Canonical ensemble

Variables:

• Number of Particles, $N$

• Volume, $V$

• Temperature, $T$

Partition Function

The classical partition function for a one-component system in a three-dimensional space, $Q_{NVT}$, is given by:

Failed to parse (Conversion error. Server ("https://wikimedia.org/api/rest_") reported: "Cannot get mml. Server problem."): {\displaystyle Q_{NVT}={\frac {V^{N}}{N!\Lambda ^{3N}}}\int d(R^{*})^{3N}\exp \left[-\beta U\left(V,(R^{*})^{3N}\right)\right]~~~~~~~~~~\left({\frac {V}{N\Lambda ^{3}}}\gg 1\right)}

where:

• $\Lambda$ is the de Broglie thermal wavelength (depends on the temperature)

• Failed to parse (Conversion error. Server ("https://wikimedia.org/api/rest_") reported: "Cannot get mml. Server problem."): {\displaystyle \beta :={\frac {1}{k_{B}T}}} , with $k_{B}$ being the Boltzmann constant, and T the temperature.

• $U$ is the potential energy, which depends on the coordinates of the particles (and on the interaction model)

• $\left(R^{*}\right)^{3N}$ represent the 3N position coordinates of the particles (reduced with the system size): i.e. $\int d(R^{*})^{3N}=1$

See also

• Ideal gas partition function