy--------------------------------------------------- 83Ch.11 Film Formation---------------------------------------------------------------- 92Ch.12 Lithography and Etching ------------------------------------------------------ 99Ch.13 Impurity Doping--------------------------------------------------------------- 105Ch.14 Integrated Devices------------------------------------------------------------- 113
1
CHAPTER 2
1. (a) From Fig. 11a, the atom at the center of the cube is surround by four
equidistant nearest neighbors that lie at the corners of a tetrahedron. Therefore
the distance between nearest neighbors in silicon (a = 5.43 Å) is
1/2 [(a/2)2 + ( a2 /2)2]1/2 = a3 /4 = 2.35 Å.
(b) For the (100) plane, there are two atoms (one central atom and 4 corner atoms
each contributing 1/4 of an atom for a total of two atoms as shown in Fig. 4a)
for an area of a2, therefore we have
2/ a2 = 2/ (5.43 × 10-8)2 = 6.78 × 1014 atoms / cm2
Similarly we have for (110) plane (Fig. 4a and Fig. 6)
(2 + 2 ×1/2 + 4 ×1/4) / a2 2 = 9.6 × 1015 atoms / cm2,
and for (111) plane (Fig. 4a and Fig. 6)
(3 × 1/2 + 3 × 1/6) / 1/2( a2 )( a
23 ) =
2
23
2
a
= 7.83 × 1014 atoms / cm2.
2. The heights at X, Y, and Z point are ,43
,41 and 4
3 .
3. (a) For the simple cubic, a unit cell contains 1/8 of a sphere at each of the eight
corners for a total of one sphere.
4 Maximum fraction of cell filled
= no. of sphere × volume of each sphere / unit cell volume
= 1 × 4ð(a/2)3 / a3 = 52 %
(b) For a face-centered cubic, a unit cell contains 1/8 of a sphere at each of the
eight corners for a total of one sphere. The fcc also contains half a sphere at
each of the six faces for a total of three spheres. The nearest neighbor distance
is 1/2(a 2 ). Therefore the radius of each sphere is 1/4 (a 2 ).
4 Maximum fraction of cell filled
= (1 + 3) 4ð[(a/2) / 4 ]3 / 3 / a3 = 74 %.
(c) For a diamond lattice, a unit cell contains 1/8 of a sphere at each of the eight
corners for a total of one sphere, 1/2 of a sphere at each of the six faces for a
total of three spheres, and 4 spheres inside the cell. The diagonal distance
2
between (1/2, 0, 0) and (1/4, 1/4, 1/4) shown in Fig. 9a is
D = 21
222
222
+
+
aaa = 3
4a
The radius of the sphere is D/2 = 38a
4 Maximum fraction of cell filled
= (1 + 3 + 4)3
383
4
aπ / a3 = ð 3 / 16 = 34 %.
This is a relatively low percentage compared to other lattice structures.
4. 1d = 2d = 3d = 4d = d
1d + 2d + 3d + 4d = 0
1d • ( 1d + 2d + 3d + 4d ) = 1d • 0 = 0
2
1d + 1d • 2d + 1d • 3d + 1d • 4d = 0
4d2+ d2 cosè12 + d2cosè13 + d2cosè14 = d2 +3 d2 cosè= 0
4 cosè = 31−
è= cos-1 (31−
) = 109.470 .
5. Taking the reciprocals of these intercepts we get 1/2, 1/3 and 1/4. The smallest
three integers having the same ratio are 6, 4, and 3. The plane is referred to as
(643) plane.
6. (a) The lattice constant for GaAs is 5.65 Å, and the atomic weights of Ga and As
are 69.72 and 74.92 g/mole, respectively. There are four gallium atoms and
four arsenic atoms per unit cell, therefore
4/a3 = 4/ (5.65 × 10-8)3 = 2.22 × 1022 Ga or As atoms/cm2,Density = (no. of atoms/cm3 × atomic weight) / Avogadro constant
= 2.22 × 1022(69.72 + 74.92) / 6.02 × 1023 = 5.33 g / cm3.
(b) If GaAs is doped with Sn and Sn atoms displace Ga atoms, donors are
formed, because Sn has four valence electrons while Ga has only three. The
resulting semiconductor is n-type.
7. (a) The melting temperature for Si is 1412 ºC, and for SiO 2 is 1600 ºC. Therefore,
SiO2 has higher melting temperature. It is more difficult to break the Si-O
bond than the Si-Si bond.
(b) The seed crystal is used to initiated the growth of the ingot with the correct
crystal orientation.
(c) The crystal orientation determines the semiconductor’s chemical and electrical
3
properties, such as the etch rate, trap density, breakage plane etc.
(d) The temperating of the crusible and the pull rate.
8. Eg (T) = 1.17 – 636)(
4.73x10 24
+
−
TT
for Si
∴ Eg ( 100 K) = 1.163 eV , and Eg (600 K) = 1.032 eV
Eg(T) = 1.519 –204)(
5.405x10 24
+
−
TT
for GaAs
∴Eg( 100 K) = 1.501 eV, and Eg (600 K) = 1.277 eV .
9. The density of holes in the valence band is given by integrating the product
N(E)[1-F(E)]dE from top of the valence band ( VE taken to be E = 0) to the
bottom of the valence band Ebottom:
p = ∫bottomE
0 N(E)[1 – F(E)]dE (1)
where 1 –F(E) = ( )[ ] /kT1 e/1 1 FEE −
+− = [ ] 1/)(e1−−+ kTEE F
If EF – E >> kT then1 – F(E) ~ exp ( )[ ]kTEEF −− (2)
Then from Appendix H and , Eqs. 1 and 2 we obtain
p = 4ð[2mp / h2]3/2 ∫bottomE
0 E1/2 exp [-(EF – E) / kT ]dE (3)
Let x a E / kT , and let Ebottom = ∞− , Eq. 3 becomes
p = 4ð(2mp / h2)3/2 (kT)3/2 exp [-(EF / kT)] ∫∞−
0 x1/2exdx
where the integral on the right is of the standard form and equals π / 2.4 p = 2[2ðmp kT / h2]3/2 exp [-(EF / kT)]
By referring to the top of the valence band as EV instead of E = 0 we have,
p = 2(2ðmp kT / h2)3/2 exp [-(EF – EV) / kT ]or p = NV exp [-(EF –EV) / kT ]
where NV = 2 (2ðmp kT / h2)3 .
10. From Eq. 18NV = 2(2ðmp kT / h2)3/2
The effective mass of holes in Si is
mp = (NV / 2) 2/3 ( h2 / 2ðkT )
= 3
23619
2m101066.2
×× − ( )( )( )300103812
10625623
234
−
−
××
.
.π
= 9.4 × 10-31 kg = 1.03 m0.Similarly, we have for GaAs
mp = 3.9 × 10-31 kg = 0.43 m0.
11. Using Eq. 19
4
( ) ( )CVVC NNkTEEEi ln22)( ++=
= (EC+ EV)/ 2 + (3kT / 4) ln
3
2)6)(( np mm (1)
At 77 K Ei = (1.16/2) + (3 × 1.38 × 10-23T) / (4 × 1.6 × 10-19) ln(1.0/0.62) = 0.58 + 3.29 × 10-5 T = 0.58 + 2.54 × 10-3 = 0.583 eV.
At 300 K Ei = (1.12/2) + (3.29 × 10-5)(300) = 0.56 + 0.009 = 0.569 eV.
At 373 K Ei = (1.09/2) + (3.29 × 10-5)(373) = 0.545 + 0.012 = 0.557 eV.
Because the second term on the right-hand side of the Eq.1 is much smaller
compared to the first term, over the above temperature range, it is reasonable to
assume that Ei is in the center of the forbidden gap.
12. KE = ( ) ( )
)(/)(
/
d
de
CFtop
C
Ftop
C
EExkTEEC
E
E
kTEEC
E
E C
EeEE
EEEEE
−≡−−
−−
−
−−
∫∫
= kT
∫∫
∞ −
∞ −
0
21
0
23
de
de
xx
xx
x
x
= kT
Γ
Γ
2325
= kTπ
π
50
5051
.
.. ××
= kT23
.
13. (a) p = mv = 9.109 × 10-31 ×105 = 9.109 × 10-26 kg–m/s
λ = ph
= 26
34
101099
106266−
−
××
.
.= 7.27 × 10-9 m = 72.7 Å
(b) nλ = λpm
m0 = 06301
.× 72.7 = 1154 Å .
14. From Fig. 22 when ni = 1015 cm-3, the corresponding temperature is 1000 / T = 1.8.
So that T = 1000/1.8 = 555 K or 282 .
15. From Ec – EF = kT ln [NC / (ND – NA)]which can be rewritten as ND – NA = NC exp [–(EC – EF) / kT ]
Then ND – NA = 2.86 × 1019 exp(–0.20 / 0.0259) = 1.26 × 1016 cm-3
or ND= 1.26 × 1016 + NA = 2.26 × 1016 cm-3
A compensated semiconductor can be fabricated to provide a specific Fermi
energy level.
16. From Fig. 28a we can draw the following energy-band diagrams:
5
17. (a) The ionization energy for boron in Si is 0.045 eV. At 300 K, all boronimpurities are ionized. Thus pp = NA = 1015 cm-3
np = ni2 / nA = (9.65 × 109)2 / 1015 = 9.3 × 104 cm-3.
The Fermi level measured from the top of the valence band is given by:
EF – EV = kT ln(NV/ND) = 0.0259 ln (2.66 × 1019 / 1015) = 0.26 eV
(b) The boron atoms compensate the arsenic atoms; we have
pp = NA – ND = 3 × 1016 – 2.9 × 1016 = 1015 cm-3
Since pp is the same as given in (a), the values for np and EF are the same asin (a). However, the mobilities and resistivities for these two samples are
different.
18. Since ND >> ni, we can approximate n0 = ND andp0 = ni
2 / n0 = 9.3 ×1019 / 1017 = 9.3 × 102 cm-3
From n0 = ni exp
−
kT
EE iF ,
we haveEF – Ei = kT ln (n0 / ni) = 0.0259 ln (1017 / 9.65 × 109) = 0.42 eV
The resulting flat band diagram is :
6
19. Assuming complete ionization, the Fermi level measured from the intrinsic
Fermi level is 0.35 eV for 1015 cm-3, 0.45 eV for 1017 cm-3, and 0.54 eV for 1019
cm-3.
The number of electrons that are ionized is given by
n ≅ ND[1 – F(ED)] = ND / [1 + e ( ) TkEE FD /−− ]
Using the Fermi levels given above, we obtain the number of ionized donors as
n = 1015 cm-3 for ND = 1015 cm-3
n = 0.93 × 1017 cm-3 for ND = 1017 cm-3
n = 0.27 × 1019 cm-3 for ND = 1019 cm-3
Therefore, the assumption of complete ionization is valid only for the case of1015 cm-3.
20. ND+ = kTEE FDe /)(
16
110
−−+ =
1350
16
e1
10.−+
=
14511
1
1016
.+
= 5.33 × 1015 cm-3
The neutral donor = 1016 – 5.33 ×1015 cm-3 = 4.67 × 1015 cm-3
4 The ratio of +D
D
N
N O
= 335764
.
. = 0.876 .
7
CHAPTER 3
1. (a) For intrinsic Si, µn = 1450, µp = 505, and n = p = ni = 9.65×109
We have 51031.3)(
11×=
+=
+=
pnipn qnqpqn µµµµρ Ω-cm
(b) Similarly for GaAs, µn = 9200, µp = 320, and n = p = ni = 2.25×106
We have 81092.2)(
11 ×=+
=+
=pnipn qnqpqn µµµµ
ρ Ω-cm.
2. For lattice scattering, µn ∝ T-3/2
T = 200 K, µn = 1300×2/3
2/3
300200
−
−
= 2388 cm2/V-s
T = 400 K, µn = 1300×2/3
2/3
300400
−
−
= 844 cm2/V-s.
3. Since 21
111µµµ
+=
∴ 5001
25011 +=
µ µ = 167 cm2/V-s.
4. (a) p = 5×1015 cm-3, n = ni2/p = (9.65×109)2/5×1015 = 1.86×104 cm-3
µp = 410 cm2/V-s, µn = 1300 cm2/V-s
ρ = pqpqnq ppn µµµ
1
1≈
+ = 3 Ω-cm
(b) p = NA – ND = 2×1016 – 1.5×1016 = 5×1015 cm-3, n = 1.86×104 cm-3
µp = µp (NA + ND) = µp (3.5×1016) = 290 cm2/V-s,
µn = µn (NA + ND) = 1000 cm2/V-s
ρ = pqpqnq ppn µµµ
1
1≈
+ = 4.3 Ω-cm
8
(c) p = NA (Boron) – ND + NA (Gallium) = 5×1015 cm-3, n = 1.86×104 cm-3
µp = µp (NA + ND+ NA) = µp (2.05×1017) = 150 cm2/V-s,
µn = µn (NA + ND+ NA) = 520 cm2/V-s
ρ = 8.3 Ω-cm.
5. Assume ND − NA>> ni, the conductivity is given by
σ ≈ qnµn = qµn(ND − NA)
We have that
16 = (1.6×10-19)µn(ND − 1017)
Since mobility is a function of the ionized impurity concentration, we can use
Fig. 3 along with trial and error to determine µn and ND . For example, if we
choose ND = 2×1017, then NI = ND+ + NA
- = 3×1017, so that µn ≈ 510 cm2/V-s
which gives σ = 8.16.
Further trial and error yields
ND≈ 3.5×1017 cm-3
and
µn ≈ 400 cm2/V-s
which gives
σ ≈ 16 (Ω-cm)-1.
6. )/( )( 2 nnbnqpnq ippn +=+= µµµσ
From the condition dσ/dn = 0, we obtain
bnn i / =
Therefore
9
b
b
bnq
nbbbnqì
ip
iip
i
m
2
1
)1(1
)/(
1
+=
+
+=
µρρ
.
7. At the limit when d >> s, CF = 2ln
π = 4.53. Then from Eq. 16
226.053.410501011010 4
3
3
=×××××=××= −
−
−
CFWIV
ρ Ω-cm
From Fig. 6, CF = 4.2 (d/s = 10); using the a/d = 1 curve we obtain
78.102.41050
10226.0)/(
4
3
=××
×=⋅⋅=−
−
CFWIV ρ mV.
8. Hall coefficient,
7.42605.0)101030(105.2
106.11010493
33
=×××××
×××==−−
−−
WIBAV
Rz
HH cm3/C
Since the sign of RH is positive, the carriers are holes. From Eq. 22
16
191046.1
7.426106.111 ×=
××==
−HqR
p cm-3
Assuming NA ≈ p, from Fig. 7 we obtain ρ = 1.1 Ω-cm
The mobility µp is given by Eq. 15b
3801.11046.1106.1
111619
=××××
==−ρ
µqpp cm2/V-s.
9. Since R ∝ ρ and pn qpqn µµ
ρ+
=1
, hence pn pn
Rµµ +
∝1
From Einstein relation µ∝D
50// == pnpn DDµµ
10
pAnD
nD
NN
NR.
R
µµ
µ
+
=1
1
50 1
1
We have NA = 50 ND .
10. The electric potential φ is related to electron potential energy by the charge (− q)
φ = +q1 (EF − Ei)
The electric field for the one-dimensional situation is defined as
E(x) = −dxdφ =
dxdE
qi1
n = ni exp
−
kTEE iF = ND(x)
Hence
EF − Ei = kT ln
i
D
n)x(N
dx)x(dN
)x(NqkT
(x) D
D
1
−=E .
11. (a) From Eq. 31, Jn = 0 and
aq
kTeN
eaNq
kTndx
dnDx ax
ax
n
n +=−== −
−
)(
- - )(0
0
µE
(b) E (x) = 0.0259 (104) = 259 V/cm.
12. At thermal and electric equilibria,
0)(
)( =+=dx
xdnqDxnqJ nnn Eµ
xNNLNNND
LNN
LxNNND
dxxdn
xnD
x
L
L
n
n
L
Ln
n
n
n
)(
))((1)(
)(1
)(
00
0
0
00
−+−−=
−−+
−=−=
µ
µµE
11
000
0
0
n ln)(
D-
NND
xNNLNNN
V L
n
n
L
LL
µµ−=
−+−
= ∫ .
13. 11166 10101010 =××==∆=∆ −LpGpn τ cm-3
151115 101010 ≈+=∆+=∆+= nNnnn Dno cm-3
.cm 101010
)1065.9( 3-1111
15
292
≈+×=∆+= pN
np
D
i
14. (a) 8
15715 1010210105
11 −− =
××××=≈
tthpp Nνσ
τ s
48 103109 −− ×=×== ppp DL τ cm
201010210 10167 =×××== −stssthlr NS σν cm/s
(b) The hole concentration at the surface is given by Eq. 67
.cm 10
20101032010
11010102
)10(9.65
1)0(
3-9
84
8178
16
29
≈
×+×
×−×+××=
+
−+=
−−
−−
lrpp
lrpLpnon SL
SGpp
ττ
τ
15. pn qpqn µµσ +=
Before illumination
nonnon ppnn == ,
After illumination
,Gnnnn pnonon τ+=∆+=
Gpppp pnonon τ+=∆+=
. )(
)()]()([
Gq
pqnqppqnnq
ppn
nopnonnopnon
τµµ
µµµµσ
+=
+−∆++∆+=∆
12
16. (a) diff , dxdp
qDJ pp −=
= − 1.6×10-19×12×41012
1−×
×1015exp(-x/12)
= 1.6exp(-x/12) A/cm2
(b) diff ,drift , ptotaln JJJ −=
= 4.8 − 1.6exp(-x/12) A/cm2
(c) Enn qnJ µ=drift , Q
∴∴ 4.8 − 1.6exp(-x/12) = 1.6×10-19×1016×1000×E
E = 3 − exp(-x/12) V/cm.
