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Hamiltonian fluid mechanics : ウィキペディア英語版
Hamiltonian fluid mechanics
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
:()=\delta^d(\vec-\vec)
and the Hamiltonian by:
:\mathcal=\int \mathrm^d x \left( \frac\rho(\nabla \varphi)^2 +e(\rho) \right),
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:
:e'' = \fracp',
where an apostrophe ('), denotes differentiation with respect to ''ρ''.
This Hamiltonian structure gives rise to the following two equations of motion:
:
\begin
\frac&=+\frac= -\nabla \cdot(\rho\vec),
\\
\frac&=-\frac=-\frac\vec\cdot\vec-e',
\end

where \vec\ \stackrel\ \nabla \varphi is the velocity and is vorticity-free. The second equation leads to the Euler equations:
:\frac + (\vec\cdot\nabla) \vec = -e''\nabla\rho = -\frac\nabla
after exploiting the fact that the vorticity is zero:
:\nabla \times\vec=\vec.
As fluid dynamics is described by non-canonical dynamics, which possess an infinite amount of Casimir invariants, an alternative formulation of Hamiltonian formulation of fluid dynamics can be introduced through the use of Nambu mechanics

抄文引用元・出典: フリー百科事典『 ウィキペディア(Wikipedia)
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