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Solids (free electron gas) Simplest model : non-interacting - - PowerPoint PPT Presentation

EE201/MSE207 Lecture 13 Solids (free electron gas) Simplest model : non-interacting electrons (no Coulomb interaction, no exchange correlation) Idea: electrons occupy energy states from the lowest energy up (fermions) At zero temperature, the


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EE201/MSE207 Lecture 13

Solids (free electron gas)

Simplest model : non-interacting electrons (no Coulomb interaction, no exchange correlation) Idea: electrons occupy energy states from the lowest energy up (fermions) At zero temperature, the highest occupied energy is called Fermi energy. So, we need to count available states. Assume many electrons, so that even though states are discrete, we always consider β€œthick slices” in energy, and are interested only in density of states. Density of states (DOS): number of available states per unit of energy (eV). Goal for today: find DOS and Fermi energy (at π‘ˆ = 0) for quantum wires (1D), quantum wells (2D), and solids (3D) DOS does not depend on temperature (except due to change of material parameters), while Fermi level depends on temperature.

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SLIDE 2

Quantum wire: large 1D well

𝑏 ≫ . . .

πΉπ‘œ = π‘œ2𝜌2ℏ2 2𝑛𝑏2

(π‘œ ≫ 1, 𝑏 is large)

πœ”π‘œ 𝑦 = 2 𝑏 sin π‘œπœŒ 𝑏 𝑦 = 2 𝑏 sin π‘™π‘œπ‘¦ π‘™π‘œ = π‘œπœŒ 𝑏

One state per

πœ€π‘™ = 𝜌 𝑏

4πœ€π‘™ 6πœ€π‘™ 8πœ€π‘™ However, it is more convenient to use both positive and negative 𝑙 (physically corresponds to two directions of momentum) Then one state per πœ€π‘™ = 2𝜌

𝑏

𝑙 πœ€π‘™ 2πœ€π‘™ 3πœ€π‘™ 5πœ€π‘™ 7πœ€π‘™ 𝑙 πœ€π‘™ 2πœ€π‘™ 3πœ€π‘™ 4πœ€π‘™ βˆ’πœ€π‘™ βˆ’2πœ€π‘™ βˆ’3πœ€π‘™ Equivalently, one state per πœ€π‘ž = ℏ πœ€π‘™ = 2πœŒβ„

𝑏

π‘ž πœ€π‘ž 2πœ€π‘ž 3πœ€π‘ž 4πœ€π‘ž βˆ’πœ€π‘ž βˆ’2πœ€π‘ž βˆ’3πœ€π‘ž (not in textbook)

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SLIDE 3

Quantum wire (cont.)

Rule:

  • ne state (quantum level) per

πœ€π‘ž = 2πœŒβ„ 𝑏

So, number of states

Δ𝑂 = Ξ”π‘ž 𝑏 2πœŒβ„

length in space Γ— length in π‘ž space 2πœŒβ„ Density of states

𝐸 𝐹 ≑ Δ𝑂 Δ𝐹 πΉπ‘œ = π‘œ2𝜌2ℏ2 2𝑛𝑏2 ⟹ Δ𝐹 = 2π‘œ 𝜌2ℏ2 2𝑛𝑏2 Ξ”π‘œ ⟹ Ξ”π‘œ Δ𝐹 = 𝑛𝑏2 π‘œπœŒ2ℏ2 = 𝑏 πœŒβ„ 𝑛 2𝐹 𝐸 𝐹 = 𝑏 πœŒβ„ 𝑛 2𝐹 Γ— 2 (spin) 𝐸 𝐹 ∝ 1 𝐹

decreases with energy Fermi energy We have 𝑂 ≫ 1 electrons, what is the maximum occupied energy?

