Gibbs distribution: Difference between revisions

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(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...)
 
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
[[Kelvin scale]] one divides by the [[Boltzmann constant]] <math>k_B</math>).
[[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 15:01, 14 February 2008

Ref 1 Eq. 3.37:

G(N)=1Z(N)exp(−H(N)Θ)

where N is the number of particles, H is the Hamiltonian of the system and Θ is the temperature (to convert Θ into the more familiar kelvin scale one divides by the Boltzmann constant kB). The constant Z(N) is found from the normalization condition (Ref. 1 Eq. 3.38)

1Γ(N)(0)Z(N)∫Vexp(−U1,...,NΘ)d3r1...d3rN∫−∞∞exp(−K(N)Θ)d3p1...d3pN=1

which leads to (Ref. 1 Eq. 3.40)

Z(N)=1VNQ(N)

where (Ref. 1 Eq. 3.41)

Q(N)=∫Vexp(−U1,...,NΘ)d3r1...d3rN

this is the statistical integral

Z≡∑ne−En/T=tre−H|T

where H is the Hamiltonian of the system.

References[edit]

  1. G. A. Martynov "Fundamental Theory of Liquids. Method of Distribution Functions", Adam Hilger (out of print)