Free-Electron Theory Flashcards

1
Q

Dulong-Petit Law

A

-heat capacity of a solid: Cv = 3R

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2
Q

Magnetic Moments of Atoms

A

-individual atoms have magnetic moments -if the electron shell is not full then there are unpaired spins which contribute to the magnetic moment -the orbital motion of electrons also generates a magnetic moment -most atoms in the periodic table are magnetic as individual atoms, but not as whole solids

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3
Q

Molar Magnetic Susceptibility Definition

A

χ = dM/dH M - magnetisation of the sample, i.e. dipole moment per unit volume H - magnetic field

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4
Q

Magnetic Susceptibility and Types of Magnets

A

-a positive χ indicates a paramagnet -a negative χ indicates a diamagnet

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5
Q

How many elements are metals, insulators or semiconductors?

A

-by plotting resistivity against atomic number, it is immediately clear that most elements have a low resistivity and are therefore metals -there are only four elemental semiconductors

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6
Q

Schrodinger Equation for Free Electrons

A

HΨ = EΨ Ψ - wave function E - energy H - Hamiltonian -in this equation, H is an operator which can be applied to the wave function, the resulting function will contain information about the energy

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7
Q

Hamiltonian for Free Electrons

A

H = -ħ²/2m ∇² + V(r) -where V(r) is the ionic potential -for free electrons V(r)=0 so H = -ħ²/2m ∇²

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8
Q

Wave Function for Free Electrons

A

-choosing a plane wave function and working in one dimension: Ψ (r) = A e^(i|k.|r) -this can be justified by noting that operating with the momentum operator (-iħ∇) gives eigenvalues of ħk which is obviously the momentum of a free electron -also A = V^(-1/2) where V is the volume of the box containing the electron

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9
Q

Normalising

A

∫ Ψ* Ψ d|r = 1 -where Ψ* is the complex conjugate -integrating from negative infinity to positive infinity -also Ψ* Ψ gives the probability of locating a particle -from negative to positive infinity the probability must be 1 since the particles does exist somewhere

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10
Q

How to show that electrons can be represented as plane waves of the form Ψ = A e^(i|k.|r)

A

-apply the momentum operator: ^p = ħ/i *∇ -to the wave function in a volume of 1 which means A=1: ħ/i *∇ e^(i|k.x) = ħk * e^(ik.x) -this gives momentum as p=ħk -using the Schrodinger equation to find energy: - ħ²/2m * ∇² Ψ= EΨ = ħ²k²/2m Ψ = E Ψ => p²/2m = E -as these results for momentum and energy are correct, the wave function is correct for an electron

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11
Q

Periodic Boundary Conditions

A

-consider an empty box of side L -periodic conditions allow functions such that: Ψ(x) = Ψ(x+L) -these boundary conditions mean that every distance L the wave function has the same value -these boundary conditions restrict the plane waves that can exist in the box

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12
Q

Possible K Values Derivation

A

-choose: e^(ikx.L) = e^(iky.L) = e^(ikz.L) = 1 -in order for e^z=1 where z is a complex number, z=2πin, where n is an integer -this gives: kx = 2π*nx/L -and similarly for ky and kz -then finding the modulus of k: k² = (2π/L)² (nx² + ny² + nz²)

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13
Q

Picturing Possible k Values

A

-imagine k space, as three dimensional space with kx on the x axis ky on y and k on z -the possible k values are whole number coordinates where the distance between the numbers in 2π/L

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14
Q

How many electrons can occupy the same k value?

A

-as electrons are fermions, only one electron (or zero electrons) can occupy a particular quantum state -however wave vector, k, alone does not determine a quantum state -a spin up electron and a spin down electron can occupy each k value

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15
Q

How to count the number of states?

A

-draw a sphere with radius kmax over the allowed states centred at (0,0,0) in k space -calculate the volume of the sphere: V = 4/3 π kmax³ -calculate the volume per k value: (2π/L)³ -divide the total volume by the volume per k value to get the number of possible k values: 1/2 * L³kmax³/3π² -to account for the spin up and spin down states, double this number to get the total number of states: N = L³kmax³/3π² -replace L³ with V, and divide by V to obtain number density, n=N/V : n = kmax³/3π² -identifying kmax with kf, the Fermi wave vector we obtain: kf³ = 3π²n