17. For E = 0 we have
02
2
=∂
∂+−−=∂∂
xp
Dpp
tp n
pp
non
τ
at steady state, the boundary conditions are pn (x = 0) = pn (0) and pn (x = W) =
pno.
Therefore
[ ]
−
−+=
p
p
nonnon
LW
LxW
pppxp
sinh
sinh
)0()(
[ ]
−=
∂∂
−=== pp
pnon
x
npp L
WL
Dppq
xp
qDxJ coth)0()0(0
[ ]
−=
∂∂
−===
p
p
pnon
Wx
npp
LWL
Dppq
xp
qDWxJ
sinh
1)0()( .
18. The portion of injection current that reaches the opposite surface by diffusion is
13
given by
)/cosh(1
)0(
)(0
pp
p
LWJ
WJ==α
26 105105050 −− ×=××=≡ ppp DL τ cm
98.0)105/10cosh(
1
220 =×
=∴−−
α
Therefore, 98% of the injected current can reach the opposite surface.
19. In steady state, the recombination rate at the surface and in the bulk is equal
surface ,
surface ,
bulk ,
bulk ,
p
n
p
n pp
ττ
∆=
∆
so that the excess minority carrier concentration at the surface
∆pn, surface = 1014⋅6
7
10
10−
−
=1013 cm-3
The generation rate can be determined from the steady-state conditions in thebulk
G = 6
14
10
10−
= 1020 cm-3s-1
From Eq. 62, we can write
02
2
=∆
−+∂
∆∂
pp
pG
xp
Dτ
The boundary conditions are ∆p(x = ∞ ) = 1014 cm-3 and ∆p(x = 0) = 1013 cm-3
Hence ∆p(x) = 1014( pLxe /9.01 −− )
where Lp = 61010 −⋅ = 31.6 µm.20. The potential barrier height
χφφ −= mB = 4.2 − 4.0 = 0.2 volts.21. The number of electrons occupying the energy level between E and E+dE is
dn = N(E)F(E)dEwhere N(E) is the density-of-state function, and F(E) is Fermi-Dirac distributionfunction. Since only electrons with an energy greater than mF qE φ+ and havinga velocity component normal to the surface can escape the solid, the thermioniccurrent density is
dEeEvhm
qvJ kTEExqEx
F
mF
)(21
3
23
)2(4 −−∞
+∫ ∫==φ
π
where xv is the component of velocity normal to the surface of the metal. Sincethe energy-momentum relationship
)(21
2222
2
zyx pppmm
PE ++==
14
Differentiation leads to m
PdPdE =
By changing the momentum component to rectangular coordinates,
zyx dpdpdpdPP =24π
Hence
zmkTp
ymkTp
xxmkTmEp
p
zyxp
mkTmEpppx
dpedpedppemh
q
dpdpdpepmh
qJ
zyfx
x
x
fzyx
22
2)2(
3
p
p
2/)2(
3
222
0
0 y
222
2
2
−∞
∞−
−∞
∞−
−−∞
∞ ∞
−∞=
∞
−∞=
−++−
∫∫∫
∫ ∫ ∫=
=
where ).(220 mFx qEmp φ+=
Since 21
2
=−∞
∞−∫ adxe ax π
, the last two integrals yield (2ðmkT) 21 .
The first integral is evaluated by setting umkT
mEp Fx =−2
22
.
Therefore we have mkT
dppdu xx=
The lower limit of the first integral can be written as
kTq
mkTmEqEm mFmF φφ =−+
22)(2
so that the first integral becomes kTqu
ktqm
m
emkTduemkT φ
φ
−−∞=∫
/
Hence
−== −
kTq
TAeThqmk
J mkTq mφπ φ exp
4 2*2
3
2
.
22. Equation 79 is the tunneling probability
110234
1931
20 m1017.2
)10054.1()106.1)(220)(1011.9(2)(2 −
−
−−
×=×
×−×=−=h
EqVmnβ
[ ] 6
12100
1019.3)220(24
1031017.2sinh(201 −
−−
×=
−××××××+=T .
23. Equation 79 is the tunneling probability
[ ]
403.0)2.26(2.24
)101099.9sinh(61)10(
1210910 =
−×××××+=
−−
−T
( )[ ]
( )9
12999 108.7
2.262.24101099.9sinh6
1)10( −
−−
− ×=
−×××××+=T .
19234
1931
20 m1099.9
)10054.1()106.1)(2.26)(1011.9(2)(2 −
−
−−
×=×
×−×=−=h
EqVmnβ
15
24. From Fig. 22As E = 103 V/s
νd ≈ 1.3×106 cm/s (Si) and νd ≈ 8.7×106 cm/s (GaAs)
t ≈ 77 ps (Si) and t ≈ 11.5 ps (GaAs)
As E = 5×104 V/s
νd ≈ 107 cm/s (Si) and νd ≈ 8.2×106 cm/s (GaAs)
t ≈ 10 ps (Si) and t ≈ 12.2 ps (GaAs).
cm/s105.9m/s109.5
101.9300101.382
22 velocity Thermal 25.
64
31
23-
00
×=×=×
×××=
==
−
mkT
mE
v thth
For electric field of 100 v/cm, drift velocity
thnd vv <<×=×== cm/s1035.11001350 5Eµ
For electric field of 104 V/cm.
thn v≈×=×= cm/s1035.1101350 74Eµ .
The value is comparable to the thermal velocity, the linear relationship between
drift velocity and the electric field is not valid.
16
CHAPTER 4
1. The impurity profile is,
The overall space charge neutrality of the semiconductor requires that the total negative
space charge per unit area in the p-side must equal the total positive space charge per
unit area in the n-side, thus we can obtain the depletion layer width in the n-side region:
1414
1032
1088.0 ××=××nW
Hence, the n-side depletion layer width is:
m0671 µ.Wn =
The total depletion layer width is 1.867 µm.
We use the Poisson’s equation for calculation of the electric field E(x).
In the n-side region,
( )
V/cm108640
)100671(103
1006710m0671
3
414
4
×−===
×−××=∴
××−=⇒==
+=⇒=
−
−
.)x(
.xq
x
.Nq
K).x(
KxNq
)x(Nq
dxd
nmax
sn
Ds
n
Ds
nDs
EE
E
E
EE
ε
εµ
εε
In the p-side region, the electrical field is:
x (µm)
(ND-NA) (cm-3)
3×1014
a =1019 cm-4
17
( )
( ) ( )V/cm108640
10802
10802
0m80
2
3
242
24
2
×−===
×−××=∴
×××−=⇒=−=
+×=⇒=
−
−
.)x(
.xaq
x
.aq
K).x(
Kaxq
)x(Nq
dxd
pmax
sp
s
'p
'
spA
s
EE
E
E
EE
ε
εµ
εε
The built-in potential is:
( ) ( ) ( ) V 52.0
0
0
=−−=−= ∫∫ ∫ −− − −
nn
p p
x
siden
x
x x sidepbi dxxdxxdxxV EEE .
2. From ( )∫−= dxxVbi E , the potential distribution can be obtained
With zero potential in the neutral p-region as a reference, the potential in the p-side
depletion region is
( ) ( ) ( )[ ] ( ) (
( ) ( )
×−×−××−=
×−×−−=×−××−=−=
−−
−−−∫ ∫3424311
4243
0
0
242
108.032
108.031
10596.7
108.032
108.031
2 108.0
2
xx
xxqa
dxxaq
dxxxVs
x x
sp εε
E
With the condition Vp(0)=Vn(0), the potential in the n-region is
( )
×−×−××−=
×+×−××−=
−−
−−
73
427
73
4214
1098.0
10067.121
1056.4
1098.0
10067.121
103
xx
xxq
xVs
n ε
The potential distribution isDistance p-region n-region
-0.8 0.000
-0.7 0.006
-0.6 0.022
-0.5 0.048
-0.4 0.081
-0.3 0.120
-0.2 0.164
-0.1 0.211
0 0.259 0.25941
3333
18
0.1 0.305788533
0.2 0.3476
03733
0.3 0.384858933
0.4 0.41755
4133
0.5 0.4456
89333
0.6 0.4692
64533
0.7 0.4882
79733
0.8 0.50273
4933
0.9 0.5126
30133
1 0.51796
5333
1.06
7
0.51898
8825
Potential Distribution
-0.100
0.000
0.100
0.200
0.300
0.400
0.500
0.600
-1 -0.5 0 0.5 1 1.5
D istance (um)
Pot
enti
al
(V)
19
3. The intrinsic carriers density in Si at different temperatures can be obtained by using Fig.22 in
Chapter 2 :
Temperature (K) Intrinsic carrier density (ni)
250 1.50×108
300 9.65×109
350 2.00×1011
400 8.50×1012
450 9.00×1013
500 2.20×1014
The Vbi can be obtained by using Eq. 12, and the results are listed in the following table.
T ni Vbi (V)
250 1.500E+0
8
0.777
300 9.65E+9 0.717
350 2.00E+1
1
0.653
400 8.50E+1
2
0.488
450 9.00E+13 0.366
500 2.20E+1
4
0.329
Thus, the built-in potential is decreased as the temperature is increased.
The depletion layer width and the maximum field at 300 K are
V/cm. 10476.11085.89.11
10715.910106.1
m 9715.010106.1
717.01085.89.1122
4
14
51519
max
1519
14
×=××
××××==
=××
××××==
−
−−
−
−
s
D
D
bis
WqN
qNV
W
ε
µε
E
20
18
16
2/1
18
18
14
195
2/1
max
101
10755.1
1010
1085.89.1130106.12
1042
.4
D
D
D
D
DA
DA
s
R
NN
NN
NNNNqV
+=×⇒
+××
×××=×⇒
+
≈ −
−
ε.E
We can select n-type doping concentration of ND = 1.755×1016 cm-3 for the junction.
5. From Eq. 12 and Eq. 35, we can obtain the 1/C2 versus V relationship for doping concentration of
1015, 1016, or 1017 cm-3, respectively.
For ND=1015 cm-3,
( ) ( ) ( )VV
NqåVV
C Bs
bi
j
−×=×××××
−×=−
=−−
837.010187.110108.8511.9101.6
0.837221 16
1514192
For ND=1016 cm-3,
( ) ( ) ( )VV
NqåVV
C Bs
bi
j
−×=×××××
−×=−
=−−
896.010187.110108.8511.9101.6
0.896221 15
1614192
For ND =1017 cm-3,
( ) ( ) ( )VV
NqåVV
C s
bi
j
−×=×××××
−×=−
=−−
956.010187.110108.8511.9101.6
0.956221 14
171419B
2
When the reversed bias is applied, we summarize a table of 2jC1/ vs V for various ND values as
following,
21
V ND=1E15 ND=1E16 ND=1E17
-4 5.741E+
16
5.812E+
15
5.883E+
14
-3.5 5.148E+
16
5.218E+
15
5.289E+1
4
-3 4.555E+1
6
4.625E+
15
4.696E+
14
-2.5 3.961E+
16
4.031E+
15
4.102E+
14
-2 3.368E
+16
3.438E+
15
3.509E+1
4
-1.5 2.774E
+16
2.844E+
15
2.915E+1
4
-1 2.181E
+16
2.251E+
15
2.322E+
14
-0.5 1.587E+
16
1.657E+
15
1.728E+
14
0 9.935E+1
5
1.064E+
15
1.134E+
14
Hence, we obtain a series of curves of 1/C2 versus V as following,
The slopes of the curves is positive proportional to the values of the doping concentration.
1/C2 vs V
0
1E+16
2E+16
3E+16
4E+16
5E+16
6E+16
7E+16
-4.5 -4 -3.5 -3 -2.5 -2 -1.5 -1 -0.5 0
Applied Voltage
1/C
^2
22
The interceptions give the built-in potential of the p-n junctions.
23
6. The built-in potential is
( )V 5686.0
1065.9106.18
0259.01085.89.111010ln0259.0
32
8ln
32
3919
142020
32
2
=
××××
×××××××=
=
−
−
i
sbi nq
kTaqkT
Vε
From Eq. 38, the junction capacitance can be obtained
( )( )
( )
3/12142019-3/12
5686.0121085.89.1110101.6
12
−×××××=
−==
−
RRbi
ssj VVV
qa
WC
εε
At reverse bias of 4V, the junction capacitance is 6.866×10-9 F/cm2.
7. From Eq. 35, we can obtain
( ) ( ) 2
2
221j
s
RbiD
Bs
bi
j
Cq
VVN
NqVV
C εε−
=⇒−
=
We can select the n-type doping concentration of 3.43×1015cm-3.
8. From Eq. 56,
169
1515
1571515
1089310659
02590020
exp1002590
020exp10
10101010
expexp
×=××
−
+
×××=
−
+
−
=−=
−−
−−
..
..
..
n
kTEE
kTEE
NUG i
tip
itn
tthnp
σσ
υσσ
and
( )
315
281419
2
cm10433
)10850(108589111061
422
−
−−−
×=⇒
××××××
×=≅⇒>>
.N
....
CqV
NVV
d
js
RDbiR ε
Q
24
( )m 266.1cm1066.12
10106.1)5.0717.0(1085.89.1122 5
1519
14
µε
=×=××
+××××=+
= −−
−
A
bis
qNVV
W
Thus
2751619 A/cm10879.71066.121089.3106.1 −− ×=×××××== qGWJ gen .
9. From Eq. 49, and D
ino N
np
2
=
We can obtain the hole concentration at the edge of the space charge region,
( ) 3170259.0
8.0
16
29)0259.0
8.0(
2
cm1042.210
1065.9 −
×=×== eeN
np
D
in .
10. ( ) ( ) ( )1/ −=−+= kTqVspnnp eJxJxJJ
V. 017.0
195.0
1
0259.0
0259.0
=⇒
−=⇒
−=⇒
V
e
eJJ
V
V
s
11. The parameters are
ni= 9.65×109 cm-3 Dn= 21 cm2/sec
Dp=10 cm2/sec τp0=τn0=5×10-7 sec
From Eq. 52 and Eq. 54
( ) ( )
( )
315
0259.0
7.029
7
19
2/
cm102.5
11065.9
10510
106.17
11
−
−−
×=
⇒
−×××
×××=
⇒
−××=−=
D
D
kT
qV
D
i
po
pkTqV
p
nopnp
N
eN
eNnD
qeL
pqDxJ
a
τ
25
( ) ( )
( )
316
0259.0
7.029
7
19
2/
cm10278.5
11065.9
10521
106.125
11
−
−−
×=
⇒
−×××
×××=
⇒
−××=−=−
A
A
kT
qV
A
i
no
nkTqV
n
ponpn
N
eN
eNnD
qeL
nqDxJ
a
τ
We can select a p-n diode with the conditions of NA= 5.278×1016cm-3 and ND =
5.4×1015cm-3.
12. Assumeôg =ôp =ôn = 10-6 s, Dn= 21 cm2/sec, and Dp = 10 cm2/sec
(a) The saturation current calculation.From Eq. 55a and ppp DL τ= , we can obtain
+=+=
00
200 11
n
n
Ap
p
Di
n
pn
p
nps
DN
D
Nqn
L
nqD
L
pqDJ
ττ
( )
212
616618
2919
A/cm1087.6
1021
101
1010
101
1065.9106.1
−
−−−
×=
+×××=
And from the cross-sectional area A = 1.2×10-5 cm2, we obtain
A10244.81087.6102.1 17125 −−− ×=×××=×= ss JAI .
(b) The total current density is
−= 1kt
qV
s eJJ
Thus
A.10244.8110244.8
A1051.41047.510244.8110244.8
170259.0
7.017
7.0
511170259.0
7.017
7.0
−−
−−
−−−
×=
−×=
×=×××=
−×=
eI
eI
V
V
26
13. From
−= 1kt
qV
s eJJ
we can obtain
V 78.0110244.8
10ln0259.01ln
0259.0 17
3
=
+
×
×=⇒
+
=
−
−
VJJV
s
.
14. From Eq. 59, and assume Dp= 10 cm2/sec, we can obtain
( ) ( )
1519
14
6
919
15
29
619
2
101061
108589112
10
106591061
10
10659
10
101061
××+×××××××+××=
+≅
−
−
−
−
−−
.
VV......
