2π x.. It is the kernel of the outgoing resolvent R

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SHARP NORM ESTIMATES OF LAYER POTENTIALS AND OPERATORS AT HIGH FREQUENCY XIAOLONG HAN AND MELISSA TACY WITH AN APPENDIX BY JEFFREY GALKOWSKI Abstract. In this paper, we investigate single and double layer potentials mapping boundary data to interior functions of a domain at high frequency. For single layer potentials, we find that the L ( Ω L (Ω norms decay in. The rate of decay depends on the curvature of Ω: The norm is 3/4 in general domains and 5/6 if the boundary Ω is curved. The double layer potential, however, displays uniform L ( Ω L (Ω bounds independent of curvature. By various examples, we show that all our estimates on layer potentials are sharp. The appendix by Galkowski gives bounds L ( Ω L ( Ω for the single and double layer operators at high frequency that are sharp modulo log. In this case, both the single and double layer operator bounds depend upon the curvature of the boundary. 1. Introduction Denote = n i=1 i as the Laplacian operator in R n. Given a piecewise smooth and bounded domain Ω R n, Green s formula yields that the solution to the Helmholtz equation in Ω u = u has the form (1.1 u(x = K (x y νy u(ydσ y νy K (x yu(ydσ y, Ω Ω where νy is the outward normal derivative at y Ω, dσ is the surface measure on Ω, and K is a fundamental solution to (, that is (1. ( K (x = δ(x. In fact, we can write K explicitly as where H (1 n K + (x = i 4 ( n π x H (1 n ( x, is the Hankel function of the first kind and order n. It is the kernel of the outgoing resolvent R + = [ ( + i0 ] 1. Let us therefore define the semiclassical single layer potential S + as S + (f = R+ (fdσ = K+ (fdσ, and the semiclassical double layer potential D + as D + (f = νk + (fdσ. Now (1.1 can be written (1.3 u = S + ( νu D + (u Ω, allowing us to construct interior eigenfunction from boundary data. In particular, u = S + ( ν u, for Dirichlet eigenfunction u Ω = 0, u = D + (u Ω, for Neumann eigenfunction ν u = 0. 010 Mathematics Subject Classification. 31B10, 31B5, 31B35. Key words and phrases. layer potentials, layer operators, high frequency, eigenfunctions, quasimodes, restriction estimates, boundedness, sharpness. 1

XIAOLONG HAN AND MELISSA TACY WITH AN APPENDIX BY JEFFREY GALKOWSKI Main results. In this paper we obtain sharp L ( Ω L (Ω bounds on S + and D+. Theorem 1.1 (Boundedness and sharpness of semiclassical single layer potentials. (i. In a general domain Ω, S + (u L (Ω c 3 4 u L ( Ω, where c depends only on Ω. Furthermore, the exponent 3/4 is sharp if the boundary Ω contains a flat piece. (ii. If Ω is curved, that is, the second fundamental form of Ω is (positive or negative definite, then S + (u L (Ω c 5 6 u L ( Ω, where c depends only on Ω. Furthermore, the exponent 5/6 is sharp if Ω is an annulus. In contrast to the case of single layer potentials, we obtain a uniform bound for double layer potentials in all domains. The sharp examples for the single layer potential all rely on concentration in the tangential direction (see Section 4. However the symbol of D + is zero in such tangential directions. Theorem 1. (Boundedness and sharpness of semiclassical double layer potentials. D + (u L (Ω c u L ( Ω, where c depends only on Ω. Furthermore, the estimate is sharp if Ω is a disc. The representation of eigenfunctions in (1.3 has applications in a variety of both theoretical and numerical studies. Hassell and Zelditch [18] use it to prove the quantum ergodicity of boundary values of eigenfunctions. In particular, they express boundary traces of Dirichlet, Neumann, and Robin eigenfunctions as eigenfunctions of integral operators produced by semiclassical layer potentials. In a similar vein Toth and Zelditch [3, 33] recently applied these potentials to prove quantum ergodic restriction (QER theorems on interior hypersurfaces. If the boundary Ω is analytic, then there exist analytic continuations of S + and D+ in the Grauert tube (a complex neighborhood of the real domain. Such complexification enables the study of zeros of eigenfunctions in the complex region (instead of in the real region, where it has a simpler characterization. For detailed discussion on the nodal intersection estimates, see Toth and Zelditch [31], El-Hajj and Toth [9]. In star shaped domains Barnett and Hassell [] develop a numerical technique for constructing Dirichlet eigenfunctions by solving a related eigenfunction problem on the boundary. They then use (1.3 to reconstruct interior eigenfunctions. Their technique allows them to control error on the boundary and so mapping norms on S + control error in the interior. In [, Remark 3.], the authors proposed the question of finding a bound on the -dependence of the single layer potential S +. In particular they ask is (1.4 S + L ( Ω L (Ω 1? Such a bound would imply that boundary error controls interior error with no loss, which would be optimal for their numerical technique. In fact, some results were achieved previously. Feng and Sheen [11] showed that the norm is uniformly bounded independent of. Spence [6] improved this to 1/. Theorem 1.1 answers Barnett and Hassell s question in the negative for general (and even curved domains. However, the estimate (1.4 might hold for strictly convex domains; see Conjecture 4.3. Weaker estimates than those of Theorem 1. were obtained by Feng and Sheen [11] and Spence [6]. Precisely, Feng and Sheen [11] proved D L ( Ω L (Ω ; while Spence [6] improved to D L ( Ω L (Ω 1/. See also the survey article [6] for related results and their applications in numerical computations. One may compare the high frequency ( results of Theorems 1.1 and 1. with the case = 0. There (1.1 reduces to the construction of a harmonic function u in Ω by its boundary data. K 0 + = N is the fundamental solution of the Laplacian: N(x = δ(x. The two convolution-type operators S(f and D(f mapping L ( Ω to L (Ω with kernels N and ν N are the classical single and double layer potentials at zero frequency. The mapping properties of these layer potentials from boundary data to interior functions and related boundary value problems have been studied extensively over the past century. See [10, 3, 35] and [7, 1] for a detailed discussion of this classical problem. In the case of classical single and double layer potentials, it is the regularity of the boundary that determines mapping properties, with the case of smooth boundaries being rather trivial. By contrast, in

