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Luke's variational principle : ウィキペディア英語版
Luke's variational principle
In fluid dynamics, Luke's variational principle is a Lagrangian variational description of the motion of surface waves on a fluid with a free surface, under the action of gravity. This principle is named after J.C. Luke, who published it in 1967.〔
〕 This variational principle is for incompressible and inviscid potential flows, and is used to derive approximate wave models like the so-called mild-slope equation,〔
〕 or using the averaged Lagrangian approach for wave propagation in inhomogeneous media.〔

Luke's Lagrangian formulation can also be recast into a Hamiltonian formulation in terms of the surface elevation and velocity potential at the free surface.〔 Originally appeared in ''Zhurnal Prildadnoi Mekhaniki i Tekhnicheskoi Fiziki'' 9(2): 86–94, 1968.〕〔
〕〔
〕 This is often used when modelling the spectral density evolution of the free-surface in a sea state, sometimes called wave turbulence.
Both the Lagrangian and Hamiltonian formulations can be extended to include surface tension effects.
==Luke's Lagrangian==

Luke's Lagrangian formulation is for non-linear surface gravity waves on an—incompressible, irrotational and inviscidpotential flow.
The relevant ingredients, needed in order to describe this flow, are:
*''Φ''(''x'',''z'',''t'') is the velocity potential,
*''ρ'' is the fluid density,
*''g'' is the acceleration by the Earth's gravity,
*''x'' is the horizontal coordinate vector with components ''x'' and ''y'',
*''x'' and ''y'' are the horizontal coordinates,
*''z'' is the vertical coordinate,
*''t'' is time, and
*∇ is the horizontal gradient operator, so ∇''Φ'' is the horizontal flow velocity consisting of ∂''Φ''/∂''x'' and ∂''Φ''/∂''y'',
*''V''(''t'') is the time-dependent fluid domain with free surface.
The Lagrangian \mathcal, as given by Luke, is:
:
\mathcal =
-\int_^ \left\
+ \frac \left| \boldsymbol\Phi \right|^2
+ \frac \left( \frac \right)^2
+ g\, z
\right )\; \textx\; \texty\; \textz\; \right\}\; \textt.

From Bernoulli's principle, this Lagrangian can be seen to be the integral of the fluid pressure over the whole time-dependent fluid domain ''V''(''t''). This is in agreement with the variational principles for inviscid flow without a free surface, found by Harry Bateman.
Variation with respect to the velocity potential ''Φ''(''x'',''z'',''t'') and free-moving surfaces like ''z''=''η''(''x'',''t'') results in the Laplace equation for the potential in the fluid interior and all required boundary conditions: kinematic boundary conditions on all fluid boundaries and dynamic boundary conditions on free surfaces.〔
〕 This may also include moving wavemaker walls and ship motion.
For the case of a horizontally unbounded domain with the free fluid surface at ''z''=''η''(''x'',''t'') and a fixed bed at ''z''=−''h''(''x''), Luke's variational principle results in the Lagrangian:
:
\mathcal =
-\, \int_^ \iint
\left\^ \rho\,
\left(
\frac
+\, \frac \left| \boldsymbol\Phi \right|^2
+\, \frac \left( \frac \right)^2
\right
)\; \textz\;
+\, \frac\, \rho\, g\, \eta^2
\right\}\; \text\boldsymbol\; \textt.
The bed-level term proportional to ''h''2 in the potential energy has been neglected, since it is a constant and does not contribute in the variations.
Below, Luke's variational principle is used to arrive at the flow equations for non-linear surface gravity waves on a potential flow.

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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