Cole equation of state: Difference between revisions

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m (Added a couple of internal links)
m (Added link to the adiabatic index)
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:<math>c^2 = \frac{\gamma B}{\rho_0}. </math>
:<math>c^2 = \frac{\gamma B}{\rho_0}. </math>


where <math>\gamma</math> is the [[Heat capacity#Adiabatic index | adiabatic index]].
Therefore, if <math>B=100 \rho_0 v^2 / \gamma</math>, the relative density fluctuations
Therefore, if <math>B=100 \rho_0 v^2 / \gamma</math>, the relative density fluctuations
will be of about 0.01.
will be of about 0.01.

Revision as of 15:02, 23 May 2012

The Cole equation of state [1][2] can be written, when atmospheric pressure is negligible, has the form

In it, is a reference density around which the density varies is an exponent and is a pressure parameter.

Usually, the equation is used to model a nearly incompressible system. In this case, the exponent is often set to a value of 7, and is large, in the following sense. The fluctuations of the density are related to the speed of sound as

where is the largest velocity, and is the speed of sound (the ratio is Mach's number). The speed of sound can be seen to be

where is the adiabatic index. Therefore, if , the relative density fluctuations will be of about 0.01.

If the fluctuations in the density are indeed small, the equation of state may be rewritten thus:


References

  1. R. H. Cole "Underwater Explosions", Princeton University Press (1948) ISBN 9780691069227
  2. G. K. Batchelor "An introduction to fluid mechanics", Cambridge University Press (1974) ISBN 0521663962