𝐹𝐺 = 𝑂 2 2𝜌2ℏ2 2𝑛𝑏2 = 𝜌2ℏ2 8𝑛 𝑂 𝑏

2

spin (absent for high B-field) 𝑂 𝑏 : (linear) density of electrons (usually measured in 1/eV) 𝐹𝐺 is usually measured in eV (sometimes in Kelvin)

(absent for high magnetic field)

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SLIDE 4

πœ” 𝑦, 𝑧 = 2 𝑏 sin π‘œπœŒ 𝑏 𝑦 2 𝑐 sin π‘šπœŒ 𝑐 𝑧

Quantum well, 2D electron gas, 2DEG (large 2D well)

(not in textbook)

𝑏 𝑐 πΉπ‘œ,π‘š = 𝜌2ℏ2 2𝑛 π‘œ2 𝑏2 + π‘š2 𝑐2 π‘œ, π‘š ≫ 1

𝑙𝑦 𝑙𝑧

⟹ 𝐹 = ℏ2 2𝑛 (𝑙𝑦

2 + 𝑙𝑧 2)

π‘œ π‘š 𝑙𝑦 𝑙𝑧

equal energy line

𝑙𝑦 𝑙𝑧 π‘žπ‘¦ π‘žπ‘§ Again the rule

Δ𝑂 = (Ξ”π‘žπ‘¦ 𝑏)(Ξ”π‘žπ‘§ 𝑐) 2πœŒβ„ 2

equal energy line

area in space Γ— area in π‘ž space 2πœŒβ„ 2 (so far no spin)

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SLIDE 5

2D electron gas (cont.)

𝑏

π‘ž

𝑐

π‘žπ‘¦ π‘žπ‘§

Δ𝑂 = (Ξ”π‘žπ‘¦ 𝑏)(Ξ”π‘žπ‘§ 𝑐) 2πœŒβ„ 2

Density of states π‘žπ‘¦ π‘žπ‘§ Ξ”π‘ž

𝐹 = π‘žπ‘¦

2 + π‘žπ‘§ 2

2𝑛 = π‘ž2 2𝑛 Δ𝐹 = 2π‘žΞ”π‘ž 2𝑛 = π‘žΞ”π‘ž 𝑛 Δ𝑂 = 𝑏𝑐 2πœŒπ‘ž Ξ”π‘ž 2πœŒβ„ 2 𝐸 𝐹 = Δ𝑂 Δ𝐹 = 𝑏𝑐 𝑛 2πœŒβ„2 𝐸 𝐹 𝐡 = 𝑛 2πœŒβ„2 Γ— 2 (spin)

(absent for high magnetic field)

𝐡 = 𝑏𝑐 (area)

𝐸(𝐹) does not depend

  • n energy 𝐹

Fermi energy π‘žπ‘¦ π‘žπ‘§

𝑂 = 𝐡 πœŒπ‘žπΊ

2

2πœŒβ„ 2 Γ— 2 spin = π΅π‘žπΊ

2

2πœŒβ„2 π‘žπΊ 𝐹𝐺 = π‘žπΊ

2

2𝑛 = πœŒβ„2 𝑛 𝑂 𝐡

2D density in space

(twice larger 𝐹𝐺 in high B-field) π‘ž

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SLIDE 6

Example

2DEG in GaAs,

π‘œ = 𝑂 𝐡 = 1012 1 cm2 .

Find Fermi energy.

𝑛eff = 0.067 𝑛0

𝐹𝐺 = πœŒβ„2 𝑛 π‘œ = 𝜌 1.05 βˆ™ 10βˆ’34Js 2 0.067 βˆ™ 9.1 βˆ™ 10βˆ’31kg βˆ™ 1016 1 m2 = = 5.68 βˆ™ 10βˆ’21J = 35 meV = 410 K

𝑙𝐢 = 1.38 βˆ™ 10βˆ’23 J K eV = 1.6 βˆ™ 10βˆ’19 J

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SLIDE 7

Large 3D well: theory of metals

𝑏 𝑑 𝑐

Same rule

Δ𝑂 = (Ξ”π‘žπ‘¦ 𝑏)(Ξ”π‘žπ‘§ 𝑐)(Ξ”π‘žπ‘¨ 𝑑) 2πœŒβ„ 3 = π‘Š Ξ”π‘žπ‘¦Ξ”π‘žπ‘§Ξ”π‘žπ‘¨ 2πœŒβ„ 3

π‘Š = 𝑏𝑐𝑑 (slightly different in textbook) π‘žπ‘§ π‘žπ‘¨ π‘žπ‘¦ π‘ž Ξ”π‘ž Density of states 𝐸 𝐹 = Δ𝑂 Δ𝐹