LAYER POTENTIALS AND OPERATORS 3 the high frequency limit, the interest is not the boundedness of S + and D+ for a particular, but rather the rate of decay of the mapping norms as. In this limit, the problem is interesting even for smooth boundaries, as Theorem 1.1 shows, the rate of decay depends on the geometric properties of the boundaries. The single and double layer operators S + and D+ are restrictions of layer potentials S+ and D+ to the boundary, that is, D + : f D+ (f Ω and S + : f S+ (f Ω. Galkowski s appendix to this paper provides estimates for both D + and S+. These operators have been studied by other mathematicians and some results were known prior to the above estimates. Please refer to the appendix for a brief discussion. Theorem A.1 (Boundedness and sharpness of semiclassical layer operators. C S + 1/ log in general domains; L ( Ω L ( Ω C /3 log if Ω is curved, and C D + 1/4 log in general domains; L ( Ω L ( Ω C 1/6 log if Ω is curved. Moreover, these estimates are sharp modulo the log. Connection with boundary estimates of eigenfunctions. Because of (1.3, there is a close relation between semiclassical layer potentials and boundary estimates of eigenfunctions. Dirichlet eigenfunction: u satisfies u = S + ( νu. Bardos, Lebeau, and Rauch [1] and Hassell and Tao [16, 17] proved that as u = S + ( νu this implies that u L (Ω 1 ν u L ( Ω, S + L ( Ω L (Ω c 1. Therefore the sharp examples for Theorem 1.1 that we produce in Section 4 are far from being normal derivatives of a Dirichlet eigenfunctions. Neumann eigenfunction: u satisfies u = D + (u Ω. Hence, as a corollary of Theorem 1., we have Corollary 1.3 (Boundary estimate of Neumann eigenfunctions. Let u be a Neumann eigenfunction of in Ω with eigenvalue. Then where C is independent of. Tataru [9] proved that u L (Ω c u L ( Ω, (1.5 u L ( Ω 1 3 u L (Ω. Putting the above results together gives both lower and upper bounds of the boundary estimates of Neumann eigenfunctions: u L (Ω u L ( Ω 1 3 u L (Ω. Furthermore, this suggests that the sharp examples for Tataru s estimate are far from saturating the double layer potential estimates. We will discuss the sharpness of above inequalities in Section 4, and construct examples for which saturation is achieved. Connection with interior hypersurface restriction estimates of eigenfunctions. One can similarly define the incoming resolvent [ R = ( i0 ] 1 and K as its kernel. Then the above theorem is also valid with the same norm for S. We will drop the ± sign in the L estimates without causing any confusion. If we write de as the spectral measure operator δ(, then Stone s formula (See e.g. [0, Chapter XIV]. (1.6 de = R+ R πi

4 XIAOLONG HAN AND MELISSA TACY WITH AN APPENDIX BY JEFFREY GALKOWSKI immediately implies the same norm bounds from L ( Ω to L (Ω. Moreover, the sharp examples of these bounds on spectral measure operators automatically provides the sharpness for single layer potentials. Proposition 1.4 (Boundedness and sharpness of spectral measure operators. (i. In a general domain Ω, de (udσ L (Ω c 3 4 u L ( Ω, and the norm is sharp if the boundary Ω contains a flat piece. (ii. If Ω is curved, then de (udσ L (Ω c 5 6 u L ( Ω. and the norms are sharp if Ω is an annulus. Notice that the kernel of de K = K+ K πi satisfies ( K = 0. To estimate the norm of de ( dσ : L ( Ω L (Ω, we consider the adjoint operator (de with the same norm. In particular, the estimates of de in Proposition 1.4 is equivalent to c (1.7 (de 3 4 u (u L ( Ω L (Ω in general domains; c 5 6 u L (Ω if Ω is curved. We provide a proof of (1.7 here. It also motivates the strategy of the main proof of Theorem 1.1. Write v = (de (u, then v is an eigenfunction in R n. In particular, let Ω 1 be a compact set such that Ω Ω 1 R n. Then v is an eigenfunction in Ω 1, and Ω can be regarded as an interior hypersurface in Ω 1. It is a classical result in scattering theory that (de : L (Ω L (Ω 1 is bounded. In fact, from the semiclassical Fourier integral operator theory, (See e.g. [5]. we have (1.8 v L (Ω 1 c 1 u L (Ω. Since Ω Ω 1, we can use the interior hypersurface restriction estimate for v from [4, ]: on general Ω, and if Ω is curved. v L ( Ω c 1 4 v L (Ω c 3 4 u L (Ω v L ( Ω c 1 6 v L (Ω c 5 6 u L (Ω Connection with interior hypersurface estimates of quasimodes and strategy of the proofs. Consider the adjoint operator (S + : L (Ω L ( Ω. Unlike (de (u, (S + (u is not an eigenfunction on the whole space R n. The failure of (S + (u to be an eigenfunction arises from a singularity in its kernel at the diagonal. Our strategy is therefore to divide the kernel into near-diagonal and off-diagonal parts. The near-diagonal part admits better bound than required, and the off-diagonal part while not an exact eigenfunction is a good approximate eigenfunction (or quasimode which can be treated within the semiclassical framework. To use the the semiclassical framework we set h = 1, then for p(x, hd = ( h 1 Laplacian eigenfunctions satisfy p(x, hdu = 0. Given any function v we may measure the quasimode error E[v] = ( h 1v See [36, Section 7.4.1] for more details on quasimodes. Restrictions of quasimodes to hypersurfaces are studied in [7] and [15]. Therefore we are able to reduce the problem of operator norm estimates to that of estimating the quasimode error of the off-diagonal contribution. A similar strategy applies to double layer potential (D +, as the off-diagonal part on the boundary resembles the normal derivative of an O L (h quasimode, and therefore we can use the result on Neumann data restriction estimates in [8].