WqnNnD
qJ
Rbi
g
i
D
i
p
pR ττ
( ) V 834.01065.9
1010ln0259.0
29
1519
=×
×=biV
Thus
RR VJ +×+×= −− 834.010872.11026.5 711
27
VR Js
0 1.713E-
07
0.1 1.755E-
07
0.2 1.941E-
07
0.3 2,129E-
07
0.4 2.316E-
07
0.5 2.503E-
07
0.6 2.691E-
07
0.7 2.878E-
07
0.8 3.065E-
07
0.9 3.252E-
07
1 3.439E-
07
28
When ND=1017 cm-3, we obtain
( ) V 953.01065.9
1010ln0259.0
29
1719
=×
×=biV
15. From Eq. 39,
( )∫∞
−=
x nonpn
dxppqQ
Current Density
0.E+00
5.E-08
1.E-07
2.E-07
2.E-07
3.E-07
3.E-07
0 0.2 0.4 0.6 0.8 1 1.2
Applied Voltage
Cur
rent
Den
sity
RR VJ +×+×= −− 956.010872.11026.5 813
Current Density
0.00E+00
5.00E-09
1.00E-08
1.50E-08
2.00E-08
2.50E-08
3.00E-08
0 0.2 0.4 0.6 0.8 1 1.2
Applied Voltage
Cur
rent
Den
sity
29
( ) ( )∫∞ −−−=
x
LxxkTqVno
n
pn dxeepq
// 1
The hole diffusion length is larger than the length of neutral region.
( )∫ −='
n
n
x
x nonp dxppqQ
( ) ( )
.C/cm10784.8
1)105(10
)1065.9(106.1
1)(
1
23
5
0
5
1
0259.0
14
16
2919
x
//
'
'
n
−
−−−−
−−
−−
−−
×=
−
−×−×××=
−
−−=
−= ∫
eee
eeeLqp
dxeepq
p
nn
p
nn
n pn
L
xx
L
xx
kT
qV
pno
x LxxkTqVno
16. From Fig. 26, the critical field at breakdown for a Si one-sided abrupt
junction is about 2.8 ×105 V/cm. Then from Eq. 85, we obtain
( ) ( ) 12
22voltagebreakdown −== B
cscB N
qW
VEE ε
( ) ( ) 115
19
2514
10106.12
108.21085.89.11 −
−
−
××××××=
258= V
( )£gm4318cm108431
101061
2581085891122 31519
14
...
..qN
VVW
B
bis =×=××
××××≅−
= −−
−ε
When the n-region is reduced to 5µm, the punch-through will take place first.
From Eq. 87, we can obtain
( )/2Winsert 29 Fig.in area shaded
mcE=
B
B
V'V
−
=
mm WW
WW
2
12143.18
52
43.185
2582' =
−
×=
−
=
mmBB W
WWW
VV V
Compared to Fig. 29, the calculated result is the same as the value under the
30
conditions of W = 5 µm and NB = 101 5 cm-3.
17. We can use following equations to determine the parameters of the diode.
kTqV
D
i
p
pkTqV
r
ikTqV
D
i
p
pF e
N
nDqe
qWne
N
nDqJ /
22//
2
2 τττ≅+=
( ) 12
22−== D
cscB N
qW
VEE ε
⇒
( ) 302590
7029
7
192
102210659
101061 −
−− ×=
××××⇒= .e
N.D
.AeNnD
AqAJ .
.
D
pkT/qV
D
i
p
pF τ
( ) ( ) 1
19
2141
2
10612
10858911130
22−
−
−−
××××
=⇒== Dc
Dcsc
B N.
..N
qW
VEEE ε
Let Ec= 4×105 V/cm, we can obtain ND = 4.05×1015 cm-3.
The mobility of minority carrier hole is about 500 at ND = 4.05×1015
∴Dp= 0.0259×500=12.95 cm2/s
Thus, the cross-sectional area A is 8.6×10-5 cm2.
18. As the temperature increases, the total reverse current also increases. That is,
the total electron current increases. The impact ionization takes place when the
electron gains enough energy from the electrical field to create an electron-
hole pair. When the temperature increases, total number of electron increases
resulting in easy to lose their energy by collision with other electron before
breaking the lattice bonds. This need higher breakdown voltage.
19. (a) The i-layer is easy to deplete, and assume the field in the depletion region is
31
constant. From Eq. 84, we can obtain.
V/cm 1087.5)10(1041101054
101104
10 56153
64
0
6
5
4 ×=××=⇒=×
×⇒=
×−∫ critical
Wdx E
EE
4 587101087.5 35 =××= −BV V
(b) From Fig. 26, the critical field is 5 × 105 V/cm.
( ) ( ) 12
22voltagebreakdown −== B
cscB N
qW
VEE ε
( ) ( ) 116
19
2514
102106.12
1051085.84.12 −
−
−
×××
××××=
8.42= V.
20. 422
4
18
cm10102
102 −−
=××=a
( )
( )238
2122
21
19
1423
212123
10844
101061
1085891123
4
2
3
4
32
/c
///
c
//
s/
cB
.
...
aq
WV
E
E
EE
−
−
−
−
−
×=
×
×
×××=
==
ε
The breakdown voltage can be determined by a selected Ec.
21. To calculate the results with applied voltage of V 5.0=V , we can use a similar calculation
in Example 10 with (1.6-0.5) replacing 1.6 for the voltage. The obtained electrostatic
potentials are V 1.1 and V 103.4 4−× , respectively. The depletion widths are
cm 103.821 5−× and cm 101.274 8−× , respectively.
Also, by substituting V 5−=V to Eqs. 90 and 91, the electrostatic potentials are V 6.6
and V 1020.3 4−× , and the depletion widths are cm 109.359 5−× and cm 103.12 8−× ,
respectively.
The total depletion width will be reduced when the heterojunction is forward-biased from
the thermal equilibrium condition. On the other hand, when the heterojunction is reverse-
32
biased, the total depletion width will be increased.
22. Eg(0.3) = 1.424 + 1.247 × 0.3 = 1.789 eV
biV = ( ) −−−∆− q/EEqE
q
EVF
Cg22
2 ( ) q/EE FC 11 −
= 1.789 – 0.21–15
17
105
1074ln
××.
qkT
–15
18
105
107ln
××
qkT
= 1.273 V
1x = ( )2
1
21
212
+ ADD
biA
NNqNvNεε
εε= ( )
21
1519
14
46114121051061
27311085846114122
+××××××××
−
−
.......
= 4.1 510 −× cm.
Since 21 xNxN AD = 21 xx =∴
m0.82 cm10282 51 µ . x W =×==∴ − .
33
CHAPTER 5
1. (a) The common-base and common-emitter current gains is given by
. 199
995.01995.0
1
995.0998.0997.0
0
00
0
=−
=−
=
=×==
αα
β
γαα T
(b) Since 0=BI and A 1010 9−×=CpI , then CBOI is A 1010 9−× . The emitter current is
( )( )
. A 102
10101991
1
6
9
0
−
−
×=
×⋅+=
+= CBOCEO II β
2. For an ideal transistor,
. 9991
999.0
0
00
0
=−
=
==
αα
β
γα
CBOI is known and equals to A 1010 6−× . Therefore,
( )
. mA 10
1010)9991(
16
0
=×⋅+=
+=−
CBOCEO II β
3. (a) The emitter-base junction is forward biased. From Chapter 3 we obtain
( ). V 956.0
1065.9
102105ln0259.0ln
29
1718
2=
×
×⋅×=
=
i
DAbi
nNN
qkT
V
The depletion-layer width in the base is
34
( )
( )
. m 105.364cm 105.364
5.0956.0102105
1102105
106.11005.12
12
junction) base-emitter theof hlayer widt-depletion (Total
2-6-
171817
18
19
12
1
µ×=×=
−
×+×
××
××⋅=
−
+
=
+
=
−
−
VVNNN
Nq
NNN
W
biDAD
As
DA
A
ε
Similarly we obtain for the base-collector function
( ). V 0.795
1065.9
10102ln0259.0
29
1617
=
×
⋅×=biV
and
( )
. m 10.2544cm 104.254
5795.010210
1102
10106.1
1005.12
2-6-
171617
16
19
12
2
µ×=×=
+
×+
××
×⋅=−
−
W
Therefore the neutral base width is
. m 904.010.254410364.51 -2221B µ=×−×−=−−= −WWWW
(b) Using Eq. 13a
( ). cm 10543.2
1021065.9
)0( 3-110259.05.017
292
×=××=== ee
Nn
epp kTqV
D
ikTqVnon
EBEB
4. In the emitter region
( ). 18.625
1051065.9
cm 10721.01052 scm 52
18
29
38
=××=
×=⋅== −−
EO
EE
n
LD
In the base region
35
( ). 465.613
102
1065.9
mc 1021040 scm 40
17
292
37
=××==
×=⋅=== −−
D
ino
pppp
Nn
p
DLD τ
In the collector region
( ). 109.312
101065.9
cm 10724.1010115 scm 115
316
29
36
×=×=
×=⋅== −−
CO
CC
n
LD
The current components are given by Eqs. 20, 21, 22, and 23:
( )
. 0
A 103.19610724.10
10312.9115102.0106.1
A 101.041110721.0
625.1852102.0106.1
A 101.596
A 101.59610904.0
613.46540102.0106.1
14-
3
3219
7-0259.05.0
3
219
5-
5-0259.05.0
4
219
=−=
×=×
×⋅⋅×⋅×=
×=−×
⋅⋅×⋅×=
×=≅
×=×
⋅⋅×⋅×=
−
−−
−
−−
−
−−
CpEpBB
Cn
En
EpCp
Ep
III
I
eI
II
eI
5. (a) The emitter, collector, and base currents are given by
. A 101.041
A 101.596
A 101.606
7-
5-
-5
×=−+=
×=+=
×=+=
CnBBEnB
CnCpC
EnEpE
IIII
III
III
(b) We can obtain the emitter efficiency and the base transport factor:
9938.010606.110596.1
5
5
=××==
−
−
E
Ep
I
Iγ
. 110596.110596.1
5
5
=××== −
−
Ep
CpT I
Iα
Hence, the common-base and common-emitter current gains are
. 3.1601
9938.0
0
00
0
=−
=
==
ααβ
γαα T
36
(c) To improve γ , the emitter has to be doped much heavier than the base.
To improve Tα , we can make the base width narrower.
6. We can sketch (0))( nn pxp curves by using a computer program:
0 . 0 0 . 2 0 . 4 0 . 6 0 . 8 1 . 0
0 . 0
0 . 2
0 . 4
0 . 6
0 . 8
1 . 0
20
1
2
5
10
W / L p<0.1
DISTANCE x
p n(x)
/pn(
0)
In the figure, we can see when 1.0<pLW ( 05.0=pLW in this case), the
minority carrier distribution approaches a straight line and can be simplified to
Eq. 15.
7. Using Eq.14, EpI is given by
37
( )
( ) .
cosh
1 1 coth
sinh
1
sinh
cosh
)1 (
sinh
cosh1
sinh
cosh1
)1 (
0
0
+−
=
+
−=
−
+
−−
−−=
−=
=
=
p
kTqV
pp
nop
pp
pkTqV
p
nop
xp
ppno
p
ppkTqVnop
x
npEp
LW
eLW
L
pDqA
LW
LW
LW
eL
pDqA
LW
Lx
Lp
LW
LxW
LepqDA
dxdp
qDAI
EB
EB
EB
Similarly, we can obtain CpI :
( )
( ) . cosh 1
sinh
1
sinh
cosh
sinh
1)1 (
sinh
cosh1
sinh
cosh1
)1 (
+−
=
+
−=
−
+
−−
−−=
−=
=
=
p
kTqV
p
p
nop
p
p
p
kTqV
p
nop
Wxp
ppno
p
ppkTqVnop
Wx
npCp
LW
e
LWL
pDqA
LW
LW
LW
eL
pDqA
LW
Lx
Lp
LW
LxW
LepqDA
dxdp
qDAI
EB
EB
EB
8. The total excess minority carrier charge can be expressed by
38
[ ]
. 2
)0(2
)2
(
)1(
)(
0
2
0
0
n
kTqVno
W
kTqVno
WkTqV
no
W
nonB
qAWp
eqAWp
Wx
xeqAp
dxWx
epqA
dxpxpqAQ
EB
EB
EB
=
=
−=
−=
−=
∫
∫
From Fig. 6, the triangular area in the base region is 2
)0(nWp . By multiplying this
value by q and the cross-sectional area A, we can obtain the same expression as BQ .
In Problem 3,
. C 103.6782
10543.210904.0102.0106.1
15-
114219
×=
×⋅×⋅×⋅×=−−−
BQ
9. In Eq. 27,
( )
. 2
2
)0(2
)0(
1
2
2
2221
Bp
np
np
kTqVC
QW
D
qAQp
W
DW
pqAD
aeaI EB
=
=
≅
+−=
Therefore, the collector current is directly proportional to the minority carrier
charge stored in the base.
10. The base transport factor is
39
( )
( )
.
cosh
1 1 coth
cosh 1
sinh
1
+−
+−
=≅
p
kTqV
p
p
kTqV
p
Ep
CpT
LW
eLW
LW
e
LW
I
I
EB
EB
α
For 1<<pLW , ( ) 1cosh ≅pLW . Thus,
( ) . 21
21
1
sech
cothsinh
1
22
2
p
p
p
pp
T
LW
LW
LW
LW
LW
−=
−=
=
⋅
=α
11. The common-emitter current gain is given by
. 11 0
00
T
T
γαγα
ααβ
−=
−≡
Since 1≅γ ,
( )( )[ ]
( ) . 12
211
21
1
22
22
22
0
−=
−−
−=
−≅
WL
LW
LW
p
p
p
T
T
ααβ
If 1<<pLW , then 220 2 WLp≅β .
12. m 54.77mc 10477.5103100 37 µ=×=×⋅== −−ppp DL τ
Therefore, the common-emitter current gain is
40
( )( )
. 1500102
1077.5422
24
2422
0
=×
×=≅−
−
WLpβ
13. In the emitter region,
6871031037401
407354
1817.
..pE =
×⋅×++=
−µ
. ..DE scm 2.2668702590 =⋅=
In the base region,
6311861021069801
125288
1617.
.n =
×⋅×++=
−µ
. ...Dp scm733063118602590 =⋅=
In the collector region,
824531051037401
407354
1517.
..pC =
×⋅×++=
−µ
. ...DC scm75118245302590 =⋅=
14. In the emitter region,
cm 10506.110269.2 36 −− ×=⋅== EEE DL τ
( ). cm 04.31
103
1065.9 3-18
292
=×
×==E
iEO N
np
In the base region,
cm 10544.510734.30 36 −− ×=⋅=nL
( ). cm 13.4656
1021065.9 3-
16
29
=××=pon
In the collector region,
cm 10428.310754.11 36 −− ×=⋅=CL
41
( ). cm 5.18624
1051065.9 3-
15
29
=××=COp
The emitter current components are given by
A 1083.526105.0
13.4656734.3010106.1 60259.06.04
419−
−
−−
×=×
⋅⋅⋅×= eI En
( ) .A 10609.8110506.1
04.31269.210106.1 90259.06.0
3
419−
−
−−
×=−×
⋅⋅⋅×= eIEp
Hence, the emitter current is
.A 10839.526 6−×=+= EpEnE III
And the collector current components are given by
A 1083.526105.0
13.4656734.3010106.1 60259.06.0
4
419−
−
−−
×=×
⋅⋅⋅×= eICn
.A 10022.110428.3
5.18624754.1110106.1 14
3
419−
−
−−
×=×
⋅⋅⋅×=CpI
Therefore, the collector current is obtained by
.A 10268.5 4−×=+= CpCnC III
15. The emitter efficiency can be obtained by
. 99998.010839.526
1083.5266
6
=×
×==−
−
E
En
IIγ
The base transport factor is
. 11083.526
1083.5266
6
=××==
−
−
En
CnT I
Iα
Therefore, the common-base current gain is obtained by
. 99998.099998.010 =×== Tγαα
The value is very close to unity.
The common-emitter current gain is
42
. 5000099998.01
99998.01 0
00 ≅
−=
−=
αα
β
16. (a) The total number of impurities in the neutral base region is
( )( ) . cm 10583.51103102
1
2-13103108518
0
55
×=−×⋅×=
−==−− ××−−
−−∫e
elNdxeNQ lWAO
W
lxAOG
(b) Average impurity concentration is
. cm 10979.6108
10583.5
3-17
5
13
×=×
×= −WQG
17. For -317 cm 10979.6 ×=AN , scm 77.7 3=nD , and
cm 10787.21077.7 36 −− ×=⋅== nnn DL τ
( )( ) 999588.0
10787.22
1081
21 23
25
2
2
=×
×−=−≅
−
−
nT
L
Wα
. 99287.0
101010583.5
77.71
1
1
1
1
419
13=
⋅×⋅+
=+
=
−EE
G
n
E
LNQ
DD
γ
Therefore,
99246.00 == Tγαα
. 6.1311 0
00 =
−=
αα
β
18. The mobility of an average impurity concentration of -317 cm 10979.6 × is about
300 Vscm2 . The average base resistivity Bρ is given by
( ) . cm- 0299.01 Ω==
WQq GnB µ
ρ
43
Therefore,
( ) ( ) . 869.11080299.0105105 533 Ω=×⋅×=×= −−− WR BB ρ
For a voltage drop of qkT ,
.A 0139.0==B
B qRkT
I
Therefore,
.A 83.10139.06.131 0 =⋅== BC II β
19. From Fig. 10b and Eq. 35, we obtain
( )AµBI ( )mACIB
C
I
I
∆∆
=0β
0 0.20 ---
5 0.95 150
10 2.00 210
15 3.10 220
20 4.00 180
25 4.70 140
0β is not a constant. At low BI , because of generation-recombination current, 0β
increases with increasing BI . At high BI , EBV increases with BI , this in turn causes
a reduction of BCV since V 5==+ ECBCEB VVV . The reduction of BCV causes a
widening of the neutral base region, therefore 0β decreases.
