Ideal gas partition function: Difference between revisions
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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} + | :<math>H(p^N, r^N)= \sum_{i=1}^N \frac{|p_i |^2}{2m} + \Phi(r^N)</math> | ||
Thus we have | Thus we have | ||
:<math>Q_{NVT}=\frac{1}{N!}\frac{1}{h^{3N}}\int dp^N \exp \left[ - \frac{|p_i |^2}{2mk_B T}\right] | :<math>Q_{NVT}=\frac{1}{N!}\frac{1}{h^{3N}}\int dp^N \exp \left[ - \frac{|p_i |^2}{2mk_B T}\right] | ||
\int dr^N \exp \left[ - \frac{ | \int dr^N \exp \left[ - \frac{\Phi(r^N)} {k_B T}\right]</math> | ||
This separation is only possible if <math>V(r^N)</math> is independent of velocity (as is generally the case). | This separation is only possible if <math>V(r^N)</math> is independent of velocity (as is generally the case). | ||
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:<math>Q_{NVT}=\frac{1}{N!} \frac{1}{h^{3N}} \left( 2 \pi m k_B T\right)^{3N/2} | :<math>Q_{NVT}=\frac{1}{N!} \frac{1}{h^{3N}} \left( 2 \pi m k_B T\right)^{3N/2} | ||
\int dr^N \exp \left[ - \frac{ | \int dr^N \exp \left[ - \frac{\Phi(r^N)} {k_B T}\right]</math> | ||
The integral over positions is known as the ''configuration integral'', <math>Z_{NVT}</math> | The integral over positions is known as the ''configuration integral'', <math>Z_{NVT}</math> | ||
:<math>Z_{NVT}= \int dr^N \exp \left[ - \frac{ | :<math>Z_{NVT}= \int dr^N \exp \left[ - \frac{\Phi(r^N)} {k_B T}\right]</math> | ||
In an [[ideal gas]] there are no interactions between particles so <math> | In an [[ideal gas]] there are no interactions between particles so <math>\Phi(r^N)=0</math> | ||
Thus <math>\exp(- | Thus <math>\exp(-\Phi(r^N)/k_B T)=1</math> for every gas particle. | ||
The integral of 1 over the coordinates of each atom is equal to the volume so for ''N'' particles | 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 <math>V^N</math> where ''V'' is the volume. | the ''configuration integral'' is given by <math>V^N</math> where ''V'' is the volume. | ||
Revision as of 15:45, 26 June 2007
The canonical partition function, Q, for a system of N identical particles each of mass m is given by
When the particles are distinguishable then the factor N! disappears. Failed to parse (SVG (MathML can be enabled via browser plugin): Invalid response ("Math extension cannot connect to Restbase.") from server "https://wikimedia.org/api/rest_v1/":): {\displaystyle H(p^N, r^N)} 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
- Failed to parse (SVG (MathML can be enabled via browser plugin): Invalid response ("Math extension cannot connect to Restbase.") from server "https://wikimedia.org/api/rest_v1/":): {\displaystyle H(p^N, r^N)= \sum_{i=1}^N \frac{|p_i |^2}{2m} + \Phi(r^N)}
Thus we have
- Failed to parse (SVG (MathML can be enabled via browser plugin): Invalid response ("Math extension cannot connect to Restbase.") from server "https://wikimedia.org/api/rest_v1/":): {\displaystyle Q_{NVT}=\frac{1}{N!}\frac{1}{h^{3N}}\int dp^N \exp \left[ - \frac{|p_i |^2}{2mk_B T}\right] \int dr^N \exp \left[ - \frac{\Phi(r^N)} {k_B T}\right]}
This separation is only possible if Failed to parse (SVG (MathML can be enabled via browser plugin): Invalid response ("Math extension cannot connect to Restbase.") from server "https://wikimedia.org/api/rest_v1/":): {\displaystyle V(r^N)} is independent of velocity (as is generally the case). The momentum integral can be solved analytically:
Thus we have
- Failed to parse (SVG (MathML can be enabled via browser plugin): Invalid response ("Math extension cannot connect to Restbase.") from server "https://wikimedia.org/api/rest_v1/":): {\displaystyle Q_{NVT}=\frac{1}{N!} \frac{1}{h^{3N}} \left( 2 \pi m k_B T\right)^{3N/2} \int dr^N \exp \left[ - \frac{\Phi(r^N)} {k_B T}\right]}
The integral over positions is known as the configuration integral, Failed to parse (SVG (MathML can be enabled via browser plugin): Invalid response ("Math extension cannot connect to Restbase.") from server "https://wikimedia.org/api/rest_v1/":): {\displaystyle Z_{NVT}}
- Failed to parse (SVG (MathML can be enabled via browser plugin): Invalid response ("Math extension cannot connect to Restbase.") from server "https://wikimedia.org/api/rest_v1/":): {\displaystyle Z_{NVT}= \int dr^N \exp \left[ - \frac{\Phi(r^N)} {k_B T}\right]}
In an ideal gas there are no interactions between particles so Failed to parse (SVG (MathML can be enabled via browser plugin): Invalid response ("Math extension cannot connect to Restbase.") from server "https://wikimedia.org/api/rest_v1/":): {\displaystyle \Phi(r^N)=0} Thus Failed to parse (SVG (MathML can be enabled via browser plugin): Invalid response ("Math extension cannot connect to Restbase.") from server "https://wikimedia.org/api/rest_v1/":): {\displaystyle \exp(-\Phi(r^N)/k_B T)=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 Failed to parse (SVG (MathML can be enabled via browser plugin): Invalid response ("Math extension cannot connect to Restbase.") from server "https://wikimedia.org/api/rest_v1/":): {\displaystyle V^N} where V is the volume. Thus we have
- Failed to parse (SVG (MathML can be enabled via browser plugin): Invalid response ("Math extension cannot connect to Restbase.") from server "https://wikimedia.org/api/rest_v1/":): {\displaystyle Q_{NVT}=\frac{V^N}{N!}\left( \frac{2 \pi m k_B T}{h^2}\right)^{3N/2}}
If we define the de Broglie thermal wavelength as Failed to parse (SVG (MathML can be enabled via browser plugin): Invalid response ("Math extension cannot connect to Restbase.") from server "https://wikimedia.org/api/rest_v1/":): {\displaystyle \Lambda} where
- Failed to parse (SVG (MathML can be enabled via browser plugin): Invalid response ("Math extension cannot connect to Restbase.") from server "https://wikimedia.org/api/rest_v1/":): {\displaystyle \Lambda = \sqrt{h^2 / 2 \pi m k_B T}}
one arrives at
- Failed to parse (SVG (MathML can be enabled via browser plugin): Invalid response ("Math extension cannot connect to Restbase.") from server "https://wikimedia.org/api/rest_v1/":): {\displaystyle Q_{NVT}=\frac{1}{N!} \left( \frac{V}{\Lambda^{3}}\right)^N = \frac{q^N}{N!}}
where
- Failed to parse (SVG (MathML can be enabled via browser plugin): Invalid response ("Math extension cannot connect to Restbase.") from server "https://wikimedia.org/api/rest_v1/":): {\displaystyle q= \frac{V}{\Lambda^{3}}}
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.
- Failed to parse (SVG (MathML can be enabled via browser plugin): Invalid response ("Math extension cannot connect to Restbase.") from server "https://wikimedia.org/api/rest_v1/":): {\displaystyle Q_{NVT}=Q_{NVT}^{\rm ideal} ~Q_{NVT}^{\rm excess}}