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Transcript of Semiconductors
Lecture 1, Slide # 1 ECE 217 © P.J. Burke, Spring 2002 Last modified 04/08/23 00:31
ECE217B, Spring 2002Advanced Semiconductor Devices II
Graduate Course, 3 units
Professor & Class SchedulePeter Burke
e-mail: [email protected]: EG 2232
Lect. Mo/We 3:00 – 4:20 pm in CS 219Office hours 4:30-5:30 pm
Lecture notes, HWs and solutions online athttp://nano.ece.uci.edu/ece_217b_advanced_semiconductor_devices.htm
and at copy center (ET base) by day of lectureTextbook:
Fundamentals of III-V Devices: HBTs, MESFETs, and HFETs/HEMTsWilliam Liu, Wiley (1999), ISBN 0-471-29700-3
Grade:60% Homework, 40% End-of-term presentation/paper
Lecture 1, Slide # 2 ECE 217 © P.J. Burke, Spring 2002 Last modified 04/08/23 00:31
Reference books:* means on reserve at the science libraryDevice physics:*Physics of Semiconductor Devices, S.M. Sze, Wiley (1981) ISBN 0-471-05661-8*Modern Semiconductor Device Physics, S.M. Sze, Wiley (1998) ISBN 0-471-15237-4*High Speed Semiconductor Devices, S.M. Sze, Wiley (1990) ISBN 0-471-62307-5*Physics of Semiconductor Devices, Michael Shur, Prentice Hall PTR (1996) ISBN 0-13-666496-2*Solid State Electronic Devices, 5th Edition, Ben G. Streetman (2000), ISBN 0-13-025706-0GaAs High-Speed Devices, C.Y. Chang and Francis Kai, Wiley (1994) ISBN 0-471-85641-X*InP-Based Materials and Devices: Physics and Technology, Osamu Wada and Hideki Hasegawa, Wiley (1994) ISBN 0-471-18191-9SiGe, GaAs, and InP Heterojunction Bipolar Transistors, Jiann S. Yuan, Wiley (1999), ISBN 0-471-19746-7*Semiconductor Device Fundamentals, Robert F. Pierret, Addison-Wesley (1995), ISBN 020154393-1*HEMTs and HBTs: Devices, Fabrication, and Circuits, Fazai Ali and Aditya Gupta, Artech House (1991), ISBN 0-89006-401-6InP HBTs: Growth, Processing, and Applications, B. Jalali and S.J. Pearton, Artech House (1994), ISBN 0-89006-724-4*Semiconductor Physics and Devices: Basic Principles, Donald A Neamen, McGraw-Hill (1997) ISBN 0-256-24214-3*Low Dimensional Semiconductor Structures: Fundamentals and Device Applications, Keith Barnham and Dimitri Vvedensky, Cambridge University Press (2001), ISBN 0-521-59103-1.Modern GaAs Processing Methods, Ralph E. Williams, Artech (1990), ISBN 0-89006-343-5, out of printElectrical and Thermal Characterization of MESFETs, HEMTs and HBTs, Robert R H Anholt, Artech House (1994), ISBN 0-89006-749-X*Fundamentals of Semiconductor Theory and Device Physics, Shyh Wang, Prentice Hall (1989), ISBN 0-13-344409-0 (out of print)*Device Electronics for Integrated Circuits, 2nd Edition, Richard S Muller and Theodore I Kamins, Wiley (1986), ISBN 0-471-88758-7, *Compound Semiconductor Device Physics, Sandip Tiwari, Academic Press (1991), ISBN 0-12-691740-X (out of print)High-frequency (microwave, mm-wave) engineering:*Microwave Engineering, 2nd Edition, David Pozar, Wiley (1997), ISBN 0-471-17096-8Microwave and RF Wireless Systems, David Pozar, Wiley (2000), ISBN 0-471-32282-2*Foundations for Microstrip Circuit Design, 2nd Edition, T.C. Edwards, Wiley (1991), ISBN 0-471-93062-8. (out of print)*Fields and Waves in Communications Electronics, 3rd Edition, Simon Ramo, John R. Whinnery, Theodore Van Duzer, Wiley (1994) ISBN 0-471-58551-3 (out of print)*Microstrip Lines and Slotlines, 2nd Edition, K.C. Gupta, Ramesh Garg, Inder Bahl, Prakash Bhartia, Artech House (1996), ISBN 0-89006-766-X*Transmission Line Design Handbook, Brian C. Wadell, Artech House (1991), ISBN 0-89006-436-9*Microwave Transistor Amplifiers: Analysis and Design, 2nd Edition, Guillermo Gonzalez, Prentice Hall (1997), ISBN 0-13-254335-4
