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Rate of convergence from the rotating Euler and shallow water equations to the rotating lake equations

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R E S E A R C H

Open Access

Rate of convergence from the rotating

Euler and shallow water equations to the

rotating lake equations

Peng Cheng

1,2

, Jianwei Yang

2*

and Dan Bai

1

*Correspondence: [email protected] 2College of Mathematics and Information Science, North China University of Water Resources and Electric Power, Zhengzhou, Henan Province 450045, P.R. China Full list of author information is available at the end of the article

Abstract

The rate of convergence from the rotating shallow water and Euler equations to the rotating lake equations is obtained when the Froude number limit is considered.

MSC: 35B25; 35Q31; 76B15

Keywords: Euler and shallow water equations; lake equations; rate of convergence; zero Froude number limit

1 Introduction and main results

The inviscid rotating Euler and shallow water equations read, in a bounded two-dimensional domain:

∂th+div

hu= , (.)

∂t

hu+divhuu+hu+h∇((h

)γ–hγ–  )

 = , (.)

with initial and boundary conditions

h,u|t==

h(x),u(x), hu·n|∂= , (.) whereγ ≥. In (.)-(.), the unknownsh=h(x,t) andu=u(x,t) = (u

(x,t),u(x,t))

denote the height of the water and the horizontal component of the fluid velocity, respec-tively. The orthogonal velocity is denoted by

u⊥=

 –  

u

u

=–u,u

and the strictly positive functionh=h(x) describes the bottom topography. The

param-eter>  is the Froude number measuring the inverse pressure forcing. Moreover, the energy for the system (.)-(.) can be defined as follows:

E(t) =

 h

u+ 

h dx, (.)

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where the potential energy

h= 

γ

hγ–γ(h)γ–

hh

(.)

is a convex function with minimum occurring ath =h

which satisfies(h)≥. It is

easy to see that the energy inequality associated with system (.)-(.) reads

d dtE

(t) = . (.)

By the initial energy bound (.) below and the following elementary convexity inequality: 

γh

h

γ

h forγ ≥, (.)

we can assume that the initial heighth

converges to a nonconstant functionh(x)

de-pending on the space variable, so it is reasonable to expect that, as→,hh

, and

(.) yields the limitdiv(hu) = . The corresponding rotating lake equations are

div(hu) = , (.) ∂t(hu) +div(huu) +hu⊥+h∇π= , (.) u|t==u(x), hu·n|∂= , div(hu) = . (.)

Thus, roughly speaking, it is also reasonable to expect from the mathematical point of view that the smooth solution to (.)-(.) converges in suitable functional spaces to the smooth solution of (.)-(.) as →, and the hydrostatic pressure π in (.) is the ‘limit’ of

(h)γ–hγ– 

in (.). This paper is devoted to the rigorous justification of the convergence of the above low Froude number limit for smooth solution of the inviscid rotating Euler and shallow water equations in a bounded two-dimensional domain. We remark that the existence and uniqueness of the classical solution of the lake equations (.)-(.) have been proved in [].

Specifically, whenγ = , equations (.)-(.) comprise the rotating and inviscid shallow water system which models large scale geophysical motions in a thin layer of fluid under the influence of the Coriolis rotational forcing and is commonly used in oceanography and atmospheric physics [–]. For the singular limit problems of the shallow water model, we refer to [, ].

In [], Cheng proved the singular limits and convergence rates of compressible Euler and rotating shallow water equations (.)-(.) withh=  toward their incompressible

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system) (.)-(.) when the Froude number tends to zero. However, no convergence rate was given in []. In this paper, our purpose is to refine the discussions in [] and obtain the rate of convergence without introducing the correction term. Furthermore, we also prove the convergence of√hu toh

uwith

huh

uL([,T];L())C

γ, which is

not contained in [].

In the following, we describe our main result. In order to simplify the presentation, we suppose that

A: h≥c> , (h,hu)∈H()×(H()) (ensuring the local-in-time existence of smooth solutions of system (.)-(.) and that(h

,hu)satisfy some appropriate com-patibility conditions on);

A: h ≥c > , u ∈ (H()),div(hu) =  (ensuring the local-in-time existence of smooth solutions of the rotating lake equations (.)-(.) and(h,u)satisfy some ap-propriate compatibility conditions on).

For a fixed> , the local existence and uniqueness of the classical solution of system (.)-(.) can be obtained under the assumptionsAandA.

Proposition .(Local existence of smooth solutions. (See [])) Let s≥be an integer.

