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MINDMAP 4 - Coggle Diagram
MINDMAP 4
THERMAL PROPERTIES I
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classical result
- In general, Cp is always have larger value than Cv
- But when temperature is approaches zero, Cp is almost the same with Cv
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- At high temperature, Cv is independent with temperature
- At low temperature, in insulator, the heat capacity drops and approaches zero as T^3
- Otherwise in conductors, the heat capacity will be constant
At room temperature, 3Nk = 3R per mole = 25 J mol−1 deg−1. (DULONG-PETIT LAW)
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THERMAL PROPERTIES II
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Einsein Model
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he assumed Planck’s (1990) quantization rule for each oscillator (vibrating oscillators (atoms) in a solid have quantized energies)
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heat capacity
- z = the number of atom in a unit formula
- So, CV approaches 0 when T appreaches 0 is true
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Debye Model
- Atoms are considered as harmonic oscillators that produce elastic waves with varying frequencies from ω = 0 to ωmax.
- Atoms are considered as harmonic oscillators that produce elastic waves with varying frequencies from ω = 0 to ωmax.
- 3N normal modes (patterns) of oscillations
- The Debye model successfully describes the temperature dependence of the heat capacity not only at high temperatures but also at low temperatures
- T3 Debye law is known for the contribution of the phonon to the heat capacity at low temperatures
The relations between the energy of a phonon E, the angular frequency ω and the wave vector q are:
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In the 3 dimensional reciprocal space, the volume for each allowed wave vector q is
Since there is a cut-off wave vector qD=ωD/vs, all the modes are confined within a sphere with radius qD.
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At high temperature, T>>TD
value of x is very small throughout the range of the integral. The classical value of Dulong-Petit obtained
At low temperature, T<<TD
- Only long wavelength acoustic modes are thermally excited
- The energy of those short wavelength modes are too high to be populated significantly at low temperatures
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The approximation of isotropic continuum in the Debye model is appropriate for the phonos in the acoustic branch and the single frequency in the Einstein model suitable for the phonons in the optical branch
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