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Difference between revisions of "Stirling's approximation"

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:<math>\ln N! \sim \int_1^N \ln x\,dx \sim N \ln N -N .</math>
 
:<math>\ln N! \sim \int_1^N \ln x\,dx \sim N \ln N -N .</math>
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==Applications in statistical mechanics==
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*[[Ideal gas Helmholtz energy function]]
 
[[Category: Mathematics]]
 
[[Category: Mathematics]]

Revision as of 12:03, 7 July 2008

James Stirling (1692-1770, Scotland)

\left.\ln N!\right. = \ln 1 + \ln 2 + \ln 3 + ... + \ln N = \sum_{k=1}^N \ln k .

Because of Euler-MacLaurin formula

\sum_{k=1}^N \ln k=\int_1^N \ln x\,dx+\sum_{k=1}^p\frac{B_{2k}}{2k(2k-1)}\left(\frac{1}{n^{2k-1}}-1\right)+R ,

where B1 = −1/2, B2 = 1/6, B3 = 0, B4 = −1/30, B5 = 0, B6 = 1/42, B7 = 0, B8 = −1/30, ... are the Bernoulli numbers, and R is an error term which is normally small for suitable values of p.

Then, for large N,

\ln N! \sim \int_1^N \ln x\,dx \sim N \ln N -N .

Applications in statistical mechanics