L01_5342_Sp11

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Semiconductor Device

Modeling and Characterization

EE5342, Lecture 1-Spring 2011

Professor Ronald L. Carter ronc@uta.edu

http://www.uta.edu/ronc/

Web Pages

* Bring the following to the first class

• R. L. Carter’s web page

– www.uta.edu/ronc/

• EE 5342 web page and syllabus

– http://www.uta.edu/ronc/5342/syllabus.htm

• University and College Ethics Policies www.uta.edu/studentaffairs/conduct/ www.uta.edu/ee/COE%20Ethics%20Statement%20Fall%2007.pdf

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First Assignment

• e-mail to listserv@listserv.uta.edu

– In the body of the message include subscribe EE5342

• This will subscribe you to the EE5342 list. Will receive all EE5342 messages

• If you have any questions, send to ronc@uta.edu, with EE5342 in subject line.

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A Quick Review of Physics

• Review of

– Semiconductor Quantum Physics

– Semiconductor carrier statistics

– Semiconductor carrier dynamics

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Bohr model H atom

• Electron (-q) rev. around proton (+q)

• Coulomb force, F=q 2 /4 pe o r 2 , q=1.6E-19 Coul, e o

=8.854E-14 Fd/cm

• Quantization L = mvr = nh/2 p

• E n

• r n

= -(mq 4 )/[8 e

= [n 2 e o

©rlc L01 19Jan2011 h]/[ p o

2 mq h 2 n 2 ] ~ -13.6 eV/n 2

2 ] ~ 0.05 nm = 1/2 A for n=1, ground state o

5

Quantum Concepts

• Bohr Atom

• Light Quanta (particle-like waves)

• Wave-like properties of particles

• Wave-Particle Duality

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Energy Quanta for Light

T max

1 mv 2

 h  f

• Photoelectric Effect:

 f o

  qV stop

• T max is the energy of the electron emitted from a material surface when light of frequency f is incident.

• f o

, frequency for zero KE, mat’l spec.

• h is Planck’s (a universal) constant

©rlc L01 19Jan2011 h = 6.625E-34 J-sec

7

Photon: A particle

-like wave

• E = hf, the quantum of energy for light. (PE effect & black body rad.)

• f = c/ l , c = 3E8m/sec, l = wavelength

• From Poynting’s theorem (em waves), momentum density = energy density/c

• Postulate a Photon “momentum” p = h/ l = hk, h = h/2 p wavenumber, k = 2 p / l

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Wave-particle

Duality

• Compton showed D p = hk initial

- hk final

, so an photon (wave) is particle-like

• DeBroglie hypothesized a particle could be wave-like, l = h/p

• Davisson and Germer demonstrated wave-like interference phenomena for electrons to complete the duality model

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Newtonian Mechanics

• Kinetic energy, KE = mv 2 /2 = p 2 /2m

Conservation of Energy Theorem

• Momentum, p = mv

Conservation of Momentum Thm

• Newton’s second Law

F = ma = m dv/dt = m d 2 x/dt 2

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Quantum Mechanics

• Schrodinger’s wave equation developed to maintain consistence with wave-particle duality and other

“quantum” effects

• Position, mass, etc. of a particle replaced by a “wave function”, Y (x,t)

• Prob. density = | Y (x,t)• Y * (x,t)|

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Schrodinger Equation

• Separation of variables gives

Y (x,t) = y (x)• f (t)

• The time-independent part of the

Schrodinger equation for a single particle with KE = E and PE = V.

 x

 

2 x

8 p h

2

2

 ( )  y    0

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Solutions for the

Schrodinger Equation

• Solutions of the form of y (x) = A exp(jKx) + B exp (-jKx)

K = [8 p 2 m(E-V)/h 2 ] 1/2

• Subj. to boundary conds. and norm.

y (x) is finite, single-valued, conts.

d y (x)/dx is finite, s-v, and conts.

 y *     dx  1

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Infinite Potential Well

• V = 0, 0 < x < a

• V --> inf. for x < 0 and x > a

• Assume E is finite, so y (x) = 0 outside of well y   

2 a sin

 n p a x

, n =

E n

 h 2 n

8 ma

2

2

 h

4

2 p k

2

2

, p  h l

1,2,3,...

 hk

2 p

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Step Potential

• V = 0, x < 0 (region 1)

• V = V o

, x > 0 (region 2)

• Region 1 has free particle solutions

• Region 2 has free particle soln. for E > V o

, and evanescent solutions for E < V o

• A reflection coefficient can be def.

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Finite Potential Barrier

• Region 1: x < 0, V = 0

• Region 1: 0 < x < a, V = V o

• Region 3: x > a, V = 0

• Regions 1 and 3 are free particle solutions

• Region 2 is evanescent for E < V o

• Reflection and Transmission coeffs.

For all E

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Kronig-Penney Model

A simple one-dimensional model of a crystalline solid

• V = 0, 0 < x < a, the ionic region

• V = V o

, a < x < (a + b) = L, between ions

• V(x+nL) = V(x), n = 0, +1, +2, +3, …, representing the symmetry of the assemblage of ions and requiring that y (x+L) = y (x) exp(jkL), Bloch’s Thm

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K-P Potential Function*

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K-P Static

Wavefunctions

• Inside the ions, 0 < x < a y (x) = A exp(j b x) + B exp (-j b x) b = [8 p 2 mE/h] 1/2

• Between ions region, a < x < (a + b) = L y (x) = C exp( a x) + D exp (a x) a = [8 p 2 m(V o

-E)/h 2 ] 1/2

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K-P Impulse Solution

• Limiting case of V o

-> inf. and b -> 0, while a 2 b = 2P/a is finite

• In this way a 2 b 2 = 2Pb/a < 1, giving sinh( a b) ~ a b and cosh( a b) ~ 1

• The solution is expressed by

P sin( b a)/( b a) + cos( b a) = cos(ka)

• Allowed values of LHS bounded by +1

• k = free electron wave # = 2 p / l

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K-P Solutions*

x x

P sin( b a)/( b a) + cos( b a) vs. b a

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K-P E(k)

Relationship*

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References

*Fundamentals of Semiconductor

Theory and Device Physics, by Shyh

Wang, Prentice Hall, 1989.

**Semiconductor Physics & Devices, by Donald A. Neamen, 2nd ed., Irwin,

Chicago.

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