LAYER POTENTIALS AND OPERATORS 5 Semiclassical interpretation. Here we provide a semiclassical description of the problem and our approach. While this description is not strictly necessary to prove Theorems 1.1 and 1. it allows us to develop a useful heuristic that gives us insight into the role of geometry in these estimates. In the semiclassical setting (with h = 1 Laplacian eigenfunctions are solutions to p(x, hdu = ( h 1u = 0, where p(x, hd has symbol p(x, ξ = ξ 1. Similarly (1. can be written as p(x, hdk + h 1 (x = h δ(x. Hörmander s theory on propagation of singularities asserts that (1.9 W F h (K \ W F h (g (x, ξ T R n : p(x, ξ = 0} = (x, ξ T R : ξ = 1} = S R n, which means that W F h (K \ W F h (g is in the bicharacteristic variety of p, and furthermore it is invariant under the Hamiltonian flow Φ t of p. Here, W F h is the semiclassical wavefront set, T R n and S R n are the cotangent and cosphere bundles of R n, and Φ t of p is the geodesic flow in R n. See [1, 36] for a complete discussion of the theory. This framework provides an heuristic to understand the improvement in Theorem 1.1 for curved domains. The dominating singularities of S + propagate through the bicharacteristic flowout, i.e., the geodesic flow. Since f is supported on Ω, the dominating singularities propagate along the lines tangent to the boundary. Therefore it is natural to expect worse estimates in the flat case where tangent lines coincide with the boundary. Next we consider the semiclassical description of the outgoing and incoming resolvents R ± and the spectral measure de. From the intersecting Lagrangian distribution theory introduced in [4] (for the semiclassical version see [13, Appendix A], R + is an intersecting Lagrangian distribution associated to two Lagrangian submanifolds [13, Theorem 3]: The conormal bundle to the diagonal, L 1 = (x, ξ, y, η T R n T R n : x = y, ξ = η}, which is the lift of W F h (g in (1.9 from in T R n to in T R n T R n ; The bicharacteristic flowout Φ t in the positive direction from the intersection of L 1 and the bicharacteristic variety S R n S R n, L = (x, ξ, y, η T R n T R n : ξ = η, η = 1, x = y + tη, t 0}. R is the same except it would be the bicharacteristic flowout in the negative direction. When we subtract them in (1.6, the diagonal part cancels and de is associated to the flowout L 0 in both directions, from the intersection of L 1 and the characteristic variety: L 0 = (x, ξ, y, η T R n T R n : ξ = η, η = 1, x = y + tη, t R}. The above characterization can also been seen in the proof of Theorem 1.1 in Section, as we cut the kernel into near-diagonal and off-diagonal parts, which correspond to the two Lagrangian submanifolds. Organisation of the paper. In Section, we prove Theorem 1.1 and in Section 3 we prove Theorem 1.. In Section 4, we show that all of these estimates are essentially sharp, and then give some further remarks concerning the relation between these bounds and the convexity of the domain. In the appendix, we prove the mapping norms of semiclassical layer operators and show that the estimates are nearly sharp. Throughout this paper, A B (A B means A cb (A cb for some constant c depending only on the domain, in particular, independent of ; A B means A B and B A; the constants c and C may vary from line to line. Acknowledgements. The problems considered in this paper were brought to us by Andrew Hassell, we thank him for the helpful discussion throughout the preparation. We also thank Alex Barnett for informing us the related work of Chandler-Wilde et al. J.G. would like to Maciej Zworski for valuable guidance, Hart Smith for discussion of sharpness of single layer operator estimates, and Andrew Hassell for discussion of sharpness of the double layer operator estimates. J.G. is grateful to the National Science Foundation for support under the National Science Foundation Graduate Research Fellowship Grant No. DGE 1106400 and grant DMS-101417. X. H. acknowledges the support of the Australian Research Council through Discovery Project DP1010019.

6 XIAOLONG HAN AND MELISSA TACY WITH AN APPENDIX BY JEFFREY GALKOWSKI. Boundedness of semiclassical single layer potentials We aim to use previously know bounds for restriction of quasimode to hypersurfaces, both in the general and curved cases. We want mapping norm bounds for S + : L ( Ω L (Ω. However to use prior results on restriction of quasimodes we actually study the adjoint operator (S + : L (Ω L ( Ω. Now (.1 (S + u(x = K(x yu(ydy, Ω where ( K = δ(x. Therefore if R Ω is the restriction operator to the boundary of Ω we must prove L (Ω L ( Ω estimates for R Ω S +. We will do this by constructing an auxiliary quasimode v defined on Rn, for which we know the restriction bounds, then the problem reduces to finding the L norm and the quasimode error of v. To begin we excise the diagonal of (S + that is let ζ : R n R + be a smooth cut off function equal to one in x y 1 and supported in x y. Then we decompose (S + as (. (S + = S 0 + S, where (.3 S 0 u(x = (.4 Su(x = Ω Ω K (x yζ K (x y ( M 1 (x y u(ydy, ( ( 1 ζ M 1 (x y u(ydy. We first show that S 0 has a better L (Ω L ( Ω mapping norm than predicted by Theorem 1.1 and therefore we may focus on the mapping norm of S. Proposition.1. Let S 0 be as defined in (.3, then (.5 S 0 u L ( Ω 3 u L (Ω. Proof. We use the explicit respresntation of K as a Hankel function. If n 3, we have that the kernel of S 0, K 0 (x, y has the bounds K 0 (x, y x y (n, and is supported in x y M 1. Fixing x we have Conversely fixing y we have Therefore by Young s inequality K 0 (x, L 1 K 0 (, y L 1 M 1 0 C M. M 1 0 C M 1. r (n r n 1 dr r (n r n dr which is better than (.5. In R, if x y M 1 S 0 u L ( Ω C M 3/ u L (Ω K 0 (x, y log ( x y C ε ( x y ε for any ε > 0. The same application of Young s inequality implies S 0 u L ( Ω C M,ε 3/ u L (Ω.

We now focus on the operator S. Let v = Su. We will treat v as a quasimode of ( h 1. Accordingly let From [7] and [15], we know that (.6 v L ( Ω h 1 4 in the general case and (.7 v L ( Ω h 1 6 LAYER POTENTIALS AND OPERATORS 7 E[v] = ( h 1v. [ ] v L (R n + h 1 E[v] L (R n [ ] v L (R n + h 1 E[v] L (R n in the case where Ω is curved. We can also obtain these bounds from [9] by considering the function e i h t v which is an approximate solution to the wave equation. It is known that (S + has mapping norm 1 from L (Ω L (R n, see for example [34]. By the arguments of Proposition.1 S 0 has mapping norm from L (Ω L (R n therefore as S = (S + S 0, v L (R n = Su L (R n 1 u L (Ω = h u L (Ω. So to obtain Theorem 1.1 it is enough to show that E[v] L (R n h u L (Ω. Rescaling this to work in terms of we require that Now v(x = Ω ( v L (R n u L (Ω. ( K(x y 1 ζ(m 1 (x y u(ydy, where ( K = δ. So applying the operator ( we have ( (.8 ( v = 1 ζ(m 1 (x y [( x K(x y]u(ydy + Ẽu, (.9 Ẽu = Ω Ω [ K(x y x (1 ζ(m 1 (x y x (1 ζ(m 1 (x y x K(x y]u(ydy. The first term in (.8 is zero as the support of ( 1 ζ(m 1 (x y is bounded away from the diagonal x = y. The second term is the error term and has kernel supported in M 1 x y M 1. It therefore suffices to show that Proposition.. If Ẽ is given by (.9, then Ẽu L (R n u L (Ω. Ẽu L (R n u L (Ω. Proof. This is similar to the proof of Proposition.1. By choosing M large enough we may assume that the argument of the Hankel function x y is large and therefore H ( β ( x y 1 x y 1 for any β. Therefore on the support of the kernel of E we have K (x y n, x K (x y n 1, x (1 ζ(m 1 (x y, x (1 ζ(m 1 (x y.

