Chapter 6: The Free Electron Gas Flashcards

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1
Q

Specific Heat in Metals: Experimental Results

A

Typically plot C/T vs T2

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2
Q

Fermi Energy

(3 points)

A
  • From Pauli Principle, each energy level can only contain two electrons. The energy level of the highest filled state is the Fermi level
    • Corresponds to a sphere in k-space
    • Radius kF = (3π​2n)1/3
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3
Q

Chemical Potential

(5 points)

A
  • Unlike phonons, number of electrons N is constant
    • Leads to chemical potential included in statistics
  • Temperature dependence very small
    • µ(300K) ≈ EF
  • When two objects brought into contact µa = µb
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4
Q

Free Electron Gas: Ground State

(Take-Away: 2 points)

A
  • Energy E = (h-bar)2k2/(2m)
  • Well-defined momentum p = (h-bar)k
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5
Q

Drude vs Sommerfeld

(4 points)

A
  • Drude assumed free mean path l = vthτ
    • Scattering at ions → WRONG!
  • Sommerfeld assumed free mean path l = vFτ
    • Scattering at imprefections
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6
Q

Free Electron Gas: Boundary Conditions

(Take-Away: 2 points)

A
  • kd = 2πni/Ld for d = x, y, z and i = 0, ±1, ±2, …
  • For every k, there exists two electrons (because of spin) with energy
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7
Q

Hall Effect

(Setup: 4 points)

A
  • Smaple has E-field in +x-direction and B-field in the +z-direction
  • Current in +x-direction leads to E-field in +y-direction → Hall Field
  • Lorentz force in -y-direction until compensated by E-field
  • Leads to charge separation
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8
Q

Temperature Dependence of Electrical Conductivity

(2 points)

A
  • σ = 1/ρ so helpful to understand dependence on resistivity
    • Due to scattering of at phonons and defects
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9
Q

Specific Heat - Electronic Contribution: Sommerfeld Approximation

(Assumptions: 2 points)

A
  • Actual internal energy U not solvable analytically
  • F(E) only deviated from F(E(T=0)) in region ±kBT around E ≈ µ
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10
Q

Temperature Dependence of Resistivity

(Graph)

A
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11
Q

Free Electron Gas

(Assumptions: 3 points)

A
  • Electrons in metal are delocalized
  • No electron-ion interactions
  • No electron-electron interactions
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12
Q

Hall Effect

(Take-Away)

A
  • Can obtain sign and charge of carriers feom Measure Hall coefficient R = -1/(ne)
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13
Q

Free Electron Gas: Ground State

(Assumptions: 4 points)

A
  • N free electrons
  • Volume V = L3
  • Temperature T = 0
  • Becuase no electron-electron interactions, can solve problem of single electron in a box with volume V
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14
Q

Sommerfeld Model

(Take-Away: 4 points)

A
  • Again σ = neµ
    • But, µ = eτ /m with l = vFτ
    • Results in higher conductivity
  • Fermi velocity used, because only electrons near Fermi energy can participate
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15
Q

2D Electron Gas

(Assumptions: 2 points)

A
  • Potential walls at z = ±L/2
  • kz restricted to πn/L for n = 1, 2, 3, …
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16
Q

Temperature Dependence of Resistivity: Phonon Scattering

(6 points)

A
  • High temperature T >> ΘD
    • ​ρ ∝ <n> ∝ T</n>
  • Low temperature T << ΘD
    • ​ρ ∝ <n> ∝ T3</n>
    • Experiment shows ρ ∝ T<span>5</span>
    • Additional T2 comes from scattering angle being small
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17
Q

Low-Dimension Electronic Systems

A

Obtained by placing potential walls in one or more directions

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18
Q

Temperature Dependence of Thermal Conductivity in Metals

A
  • From Wiedemann-Franz Law: K(T) = LσT ∝ T /ρ
19
Q

Fermi Gas: Pressure

A
20
Q

Electron Density of States in Momentum Space

(2 points)

A
  • One state per unit volume
  • Two electrons per state
21
Q

Drude Model

(Take-Away)

A
  • σ = neµ
22
Q

Fermi-Dirac Distribution

(3 points)

A
  • Gives the probability that a state with energy E is occupied for a given temperature
    • µ ≡ chemical potential
    • Because kBT << EF , only small number of electrons redistributed
23
Q

Fermi Gas: Total Energy per Electron

A
  • Even at T = 0, still very high
24
Q

Drude Model

(Assumptions: 6 points)

A
  • Electrons in metal behave clasically like a gas of particles
    • Move with thermal velocity vth
    • Collide with atomic cores
  • Acceleration comes from electric field
  • Deceleration comes from collision
    • Relaxes velocity within τ
25
Q

Wiedemann-Franz Law

(2 points)

A
  • Gives relationship between thermal conductivity K and electrical conductivity σ
  • K/(σT) = L → constant: Lorentz number
26
Q

Other Fermi Quantities

A
  • Fermi temperature kBTF = EF
  • Fermi wavelength kF λF = 2π
  • Fermi velocity: mvF = pF = (h-bar)kF
27
Q

Specific Heat - Electronic Contribution: Classical Treatment

(Take-Away)

A

100x larger than experiment, because of Pauli Principle

28
Q

Specific Heat - Electronic Contribution: Classical Treatment

(Assumptions: 2 points)

A
  • Each electrons has 3/2*kBT energy
  • Factor of 2 from spin
29
Q

Electron Density of States in Energy Space

(Graphs)

A
30
Q

Sommerfeld Model

(Assumptions: 5 points)

A
  • Electrons are gas of free fermions
    • Obey Schrodinger’s equation
    • Obey Pauli Principle
  • Entire Fermi sphere responds to external E
  • When external E turned off, relaxation occurs ∝ e−t/τ due to scattering
31
Q

Electron Density of States in Energy Space

(Equations)

A
32
Q

Free Electron Gas

A

An ideal gas of free, non-interacting electrons

33
Q

Free Electron Gas: Boundary Conditions

(Boundary Condition)

A
  • ψk(x,y,z) = ψk(x + Lx,y,z) = ψk(x,y + Ly,z) = ψk(x,y,z + Lz)
34
Q

Thermal Conductivity in Metals

A
  • Can be calculated according to kinetic gas theory like phonons
  • Kph << Kel for metals
35
Q

2D Electron Gas

(Take-Away)

A
  • There exists confinement energy ∆E ∝ L−2
  • Creates 2D parabolic sub-bands in xy-plane
36
Q

Fermi Gas at Finite Temperature

(2 points)

A
  • For T > 0, smearing out of Fermi edge
    • Distributed according to Fermi-Dirac statistics
37
Q

Fermi Gas: Compressibility

A
38
Q

Temperature Dependence of Electric Conductivity

(Graph)

A
39
Q

Specific Heat - Electronic Contribution: Sommerfeld Approximation

(Take-Away: 3 points)

A
  • Only electrons near EF can redistribute and contribute to specific heat
    • Number of electrons Nth ≈ D(EF)kBT
    • Justification for CV ∝ T
40
Q

Drude Model

(Overview: 4 points)

A
  • Historically oldest model
  • Correctly predicts
    • J**q ∝ **E
    • Weidemann-Franz Relation
41
Q

Temperature Dependence of Resistivity: Defects Scattering

(3 points)

A
  • Number of defects is constant
    • ρ0 ≡ residual resistance is constant (independent of T)
    • At low T, phonon scattering vanishes, and only residual remains
42
Q

Electrical Conductivity

A
43
Q

Electron Motion in Magnetic Field

A
  • Electrons now feel Lorentz force