Solid State Physics Flashcards

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1
Q

What is a lattice and a basis?

A

Lattice: Describes the underlying periodicity of the structure.

Basis: Group of atoms being repeated.

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2
Q

What is a Bravais Lattice?

A

A periodic array of points that look identical from every point.

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3
Q

What is the primitive unit cell?

A

The minimum volume that fills all space when translated by all lattice vectors.

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4
Q

What is the volume of the primitive unit cell in lattice vectors?

A

V = |a1 * (a2 x a3)|

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5
Q

How many lattice points does a primitive unit cell contain?

A

One.

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6
Q

How is the volume of the Weigner-Seitz cell defined?

A

The volume enclosed by planes that perpendicularly bisect the lines to the nearest lattice points.

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7
Q

How does Bragg reflection work?

A

Lattice planes reflect x-rays specularly, with constuctive interference when paths drift by n*2pi.

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8
Q

State Bragg’s Law.

A

2dsin(theta) = n*lamda

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9
Q

For Bragg’s Law, what is the use of using a neutron beam over X-rays?

A

Neutrons are scattered only by nuclei, not electrons, and so are more useful in studying light elements.

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10
Q

How do you find the Miller indices of a crystal plane?

A
  • Take any lattice plane and find its intercepts, m1, m2, and m3, relative to the crystallographic axis.
  • Find reciprocals 1/m1, 1/m2, 1/m3
  • Scale all reciprocals by a common factor to find the smallest set of integers; h,k,l.
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11
Q

How is the reciprocal lattice defined?

A

The reciprocal lattice is the set of all wavevectors k that yield plane waves with the periodicity of a Bravais lattice.

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12
Q

How do reciprocal wavevectors G relate to lattice vectors R?

A

exp( i(G*R)) = 1

or GR = 2pin

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13
Q

How do lattice vectors a1, a2 and a3 relate to reciprocal lattice vectors b1, b2 and b3?

A
  • b1 = 2pi/V * (a2 x a3)
  • b2 = 2pi/V * (a3 x a1)
  • b3 = 2pi/V * (a1 x a2)

where volume V = a1 * (a2 x a3)

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14
Q

What is the formula for the volume of a reciprocal unit cell?

A

V = b1 * (b2 x b3)

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15
Q

What is the formula for distance between reciprocal crystal planes?

A

d_hkl = 2pi / | G_hkl |

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16
Q

What is the formula for distance between reciprocal planes of a cubic crystal?

A

d = a / sqrt( h^2 + k^2 + l^2 )

where a = lattice constant

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17
Q

How is momentum transfer Q defined in Laue diffraction, with regard to wave vectors?

A

Q = k’ - k

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18
Q

What is the Laue condition for diffraction?

A

Q = G

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19
Q

How is the structure factor S_G defined?

A

S_G = sum[ f_j * exp( i(-G * r_j)) ]

where f_j = integral [ n_j (rho) * exp( -G * rho) ], the atomic form factor in the amplitude scattered by the electron.

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20
Q

How is the Brillouin zone defined?

A

The Brillouin zone is the Weigner-Seitz cell of the reciprocal lattice; i.e. it is formed by the volume enclosed of the perpendicular bisectors of lines to nearest atoms.

It has the same volume as the primitive unit cell of the reciprocal lattice.

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21
Q

How does the Brillouin zone play into the Laue condition for diffraction?

A

When G = Q = k’ - k is satisfied, k terminates of the Brillouin zone boundary. This is a sufficient condition for diffraction; i.e if a wavevector terminates on the BZ boundary, the wave will be diffracted.

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22
Q

What is the dispersion relation for monatomic atoms on a 1D chain?

A

w^2 = 4C/m * sin^2(ka/2)

where C is the spring constant, m is the atomic mass, and a is the lattice constant.

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23
Q

What does the dispersion relation describe?

A

It describes how frequency of an elastic wave (w) changes with wavevector k (where k = 2pi/wavelength).

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24
Q

In regards to atomic displacement, why is the first Brillouin zone boundary unique?

A

The first BZ, i.e -pi/a

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25
Q

To find solutions of 1D chain problems, what steps are needed?

A
  • Use equations of motion (F=ma, F=kx) on displacements of atoms, u_n and v_n.
  • Try travelling wave solutions: u_n = u_0exp[ i(kna - wt)]
  • Substitute.
  • If necessary, express equations in the form of a matrix, and find the determinant for solutions.
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26
Q

What is a phonon?

