Ee606-s09-lecture3

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EE‐606: Solid State Electronics Lecture 3: Elements of Quantum Mechanics Muhammad Ashraful Alam [email protected]

Alam ECE‐606 S09

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Outline

1) Why do we need quantum physics 2) Quantum concepts 3) Formulation of quantum mechanics 4) Conclusions

Reference: Vol. 6, Ch. 1 (pages 23‐32)

Alam ECE‐606 S09

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Do I really need Quantum Mechanics ? Original Problem

Periodic Structure

Electrons in periodic potential: Problem we want to solve

If it were large objects, like a skier skiing past a set of obstacles, Newton’s mechanics would work fine, but in a micro-world …… Alam ECE‐606 S09

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Carrier Density

Carrier number = Number of states x filling factor Chapters 2‐3

Chapter 4

Total number of occupants = Number of apartments X The fraction occupied

Alam ECE‐606 S09

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Outline

1) Why do we need quantum physics 2) Quantum concepts 3) Formulation of quantum mechanics 4) Conclusions

Alam ECE‐606 S09

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Four Quantum Concepts ..

• Blackbody Radiation

• Photoelectric Effect • Bohr Atom • Wave Particle Duality

Alam ECE‐606 S09

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(1) black‐body radiation 2000 K

1000 K

300 K

Alam ECE‐606 S08

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Rayleigh-Jeans Formula

2000 K

(u)

u ∝ k BT / λ 4 log(u ) = −4 log(λ ) + log(T ) Wein’s Formula

u∝

e

− β / λT

λ

5

Plank’s fitting formula

1  1  u ∝ 5  β / λT − 1  λ e Alam ECE‐606 S08

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Interpretation of Plank’s Formula dλ 1  1  dλ u ( f , T ) = u (λ , T ) ~ 5  β / λT  df λ  e − 1  df 1   2 ~ f × hf ×  hf / kT  −1  e nos. of modes

c λ= f

Occupation Probability

Energy of mode

EM emission occurs in discrete quanta of

E = hf

n=1,2, …….. N

Alam ECE‐606 S09

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Recent Example: COBE Data

J.C. Mather, Astrophysics J., 1990.

Show that the cosmic background temperature is approximately 3K. Can you “see” this radiation? Alam ECE‐606 S09

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(2) Photoelectric Effect

E = (hf‐W) Electrons

Light (hf)

υ

hf

mυ 2 = hf − W

cathode

VR

VR

W

( 2)

VR ≈ 1

W

hf

Absorption occurs in quanta as well, consistent with photons having E=hf Alam ECE‐606 S09

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Origin of Quantization

frequency

1   1 Em ,n = const ×  2 − 2  n  m Alam ECE‐606 S09

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(3) Bohr Atom .. Assume that angular momentum is quantized:

υ = n! / m0 rn

Alam ECE‐606 S09

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(3) Bohr Atom (continued) …

1   1 Em ,n = const ×  2 − 2  n  m Alam ECE‐606 S09

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(4) Wave‐Particle Duality Photons act both as wave and particle, what about electrons ?

E = m0 c + p c 2 4

hf = pc

2 2

m0=0 (photon rest mass)

p = hf / c = h / λ (because c = λf ) =!k (because k = 2π / λ ) Alam ECE‐606 S09

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Outline

1) Why do we need quantum physics 2) Quantum concepts 3) Formulation of Schrodinger Equation 4) Conclusions

Alam ECE‐606 S09

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Schrodinger Equation 2 2 2 4  E = m0 c + p c ≈ m0 c 1 + p c / 2m0 c + ... 2 4

E − m0c

2 2

2

2

= V + (p / 2m0 ) 2

hf = !ω = V + (! k / 2m0 ) 2 2

Alam ECE‐606 S09

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Schrodinger Equation (continued)

!ω = V + (! k / 2m0 ) 2 2

Assume,

Ψ ( x, t ) = A exp(−i (ωt − kx))

d Ψ / dt = −iωΨ and d Ψ / dx = −k Ψ 2

2

2

! d Ψ dΨ − + V Ψ = i! 2 2m0 dx dt 2

2

Alam ECE‐606 S09

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Conclusions 1. Given chemical composition and atomic arrangements, we are ready to compute electron density by using quantum mechanics. 2. We discussed the origin of quantum mechanics – experiments p were inconsistent with the classical theory. y 3. We saw how Schrodinger equation could arise as a consequence of quantization and relativity, but this is not a derivation. 4. We will solve some toy problems in the next class to get a feeling of how to use quantum mechanics. Alam ECE‐606 S09

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