8 XIAOLONG HAN AND MELISSA TACY WITH AN APPENDIX BY JEFFREY GALKOWSKI Therefore we may write Ẽu = K(x yu(ydy, where K(x y n and is supported on M 1 x y M 1. Now Therefore by Young s inequality as required. M 1 K( L 1 n r n 1 dr 1. 0 Ẽu L (R n u L (Ω 3. Boundedness of semiclassical double layer potentials We now address the mapping norms of the double layer potential (3.1 D + u = νy K (x yu(ydσ y. Ω We proceed in a similar fashion as the proof for the single layer potential working instead with the adjoint operator (D +. Let ζ : R n R be a smooth cut off function equal to one in x 1 and supported in x. Then we decompose D as (3. (D + = D 0 + D where (3.3 D 0 u = and (3.4 Du = Ω Ω νx K (x yζ ( M 1 (x y u(ydy [ ( ] νx K(x y 1 ζ M 1 (x y u(ydy. Similar to the single layer potential case we will treat D 0 by Young s inequality and D by quasimode methods. Proposition 3.1. Let D 0 be as defined in (3.3 then Proof. We have that νx K (x y = i 4 ( [ ( x y x y ν x ( n x y D 0 u L ( Ω 1/ u L (Ω π x y π x y n n H ( n Therefore on the support of the kernel of D 0 we have that H ( n ( x y νx K (x y x y (n 1 ( ( x y 1 π x y n H ( n ( x y We cannot directly apply Young s inequality as K(, y L 1 is not bounded. However if we decompose dyadically we may use Young s inequality on each piece and, since K(x, L 1 is much better than O(1, recover something summable. Accordingly we write D 0 = where (3.5 D j 0 u = Ω j νy K (x yζ D j 0 j=0 ( M 1 (x y u(ydy Ω j = Ω y j M 1 x y j+1 M 1 }. Now applying Young s inequality to each D0 i we have D j 0 u L ( Ω ( j n 1 ( j 1 n ( j 1 n 1 u L (Ω ]

LAYER POTENTIALS AND OPERATORS 9 1/ j/ u L (Ω and therefore D 0 u L ( Ω 1/ u L (Ω as claimed. Proposition 3.. Let D be given by (3.4 then Du L ( Ω u L (Ω Proof. We note that if we define the auxiliary function w by (3.6 w = Du then (3.7 w = ν v + Ẽu where Ẽu = ( K M (x y νy ζ M 1 (x y u(ydy Ω and v is the quasimode v = Su introduced in the proof of Theorem 1.1. From [8] and [9] we know that normal derivatives of quasimodes enjoy the hypersurface restriction bound ν v L ( Ω v L (Ω therefore by the L (Ω L (R n mapping properties of the single layer potential (3.8 ν v L ( Ω u L (Ω. So we can restrict our attention to Ẽu. We write Ẽu = Ẽ(x, yu(ydy and note by Young s inequality Ẽu L ( Ω sup x,y On the support of Ẽ(x, y we have that Therefore for n we have and For n = and so for any ɛ > 0 and therefore setting ɛ < 1/ as required. Ω Ẽ(x, 1/ L1 Ẽ(, y 1/ L u 1 L (Ω. K (x y n n K (x y log n = sup Ẽ(x, n 1 n 1 x sup Ẽ(, y n 1 (n 1 1. y sup Ẽ(x, log 1 log x sup Ẽ(, y log 1 log y Ẽu L ( Ω 1+ɛ ɛ u L (Ω Ẽu L ( Ω u L (Ω

10 XIAOLONG HAN AND MELISSA TACY WITH AN APPENDIX BY JEFFREY GALKOWSKI 4. Sharp examples and further remarks In this section, we construct examples to show that the estimates in Theorems 1.1 and 1. are in fact sharp. That is, we prove that lower bounds hold in some domains for some sequences of functions. Furthermore, we make some remarks on single layer potentials and spectral measure operators in strictly convex domains. 4.1. Sharpness of Theorem 1.1: Semiclassical single layer potentials in general domains. In the view of the Stone s formula (1.6 and Proposition 1.4, we only need to prove the sharpness of de, and then the sharpness of S follows immediately. In fact, we construct functions f } on the square [ 1, 1] n 1 such that (4.1 de (f dσ L ([ 1,1] n 1 [0,1] f L ([ 1,1] n 1 c 3 4. Throughout this subsection, we denote x = (x, x n R n where x R n 1 and x n R. We develop our sharp example through a series of lemmas. First we observe the following fact. Lemma 4.1. Write Ω = [ 1, 1] [ 1, 1] R n 1, for 0 there exists an L normalized function f such that (1 supp f Ω, ( ˆf 0, (3 ˆf (ξ c 1 if ξ η 1 for η = (, 0,..., 0 and some positive constant c 1 depending only on the dimension. Proof of Lemma 4.1. Fix a Schwartz function ϕ such that ˆϕ 0 and ˆϕ = 1 in Ω. Let f 0 = ϕχ Ω / ϕχ Ω L (R n 1, obviously supp f 0 Ω, and we verify that f 0 also satisfies ( and (3 above. Since χ Ω is even, and n 1 ˆχ Ω (ξ sin(ξ i =, ξ i we obtain ˆf 0 = c ˆϕ ˆχ Ω 0. Now we compute ˆf 0 (ξ = c ˆϕ(η ˆχ Ω (ξ η dη c R n 1 i=1 η 1 ˆχ Ω (ξ η dη c 1, if ξ η 0 1. Therefore if we set f (x = e ix η f 0 (x, we have constructed of function that satisfies all the required condtions. Now denote Ω = Ω [0, 1] R n, and let supp f Ω x n = 0}. We claim that f is our desired sharp example. That is de (f dσ L (Ω = de (fdσχ Ω L (R n c 3 4. To facilitate our calculation we will replace χ Ω with a function g designed to make calculation on the Fourier transform side easy. We need the following lemma. Lemma 4.. There exists a function g such that (1 supp g Ω, ( 0 g c for some constant c > 0 depending only on the dimension, (3 ĝ(ξ c 3 in ξ c 4 } for some positive constants c 3 and c 4 1 dimension. depending only on the Proof of Lemma 4.. Fix z = (0,..., 0, 1 Ω, and write ϕ = χ x z 1. Let g = ϕ ϕ, then both (1 4 and ( above are satisfied, and [ ] ĝ(0 = [ ˆϕ(0] = ϕ(xdx > 0. R n Thus, ĝ(ξ c 3 in ξ c 4 } because ĝ is continuous. In order to evaluate de (f dσ L (Ω, notice that f dσ(ξ = ˆf (ξ and [de (f dσ] (ξ = δ( ξ f dσ(ξ = ˆf (ξ dµ,

