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The classical configuration integral, more commonly called the partition function, and sometimes referred to as the configurational partition function[1], for a system with
particles is defined as follows:
-
![\displaystyle
Z_N
:=
\int\limits_V
\exp
\left[
- \beta U (x_1 , \cdots , x_N)
\right]
d^3 x_1 \cdots d^3 x_N](http://wpcontent.answers.com/math/c/8/9/c890ad5b350210cddf75bdac01aa2f3b.png)
(1)
where
is the volume enclosing the
particles,
a constant defined as
-

(2)
with
being the Boltzmann constant
the thermodynamic temperature
the potential energy of interparticle forces,
the positions in the 3-D space
of the
particles, with
and
the
coordinate of the
particle, and
an infinitesimal volume. The configuration integral has many applications from the ligand-receptor binding affinity in biochemistry to turbulence in fluid mechanics. For a detailed derivation, see the comprehensive article[2].
References
- ^ See, e.g., K. Lucas, Molecular Models for Fluids, Cambridge University Press, 2007 (p.270, Read from Google Book).
- ^ Vu-Quoc, Loc. "Configuration_integral_(statistical_mechanics)". http://clesm.mae.ufl.edu/wiki.pub/index.php/Configuration_integral_(statistical_mechanics). Retrieved 2008-10-12.
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