Notes: • Reminder, Exam: Tues, Oct 13. § § § In class. Covers through ch. 5 Open book = Kittel only. • HW 4: Can turn in next Thursday, Oct. 8. (I will have solutions ready.) Quantized Modes, shown last time: − β!ω ⎡1 e k ,ν E = ∑ !ωk ,ν ⎢ + − β!ω k ,ν 2 1 − e k ,ν ⎣ ⎤ ⎡1 ⎤ = ! ω + n ⎥ ∑ k ,ν ⎢ kν ⎥ 2 ⎣ ⎦ ⎦ k ,ν nk ,ν = 1 e β!ω k ,ν −1 • Planck formula, sum over lattice normal modes kT << !ω : E ≈ !ωk ,ν e kT >> !ω : E ≈ kT − β!ω k ,ν For each mode; except doesn’t work for lowest acoustic modes; Also omitted zero-point term. for each mode: Classical result. Quantized Modes, shown last time: − β!ω ⎡1 e k ,ν E = ∑ !ωk ,ν ⎢ + − β!ω k ,ν 2 1 − e k ,ν ⎣ ⎤ ⎡1 ⎤ = ! ω + n ⎥ ∑ k ,ν ⎢ kν ⎥ 2 ⎣ ⎦ ⎦ k ,ν nk ,ν = 1 e β!ω k ,ν −1 • Planck formula, sum over lattice normal modes kT << !ω : E ≈ !ωk ,ν e − β!ω k ,ν For each mode; except doesn’t work for lowest acoustic modes; Also omitted zero-point term. Debye model works very well at low T. ω ≅ kc Specific heat ~ T3 kT >> !ω : E ≈ kT for each mode: Classical result. Dulong-Petit law (as expected by correspondence principle). 3N total modes: CV = 3Nk B / V includes basis Specific Heat (Debye model): 1 ω ⎡ ⎤ E = ∑ ω k,ν ⎢ β ω k,ν = D( ω )d ω β ω ⎥⎦ ∫ e −1 e −1 ⎣ k,ν D(ω)/V ∂ C= ∂T ωD ∫ 0 Debye model showed last time. ω D = c 3 6π 2 n ≡ c 3 6π 2 N / V 3ω 2 ω dω 3kB4T 3 = 2 3 3 2 3 β ω 2π c e −1 2π c kT << !ω : ∫ 0 T x 4 dx e x T3 = 9kB n 3 x 2 (e −1) ΘD ΘD ∫ 0 T x 4 dx e x (e x −1)2 ∞ x 4 dxe x 4π 4 1 / T → ∞; ∫ x = 2 (e − 1) 15 0 kT >> !ω : ΘD CV = 3Nk B / V C = (12 / 5)π 4 nk BT 3 / Θ3D ≡ βT 3 classical limit, also easy to show. Specific Heat, Phonon notes: 3 T C = 9k B n 3 ΘD ΘD (Debye) ∫ 0 T x 4 dxe x (e x − 1) 2 • Normally at low temperatures two terms observed, phonons + metallic electrons (for non-magnets). C ≡ βT 3 + γT • Phonons “elementary excitations in crystal vacuum ”. • Zero-point contribution small; detectable. • Einstein vs. Debye: Atoms as independent SHO’s (Einstein) applies in some cases (optical modes) • Scattering by phonons: often is the most important electrical resistivity contribution. Crystal Momentum: o “Crystal momentum” is k-vector we have been using ! ! (K-vector in text). (Momentum: p = "k ) o Crystal potential mixes states with k, k ± G . o Result: k can only be specified ± G. “Folding” process brings k ± G states together. Thus we only need to define k in a single Brillouin zone. Free-space translation QM result [Tr! , H ] = 0 [T , H ] = 0 ! R Discrete translation ! pr! = constant of motion ! crystal k = constant of motion Crystal Momentum: o Crystal momentum: k-vector folded with states k ± G. ! ! ! ! Laue condition k − k ′ ≡ q = G ! ! ! ! 3 A ∝ ∫ d r n(r ) exp i[k − k ′] ⋅ r ( ) vol Lattice symmetry; Fourier components have wave-vectors G ! crystal k = conserved o Crystal potential mixes states with k, k ± G . ! ! ! U (r ) = U (r + R) ! ! ! ! ψ k (r ) = ∑G! CG ei ( k +G )⋅r Bloch theorem – later chapters. Anharmonic lattice effects: ► Real vibrational potential not precisely quadratic; most cases can be treated as perturbation. Results: • Thermal expansion as higher vibrational states become populated. • Phonon states not stationary states; finite lifetime. • Leads to “phonon-phonon scattering”: energy and crystal momentum conserved. Anharmonic lattice effects: Neutron scattering: • Neutron energy vs. k comparable to phonon (& magnetic) excitations • Used to observe both elastic and inelastic scattering. Neutron scattering: Atomic displacements Elastic scattering attenuation measured this way – This vs. T – appendix A; example ReO3 Debye-Waller Factor. (Rodriguez et al., J Appl Phys 2009)