Lecture 1, Slide # 3 ECE 217 © P.J. Burke, Spring 2002 Last modified 04/08/23 00:31
ECE217B Advanced Semiconductor Devices II (3) S. Metal-semiconductor field-effect transistors (MESFET), heterojunction bipolar transistors (HBT), microwave semiconductor devices, equivalent circuits, device modeling and fabrication, microwave amplifiers, transmitters, and receivers. Prerequisite: ECE114A.
HW will be hard if you do not meet the prerequisite.
Lecture 1, Slide # 4 ECE 217 © P.J. Burke, Spring 2002 Last modified 04/08/23 00:31
Course Outline1. Review of basic semiconductor physics and III-Vs
2. Two-terminal devices
3. HBT DC properties
4. HBT high frequency properties
5. FET DC properties
6. FET high frequency properties
7. Noise models
8. Quantum devices: resonant tunneling diodes
9. Nano-scale devices: Landauer-Buttiker formalism, single electron transistors, quantum point contacts, quantum dots, carbon nanotubes
Lecture 1, Slide # 5 ECE 217 © P.J. Burke, Spring 2002 Last modified 04/08/23 00:31
Also
As needed by the class:
1. Electromagnetic wave propagation in infinite media
2. Coaxial and microstrip transmission lines
3. S-parameters, reflections, impedances, gains, and Smith chart
Lecture 1, Slide # 6 ECE 217 © P.J. Burke, Spring 2002 Last modified 04/08/23 00:31
III-V vs. Silicon
• Silicon is inexpensive and mature
• Why bother with III-V?– Speed– Power– Noise– Optically active
• These are niche markets, but it’s a big niche
Lecture 1, Slide # 7 ECE 217 © P.J. Burke, Spring 2002 Last modified 04/08/23 00:31
Speed
From Sze, Physics of Semiconductor Devices
Lecture 1, Slide # 8 ECE 217 © P.J. Burke, Spring 2002 Last modified 04/08/23 00:31
Speed
From Sze, Physics of Semiconductor Devices
Lecture 1, Slide # 9 ECE 217 © P.J. Burke, Spring 2002 Last modified 04/08/23 00:31
High speed HEMTs:
fT = vmax /(2 L )
Si 0.18 m CMOS @ 30 GHz
InP based @ 362 GHz (fastest)
Endoh et al, 12th Intl. Conf. on InP, 2000 (Fujitsu)
(draw in Si, SiGe)
Lecture 1, Slide # 10 ECE 217 © P.J. Burke, Spring 2002 Last modified 04/08/23 00:31
Noise
From Sze, Physics of Semiconductor Devices
Lecture 1, Slide # 11 ECE 217 © P.J. Burke, Spring 2002 Last modified 04/08/23 00:31
Optics
(Adapted from Streetman, Solid State Electronic Devices)
0.01
0.1
1
10
100A
tten
uatio
n (d
B/k
m)
1.81.61.41.21.00.8
Wavelength (m)
RayleighScattering
Infraredaborption
Lecture 1, Slide # 12 ECE 217 © P.J. Burke, Spring 2002 Last modified 04/08/23 00:31
Band gap engineering
• Controlled growth of any structure you can imagine in the z-direction
• Important to LATTICE MATCH
• Dislocations/misfits INCREASE the non-radiative recombination rate, causing higher laser threshold currents
• GaAs, InP typical substrates
• MBE, MOCVD, LPE
Lecture 1, Slide # 13 ECE 217 © P.J. Burke, Spring 2002 Last modified 04/08/23 00:31
MBE
epitaxial growth
GaAs
AlAs
AlAs
1.4 eV2.2 eV
V
z
Also InP, InGaAs, InAlAs, InGaAsP …
Lecture 1, Slide # 14 ECE 217 © P.J. Burke, Spring 2002 Last modified 04/08/23 00:31
MBE
4 atom per layer!
