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Positive linear stratified energy and diffusion

Statement

Let I⊆R be a nonempty open interval, assume the Axiom of Countable Choice ACω, and use the periodic domain T3=R3/(2πZ)3 with Lebesgue measure λ3 on Q3=[0,2π]3, where dx=dλ3(x) and the time-space integral is iterated with the spatial integral first. Let f∈R, N>0, and ν,κ≥0 be constants. Suppose u,b are continuously differentiable in time and space with continuous second spatial derivatives, and π has continuous first spatial derivatives; all fields are 2π-periodic and satisfy

ut+fe3×u+∇π=be3+νΔu,∇⋅u=0,bt+N2u3=κΔb.

Define the positive energy per reference density

E(t):=12∫Q3(∣u(t,x)∣2+b(t,x)2N2) dx.

Then for every t0<t1 in I,

E(t1)−E(t0)=−∫t0t1∫Q3(ν∣∇u∣2+κN2∣∇b∣2) dx dt.

Thus the inviscid model conserves E, and the stated nonnegative diffusion coefficients make it nonincreasing. Here N>0 fixes the positive buoyancy-frequency convention; the weight 1/N2 is positive for every nonzero real N, while the displayed functional is undefined at N=0. This is an exact identity conditional on the displayed smooth linear Boussinesq equations; it is not a nonlinear or compressible stability theorem. A discrete analogue requires a skew Coriolis operator and compatible pressure/divergence pairing in the actual discretization; no claim is made for arbitrary schemes.

Statement references

Equation family and pointwise regularity: Rotating stratified and shallow-water equation families.

Continuous functions on closed rectangles are Riemann integrable: Every continuous function on a closed nondegenerate rectangle in Rm is Riemann integrable.

Under ACω, bounded Borel Riemann integrands on finite-dimensional boxes have the same Lebesgue and Riemann integrals: Borel Darboux integrands in finite dimension.

Riemann integration over products of rectangles and equality with iterated integrals: Riemann--Fubini on product rectangles, with lower and upper section integrals and content-zero exceptional sections.

Newton–Leibniz for a continuous endpoint function with an integrable interior derivative: Newton–Leibniz needs only continuity on [a,b], differentiability on (a,b), and a Riemann-integrable extension of the interior derivative.

Under ACω, bounded Riemann integrable functions on closed intervals are Lebesgue integrable with the same integral: A bounded Riemann integrable function on a closed bounded interval is Lebesgue measurable and has the same integral.

Linearity of the multidimensional Riemann integral: Linearity, monotonicity, the absolute-value estimate and coordinate-slice additivity for the Riemann integral in Rm.

Geoffrey K. Vallis, Fluid Dynamics of the Atmosphere and Ocean, §1.6.2–1.6.3, pp. 15–17: full lecture notes, PDF.

Facts & Assumptions

Given: I⊆R is nonempty and open; the Axiom of Countable Choice ACω; u,b,π are classical and 2π-periodic in each spatial coordinate; f∈R, N>0, and ν,κ≥0; the displayed equations hold pointwise.

[F1]

Rotating stratified and shallow-water equation families: the stratified branch on T3 is ut+fe3×u+∇π=be3+νΔu, ∇⋅u=0, and bt+N2u3=κΔb, with constant f∈R, N>0, and ν,κ≥0.

[F2]

Rotating stratified and shallow-water equation families: for a scalar field q, ∇q=(∂x1q,∂x2q,∂x3q); for a vector field w, ∇⋅w=∑j∂xjwj, Δw is componentwise, ∣w∣2=∑jwj2, and ∣∇w∣2=∑i,j(∂xjwi)2; e3×w=(−w2,w1,0).

[A1]

The fields satisfy these equations with the regularity in the statement. The energy density, its time derivative, and the dissipation integrand below are continuous on each compact time interval times Q3. At each fixed time, the pressure and every spatial flux derivative below are continuous on Q3; no continuity in time of the pressure itself is assumed.

[A2]

Countable Choice ACω means that every N-indexed family of nonempty sets has a choice function; it is used for the cited Lebesgue-measure and Riemann-to-Lebesgue comparison results (The Axiom of Countable Choice (ACω)).

[L1]

Every continuous real function on a closed nondegenerate rectangle in Rm, m≥1, is Riemann integrable (Every continuous function on a closed nondegenerate rectangle in Rm is Riemann integrable).

[L2]

Assuming ACω, every bounded Borel Riemann-integrable real function on a closed nondegenerate box is Lebesgue integrable and its Lebesgue and Riemann integrals agree (Borel Darboux integrands in finite dimension).