Δ𝑂 = π‘Š 4πœŒπ‘ž2Ξ”π‘ž 2πœŒβ„ 3 Δ𝐹 = Ξ” π‘ž2 2𝑛 = π‘ž 𝑛 Ξ”π‘ž Δ𝑂 Δ𝐹 = π‘Š 4πœŒπ‘žπ‘› 2πœŒβ„ 3 = π‘Š 𝑛 2𝑛𝐹 2𝜌2ℏ3 = π‘Š 𝑛3/2 𝐹 2 𝜌2ℏ3 𝐸(𝐹) π‘Š = 𝑛3/2 𝐹 2 𝜌2ℏ3 Γ— 2 (spin)

3D: 𝐸 𝐹 ∝ 𝐹 2D: 𝐸 𝐹 ∝ 𝐹0 1D: 𝐸 𝐹 ∝ 1 𝐹 Some people call 𝐸(𝐹)/π‘Š density of states

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SLIDE 8

Theory of metals (cont.)

𝑏 𝑑 𝑐 Δ𝑂 = π‘Š Ξ”π‘žπ‘¦Ξ”π‘žπ‘§Ξ”π‘žπ‘¨ 2πœŒβ„ 3

π‘Š = 𝑏𝑐𝑑 π‘žπ‘§ π‘žπ‘¨ π‘žπ‘¦ π‘žπΊ

Fermi energy 𝑂 = π‘Š 4 3 πœŒπ‘žπΊ

3

2πœŒβ„ 3 βˆ™ 2 spin = π‘Š π‘žπΊ

3

3𝜌2ℏ3 π‘žπΊ = ℏ 3𝜌2 𝑂 π‘Š

1/3

𝐹𝐺 = π‘žπΊ

2

2𝑛 = ℏ2 2𝑛 3𝜌2 𝑂 π‘Š

2/3

𝑙𝐺 = π‘žπΊ ℏ = 3𝜌2 𝑂 π‘Š

1/3

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SLIDE 9

Example 1

Copper (Cu) mass density 𝜍 = 8.96 g cm3 atomic mass 𝑁 = 63.5 g mole

Find 𝐹𝐺

𝑂 π‘Š = 1 βˆ™ atoms m3 = 𝜍 𝑂

𝐡

𝑁 = 8.96 βˆ™ 103 kg m3 6.02 βˆ™ 1023 1 mole 63.5 βˆ™ 10βˆ’3 kg mole = 8.5 βˆ™ 1028 1 m3

𝐹𝐺 = ℏ2 2𝑛 3𝜌2 𝑂 π‘Š

2/3

𝐹𝐺 = ℏ2 2𝑛 3𝜌2 𝑂 π‘Š

2/3

= 1.05 βˆ™ 10βˆ’34 2 2 βˆ— 9.1 βˆ™ 10βˆ’31 3 βˆ™ 3.142 βˆ™ 8.5 βˆ™ 1028 2/3 = = 1.1 βˆ™ 10βˆ’18J = 7.0 eV = 8.1 βˆ™ 104K

𝑙𝐢 = 1.38 βˆ™ 10βˆ’23 J K eV = 1.6 βˆ™ 10βˆ’19 J π‘ˆ

𝐺 ≫ 300 K ! degenerate electron gas

Fermi velocity 𝑀𝐺 =

2𝐹𝐺 𝑛 = 1.6 βˆ™ 106 m s

(very high but still nonrelativistic)

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SLIDE 10

Example 2

GaAs (bulk), doping of 1018 1 cm3 𝑛eff = 0.067 𝑛0

Find 𝐹𝐺 𝐹𝐺 = ℏ2 2𝑛 3𝜌2 𝑂 π‘Š

2/3

= 1.05 βˆ™ 10βˆ’34 2 2 βˆ— 0.067 βˆ™ 9.1 βˆ™ 10βˆ’31 3𝜌2 βˆ™ 1024 2/3 = = 8.65 βˆ™ 10βˆ’21J = 54 meV = 630 K

still > 300 K, behaves almost as a metal (degenerate semiconductor) However, if doping of 1017cmβˆ’3, then only 140 K.