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Equivalence of inverse problems for 2D elasticity and for the thin plate with finite measurements and its applications

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Equivalence of inverse problems for 2D elasticity and for the thin plate with finite measurements and its applications

Hyeonbae Kang Graeme Milton Jenn-Nan Wang

Abstract

In this paper, we prove that the inverse problems for 2D elasticity and for the thin plate with boundary data (finite or full measurements) are equivalent. Having proved this equivalence, we can solve inverse problems for the plate equation with boundary data by solving the corresponding inverse problems for 2D elasticity, and vice versa.

For example, we can derive bounds on the volume fraction of the two-phase thin plate from the knowledge of one pair of boundary measurements using the known result for 2D elasticity [6]. Similarly, we give another approach to the size estimate problem for the thin plate studied by Morassi, Rosset, and Vessella [7, 8].

1 Introduction

In this note we would like to connect the inverse boundary value problem for thin plate to that for 2D elasticity. To begin, we first discuss the inverse boundary value problem for the thin plate. Let Ω ⊂ R2be a simply-connected bounded domain with smooth boundary

∂Ω. Supposed that the middle surface of the thin plate with uniform thickness h occupies Ω. In the Kirchhoff-Love theory of thin elastic plates, the transversal displacement u satisfies

div div(C∇2u) = 0 in Ω, (1.1)

where ∇2u is the Hessian matrix of u, i.e.,

2u =u,11 u,12 u,12 u,22

 ,

and C = (Cijkl(x)), i, j, k, l = 1, 2, is a 4th order tensor satisfying that C ∈ L(Ω), (symmetry property) Cijkl(x) = Cjikl(x) = Cklij(x) ∀ x ∈ Ω a.e., (1.2) and there exists γ > 0 such that

(strong convexity) CA · A ≥ γ|A|2 ∀ x ∈ Ω a.e., (1.3)

Department of Mathematics, Inha University, Incheon 402-751, Korea (hbkang@inha.ac.kr).

Department of Mathematics, University of Utah, 155 S 1400 E RM 233, Salt Lake City, Utah 84112, USA (milton@math.utah.edu).

Department of Mathematics, NCTS (Taipei), National Taiwan University, Taipei 106, Taiwan (jn- wang@math.ntu.edu.tw).

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for every 2×2 symmetric matrix A. Hereafter, for any function u, u,jdenotes the derivative of u with respect to xj. The Dirichlet data associated with (1.1) is described by the pair {u, u,n} and the Neumann data by the pair

(C∇2u)n · n = −Mn, div(C∇2u) · n + ((C∇2u)n · t),t = (Mt),t,

where n is the boundary normal, t is the unit tangent vector field along ∂Ω in the positive orientation, u,n = ∇u · n, and u,t = ∇u · t. The quantities Mn and Mt are known as the twisting moment and the bending moment applied on the boundary ∂Ω.

The 2D elasticity equation is given by

div σ = 0 in Ω, (1.4)

where σ is the stress, which is related to the strain ε = (∇v + (∇v)T)/2 (T for transpose) by Hooke’s law

ε = Sσ.

Here v is the displacement field and S is known as the compliance tensor. We assume that S ∈ L(Ω), and that S satisfies the symmetry condition (1.2) and the strong convexity condition (1.3) (with a possibly different constant). The Dirichlet and Neumann conditions for (1.4) are described by v and σn, respectively.

It is widely known that (1.1) and (1.4) are equivalent (see for example [5]) as long as Ω is simply connected. As for the equivalence of boundary data, Ikehata [4] showed that when the full measurements (the Dirichlet-to-Neumann map or the Neumann-to-Dirichlet map) are allowed, knowing one set of boundary data uniquely determines the other one.

Consequently, the two inverse boundary value problems with the full measurements are equivalent. Note that Ikehata’s result was a uniqueness proof. We would also like to mention that explicit formulas for constructing the Dirichlet data (u, u,n) of the thin plate from the traction data σn of 2D elasticity were given in [3, p.158]. However, to the best of our knowledge, it does not seem that the relation between the individual boundary data {v} and {Mn, Mt} is known.

It is the purpose of this paper to clarify the relation between the boundary data {v, σn}

and {u, u,n, Mn, Mt}. In fact, we show that v on ∂Ω explicitly determines (Mn, Mt), and, following [3], show that σn on ∂Ω explicitly determines (u, u,n), and vice versa. As a consequence, the Dirichlet (resp. Neumann) boundary value problem for 2D elasticity equation is equivalent to the Neumann (resp. Dirichlet) boundary value problem for the thin plate equation, and thus the two inverse boundary value problems with finite measurements are equivalent. We emphasize that the results of this paper hold for tensors C and S which may depend on x (i.e., which have spatial variations), and which may be anisotropic.

