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Semiconductor Device Modeling and Characterization EE5342, Lecture 1-Spring 2011 Professor Ronald L. Carter

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Presentation on theme: "Semiconductor Device Modeling and Characterization EE5342, Lecture 1-Spring 2011 Professor Ronald L. Carter"— Presentation transcript:

1 Semiconductor Device Modeling and Characterization EE5342, Lecture 1-Spring 2011 Professor Ronald L. Carter ronc@uta.edu http://www.uta.edu/ronc/

2 ©rlc L01 19Jan20112 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

3 ©rlc L01 19Jan20113 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.

4 ©rlc L01 19Jan20114 A Quick Review of Physics Review of –Semiconductor Quantum Physics –Semiconductor carrier statistics –Semiconductor carrier dynamics

5 ©rlc L01 19Jan20115 Bohr model H atom Electron (-q) rev. around proton (+q) Coulomb force, F=q 2 /4  o r 2, q=1.6E-19 Coul,  o =8.854E-14 Fd/cm Quantization L = mvr = nh/2  E n = -(mq 4 )/[8  o 2 h 2 n 2 ] ~ -13.6 eV/n 2 r n = [n 2  o h]/[  mq 2 ] ~ 0.05 nm = 1/2 A o for n=1, ground state

6 ©rlc L01 19Jan20116 Quantum Concepts Bohr Atom Light Quanta (particle-like waves) Wave-like properties of particles Wave-Particle Duality

7 ©rlc L01 19Jan20117 Energy Quanta for Light Photoelectric Effect: 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 h = 6.625E-34 J-sec

8 ©rlc L01 19Jan20118 Photon: A particle -like wave E = hf, the quantum of energy for light. (PE effect & black body rad.) f = c/, c = 3E8m/sec, = wavelength From Poynting’s theorem (em waves), momentum density = energy density/c Postulate a Photon “momentum” p = h/  = hk, h = h/2  wavenumber, k =  2  /

9 ©rlc L01 19Jan20119 Wave-particle Duality Compton showed  p = hk initial - hk final, so an photon (wave) is particle-like DeBroglie hypothesized a particle could be wave-like,  = h/p Davisson and Germer demonstrated wave-like interference phenomena for electrons to complete the duality model

10 ©rlc L01 19Jan201110 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

11 ©rlc L01 19Jan201111 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”,  (x,t) Prob. density = |  (x,t)   (x,t)|

12 ©rlc L01 19Jan201112 Schrodinger Equation Separation of variables gives  (x,t) =  (x)  (t) The time-independent part of the Schrodinger equation for a single particle with KE = E and PE = V.

13 ©rlc L01 19Jan201113 Solutions for the Schrodinger Equation Solutions of the form of  (x) = A exp(jKx) + B exp (-jKx) K = [8  2 m(E-V)/h 2 ] 1/2 Subj. to boundary conds. and norm.  (x) is finite, single-valued, conts. d  (x)/dx is finite, s-v, and conts.

14 ©rlc L01 19Jan201114 Infinite Potential Well V = 0, 0 < x < a V --> inf. for x a Assume E is finite, so  (x) = 0 outside of well

15 ©rlc L01 19Jan201115 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.

16 ©rlc L01 19Jan201116 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

17 ©rlc L01 19Jan201117 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  (x+L) =  (x) exp(jkL), Bloch’s Thm

18 ©rlc L01 19Jan201118 K-P Potential Function*

19 ©rlc L01 19Jan201119 K-P Static Wavefunctions Inside the ions, 0 < x < a  (x) = A exp(j  x) + B exp (-j  x)  = [8  2 mE/h] 1/2 Between ions region, a < x < (a + b) = L  (x) = C exp(  x) + D exp (-  x)  = [8  2 m(V o -E)/h 2 ] 1/2

20 ©rlc L01 19Jan201120 K-P Impulse Solution Limiting case of V o -> inf. and b -> 0, while  2 b = 2P/a is finite In this way  2 b 2 = 2Pb/a < 1, giving sinh(  b) ~  b and cosh(  b) ~ 1 The solution is expressed by P sin(  a)/(  a) + cos(  a) = cos(ka) Allowed values of LHS bounded by +1 k = free electron wave # = 2  /

21 ©rlc L01 19Jan201121 K-P Solutions* P sin(  a)/(  a) + cos(  a) vs.  a x x

22 ©rlc L01 19Jan201122 K-P E(k) Relationship*

23 ©rlc L01 19Jan201123 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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