Ideal gas partition function: Difference between revisions

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m (Hamiltonian now denoted as H (capital), to avoid confusion with h (Plank's constants))
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for a system of ''N'' identical particles each of mass ''m''
for a system of ''N'' identical particles each of mass ''m''


:<math>Q_{NVT}=\frac{1}{N!}\frac{1}{h^{3N}}\int\int dp^N dr^N \exp \left[ - \frac{h(p^N, r^N)}{k_B T}\right]</math>
:<math>Q_{NVT}=\frac{1}{N!}\frac{1}{h^{3N}}\int\int dp^N dr^N \exp \left[ - \frac{H(p^N, r^N)}{k_B T}\right]</math>


When the particles are distinguishable then the factor ''N!'' disappears. <math>h(p^N, r^N)</math> is the Hamiltonian
When the particles are distinguishable then the factor ''N!'' disappears. <math>H(p^N, r^N)</math> is the Hamiltonian


(Sir William Rowan Hamilton 1805-1865 Ireland)
(Sir William Rowan Hamilton 1805-1865 Ireland)
corresponding to the total energy of the system.
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.
''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
The Hamiltonian can be written as the sum of the kinetic and the potential energies of the system as follows


:<math>h(p^N, r^N)= \sum_{i=1}^N \frac{|p_i |^2}{2m} + V(r^N)</math>
:<math>H(p^N, r^N)= \sum_{i=1}^N \frac{|p_i |^2}{2m} + V(r^N)</math>


Thus we have  
Thus we have  

Revision as of 09:37, 23 February 2007

Canonical ensemble partition function, Q, for a system of N identical particles each of mass m

QNVT=1N!1h3N∫∫dpNdrNexp[−H(pN,rN)kBT]

When the particles are distinguishable then the factor N! disappears. H(pN,rN) 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

H(pN,rN)=∑i=1N|pi|22m+V(rN)

Thus we have

QNVT=1N!1h3N∫dpNexp[−|pi|22mkBT]∫drNexp[−V(rN)kBT]

This separation is only possible if V(rN) is independent of velocity (as is generally the case). The momentum integral can be solved analytically:

∫dpNexp[−|p|22mkBT]=(2πmkbT)3N/2

Thus we have

QNVT=1N!1h3N(2πmkBT)3N/2∫drNexp[−V(rN)kBT]


The integral over positions is known as the configuration integral, ZNVT

ZNVT=∫drNexp[−V(rN)kBT]

In an ideal gas there are no interactions between particles so V(rN)=0 Thus exp(−V(rN)/kBT)=1 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 VN where V is the volume. Thus we have

QNVT=VNN!(2πmkBTh2)3N/2

If we define the de Broglie thermal wavelength as Λ where

Λ=h2/2πmkBT

one arrives at

QNVT=1N!(VΛ3)N


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.

QNVT=QNVTidealQNVTexcess