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Pressure of an Ideal Gas

Relates the pressure of an ideal gas to its temperature and volume, derived from the kinetic theory of gases.
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The statement of the theorem

Let S\mathcal{S} be a system of NN non-interacting particles of mass mm confined to a volume VV at temperature TT. The system's Hamiltonian is H=i=1Npi22m\mathcal{H} = \sum_{i=1}^{N} \frac{\vec{p}_i^2}{2m}. The pressure PP is defined by the average momentum flux tensor Π\langle \Pi \rangle exerted on the container walls. For an ideal gas, the equation of state is derived from the partition function ZZ: Z=1N!(Vh3)N(2πmkBTh2)3N/2Z = \frac{1}{N!}\left(\frac{V}{h^3}\right)^N \left(\frac{2\pi m k_B T}{h^2}\right)^{3N/2} where kBk_B is the Boltzmann constant and hh is Planck's constant. The internal energy UU is related to ZZ by U=(lnZβ)V,NU = -\left(\frac{\partial \ln Z}{\partial \beta}\right)_{V, N}, where β=1/(kBT)\beta = 1/(k_B T). By the equipartition theorem and the ideal gas law, the pressure PP is given by the thermodynamic relation: P=NkBTV=nRTVP = \frac{N k_B T}{V} = \frac{n R T}{V} where n=N/NAn = N/N_A is the number density and R=NAkBR = N_A k_B is the universal gas constant.
Source: Wikipedia