Having established the equivalence of the boundary data, we can solve some inverse problems for the thin plate via the corresponding results for 2D elasticity, and of course, vice versa. For example, we can derive bounds on the volume fraction of the 2-phase thin plate via the result for 2D elasticity obtained by Milton and Nguyen [6]. On the other hand, the estimate of the size of an inclusion for the thin plate studied by Morrassi, Rosset, and Vessella [7, 8] is equivalent to the same problem for 2D elasticity, which was solved by Alessandrini, Morassi, and Rosset [1] (corrected in [2]). Moreover, we can also study the

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size estimate problem for 2D elasticity with certain anisotropic media through the similar result for the thin plate obtained by Morassi, Rosset, and Vessella in [9].

The paper is organized as follows. In Section 2, we prove the explicit relations between the boundary data of the thin plate and that of 2D elasticity. In Section 3, we discuss the application of this equivalence to the size estimate problem for the thin plate equation.

2 Equivalence of boundary data for the plate and for 2D elasticity

It is well known that when the domain is simply connected, the plate equation is equivalent to 2D elasticity equation, and vice versa. To describe the equivalence, let us define the rotational, self-adjoint, 4th order tensor R by

RA = RTAR (2.1)

for every 2 × 2 matrix A, where

R= 0 1

−1 0

 .

Then the equivalence between (1.1) and (1.4) is given by

C = RSR (2.2)

and

σ = RT(∇2u)R (= R(∇2u)), (2.3) where in the context of 2D elasticity u is known as the Airy stress function. As a conse- quence of these two relations, we have

C∇2u = RTεR. (2.4)

Recall that the Neumann data for the thin plate equation are given by (C∇2u)n · n = −Mn, div(C∇2u) · n + ((C∇2u)n · t),t = (Mt),t.

A comment on (Mt),t is helpful. Since divdiv(C∇2u) = 0, there exists a potential ψ such that

div(C∇2u) = (ψ,2, −ψ,1), and hence

div(C∇2u) · n = ∇ψ · t = ψ,t on ∂Ω (2.5) since t = −Rn. Integrating (2.5) along ∂Ω from some x0∈ ∂Ω and choosing an appro- priate ψ(x0), we obtain

ψ + (C∇2u)n · t = Mt on ∂Ω. (2.6)

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2.1 Traction vs Dirichlet data

Here, following [3, p.158], we connect the traction data for 2D elasticity to the Dirichlet data of the thin plate. It follows from (2.3) that

RTσn = (∇2u)t =∇u,1· t

∇u,2· t



. (2.7)

Thus by integrating RTσn along ∂Ω, we recover ∇u = [u,1, u,2]T (up to a constant) on

∂Ω. So u,n and u,t are recovered. By integrating u,t along ∂Ω we recover u on ∂Ω. On the other hand, from u and u,n we determine ∇u on ∂Ω and therefore σn through (2.7).

2.2 Displacement vs Moments

Now we turn to the relation between the displacement of 2D elasticity and the moments of the thin plate. Since ε = 12(∇v + (∇v)T), we have

RTεR=

 v2,212v1,212v2,1

12v1,212v2,1 v1,1

 . Thus we obtain

div RTεR="v2,1212v1,2212v2,12 v1,1212v1,2112v2,11

#

=

"1

2v2,1212v1,22

1

2v1,1212v2,11

#

= RT"(12v1,212v2,1),1

(12v1,212v2,1),2

#

= RT∇(1

2v1,2−1 2v2,1), which implies

n · (div RTεR) = (Rn) · ∇(1

2v1,2−1 2v2,1)

= −t · ∇(1

2v1,2− 1 2v2,1)

= (1

2v2,1−1 2v1,2),t. It then follows from (2.5) that

ψ,t = n · div(C∇2u) = (1

2v2,1−1 2v1,2),t, and from (2.6) that

Mt= 1

2(v2,1− v1,2) + (RTεRn) · t. (2.8) Observe that 12(v2,1− v1,2) can be expressed as

1

2(v2,1− v1,2) =

 RT

 0 −12(v2,1− v1,2)

1

2(v2,1− v1,2) 0

 Rn



· t.

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We also have

(RTεRn) · t =

 RT

 v1,1 12v1,2+12v2,1

1

2v1,2+12v2,1 v2,2

 Rn



· t.

