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Derivation

Debye Model of Phonon Heat Capacity

D-242 Home PU-302 Threads matter · waves · energy · chance Depends on Bose-Einstein and Fermi-Dirac Occupation Numbers, Planck's Law from the Photon Gas
Statement

Treating the normal modes of a crystal as a gas of independent quantized harmonic oscillators (phonons) with a linear dispersion \( \omega = v_s k \) and a single cutoff frequency \( \omega_D \) fixed by requiring exactly \( 3N \) modes, the Debye model gives the lattice internal energy \( U(T) \) and hence the molar heat capacity \( C_V = 9 N k_B \left(\dfrac{T}{\Theta_D}\right)^{3} \displaystyle\int_0^{\Theta_D/T} \dfrac{x^4 e^x}{(e^x-1)^2}\,dx \), which reduces to the Dulong–Petit value \( 3 N k_B \) for \( T \gg \Theta_D \) and to the \( T^3 \) law \( C_V = \dfrac{12\pi^4}{5} N k_B \left(\dfrac{T}{\Theta_D}\right)^{3} \) for \( T \ll \Theta_D \).

Why it matters

The Dulong–Petit rule \( C_V = 3 N k_B \) is a triumph of classical equipartition, but experiment shows the heat capacity of every insulating solid collapses to zero as \( T \to 0 \). The Einstein model captured the fall but decayed exponentially, too fast. Debye's insight — that the low-energy modes are long-wavelength sound waves with arbitrarily small frequency — produces the correct universal \( T^3 \) approach to zero, one of the cleanest confirmations of the quantization of lattice vibrations.

The same phonon-gas machinery, with a Debye cutoff replacing the infinite photon spectrum, underlies thermal conductivity, the third law of thermodynamics for solids, and the entropy budget that sets equations of state at low temperature. Debye's \( \Theta_D \) is a single material parameter that collapses the heat-capacity curves of chemically unrelated solids onto one universal shape.