The following chart shows 0β as function of BI . It is obvious that 0β is not a
constant.
44
0 5 10 15 20 25 301 0 0
1 5 0
2 0 0
2 5 0
IB (µA)
β 0
20. Comparing the equations with Eq. 32 gives
11 aIFO = , 12 aIROR =α
21 aIFOF =α , and . 22aI RO =
Hence,
no
EO
p
E
E
F
pn
DD
LWa
a
⋅⋅+==
1
1
11
21α
. 1
1
22
12
no
CO
p
C
C
R
pn
DD
LWa
a
⋅⋅+==α
21. In the collector region,
cm 101.414 102 36 −− ×=⋅== CCC DL τ
( ) . cm 101.863 1051065.9 3-415292 ×=××== CiCO Nnn
From Problem 20, we have
45
99995.01031.9
31.9101
10105.0
1
1
1
1
23
4
=×
⋅⋅×+=
⋅⋅+=
−−
−
no
EO
p
E
E
F
pn
DD
LW
α
876.01031.910863.1
102
10414.1105.0
1
1
1
1
2
4
3
4
=××⋅⋅
××+
=⋅⋅+
=
−−
−
no
CO
p
C
C
R
pn
DD
LW
α
A 1049.1
1031.91
105.01031.910
105106.1
14
44
2419
11
−
−−−−
×=
⋅+×
×⋅⋅×⋅×=
+==
E
EOEnopFO L
nDW
pDqAaI
. A 107.1
10414.1
10863.12
105.0
1031.910105106.1
14
3
4
4
2419
22
−
−−−−
×=
×
×⋅+
××⋅
⋅×⋅×=
+==
C
COCnopRO L
nDW
pDqAaI
The emitter and collector currents are
( )A 10715.1
1 4−×=
+−= RORkTqV
FOE IeII EB α
( ). A 10715.1
1 4−×=
+−= ROkTqV
FOFC IeII EBα
Note that these currents are almost the same (no base current) for 1<<pLW .
22. Referring Eq. 11, the field-free steady-state continuity equation in the collector region is
( ) ( ). 0
2C
2
=−
−
C
poCC
n'xn
'dx'xnd
Dτ
The solution is given by ( CCC DL τ= )
( ) . 21CC L'xL'x
C eCeC'xn −+=
Applying the boundary condition at ∞='x yields
46
. 021 =+ ∞−∞ CC LL eCeC
Hence 01 =C . In addition, for the boundary condition at 0='x ,
( )020
2 CL nCeC C ==−
( ) ( ) . 1.0 −= kTqVCOC
CBenn
The solution is
( ) ( ) . 1 CCB L'xkTqVCOC eenxn −−=
The collector current can be expressed as
( ) ( )( ) ( ) . 1 1
1 1
2221
0
−−−=
−
+−−=
−+
−=
==
kTqVkTqV
kTqV
C
COCnopkTqVnop
'x
CC
Wx
npC
CBEB
CBEB
eaea
eLnD
W
pDqAe
W
pDqA
'dxdn
qDAdx
dpqDAI
23. Using Eq. 44, the base transit time is given by
( ).
. DW pB s 101.25
1021050
2 10-
242 ×=
××==
−
τ
We can obtain the cutoff frequency :
. GHz 1.27 21 =≅ BTf πτ
From Eq. 41, the common-base cutoff frequency is given by:
. GHz 1.275 998.0
1027.1
9
0 =×=≅ αα Tff
The common-emitter cutoff frequency is
( ) ( ) . .. f f MHz 2.55102751998011 90 =××−=−= αβ α
Note that βf can be expressed by
( ) ( ) TT ffff0
000
1 1 1 β
ααα αβ =×−=−= .
47
24. Neglect the time delays of emitter and collector, the base transit time is given by
s1083.311052
12
1 12
9
−×=××
==ππ
τT
B f.
From Eq. 44, W can be expressed by
BpDW τ2= .
Therefore,
. m0.252
cm102.52
1083.311025-
12
µ=×=
×××= −W
The neutral base width should be 0.252 µm.
25. gE∆ =9.8% ×1.12 ≅ 110 meV.
oβ ~exp
∆kT
E g
( )( )C0
C100
°°
∴
o
o
ββ
= exp
−
k
k
273meV110
373meV110
= 0.29.
26.
−=
−=
0259.0
424.1)(expexp
)BJT()HBT(
0
0xE
kT
EE gEgBgE
ββ
where
. 145.0 ,143.0125.09.1
45.0 ,247.1424.1)(
≤<++=
≤+=
xxx
xxxEgE
The plot of )BJT()HBT( 00 ββ is shown in the following graph.
48
Note that )HBT(0β increases exponentially when x increases.
27. The impurity concentration of the n1 region is -314 cm 10 . The avalanche
breakdown voltage (for mWW > ) is larger than 1500 V ( m 100 µ>mW ). For a
reverse block voltage of 120 V, we can choose a width such that punch-through
occurs, i.e.,
. 2
2
s
DPT
WqNV
ε=
Thus,
. cm 1096.32 3−×=
ε=
D
PTs
qNV
W
When switching occurs,
. 121 ≅+ αα
That is,
6.04.01
ln5.00
1
=−=
=
JJ
W
Lpα
. 51.1
106.391025
5.06.0
ln4
4
0
=×
×=
−
−
JJ
49
Therefore,
250 cmA 1025.25.4 −×=≅ JJ
. cm 4.441025.2
101Area 2
5
3
=×
×==−
−
JI s
28. In the 2np2n1 −− transistor, the base drive current required to maintain current conductionis
KII )1( 21 α−= .In addition, the base drive current available to the 2np2n1 −− transistor with areverse gate current is
gA III −= 12 α .
Therefore, when use a reverse gate current, the condition to obtain turn-off of the thyristor
is given by
12 II <or KgA III )1( 21 αα −<− .Using Kirchhoff’s law, we have
gAK III −= .Thus, the condition for turn-on of the thyristor is
Ag II2
21 1
ααα −+
> .
Note that if we define the ratio of IA to Ig as turn-off gain, then the maximum turn-offgain maxβ is
121
2max −+
=ααα
β .
50
CHAPTER 6
1.
ECEF
Ei
EV
VG = VT
ψS
= 2ψB
METAL OXIDE n-TYPE SEMICONDUCTOR
51
2.
3.
ECEi
EF
EV
n+ POLYSILICON OXIDE p-TYPE SEMICONDUCTOR
n+ POLYSILICON OXIDE p-TYPE SEMICONDUCTOR
φms
VG = VFB = φφms
EFECEi
EV
EC
EiEF
EV
52
4.
0 W x
-dqND
QM
QP
ρS(x)
-d 0 W
x
E (x)
-d 0 W
x
ψ (x)
V Voψs
(a)
(b)
(c)
53
5. A
i
As
mNq
nN
kT
W2
ln
2
=ε
= 21619
9
1614
1051061
10659
105ln026010858911
×××
×
××××
−
−
.
....
= 1.5 ×10-5 cm = 0.15 µ m.
6. msox
ox
WdC
)/(min εεε
+=
µ150.Wm = m From Prob. 5
8
57
14
100361051
91193
108
1085893 −
−−
−
×=××+×
××=∴ .
...
..Cmin F/cm2 .
7. V42010659
10ln0260ln
9
17
..
.nN
qkT
i
AB =
×==ψ
s
As
WqNε
=E at intrinsic Bs ψψ =
51719
14
1074.010106.1
42.01085.89.1122 −−
−
×=××
××××==A
ss
qNW
ψεcm
5
14
51719
1011110858911
10740101061×=
××××××
=−
−−
...
..sE V/cm
Eo = Esoxε
ε s = 1.11 ×105×93911
.. = 3.38 ×105 V/cm
V = Vo+ sψ = Eod + sψ = ( )75 10510383 −×××. +0.42. = 0.59 V.
8. At the onset of strong inversion, sψ =2 Bψ ⇒ VG=VT
thus, VG =o
mA
CWqN
+2 Bψ
From Prob. 5, Wm = 0.15£gm, Bψ = 0.026ln
××
9
16
10659
105
.= 0.4 V
Co =6
14
10
1085893−
−×× .. = 3.45×10-7 F/cm2
GV∴ =7
51619
10453
10511051061−
−−
××××××
...
+0.8 = 0.35 + 0.8 = 1.15V.
54
9. ∫−
−−
−
×××==610
0
2617
6
1917 ])10(10
21
[10
106.1)10(
1dyyq
dQot
= 8×10-9 C/cm2
2
7
9
1032.21045.3
108 −−
−
×=×
×==∆o
otFB C
QV V.
10. ∫=d
otot dyyyd
Q
0 )(
1ρ
)(105 11 xqot δρ ××= , where
×≠×=∞
=−
−
7
7
105,0
105,)(
y
yxδ
19711
6106.1105105
101 −−
−××××××=∴ otQ
= 4×10-8 C/cm2
12.01045.3
1047
8
=×
×==∆∴−
−
o
otFB C
QV V
11. ∫−
×××=610
0
23 )105(1
dyyqyd
Qot
= 2.67×10-8 C/cm2
2
7
8
1074.71045.31067.2 −
−
−
×=××==∆∴
o
otFB C
QV V.
12. moo
otFB N
dd
Cq
CQ
V ××==∆ , where Nm is the area density of Qm.
11
19
7
1047.6106.1
1045.33.0 ×=×
××=×∆=⇒−
−
qCV
N oFBm cm-2 .
13. Since )( TGD VVV −<< , the first term in Eq. 33 can be approximated as
DBGon V)V(CLZ ψµ 2− .
Performing Taylor’s expansion on the 2nd term in Eq. 33, we obtain
D/
B/
BD/
B/
B/
B/
BD V)()(V)()()()V( 212321232323 223
2223
222 ψψψψψψ =−+≅−+
Equation 33 can now be re-written as
.)10(10531
106.110
1 362319
6
−−−
×××××=
55
DTGon
Do
BAsBGon
DBo
AsDBGonD
V)VV(C)LZ
(
VC
)(qNVC
LZ
VC
qNV)V(C
LZ
I
−≅
+−≅
×−−≅
µ
ψεψµ
ψε
ψµ
222
2232
32
2
where o
BAsBT C
)(qNV
ψεψ
222 += .
14. When the drain and gate are connected together, DG VV = and the MOSFET is
operated in saturation )( DsatD VV > . DI can be obtained by substituting
DsatD VV = in Eq. 33
[ ]
−+
−
−==
2/32/3 )(2)2(2
32
22 BBDsat
o
AsDsatB
DsatonVVD V
C
qNV
VC
LZ
IGD
ψψε
ψµ
where DsatV is given by Eq. 38. Inserting the condition 0)( == LyQn into Eq.27 yields
02221 =−++= GBBDsatAs
oDsat V)V(qN
CV ψψε
For BDsatV ϕ2<< , the above equation reduces to
TBo
BAsDG V
C
)(qNVV =+== ψ
ψε2
22 .
Therefore a linear extrapolation from the low current region to 0=DI will yieldthe threshold voltage value.
15. 400109.65
1050.026lnln
9
16
.)nN
(q
kT
i
A =
××==
−ψ V
7
161914
10453
105106110858911−
−−−
×××××××=≡
....
C
qNK
o
Asε
= 0.27
+−+−≅∴
2
2 2112
KV
KVV GBGDsat ψ
= ])27.0(
1011[)27.0(8.05 2
2 +−+−
= 3.42 V
27
)7.05(12
1045.380010)(
2−
××××=−=
−
TGon
Dsat VVL
CZI
µ
= 2.55×10-2 A.
56
16. The device is operated in linear region, since 1.0=DV V < 5.0)( =− TG VV V
Therefore, )(. TGonD
Dd VVC
LZ
V
Ig
constGV−=
∂∂
==
µ
= 5.01045.350025.05 7 ×××× −
= 1.72×10-3 S.
17. DonG
Dm VC
LZ
VI
gconstDV
µ=∂∂
== .
= 1.01045.350025.05 7 ×××× −
=3.45×10-4 S.
18. o
BAsBFBT C
qNVV
ψεψ
22 ++= , )
1065.9
10ln(026.0
9
17
×=Bψ
7
1019
1045.3105106.1
2 −
−
××××−−−=−= B
g
o
fFB
E
C
QV
msψφ
= 102.042.056.0 −=−−− V
7
191714
1045.3106.142.0101085.89.112
84.01−
−−
×××××××++−=∴ TV
= 49.084.01 ++−= 0.33 V
( msφ can also be obtained from Fig. 8 to be – 0.98 V).
19. 71045.3
33.07.0−×
+= BqF
11
19
7
108106.1
1045.337.0 ×=×
××=−
−
BF cm-2 .
20. 14.042.056.02
−=+−=+−= Bg
ms
Eψφ V
7
171914
1045.342.010106.11085.89.112
84.002.014.0
22
−
−−
×××××××−−−−=
−−−=o
BDsB
o
fmsT C
qN
C
QV
ψεψφ
= 49.1− V.
57
21. 71045.3
49.17.0−×
+−=− BqF
12
19
7
107.1106.1
1045.379.0 ×=×
××=−
−
BF cm-2 .
22. The bandgap in degenerately doped Si is around 1eV due to bandgap-
narrowing effect. Therefore,
86.0114.0 =+−=msφ V49.049.084.002.086.0 −=−−−=∴ TV V.
58
23. 42.01065.9
10ln026.0
9
17
=
×=Bψ V
o
oo
o
BAsB
o
fmsT
C.
.
C....
.C
..
C
qN
C
qQV
8
1917141119
10215140
106142010108589112840
101061980
22
−
−−−
×+−=
××××××++××−−=
++−=ψε
ψφ
ddCo
1314 1045.31085.89.3 −− ×=××=
14.201045.3
102.1520
13
8
>×
××⇒>−
−dVT
51057.4 −×>∴ d cm = 0.457 µm.
24. A£g 1.0at V 5.0 == dT IV
Subthreshold swing =
1
0
0
loglog−
==
−
−
T
VDVVD
V
IIGTG
0log7
5.01.0
=−−=
GVDI
12log 0 −==GVDI A 101 120
−= ×=∴
GVDI .
25.
( ) 22
2 BBSB
o
AsT V
C
NqV ψψ
ε−+=∆
V 42.0)1065.9
10ln(026.0
9
17
=×
=Bψ
7
7
14
109.6105
1085.89.3 −−
−
××
××=oC F/cm2
V 1.0=∆ TV if we want to reduce ID at VG = 0 by one order of magnitude,
since the subthreshold swing is 100 mV/decade.
( )V. 83.0
84.084.0109.6
101085.89.4106.121.0
7
171419
=∴
−+×
××××××=−
−−
BS
BS
V
V
26. Scaling factor κ =10
Switching energy = 2)(21
VAC ⋅
59
κ
κ
κε
VV
AA
Cd
C ox
=′
=′
==′
2
∴scaling factor for switching energy : 1000
1111322 ==⋅⋅
κκκκ
A reduction of one thousand times.
27. From Fig. 24 we have
−+−=∆−=∆−=+
∆−=
++−=∆
=−∆+∆∴
−+=∆+
12
1112
222
'
2'
2
022
)()(2
222
j
mj
jmjj
jmj
mmjj
rW
L
r
LLL
LLL
LL
rWrr
rWr
WWrr
From Eq. 17 we have
.12
1)2
'(
)regionr rectangula thein charge space region al trapezaid thein charge space(
−+−=−
+=
−=∆
jo
jmA
o
mA
o
mA
oT
rW
LC
rWqN
CWqN
LLL
CWqN
CV
28. Pros:1. Higher operation speed.2. High device density
Cons:1. More complicated fabrication flow.2. High manufacturing cost.
29. The maximum width of the surface depletion region for bulk MOS
nm 49
cm 109.4
105106.1)1065.9/105ln(026.01085.89.11
2
)/(ln2
6
1719
91714
2
=×=
×××××××××=
=
−
−
−
A
iAsm Nq
nNkTW
ε
For FD-SOI, nm 49=≤ msi Wd .
60
30. o
siABFBT C
dqNVV ++= ψ2
V. 18.0
28.01.0 1063.8
103105106.192.002.1
F/cm 1063.8104
1085.89.3
V 92.0)(ln22
V 02.11065.9
105ln026.0
212.1
)(ln2
7
61719
27
7
14
9
17
=+−=
××××××++−=∴
×=×
××=
=×=
−=
×
×−−=−−==
−
−−
−−
−
T
o
i
AB
i
AgmsFB
V
C
nN
qkT
nN
qkTE
V
ψ
φ
31. oC
sidqNTV
A ∆=∆
mV 461063.8
105105106.17
71719
=×
×××××=−
−−
Thus, the range of VT is from (0.18-0.046)= 0.134 V to (0.18+0.046) = 0.226 V.
32. The planar capacitor
C = 15
6
1424
1045.3101
1086.89.3)101( −−
−−
×=×
×××=dA oxε F
For the trench capacitor
A = 4× 7 µm2+ 1 µm2 = 29 µm2
C = 29 ×3.45 ×10-15 F = 100 × 10-15 F.