Under the assumptions Aand A,there exist T> and a unique smooth solution(h,u)

to the system(.)-(.)defined in the time interval[,T],with

h,uC[,T

];Hs()

C[,T];Hs+()

. Now the main result of this paper reads as follows.

Theorem . Let(h,u)H()×(H())be the smooth solution of system(.)-(.) established in Proposition.and let u be a classical solution of the rotating lake equations

(.)-(.)with the initial data uwhich satisfies assumptions Ain L∞([,T∗];Hs())and Tis the existence time of (.)-(.).Furthermore,we assume that the initial condition

hdx+

h

u

–

hu 

dx(.)

holds for some positive constant C> .Then there exists a constant C> ,independent of

,such that as→,we have TTand the following estimate:

h

h

γ

L∞([,T];())C

γ, (.)

hu

hu

L∞([,T];L())C

γ, (.)

huhu

L∞([,T];Lγ

γ+())C

γ (.)

for all T∈(,T∗].

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2 Proof of the theorem

We defineT =min(T

∗,T) >  so that the exact solution and the approximate solution

are both defined in the time interval [,T].

From the energy (.) and the energy equality (.), we have

 h

u+ 

hdx

=

 h

u

 

+ 

hdxC. (.)

Therefore, from (.), we have the following properties:

hu is bounded inL,T;L(), (.)

h

h

γ

is bounded inL∞,T;L(). (.)

Thus from (.), we have

hh

L([,T];Lγ())C

γ. (.)

In fact, we will find that hh

L∞([,T];Lγ())→ has a faster rate of convergence.

Now we define the modulated energy functionalH(t) as follows:

H(t) =

 h

uu+

hdx, (.)

whereuis the classical solution of the rotating lake equations (.)-(.). To derive the integration inequality forH(t), we useuas a test function in equation (.) to yield the

following equality:

hu·u dx= –

hu·u(t= )dx

t

hu·∂su dx ds

t

huu:u dx ds+ t

hu·u dx ds

+ 

t

hu· ∇hγ–––dx ds. (.)

From (.)-(.), we find the energy identity of the rotating lake equations: 

d dt

h|u|dx= ,

which implies that

h|u|dx=

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Using (.)-(.) and the energy inequality (.), by integration by parts, we can calculate

H(t) as follows:

H(t) =E(t) –

hu·u dx+

h|u|dx

=H() –  

h|u|dx+

 

h|u|dx

t

huu:u dx ds+ t

hu·u dx ds

+ 

t

hu· ∇hγ–––dx ds

t

hu·∂su dx ds

=H() –  

h|u|dx+

 

h|u|dx

t

hu·∂su dx ds+

k=

Ik, (.)

where

I= –

t

huu:u dx ds, I=

t

hu⊥·u dx ds,

I=

t

hu· ∇hγ–––dx ds.

It is noted that the first two terms on the right hand side of the above inequality is canceled in terms of (.).

Now, we begin to treat the integralsIk(k= , , , ) term by term. To deal with the

ki-netic partI, we rewrite it as

I= –

t

huuuu:∇u dx ds

t

huu:∇u dx ds

+

t

huu:∇u dx ds

t

huu:∇u dx ds

C

t

H

(s)ds+I+I,

where

I= –

t

huu:∇u dx ds,

I=

t

huu:∇u dx ds

t

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Using integration by parts and the boundary conditions ofhu andu, we have

I=

  t

|u|divhudx ds

= –  t

|u|∂shdx ds

= –  td ds

|u|hdx ds+

t

hu·∂su dx ds dx ds

= 

h|u|dx

 

h|u|dx+

t

hu·∂su dx ds.

Furthermore, we have

I=

t

huiuj∂juidx dst

huiuj∂juidx ds

= t

huhu·(u· ∇)udx ds.

Therefore, we obtain

I≤C

t

H

(s)ds+ 

h|u|dx

 

h|u|dx

+

t

hu· su dx ds

+ t

huhu·(u· ∇)udx ds. (.)

Using the anti-symmetric property (u)·u= –u ·uand the orthogonal property

u·u⊥= , we obtain

I=

t

huhu·udx ds. (.)

Finally, we deal with the potential partI. In view of (.) and the boundary condition

ofu, we have

u· ∇h= –hdivu,

t

divu dx ds= – γ

γ– 

t

hu· ∇h

γ–

dx ds= .

Thus, we obtain

I=

t

hu· ∇hγ–dx ds

t

hu· ∇hγ–

dx ds

=γ– 

γ

t

u· ∇hγdx dsγ – 

t

hhγ–u· ∇hdx ds

= –γ– 

γ

t

hγdivu dx ds+γ – 

t

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= –γ– 

γ

t

hγ–γhhγ–+ (γ – )divu dx ds

C

t

H

(s)ds. (.)