Assumptions
Harmonic lattice.If atomic potentials are anharmonic the modes couple, phonons acquire finite lifetimes and thermal expansion appears; \( C_V \) picks up corrections and \( C_p \neq C_V \).
Linear, isotropic dispersion \( \omega = v_s k \) with one sound speed.Real crystals have three acoustic branches with different, direction-dependent speeds and curvature; dropping isotropy means \( g(\omega) \) is no longer \( \propto \omega^2 \) except in the \( \omega \to 0 \) limit.
A single sharp cutoff \( \omega_D \) fixed by mode counting.The true vibrational spectrum has van Hove singularities and a jagged upper edge; replacing it by a sharp \( \omega_D \) is exact only for the total mode count and the \( \omega\to 0 \) behaviour, so mid-temperature \( C_V \) is only approximate.
Three polarizations per wavevector, all treated with the same \( v_s \).Longitudinal and transverse branches actually have different speeds; using one effective \( v_s \) (a harmonic-type average) is what makes \( \Theta_D \) a single number rather than three.
Phonon number unconserved; Bose–Einstein occupation with \( \mu = 0 \).If a chemical potential were needed the occupation would shift; but lattice quanta are freely created and destroyed, so \( \mu = 0 \) and each mode carries \( \langle n \rangle = (e^{\hbar\omega/k_BT}-1)^{-1} \).
Derivation
1
\[ \omega = v_s k, \qquad \mathbf{k}=\frac{2\pi}{L}(n_x,n_y,n_z) \]
Model each normal mode as a plane wave in a cubic box of side \( L \), volume \( V=L^3 \), with periodic boundary conditions quantizing \( \mathbf{k} \). Linear dispersion is the long-wavelength (elastic-continuum) limit of any acoustic branch. A
2
\[ dN_{\text{modes}} = 3 \cdot \frac{V}{(2\pi)^3}\, 4\pi k^2\, dk \]
Count allowed \( \mathbf{k} \)-points: each occupies volume \( (2\pi/L)^3 \) of \( k \)-space, so the density of points is \( V/(2\pi)^3 \); multiply by the spherical shell \( 4\pi k^2 dk \) and by the factor \( 3 \) for the three polarizations. A
3
\[ g(\omega)\,d\omega = \frac{3V}{2\pi^2}\,\frac{\omega^2}{v_s^3}\,d\omega \]
Change variable with \( k=\omega/v_s \), \( dk=d\omega/v_s \). This defines the Debye density of states \( g(\omega)=\dfrac{3V\omega^2}{2\pi^2 v_s^3} \), valid rigorously only as \( \omega\to 0 \) but extended to all \( \omega \) in the model. B
4
\[ \int_0^{\omega_D} g(\omega)\,d\omega = 3N \;\Longrightarrow\; \frac{3V}{2\pi^2 v_s^3}\cdot\frac{\omega_D^3}{3}=3N \]
A crystal of \( N \) atoms has exactly \( 3N \) mechanical degrees of freedom, hence \( 3N \) normal modes. Fixing the total under \( g(\omega) \) pins the cutoff. This is the single physical input that closes the model. B
5
\[ \omega_D = v_s\left(6\pi^2\,\frac{N}{V}\right)^{1/3}, \qquad \Theta_D \equiv \frac{\hbar\omega_D}{k_B} \]
Solve step 4 for \( \omega_D \); the number density \( N/V \) enters through the cube root. Define the Debye temperature \( \Theta_D \) as the energy scale \( \hbar\omega_D \) in kelvin — the model's one adjustable parameter. A
6
\[ U = \int_0^{\omega_D} \hbar\omega\,\langle n(\omega)\rangle\, g(\omega)\,d\omega,\qquad \langle n\rangle=\frac{1}{e^{\hbar\omega/k_BT}-1} \]
Each mode is a quantized oscillator; measuring energy from the zero-point level, its thermal energy is \( \hbar\omega\langle n\rangle \) with the Bose–Einstein occupation at \( \mu=0 \) (prior result: quantum-occupation-statistics-bose-fermi). Sum over modes via \( g(\omega) \). B
7
\[ U = \frac{3V\hbar}{2\pi^2 v_s^3}\int_0^{\omega_D}\frac{\omega^3}{e^{\hbar\omega/k_BT}-1}\,d\omega \]
Insert \( g(\omega) \) from step 3. Note the integrand \( \omega^3/(e^{\hbar\omega/k_BT}-1) \) is exactly the Planck form (prior result: planck-blackbody-law-from-photon-gas), differing from radiation only by three polarizations instead of two and by the finite upper limit \( \omega_D \). B
8
\[ x \equiv \frac{\hbar\omega}{k_BT},\qquad U = 9N k_B T \left(\frac{T}{\Theta_D}\right)^{3}\int_0^{\Theta_D/T}\frac{x^3}{e^x-1}\,dx \]
Substitute the dimensionless \( x \); the upper limit becomes \( \hbar\omega_D/k_BT=\Theta_D/T \). Using \( \omega_D^3=6\pi^2 N v_s^3/V \) from step 5 to absorb the prefactor gives the compact universal form — every material collapses onto one curve in \( T/\Theta_D \). C
9
\[ C_V=\left(\frac{\partial U}{\partial T}\right)_V = 9N k_B\left(\frac{T}{\Theta_D}\right)^{3}\int_0^{\Theta_D/T}\frac{x^4 e^x}{(e^x-1)^2}\,dx \]
Differentiate step 8 with respect to \( T \). Both the explicit \( T \)-prefactors and the \( T \)-dependent upper limit contribute; the boundary term from the limit cancels against a piece of the prefactor derivative, leaving the single integral shown. C
10
\[ T\ll\Theta_D:\quad \int_0^{\Theta_D/T}\!\to\int_0^{\infty}\frac{x^4 e^x}{(e^x-1)^2}\,dx=\frac{4\pi^4}{15} \]
At low \( T \) the upper limit \( \Theta_D/T\to\infty \); the integrand decays exponentially so extending to \( \infty \) costs only exponentially small error. The definite integral is a standard result (equal to \( 4\zeta(4)\,\Gamma(4)/... \), evaluating to \( 4\pi^4/15 \)). C
11
\[ C_V=\frac{12\pi^4}{5}\,N k_B\left(\frac{T}{\Theta_D}\right)^{3}\quad(T\ll\Theta_D) \]
Multiply step 10's constant \( \tfrac{4\pi^4}{15} \) by the prefactor \( 9Nk_B(T/\Theta_D)^3 \). The \( T^3 \) law emerges purely from the \( \omega^2 \) density of states of long-wavelength acoustic modes. B
12
\[ T\gg\Theta_D:\quad \frac{x^4 e^x}{(e^x-1)^2}\to x^2,\quad \int_0^{\Theta_D/T} x^2\,dx=\frac{1}{3}\left(\frac{\Theta_D}{T}\right)^3 \]
For \( T\gg\Theta_D \) all \( x\le\Theta_D/T \) are small; expand \( e^x\approx 1+x \) so the integrand \( \to x^2 \). Integrating and inserting into step 9, the \( (T/\Theta_D)^3 \) prefactor cancels the \( (\Theta_D/T)^3 \). B
13
\[ C_V \to 3N k_B\quad(T\gg\Theta_D) \]
The cancellation leaves the classical Dulong–Petit constant: \( 3N \) oscillators each carrying \( k_B \) of heat capacity, exactly equipartition's \( 2\times\tfrac12 k_B \) per mode. Quantum statistics reproduces the classical limit when \( k_BT \) exceeds every mode energy. A
Result
\[ C_V = 9N k_B\left(\frac{T}{\Theta_D}\right)^{3}\int_0^{\Theta_D/T}\frac{x^4 e^x}{(e^x-1)^2}\,dx \;\xrightarrow[T\ll\Theta_D]{}\; \frac{12\pi^4}{5}N k_B\left(\frac{T}{\Theta_D}\right)^{3},\quad \xrightarrow[T\gg\Theta_D]{}\; 3N k_B \]