33. 11
3
14 101.31045.2
105 −−
− ×=×
××==d
dVCI A
34. )( Toipo VVCLZ
g −= µ
4 × 10-5 = A ( TV−− 5 ) VVT 7=∴ 1 × 10-5 = A( 25 +− ) 9)2(7 =−−=∆V V.
35. 0
2C
qNVV BAs
BFBT
ψεψ ++=
61
V 0.980.420.56
022
V 42.01065.9
10ln026.0
F/cm1045.310
10854.89.3
9
17
B
28
5
14
0
−=−−=
−−−=−=
=
×
=
×=××= −−
−
Bgf
msFB
EQV
C
ψφ
ψ
V 4.34
4.90.420.98 1045.3
106.142.0101085.89.11242.098.0 8
191714
=++−=
×××××××++−=∴ −
−−
TV
V. 2.02
32.234.4
V 2.32
1045.3106.11058
1911
0
=−=
−=×
×××−=−=∆−
−
T
fFB
V
C
QV
62
CHAPTER 7
1. From Eq.1, the theoretical barrier height is
eV 54.001.455.4 =−=−= χφφ mBn
We can calculate Vn as
V 188.0)102
1086.2ln(0259.0ln
16
19
=×
×==D
Cn N
Nq
kTV
Therefore, the built-in potential is
V 352.0188.054.0 =−=−= nBnbi VV φ .
2. (a) From Eq.11
/V/F)(cm 103.202
10)6.42.6()/1( 2214142
×−=−−
×−=dV
Cd
3-16
2 cm 107.4/)/1(
12×=
−=
dVCdqN
sD ε
V 06.0107.4
107.4ln0259.0ln
16
17
=
××==
D
Cn N
Nq
kTV
From Fig.6, the intercept of the GaAs contact is the built-in potential Vbi,
which is equal to 0.7 V. Then, the barrier height is
V 76.0=+= nbiBn VVφ
(b) 217 A/cm 105×=sJ
8* =A A/K2-cm2 for n– type GaAs
kTqs
BneTAJ /2* φ−=
eV 72.0105
)300(8ln0259.0)ln( 7
22*
=
×
×== −
sBn J
TAq
kTφ
The barrier height from capacitance is 0.04 V or 5% larger.
63
(c) For V = –1 V
m 0.222 cm 1022.2
107.4106.1)17.0(1009.12)(2
5
1619
12
µ
ε
=×=
×××+××=
+=
−
−
−
D
Rbis
qNVV
W
V/cm 1043.1 5×==s
Dm
WqNε
E
28 F/cm 1022.5 −×==W
C sε.
3. The barrier height is
V 64.001.465.4 =−=−= χφφ mBn
V 177.0103
1086.2ln0259.0ln
16
19
=
×××==
D
Cn N
Nq
kTV
The built-in potential is
V 463.0177.064.0 =−=−= nBnbi VV φ
The depletion width is
ìm 142.0463.0103106.11085.89.112)(2
1619
14
=×××××××=
−= −
−
D
bis
qNVV
Wε
The maximum electric field is
V/cm. 1054.6)1085.8(9.11
)1042.1()103()106.1(0)( 4
14
51619
×=××
×××××====−
−
WqN
xs
D
εEE m
4. The unit of C needs to be changed from µF to F/cm2, so
1/C2 = 1.74×1015 – 2.12×1015 Va (cm2/F)2
Therefore, we obtain the built-in potential at 1/C2 = 0
V 74.01012.21057.1
15
15
=××=biV
64
From the given relationship between C and Va, we obtain
152
1012.2
1
×−=
adVC
d (cm2/F)2/V
From Eq.11
×××××=
−=
−− 151419
2
1012.21
1085.89.11106.12
/)/1(12
dVCdqN
sD ε
-315 cm 106.5 ×=
V 161.0106.5
1086.2ln0259.0ln
16
19
=
××==
D
Cn N
Nq
kTV
We can obtain the barrier height
V. 901.0161.074.0 =+=+= nbiBn VVφ
5. The built-in potential is
V 605.0
195.08.0
105.11086.2
ln0259.08.0
ln
16
19
=−=
××−=
−=D
CBnbi N
Nq
kTV φ
Then, the work function is
V. 81.4
01.48.0
=+=+= χφφ Bnm
6. The saturation current density is
65
27
2
2*
A/cm 1081.3
0259.08.0
exp)300(110
exp
−×=
−××=
−
=kTq
TAJ Bns
φ
The injected hole current density is
211163
29192
A/cm 1019.1105.1101
)1065.9(12106.1 −−
−
×=×××
××××==Dp
ippo NL
nqDJ
)1(
)1(
currentElectron current Hole
/
/
−
−=
kTqVs
kTqVpo
eJ
eJ
.1031081.31018.1 5
3
11−
−
−
×=××==
s
po
J
J
7. The difference between the conduction band and the Fermi level is given by
V. 04.0101
107.4ln0259.0
17
17
=
××=nV
The built-in potential barrier is then
V 86.004.09.0 =−=biV
For a depletion mode operation, VT is negative. Therefore, From Eq.38a
m.ì 0.108 cm 1008.1
86.01019.2106.1
86.01085.84.12210106.1
2
086.0
5
2
12
2
14
172192
=×>
>××
>×××××
==
<−=
−
−
−
−
−
a
a
aNqaV
VV
s
DP
PT
ε
66
8. From Eq.33 we obtain
DbiG
P
p
Pm V
VVV
VI
g 2 2 +
=
= Dbi
Psn VVV
aLZ
εµ
62.41085.84.122
)103(107106.12 14
2516192
=×××
×××××==−
−−
s
DP
aqNV
ε V
mg ∴ = 184.062.4
105.1103.01085.84.124500105
44
144
××××
×××××−−
−−
= 1.28×10-3 S = 1.28 mS.
9. (a) The built-in voltage is
×−=−= 17
17
10107.4
ln025.09.0nBnbi VV φ = 0.86 V
At zero bias, the width of the depletion layer is
2
D
bis
qNV
Wε
= = 1719
12
10106.186.01009.12
×××××
−
−
= 1.07 × 10-5 cm
= 0.107 µm
Since W is smaller than 0.2 µm, it is a depletion-mode device.
(b) The pinch-off voltage is
14
517192
1085.84.122)102(10106.1
2 −
−−
××××××==
s
DP
aqNV
ε = 2.92 V
and the threshold voltage is
VT = Vbi – VP = 0.86 – 2.92 = –2.06 V.
10. From Eq.31b, the pinch-off voltage is
67
14
517192
1085.84.122)102(10106.1
2 −
−−
××××××==
s
DP
aqNV
ε= 0.364 V
The threshold voltage is
VT = Vbi – Vp = 0.8 – 0.364 = 0.436 V
and the saturation current is given by Eq. 39
( )2
2 TGns
Dsat VVaL
ZI −=
µε
= 42
44
144
107.4)436.00()101()105.0(245001085.84.121050 −
−−
−−
×=−××××
×××××A.
11. 0.85 – 0.0259ln 2
14
1917
1085.84.122106.1107.4
aN
ND
D−
−
×××××
−
× = 0
For ND = 4.7 × 1016 cm-3
a = DD NN
)107.3(107.4ln0259.085.0
321
17 ×
×−
= 1.52 ×10-5 cm = 0.152 µm
For ND = 4.7 × 1017 cm-3
a = 0.496 × 10-5 cm = 0.0496 µm.
12. From Eq.48 the pinch-off voltage is
TC
BnP VqE
V −∆
−= φ
= 0.89 – 0.23 – (–0.5)
= 0.62 V
and then,
14
21
181921
1085.83.122103106.1
2 −
−
×××××××== ddqN
Vs
DP ε
= 0.62 V
68
d1 = 1.68 × 10-6 cm
d1= 16.8 nm
Therefore, this thickness of the doped AlGaAs layer is 16.8 nm.
13. The pinch-off voltage is
4
7181921
1085.83.122)1050(10106.1
2 −
−−
×××××××==
s
DP
dqNV
ε = 1.84 V
The threshold voltage is
PC
BnT VqE
V −∆−= φ
= 0.89 – 0.23 – 1.84
= –1.18 V
When ns = 1.25× 1012 cm-2, we obtain
[ ] 12
70
19
14
1025.1)18.1(010)850(106.1
1085.83.12 ×=−−××++××
××=−−
−
dns
and then
d0 +58.5 = 64.3
d0 = 5.8 nm
The thickness of the undoped spacer is 5.8 nm.
14. The pinch-off voltage is
14
27171921
1085.83.122)1050(105106.1
2 −
−−
××××××××==
s
DP
dqNV
ε= 1.84 V
The barrier height is
79.084.125.03.1 =++−=+∆+= PC
TBn VqE
Vφ V
69
The 2DEG concentration is
[ ] 12
719
14
1029.1)3.1(010)81050(106.1
1085.83.12 ×=−−××++××
××=−−
−
sn cm-2.
15. The pinch-off voltage is
4
21
181921
1085.83.122101106.1
5.12 −
−
×××××××=== ddqN
Vs
DP ε
The thickness of the doped AlGaAs is
1819
14
1 10106.11085.83.1225.1
××××××= −
−
d = 4.45×10-8 cm = 44.5 nm
93.05.123.08.0 −=−−=−∆
−= PC
BnT VqE
V φ V.
16. The pinch-off voltage is
212
dqN
Vs
DP ε
=
= ( )27
14
1819
10351085.83.122103106.1 −
−
−
×××××××
= 2.7 V
the threshold voltage is
pC
BnT VqE
V −∆−= φ
= 0.89 – 0.24 – 2.7
= –2.05 V
Therefore, the two-dimensional electron gas is
[ ] 12
719
14
102.3)05.2(010)835(106.1
1085.83.12 ×=−−××+××
××=−−
−
sn cm-2.
70
CHAPTER 8
1. Z0 =CL
nH 25.1175102 21220 =××=⋅= −ZCL .
2. 222
2
+
+
=
dp
bn
amc
f r
( ) ( )
. GHz 616.11162
m/s103
40102
8
22
=××=
++= c
3. pngbi VVqEV ++≅ )/( = 1.42+0.03+0.03 = 1.48 V
( )
( )
. F/cm 1013.61089.11016.1
nm 18.9 cm1089.1
25.048.110101010
106.11016.12
2
276
12
6
1919
1919
19
12
−−
−
−
−
−
×=××==
=×=
−
×+
×××=
+
+=
WC
VVNNNN
qW
S
biDA
DAS
ε
ε
4. exp1exp 0
+
−
=
kTqV
IVV
VV
IIPP
p
From Fig. 4, We note that the largest negative differential resistance occurs between Vp<V<VV.
The corresponding voltage can be obtained from the condition d2I/d2V = 0. By neglecting the
second term in Eq. 5, we obtain
71
( )
. 2.27
0367.0 1.02.0
1exp 1.0
2.0101.0
10
V2.01.022
01 exp 2
1 exp
1
2.0
2
22
2.0
322
2
2
Ω−=
=
−=
−
×−=
=×==∴
=
−
+−=
−
−≅
−
−−
V
V
P
PP
P
P
P
PP
P
P
P
dVdI
R
dVdI
VV
VV
VVI
VI
dVId
VV
VVI
VI
dVdI
5. (a) RSC = SS
W
SS
W
vAW
dxvA
IxI
dxI εε 2
11 2
0
0 ==∆ ∫∫ E
( ) Ω=×××
×=−−
−
137101005.1 )105(2
1012
7124
24
(b) The breakdown voltage for ND = 1015 cm-3 and W = 12 µm is 250 V (Refer to Chapter 4).
The voltage due to RSC is
( ) =×××= − 13710510 43SCIR 68.5 V
The total applied voltage is then 250 + 68.5 = 318.5 V.
6. (a) The dc input power is 100V(10-1A) = 10W. For 25% efficiency, the power dissipated as
heat is 10W(1-25%) = 7.5 W.
C75)C/W10(W5.7 ooT =×=∆
(b) =×=∆ C75)C/mV60( ooBV 4.5 V
The breakdown voltage at room temperature is (100-4.5) = 95.5V .
7. (a) For a uniform breakdown in the avalanche region, the maximum electric field is
Em = 4.4 ×105 V/cm. The total voltage at breakdown across the diode is
72
( )
( ) ( )
V 8.742.576.17
100.4-3 1009.1
105.1106.1104.4104.0104.4
4
12
1219545
=+=
×
×
×××−×+××=
−
−+=
−−
−−
AS
mAmB xWqQ
xVε
EE
(b) The average field in the drift region is
( ) V/cm102.2104.03
2.57 5
4×=
×− −
This field is high enough to maintain velocity saturation in the drift region.
(c) ( ) ( ) . GHz 19104.032
10
2 4
7
=−
=−
=−
A
S
xW
vf
8. (a) In the p layer
E1(x) = s
m
xqNε
1−E 0 bx ≤≤ = 3 µm
E2(x) =s
m
bqNε
1−E b Wx ≤≤ = 12 µm
E2(x) should be larger than 105 V/cm for velocity saturation
51 10≥−∴s
m
bqNε
E
or Em 11515 1066.41010 −×+=+≥s
bqNε
N1.
This equation coupled the plot of Em versus N in Chapter 3 gives
N1 = 7 × 1015 cm-3 for Em = 4.2 × 105 V/cm
2
EE bV m
B
)( 2−=∴ +E2W = 45
45
109102
10310)12.4( −−
××+×××−
73
= 138 V
(b) Transit time t = 7
4
1010)312(
−×−=−
svbW
= 9×10-15 = 90 ps .
9. (a) For transit-time mode, we require n0L ≥ 1012 cm-2.
316412120 cm10101/10/10 −− =×=≈ Ln
(b) t = L/v = 10-4 / 107 = 10-11 s = 10 ps
(c) The threshold field for InP is 10.5 kV/cm; the corresponding applied voltage is
( ) V 525.01012
105.10 43
=×
×= −V
The current is
( ) ( ) 86.3101025.5104600106.1 4316190 =××××××=== −−AnqJAI n Eµ A
The power dissipated in the device is then
W 02.2== IVP .
10. (a) Referring to Chapter 2, we have
319172
3
0
017
23
23
2
cm1033.371107.407.02.1
107.4
22
−×=××=
×=
=
=
mm
m
mN
kTmN
nL
nUCL
nUCU
h
π
(b) For Te = 300 K
( )4104.4
97.11 exp710259.0
eV31.0exp71)/exp(
−×=
−×=
−×=∆− e
CL
CU kTENN
(c) For Te = 1500 K
74
( ) ( )
5.6
394.2 exp71300/1500 0259.0
eV31.0exp71)/exp(
=
−×=
−×=∆− e
CL
CU kTENN
Therefore, at Te = 300 K most electrons are in the lower valley. However, at Te = 1500 K ,
87%, i.e., 6.5/(6.5+1), of the electrons are in the upper valley.
11. The energy En for infinitely deep quantum well is
2
2*
2
8n
Lm
hEn =
( )( )LE
Lmnh
LEn 13
*
22 2 2
8=−=
∆∆ −
LLE
En ∆=∆ 12
meV 31 =∆∴ E , =∆ 2E 11 meV .
12. From Fig. 14 we find that the first excited energy is at 280 meV and the width is 0.8 meV. For
same energy but a width of 8 meV, we use the same well thickness of 6.78 nm for GaAs, but
the barrier thickness must be reduced to 1.25 nm for AlAs.
The resonant-tunneling current is related to the integrated flux of electrons whose energy is in
the range where the transmission coefficient is large. Therefore, the current is proportional to
the width nE∆ , and sufficiently thin barriers are required to achieve a high current density.
75
CHAPTER 9
1. Eq.9)(From eV 2.071.24/0.6)m6.0( ==µhv
α (0.6 µm) = 3×104 cm-1
The net incident power on the sample is the total incident power minus the reflected
power, or 10 mW.
( ) 31032 1051104 −×−− ×=− We
W = 0.231 µm.
The portion of each photon’s energy that is converted to heat is
%4.3107.2
42.107.2 =−=−ν
ν
h
Eh g
The amount of thermal energy dissipated to the lattice per second is
31.4%×5 = 1.57 mW.
2. For λ = 0.898 µm, the corresponding photon energy is
eV38.124.1 ==λ
E
From Fig. 18, we obtain 2n (Al0.3Ga0.7As) = 3.38
( )( )
( )[ ]( )
. %15.30315.0
38.31
2117cos138.314cos14
.21172958.038.31
sin
2221
21
2
1
==
+′−××=
+−
=
′=⇒===
oc
occ
nn
nnEfficiency
nn
θ
θθ
3. From Eq. 15
29601393
13932
..
.R =
+
−=
(a) The mirror loss
76
58.40296.01
ln10300
11ln
14
=
×=
−RL cm-1.
(b) The threshold current reduction is
( ) ( )( )
%.6.3658.4010
90.0296.01
ln103002
158.40
1ln
1
1ln
211
ln1
296.09.0,296.0296.0
4
21
21
=+
⋅×⋅−
=
+
+−
+
≈
===−=
−
RL
RRLRL
RJRRJRJ
th
thth
α
αα
4. From Eq. 10
cc nnnn
θθ sinsin 212
1 ⋅=⇒=
From Eq. 14
( ) ( )( )45 101sin16.3108exp1exp1 −×⋅−⋅×−−=∆−−≅Γ cdnC θ
For θc = 84o n1 = 3.58 Γ1 = 0.794
θc = 78o n2 = 3.52 Γ2 = 0.998 .
