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Microlocal Analysis and Spectral Theory in honor of J. Sjstrand Luminy, Sept 26, 2013 Two Partial Data Problems Gunther Uhlmann University of Washington and University of Helsinki Outline: Calderns problem with partial data


  1. Microlocal Analysis and Spectral Theory in honor of J. Sjöstrand Luminy, Sept 26, 2013 Two Partial Data Problems Gunther Uhlmann University of Washington and University of Helsinki

  2. Outline: ◮ Calderón’s problem with partial data ◮ Travel time tomography with partial data

  3. CALDER ´ ON’S PROBLEM Ω ⊂ R n ( n = 2 , 3) Can one determine the electrical conductivity of Ω , γ ( x ) , by making voltage and current measurements at the boundary? (Calder´ on; Geophysical prospection) Early breast cancer detection Normal breast tissue 0.3 mho Cancerous breast tumor 2.0 mho 1

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  5. REMINISCENCIA DE MI VIDA MATEMATICA Speech at Universidad Aut´ onoma de Madrid accepting the ‘Doctor Honoris Causa’: My work at “Yacimientos Petroliferos Fiscales” (YPF) was very interesting, but I was not well treated, otherwise I would have stayed there. 3

  6. ACT3 imaging blood as it leaves the heart (blue) and fills the lungs (red) during systole.

  7. (Loading DBarPerfMovie1.avi) Thanks to D. Issacson

  8. CALDER ´ ON’S PROBLEM (EIT) Consider a body Ω ⊂ R n . An electrical potential u ( x ) causes the current I ( x ) = γ ( x ) r u The conductivity γ ( x ) can be isotropic, that is, scalar, or anisotropic, that is, a matrix valued function. If the current has no sources or sinks, we have div( γ ( x ) r u ) = 0 in Ω 11

  9. div( γ ( x ) r u ( x )) = 0 γ ( x ) = conductivity, � � u � @ Ω = f f = voltage potential at @ Ω � � Current flux at @ Ω = ( ν · γ r u ) � @ Ω were ν is the unit outer normal. Information is encoded in map � � Λ γ ( f ) = ν · γ r u � @ Ω EIT (Calder´ on’s inverse problem) Does Λ γ determine γ ? Λ γ = Dirichlet-to-Neumann map 12

  10. Theorem n ≥ 3 (Sylvester-U, 1987) γ ∈ C 2 (Ω) , 0 < C 1 ≤ γ ( x ) ≤ C 2 on Ω Λ γ 1 = Λ γ 2 ⇒ γ 1 = γ 2 • Extended to γ ∈ C 3 / 2 (Ω) (Päivarinta-Panchenko-U, Brown-Torres, 2003) • γ ∈ C 1 + ǫ (Ω) , γ conormal (Greenleaf-Lassas-U, 2003) • γ ∈ C 1 (Ω) , (Haberman-Tataru, 2013). Complex-Geometrical Optics Solutions (CGO) • Reconstruction (A. Nachman, R. Novikov 1988) • Stability (G. Alessandrini 1988) • Numerical Methods (D. Issacson, J. Müller, S. Siltanen)

  11. Reduction to Schr¨ odinger equation div( γ r w ) = 0 u = p γw Then the equation is transformed into: (∆ − q ) u = 0 , q = ∆ p γ � � n @ 2 X ∆ = p γ @x 2 i =1 i (∆ − q ) u = 0 � � u � @ Ω = f � Define Λ q ( f ) = @u � � @ Ω @ν ν = unit-outer normal to @ Ω. 16

  12. IDENTITY Z Z � � � � � � Ω ( q 1 − q 2 ) u 1 u 2 = (Λ q 1 − Λ q 2 ) u 1 u 2 � @ Ω dS � @ Ω @ Ω (∆ − q i ) u i = 0 If Λ γ 1 = Λ γ 2 ) Λ q 1 = Λ q 2 and Z Ω ( q 1 − q 2 ) u 1 u 2 = 0 GOAL: Find MANY solutions of (∆ − q i ) u i = 0. 17

  13. CGO SOLUTIONS on: Let ρ 2 C n , ρ · ρ = 0 Calder´ η, k 2 R n , | η | = | k | , η · k = 0 ρ = η + ik u = e x · ρ = e x · η e ix · k 8 > > exponentially decreasing , x · η < 0 > < ∆ u = 0, u = oscillating, x · η = 0 > > > : exponentially increasing , x · η > 0 18

  14. COMPLEX GEOMETRICAL OPTICS (Sylvester-U) n ≥ 2 , q 2 L 1 (Ω) Let ρ 2 C n ( ρ = η + ik, η, k 2 R n ) such that ρ · ρ = 0 ( | η | = | k | , η · k = 0). Then for | ρ | sufficiently large we can find solutions of (∆ − q ) w ρ = 0 on Ω of the form w ρ = e x · ρ (1 + Ψ q ( x, ρ )) with Ψ q ! 0 in Ω as | ρ | ! 1 . 19