Reading. The heat capacity of an insulating solid is a single universal function of \( T/\Theta_D \). At high temperature every one of the \( 3N \) modes is thermally excited and carries \( k_B \), giving Dulong–Petit. As \( T \) falls below \( \Theta_D \), modes with \( \hbar\omega > k_BT \) freeze out; because the surviving long-wavelength modes have a density of states \( \propto \omega^2 \), the number of active modes scales as \( T^3 \) and so does \( C_V \). The Debye temperature \( \Theta_D \) marks the crossover: stiff, light solids (diamond, \( \Theta_D\approx 2230\,\mathrm{K} \)) stay "quantum-frozen" to high \( T \); soft, heavy ones (lead, \( \Theta_D\approx 105\,\mathrm{K} \)) reach the classical plateau near room temperature.

Units check. \( N k_B \) has units \( \mathrm{J\,K^{-1}} \) (heat capacity). The prefactor \( 9(T/\Theta_D)^3 \) and the integral are dimensionless since \( x=\hbar\omega/k_BT \) is dimensionless. In the low-\( T \) form, \( (T/\Theta_D)^3 \) is dimensionless and \( \tfrac{12\pi^4}{5} \) is a pure number, leaving \( \mathrm{J\,K^{-1}} \). The Dulong–Petit limit \( 3Nk_B \) is manifestly \( \mathrm{J\,K^{-1}} \); per mole \( N=N_A \) gives \( 3R \approx 24.9\,\mathrm{J\,mol^{-1}K^{-1}} \).