(From Streetman, Solid State Electronic Devices)
Lecture 1, Slide # 15 ECE 217 © P.J. Burke, Spring 2002 Last modified 04/08/23 00:31
Band gaps
Lecture 1, Slide # 16 ECE 217 © P.J. Burke, Spring 2002 Last modified 04/08/23 00:31
Outline• Quantum mechanics• Free electrons in a box (Fermi gas)• Band theory of solids• Fermi/Dirac distribution function• Doping• Electrical conduction in semiconductors
– Drift– Diffusion
• Haynes/Schockley experiment• All bulk this week (discuss)
Lecture 1, Slide # 17 ECE 217 © P.J. Burke, Spring 2002 Last modified 04/08/23 00:31
Free electron theory of solids• Each atom in the solid “gives up” one electron
• Each electron is free to move where-ever it wants, with no scattering
• Amazingly, this simple idea makes predictions that are true!
• Not for semiconductors, but metals
• Still need to understand this for semiconductors
Lecture 1, Slide # 18 ECE 217 © P.J. Burke, Spring 2002 Last modified 04/08/23 00:31
Electrons are waves, too.
Lecture 1, Slide # 19 ECE 217 © P.J. Burke, Spring 2002 Last modified 04/08/23 00:31
Quantum mechanics of free particles:
2),( tr
is probability of finding an electron at point r at time t.
is complex, and both real and imaginary parts are physical.
Lecture 1, Slide # 20 ECE 217 © P.J. Burke, Spring 2002 Last modified 04/08/23 00:31
Quantum mechanics of free particles:
2),( tr
is probability of finding an electron at point r at time t.
)(~),( trkietr
For a free particle:
kp
m
k
m
pE
2
)(
2
22
Momentum: Energy:
/E is complex, and both real and imaginary parts are physical.
Lecture 1, Slide # 21 ECE 217 © P.J. Burke, Spring 2002 Last modified 04/08/23 00:31
Schrodinger equation:
),(2
),(2
22
txxm
txt
i
(Time dependent)
(1 dimension)
Lecture 1, Slide # 22 ECE 217 © P.J. Burke, Spring 2002 Last modified 04/08/23 00:31
Schrodinger equation:
),(2
),(2
22
txxm
txt
i
)(),( tkxieAtx Let
(Time dependent)
A is a (complex) constant.
(1 dimension)
Lecture 1, Slide # 23 ECE 217 © P.J. Burke, Spring 2002 Last modified 04/08/23 00:31
Schrodinger equation:
),(2
),(2
22
txxm
txt
i
)(),( tkxieAtx Then
Let
)()( )(),( tkxitkxi eAiieAt
itrt
i
(Time dependent)
A is a (complex) constant.
(1 dimension)
Lecture 1, Slide # 24 ECE 217 © P.J. Burke, Spring 2002 Last modified 04/08/23 00:31
Schrodinger equation:
),(2
),(2
22
txxm
txt
i
)(),( tkxieAtx
),()( txEeAE tkxi
Then
Let
)()( )(),( tkxitkxi eAiieAt
itrt
i
(Time dependent)
A is a (complex) constant.