5. From Eq. 16 we have
Lnm 2 =λ .
Differentiating the above equation with respect to λ, we obtain
λλλ
dnd
Lmddm
2=+ .
77
Substituting λLn2 for m and letting dm/dλ = - ∆m/∆λ, yield
−
∆=∆∴
=+
∆∆−
λλ
λλ
λλλλ
dnd
nLn
m
dnd
LLnm
12
22
2
and( )
( ) ( ).nm 97.0m107.9
5.258.389.0
130058.32
189.0 42
=µ×=
−
×=∆ −λ
6. From Eq. 22
+
Γ=
RLg
1ln
11α and Eq. 15
2
1
1
+
−=n
nR
R1 = 0.317, R2 = 0.311
( )
( ) 217311.01
ln10100
1100
998.01
78
270317.01
ln10100
1100
794.01
84
4
4
=
×+=
=
×+=
−
−
o
o
g
g
×=
⋅′ − RRL1
ln10100
199.0
1ln
21
4
For R1 = 0.317
50317.01
ln10100
199.0317.0
1ln
21
4 =′⇒
×=
⋅′ −L
L µm
For R2 = 0.311
43.50311.01
ln10100
199.0311.0
1ln
21
242
=′⇒
×=
⋅′ −L
L µm.
7. From Eq. 23a
78
For R = 0.317
2
4cmA 1000
99.0317.01
ln101002
110010 −
−=
×××+×=thJ
and so mA 5105101001000 44 =××××= −−thI
For R = 0.311
β ∝Γ ⇒ β2 = 0.1×0.998/0.764 = 0.13
2
4cmA 766
99.0311.01
ln101002
110066.7 −
−=
×××+×=thJ
and so mA 83.310510100766 44 =××××= −−thI .
8. From the equation, we have for m = 0:
0442 =± oBB LnLn λλλ m (25a)
which can be solved as
+±−±=
2
16164 22o
B
LnLnLn λλ (25b)
There are several variations of ± in this solutions. Take the solution which is the only
practical one, i.e., λB ≈ λo, gives λB = 1.3296 or 1.3304 µm.
m196.04.32
33.1 µ=×
≅d .
9. The threshold current in Fig. 26b is given by
Ith = I0 exp (T/110).
Therefore
( ) 1C0091.0
11011 −
==≡ oth
th dTdI
Iξ .
If T0 = 50 oC, the temperature coefficient becomes
79
( ) 1C02.0
501 −== oξ .
which is larger than that for T0 = 110 oC. Therefore the laser with T0 = 50 oC is worse
for high-temperature operation.
10. (a) ∆I = q (µn + µp) ∆nEA
( )
( )( )( )313
219
3
cm1010126.01017003600106.1
1083.2
−−−
−
=××+×
×=
+∆=−=∆∴
AqI
pairsholeelectronnpn Eµµ
(b) sµτ 1206.231083.2 3
=×=−
(c) ( ) ( ) 9
4
313 105.2
102.110
exp10exp ×=
×
−=−∆=∆ −
−
τtntn cm-3 .
11. From Eq. 33
A55.21055.2
101050001063000
310
85.0
6
4
106
µ=×=
×
⋅×⋅⋅
×
⋅=
−
−
−−
qqI p
and from Eq. 35
Gain 91010
500010630004
10
=×
⋅×⋅==−
−
Ln Eτµ
.
12. From Eq. 36
⋅=
⋅
=
⋅
=
−
qh
Rq
hP
I
h
P
q
I
opt
poptp ννν
η1
The wavelength λ of light is related to its frequency ν by ν = c/λ, where c is the velocity of
light in vacuum. Therefore νh /q = hc / λq and h = 6.625×10-34 J-s, c = 3.0×1010 cm/s, q =
1.6×10–19 coul, 1 eV = 1.6×10–19 J.
80
Therefore, h v/q = 1.24 / λ (µm)
Thus, η = (R×1.24) / λ and R = (ηλ) / 1.24.
13. The electric field in the p-layer is given by
( )s
m
xqNx
ε1
1 −= EE bx ≤≤0 ,
where Em is the maximum field. In the p layer, the field is essentially a constant given by
( ) WxbbqN
xs
m ≤<−= 1
εEE 2
The electric field required to maintain velocity saturation of holes is ~ 105 V/cm.
Therefore
51 10≥−s
m
bqNε
E
or
111515 1066.41010 N
bqN
sm
−×+=+≥ε
E .
From the plot of the critical field versus doping, the corresponding Em are obtained :
N1 = 7×1015 cm-3
Em = 4.2×105 V/cm
The biasing voltage is given by
( ) ( ) ( )
V.138
109102
103102.32
4545
22
=
×+×××=+−
= −−
Wb
V mB E
E E
The transit time is
( )ps. 90109
10
109 117
4
=×=×=−≈ −−
s
bWt
ν
81
14. (a) For a photodiode, only a narrow wavelength range centered at the optical signal
wavelength is important; whereas for a solar cell, high spectral response over a broad
solar wavelength range are required.
(b) Photodiode are small to minimize junction capacitance, while solar cells are large-area
device.
(c) An important figure of merit for photodiodes is the quantum efficiency (number of
electron-hole pairs generated by incident photon), whereas the main concern for solar
cells is the power conversion efficiency (power delivered to the load per incident solar
energy).
15. kTE
p
p
Dn
n
AVCs
geD
ND
NNAqNI −
+=
ττ11
)a(
( )( )( )
( )
( )( )1
A1028.2
1067.51043.2
1055.2
1051
103.9
107.11
1066.21086.2106.12
12
2.431420
12.1
719516
191919
−−=
−=
×=
××=
×
××
+×
××××=
−
−−
−−−
−
kTqVsL
LkTqV
s
kTeV
eIII
IeII
e
e
V 0 0.1 0.2 0.3 0.4 0.5 0.6 0.65 0.7 (V)
)1( −kTqV
s eI0 1.1×10-
75×10-6 2.5×10-
41.1×10-
20.55 26.8 179 1520 (mA)
IL 95 95 95 95 95 94.5 68.2 -84 -1425 (mA)
(b) V 68.01028.2
1095ln0259.0ln
12
3
=
××=
=
−
−
s
LOC I
Iq
kTV
(c) ( ) VIeVIP LkTqV
s −−= 1
82
( )( ) L
kTqVs
LkTqV
skTqV
s
IVeI
IekT
qVIeI
dV
dP
−+≈
−+−==
1
10
( )
V.V
VI
Ie
m
s
LkTqV
640
1
=
+=∴
( )[ ]
mW52
0259.07.241ln0259.068.01095
1ln
3
=
−+−×=
−
+−==
−
qkT
kTqV
qkT
VIVIP nOCLmmm
0
50
100
0 0.2 0.4 0.6 0.8
V (V)
I (m
A)
16. From Eq. 38 and 39
( ) LkT/qV
s IeII −−= 1 and
≅
+=
s
L
s
Loc I
Iq
kTII
qkT
V ln1ln
A1049323 1002585060 −−− ×=⋅== .eeII ..kTqVLs
02585.01010493.23 VeI ⋅×−= − and P = I V
83
V I P0 3.00 0.00
0.1 3.00 0.300.2 3.00 0.600.3 3.00 0.900.4 3.00 1.200.5 2.94 1.47
0.51 2.91 1.480.52 2.86 1.490.53 2.80 1.480.54 2.71 1.460.55 2.57 1.41
0.6 0.00 0.00
0.00
0.50
1.00
1.50
2.00
0 0.5 1
V (volts)P
(wat
ts)
∴Maximum power output = 1.49 W Fill Factor
.83.0
36.049.1
=×
==≡ocL
m
ocL
mm
VIP
VIVI
FF
17. From Fig. 40
The output powers for Rs = 0 and Rs = 5 Ω can be obtained from the area
P1 (Rs = 0) = 95 mA×0.375V = 35.6 mW,
P2 (Rs = 5 Ω) = 50 mA×0.18V = 9.0 mW
∴For Rs = 0 P1/ P1 = 100%
For Rs = 5 Ω P2/ P1 = 9/35.6 = 25.3%.
18. The efficiencies are 14.2% (1 sun), 16.2% (10-sun), 17.8% (100-sun), and 18.5%
(1000-sun).
Solar cells needed under 1-sun condition
84
( ) ( )( ) ( )
sun.-1000forcells13001%2.1410%5.18
sun-100forcells1251%2.1410%8.17
sun-10for cells4.111%2.1410%2.16
-1-1
ionconcentrationconcentrat
=×
×=
=×
×=
=×
×=
××
=sunPsun
P
in
in
ηη
85
CHAPTER 10
1. C0 = 1017 cm-3
k0(As in Si) = 0.3
CS= k0C0(1 - M/M0)k0-1
= 0.3×1017(1- x)-0.7 = 3×1016/(1 - l/50)0.7
x 0 0.2 0.4 0.6 0.8 0.9
l (cm) 0 10 20 30 40 45
CS (cm-3) 3×1016 3.5×1016 4.28×1016 5.68×1016 1.07×1017 1.5×1017
0
2
4
6
8
10
12
14
16
0 10 20 30 40 50
l (cm)
N D (1016 cm-3)
2. (a) The radius of a silicon atom can be expressed as
Å175.143.583
so
83
=×=
=
r
ar
(b) The numbers of Si atom in its diamond structure are 8.
So the density of silicon atoms is
322
33atoms/cm 100.5
)Å43.5(88 ×===
an
(c) The density of Si is
86
3
23
2223
cm / g 1002.6
10509.28
/1
1002.6/
×
××=
×=
n
Mρ = 2.33 g / cm3.
3. k0 = 0.8 for boron in silicon
M / M0 = 0.5
The density of Si is 2.33 g / cm3.
The acceptor concentration for ρ = 0.01 Ω–cm is 9×1018 cm-3.
The doping concentration CS is given by
1
0
000)1( −−= k
s MM
CkC
Therefore
318
2.0
18
1
0
0
0
cm108.9
)5.01(8.0109
)1( 0
−
−−
×=
−×=
−=
k
s
MM
k
CC
The amount of boron required for a 10 kg charge is
2218 102.4108.9338.2000,10 ×=×× boron atoms
So that
boron g75.0atoms/mole1002.6
atoms102.4g/mole8.10
23
22
=×
×× .
4. (a) The molecular weight of boron is 10.81.
The boron concentration can be given as
318
2
233
atoms/cm1078.9 1.014.30.10
1002.6g81.10/g1041.5
fersilicon wa of volumeatomsboron ofnumber
×=××
×××=
=
−
bn
(b) The average occupied volume of everyone boron atoms in the wafer is
87
3
18cm
1078.911×
==bn
V
We assume the volume is a sphere, so the radius of the sphere ( r ) is the
average distance between two boron atoms. Then
cm109.243 7−×==πV
r .
5. The cross-sectional area of the seed is
22
cm 24.0255.0 =
π
The maximum weight that can be supported by the seed equals the product of the
critical yield strength and the seed’s cross-sectional area:
kg 480g108.424.0)102( 56 =×=××
The corresponding weight of a 200-mm-diameter ingot with length l is
m. 56.6cm 656
g 4800002
0.20)g/cm33.2(
2
3
==∴
=
l
lπ
6. We have1
000
0
1/−
−=
k
s MM
kCC
Fractional 0 0.2 0.4 0.6 0.8 1.0solidified
0/CsC 0.05 0.06 0.08 0.12 0.23 ∞
88
7. The segregation coefficient of boron in silicon is 0.72. It is smaller than unity, so the solubility
of B in Si under solid phase is smaller than that of the melt. Therefore, the excess B atoms will
be thrown-off into the melt, then the concentration of B in the melt will be increased. The tail-
end of the crystal is the last to solidify. Therefore, the concentration of B in the tail-end of
grown crystal will be higher than that of seed-end.
8. The reason is that the solubility in the melt is proportional to the temperature, and the
temperature is higher in the center part than at the perimeter. Therefore, the solubility is higher
in the center part, causing a higher impurity concentration there.
9. The segregation coefficient of Ga in Si is 8 ×10-3
From Eq. 18
Lkxs ekCC /
0 )1(1/ −−−=
We have
cm. 24
ln(1.102) 250
105/10511081
ln 1082
/11
ln
1615
3
3-
0
==
××−
×−×
=
−
−=
−
CCk
kL
xs
10. We have from Eq.18
])/exp()1(1[0 LxekekCsC −−−=
So the ratio )]/exp()1(1[0/ LxekekCsC −−−== 1/at 52.0)13.0exp()3.01(1 ==×−•−− Lx= 38.0 at x/L = 2.
0.01
0.11
0.21
0 0.2 0.4 0.6 0.8 1
Fraction Solidified
Cs/
Co
89
11. For the conventionally-doped silicon, the resistivity varies from 120 Ω-cm to 155 Ω-cm. The
corresponding doping concentration varies from 2.5×1013 to 4×1013 cm-3. Therefore the range of
breakdown voltages of p+ - n junctions is given by
V 11600 to7250/109.2)(106.12
)103(1005.1
)(2
171
19
2512
12
=×=××
×××=
≅
−−
−
−
BB
Bcs
B
NN
Nq
VEε
V 4350725011600 =−=∆ BV
%307250/2
±=
∆
∴ BV
For the neutron irradiated silicon, ρ = 148 ± 1.5 Ω-cm. The doping concentration is
3×1013 (±1%). The range of breakdown voltage is
. V 9762 to9570
%)1(103/109.2/103.1 131717
=
±××=×= BB NV
V 19295709762 =−=∆ BV
%19570/2
±=
∆
∴ BV.
12. We have
ls
CCCC
MM
ms
lm
l
s =−−
==b
b
Tat liquid ofweight Tat GaAs ofweight
Therefore, the fraction of liquid remained f can be obtained as following
65.03016
30 =+
≈+
=+
=ls
lMM
Mf
ls
l .
13. From the Fig.11, we find the vapor pressure of As is much higher than that of the Ga.
Therefore, the As content will be lost when the temperature is increased. Thus the
composition of liquid GaAs always becomes gallium rich.
90
14.
−×=×=−=)300/(
8.88exp105)/eV 3.2exp(105)/exp( 2222
TkTkTENn ss
= K 300 C27at 0cm1023.1 0316 =≈× −−
= K 1173 C900at cm107.6 0312 =× −
= K 1473 C1200at cm107.6 0314 =× − .
15. )2/exp(` kTENNn ff −=
= )300//(7.94242/1.1/8.32722 1007.7101105 TkTeVkTeV eee −−− ××=××××
= 1027.5 17−× at 27oC = 300 K
=2.14×1014 at 900oC = 1173 K.
16. 37 × 4 = 148 chips
In terms of litho-stepper considerations, there are 500 µm space tolerance between the
mask boundary of two dice. We divide the wafer into four symmetrical parts for
convenient dicing, and discard the perimeter parts of the wafer. Usually the quality of the
perimeter parts is the worst due to the edge effects.
91
17. MkT
dvf
dvvf
v
v
av πν
8
0
0 ==∫∫
∞
∞
Where
−
=
kTM
kTM
f2
exp2
4 22
2/3ν
νπ
ν
M: Molecular mass
k: Boltzmann constant = 1.38×10-23 J/k
T: The absolute temperature
ν: Speed of molecular
So that
cm/sec1068.4m/sec 4681067.129
3001038.122 4
27
23
×==××
×××=−
−
πνav .
18. cm)Pain (
66.0P
=λ
92
Pa 104.4150
66.066.0 3−×===∴λ
P .
19. For close-packing arrange, there are 3 pie shaped sections in the equilateral triangle.
Each section corresponds to 1/6 of an atom. Therefore
dd
N s
23
21
61
3
triangle theof area trianglein the contained atoms ofnumber
×
×==
=282 )1068.4(3
2
3
2−×
=d
= 214 atoms/cm 1027.5 × .
20. (a) The pressure at 970°C (=1243K) is 2.9×10-1 Pa for Ga and 13 Pa for As2. The
arrival rate is given by the product of the impringement rate and A/πL2 :
Arrival rate = 2.64×1020
2L
A
MT
Pπ
= 2.64×1020
×
×
× −
2
1
12
5
124372.69
109.2
π = 2.9×1015 Ga molecules/cm2 –s The growth rate is determined by the Ga arrival rate and is given by
(2.9×1015)×2.8/(6×1014) = 13.5 Å/s = 810 Å/min .
(b) The pressure at 700ºC for tin is 2.66×10-6 Pa. The molecular weight is 118.69.
Therefore the arrival rate is
s⋅×=
×
×
××
−210
2
620 cmmolecular/ 1028.2
125
97369.118
1066.21064.2
π
If Sn atoms are fully incorporated and active in the Ga sublattice of GaAs, we have an
dd
93
electron concentration of
. cm 1074.12
1042.4109.21028.2 3-17
22
15
10
×=
×
××
21. The x value is about 0.25, which is obtained from Fig. 26.
22. The lattice constants for InAs, GaAs, Si and Ge are 6.05, 5.65,5.43, and 5.65 Å,
respectively (Appendix F). Therefore, the f value for InAs-GaAs system is
066.005.6)05.665.5( −=−=f
And for Ge-Si system is
. 39.065.5)65.543.5( −=−=f
94
CHAPTER 11
1. From Eq. 11 (with ô=0)
x2+Ax = Bt
From Figs. 6 and 7, we obtain B/A =1.5 µm /hr, B=0.47 µm 2/hr, therefore A=
0.31 µm. The time required to grow 0.45µm oxide is
min 44hr 0.720.45)0.31(0.450.47
1 2 ==×+=+= Ax)(xB1
t 2 .