[L3]

For a Riemann-integrable function on a product of nondegenerate closed rectangles, if every section in a chosen order is Riemann integrable, the ordinary iterated Riemann integral in that order exists and equals the product Riemann integral; integrability on the product alone does not guarantee that every section is integrable (Riemann--Fubini on product rectangles, with lower and upper section integrals and content-zero exceptional sections).

[L4]

If G is continuous on [a,b], differentiable on (a,b), and G′ has a Riemann-integrable extension f to [a,b], then ∫abf=G(b)−G(a) (Newton–Leibniz needs only continuity on [a,b], differentiability on (a,b), and a Riemann-integrable extension of the interior derivative).

[L5]

Assuming ACω, a bounded Riemann-integrable real function on a closed interval is Lebesgue integrable and has the same Lebesgue and Riemann integral (A bounded Riemann integrable function on a closed bounded interval is Lebesgue measurable and has the same integral).

[L6]

The multidimensional Riemann integral is linear on integrable functions over a nondegenerate rectangle (Linearity, monotonicity, the absolute-value estimate and coordinate-slice additivity for the Riemann integral in Rm).

Proof

1.1givenF1F2A1algebra

Dot the momentum equation with u. Since u⋅(e3×u)=0 pointwise and u⋅∇π=∇⋅(πu) by the component definitions in [F2] and ∇⋅u=0, this gives ∂t(∣u∣2/2)+∇⋅(πu−ν∑i=13ui∇ui)=bu3−ν∣∇u∣2. Here u⋅Δu=∇⋅(∑iui∇ui)−∣∇u∣2 follows by the product rule, component by component.

1.2A1A2L1L2L3L5

Fix t0<t1 and set K=[t0,t1]×Q3. For each rectangle A, write RA(F) for the Riemann integral of a Riemann-integrable F over A. The energy density, its time derivative, and the dissipation integrand are continuous on K and on its closed coordinate subrectangles; hence they are bounded and Riemann integrable by [L1], and Borel because the inverse image of an open set is relatively open. Under [A2], [L2] identifies their Riemann integrals with their Lebesgue integrals on K and on each spatial slice. For any such continuous F(t,x), [L3] gives a Riemann-integrable section integral gF(t)=RQ3(F(t,⋅)) and RK(F)=R[t0,t1](gF); [L2] identifies each spatial section integral with its Lebesgue integral, and [L5] identifies the outer interval integral of gF with its Lebesgue integral. Thus the nested Lebesgue dissipation integral in the statement exists and equals its product Riemann integral on K.

2.1givenF1F2A1step 1.1algebra

Multiply the buoyancy equation by b/N2 and use bΔb=∇⋅(b∇b)−∣∇b∣2 to get ∂t(b2/(2N2))+∇⋅(−(κ/N2)b∇b)=−bu3−(κ/N2)∣∇b∣2. Adding this to step 1.1 cancels the two bu3 terms and yields a local energy balance with flux πu−ν∑iui∇ui−(κ/N2)b∇b and dissipation ν∣∇u∣2+(κ/N2)∣∇b∣2.

3.1givenA1A2F1F2L1L2L3L4L6step 1.2step 2.1algebra∎

Write e=12(∣u∣2+b2/N2), F=πu−ν∑i=13ui∇ui−(κ/N2)b∇b, and D=ν∣∇u∣2+(κ/N2)∣∇b∣2, so step 2.1 gives ∂te+∇⋅F=−D. Fix a time t. Each ∂xjFj(t,⋅) is continuous on Q3; [L4] in xj gives its integral as the periodic endpoint difference Fj∣xj=2π−Fj∣xj=0=0. Applying [L1], [L3], and [L6] only in space gives RQ3(∇⋅F(t,⋅))=0, hence RQ3(∂te(t,⋅))=−RQ3(D(t,⋅)). Integrate this last equality in time; step 1.2 makes both section-integral functions Riemann integrable, and [L3] gives RK(∂te)=−RK(D). For each fixed x, [L4] in time applied to e and then [L3] yield RK(∂te)=RQ3(e(t1,⋅)−e(t0,⋅)). By [L6] and [L2] at the endpoints, this is E(t1)−E(t0); by step 1.2, RK(D) is the displayed nested Lebesgue dissipation integral. No time integral of an individual pressure-flux derivative is used. Since N>0, E(t)≥0; since ν,κ≥0, the dissipation is nonnegative, and when ν=κ=0 it vanishes.

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