(1 dimension)
Lecture 1, Slide # 25 ECE 217 © P.J. Burke, Spring 2002 Last modified 04/08/23 00:31
Schrodinger equation:
),(2
),(2
22
txxm
txt
i
)(),( tkxieAtx
),()( txEeAE tkxi
Then
Let
)(22
)(2
22
2
22
22),(
2tkxitkxi eAik
meA
xmtx
xm
)()( )(),( tkxitkxi eAiieAt
itrt
i
(Time dependent)
A is a (complex) constant.
(1 dimension)
Lecture 1, Slide # 26 ECE 217 © P.J. Burke, Spring 2002 Last modified 04/08/23 00:31
Schrodinger equation:
),(2
),(2
22
txxm
txt
i
)(),( tkxieAtx
),()( txEeAE tkxi
Then
Let
)(22
)(2
22
2
22
22),(
2tkxitkxi eAik
meA
xmtx
xm
)()( )(),( tkxitkxi eAiieAt
itrt
i
),(22
2)(
22
txm
peA
m
k tkxi
(Time dependent)
A is a (complex) constant.
(1 dimension)
Lecture 1, Slide # 27 ECE 217 © P.J. Burke, Spring 2002 Last modified 04/08/23 00:31
Schrodinger equation:
),(2
),(2
),(2
2
2
2
2
222
2
trzyxm
trm
trt
i
(3 dimensions)
Lecture 1, Slide # 28 ECE 217 © P.J. Burke, Spring 2002 Last modified 04/08/23 00:31
Schrodinger equation:
),(2
),(2
),(2
2
2
2
2
222
2
trzyxm
trm
trt
i
tzkykxkitrki zyxeAeAtr )()(),(Let
(3 dimensions)
Lecture 1, Slide # 29 ECE 217 © P.J. Burke, Spring 2002 Last modified 04/08/23 00:31
Schrodinger equation:
),(2
),(2
),(2
2
2
2
2
222
2
trzyxm
trm
trt
i
tzkykxkitrki zyxeAeAtr )()(),(
Then
Let
),(),()(),( trEtriitrt
i
(3 dimensions)
as before.
Lecture 1, Slide # 30 ECE 217 © P.J. Burke, Spring 2002 Last modified 04/08/23 00:31
Schrodinger equation:
),(2
),(2
),(2
2
2
2
2
222
2
trzyxm
trm
trt
i
tzkykxkitrki zyxeAeAtr )()(),(
Then
Let
)(2
2
2
2
2
22
2
2
2
2
2
22
2),(
2trkieA
zyxmtr
zyxm
),(),()(),( trEtriitrt
i
(3 dimensions)
as before.
But:
Lecture 1, Slide # 31 ECE 217 © P.J. Burke, Spring 2002 Last modified 04/08/23 00:31
Schrodinger equation:
),(2
),(2
),(2
2
2
2
2
222
2
trzyxm
trm
trt
i
tzkykxkitrki zyxeAeAtr )()(),(
Then
Let
)(2
2
2
2
2
22
2
2
2
2
2
22
2),(
2trkieA
zyxmtr
zyxm
),(),()(),( trEtriitrt
i
(3 dimensions)
as before.
But:
),(2
)(
2
2222)(222
2
trm
kkkeAikikik
mzyxtrki
zyx
Lecture 1, Slide # 32 ECE 217 © P.J. Burke, Spring 2002 Last modified 04/08/23 00:31
Schrodinger equation:
),(2
),(2
),(2
2
2
2
2
222
2
trzyxm
trm
trt
i
tzkykxkitrki zyxeAeAtr )()(),(
Then
Let
)(2
2
2
2
2
22
2
2
2
2
2
22
2),(
2trkieA
zyxmtr
zyxm
),(),()(),( trEtriitrt
i
),(22
2)(
22
trm
peA
m
k trki
(3 dimensions)
as before.
