AME 60634 Int. Heat Trans. Non-Continuum Energy Transfer: Phonons D. B. Go Slide 1 AME 60634 Int. Heat Trans. The Crystal Lattice • The crystal lattice is the organization of atoms and/or molecules in a solid simple cubic body-centered cubic hexagonal a NaCl Ga4Ni3 tungsten carbide cst-www.nrl.navy.mil/lattice • The lattice constant ‘a’ is the distance between adjacent atoms in the basic structure (~ 4 Å) • The organization of the atoms is due to bonds between the atoms – Van der Waals (~0.01 eV), hydrogen (~kBT), covalent (~1-10 eV), ionic (~1-10 eV), metallic (~1-10 eV) D. B. Go Slide 2 AME 60634 Int. Heat Trans. The Crystal Lattice • Each electron in an atom has a particular potential energy – electrons inhabit quantized (discrete) energy states called orbitals – the potential energy V is related to the quantum state, charge, and distance from the nucleus -Z nl e 2 V ( r) = r • As the atoms come together to form a crystal structure, these potential energies overlap hybridize forming different, quantized energy levels bonds • This bond is not rigid but more like a spring potential energy D. B. Go Slide 3 AME 60634 Int. Heat Trans. Phonons Overview • A phonon is a quantized lattice vibration that transports energy across a solid • Phonon properties – frequency ω – energy ħω • ħ is the reduced Plank’s constant ħ = h/2π (h = 6.6261 10-34 J s) – wave vector (or wave number) k =2π/λ – phonon momentum = ħk – the dispersion relation relates the energy to the momentum ω = f(k) • Types of phonons - mode different wavelengths of propagation (wave vector) - polarization direction of vibration (transverse/longitudinal) - branches related to wavelength/energy of vibration (acoustic/optical) heat is conducted primarily in the acoustic branch • Phonons in different branches/polarizations interact with each other scattering D. B. Go Slide 4 AME 60634 Int. Heat Trans. Phonons – Energy Carriers • Because phonons are the energy carriers we can use them to determine the energy storage specific heat • We must first determine the dispersion relation which relates the energy of a phonon to the mode/wavevector • Consider 1-D chain of atoms approximate the potential energy in each bond as parabolic D. B. Go 1 2 u( x ) = gx 2 x = r - ro g º spring constant Slide 5 AME 60634 Int. Heat Trans. Phonon – Dispersion Relation - we can sum all the potential energies across the entire chain N 1 U = gå [ x na - x(n +1)a ] 2 n=1 2 - equation of motion for an atom located at xna is d 2 x na ¶U F=m == -g[2x na - x(n-1)a - x(n +1)a ] 2 dt ¶x na nearest neighbors - this is a 2nd order ODE for the position of an atom in the chain versus time: xna(t) - solution will be exponential of the form ( i( kna-wt )) form of standing wave x na ( t ) ~ e - plugging the standing wave solution into the equation of motion we can show that w( k) = 2 D. B. Go ( ) g sin ka 2 m dispersion relation for an acoustic phonon Slide 6 AME 60634 Int. Heat Trans. Phonon – Dispersion Relation - it can be shown using periodic boundary conditions that k= 2p l lmin = 2a smallest wave supported by atomic structure w( k) - this is the first Brillouin zone or primative cell that characterizes behavior for the entire crystal k - the speed at which the phonon propagates is given by the group velocity vg = dw g »a dk m speed of sound in a solid - at k = π/a, vg = 0 the atoms are vibrating out of phase with there neighbors D. B. Go Slide 7 AME 60634 Int. Heat Trans. D. B. Go Phonon – Real Dispersion Relation Slide 8 AME 60634 Int. Heat Trans. Phonon – Modes • As we have seen, we have a relation between energy (i.e., frequency) and the wave vector (i.e., wavelength) • However, only certain wave vectors k are supported by the atomic structure – these allowable wave vectors are the phonon modes a 1 0 kmax λmin = 2a p Mp = = a L λmax = 2L modes : k = D. B. Go p 2p 3p , L L , L ,..., (M -1)p L M-1 kmin = M p L note: k = Mπ/L is not included because it implies no atomic motion Slide 9 AME 60634 Int. Heat Trans. Phonon: Density of States • The density of states (DOS) of a system describes the number of states (N) at each energy level that are available to be occupied – simple view: think of an auditorium where each tier represents an energy level more available seats (N states) in this energy level fewer available seats (N states) in this energy level The density of states does not describe if a state is occupied only if the state exists occupation is determined statistically simple view: the density of states only describes the floorplan & number of seats not the number of tickets sold D. B. Go http://pcagreatperformances.org/info/merrill_seating_chart/ Slide 10 AME 60634 Int. Heat Trans. Phonon – Density of States w( k) more available modes k (N states) in this dω energy level fewer available modes k (N states) in this dω energy level k Density of States: D(w ) = 1 dN " dw chain rule D(w ) = 1 dN dk 1 dN 1 = " dk dw " dk v g For 1-D chain: modes (k) can be written as 1-D chain in k-space dk p = dN L D. B. Go Þ D (w ) = 1L 1 1 = L p vg p vg Slide 11 AME 60634 Int. Heat Trans. Phonon - Occupation The total energy of a single mode at a given wave vector k in a specific polarization (transverse/longitudinal) and branch (acoustic/optical) is