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16
Q

Derive the free electron density of states

A

-calculate the volume of a sphere in k space: 4/3 * π * kf³ -divide by the volume per point in k space (2/L)³ : 1/2*L³kf³/3π² = 1/2 * Vkf³/3π² -multiply by two for spin up and spin down states to get the total number of states: N = Vkf³/3π² -number of states per unit volume in k space can be found by dividing by V -use the equation E = ħ²kf²/2m to write N in terms of E : N = V*(2mE)^(3/2) / 3π²ħ³ -differentiate with respect to E to find the density of states; dN/dE = g(E) = V(2m)^(3/2)*√E / 2π²ħ³

17
Q

Define g(E)

A

-total number of states with energy E (not number if occupied states) -by definition g(E) = dN/dE

18
Q

Define g(E)dE

A

-total number of states with energy between E and E+dE

19
Q

Describe the graph of g(E) against E

A

-since g(E) = V(2m)^(3/2)*√E / 2π²ħ³ , the graph follow a √E shape -this graph does not change significantly with temperature -the graph shows that there are more possible states per energy at higher energy levels eventhough we know that electrons obey the Pauli exclusion principle -this is because there are many sets of k values that give the same magnitude of momentum and therefore the same energy, but are moving in a different direction, but only two states (spin up/down) can occupy each energy

20
Q

How are the electron states filled?

A

-at every energy there can be two electrons, one spin up and one spin down -the states are filled from the lowest energy state up with two electrons per energy

21
Q

Why does temperature have almost no effect on the electron density of states?

A

-electron states are filled from the lowest energy state upwards -reducing the temperature to T=0K does not effect the electrons since there is no available lower energy state for an electron to move to if you were to take energy away from it -therefore nothing happens

22
Q

How to find the number of free electrons per unit volume in a given material Density Method

A

-find number of valence electrons Z from the periodic table e.g. first column elements donate 1 electron, 2nd column electrons donate 2 electrons etc. -look up the density ρ -find the atomic mass (mass of 1 mole of the material) M -recall Advogadro’s Number Na -then sub into: n = Na*Z*ρ / M

23
Q

How to find the number of free electrons per unit volume in a given material Unit Cell Method

A

-find number of valence electrons Z from the periodic table e.g. first column elements donate 1 electron, 2nd column electrons donate 2 electrons etc. -find N, the number of atoms per unit cell, 4 for a face centred cubic -look up ao, the length of the unit cell -sub into: n = Z * N / ao³

24
Q

How to calculate the number of possible states with the Fermi energy

A

N = V*(2mE)^(3/2) / 3π²ħ³ => dN/N = 3/2 * dE/E dN/dE = 3/2 * N/E => g(Ef) = 3/2 * N/Ef

25
Q

What stops electron energy from changing with temperature?

A

-when there are no available states the electron energy cannot change -at most temperatures kT is so small in comparison to Ef that changing the temperature has no measurable impact on the energy of the electrons

26
Q

How to find the total number of states given the density of states?

A

N = ∫ g(E) dE -where the integral is taken form 0 to infinity

27
Q

Electrochemical Potential

A

look up

28
Q

Fermi-Dirac Distribution

A

f(E) = 1 / (e^[(E-Ef)/kb*T] + 1) -f tells you the probability that a state with energy E will be occupied at a given temperature T

29
Q

Formula for the Number of Occupied States

A

Nocc = g(E)*f(E)dE

30
Q

Heat Capacity Equation

A

C = dE/dT = π²/3*g(Ef)*kb²*T ≈ 2*g(Ef)*kb²*T

31
Q

Magnetic Moment of a Free Electron

A

μ = -g*μb*s -where g is the Lande g-factor which is 2 for an electron -and μb is the Bohr magneton, eћ/2m -and s is the spin quantum number 1/2 for an electron -so for an electron: μ = μb

32
Q

Magnetisation

A

-the dipole moment per unit volume; M = μ/V = g(Ef)*μb²*B

33
Q

Magnetic Suscetibility

A

-how easy it is to magnetise a material, a higher number means it is easier; Χ = dM/dH = μo*μb²*g(Ef)

34
Q

Spin Resolved Density of States in a Magnetic Field Description

A

-g(E) has been split into spin up and spin down states -in a magnetic field the energy of a dipole is given by: E = -μ*B -for a free electron μ=μb -so electrons with their spin aligned with the field will have their energy lowered by μb*B -and electrons with their spin opposite to the field will have their energy increased by μb*B -to normalise the Fermi energy, make it the same for spin up and spin down electrons, some electrons will flip spins giving a net difference of -μb to +μb which =2μb -since there are now different numbers of spin up and spin down electrons the sample has a magnetic moment: m = μb [Nu - Nd]