Ideal gas partition function: Difference between revisions
No edit summary |
Carl McBride (talk | contribs) No edit summary |
||
Line 47: | Line 47: | ||
one arrives at | one arrives at | ||
:<math>Q_{NVT}=\frac{1}{N!} \left( \frac{V}{\Lambda^{3}}\right)^N</math> | :<math>Q_{NVT}=\frac{1}{N!} \left( \frac{V}{\Lambda^{3}}\right)^N = \frac{q^N}{N!}</math> | ||
where | |||
:<math>q= \frac{V}{\Lambda^{3}}</math> | |||
is the single particle translational partition function. | |||
Revision as of 16:11, 21 May 2007
Canonical ensemble partition function, Q, for a system of N identical particles each of mass m
When the particles are distinguishable then the factor N! disappears. is the Hamiltonian (Sir William Rowan Hamilton 1805-1865 Ireland) corresponding to the total energy of the system. H is a function of the 3N positions and 3N momenta of the particles in the system. The Hamiltonian can be written as the sum of the kinetic and the potential energies of the system as follows
Thus we have
This separation is only possible if is independent of velocity (as is generally the case). The momentum integral can be solved analytically:
Thus we have
The integral over positions is known as the configuration integral,
In an ideal gas there are no interactions between particles so Thus for every gas particle. The integral of 1 over the coordinates of each atom is equal to the volume so for N particles the configuration integral is given by where V is the volume. Thus we have
If we define the de Broglie thermal wavelength as where
one arrives at
where
is the single particle translational partition function.
Thus one can now write the partition function for a real system can be built up from
the contribution of the ideal system (the momenta) and a contribution due to
particle interactions, i.e.