Inserting the estimates (.)-(.) into (.), we have, from (.),

H(t) =H() +C t

H(s)ds

+ t

huhu∂su+ (u· ∇u)u+u

dx ds

=H() +C

t

H

(s)ds+

t

huhu· ∇πdx ds. (.)

From the continuity equation (.), the initial conditions (.), the estimate (.), and the Hölder inequality, we get, by integration by parts,

t

hu· ∇πdx ds=

hh

πdx

h

–h

πdx

t

hh

∂sπdx ds

hhLγ() π

L

γ

γ–()+h

–hLγ() π

L

γ γ–()

+hhL([,T];Lγ()) ∂tπ

L∞([,T];Lγγ–())

Cγ (.)

and – t

hu· ∇πdx ds= –

t

hh

u· ∇πdx ds

hh

L([,T];Lγ()) u

L∞([,T];L

γ γ–())

× ∇π

L∞([,T];L

γ γ–())

Cγ. (.)

Combining (.) with (.)-(.), one gets

H(t)H() +C t

H(s)ds+Cγ,t(,T].

Using the initial conditions (.), we haveH()Cγ since

h

u–u 

dx≤

h

u–

hu 

dx+ 

h–

hu  dx

≤h

u–

hu 

L()+  u

L∞()

h – h 

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≤h

u

–

hu 

L()+Ch

–h 

()

.

Here, we also have used assumption (A) and the following elementary inequality:

|√x–√x|≤

c|x–x| , x

,x≥c> , (.)

the Hölder inequality and the finite measure of. Then, with the help of the Gronwall inequality, we get

H

(t)≤,t(,T]. (.)

Using the Hölder inequality, we have

hu

hu

L()≤ √

hu

uL()+  √

hh

uL()

+Chh

 

L() uL∞()

(.)

for anyt∈(,T]. In view of (.) and using the Hölder inequality, we have huh

u

Lγ γ+()≤

huuL

γ γ+()+ 

hh

u

Lγ γ+()

≤√hLγ()

huuL()

+ √hh

Lγ() u

L

γ γ–()

(.)

for anyt∈(,T]. By a standard argument on the time extension of smooth solutions, we

obtainTT

∗,i.e. T=T

∗. With the aid of (.) and (.)-(.), we conclude that the proof of Theorem . is finished.

Competing interests

The authors declare that they have no competing interests.

Authors’ contributions

All authors carried out the proof. All authors read and approved the final manuscript.

Author details

1Institute of Water Resources and Hydro-electric Engineering, Xi’an University of Technology, Xi’an, Shanxi Province 710048, P.R. China.2College of Mathematics and Information Science, North China University of Water Resources and Electric Power, Zhengzhou, Henan Province 450045, P.R. China.

Acknowledgements

J. Yang’s research was partially supported by the Joint Funds of the National Natural Science Foundation of China (Grant No. U1204103).

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References

1. Levermore, CD, Oliver, M, Titi, ES: Global well-posedness for models of shallow water in a basin with a varying bottom. Indiana Univ. Math. J.45, 479-510 (1996)

2. Ghil, M, Childress, S: Topics in Geophysical Fluid Dynamics: Atmospheric Dynamics, Dynamo Theory, and Climate Dynamics. Applied Mathematical Sciences, vol. 60. Springer, New York (1987)

3. Majda, A: Introduction to PDEs and Waves for the Atmosphere and Ocean, vol. 9. Am. Math. Soc., Providence (2003) 4. Oliver, M: Variational asymptotics for rotating shallow water near geostrophy: a transformational approach. J. Fluid

Mech.551, 197-234 (2006)

5. Pedlosky, J: Geophysical Fluid Dynamics. Springer, Berlin (1992)

6. Bernardi, C, Pironneau, O: On the shallow water equations at low Reynolds number. Commun. Partial Differ. Equ.16, 59-104 (1991)

7. Bresch, D, Desjardins, B: Existence of global weak solutions for a 2D viscous shallow water equations and convergence to the quasi-geostrophic model. Commun. Math. Phys.238, 211-223 (2003)

8. Cheng, B: Singular limits and convergence rates of compressible Euler and rotating shallow water equations. SIAM J. Math. Anal.44, 1050-1076 (2012)

9. Wu, KC: Low Froude number limit of the rotating shallow water and Euler equations. Proc. Am. Math. Soc.142, 939-947 (2014)

References

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