But:
),(2
)(
2
2222)(222
2
trm
kkkeAikikik
mzyxtrki
zyx
Lecture 1, Slide # 33 ECE 217 © P.J. Burke, Spring 2002 Last modified 04/08/23 00:31
Quantum mechanics of free particles:
)(~),( trkietr
)()( )(),( tkxi
n
txkin ekAdkeAtr nn
Generally,
is also a possibility.
Lecture 1, Slide # 34 ECE 217 © P.J. Burke, Spring 2002 Last modified 04/08/23 00:31
Time-independent Schrodinger equation
)(),( trkieAtr
Lecture 1, Slide # 35 ECE 217 © P.J. Burke, Spring 2002 Last modified 04/08/23 00:31
Time-independent Schrodinger equation
)(),( trkieAtr
tizkykxkitzkykxki eeAeA zyxzyx )()(
Lecture 1, Slide # 36 ECE 217 © P.J. Burke, Spring 2002 Last modified 04/08/23 00:31
Time-independent Schrodinger equation
)(),( trkieAtr
tizkykxkitzkykxki eeAeA zyxzyx )()(
)(rCall this
Lecture 1, Slide # 37 ECE 217 © P.J. Burke, Spring 2002 Last modified 04/08/23 00:31
Time-independent Schrodinger equation
)(),( trkieAtr
tizkykxkitzkykxki eeAeA zyxzyx )()(
)(rCall this
tiertr )(),(
Lecture 1, Slide # 38 ECE 217 © P.J. Burke, Spring 2002 Last modified 04/08/23 00:31
Time-independent Schrodinger equation
)(),( trkieAtr
tizkykxkitzkykxki eeAeA zyxzyx )()(
)(rCall this
tiertr )(),(
),(2
),( 22
trm
trt
i
From:
Lecture 1, Slide # 39 ECE 217 © P.J. Burke, Spring 2002 Last modified 04/08/23 00:31
Time-independent Schrodinger equation
)(),( trkieAtr
tizkykxkitzkykxki eeAeA zyxzyx )()(
)(rCall this
tiertr )(),(
),(2
),( 22
trm
trt
i
titititi erm
trm
erEeriiert
itrt
i
)(2
),(2
)()()(),( 22
22
From:
Lecture 1, Slide # 40 ECE 217 © P.J. Burke, Spring 2002 Last modified 04/08/23 00:31
Time-independent Schrodinger equation
)(),( trkieAtr
tizkykxkitzkykxki eeAeA zyxzyx )()(
)(rCall this
tiertr )(),(
),(2
),( 22
trm
trt
i
titititi erm
trm
erEeriiert
itrt
i
)(2
),(2
)()()(),( 22
22
From:
)()(2
22
rErm
Lecture 1, Slide # 41 ECE 217 © P.J. Burke, Spring 2002 Last modified 04/08/23 00:31
Confined particles: A box
L
L
L
Goal: find )(r
Similar to electric field inside the box.
Lecture 1, Slide # 42 ECE 217 © P.J. Burke, Spring 2002 Last modified 04/08/23 00:31
L
L
L
z
y
x
Goal: find )(r
0)(2 r
Everywhere outside the box
In particular,
0)(2 r
on the boundaries.
As before, we will consider all six surfaces:
Lecture 1, Slide # 43 ECE 217 © P.J. Burke, Spring 2002 Last modified 04/08/23 00:31
Boundary conditions:
L
L
L
)()( zkykxki zyxeAr
z
y
x
The plane x=0:
Try:
Lecture 1, Slide # 44 ECE 217 © P.J. Burke, Spring 2002 Last modified 04/08/23 00:31
Boundary conditions:
L
L
L
)()( zkykxki zyxeAr
z
y
x
The plane x=0:
Does not solve boundary condition!!!
