Blundell Thermal Physics · Problem 24.2

Phonons

Physics — Statistical Mechanics · debye-internal-energy-substitution

Problem

Show that eqn 24.22 can be rewritten as U=98NAℏωD+9RTxD3∫0xDx3 dxex−1,(24.35)U = \frac{9}{8}N_A\hbar\omega_{\rm D} + \frac{9RT}{x_{\rm D}^3}\int_0^{x_{\rm D}}\frac{x^3\,{\rm d}x}{e^x - 1}, \tag{24.35} by making the substitution x=ℏβωx = \hbar\beta\omega, and hence xD=ℏβωDx_{\rm D} = \hbar\beta\omega_{\rm D}.
Intuitive explanation

The Debye model expresses internal energy as an integral over all phonon frequencies, weighted by their thermal occupation. By introducing the dimensionless variable x=ℏβωx = \hbar\beta\omega (where β=1/kBT\beta = 1/k_BT), you transform the frequency integral into a universal form that separates the zero-point energy (the 98\frac{9}{8} term) from the temperature-dependent contribution. The key is recognizing that this substitution converts the Debye cutoff frequency ωD\omega_D into the dimensionless Debye temperature parameter xDx_D, making the integral dimensionally consistent and revealing how thermal energy scales with temperature through the 1/(ex−1)1/(e^x-1) Bose–Einstein factor.

Intuitive explanation

The Debye model expresses internal energy as an integral over all phonon frequencies, weighted by their thermal occupation. By introducing the dimensionless variable x=ℏβωx = \hbar\beta\omega (where β=1/kBT\beta = 1/k_BT), you transform the frequency integral into a universal form that separates the zero-point energy (the 98\frac{9}{8} term) from the temperature-dependent contribution. The key is recognizing that this substitution converts the Debye cutoff frequency ωD\omega_D into the dimensionless Debye temperature parameter xDx_D, making the integral dimensionally consistent and revealing how thermal energy scales with temperature through the 1/(ex−1)1/(e^x-1) Bose–Einstein factor.

Related theory

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