LAYER POTENTIALS AND OPERATORS 11 where dµ is the surface measure on ξ = }. Using the function g constructed in Lemma 4., for any ξ such that ξ 0 ξ c 4 and ξ η 1 } := G, we have [de (f dσ] ĝ(ξ c 3 ˆf (η dµ c c 1 c 3 c4 n 1, η =} η ξ c 4 } in which we use the geometric fact that the area measure η = } η ξ c 4 } c4 n 1 if ξ is a fixed point near the sphere with 0 ξ c 4 < 1 4. Recall that η = (, 0,..., 0, then the volume measure of G has G = 0 ξ c 4 and ξ η 1 }. Therefore, de (f dσg L (R n = c [de (f dσ] ĝ L (R n c 1 G 1 c 3 4. Now, since g is supported in Ω and bounded from above, de (f dσ L (Ω = de (f dσχ Ω L (R n c 1 de (f dσg L (R n c 3 4, and we have obtained (4.1. 4.. Sharpness of Theorem 1.1: Semiclassical single layer potentials in curved domains. As in Section 4.1, we only need to prove the sharpness of de. We construct functions f } such that de (f dσ L (4. (Ω c 5 6 f L ( Ω where Ω is annulus. Let B 1 = x R, x < 1}, B = x R, x < }, and Ω = x R, 1 < x < }. We work in polar coordinates (r, θ and set f k (x = e ikθ L ( Ω. Then u(x = de (f k dσ(x = aj k (re ikθ, in which J k is the Bessel function of the first kind and order k. We pick = j k,1 as the first positive zero of J k. Then u solves the Dirichlet boundary value problem u = u in B 1, We need to show that u = 0, r u = e ikθ on B 1. u L (Ω c 5 6. From [8, Section 10.1.40], J k ( = O(k 3. Thus 1 (4.3 a = J k ( = O(k 1 3. We also have (4.4 = k + c 5 k 1 3 + O(k 1 3, where c 5 = 1.86... is an independent constant. Since ( + u = 0, [ r + 1 ( ] r r + k r u = 0. Furthermore, r u(x = aj k (reikθ and r u(x = a J k (reikθ. To evaluate u L (Ω, notice that in R n, = r + n 1 r + 1 r r S n 1, in which S n 1 is the Laplacian on the sphere S n 1. Then the commutator [ [, r r ] = r + n 1 r + 1 ] r r S n 1, r r

1 XIAOLONG HAN AND MELISSA TACY WITH AN APPENDIX BY JEFFREY GALKOWSKI = [ r, r r ] + = r + =. [ n 1 r (n 1 r + r r S n 1 Using the above facts and Green s formula, we have u = u ū = which implies (4.5 x <R x <R = = = = = x <R x <R x <R x =R x =R x =R ] [ ] 1 r, r r + r S n 1, r r x <R [ +, r r ]u ū [, r r ]u ū ( + (r r u ū r r u ( + ū r (r r u ū r r u r ū r u ū + r r u ū r r u [ r( k r ]u ū r r u = a πr [ ( k R (J k (R + (J k(r ], u = a πr [( ] 1 k R (J k (R + (J k(r. If R = 1, then note that is a zero of J k. As (4.3 gives a 1 3 and J k ( = J k (j k,1 3 in [8, Section 10.1.40], ( 1 (4.6 u L (B 1 = u = a π J k( = c 1. x <1 If R =, then (4.7 u L (B = a π [( ] 1 1 k 4 (J k ( + (J k( c 5 6. Here, we use the asymptotic expansions of Bessel functions for large orders in [8] ( 1 ( 1 J k (k sec β cos k tan β kβ 1 k tan β 4 π, and ( 1 ( sin(β J k(k sec β sin k tan β kβ 1 k 4 π, in which sec β = /k in the view of (4.4, and thus β π 3. Therefore, as required. u L (Ω = u L (B u L (B 1 c 5 6, 4.3. Further remark: Semiclassical single layer potentials in strictly convex domains. If we choose R = 1 + ε in (4.5 for any fixed ε > 0, then (4.7 u L (B 1+ε c 5 6 is valid when k, and therefore, is large. (We can argue similarly by setting β asymptotically fixed depending only on ε. Comparing (4.6 and (4.7, we see that the L norm of u is essentially concentrated outside the disc. As discussed in the Introduction, this is because the estimates are dominated by the semiclassical singularities of u, which propagate along the tangent lines of the circle. All such lines lie outside of B 1. Therefore, u L (B 1 1 is smaller than u L (B 1+ɛ \B 1 5 6.

LAYER POTENTIALS AND OPERATORS 13 However, in the case when the domain is flat as in Section 4.1, the tangent lines coincide with the boundary, one may get worse L bound for u ( 3 4. The above observation motivates us to consider the problem in strictly convex domains, in which case all the tangent lines lie outside the domain. Analogously to the unit disc, we make the following conjecture. Conjecture 4.3. If Ω is strictly convex, then (4.8 S (f L (Ω c 1 f L ( Ω, and (4.9 de (fdσ L (Ω c 1 f L ( Ω. The computation in Section 4. already gave the sharp example in this case once one observes (4.6, which says de (f dσ L (Ω = c 1 f L ( Ω is valid in the unit ball for some constant c and functions f }. In fact, the estimates in Conjecture 4.3 are sharp in any strictly convex domain: From [1, 16, 17], u L (Ω 1 ν u L ( Ω, where u is a Dirichlet eigenfunction in Ω, therefore u = S ( ν u, and (4.8 and (4.9 are sharp in all strictly convex domains. 4.4. Sharpness of Theorem 1.: Semiclassical double layer potentials. We show the sharpness in the unit ball: D (f dσ L (4.10 (Ω c f L ( Ω for some constant c and functions f }. Consider the Neumann eigenfunctions: u = u in B 1, ν u = 0, u = e ikθ on B 1. Then, adopting the same notations as in Section 4., we have u(x = D (f k dσ(x = aj k (re ikθ, in which = j k,l is the l-th zero of J k, and a = 1/J k(. We use identity (4.5 with R = 1 and J k ( = 0 to obtain ( 1 u L (B 1 = u = π (1 k x <1 c, by picking k. In fact, = j k,l as l k. On the other hand, to saturate the inequality (1.5: u L ( B 1 1 3 u L (B 1, we pick = j k,1 as the first zero of J k. From [8, Section 10.1.40], we have then As u L ( B 1 1 this implies that = j k,1 = k + O(k 1 3, ( u L (B 1 = π 1 k (j k,1 = O(k 1 3 = O( 1 3. u L ( B 1 c 1 3 u L (B 1. See also [16, Example 7] on the boundary estimates of Neumann eigenfunctions.