)()(),,0( zkykizkykxki zyzyx eAeAzyx 0
Try:
Lecture 1, Slide # 45 ECE 217 © P.J. Burke, Spring 2002 Last modified 04/08/23 00:31
Boundary conditions:
L
L
L
)()( zkykxki zyxeAr
z
y
x
The plane x=0:
)( zkykxki zyxeA
Let’s try something:
Lecture 1, Slide # 46 ECE 217 © P.J. Burke, Spring 2002 Last modified 04/08/23 00:31
Boundary conditions:
L
L
L
)()( zkykxki zyxeAr
z
y
x
The plane x=0:
)( zkykxki zyxeA )()( zkykixikxik zyxx eeeAr
baba eee
Let’s try something:
Lecture 1, Slide # 47 ECE 217 © P.J. Burke, Spring 2002 Last modified 04/08/23 00:31
Boundary conditions:
L
L
L
)()( zkykxki zyxeAr
z
y
x
The plane x=0:
)( zkykxki zyxeA )()( zkykixikxik zyxx eeeAr
)(),,0( zkykixikxik zyxx eeeAzyx 0 0
baba eee
Let’s try something:
Lecture 1, Slide # 48 ECE 217 © P.J. Burke, Spring 2002 Last modified 04/08/23 00:31
Boundary conditions:
L
L
L
)()( zkykxki zyxeAr
z
y
x
The plane x=0:
)( zkykxki zyxeA )()( zkykixikxik zyxx eeeAr
)(),,0( zkykixikxik zyxx eeeAzyx 0 0
baba eee
0)(00 zkyki zyeeeA
Let’s try something:
Lecture 1, Slide # 49 ECE 217 © P.J. Burke, Spring 2002 Last modified 04/08/23 00:31
Boundary conditions:
L
L
L
)()( zkykxki zyxeAr
z
y
x
The plane x=0:
Does solve boundary condition!!!
)( zkykxki zyxeA )()( zkykixikxik zyxx eeeAr
)(),,0( zkykixikxik zyxx eeeAzyx 0 0
baba eee
0)(00 zkyki zyeeeA
Let’s try something:
Lecture 1, Slide # 50 ECE 217 © P.J. Burke, Spring 2002 Last modified 04/08/23 00:31
Boundary conditions:
L
L
L
z
y
x
The plane x=L:
)()( zkykixikxik zyxx eeeAr
)()sin(2 zkykix
zyexkiA
?0)sin(2),,( )( zkykix
zyeLkiAzyLx
ii eei
2
1)sin(
Lnkn /
If and only if:
Lecture 1, Slide # 51 ECE 217 © P.J. Burke, Spring 2002 Last modified 04/08/23 00:31
Boundary conditions:
L
L
L
z
y
x
The plane x=L:
)()( zkykixikxik zyxx eeeAr
Lecture 1, Slide # 52 ECE 217 © P.J. Burke, Spring 2002 Last modified 04/08/23 00:31
Boundary conditions:
L
L
L
z
y
x
The plane x=L:
)()( zkykixikxik zyxx eeeAr
)()sin(2 zkykix
zyexkiA
ii eei
2
1)sin(
Lecture 1, Slide # 53 ECE 217 © P.J. Burke, Spring 2002 Last modified 04/08/23 00:31
Boundary conditions:
L
L
L
z
y
x
The plane x=L:
)()( zkykixikxik zyxx eeeAr
)()sin(2 zkykix
zyexkiA
?0)sin(2),,( )( zkykix
zyeLkiAzyLx
ii eei
2
1)sin(
Lecture 1, Slide # 54 ECE 217 © P.J. Burke, Spring 2002 Last modified 04/08/23 00:31
Boundary conditions:
L
L
L
z
y
x
The plane x=L:
)()( zkykixikxik zyxx eeeAr
)()sin(2 zkykix
zyexkiA
?0)sin(2),,( )( zkykix
