Thermodynamicsundergraduategraduate

Sackur-Tetrode Equation

Also known as: Absolute entropy of ideal gas · Quantum-corrected Boltzmann entropy

Entropy counts accessible microstates in units of h³ per degree of freedom; the 5/2 is the 3/2 kinetic + 1 from volume/particle indistinguishability.

S=NkB[ln(VN(4πmE3Nh2)3/2)+52]S = Nk_B\left[\ln\left(\frac{V}{N}\left(\frac{4\pi m E}{3Nh^2}\right)^{3/2}\right) + \frac{5}{2}\right]
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Phase-space visualisation: each particle shown as a dot in 2D momentum-position space. As T rises, the dots spread into a larger phase-space volume, illustrating S = k_B ln Ω.

Equivalent forms

S=NkB[ln(kBTP(2πmkBTh2)3/2)+52]S = Nk_B\left[\ln\left(\frac{k_B T}{P}\,\left(\frac{2\pi m k_B T}{h^2}\right)^{3/2}\right) + \frac{5}{2}\right]
SNkB=lnV/Nλth3+52,λth=h2πmkBT\frac{S}{Nk_B} = \ln\frac{V/N}{\lambda_{th}^3} + \frac{5}{2}, \quad \lambda_{th}=\frac{h}{\sqrt{2\pi m k_B T}}
The thermal de Broglie wavelength λ_th appears naturally: the classical regime is exactly when λ_th ≪ (V/N)^{1/3}.