14 XIAOLONG HAN AND MELISSA TACY WITH AN APPENDIX BY JEFFREY GALKOWSKI Appendix A. The Single and Double Layer Operators By Jeffrey Galkowski i In this appendix, we give high frequency estimate for the double and single layer operators. We do this by adapting the methods of [14] to the double layer operator. The estimates on single layer operators appear in [14, Theorem 1.], but we repeat them below for the convenience of the reader. We use the same notation as in the prequel. In addition, let γ : H s (R d H s 1/ ( Ω, s > 1/ denote restriction to Ω. Then, define the single layer operator, and the double layer operator where S + := γs+ : L ( Ω L ( Ω D + f(x = D + : L ( Ω L ( Ω Ω νy K (x yf(ydy. Theorem A.1. Let Ω R d be a finite union of compact embedded C hypersurfaces. Then there exists 0 such that for > 0, (A.1 S + L ( Ω L ( Ω C 1 log, D + L ( Ω L ( Ω C 1 4 log. Moreover, if Ω is a finite union of compact subsets of curved C hypersurfaces, then (A. S + L ( Ω L ( Ω C 3 log, D + L ( Ω L ( Ω C 1 6 log. Moreover, modulo the factor log, all of the above estimates are sharp. Such mapping bounds of layer operators in lower dimension cases (d =, 3 have been studied by Chandler-Wilde, Graham, Langdon, and Lindner [5]. In particular, they showed the upper bounds S + L ( Ω L ( Ω c (d 3/ and D + L ( Ω L ( Ω c (d 1/. In -dim, they also proved that S + L ( Ω L ( Ω c 1/ if Ω contains a flat piece and c /3 if Ω is curved. In -dim they also show the existence of Ω with D + L ( Ω L ( Ω C 1/4 and curved Ω with D + L ( Ω L ( Ω C 1/8. The special cases of the circle and sphere are studied previously by various authors. We refer to [5] for more background in this area. This appendix improves these estimates by giving nearly sharp bounds in all dimensions. We also point out that the approaches to prove estimates for semiclassical layer potentials and operators are completely different. In section A.1 we prove the upper bounds in Theorem A.1. In sections A. and A.3 we show that the exponents on in Theorem A.1 are sharp. Remark: If we impose the condition that Ω is convex with piecewise smooth, C 1,1 boundary, then we expect that D + is uniformly bounded in but we do not consider that here. A.1. Proof of Theorem A.1. To analyze the single and double layer operators, we rewrite them in terms of the outgoing free resolvent. In particular, we have that S + = γr+ γ where R + is the outgoing free resolvent. To understand D + in relation to the free resolvent, we let L be a vector field with L Ω = ν. Then, for x 0 Ω, x Ω, we have D + f(x = lim R + x 0 x (x 0 y(l (fdσ(y 1 f(x = lim x 0 x R+ L (fdσ(x 0 1 f(x. where L = L divl and R 0 is the outgoing free resolvent (see for example [19, Section 5], [30, Section 7.11]. Moreover, D + : L ( Ω L ( Ω. Let := +. i J.G. s address is Department of Mathematics, University of California, Berkeley, CA 9470-3840, USA, and e-mail address is jeffrey.galkowski@math.berkeley.edu.

LAYER POTENTIALS AND OPERATORS 15 Lemma A.. Suppose that for Γ R d any compact embedded C hypersurface, and some α, β > 0, (A.3 L fδ Γ (ξδ( ξ rdξ C Γ r α f L (Γ, (A.4 fδ Γ (ξδ( ξ rdξ C Γ r β f L (Γ. Let Γ 1, Γ R d be compact embedded C hypersurfaces. Let L be a vector field with L = ν on Γ 1 for some choice of normal ν on Γ 1 and ψ C0 (R with ψ 1 in neighborhood of 0. Then define for f L (Γ 1, g L (Γ Q 0,Γ 1,Γ (f, g := R + (ψ( 1 Dfδ Γ1 ḡδ Γ, Q 1,Γ 1,Γ (f, g := R + (ψ( 1 DL (fδ Γ1 ḡδ Γ. Then for Im > 0, c > 0, (A.5 (A.6 Q 0,Γ 1,Γ (f, g C Γ1,Γ α 1 log f L (Γ 1 g L (Γ Q 1,Γ 1,Γ (f, g C Γ1,Γ,ψ α+β 1 log f L (Γ 1 g L (Γ Proof. We follow [14] to prove the lemma. First, observe that due to the compact support of fδ Γ, (A.3 and (A.4 imply that for Γ R d, ξ L fδ Γ (ξ (A.7 (A.8 Now, gδ Γ H 1 ɛ (R d, and δ( ξ r C r α f L (Γ, fδ ξ Γ (ξ δ( ξ r C r β f L (Γ. (A.9 R + (ψ( 1 D L (fδ Γ1 C (R d, R + (ψ( 1 D fδ Γ1 C (R d. We only consider c > 0 to avoid considering the low frequency divergence in low dimensions. However, this can be handled as in [14]. By Plancherel s theorem, Q 1,Γ 1,Γ (f, g = ψ( 1 L ξ fδ Γ1 (ξ gδ Γ (ξ ξ, Q 0,Γ 1,Γ (f, g = ψ( 1 fδ ξ Γ1 (ξ gδ Γ (ξ ξ. Thus, to prove the lemma, we only need estimate (A.10 ψ( 1 F (ξ G(ξ ξ ξ where by (A.3, (A.4, (A.7, and (A.8 F L (Sr d 1 + ξf L (Sr d 1 C r δ 1 f L (Γ, G L (Sr d 1 + ξg L (Sr d 1 C r δ g L (Γ. Consider first the integral in (A.10 over ξ 1. Since ξ ξ, by the Schwartz inequality, (A.3, and (A.4 this piece of the integral is bounded by F (ξ G(ξ ψ( 1 ξ ξ 1 ξ 1 M r 1 r F (rθ G(rθdS(θdr Sr d 1 C f L (Γ g L (Γ r δ 1+δ 1 r 1 dr M r 1 C f L (Γ g L (Γ δ 1+δ 1 r 1 dr M r 1 (A.11 C δ 1+δ 1 log f L (Γ g L (Γ. Remark: The estimate (A.11 is the only term where the log appears. Next, if Im 1, then ξ, and by (A.3, (A.4 F (ξ G(ξ ξ dξ C δ 1+δ 1 f L (Γ g L (Γ. ξ 1 Thus, we may restrict our attention to 0 Im 1 and ξ 1.

