Gibbs distribution: Difference between revisions
Carl McBride (talk | contribs) (New page: Ref 1 Eq. 3.37: :<math>\mathcal{G}_{(N)} = \frac{1}{Z_{(N)}} \exp \left( - \frac{H_{(N)}}{\Theta}\right)</math> where <math>N</math> is the number of particles, <math>H</math> is the [[H...) |
Carl McBride (talk | contribs) m (Changed Kelvin to kelvin) |
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where <math>N</math> is the number of particles, <math>H</math> is the [[Hamiltonian]] of the system | where <math>N</math> is the number of particles, <math>H</math> is the [[Hamiltonian]] of the system | ||
and <math>\Theta</math> is the temperature (to convert <math>\Theta</math> into the more familiar | and <math>\Theta</math> is the temperature (to convert <math>\Theta</math> into the more familiar | ||
[[ | [[temperature |kelvin scale]] one divides by the [[Boltzmann constant]] <math>k_B</math>). | ||
The constant <math>Z_{(N)}</math> is found from the normalization condition (Ref. 1 Eq. 3.38) | The constant <math>Z_{(N)}</math> is found from the normalization condition (Ref. 1 Eq. 3.38) | ||
Latest revision as of 14:01, 14 February 2008
Ref 1 Eq. 3.37:
where is the number of particles, is the Hamiltonian of the system and is the temperature (to convert into the more familiar kelvin scale one divides by the Boltzmann constant 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 k_B} ). The constant 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_{(N)}} is found from the normalization condition (Ref. 1 Eq. 3.38)
- 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 \frac{1}{\Gamma_{(N)}^{(0)}Z_{(N)}} \int_V \exp \left( - \frac{U_1,..., _N}{\Theta}\right) ~{\rm d}^3r_1 ... {\rm d}^3r_N \int_{- \infty}^{\infty} \exp \left( - \frac{K_{(N)}}{\Theta}\right) ~{\rm d}^3p_1 ... {\rm d}^3p_N =1}
which leads to (Ref. 1 Eq. 3.40)
- 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_{(N)}= \frac{1}{V^N} Q_{(N)}}
where (Ref. 1 Eq. 3.41)
this is the statistical 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 \equiv \sum_n e^{-E_n/T}= {\rm tr} ~ e^{-H|T}}
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 H} is the Hamiltonian of the system.
References[edit]
- G. A. Martynov "Fundamental Theory of Liquids. Method of Distribution Functions", Adam Hilger (out of print)