Limiting cases
  • \( T\to 0 \): \( C_V\to \tfrac{12\pi^4}{5}Nk_B (T/\Theta_D)^3 \to 0 \) — the correct third-law behaviour; entropy \( S=\int C_V\,dT/T \) also vanishes as \( T^3 \).
  • \( T\to\infty \): \( C_V\to 3Nk_B \), the Dulong–Petit plateau, independent of \( \Theta_D \) and of quantum mechanics.
  • \( T=\Theta_D \): the crossover region; \( C_V\approx 0.95\times 3Nk_B \), already \( 95\% \) of classical, so \( \Theta_D \) roughly marks "nearly classical".
  • \( \Theta_D\to 0 \) (very soft solid): classical everywhere above absolute zero; the \( T^3 \) window shrinks toward \( T=0 \).
  • Two dimensions: the same argument with \( g(\omega)\propto\omega \) gives a \( T^2 \) low-temperature law; in \( d \) dimensions \( C_V\propto T^d \).
  • Metals: add the electronic linear term \( \gamma T \); at low \( T \), \( C_V = \gamma T + \beta T^3 \), and a plot of \( C_V/T \) versus \( T^2 \) is a straight line whose slope gives \( \Theta_D \).
Breaks when
  • Metals at very low temperature. The conduction electrons contribute a heat capacity \( \gamma T \) that dominates the \( \beta T^3 \) lattice term below a few kelvin; the pure Debye \( T^3 \) law then fails and one must add the Sommerfeld electronic term.
  • Optical branches and real dispersion. Debye's single acoustic-like spectrum ignores optical phonons and dispersion curvature. In solids with a basis (e.g. NaCl, diamond) the mid-temperature \( C_V \) departs from the universal curve; \( \Theta_D \) fitted at low \( T \) differs from that fitted near \( \Theta_D \), so \( \Theta_D(T) \) drifts.
  • Strong anharmonicity / near melting. Above \( \Theta_D \), thermal expansion and mode–mode coupling make \( C_p-C_V \) non-negligible and push \( C_V \) above \( 3Nk_B \); the harmonic phonon-gas picture breaks down.
  • Magnetic, glassy, or low-dimensional solids. Amorphous solids show an anomalous \( \sim T \) term from two-level tunnelling systems; magnetic solids add a spin-wave \( T^{3/2} \) contribution — neither is in the Debye model.
Failure modes
  • Using two polarizations instead of three. Copying the photon result (transverse only) drops the longitudinal branch; the factor becomes \( 2 \) not \( 3 \) and Dulong–Petit comes out wrong. Phonons have one longitudinal plus two transverse modes.
  • Forgetting the finite upper limit at high \( T \). Extending the integral to \( \infty \) is only legal at low \( T \). At high \( T \) the cutoff is essential — it is what caps \( C_V \) at \( 3Nk_B \) instead of diverging.
  • Including zero-point energy in \( \langle n\rangle \). The occupation is \( 1/(e^{\hbar\omega/k_BT}-1) \), not \( \tfrac12 + 1/(e^{...}-1) \), for heat capacity — the constant \( \tfrac12\hbar\omega \) is \( T \)-independent and drops out of \( \partial U/\partial T \).
  • Mislabelling the low-\( T \) constant. Writing \( \int_0^\infty x^4 e^x/(e^x-1)^2 dx \) as \( \pi^4/15 \) (the \( x^3/(e^x-1) \) value) instead of \( 4\pi^4/15 \). They differ by a factor \( 4 \); the correct coefficient is \( 12\pi^4/5 \), not \( 3\pi^4/5 \).
  • Confusing \( C_V \) and \( C_p \). The derivation gives \( C_V \); comparing directly to measured \( C_p \) without the \( C_p-C_V=TV\alpha^2/\kappa_T \) correction misfits \( \Theta_D \) at higher \( T \).
  • Treating \( \Theta_D \) as fundamental. \( \Theta_D \) is a fitted effective parameter, not a fixed material constant; the "best" value depends on which temperature window is fitted.
Discussion

The heart of the Debye result is that heat capacity counts thermally accessible modes. A mode contributes its full classical \( k_B \) only when \( k_BT \gtrsim \hbar\omega \); colder than that it is "frozen", exponentially unlikely to hold even one quantum. What makes solids different from the Einstein model is that there is no lowest nonzero frequency: acoustic modes run continuously down to \( \omega\to 0 \). No matter how cold, some modes are always active, so \( C_V \) never falls exponentially — it falls as a power law set by how the mode count grows from zero, namely \( g(\omega)\propto\omega^2 \), giving \( T^3 \).