16 XIAOLONG HAN AND MELISSA TACY WITH AN APPENDIX BY JEFFREY GALKOWSKI We consider Re 0, the other case following similarly, and write 1 ξ = 1 ξ ξ + ξ ξ log( ξ, where the logarithm is well defined since Im( ξ < 0. Let χ(r = 1 for r 1 and vanish for r 3. We then use integration by parts, together with (A.3, (A.4, (A.7, and (A.8 to bound 1 ξ χ( ξ F (ξ G(ξ ξ + ξ ξ log( ξ dξ C δ 1+δ 1 f L (Γ g L (Γ. Now, taking δ 1 = δ = α gives (A.5, and taking δ 1 = α and δ = β gives (A.6. We now prove the estimates (A.3 and (A.4. Lemma A.3. Let Γ R d be a compact C embedded hypersurface. For L = ν on Γ, estimate (A.3 holds with α = 1. Estimate (A.4 holds with β = 1/4. Moreover, if Γ is curved, then (A.4 holds with β = 1/6. Proof. Let A : H s (R d H s 1 (R d. To estimate A (fδ Γ (ξ δ( ξ r, write A (fδ Γ (ξδ( ξ r, φ(ξ = A (f(xδ Γ δ( ξ rφ(ξe i x,ξ dxdξ = where (A.1 T r φ = δ( ξ rφ(ξe i x,ξ dξ. Γ fat r φdx For χ C 0 (Rd, χt φ is a quasimode of the Laplacian with eigenvalue = r in the sense of [7]. Thus, we can use the restriction bounds for eigenfunctions found in [4], [15], [8], and [7], to obtain estimates on T φ. To prove (A.4, let A = I. Then, by [4, Theorem 3], [7, Theorem 1.7] (A.13 χt r φ L (Γ r 1 4 χt φ L (R d, and if Γ is curved, then by [15, Theorem 1.3] (A.14 χt r φ L (Γ r 1 6 χt φ L (R d. Remark: Estimates (A.13 and (A.14 continue to hold on C 1,1 and C,1 curved hypersurfaces respectively ([3] [14]. Next, we take A = L to obtain (A.3. Observe that χlt r φ = LχT r φ + [χ, L]T r φ with [χ, L] C 0 (Rd. Therefore, [χ, L]T r φ is a quasimode of the Laplacian with eigenvalue r. Hence, using the fact that L = ν on Γ together with [8, Theorem 0.3], we can estimate LT φ. (A.15 χlt r φ L (Γ LχT r φ L (Γ + [L, χ]t r φ L (Γ Cr χt r φ L (R d. To complete the proof of the Lemma, we estimate χt φ L (R d. We have that χt r φ L (R d = ˆχ gδ( ξ r L (R d. Therefore, ˆχ gδ( ξ r L (R d = ˆχ(ξ ηg(ηdη dξ Sr d 1 g ˆχ(ξ η dηdξ L (Sr d 1 Sr d 1 g L (Sr d 1 S d 1 r C N ξ r N dηdξ C g L (S d 1 r. Combining this with (A.13, (A.14 and (A.15 completes the proof of the Lemma.

LAYER POTENTIALS AND OPERATORS 17 To complete the proof of Theorem A.1 we need an estimate on the high frequency component of S + and D +. Let γ± : H s (Ω ± H s 1/ ( Ω, s > 1/ denote the restriction map where Ω + = Ω and Ω = R d \ Ω. Then we have Lemma A.4. Let M > 1 and ψ C0 (R with ψ 1 for ξ < M. Suppose that Ω is a finite union of compact embedded C hypersurfaces. Then (A.16 (A.17 γr + (1 ψ( 1 D γ = O L ( Ω L ( Ω( 1, γ ± R + (1 ψ( 1 D L γ = O L ( Ω L ( Ω(1. Proof. Let h 1 =. Then R + h (1 ψ(hd h Ψ (see, for example, [13, Theorem 3] where Ψ k 1 denotes the class of semiclassical pseudodifferential operators of order k (see [36] for a detailed account of the theory of semiclassical analysis. Now, let Γ 1, Γ R d be embedded C hypersurfaces and denote by γ i : H s (R d H s 1/ (Γ i, s > 1/ and by γi its adjoint. Then (A.18 γ i = O H s (R d H s 1/ (Γ i (h 1/. Hence, we have γ i R + h (1 ψ( hd γ 1 j = O L L (h. Since γ = i γ i, we have proven estimate (A.16 The strategy for obtaining the bound (A.17 will be to compare D + at high frequency with the corresponding operators for = 0. First, observe that R 0 + (1 ψ( hd h Ψ. We consider A h 1 := (R + h R + 1 0 (1 ψ( hd = h R + h R + 1 0 (1 ψ( hd. Hence, A h 1 h Ψ 4. We will bound To do so, consider the adjoint B h := γ i A h 1(1 ψ( hd L γ j. B h = γ j L(1 ψ( hd A h 1γ i. Then, observe that since Γ j is smooth, we may extend L off of Γ j to a smooth vector field, L, without changing B h. Hence, using (A.18, and the fact that L = O H s H s 1(h 1, we have that B h = O L L (1. Now, by [19, Section 5] γ ± R + 0 (1 ψ( hd L γ : L ( Ω L ( Ω for Ω a finite union of compact embedded C hypersurfaces. Hence, γ ± R + h 1 (1 ψ( hd L γ = γ ± R + 0 (1 ψ( hd L γ + γa h 1L γ = O L ( Ω L ( Ω(1 and we have proven (A.17 Taking Ω = i Γ i and applying Lemmas A. and Lemma A.4 finishes the proof of Theorem A.1. A.. Sharpness of the single layer operator estimates. We now show that the estimates on S + in Theorem A.1 are sharp modulo the log losses. We use a different approach from that in [5, Theorem 4.] where the authors construct examples giving the same lower bounds. These examples rely on the concentration of semiclassical singularities in small neighborhoods of glancing rays. First, recall as above that the spectral measure operator is denoted by de (see (1.6. Then, (A.19 But, de has kernel Thus, γde γ = S+ S πi 1 (π d e i x y,ξ dξ. S d 1 γde γ = C d 1 γt T γ.

18 XIAOLONG HAN AND MELISSA TACY WITH AN APPENDIX BY JEFFREY GALKOWSKI where T is the operator in (A.1. By [4], [15], the estimates (A.13 and (A.14 are sharp and hence for 0, C γde γ 1 Γ general L (Γ L (Γ C 3 Γ curved. Putting this together with (A.19 gives that as desired. S + L (Γ L (Γ C 1 Γ general C 3 Γ curved A.3. Sharpness of the double layer operator estimates. We will show that there exist smooth embedded hypersurfaces Γ such that for 0, C (A.0 D + 1/4 Γ general L (Γ L (Γ C 1/6 Γ curved. In the flat case, our examples are adaptations of those given in [5, Theorems 4.6] to higher dimensions. However, in the curved case, the example we provide is more subtle and improves the lower bound D + L (Γ C 1/8 given in [5, Theorem 4.7] The idea will be to use a family functions which is microlocalized at a point ((x, 0, ξ T Γ such that ξ < 1 and the geodesic (x, 0 + t(ξ, 1 ξ : t R} is tangent to Γ at some point away from (x, 0. A.3.1. Flat case. Let Γ 1 := (x 1, x, x R d : 1/ < x 1 < 3/, x = 0, x < 1} Γ := (x 1, x, x R d : x 1 = 0, x + x < 1}. Let χ Cc (R d 1 have χ 0, χ L = 1, and ˆχ(0 1/. That is χ(x, x dx dx 1/. Then, denote by χ := χ(m γ (x, x and observe that χ L = C M (d 1γ/, χ dx dx C M (d 1γ where M > 0 will be chosen later and γ 1/. Now, let Γ R d be a smooth embedded hypersurface such that Γ 1 Γ Γ. Suppose also that f L (Γ is supported on Γ. Then, D + f Γ 1 = ( νy R + (x yf(ydy Γ Now, for x y > ɛ, (A.1 νy R + (x y = C d d 1 x y, ν y ( e i x y (d 1/ x y (d 1/ + O(( x y (d+1/ x y We will consider χ as a function in L (Γ. Thus, since for x Γ 1 and y Γ, x y ɛ, we consider (d 1/ e i x y x y, ν y Γ x y (d+1/ χ (ydy. We are interested in obtaining lower bounds for the L norm on Γ 1. In particular, let ψ C0 ψ(z = 1 for z 1. Then, let ψ,1 (z = ψ(m γ z and ψ, (z = ψ(m γ z. We estimate u = ψ, (x 1 1ψ,1 (x (d 1/ e i x y x y, ν y Γ x y (d+1/ χ (ydy on Γ 1. For x Γ 1 supp ψ,1 (x ψ, (x 1 1 and y supp χ (A. x y, ν y x y = 1 + O( γ, x y = x 1 (1 + O( γ. (R with