2. After a window is opened in the oxide for a second oxidation, the rate constants are
B = 0.01 µm 2/hr, A= 0.116 µm (B/A = 6 ×10-2 µm /hr).
If the initial oxide thickness is 20 nm = 0.02 µm for dry oxidation, the value
ofôcan be obtained as followed:
(0.02)2 + 0.166(0.02) = 0.01 (0 +ô)
or
ô= 0.372 hr.
For an oxidation time of 20 min (=1/3 hr), the oxide thickness in the window
area is
x2+ 0.166x = 0.01(0.333+0.372) = 0.007
or
x = 0.0350 µm = 35 nm (gate oxide).
For the field oxide with an original thickness 0.45 µm, the effectiveôis given by
ô= .hr 72.27)45.0166.045.0(01.01
)(1 22 =×+=+ AxxB
x2+ 0.166x = 0.01(0.333+27.72) = 0.28053
or x = 0.4530 µm (an increase of 0.003µm only for the field oxide).
3. x2 + Ax = B )( τ+t
)(4
)2
(2
2 τ+=−+ tBAA
x
95
++=+ )(
4 )
2(
22 τt
BA
BA
x
when t >> τ , t >> B
A4
2
,
then, x2 = Bt
similarly,
when t >> τ , t >> B
A4
2
,
then, x = )( τ+tAB
4. At 980 (=1253K) and 1 atm, B = 8.5×10-3 µm 2/hr, B/A = 4×10-2 µm /hr (from Figs. 6
and 7). Since A a2D/k , B/A = kC0/C1, C0 = 5.2×1016 molecules/cm3 and C1 =
2.2×1022 cm-3 , the diffusion coefficient is given by
.s/cm104.79
hr/m101.79
hr/m 102.5
102.22105.8
222
29-
23
2
16
223
0
1
0
1
×=
×=×××
=
=
⋅==
−
µ
µ
CCB
CC
ABAAk
D
5. (a) For SiNxHy
2.11
NSi ==
x
4 x = 0.83
atomic % 2083.01
100H =
++=
yy
4 y = 0.46
The empirical formula is SiN 0.83H0.46.
(b) ñ= 5× 1028e-33.3×1.2 = 2× 1011 Ù-cm
As the Si/N ratio increases, the resistivity decreases exponentially.
96
tA
3C 01
OTa 52
εε=
AAA 020302ONO
tttC
1εεεεεε
++=
( )tA
32
032ONO 2
Cεε
εεε+
=
( )tA
tA
32
2032101
23 εεεεεεε
+=
6. Set Ta2O5 thickness = 3t, ε1 = 25
SiO2 thickness = t, ε2 = 3.9 Si3N4 thickness = t, ε3 = 7.6, area = A then
( ) ( )37.5
6.79.336.729.325
3
2
C
C
32
321
ONO
OTa 52 =××
×+=+
=εε
εεε.
7. Set BST thickness = 3t, ε1 = 500, area = A1
SiO2 thickness = t, ε2 = 3.9, area = A2
Si3N4 thickness = t, ε3 = 7.6, area = A2
then
.0093.0A
A
2
1 =
8. Let
Ta2O5 thickness = 3t, ε1 = 25 SiO2 thickness = t, ε2 = 3.9 Si3N4 thickness = t, ε3 = 7.6 area = A then
dA
tA 0201
3εεεε =
.468.03
1
2 tt
d ==εε
97
9. The deposition rate can be expressed as
r = r0 exp (-Ea/kT)
where Ea = 0.6 eV for silane-oxygen reaction. Therefore for T1 = 698 K
−== 11
6.0 exp2)()(
211
2
kTkTTrTr
ln 2 =
− 300
698300
0259.0
6.0
2T
4 T2 =1030 K= 757 .
10. We can use energy-enhanced CVD methods such as using a focused energy
source or UV lamp. Another method is to use boron doped P-glass which will
reflow at temperatures less than 900 .
11. Moderately low temperatures are usually used for polysilicon deposition, and
silane decomposition occurs at lower temperatures than that for chloride
reactions. In addition, silane is used for better coverage over amorphous
materials such SiO 2.
12. There are two reasons. One is to minimize the thermal budget of the wafer,
reducing dopant diffusion and material degradation. In addition, fewer gas
phase reactions occur at lower temperatures, resulting in smoother and better
adhering films. Another reason is that the polysilicon will have small grains. The
finer grains are easier to mask and etch to give smooth and uniform edges.
However, for temperatures less than 575 ºC the deposition rate is too low.
13. The flat-band voltage shift is
FBV∆ = 0.5 V ~ 0C
Qot
28
8
14
0 F/cm109.610500
1085.89.3 −−−
−
×=×
××==d
C oxε.
4 Number of fixed oxide charge is
98
2-11
19
80 cm101.2
106.1109.65.05.0
×=×
××=−
−
q
C
To remove these charges, a 450 heat treatment in hydrogen for about 30
minutes is required.
14. 20/0.25 = 80 sqs.
Therefore, the resistance of the metal line is
5×50 = 400 Ω .
15. For TiSi2
30 × 2.37 = 71.1nm For CoSi2
30 × 3.56 = 106.8nm.
16. For TiSi2 :
Advantage: low resistivity
It can reduce native-oxide layers
TiSi2 on the gate electrode is more resistant to high-field-
induced hot-electron degradation.
Disadvantage: bridging effect occurs.
Larger Si consumption during formation of TiSi2
Less thermal stability
For CoSi2 :
Advantage: low resistivity
High temperature stability
No bridging effect
A selective chemical etch exits
Low shear forces
Disadvantage: not a good candidate for polycides
99
Ω×=×××
××==−−
− 3
44
6 102.3103.01028.0
11067.2
AL
R ρ
F..
...
S
TL
d
AC 13
4
64414
109210360
1010110301085893 −−
−−−
×=×
×××××××===
εε
ns 42.0101.2102 133 =×××= −RC
Ω×=×××
××== − 3
44
6 102.3103.01028.0
11067.2
AL
R ρ
F107.81036.0
31103.01085.89.3 13
4
414−
−−
×=×
××××××===STL
dA
Cεε
.
17. (a)
ns 93.0109.2103.2 155 =×××= −RC
(b) Ω×=×××
××==−−
− 3
44
6 102103.01028.0
1107.1
LA
R ρ
F101.21036.0
1103.01085.88.2dA 13
4
414−
−
−−
×=×
×××××===STL
Cεε
(c) We can decrease the RC delay by 55%. Ratio = 093
42.0 = 0.45.
18. (a)
RC = 3.2 ×103 ×8.7 × 10-13 = 2.8 ns.
(b) Ω×=×××
××== − 3
44
6 102103.01028.0
1107.1
AL
R ρ
F103.61036.0
31103.01085.88.2d
13
4
414−
−−
×=×
××××××===STLA
C εε
ns. 5.2107.8102.3
ns 5.2107.8102133
133
=×××=
=×××=−
−
RC
RC
19. (a) The aluminum runner can be considered as two segments connected in series:
20% (or 0.4 mm) of the length is half thickness (0.5 µm) and the remaining
1.6 mm is full thickness (1µm). The total resistance is
××
+×
×=
+= −−−−
−
)105.0(10
04.0
1010
16.0103 4444
6
2
2
1
1
AAR
llρ
= 72 Ù.
100
The limiting current I is given by the maximum allowed current density times
cross-sectional area of the thinner conductor sections:
I = 5×105 A/cm2× (10-4×0.5×10-4) = 2.5×10-3 A = 2.5 mA.
The voltage drop across the whole conductor is then
A 105.272 3−××Ω== RIV = 0.18V.
20.
=
h: height , W : width , t : thickness, assume that the resistivities of the cladding
layer and TiN are much larger than CuA and ρρ l
5.0)1.05.0(7.2
×−=
××= ll
WhR AlAl ρ
)25.0()25.0(7.1
ttWhR CuCu −×−
=×
×= llρ
When CuAl RR =
Then 2)25.0(
7.15.04.0
7.2t−
=×
⇒ t = 0.073 µm = 73 nm .
40 n m
60 n m
AlCu
0.5 µm
0.5 µm
101
CHAPTER 12
1. With reference to Fig. 2 for class 100 clean room we have a total of 3500 particles/m3 withparticle sizes ≥ 0.5 µm
350010021 × = 735 particles/m2 with particle sizes ≥ 1.0 µm
3500100
5.4 × = 157 particles/m2 with particle sizes ≥ 2.0 µm
Therefore, (a) 3500-735 = 2765 particles/m3 between 0.5 and 1 µm(b) 735-157 = 578 particles/m3 between 1 and 2 µm(c) 157 particles/m3 above 2 µm.
2. AD
neY 1
9
1
−
=Π=
A = 50 mm2 = 0.5 cm2
%1.302.1)5.01(1)5.025.0(4)5.01.0(4 ==××= −×−×−×− eeeeY .
3. The available exposure energy in an hour is 0.3 mW2/cm2 × 3600 s =1080 mJ/cm2
For positive resist, the throughput is
wafers/hr71401080 =
For negative resist, the throughput is
r wafers/h0129
1080 = .
4. (a) The resolution of a projection system is given by
178.065.0
m£g193.06.01 =×==
NAklm
λ µm
== 222 )65.0(
m193.05.0
)(µλ
NAkDOF = 0.228 µm
(b) We can increase NA to improve the resolution. We can adopt resolution enhancement
techniques (RET) such as optical proximity correction (OPC) and phase-shifting Masks
(PSM). We can also develop new resists that provide lower k1 and higher k2 for better
resolution and depth of focus.
(c) PSM technique changes k1 to improve resolution.
5. (a) Using resists with high γ value can result in a more vertical profile but throughput
decreases.
(b) Conventional resists can not be used in deep UV lithography process because these resists
have high absorption and require high dose to be exposed in deep UV. This raises the
102
concern of damage to stepper lens, lower exposure speed and reduced throughput.
6. (a) A shaped beam system enables the size and shape of the beam to be varied, thereby
minimizing the number of flashes required for exposing a given area to be patterned.
Therefore, a shaped beam can save time and increase throughput compared to a Gaussian
beam.
(b) We can make alignment marks on wafers using e-beam and etch the exposed marks. We can
then use them to do alignment with e-beam radiation and obtain the signal from these marks
for wafer alignment.
X-ray lithography is a proximity printing lithography. Its accuracy requirement is very high,
therefore alignment is difficult.
(c) X-ray lithography using synchrotron radiation has a high exposure flux so X-ray has better
throughput than e-beam.
7. (a) To avoid the mask damage problem associated with shadow printing, projection printing
exposure tools have been developed to project an image from the mask. With a 1:1
projection printing system is much more difficult to produce defect-free masks than it is
with a 5:1 reduction step-and-repeat system.
(b) It is not possible. The main reason is that X-rays cannot be focused by an optical lens.
When it is through the reticle. So we can not build a step-and-scan X-ray lithography
system.
8. As shown in the figure, the profile for each case is a segment of a circle with origin at the
initial mask-film edge. As overetching proceeds the radius of curvature increases so that
the profile tends to a vertical line.
9. (a) 20 sec
0.6 × 20/60 = 0.2 µm…..(100) plane
0.6/16 × 20/60 = 0.0125 µm……..(110) plane
0.6/100 × 20/60 = 0.002 µm…….(111) plane
22.12.025.120 =×−=−= lWWb µm
(b) 40 sec
0.6 × 40/60 = 0.4 µm….(100)plane
103
0.6/16 × 40/60 = 0.025 µm…. (110) plane
0.6/100 × 40/60 = 0.004 µm…..(111) plane
4.025.120 ×−=−= lWWb = 0.93 µm
(c) 60 sec
0.6 ×1 = 0.6 µm….(100)plane
0.6/16 ×1 = 0.0375 µm…. (110) plane
0.6/100 ×1= 0.006 µm…..(111) plane
=×−=−= 6.025.120 lWWb 0.65 µm.
10. Using the data in Prob. 9, the etched pattern profiles on <100>-Si are shown in below.
(a) 20 sec l = 0.012 µm, 5.10 == bWW µm
(b) 40 sec l = 0.025 µm, 5.10 == bWW µm
(c) 60 sec l = 0.0375 µm 5.10 == bWW µm.
11. If we protect the IC chip areas (e.g. with Si3N4 layer) and etch the wafer from the top, thewidth of the bottom surface is
18846252100021 =×+=+= lWW µm
The fraction of surface area that is lost is
221
2 /)( WWW − × 100%=(18842-10002) /18842× 100% = 71.8 %
In terms of the wafer area, we have lost
71.8 % × 2)2/15(π =127 cm2
Another method is to define masking areas on the backside and etch from the back. The widthof each square mask centered with respect of IC chip is given by
6252100021 ×−=−= lWW = 116 µm
Using this method, the fraction of the top surface area that is lost can be negligibly small.
12. 1 Pa = 7.52 m Torr
104
PV = nRT
7.52 /760 × 10-3 = n/V ×0.082 × 273
n/V = 4.42 × 10-7 mole/liter = 4.42 × 10-7 × 6.02 × 1023/1000 =2.7 ×1014 cm-3
mean–free–path
P/105 3−×=λ cm = 5× 10-3 ×1000/ 7.52 = 0.6649 cm = 6649 µm
150Pa = 1128 m Torr
PV = nRT
105
1128/ 760 × 10-3 = n/V × 0.082 × 273
n/V = 6.63 × 10-5 mole/liter = 6.63 ×10-5×6.02×1023/1000 = 4 × 1016 cm-3
mean-free-path
P/105 3−×=λ cm = 5× 10-3 ×1000/1128 = 0.0044 cm = 44 µm.
13. Si Etch Rate (nm/min) = 2.86 × 10-13 × RTE
F
a
eTn−
×× 21
= 2.86 × 10-13 ×3×1015× 298987.1
1048.2
21
3
)298( ××−
× e
= 224.7 nm/min.
14. SiO2 Etch Rate (nm/min) = 0.614× 10-13 ×3×1015× 298987.1
1076.3
21
3
)298( ××−
× e = 5.6 nm/min
Etch selectivity of SiO 2 over Si = 025.07.224
6.5 =
Or etch rate (SiO 2)/etch rate (Si) = 025.086.2614.0 298987.1
)48.276.3(
=× ×+−
e .
15. A three–step process is required for polysilicon gate etching. Step 1 is a nonselective etch
process that is used to remove any native oxide on the polysilicon surface. Step 2 is a high
polysilicon etch rate process which etches polysilicon with an anisotropic etch profile. Step 3 is
a highly selective polysilicon to oxide process which usually has a low polysilicon etch rate.
16. If the etch rate can be controlled to within 10 %, the polysilicon may be etched 10 % longer or
for an equivalent thickness of 40 nm. The selectivity is therefore
40 nm/1 nm = 40.
17. Assuming a 30% overetching, and that the selectivity of Al over the photoresist maintains 3.
The minimum photoresist thickness required is
106
(1+ 30%) × 1 µm/3 = 0.433 µm = 433.3 nm.
18. e
e mqB=ω
31
199
101.9106.1
1045.22−
−
×××=×× B
π
B = 8.75 × 10-2(tesla)
= 875 (gauss).
19. Traditional RIE generates low-density plasma (109 cm-3) with high ion energy. ECR and ICP
generate high-density plasma (1011 to 1012 cm-3) with low ion energy. Advantages of ECR and
ICP are low etch damage, low microloading, low aspect-ratio dependent etching effect, and
simple chemistry. However, ECR and ICP systems are more complicated than traditional RIE
systems.
20. The corrosion reaction requires the presence of moisture to proceed. Therefore, the first line of
defense in controlling corrosion is controlling humidity. Low humidity is essential,. especially
if copper containing alloys are being etched. Second is to remove as much chlorine as possible
from the wafers before the wafers are exposed to air. Finally, gases such as CF4 and SF6 can be
used for fluorine/chlorine exchange reactions and polymeric encapsulation. Thus, Al-Cl bonds
are replaced by Al-F bonds. Whereas Al-Cl bonds will react with ambient moisture and start
the corrosion process , Al-F bonds are very stable and do not react. Furthermore, fluorine will
not catalyze any corrosion reactions.
107
CHAPTER 13
1. Ea(boron) = 3.46 eV, D0 = 0.76 cm2/sec
From Eq. 6, /scm10142.4122310614.8
46.3exp76.0)exp( 215
50−
−×=
××−=−=
kTE
DD a
cm 1073.2180010142.4 615 −− ×=××== DtL
From Eq. 9,
××==
−6
20
1046.5 erfc108.1)
2(erfc)(
xLx
CxC s
If 320 /cmatoms 108.1)0(,0 ×== Cx ; x = 0.05 ×10-4, C(5× 10-6) = 3.6 × 1019
atoms/cm3; x = 0.075 ×10-4 , C(7.5×10-6) = 9.4 ×1018 atoms/cm3; x = 0.1×10-4,
C(10-5) = 1.8 × 1018 atoms/cm3;
x = 0.15× 10-4, C(1.5×10-5) = 1.8× 1016 atoms/cm3.