zyeLkiAzyLx
ii eei
2
1)sin(
Lnkn /
If and only if:
Lecture 1, Slide # 55 ECE 217 © P.J. Burke, Spring 2002 Last modified 04/08/23 00:31
Boundary conditions:
L
L
L
z
y
x
)sin()sin()sin()2()( 3 zkykxkAirzynx nn
Lnk xnx/
We can do the same for y, z:
Lnk yny/Lnk znz
/
Lecture 1, Slide # 56 ECE 217 © P.J. Burke, Spring 2002 Last modified 04/08/23 00:31
Boundary conditions:
L
L
L
z
y
x
)sin()sin()sin()2()( 3 zkykxkAirzynx nn
Lnk xnx/
We can do the same for y, z:
)(2
)/(
2
)( 222222222
zyx
nnnnnn
m
L
m
kkkE zyx
These are the allowed energy levels, or “quantum states”
Lnk yny/Lnk znz
/
Lecture 1, Slide # 57 ECE 217 © P.J. Burke, Spring 2002 Last modified 04/08/23 00:31
Many electrons:
L
L
L
z
y
x
)(2
)/( 22222
zyx nnnm
LE
These are the allowed energy levels, or “quantum states”
Pauli exclusion principle: Each unique combination of nx, ny, nz canonly have two electrons (spin up, spin down).
Lecture 1, Slide # 58 ECE 217 © P.J. Burke, Spring 2002 Last modified 04/08/23 00:31
Energy spectrum of free particles:
nx=1, ny=1, nz=1
energy
nx=2, ny=1, nz=1 nx=1, ny=2, nz=1 nx=1, ny=1, nz=2
Etc.
Lecture 1, Slide # 59 ECE 217 © P.J. Burke, Spring 2002 Last modified 04/08/23 00:31
Density of states:
energy
?dENENumber of states with energy between E and E + dE
E
E+dE
How many states?
If L is large, states are very close together.Approximate as a continuum.
?)( dEENumber of states with energy between E and E + dE per volume.
Lecture 1, Slide # 60 ECE 217 © P.J. Burke, Spring 2002 Last modified 04/08/23 00:31
Density of states:Easier first to think of in k-space:
Density of states in k-space is uniform:
One state per (/L)3:
kx
ky
kz
Lecture 1, Slide # 61 ECE 217 © P.J. Burke, Spring 2002 Last modified 04/08/23 00:31
Density of states:Easier first to think of in k-space:
Density of states in k-space is uniform:
One state per (/L)3:
From Verdeyen
Lecture 1, Slide # 62 ECE 217 © P.J. Burke, Spring 2002 Last modified 04/08/23 00:31
Density of states:
kx
ky
kz
?dkNk
Number of states between k, k+dk:
222zyx kkkk
Lnk xnx/
Lnk yny/Lnk znz
/
From Verdeyen
Lecture 1, Slide # 63 ECE 217 © P.J. Burke, Spring 2002 Last modified 04/08/23 00:31
?dkNkVolume of spherical shell=4k2dk/88 is for upper right quadrant
Number of states in volume=Volume x States/volume
States/volume = 1 / (/L)3:
2
23
32 2
)/(
18/4
dkk
LL
dkkdkNk
2
2
volume dkkdkN
dk kk
HW you will do calculation for 2 dimensional world.