The kinship with blackbody radiation is exact and illuminating. A photon gas and a phonon gas are both massless Bose gases with linear dispersion and \( \mu=0 \); the energy density integrand is identical. The only structural differences are that phonons have three polarizations (photons two) and, crucially, a finite spectrum cut off at \( \omega_D \) because a lattice has a shortest meaningful wavelength (\( \sim \) interatomic spacing) whereas the electromagnetic vacuum has none. Remove the cutoff and the phonon energy would grow as \( T^4 \) forever, the Stefan–Boltzmann law — indeed at low \( T \), before the cutoff is felt, the phonon energy does scale as \( T^4 \), which is exactly why its derivative \( C_V\propto T^3 \).

The Debye temperature is a compact fingerprint of a solid's stiffness and mass: \( \Theta_D\propto v_s (N/V)^{1/3} \), and since \( v_s\sim\sqrt{\text{stiffness}/\text{density}} \), hard light solids have high \( \Theta_D \) and soft heavy ones low. It sets not only the heat-capacity crossover but roughly the temperature above which classical transport and equipartition become good approximations, and it appears in the Lindemann melting criterion and the Bloch–Grüneisen resistivity of metals.

At a deeper level the \( T^3 \) law is a statement about the low-energy fixed point of the elastic continuum: at long wavelengths every crystal, whatever its microscopic detail, looks like an isotropic elastic medium with three linearly dispersing Goldstone modes of broken translational symmetry. The universality of the \( T^3 \) coefficient (fixed entirely by the sound speeds through \( \Theta_D \)) is a hydrodynamic, symmetry-protected result — the sharp cutoff and the density of states above it are model artefacts that never enter the \( T\to 0 \) limit. This is why the low-temperature Debye law is quantitatively reliable even though the model's mid-spectrum \( g(\omega) \) is crude.

Common misconceptions. Debye did not assume all atoms vibrate at one frequency (that is Einstein); he assumed a continuum of frequencies up to a cutoff. The \( T^3 \) law is not caused by the cutoff — it comes from the \( \omega\to 0 \) modes, and the cutoff is irrelevant at low \( T \). And \( \Theta_D \) is not a phase-transition temperature: nothing special happens to the solid at \( T=\Theta_D \); it is merely where the heat capacity is about \( 95\% \) of its classical value.

Worked examples
1
\[ \text{Copper: } \Theta_D=343\,\mathrm{K}. \text{ Find the molar lattice } C_V \text{ at } T=30\,\mathrm{K}. \]
Since \( T=30\,\mathrm{K}\ll\Theta_D=343\,\mathrm{K} \) (ratio \( 0.087 \)), the \( T^3 \) law applies. Use \( C_V=\tfrac{12\pi^4}{5}R\,(T/\Theta_D)^3 \) with \( R=8.314\,\mathrm{J\,mol^{-1}K^{-1}} \). A
\[ C_V=\frac{12\pi^4}{5}R\left(\frac{T}{\Theta_D}\right)^3 \]
Symbolic form first; \( \tfrac{12\pi^4}{5}=233.78 \). A
\[ \left(\frac{30}{343}\right)^3=(0.08746)^3=6.69\times10^{-4} \]
Evaluate the ratio cubed. A
\[ C_V=233.78\times 8.314\times 6.69\times10^{-4}\,\mathrm{J\,mol^{-1}K^{-1}} \]
Insert numbers. A
\[ C_V \approx 1.30\ \mathrm{J\,mol^{-1}\,K^{-1}} \]

Reading. This is only \( 1.30/24.9\approx 5\% \) of the Dulong–Petit value \( 3R=24.9\,\mathrm{J\,mol^{-1}K^{-1}} \) — most modes are frozen at \( 30\,\mathrm{K} \). (This ignores the electronic \( \gamma T \) term, which for copper adds only \( \sim 0.02\,\mathrm{J\,mol^{-1}K^{-1}} \) at \( 30\,\mathrm{K} \), a \( 1\% \) correction.)

