Phonons Flashcards
Simple 1D Model of Atoms
Description
-atoms with mass M separated by a distance a and connected by springs with spring constant K
Simple 1D Model of Atoms
Equation of Motion
-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’’ = -ω²un
Simple 1D Model of Atoms
Difference Equation for Displacements
-sub un’’ = -ω²un into the equation of motion:
-Mω²un = K(un+1 + un-1 - 2un)
-therefore we can expect travelling wave solutions of the form:
u±1 = ue^(inqa)*e^(±iqa)
-where a is the atomic separation distance and q is the phonon wave vector
Simple 1D Model of Atoms
Derivation of the Dispersion Relation for Phonons
-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)
Phonon Dispersion Relation
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
What are phonons?
-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)
Energies of Phonons
-the same as the energies of the quantum harmonic oscillator:
En = (n + 1/2)*ℏω
Distribution Function for Phonons
-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
Relationship Between Phonon Wavevector and Wavelength
q = 2π/λ
Minimum and Maximum Phonon Wavelengths
- 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
Phonon Heat Capacity
Einstein
- 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
Number of States as a Function of Wavevector
-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
Debye Wavevector Equation
-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
Alternative name for 3N
-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
Phonon Density of States Derivation
-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 = V3ω²/2π²vs³ dω