A

A phonon is a quantum of energy of a mechanical excitation, similar to photons.

They are bosons with spin 0, and so obey Bose-Einstein statistics: when a mode is excited to quantum number n, it is said to be occupied by n phonons:

n(w) = 1 / [exp( hbar * w / k_b * T) - 1]

Phonons carry energy hbarw and momentum hbark, known as crystal momentum.

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27
Q

How would you express the components of total heat capacity of a generic crystal?

A

Cv = Cv_phonons + Cv_electrons + Cv_magnetic

Cv_phonons is found in all solids.

Cv_electrons is only found in metals.

Cv_magnetic is only found in magnets.

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28
Q

How does heat capacity Cv relate to energy E and temperature T?

A

Cv = dE/dT

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29
Q

For a crystal of N atoms, what is its classical heat capacity?

A

Cv = 3Nk_b

where k_b is the Boltzmann constant. This formula breaks down at low temperatures.

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30
Q

In Debye Theory, what is the formula for total lattice energy E?

A

E = integral [0 -> w_D] [hbar*w * g(w) * u(w)] dw per branch.

Where g(w) is the density of states and u(w) is the bose-einstein factor, 1/(e^(hbar*w/kt)).

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31
Q

What assumptions does Debye Theory make?

A
  • The crystal is harmonic (independent modes)
  • Elastic waves are non-dispersive (w = k*v_s)
  • Crystal is isotropic
  • There is a high-frequency cutoff, w_D.
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32
Q

In Debye theory, how many unit cells are the there in a crystal?

A

N = integral [0 -> w_D] {g(w)*dw]

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33
Q

What happens in a ‘Normal’ and an ‘Umklapp’ event? How does it affect heat flow?

A
  • Phonons interact and scatter off each other (k1 + k2 = k3), which defines the thermal conductivity of a crystal.
  • In normal events, k3 is within the 1st BZB.
  • In Umklapp events, k3 lies outside the 1st BZB, but can be translated into it by reciprocal lattice vector G, producing a phonon sometimes going the opposite direction.
  • Heat flow carried by phonons is unaffect by normal (N) events, but is impeded by Umklapp scattering, so U events contribute to thermal resistivity.
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34
Q

What assumptions does the Free Electron Theory make?

A
  • A fixed background of fixed positive charges doe to nuclei
  • Valence electrons propagate freely without interacting with ion cores or other electrons.
  • Zero potential energy.
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35
Q

How is the speed of sound v_s (i.e. group velocity v_g) related to frequency w and wavevector k? What about phase velocity v_p?

A

v_s = v_g = dw/dk

v_p = w/k

36
Q

In regards to interatomic potentials, what is anharmonicity? What are its consequences?

A
  • Anharmonicity is the idea that force exerted on an atom is not directly proportional to its displacement, due to either core repulsion or Coulomb attraction.
  • Assuming this, there is thermal expansion: > a, as it costs less energy to expand than contract.
  • Phonons also interact with each other, and causes momentary expansion or contraction of a lattice. Phonons scattering off each other determine the thermal conductivity of a solid.
37
Q

How is thermal current density j_u related to thermal conductivity K and temperature gradient?

A

j_u = -K * dT/dx

38
Q

What is the formula for thermal conductivity K, based on kinetic theory of gases?

A

K = 1/3 * v * l * Cv

where v = average velocity of sound, l = mean free path, and Cv = heat capacity per unit volume

39
Q

What is mean free path l proportional to? What happens to l as T varies?

A
  • l is proportional to 1 / # phonons
  • At high T, (T > Debye temp. T_D) all phonon modes up to hbar*w_D are excited, and so there are many photons with large enough |k| to produce Umklapp events. Energy is proportional to T, so # phonons is proportional to T, and so l is proportional to 1/T.
  • At intermediate T (T ~ T_D), U-events start to stop as the average energy of phonons decreases. # phonons ~ exp( -T_D/T), so l is proportional to exp(T_D/T).
  • At low T (T
40
Q

What is the equation for density of states (wrt phonon energy e) in the Free Electron Model?

A

g(e) = V/2pi^2 * (2m/hbar^2)^(3/2) * e^1/2

This comes from calculating the density of states w.r.t. k, multiplying by 2 to account for spin, and substituting the formula for energy of a phonon.

