Hamiltonian fluid mechanics: Difference between revisions
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Take the simple example of a [[barotropic]], [[inviscid]] [[vorticity-free]] fluid. |
Take the simple example of a [[barotropic]], [[inviscid]] [[vorticity-free]] fluid. |
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Then, the conjugate fields are the [[mass density]] field ''ρ'' and the [[velocity potential]] ''φ''. The [[Poisson bracket]] is given by |
Then, the [[Conjugate variables|conjugate fields]] are the [[mass density]] field ''ρ'' and the [[velocity potential]] ''φ''. The [[Poisson bracket]] is given by |
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:<math>\{\varphi(\vec{x}),\rho(\vec{y})\}=\delta^d(\vec{x}-\vec{y})</math> |
:<math>\{\varphi(\vec{x}),\rho(\vec{y})\}=\delta^d(\vec{x}-\vec{y})</math> |
Revision as of 19:11, 8 September 2014
Hamiltonian fluid mechanics is the application of Hamiltonian methods to fluid mechanics. This formalism can only apply to nondissipative fluids.
Irrotational barotropic flow
Take the simple example of a barotropic, inviscid vorticity-free fluid.
Then, the conjugate fields are the mass density field ρ and the velocity potential φ. The Poisson bracket is given by
and the Hamiltonian by:
where e is the internal energy density, as a function of ρ. For this barotropic flow, the internal energy is related to the pressure p by:
where an apostrophe ('), denotes differentiation with respect to ρ.
This Hamiltonian structure gives rise to the following two equations of motion:
where is the velocity and is vorticity-free. The second equation leads to the Euler equations:
after exploiting the fact that the vorticity is zero:
See also
References
- R. Salmon (1988). "Hamiltonian Fluid Mechanics". Annual Review of Fluid Mechanics. 20: 225–256. Bibcode:1988AnRFM..20..225S. doi:10.1146/annurev.fl.20.010188.001301.
- T. G. Shepherd (1990). "Symmetries, conservation laws, and Hamiltonian structure in geophysical fluid dynamics". Advances in Geophysics. 32: 287–338. Bibcode:1990AdGeo..32..287S. doi:10.1016/S0065-2687(08)60429-X.