Lecture 1, Slide # 64 ECE 217 © P.J. Burke, Spring 2002 Last modified 04/08/23 00:31
?)( dEE
Lecture 1, Slide # 65 ECE 217 © P.J. Burke, Spring 2002 Last modified 04/08/23 00:31
?)( dEE
dEEdkk )( We use:
Lecture 1, Slide # 66 ECE 217 © P.J. Burke, Spring 2002 Last modified 04/08/23 00:31
?)( dEE
2
2
dkk
dkk
dEEdkk )( We use:
Lecture 1, Slide # 67 ECE 217 © P.J. Burke, Spring 2002 Last modified 04/08/23 00:31
?)( dEE
2
2
dkk
dkk
E
dEmdk
mEk
m
kE
2
22
2 22
22
dEEdkk )( We use:
Lecture 1, Slide # 68 ECE 217 © P.J. Burke, Spring 2002 Last modified 04/08/23 00:31
?)( dEE
2
2
dkk
dkk
E
dEmdk
mEk
m
kE
2
22
2 22
22
dEEdkk )( We use:
Lecture 1, Slide # 69 ECE 217 © P.J. Burke, Spring 2002 Last modified 04/08/23 00:31
?)( dEE
2
2
dkk
dkk
E
dEmdk
mEk
m
kE
2
22
2 22
22
dEEdkk )( We use:
dEEm
dEE 2/12/32
2/32/32)(
Lecture 1, Slide # 70 ECE 217 © P.J. Burke, Spring 2002 Last modified 04/08/23 00:31
Fermi gas:
energy
At zero temperature, as we add electrons to thebox, we gradually fill up all the states.(DISCUSS PAULI EXCLUSION PRINCIPLE-IMPORTANT!)
When we are done filling the box, the energyof the last electron is called the “Fermi energy.”
“Gas” means we neglect electron-electron interactions.
All these states are filled with electrons.
E=0
E=EFermi
energy
P(E
)
Lecture 1, Slide # 71 ECE 217 © P.J. Burke, Spring 2002 Last modified 04/08/23 00:31
Fermi energy:
energy
All these states are filled with electrons.
E=0
E=EFermi
ff EE
dEEm
LN0
2/12/32
2/32/13
0 E
2dEelectrons #
Lecture 1, Slide # 72 ECE 217 © P.J. Burke, Spring 2002 Last modified 04/08/23 00:31
Fermi energy:
energy
All these states are filled with electrons.
E=0
E=EFermi
ff EE
dEEm
LN0
2/12/32
2/32/13
0 E
2dEelectrons #
2/32/32
2/32/13
3
22electrons # fE
mL
Lecture 1, Slide # 73 ECE 217 © P.J. Burke, Spring 2002 Last modified 04/08/23 00:31
Fermi energy:
energy
All these states are filled with electrons.
E=0
E=EFermi
ff EE
dEEm
LN0
2/12/32
2/32/13
0 E
2dEelectrons #
2/32/32
2/32/13
3
22electrons # fE
mL
3/2
3
3/43/22 electrons #
2
3
LmE f
Lecture 1, Slide # 74 ECE 217 © P.J. Burke, Spring 2002 Last modified 04/08/23 00:31
Fermi energy:
energy
All these states are filled with electrons.
E=0
E=EFermi
ff EE
dEEm
LN0
2/12/32
2/32/13
0 E
2dEelectrons #
2/32/32
2/32/13
3
22electrons # fE
mL
3/2
3
3/43/22 electrons #
2
3
LmE f
In a typical metal, L ~ 0.1 nm.Ef ~ 10 eV
Lecture 1, Slide # 75 ECE 217 © P.J. Burke, Spring 2002 Last modified 04/08/23 00:31
Occupation probability:
E=EFermi
energy
P(E
)
P(E) = probability of occupying a state with energy E
What about finite temperature?
1
0
Lecture 1, Slide # 76 ECE 217 © P.J. Burke, Spring 2002 Last modified 04/08/23 00:31
Recall Boltzmann factor P():
“The probability for a physical system to be in a state with energy is proportional to .”
Boltzmann:
TkBe /
This is actually not quite true. It is classical.A quantum calculation shows for electrons:
1
1)( /)( kTEE fe
EP
Called Fermi-Dirac distribution function.Boltzman is high-energy limit (discuss!)
Lecture 1, Slide # 77 ECE 217 © P.J. Burke, Spring 2002 Last modified 04/08/23 00:31
Fermi-Dirac:
E=EFermi
energy
P(E
)
1
1)( /)( kTEE fe
EP
kTP=1/2 at Ef for all temperatures.
1
0