From (2.8) we thus find Mt=



RTv1,1 v1,2

v2,1 v2,2

 Rn



· t

= −t · RT(∇v)t = −(Rt) · (∇v)t = −n · (∇v)t. (2.9) We also deduce from the definition of Mnthat

Mn= n · (RTεR)n = t · εt = t · (∇v)t. (2.10) Formulae (2.9) and (2.10) show that Mn and Mt can be recovered from v,t. On the other hand, we can recover v,t from Mt and Mn, i.e., v,t = −Mtn + Mnt. By integrating v,t

along ∂Ω, we then determine v on ∂Ω.

3 Applications to inverse problems

3.1 Estimating the volume of an inclusion for the thin plate with isotropic phases

In this section, we want to discuss the size estimate problem for the thin plate equation based on the similar problem for 2D elasticity. Now we assume that the thin plate is made of an isotropic medium, i.e, the fourth order tensor C is given by

Cijkl= 1

2B(1 − ν)(δikδjl+ δilδjk) + Bνδijδkl. (3.1) The scalar B is called the bending stiffness and is defined by

B = h3 12

 E

1 − ν2

 ,

where E is the Young’s modulus, and ν is the Poisson’s coefficient. Both E and ν can be written in terms of the Lam´e coefficients as follows:

E = µ(2µ + 3λ)

µ + λ and ν = λ

2(µ + λ). In terms of these the strong convexity condition (1.3) reads as

µ > γ and 2µ + 3λ > γ.

Now assume that the plate is made by two different materials in the sense that λ = λ1χ1+ λ2χ2, µ = µ1χ1+ µ2χ2,

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where

χj =

(1 in phase j, 0 otherwise.

Suppose that u is the solution of the thin plate equation (1.1) having boundary data {u, u,n, Mn, Mt} with

(C∇2u)n · n = −Mn, div(C∇2u) · n + ((C∇2u)n · t),t = (Mt),t.

The inverse problem here is to estimate the volume fraction f1 of phase 1 (or f2) using {u, u,n, Mn, Mt}.

By (2.2), we find that the thin plate equation with elastic tensor (3.1) is equivalent to 2D elasticity with a compliance tensor S = (Sijkl), where

Sijkl = 1

0ikδjl+ δilδjk) +1 4(1

κ − 1 µ0ijδkl where

κ = 2

B(1 + ν) (bulk modulus), µ0 = 2

B(1 − ν) (shear modulus).

In other words, Hooke’s law is given by ε = 1

0σ +1 4(1

κ − 1

µ0)Tr(σ)I2 where I2 is the identity matrix, and the equilibrium equation is

div σ = 0 in Ω.

Using the result in the previous section, we can determine the displacement v and the traction σn on ∂Ω from {u, u,n, Mn, Mt}. So to solve the size estimate problem for the thin plate, it suffices to solve the same problem for 2D elasticity.

Therefore, when all moduli involved are known, the result obtained by Milton and Nguyen [6] will give us bounds on the volume fraction and also the attainability condi- tions for these bounds for the two-phase thin plate with homogeneous isotropic phases.

There are two approaches used in [6] – the method of translation and the method of split- ting. These methods depend on suitable null-Lagragians, which are (possibly nonlinear) functionals of fields that can be expressed in terms of the boundary measurements. For 2D elasticity, it is known that hσi, hεi, hdetσi, are null-Lagrangians, where hf i is the av- erage of the field f . Thus, from relations (2.3) and (2.4), we immediately get that h∇2ui, hC∇2ui, and hdet∇2ui are null-Lagrangians for the thin plate. It is interesting to point out that hdetC∇2ui is not a null-Lagrangian for the thin plate. This corresponds to the fact that hdetεi is not a null-Lagrangian for 2D elasticity.

We now consider the case where the two phases of the plate are themselves inhomo- geneous, with spatially varying moduli. Assume that the medium in, say, phase 1, is given, but the medium in phase 2 is unknown. We also want to find upper and lower bounds on the volume of the unknown inclusion (phase 2) from one set of measurements of {u, u,n, Mn, Mt}. Under suitable conditions, this problem was solved in [7] (with the

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on some quantitative estimates of the unique continuation property for the thin plate.

Using the equivalence of inverse problems for the thin plate and for 2D elasticity, we can convert the size estimate problem for the plate just described to the same problem for 2D elasticity, which was solved in [1] (and also in [2]).

3.2 Estimating the volume of inclusion for 2D elasticity with anisotropic medium

Now we assume that 2D elastic body is made of inhomogeneous and anisotropic medium with compliance tensor S = (Sijkl). Due to the symmetry property for the compliance tensor S, we can denote













S1111 = F, S1122= S2211= B, S1112 = S1121 = S1211 = S2111 = −D, S2212 = S2221 = S1222 = S2122 = −C, S1212 = S1221 = S2112 = S2121 = E, S2222 = A.