The m15.0)(erfc 2 1- µ==s
subj C
CDtx
Total amount of dopant introduced = Q(t)
= 141054.52 ×=LCsπ
atoms/cm2.
2. /scm1096.4132310614.8
46.3exp76.0exp 214
50−
−×=
××−=
−
=kT
EDD a
From Eq. 15, 319atoms/cm10342.2),0( ×===Dt
StCCS
π
××=
=
−5
19
10673.2erfc10342.2
2erfc)(
xLx
CxC S
If x = 0, C(0) = 2.342 × 1019 atoms/cm3; x = 0.1×10-4, C(10-5) = 1.41×1019 atoms/cm3;
x = 0.2×10-4, C(2×10-5) = 6.79×1018 atoms/cm3; x = 0.3×10-4, C(3×10-5) = 2.65×1018
108
atoms/cm3;
x = 0.4×10-4, C(4×10-5) = 9.37×1017 atoms/cm3; x = 0.5×10-4, C(5×10-5) = 1.87×1017
atoms/cm3;
x = 0.6×10-4, C(6×10-5) = 3.51×1016 atoms/cm3; x = 0.7×10-4, C(7×10-5) = 7.03×1015
atoms/cm3;
x = 0.8×10-4, C(8×10-5) = 5.62×1014 atoms/cm3.
The m 72.0ln4 µπ
==DtC
SDtx
B
j .
3.
××
×=× −
−
t13
81815
103.2410
exp101101
t = 1573 s = 26 min
For the constant-total-dopant diffusion case, Eq. 15 gives Dt
SCS
π=
2131318 atoms/cm104.31573103.2101 ×=××××= −πS .
4. The process is called the ramping of a diffusion furnace. For the ramp-down situation, the
furnace temperature T is given by
T = T0 - rt
where T0 is the initial temperature and r is the linear ramp rate. The effective Dt product
during a ramp-down time of t1 is given by
dttDDtt
eff )()(1
0 ∫=
In a typical diffusion process, ramping is carried out until the diffusivity is
negligibly small. Thus the upper limit t1 can be taken as infinity:
...)1(111
000
++≈−
=T
rt
TrtTT
109
and
2
0
02
000
0000 exp)(...))(exp(exp...)1(expexp
kT
trETD
kT
trEkT
ED
Trt
kTE
DkTEDD aaaaa
−≈
−−=
++
−=
−=
where D(T0) is the diffusion coefficient at T0. Substituting the above equation into the
expression for the effective Dt product gives
∫∞
=−
≈
0
2
002
0
0 )(exp)( )(a
aeff rE
kTTDdt
kT
trETDDt
Thus the ramp-down process results in an effective additional time equal to kT02/rEa at
the initial diffusion temperature T0.
For phosphorus diffusion in silicon at 1000°C, we have from Fig. 4:
D(T0) = D (1273 K) = 2× 10-14 cm2/s
sKr /417.06020
7731273=
×
−=
Ea = 3.66 eV
Therefore, the effective diffusion time for the ramp-down process is
min5.191)106.166.3(417.0
)1273(1038.119
2232
0 ≈=××
×=
−
−
srE
kT
a
.
5. For low-concentration drive-in diffusion, the diffusion is given by Gaussian distribution.
The surface concentration is then
==
kTE
tDS
DtS
tC a
2exp),0(
0ππ
tCt
kTE
D
SdtdC a ×−=
−
= 5.0
22exp
2/3
0π
110
or t
dt
C
dC×−= 5.0
which means 1% change in diffusion time will induce 0.5% change in surface
concentration.
220 222
expkT
EC
kT
E
kT
E
tD
SdTdC aaa −=
−
=
π
or T
dT
T
dT
T
dT
kT
E
C
dCa ×−=×
×××
××−=×
−=
−
−
9.1612731038.12
106.16.3
2 23
19
which means 1% change in diffusion temperature will cause 16.9% change in
surface concentration.
6. At 1100°C, ni = 6×1018 cm-3. Therefore, the doping profile for a surface concentration
of 4 × 1018 cm-3 is given by the “intrinsic” diffusion process:
=Dt
xCtxC s
2erfc),(
where Cs = 4× 1018 cm-3, t = 3 hr = 10800 s, and D = 5x10-14 cm2/s. The
diffusion length is then
m232.0cm1032.2 5 µ=×= −Dt
The distribution of arsenic is
××=
−5
18
1064.4erfc104)(
xxC
The junction depth can be obtained as follows
×
×= −5
1815
1064.4erfc10410 jx
xj = 1.2× 10-4 cm = 1.2 µm.
7. At 900°C, ni = 2× 1018 cm-3. For a surface concentration of 4×1018 cm-3, given by
111
the “extrinsic” diffusion process
/scm1077.3102104
8.45 216
18
1811731038.1
106.105.4
0
23
19
−××
××−−
×=×××=×= −
−
enn
eDDi
kT
Ea
nm 3.32cm1023.3108001077.36.16.1 616 =×=××== −−Dtx j .
8. Intrinsic diffusion is for dopant concentration lower than the intrinsic carrier
concentration ni at the diffusion temperature. Extrinsic diffusion is for dopant
concentration higher than ni.
9. For impurity in the oxidation process of silicon,
=t coefficein nsegregatio 2SiO inimpurity of ionconcentrat mequilibriu
silicon inimpurity of ionconcentrat mequilibriu .
10. . 006.0500
3105103
13
11
==××=κ
11. 0.5 = 1.1 + qFB/Ci
7
6
14
1045.310
1085.89.3 −−
−
×=××==d
C sox
ε
212
19
7
cm103.16.0106.11045.3 −
−
−
×=×××=BF
1912
2
5
106.1103.1)16.10(
10 −−
×××=tπ
the implant time t = 6.7 s.
12. The ion dose per unit area is
212
2
19
6
ions/cm 1038.2)
210
(
106.1
6051010
×=×
××××
==−
−
πAqIt
AN
From Eq. 25 and Example 3, the peak ion concentration is at x = Rp. Figure. 17
indicates the σp is 20 nm.
112
Therefore, the ion concentration is
317
7
12
cm1074.421020
1038.2
2−
−×=
××=
ππσ p
S.
13. From Fig. 17, the Rp = 230 nm, and σp = 62 nm.
The peak concentration is
320
7
15
cm1029.121062
102
2−
−×=
××=
ππσp
S
From Eq. 25,
−−×=
2
2
2015
2
)(exp1029.110
p
pj Rx
σ
xj = 0.53 µm.
14. Dose per unit area = 211
198
140 cm106.8
106.11025011085.89.3 −−−
−
×=×××
×××=∆
=q
VC
qQ T
From Fig. 17 and Example 3, the peak concentration occurs at 140 nm from the
surface. Also, it is at (140-25) = 115 nm from the Si-SiO 2 interface.
15. The total implanted dose is integrated from Eq. 25
∫∞
×=−=
−+=
−−=
0 2
2
9989.12
)]3.2(erfc2[2
)2
(erfc1122
)(exp
2
SSRSdx
RxSQ
p
p
p
p
p
Tσσπσ
The total dose in silicon is as follows (d = 25 nm):
8991.12
)]87.1(erfc2[2
)2
(erfc1122
)(exp
2
2
2
∫∞
×=−=
−−+=
−−=
dp
p
p
p
p
Si
SSdRSdx
RxSQ
σσπσ
the ratio of dose in the silicon = QSi/QT = 99.6%.
113
16. The projected range is 150 nm (see Fig. 17).
The average nuclear energy loss over the range is 60 eV/nm (Fig. 16).
60× 0.25 = 15 eV (energy loss of boron ion per each lattice plane)
the damage volume = VD = π (2.5 nm)2(150 nm) = 3× 10-18 cm3
total damage layer = 150/0.25 = 600
displaced atom for one layer = 15/15 = 1
damage density = 600/VD = 2×1020 cm-3
2×1020/5.02×1022 = 0.4%.
17. The higher the temperature, the faster defects anneal out. Also, the solubility of
electrically active dopant atoms increases with temperature.
18. ox
t CQ
V 1V 1 ==∆
where Q1 is the additional charge added just below the oxide-semiconductorsurface by ion implantation. COX is a parallel-plate capacitance per unit area
given by d
C sox
ε=
(d is the oxide thickness, sε is the permittivity of the semiconductor)
cm104.0
F/cm1085.89.31V6
14
1 −
−
××××=∆= oxtCVQ = 8.63
2
7
cmC
10−×
19
7
106.11063.8
−
−
××
= 5.4 ×1012 ions/cm2
Total implant dose = %45104.5 12×
= 1.2 × 1013 ions/cm2.
19. The discussion should mention much of Section 13.6. Diffusion from a surface film
avoids problems of channeling. Tilted beams cannot be used because of
shadowing problems. If low energy implantation is used, perhaps with
preamorphization by silicon, then to keep the junctions shallow, RTA is also
114
necessary.
20. From Eq.35
84.022.0
6.04.0erfc
21 =
−=S
Sd
The effectiveness of the photoresist mask is only 16%.
023.022.0
6.01erfc
21 =
−=S
Sd
The effectiveness of the photoresist mask is 97.7%.
21. 510 2
1 −==u
eT
2-u
π
02.3=∴u
d = Rp + 4.27 pσ = 0.53 + 4.27 × 0.093 = 0.927 µm.
115
CHAPTER 14
1. Each U-shape section (refer to the figure) has an area of 2500 µm × 8 µm = 2 ×
104 µm2. Therefore, there are (2500)2/2 ×104 = 312.5 U-shaped section. Each
section contains 2 long lines with 1248 squares each, 4 corner squares, 1 bottom
square, and 2 half squares at the top. Therefore the resistance for each section is
1 kΩ /¡ (1248×2 + 4×0.65 +2) = 2500.6 kΩ
The maximum resistance is then
312.5×2500.6 = 7.81 × 108 Ω = 781 MΩ
2. The area required on the chip is
25
14
127
cm 1035.41085.89.3
)105)(1030( −−
−−
×=××××==
ox
dC
Aε
= 4.35 × 103 µm2 = 66 × 66 µm
116
Refer to Fig.4a and using negative photoresist of all levels
(a) Ion implantation mask (for p+ implantation and gate oxide)
(b) Contact windows (2×10 µm)
(c) Metallization mask (using Al to form ohmic contact in the contact window
and form the MOS capacitor).
Because of the registration errors, an additional 2 µm is incorporated in all critical
dimensions.
117
3. If the space between lines is 2 µm, then there is 4 µm for each turn (i.e., 2×n, for
one turn). Assume there are n turns, from Eq.6, L ≈ µ0n2r ≈ 1.2 × 10-6n2r, where r
can be replaced by 2 × n. Then, we can obtain that n is 13.
118
4. (a) Metal 1, (b) contact hole, (c) Metal 2.
(a) Metal 1,
(b) contact hole,
(c) Metal 2.
119
5. The circuit diagram and device cross-section of a clamped transistor are shown in
(a) and (b), respectively.
6. (a) The undoped polysilicon is used for isolation.
(b) The polysilicon 1 is used as a solid-phase diffusion source to form the
extrinsic base region and the base electrode.
(c) The polysilicon 2 is used as a solid-phase diffusion source to form the emitter region
and the emitter electrode.
7. (a) For 30 keV boron, Rp = 100 nm and ∆Rp = 34 nm. Assuming that Rp and ∆Rp
for boron are the same in Si and SiO 2 the peak concentration is given by
316
7
11
cm 104.9)1034(2
108
2−
−×=
××=
∆ ππ pR
S
120
The amount of boron ions in the silicon is
( )
211
11
2
2
cm1088.7
3402
750erfc2
2108
2erfc2
2
2exp
2
−
∞
×=
×
−×=
∆
−−=
∆
−−
∆= ∫
p
p
dp
p
p
R
dRS
dxR
Rx
R
SqQ
π
Assume that the implanted boron ions form a negative sheet charge near the Si-
SiO2 interface, then
( ) 91.01025/1085.89.3
)1088.7(106.1/
714
1119
=×××
×××=
=∆−−
−
oxT CqQ
qV V
(b) For 80 keV arsenic implantation, Rp = 49 nm and ∆ Rp = 18 nm. The peak arsenic
concentration is 321
7
16
cm 1021.2)1018(
10
2−
−×=
××=
∆ ππ pR
S.
121
8. (a) Because (100)-oriented silicon has lower (~ one tenth) interface-trapped charge and
a lower fixed oxide charge.
(b) If the field oxide is too thin, it may not provide a large enough threshold
voltage for adequate isolation between neighboring MOSFETs.
(c) The typical sheet resistance of heavily doped polysilicon gate is 20 to
30 Ω /¡, which is adequate for MOSFETs with gate lengths larger than 3 µm. For
shorter gates, the sheet resistance of polysilicon is too high and will cause large
RC delays. We can use refractory metals (e.g., Mo) or silicides as the gate
material to reduce the sheet resistance to about 1 Ω /¡.
122
(d) A self-aligned gate can be obtained by first defining the MOS gate structure, then
using the gate electrode as a mask for the source/drain implantation. The self-
aligned gate can minimize parasitic capacitance caused by the source/drain
regions extending underneath the gate electrode (due to diffusion or
misalignment).
(e) P-glass can be used for insulation between conducting layers, for diffusion and
ion implantation masks, and for passivation to protect devices from impurities,
moisture, and scratches.
9. The lower insulator has a dielectric constant ε1/ε0 = 4 and a thickness d1= 10 nm The
upper insulator has a dielectric constant ε2/ε0 = 10 and a thickness d2 = 100 nm. Upon
application of a positive voltage VG to the external gate, electric field E1 and E2 are
established in the d1 and d2 respectively. We have, from Gauss’ law, that ε1E1 = ε2E2
+Q and VG = E1d1 + E2d2
where Q is the stored charge on the floating gate. From these above two equations, we
obtain
( ) ( )212121211 // dd
QddVG
εεεε ++
+=E
J 5
14
77
1 1026.22.01085.8
10010
104104
10010
101010 ×−=
××
+
+
+
×==
−
−Eσ
(a) If the stored charge does not reduce E1 by a significant amount (i.e., 0.2 >> 2.26×105
Q, we can write
( )∫ −− ×=××=∆≈=
0
861 1051025.02.02.0'
tCtdtQ Eσ
( ) ( ) 565.010100/1085.810
105714
8
2
=×××
×==∆−−
−
CQ
VT V
123
(b) when 0, →∞→ Jt we have ≅×→ 51026.2/2.0Q 8.84×10-7 C.
Then ( ) 98.910/1085.810
1084.8514
7
2
=×××==∆
−−
−
CQ
VT V.
10.
124
11. The oxide capacitance per unit area is given by
7105.32 −×==d
CSiO
ox
εF/cm2
and the maximum current supplied by the device is
( ) ( ) 5105.35.0
521
21 272 ≈−×=−≈ −
TGTGoxDS VVm
mVVC
LW
Iµ
µµ mA
125
and the maximum allowable wire resistance is 0.1 V/5 mA, or 20Ω. Then, the
length of the wire must be
074.0cm107.2
cm10208
28
=−Ω×
×Ω=×≤−
−
ρAreaR
L cm
or 740 µm. This is a long distance compared to most device spacing. When
driving signals between widely spaced logic blocks however, minimum feature
sized lines would not be appropriate.
12.
126
127
13. To solve the short-channel effect of devices.
14. The device performance will be degraded from the boron penetration. There are
methods to reduce this effect: (1) using rapid thermal annealing to reduce the
time at high temperatures, consequently reduces the diffusion of boron, (2) using
nitrided oxide to suppress the boron penetration, since boron can easily combine
with nitrogen and becomes less mobile, (3) making a multi-layer of polysilicon
to trap the boron atoms at the interface of each layer.
15. Total capacitance of the stacked gate structure is :
C =
+×=
+×
1025
5.07
1025
5.07
2
2
1
1
2
2
1
1
ddddεεεε
= 2.12
d9.3
= 2.12
12.29.3=∴d =1.84 nm.
16. Disadvantages of LOCOS: (1) high temperature and long oxidation time cause VT
shift, (2) bird’s beak, (3) not a planar surface, (4) exhibits oxide thinning effect.
Advantages of shallow trench isolation: (1) planar surface, (2) no high
temperature processing and long oxidation time, (3) no oxide thinning effect, (4)
no bird’s beak.
17. For isolation between the metal and the substrate.
18. GaAs lacks of high-quality insulating film.
128
19. (a)
( )
( ) ns. 38.11038.11003.692000
105.01011
1085.89.3105.01
110
914
4
414
8
5
=×=××=
××××××
×××=
=
−−
−
−−
−−
s
dA
AL
RC oxερ
(b) For a polysilicon runner
( )ns 207
s 1007.21003.6910
130 714
4
=
×=×
=
=
−−−
dA
WL
RRC oxsquare ε
Therefore the polysilicon runner’s RC time constant is 150 times larger than the
aluminum runner.
20. When we combine the logic circuits and memory on the chip, we need multiple
supply voltages. For reliability issue, different oxide thicknesses are needed for
different supply voltages.
21. (a) nitrideOTatotal
11152
CCC +=
hence 3.17710
2575
9.3 =+=EOT Å
(b) EOT = 16.7 Å.