Phonons Flashcards

1
Q

Simple 1D Model of Atoms

Description

A

-atoms with mass M separated by a distance a and connected by springs with spring constant K

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
2
Q

Simple 1D Model of Atoms

Equation of Motion

A

-an equation of motion can be written down in terms of the displacement of the nth atom, un:
M d²un/dt² = -2Kun + K(un+! + un-1)
-we therefore expect a time dependence proportional to e^(iωt)
-so:
un’’ = -ω²
un

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
3
Q

Simple 1D Model of Atoms

Difference Equation for Displacements

A

-sub un’’ = -ω²un into the equation of motion:
-M
ω²un = K(un+1 + un-1 - 2un)
-therefore we can expect travelling wave solutions of the form:
u±1 = u
e^(inqa)*e^(±iqa)
-where a is the atomic separation distance and q is the phonon wave vector

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
4
Q

Simple 1D Model of Atoms

Derivation of the Dispersion Relation for Phonons

A

-substitute the travelling wave solutions for un, un+1 and un-1 into the equation of motion:
-Mω²ue^(inqa) = Ku[e^(i(n+1)qa) + e^(i(n-1)qa) - 2e^(inqa)]
-cancel u*e^(inqa) and use trigonometric double angle formula for cos to find the dispersion relation:
ω = √[4K/M] * sin(qa/2)

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
5
Q

Phonon Dispersion Relation

A

ω = √[4K/M] * sin(qa/2)

-where M is the mass of an atom, K is the spring constant, q is the phonon wave vector and a is the interatomic distance

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
6
Q

What are phonons?

A

-the normal modes of a collection of harmonic oscillators characterised by wavevectors k and angular frequencies ω, and have a dispersion relation given by;
ω = √[2K/M] * sin(qa/2)

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
7
Q

Energies of Phonons

A

-the same as the energies of the quantum harmonic oscillator:
En = (n + 1/2)*ℏω

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
8
Q

Distribution Function for Phonons

A

-phonons are bosons so are governed by the Bose-Einstein distribution function;
n(ω) = 1 / [exp(ℏω/kb*T) - 1]
-note that the chemical potential is missing from the numerator of the Boltzmann factor since bosons are not conserved

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
9
Q

Relationship Between Phonon Wavevector and Wavelength

A

q = 2π/λ

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
10
Q

Minimum and Maximum Phonon Wavelengths

A
  • there is no maximum phonon wavelength since it will be as big as the size of the sample of the metal
  • the minimum allowed wavelength is the distance between atoms ~3Å, this corresponds to maximum energy
How well did you know this?
1
Not at all
2
3
4
5
Perfectly
11
Q

Phonon Heat Capacity

Einstein

A
  • the first person to expain heat capacity due to lattic vibrations was Einstein
  • he modelled each atom as a harmonic oscillator independent from the others and calculated the occupation of each energy level using a Boltzmann factor and then summed over all levels
  • although this works at high temperatures predicting 3R, it predicts a low temperature heat capacity which does not agree to well with experiment
  • the problem with this method is that the atoms don’t vibrate independently but collectively
How well did you know this?
1
Not at all
2
3
4
5
Perfectly
12
Q

Number of States as a Function of Wavevector

A

-consider a linear chain with spacing L/2π = Na/2π
-and a sphere of radius q for the phonon wave vector
-multiply by three for the three polarisations of the phonons:
Ν(q) = q³V/2π²
-where Ν is greek letter Nu

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
13
Q

Debye Wavevector Equation

A

-starting with the number of states in terms of q:
Ν(q) = q³V/2π²
-but Ν=3N, where 3 is the number of degrees of translational freedom and N is the number of atoms
-taking qD to be the Debye wavevector, analogous to kf, we can write:
6π²n = qD³

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
14
Q

Alternative name for 3N

A

-3N, the number of translational degrees of freedom multiplied by the number of atoms, is also called the number of normal modes of the system

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
15
Q

Phonon Density of States Derivation

A

-start with the number of states in terms of q:
Ν(q) = q³V/2π²
-the velocity of sound is given by vs=ω/q, so:
Ν(q) = V/2π² * ω³/vs³
-to find the density of states, differentiate with respect to ω:
D(ω) = V3ω²/2π² * 1/vs³
-as for electrons the density of states is defined to be the number of states in the range ω -> ω+dω and is written:
D(ω)dω = V
3ω²/2π²vs³ dω

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
16
Q

Phonon Derivation of States

Formula

A

D(ω)dω = V 3ω²/2π²vs³ dω

-the integral of this is obviously equal to 3N

17
Q

Phonon Total Internal Energy

A

U(T) = ∫ ℏω D(ω) fb(ω,T) dω
-where the integral is taken between 0 and ωD
-after substitution:
U(T) = 3Vℏ/2π²vs³ * ∫ω³/[e^(ℏω/kbT)-1] dω
-where the integral is taken between 0 and ωD

18
Q

Phonon Heat Capacity

Derivation

A

C = d/dT U(T)
-sub in for U(T):
C = 3Vℏ/2π²vs³kbT² * ∫[e^(ℏω/kbT)ω^4]/[e^(ℏω/kbT)-1]² dω
-changing variable x=ℏω/kbT we can write:
C = 9Nkb(T/θD)³ *
∫[x^4
e^x]/[e^(x)-1]² dx

19
Q

Debye Temperature Formula

A

θD = ℏvs/kb * (6π²n)^(1/3)

20
Q

Phonon Heat Capacity at Low Temperatures

A

-at low temperatures (T<

21
Q

Phonon Heat Capacity at High Temperatures

A

-at high temperatures (T»θD), i.e. x<1 sp the integrand becomes ~x²:
C = 3R
-which is the Dulong-Petit Law

22
Q

Heat Capacity From Electrons and Phonons

A

C = γT + αT³

  • the linear term is the electron contribution and the cubic term is the phonon contribution
  • data is normally plotted as C/T against T² giving γ as the y intercept and α as the gradient
23
Q

What is the relationship between the velocity of sound and the Debye temperature

A

-velocity of sound is proportional to the Debye temperature