1. Hyperbolic Heat Equation 1-D BTE assume Integrate over velocity space assuming that  is an averaged relaxation time (4.63a) (4.64) or

2. In 3-D Maxwell-Cattaneo equation Energy equation without convection Cattaneo equation

3. Without internal heat generation Damped wave equation Decay in amplitude: For an insulator: hyperbolic equation speed of thermal wave

4. Hyperbolic heat equation : valid strictly when t p >  semi-infinite solid under a constant heat flux at the surface propagation speed : v tw pulse wavefront: x 1 = v tw t 1, x 2 = v tw t 2 short pulselong pulse In the case of a short pulse, temperature pulse propagates and its height decays by dissipating its energy to the medium as it travels.

5.  Entropy Local energy balance Local entropy balance Entropy production rate Hyperbolic heat equation sometimes predicts a negative entropy generation. (Energy transferred from lower-temp. region to higher- temp. region) Negative entropy generation is not a violation of the 2nd law of thermodynamics Because the concept of “temperature” in the hyperbolic heat equation cannot be interpreted in the conventional sense due to the lack of local thermal equilibrium

6. Dual-Phase-Lag Model Finite buildup time after a temperature gradient is imposed on the specimen for the onset of a heat flow: on the order of the relaxation time  Lag between temperature rise and heat flow In analogy with the stress-strain relationships of viscoelastic materials with instantaneous elasticity When → Cattaneo eq. electrons → lattice phonons → temperature rise

7. By assuming that retardation time : effective conductivity (heat diffusion) : elastic conductivity (hyperbolic heat)

8. dual-phase-lag model First order approximation : intrinsic thermal properties of the bulk material

9. The requirement may cause. The heat flux depends not only on the history of the temperature gradient but also on the history of the time derivative of the temperature gradient. → Cattaneo eq. When → Fourier law

10.  Solid-fluid heat exchanger immersed long thin solid rods in a fluid inside a sealed pipe insulated from the outside rod diameter d, number of rods N inner diameter of pipe D total surface area per unit length total cross-sectional area of the rods total cross-sectional area of the fluid average convection heat transfer coefficient h

11. assume Due to the initial temperature difference between the rod and the fluid, a local equilibrium is not established at any x inside the pipe until after a sufficiently long time.

12. Two-Temperature Model electrons → electron-phonon interaction → phonons Under the assumption that the electron and phonon systems are each at their own local equilibrium, but not in mutual equilibrium (valid when t >  ) e : electron, s : phonon C : volumetric heat capacity =  c p G : electron-phonon coupling constant

13. Assume the the lattice temperature is near or above the Debye temperature so that electron-electron scattering and electron-defects scattering are insignificant compared with electron-phonon scattering. (5.25) (5.55b)  eq : thermal conductivity at or(5.10)

14.  q : not the same as the relaxation time  due to collision Thermalization time: thermal time constant for the electron system to reach an equilibrium with the phonon system

15. Heat Conduction Across Layered Structures Equation of Phonon Radiative Transfer (EPRT) S 0 : electron-phonon scattering  Phonon BTE in 1-D system or

16. phonon Intensity: summation over the three phonon polarizations phonon intensity under non-equilibrium distribution function : energy transfer rate in a direction from a unit area, per unit frequency, per unit solid angle + forward direction (  > 0 ) - forward direction (  < 0 ) T1T1 T2T2  

17. Equation of Phonon Radiative Transfer (EPRT) Radiative Transfer Equation (RTE) optical thickness of the medium neglecting scattering acoustical thickness of the mediumcorresponds to

18. Equilibrium intensity, Bose-Einstein statistics analogy to blackbody intensity

19. integrating over all frequency → total intensity for all 3 phonon modes : Phonon Stefan-Boltzmann constant v a : average phase velocity of the 2 transverse and 1 longitudinal phonon modes

20. At temperature higher than Debye temperature high frequency limit because the shortest wavelength of the lattice wave should be on the order of atomic distances, the lattice constants energy flux at phonon equilibrium: I * invariant with direction particle flux

21. energy carried by a phonon = energy flux / particle flux energy density = energy carried by a phonon X number of phonons per unit volume At low temperature At high temperature Dulong-Petit law:

22.  radiative equilibrium total quantities

23. T1T1 T2T2   Solution to EPRT steady state  Two-flux method in planar structures boundary conditions: gray medium, diffuse and gray walls

24.  Solutions to EPRT  Heat Flux (spectral)

25. For diffuse surface total heat flux

26. Heat flux at very low temperature Heat flux between blackbodies with small T difference Thermal conductivity

27. acoustically thick limit

28.  Effective Conductivity of the Film

29.  Thermal Resistance Network effective thermal conductivity of the whole layered structure

30. Internal thermal resistance with Fourier’s law Thermal resistance at the interface Thermal resistance at the boundaries

31. Thermal Boundary Resistance (TBR) THTH 123 TLTL  Acoustic Mismatch Model specular reflection of phonons similar to geometric optics no scattering or diffusion  Diffuse Mismatch Model diffusive reflection of phonons no information (except for energy) retained after a scattering  Thermal Contact Resistance due to incomplete contact between two materials thermal resistance between two bodies, usually with very rough surfaces,  rms > 0.5  m  Thermal Boundary Resistance due to the difference in acoustic properties of adjacent materials

32.  Acoustic Mismatch Model (AMM) For longitudinal phonon modes with linear dispersion in a Debye crystal (equilibrium, isotropic, perfect contact) transmission coefficient Snell’s law

33. Let : hemispherical transmission

34. Snell’s law critical angle:  C

35. For longitudinal phonon modes with linear dispersion in a Debye crystal (equilibrium, isotropic, perfect contact)

37. In the low temperature limit, For all 3 phonon modes Thermal boundary resistance

38. TBR by AMM is proportional to T -3. AMM assumes perfect specular reflection which is valid only when the characteristic wavelength of the phonons is much larger than the surface roughness. (  mp >>  rms ) → DMM (Diffuse Mismatch Model) When the temperature difference is small, a : lattice constant

39.  Diffusion Mismatch Model (DMM) In DMM, all phonons striking the interface are scattered once, and are emitted into the adjoining substances elastically (  = 0 ) with a probability proportional to the phonon density of states (DOS) in the respective substances. Distribution of the emitted phonons is independent of the incident phonon, whether it is from side 1 or 2, longitudinal or transverse. integration over the solid angle

40. at low temperature by DMM (  12 ) with the assumption

41. Measured Data TBR between indium and sapphire[2]. X, normal indium; ● super conducting indium. Data B are for roughened sapphire surface. A and C are for smooth sapphire surfaces with different indium thicknesses. AMM predicts a flat line at 20.4 cm 2 K 4 /W