Thermal Properties - Phonons II - continued
Outline
From previous lectures:
Typical Crystal Structures
Diffraction, Fourier Analysis, and the Reciprocal Lattice
Crystal binding, elastic waves
Vibration waves in crystals: dispersion curves, quantization
Last Lecture: Thermal properties, first part
Planck disptribution, Bose-Einstein Statistics
Density of states, Internal energy, Heat capacity
Normal mode enumeration -- # k points = number of cells
Debye Model - T3 law at low T
Einstein Model
Anharmonicity - treated cursorily
Anharmonicity is responsible for:
Scattering of phonons
Thermal expansion
Gruneisen Constant
Thermal conductivity
Basic law: j = - K dT/dx, where K = thermal conductivity. This describes
flow of energy (power per unit area) in the direction of minus the thermal gradient
For particles (gas of ordinary molecules or phonons),
K = (1/3) C v L, where C = heat capacity, v = mean velocity, L = mean
free path
Essential point: particles scatter to come to local thermal eqilibrium
Heat flow in a solid involves transport of energy by phonons
Phonons scatter and come to local thermal
equilibrium in each local region (scattering due to anharmonicity and to defects)
Formulas in lecture for low temperature( K~T3)
and high temperature ( K~T-1)
Maximum at intermediate temperature
Special role of Umklapp scattering (G unequal 0)
Additional topics (extra material not required)
Recent results with isotopically pure crystals
Nanostructures - atomic wires, nanotubes, etc.
Summary of Part I of course
Email clarification questions and corrections to
rmartin@uiuc.edu
Email questions on solving problems to
xin2@.uiuc.edu