Stirling's approximation: Difference between revisions
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| N || N! (exact) || N! (Stirling) || Error (%) | | N || N! (exact) || N! (Stirling) || Error (%) | ||
|- | |- | ||
| | |3 || 6 || 5.83620959 || 2.81 | ||
|- | |- | ||
| | |4 || 24 || 23.5061751 || 2.10 | ||
|- | |- | ||
| | |5 || 120 || 118.019168 || 1.67 | ||
|- | |- | ||
| | |6 || 720 || 710.078185 || 1.40 | ||
|- | |- | ||
| | |7 || 5040 || 4980.39583 || 1.20 | ||
|- | |- | ||
|10 || 3628800 || 3598695.62 || | |8 || 40320 || 39902.3955 || 1.05 | ||
|- | |||
|9 || 362880|| 359536.873 || 0.93 | |||
|- | |||
|10 || 3628800 || 3598695.62 || 0.84 | |||
|} | |} | ||
As one usually deals with number of the order of the [[Avogadro constant ]](<math>10^{23}</math>) this formula is essentially exact. | As one usually deals with number of the order of the [[Avogadro constant ]](<math>10^{23}</math>) this formula is essentially exact. | ||
In [[Computer simulation techniques | computer simulations]] the number of atoms or molecules (N) is invariably greater than 100, where the | |||
percentage error is less than . | |||
==Applications in statistical mechanics== | ==Applications in statistical mechanics== | ||
*[[Ideal gas Helmholtz energy function]] | *[[Ideal gas Helmholtz energy function]] | ||
[[Category: Mathematics]] | [[Category: Mathematics]] | ||
Revision as of 13:08, 5 November 2008
James Stirling (1692-1770, Scotland)
- 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 \left.\ln N!\right. = \ln 1 + \ln 2 + \ln 3 + ... + \ln N = \sum_{k=1}^N \ln k .}
Because of Euler-MacLaurin formula
- 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 \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,
- 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 \ln N! \sim \int_1^N \ln x\,dx \sim N \ln N -N .}
after some further manipulation 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 N! = \sqrt{2 \pi N} \; N^{N} e^{-N} e^{\lambda_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 \frac{1}{12N+1} < \lambda_N < \frac{1}{12N}.}
For example:
| N | N! (exact) | N! (Stirling) | Error (%) |
| 3 | 6 | 5.83620959 | 2.81 |
| 4 | 24 | 23.5061751 | 2.10 |
| 5 | 120 | 118.019168 | 1.67 |
| 6 | 720 | 710.078185 | 1.40 |
| 7 | 5040 | 4980.39583 | 1.20 |
| 8 | 40320 | 39902.3955 | 1.05 |
| 9 | 362880 | 359536.873 | 0.93 |
| 10 | 3628800 | 3598695.62 | 0.84 |
As one usually deals with number of the order of the Avogadro 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 10^{23}} ) this formula is essentially exact. In computer simulations the number of atoms or molecules (N) is invariably greater than 100, where the percentage error is less than .