Units check. \( R \) carries \( \mathrm{J\,mol^{-1}K^{-1}} \); the ratio cubed and \( \tfrac{12\pi^4}{5} \) are dimensionless, so the answer is \( \mathrm{J\,mol^{-1}K^{-1}} \).

2
\[ \text{Aluminium: mass density } \rho=2700\,\mathrm{kg\,m^{-3}},\ M=27.0\,\mathrm{g\,mol^{-1}},\ \bar v_s=5100\,\mathrm{m\,s^{-1}}. \text{ Estimate } \Theta_D. \]
Use \( \Theta_D=\dfrac{\hbar v_s}{k_B}\left(6\pi^2\,\dfrac{N}{V}\right)^{1/3} \) with the atomic number density \( N/V=\rho N_A/M \). B
\[ \frac{N}{V}=\frac{\rho N_A}{M}=\frac{2700\times 6.022\times10^{23}}{27.0\times10^{-3}}\,\mathrm{m^{-3}} \]
Convert molar mass to \( \mathrm{kg\,mol^{-1}} \): \( M=0.0270\,\mathrm{kg\,mol^{-1}} \). A
\[ \frac{N}{V}=6.02\times10^{28}\,\mathrm{m^{-3}} \]
Number density of atoms. A
\[ \left(6\pi^2\,\frac{N}{V}\right)^{1/3}=\left(59.22\times 6.02\times10^{28}\right)^{1/3}=\left(3.566\times10^{30}\right)^{1/3}=1.528\times10^{10}\,\mathrm{m^{-1}} \]
This is \( k_D=\omega_D/v_s \), the Debye wavevector. B
\[ \Theta_D=\frac{\hbar v_s k_D}{k_B}=\frac{1.055\times10^{-34}\times 5100\times 1.528\times10^{10}}{1.381\times10^{-23}}\,\mathrm{K} \]
Assemble; \( \hbar=1.055\times10^{-34}\,\mathrm{J\,s} \), \( k_B=1.381\times10^{-23}\,\mathrm{J\,K^{-1}} \). A
\[ \Theta_D \approx 595\ \mathrm{K} \]

Reading. The elastic-continuum estimate (\( \sim 595\,\mathrm{K} \)) overshoots the calorimetric value for aluminium (\( \approx 428\,\mathrm{K} \)) by about \( 40\% \) — expected, since a single averaged \( v_s \) and the sharp-cutoff approximation are crude; using the proper harmonic average of longitudinal and transverse speeds brings it much closer.

Units check. \( k_D \) has units \( \mathrm{m^{-1}} \); \( \hbar v_s k_D \) is \( \mathrm{J\,s}\cdot\mathrm{m\,s^{-1}}\cdot\mathrm{m^{-1}}=\mathrm{J} \); dividing by \( k_B\ (\mathrm{J\,K^{-1}}) \) gives \( \mathrm{K} \).