Suppose that the elastic body consists of two different media, i.e., S = S0χ1+eSχ2. Likewise, the stress tensor σ satisfies

divσ = 0 and ε = Sσ in Ω.

Now assume that S0 is given and eS is unknown. We are now interested in estimating the size of χ2 by one boundary measurement {v, σn}.

In view of the relation (2.2), the corresponding elastic tensor C = C0χ1+ eCχ2 = (Cijkl) of the thin plate is given as





















C1111 = S2222 = A, C1122 = S2211 = B, C1112 = −S2212= C, C2212 = −S1112= D, C1212 = S1212 = E, C2222 = S1111 = F.

So the problem above is equivalent to the size estimate problem for the thin plate with elastic tensor C using {u, u,n.Mn, Mt}. This problem has been studied by Morassi, Rosset, and Vessella [9]. A key ingredient in the proof of [9] is the three-ball inequality for the plate equation with elastic tensor C0. The three-ball inequality is proved under a so- called Dichotomy condition for C0, which permits us to decompose the fourth order elliptic operator associated with the thin plate equation into a product of two second order elliptic

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operators. We now write this Dichotomy condition in terms of S0= (Sijkl0 ). We define













S11110 = F0, S11220 = S22110 = B0, S11120 = S11210 = S12110 = S21110 = −D0, S22120 = S22210 = S12220 = S21220 = −C0, S12120 = S12210 = S21120 = S21210 = E0, S22220 = A0,

a0= A0, a1 = 4C0, a2 = 2B0+ 4E0, a3= 4D0, a4= F0, and the matrix

M(x) =

a0 a1 a2 a3 a4 0 0 0 a0 a1 a2 a3 a4 0 0 0 a0 a1 a2 a3 a4

4a0 3a1 2a2 a3 0 0 0 0 4a0 3a1 2a2 a3 0 0 0 0 4a0 3a1 2a2 a3 0 0 0 0 4a0 3a1 2a2 a3

(Here we use similar notations as in [9]). Then the Dichotomy condition is defined as 1

a0 |detM(x)| > 0 or 1

a0 |detM(x)| = 0 ∀ x ∈ ¯Ω. (3.2) Assume that (3.2) holds and S0 ∈ C1,1(Ω) (equivalently, C0 ∈ C1,1(Ω)). Then one can es- timate the size of χ2 by one boundary measurement {v, σn} under the fatness assumption (see [9, Theorem 3.2] for details).

Acknowledgements

HK was partially supported by National Research Foundation of Korea through NRF grants No. 2009-0085987 and 2010-0017532. GWM was partially supported by the Na- tional Science Foundation of the USA through grant DMS-0707978. JNW was partially supported by the National Science Council of Taiwan through grants 100-2628-M-002-017 and 99-2115-M-002-006-MY3.

References

[1] G. Alessandrini, A. Morassi, and E. Rosset, Detecting an inclusion in an elastic body by boundary measurements, SIAM J. Math. Anal., 33 (2002), 1247-1268.

[2] G. Alessandrini, A. Morassi, E. Rosset, and S. Vessella, On doubling inequalities for elliptic systems, J. Math. Anal. App., 357, (2), (2009), 349-355.

[3] M.E. Gurtin, The Linear Theory of Elasticity. Encyclopedia of Physics, vol. VIa/2, Mechanics of. Solids, Springer-Verlag, Berlin-Heidelberg-New York (1972).

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[4] M. Ikehata, A relationship between two Dirichlet to Neumann maps in anisotropic elastic plate theory, J. Inv. Ill-posed Problems, 4 (1996), 233-243.

[5] G.W. Milton, The Theory of Composites, Cambridge Monographs on Applied and Computational Mathematics, Cambridge University Press, 2002.

[6] G.W. Milton and H. L. Nguyen, Bounds on the volume fraction of 2-phase, 2- dimensional elastic bodies and on (stress, strain) paris in composite, arXiv:1108.5764.

[7] A. Morassi, E. Rosset, and S. Vessella, Size estimates for inclusions in an elastic plate by boundary measurements, Indiana Univ. Math. J., 56 (2007), 2325-2384.

[8] A. Morassi, E. Rosset, and S. Vessella, Detecting general inclusions in elastic plates, Inverse Problems, 25 (2009), 0450091 (14pp).

[9] A. Morassi, E. Rosset, and S. Vessella, Estimating area of inclusions in anisotropic plates from boundary data, arXiv:1109.3397.

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