Hence, we have u Γ1 = C d ψ, (x 1 1ψ,1 (x (d 1/ e ix 1 and on x < M 1 γ, LAYER POTENTIALS AND OPERATORS 19 x (d 1/ 1 u Γ1 (x 1, x Cψ, (x 1 1 (d 1/ (1 + O( 1 γ M + O( M γ χ dy χ dy C (d 1/ (d 1γ. So, u L (Γ 1 C Γ 1 x <C γ ψ,(x 1 1 d 1 (d 1γ C d 1 (3d 4γ γ. Thus, using elementary estimates on the remainder terms D + χ C u C d 1 (3d 4γ γ. Hence, D + χ C (d 1(1 γ+γ γ. χ Thus, choosing γ = 1/, γ = 0 and M large enough, as desired. D + χ C 1/4 χ A.3.. Curved case. In order to obtain the lower bound in the curved case, we will need to arrange to hypersurfaces, Γ 1 and Γ parametrized respectively by γ, σ : B(0, ɛ R d 1 R d such that γ(x σ(y = γ(0 σ(0 + O( x 1 y 1 3 + O( x y where x = (x 1, x R d 1. To do this, let γ : ( ɛ, ɛ R be a smooth unit speed curve with curvature κ(t = γ (t and normal vector n(t = γ (t/κ(t. We assume κ(0 0 and κ (0 0. Then, let σ(t be the loci of the osculating circle for γ(t. That is, σ γ Finally, define Figure 1. We show an example of a curve γ and its loci of osculating circles, σ. σ(t = γ(t + n(t κ(t. γ(x := ( γ(x 1 + n(x 1 x, x, σ(x := ( σ(x 1 + γ (x 1 x, x. Then we have γ(y σ(x = γ(y 1 σ(x 1 + O( x + y + x y. Let d(x 1, y 1 = γ(y 1 σ(x 1. Then, Hence, x1 d(x 1, x 1 = x 1 d(x 1, x 1 = 0. d(x 1, y 1 = d(x 1, x 1 + O( x 1 y 1 3

0 XIAOLONG HAN AND MELISSA TACY WITH AN APPENDIX BY JEFFREY GALKOWSKI and we have near x = y = 0, Moreover, Now, with χ C 0 (Rd 1, let Then, γ(y σ(x = γ(0 σ(0 + O( x 1 y 1 3 + O( x + y. σ(x γ(y, ν y γ(y σ(x χ L (R d 1 = C M d γ 1 γ 1, = 1 + O( x y. χ = χ(m( γ 1 x 1, γ x. B(0,ɛ χ dx 1 dx C M (d γ γ 1. Next, define χ,1 L (Γ 1 by χ,1 (γ(y := χ (y and χ, L (Γ by χ, (σ(x := χ (x. Then (A.3 χ,1 L (Γ 1, χ, L (Γ C χ L (R d 1, χ,1, χ, C χ. Γ 1 Γ B(0,ɛ Moreover, for x, y supp χ (A.4 γ(y σ(x = γ(0 σ(0 +O(M 1 ( 3γ 1 + γ σ(x γ(y, ν y, = 1+O( γ 1 + γ. γ(y σ(x Hence, choosing γ 1 = 1/3 and γ = 1/ and M large enough, using (A.3, (A.4 in (A.1 we have χ, (xd + χ,1 L (Γ C d 1 d 1 3 d 4 1 6 which implies D + χ,1 L (Γ C 1 6 χ,1 L (Γ 1. All that remains to show is that Γ and Γ 1 can be chosen so that they are curved. To see this, let γ be a unit speed reparametrization of t (t + 1, (t + 1. (This example is shown in Figure 1. Then, a parametrization of Γ 1 is given by ( (t, x (t + 1, (t + 1 ( (t + 1, 1 + 1 + 4(t + 1 x, x and a parametrization of Γ is given by (t, x ( ( 4(t + 1 3, 3(t + 1 + 1 + (1, (t + 1 1 + 4(t + 1 x, x. Then, a simple calculation verifies that near (0, 0 these surfaces are curved. Hence, letting Γ be a curved hypersurface containing Γ 1 and Γ completes the proof of the estimate (A.0 References [1] C. Bardos, G. Lebeau, and J. Rauch. Sharp sufficient conditions for the observation, control, and stabilization of waves from the boundary. SIAM J. Control Optim., 30(5:104 1065, 199. [] A. Barnett and A. Hassell. Fast computation of high frequency dirichlet eigenmodes via the spectral flow of the interior neumann-to-dirichlet map. arxiv:111.5665, 011. [3] M. Blair. l q bounds on restrictions of spectral clusters to submanifolds for low regularity metrics. Analysis and PDE, To appear. [4] N. Burq, P. Gérard, and N. Tzvetkov. Restrictions of the Laplace-Beltrami eigenfunctions to submanifolds. Duke Math. J., 138(3:445 486, 007. [5] S. N. Chandler-Wilde, I. G. Graham, S. Langdon, and M. Lindner. Condition number estimates for combined potential boundary integral operators in acoustic scattering. J. Integral Equations Appl., 1(:9 79, 009. [6] S. N. Chandler-Wilde, I. G. Graham, S. Langdon, and E. A. Spence. Numerical-asymptotic boundary integral methods in high-frequency acoustic scattering. Acta Numer., 1:89 305, 01. [7] D. Colton and R. Kress. Inverse acoustic and electromagnetic scattering theory, volume 93 of Applied Mathematical Sciences. Springer-Verlag, Berlin, second edition, 1998. [8] NIST Digital Library of Mathematical Functions. http://dlmf.nist.gov/, Release 1.0.6 of 013-05-06. [9] L. El-Hajj and J. Toth. Intersection bounds for nodal sets of planar neumann eigenfunctions with interior analytic curves. arxiv:111.3395, 01. [10] E. B. Fabes, M. Jodeit, Jr., and N. M. Rivière. Potential techniques for boundary value problems on C 1 -domains. Acta Math., 141(3-4:165 186, 1978. [11] X. Feng and D. Sheen. An elliptic regularity coefficient estimate for a problem arising from a frequency domain treatment of waves. Trans. Amer. Math. Soc., 346(:475 487, 1994.

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