Problems
  1. A solid has \( \Theta_D=200\,\mathrm{K} \). By what factor does its lattice heat capacity change when the temperature is doubled from \( 10\,\mathrm{K} \) to \( 20\,\mathrm{K} \)?
    SolutionBoth temperatures satisfy \( T\ll\Theta_D \), so \( C_V\propto T^3 \). Doubling \( T \) multiplies \( C_V \) by \( 2^3=8 \). Numerically, at \( 10\,\mathrm{K} \): \( C_V=233.78\times 8.314\times(10/200)^3=233.78\times8.314\times1.25\times10^{-4}=0.243\,\mathrm{J\,mol^{-1}K^{-1}} \); at \( 20\,\mathrm{K} \): \( 0.243\times 8=1.94\,\mathrm{J\,mol^{-1}K^{-1}} \). Factor \( =8 \).
  2. Show that the phonon internal energy at low temperature scales as \( T^4 \), and relate its coefficient to the \( C_V \) coefficient.
    SolutionAt \( T\ll\Theta_D \), \( U=9Nk_BT(T/\Theta_D)^3\int_0^\infty x^3/(e^x-1)\,dx \). The integral is \( \pi^4/15 \), so \( U=9Nk_B\,\dfrac{\pi^4}{15}\dfrac{T^4}{\Theta_D^3}=\dfrac{3\pi^4}{5}\dfrac{Nk_B T^4}{\Theta_D^3} \). Then \( C_V=\partial U/\partial T=\dfrac{12\pi^4}{5}\dfrac{Nk_B T^3}{\Theta_D^3} \), consistent with the boxed low-\( T \) law. The factor \( 4 \) from differentiating \( T^4 \) turns the \( 3 \) into \( 12 \).
  3. For a metal, low-temperature data give \( C_V/T = \gamma + \beta T^2 \) with \( \gamma=0.70\,\mathrm{mJ\,mol^{-1}K^{-2}} \) and \( \beta=0.048\,\mathrm{mJ\,mol^{-1}K^{-4}} \). Find \( \Theta_D \).
    SolutionThe lattice term is \( \beta T^3 \) with \( \beta=\dfrac{12\pi^4}{5}\dfrac{R}{\Theta_D^3} \) per mole. Solve \( \Theta_D=\left(\dfrac{12\pi^4 R}{5\beta}\right)^{1/3} \). With \( R=8.314\,\mathrm{J\,mol^{-1}K^{-1}} \) and \( \beta=4.8\times10^{-5}\,\mathrm{J\,mol^{-1}K^{-4}} \): \( \dfrac{12\pi^4\times8.314}{5\times4.8\times10^{-5}}=\dfrac{233.78\times8.314}{4.8\times10^{-5}}=4.05\times10^{7} \). Cube root: \( \Theta_D=(4.05\times10^{7})^{1/3}\approx 344\,\mathrm{K} \) (this is essentially copper).
  4. At what temperature, as a fraction of \( \Theta_D \), does the exact Debye \( C_V \) reach \( 90\% \) of the Dulong–Petit value? Estimate using the high-\( T \) expansion \( C_V\approx 3Nk_B\left[1-\tfrac{1}{20}(\Theta_D/T)^2\right] \).
    SolutionSet \( 1-\tfrac{1}{20}(\Theta_D/T)^2=0.90 \Rightarrow (\Theta_D/T)^2=0.10\times20=2.0 \Rightarrow \Theta_D/T=1.414 \Rightarrow T=\Theta_D/1.414=0.707\,\Theta_D \). So \( C_V \) is at \( 90\% \) of Dulong–Petit near \( T\approx 0.71\,\Theta_D \). (The exact numerical answer is close, \( T\approx 0.70\,\Theta_D \), confirming the leading correction is adequate here.)
  5. Diamond has \( \Theta_D\approx 2230\,\mathrm{K} \) and lead \( \Theta_D\approx 105\,\mathrm{K} \). Compare their molar lattice heat capacities at \( T=300\,\mathrm{K} \).
    SolutionLead: \( T/\Theta_D=300/105=2.86\gg1 \), so \( C_V\approx 3R=24.9\,\mathrm{J\,mol^{-1}K^{-1}} \) (fully classical). Diamond: \( T/\Theta_D=300/2230=0.135\ll1 \), so use \( T^3 \): \( C_V=233.78\times8.314\times(0.1345)^3=233.78\times8.314\times2.43\times10^{-3}=4.72\,\mathrm{J\,mol^{-1}K^{-1}} \) — the \( T^3 \) formula overestimates here since \( 0.135 \) is not deeply in the low-\( T \) regime; the true value is \( \approx 6\,\mathrm{J\,mol^{-1}K^{-1}} \). Either way diamond sits far below Dulong–Petit at room temperature while lead is already there, because diamond is stiff and light (huge \( \Theta_D \)) whereas lead is soft and heavy.