given by the probability of occupation for that energy state æ 1ö E = ç n k, p,b + ÷ w k,p,b è 2ø This in general comes from the treatment of all phonons as a collection of single harmonic oscillators (spring/masses). However, the masses are atoms and therefore follow quantum mechanics and the energy levels are discrete (can be derived from a quantum treatment of the single harmonic oscillator). number of energy of phonons phonons Phonons are bosons and the number available is based on Bose-Einstein statistics n k, p,b = 1 æ w k, p,b ö expç ÷ -1 è kB T ø kB º Boltzmann constant =1.3807 ´10-23 J D. B. Go K Slide 12 AME 60634 Int. Heat Trans. Phonons – Occupation The thermodynamic probability can be determined from basic statistics but is dependant on the type of particle. Maxwell-Boltzmann statistics boltzons: gas distinguishable particles bosons: phonons indistinguishable particles fermions: electrons indistinguishable particles and limited occupancy (Pauli exclusion) D. B. Go Maxwell-Boltzmann distribution f (e) = Bose-Einstein statistics Fermi-Dirac statistics 1 æe - mö expç ÷ è kB T ø Bose-Einstein distribution f (e) = 1 æe - mö expç ÷ -1 k T è B ø Fermi-Dirac distribution f (e) = 1 æe - mö expç ÷ +1 k T è B ø Slide 13 AME 60634 Int. Heat Trans. Phonons – Specific Heat of a Crystal • Thus far we understand: – phonons are quantized vibrations – they have a certain energy, mode (wave vector), polarization (direction), branch (optical/acoustic) – they have a density of states which says the number of phonons at any given energy level is limited – the number of phonons (occupation) is governed by Bose-Einstein statistics • If we know how many phonons (statistics), how much energy for a phonon, how many at each energy level (density of states) total energy stored in the crystal! SPECIFIC HEAT æ 1ö U = å ò ç n p,b + ÷ w p,b D(w p,b )dw è 2ø p,b 0 w total energy in the crystal specific heat D. B. Go ¶U C= ¶T Slide 14 AME 60634 Int. Heat Trans. Phonons – Specific Heat • As should be obvious, for a real. 3-D crystal this is a very difficult analytical calculation – high temperature (Dulong and Petit): – low temperature: C ~ T 3 C = 3NkB • Einstein approximation – assume all phonon modes have the same energy good for optical phonons, but not acoustic phonons – gives good high temperature behavior • Debye approximation æT ö C ~ 234N A kB ç ÷ è TD ø 3 – assume dispersion curve ω(k) is linear – cuts of at “Debye temperature” – recovers high/low temperature behavior but not intermediate temperatures – not appropriate for optical phonons D. B. Go Slide 15 AME 60634 Int. Heat Trans. Phonons – Thermal Transport • Now that we understand, fundamentally, how thermal energy is stored in a crystal structure, we can begin to look at how thermal energy is transported conduction • We will use the kinetic theory approach to arrive at a relationship for thermal conductivity – valid for any energy carrier that behaves like a particle • Therefore, we will treat phonons as particles – think of each phonon as an energy packet moving along the crystal G. Chen D. B. Go Slide 16 AME 60634 Int. Heat Trans. Phonons – Thermal Conductivity • Recall from kinetic theory we can describe the heat flux as dNEv x 2 dNE 2 dU qx = -v xt = -v x t = -v x t dx dx dx • Leading to 1 2 dU dT dT qx = - v t = -k 3 dT dx dx Fourier’s Law 1 2 k = vg t C 3 D. B. Go what is the mean time between collisions? Slide 17 AME 60634 Int. Heat Trans. Phonons – Scattering Processes There are two basic scattering types collisions • elastic scattering (billiard balls) off boundaries, defects in the crystal structure, impurities, etc … – energy & momentum conserved td = 1 asrdefect v g L tb = vg • inelastic scattering between 3 or more different phonons – normal processes: energy & momentum conserved • do not impede phonon momentum directly – umklapp processes: energy conserved, but momentum is not – resulting phonon is out of 1st Brillouin zone and transformed into 1st Brillouin zone • impede phonon momentum dominate thermal conductivity æ qD ö tu » A expç ÷ wq D è gT ø T D. B. Go Slide 18 AME 60634 Int. Heat Trans. Phonons – Scattering Processes • Collision processes are combined using Matthiesen rule effective relaxation time 1 t = 1 td + 1 tb + 1 tu • Effective mean free path defined as = tv g Molecular description of thermal conductivity 1 1 k = vg2t C = vg C 3 3 When phonons are the dominant energy carrier: • increase conductivity by decreasing collisions (smaller size) • decrease conductivity by increasing collisions (more defects) D. B. Go Slide 19 AME 60634 Int. Heat Trans. Phonons – What We’ve Learned • Phonons are quantized lattice vibrations – store and transport thermal energy – primary energy carriers in insulators and semi-conductors (computers!) • Phonons are characterized by their – – – – energy wavelength (wave vector) polarization (direction) branch (optical/acoustic) acoustic phonons are the primary thermal energy carriers • Phonons have a statistical occupation, quantized (discrete) energy, and only limited numbers at each energy level – we can derive the specific heat! • We can treat phonons as particles and therefore determine the thermal conductivity based on kinetic theory D. B. Go Slide 20