41
Q

What is the Fermi Energy? What is the formula for it in the Free Electron Model?

A
  • Fermi Energy is the energy at which states are filled up to at T=0.
  • e_F = hbar^2 / 2m * ( 3 pi^2 N / V)^(2/3)
  • This corresponds to the filling of all k-states inside a sphere of radius k_F, the Fermi Radius.
42
Q

What is the formula for the Fermi Radius?

A
  • k_F = (3pi^2 N / V) ^ (2/3)
43
Q

How is total heat capacity Cv related to T?

A

Cv_total = Cv_phonon + Cv_electron
= bT^3 + gT

where g = pi^2/2 * N/e_F * k_b * T

44
Q

What happens to the Fermi Surface in the presence of an electric field?

A

The Fermi Surface is shifted in the direction of the field, as the electric field applies force to all electrons, via the Lorentz force.

45
Q

State the Wiedemann-Franz law.

A

K/(sigma * T) = L

Where K =thermal conductivity, sigma = electric conductivity, and L = Lorentz number (constant).

46
Q

What is the Hall effect? What is its formula?

A
  • When a metal is placed in magnetic field B and a current j flows through it, a transverse electric field E appears:
  • E = R * (B x j)

where R is the Hall coefficient.

47
Q

What is the formula for the Hall coefficient?

A

E = - 1/n_e,

where n_e is the electron concentration.

48
Q

What is the tight binding model?

A

Electron bands emerge due to overlap of the wavefunctions of isolated atoms as they are brought closer to form a solid.

49
Q

What is Bloch’s Theorem?

A

Wave functions in a periodic potential differ from a plane wave of a free electron only by a periodic modulation. I.e, if V(r) = V(r+R) where R is any lattice vector, then irrespective of the form of V(r) the solutions of the Schrodingher equation is of the form:

phi(r) = u(r)exp(ikr)

where u(r) = u(r+R), i.e. u(r) has the periodicity of the lattice.

An alternative statement:

phi(r+R) = exp(ik*R) * phi(r)

50
Q

What is the Meissner effect?

A

The exclusion of magnetic flux for the interior of a superconductor.

i.e. Susceptibility chi = -1

51
Q

What is the critical field?

A

The magnetic field strength at which superconductivity is destroyed.

52
Q

What are screening currents?

A

If the interior magnetic field of a superconductor is 0, then there must be electric currents created to counteract the field, found on the surface of the superconductor to penetration depth lamda.

53
Q

What is the demagnetisation factor of a long thin rod, a sphere, and an infinite disc? What is the formula for demagnetization?

A

0, 1/3, 1

H_inside = D * H_applied

54
Q

What is persistent current in a superconductor?

A

It is trapped flux that causes a current to flow ‘forever’ around a superconductor, with resistance very very close to 0.

55
Q

What is the critical current?

A

Similar to critical field, critical current is the current strength around a superconductor at which superconductivity is destroyed. Also known as the ‘Silsbee Hypothesis’.

56
Q

What is the temperature dependence of the critical current, Bc?

A

It is an approximation:

Bc (T) ~ Bc (0) (1 - (T/Tc)^2)

i.e Bc becomes quadratically smaller as T increases, until it reaches critical temperature, Tc.

57
Q

How is the Gibbs energy of the superconducting state, Gs, and the Gibbs energy of the normal state, Gn, related to critical field, Bc?

A

Gn (0, T) - Gs (0, T) = Bc^2 / (2* mu_0)

58
Q

For type-2 superconductors, what happens above the first critical field?

A

Above Bc, the type-2 superconductor is in a ‘mixed state’, where magnetic flux penetrates the material but doesn’t destroy the superconductivity.

59
Q

What is the London equation?

A

j = - (ne^2 / m) A

Where n is the number of electrons per unit volume, e is electron charge, m is electron mass, and A is vector potential.

60
Q

What relates penetration depth L to magnetic field B?

A

del^2 B = (1 / L^2) B

61
Q

What is the equation for magnetic flux Phi in a superconductor?

A

Phi = n Phi (0),

Where n = integer and Phi (0) = h / 2e

Provides evidence of ‘Cooper Pairs’

62
Q

What formula determines between type-1 and type-2 superconductors?

A
  • If S/L > 1, it is type-1

- If S/L

63
Q

What is the difference between direct and indirect band gaps?

A

If the minimal energy state in the conduction band and the maximal energy state of the valence band has the same k-vector, it is a ‘direct’ band gap, and can be crossed by just a photon of energy ~hbar*w.

An ‘indirect’ band gap has the min state of the conduction band and the max state of the valence band at different k-vectors, and so usually requires both a photon to cross the energy gap, and a phonon to cross the difference in k (i.e. the momentum).

See diagrams in notes.

64
Q

What is the formula for effective mass of an electron, m_e*?

A

m_e* = hbar^2 / (d^2 e/ dk^2)

I.e. it depends on band curvature.

65
Q

What is a ‘hole’?

A

It represents the empty state where a electron would be in a band, and is treated as a particle in its own right.

It has:

  • positive effective mass m*
  • positive charge +e
  • ‘upwards’ dispersion
66
Q

What is the law of mass action?

A

Regardless of doping, the product of electron and hole densities is constant at equilibrium. This constant depends on T:

n_p = N_c * N_v * exp(-e_G / (k_b * T))

Where n_p is carrier density, N_c is the number of electrons, N_v is the number of holes, and e_G is the ground energy (i.e energy at top of valence band).

67
Q

What is the difference between intrinsic and extrinsic semiconductors?

A

Intrinsic semiconductors are undoped, while extrinsic semiconductors are doped with impurities.

68
Q

What is charge neutrality in intrinsic semiconductors?

A

The number of holes equals the number of electrons, i.e. n=p

69
Q

What is the formula for chemical potential in semiconductors, mu?

A

mu (T) = 1/2 e_G + 1/2 k_b T ln( N_v / N_c)

So if T=0 or N_c = N_v, mu = 1/2 e_G

70
Q

What is the difference between n-type and p-type semiconductors?

A

Impurities in extrinsic semiconductors can act as either donors or acceptors of electrons.

If donors are the majority, it is n-type.

If acceptors are the majority, it is p-type.

71
Q

In extrinsic semiconductors, what is carrier concentration, n_i, proportional to?

A

From the law of mass action,

n_i^2 = n*p is proportional to exp( -e_G / (k_b * T)).

72
Q

What is the Diode equation?

A

Current I = I_0 * (exp( eV/kT) - 1)

Where I = current, I_0 = bias current of the diode.

I_0 is proportional to exp( -e_G/kT)

73
Q

How is magnetism of a solid, M, related to magnetic intensity, H?

A

M = chi*H,

Where chi = magnetic susceptibility.

74
Q

What is the difference between diamagnetic materials and paramagnetic materials?

A

In diamagnets, chi 0

75
Q

What is the Curie Law?

A

The Curie Law is the thermodynamic equation of states for an ideal paramagnet:

chi = C/T

Where C is the ‘Curie constant’.

76
Q

What is the equation for a magnetic dipole moment, mu?

A

mu = mu_b * l

Where mu_b is the Bohr Magneton.

77
Q

What is the formula for Zeeman energy in a magnetic field? What is the formula for the magnetic moment operator?

A

E = -mu * B,

where mu in this case is the dipole moment operator:

mu = -gmu_bJ/hbar

78
Q

What is the thermodynamic equation for magnetic work?

A

dW = B * dm

Where B is the applied field and m is magnetic moment.

79
Q

In regards to angular momentum components L and S, what is the magnetic moment, mu?

A

mu = -mu_B * (L + 2S)

80
Q

What is the formula for the thermally averaged magnetic moment?

A

In direction z:

= g * mu_B * S * tanh ( g * mu_B * S * B / kT)

81
Q

What is the formula for the thermally averaged magnetic moment of a free ion in a low field?

A

= g_J^2 * mu_B^2 * J(J+1) * B / 3kT

82
Q

What is the formula for Pauli paramagnetic susceptibility, chi? What is the free-electron diamagnetic contribution?

A
  • chi_para = (3N * mu_0 * mu_B^2) / 2e_F

- chi_dia = - 1/3 chi_para

83
Q

What is the formula for electromagnetic momentum?

A

p = mv + qA

Where q = particle charge, A = vector potential, v = velocity and m = mass.

84
Q

What is the Curie-Weiss Law?

A

Chi = M / H = C / (T - theta)

Where C is the Curie constant, and theta is the ‘Curie - Weiss’ constant.

85
Q

What is the formula for the Curie-Weiss constant, theta?

A

theta = 1/3 * z * J (S(S+1))