  15. Proof Λ q 1 = Λ q 2 ) q 1 = q 2 Z Ω ( q 1 − q 2 ) u 1 u 2 = 0 u 1 = e x · ρ 1 (1 + Ψ q 1 ( x, ρ 1 )) , u 2 = e x · ρ 2 (1 + Ψ q 2 ( x, ρ 2 )) ρ 1 · ρ 1 = ρ 2 · ρ 2 = 0 , ρ 1 = η + i ( k + l ) ρ 2 = − η + i ( k − l ) | η | 2 = | k | 2 + | l | 2 η · k = η · l = l · k = 0 , Z Ω ( q 1 − q 2 ) e 2 ix · k (1 + Ψ q 1 + Ψ q 2 + Ψ q 1 Ψ q 2 ) = 0 Z Ω ( q 1 − q 2 ) e 2 ix · k = 0 Letting | l | ! 1 8 k = ) q 1 = q 2 20

  16. PARTIAL DATA PROBLEM Suppose we measure supp f ⊆ Γ 0 Λ γ ( f ) | Γ , Γ, Γ 0 open subsets of @ Ω Can one recover γ ? Important case Γ = Γ 0 . 23

  17. EXTENSION OF CGO SOLUTIONS u = e x · ρ (1 + Ψ q ( x, ρ )) ρ 2 C n , ρ · ρ = 0 (Not helpful for localizing) Kenig-Sj¨ ostrand-U (2007), u = e τ ( ' ( x )+ i ψ ( x )) ( a ( x ) + R ( x, τ )) τ 2 R , ' , ψ real-valued, R ( x, τ ) ! 0 as τ ! 1 . ' limiting Carleman weight, r ' · r ψ = 0 , |r ' | = |r ψ | Example: ' ( x ) = ln | x − x 0 | , x 0 / 2 ch (Ω) 24

  18. CGO SOLUTIONS u = e τ ( ' ( x )+ i ψ ( x )) ( a 0 ( x ) + R ( x, τ )) R ( x, τ ) τ !1 ! 0 in Ω − ' ( x ) = ln | x − x 0 | Complex Spherical Waves Theorem (Kenig-Sj¨ ostrand-U) Ω strictly convex. � � � � Λ q 1 � Γ = Λ q 2 � Γ , Γ ⊆ @ Ω , Γ arbitrary ) q 1 = q 2 25

  19. Complex Spherical Waves (Loading reconperfect1.mpg)

  20. Theorem (Kenig-Sj¨ ostrand-U) Ω strictly convex. � � � � Λ q 1 � Γ = Λ q 2 � Γ , Γ ⊆ @ Ω , Γ arbitrary ) q 1 = q 2 u τ = e τ ( ' + i ψ ) a τ ' ( x ) = ln | x − x 0 | , x 0 2 \ ch (Ω) Eikonal: r ' · r ψ = 0 , |r ' | = |r ψ | ψ ( x ) = d ( x − x 0 | x − x 0 | , ! ) , ! 2 S n − 1 : smooth for x 2 ¯ Ω. Transport: ( r ' + i r ψ ) · r a τ = 0 (Cauchy-Riemann equation in plane generated by r ' , r ψ ) 27

  21. ' ( x ) = ln | x − x 0 | , x 0 2 \ ch (Ω) Carleman Estimates > u | @ Ω = @ u @ν | @ Ω − = 0 @ Ω ± = { x 2 @ Ω; r ' · ν < 0 } Z Z < r ' , ν > | e − τ' ( x ) @ u @ν | 2 ds ≤ C Ω | (∆ − q ) ue − τ' ( x ) | 2 ds @ Ω + τ This gives control of @ u @ν | @ Ω + , δ , @ Ω + , δ = { x 2 @ Ω , r ' · ν ≥ δ } 28

  22. Outline: ◮ Calderón’s problem with partial data ◮ Travel time tomography with partial data

  23. Travel Time Tomography (Transmission) Global Seismology Inverse Problem: Determine inner structure of Earth by measuring travel time of seismic waves. 1

  24. Tsunami of 1960 Chilean Earthquake Black represents the largest waves, decreasing in height through purple, dark red, orange and on down to yellow. In 1960 a tongue of massive waves spread across the Pacific, with big ones through- out the region. 2

  25. Human Body Seismology ULTRASOUND TRANSMISSION TOMOGRAPHY(UTT) Z 1 T = = Travel Time (Time of Flight) . c ( x ) ds γ 3

  26. THIRD MOTIVATION OCEAN ACOUSTIC TOMOGRAPHY Ocean Acoustic Tomography Ocean Acoustic Tomography is a tool with which we can study average temperatures over large regions of the ocean. By measur- ing the time it takes sound to travel between known source and receiver locations, we can determine the soundspeed. Changes in soundspeed can then be related to changes in temperature. 4

  27. REFLECTION TOMOGRAPHY Scattering Obstacle Points in medium 5

  28. REFLECTION TOMOGRAPHY Oil Exploration Ultrasound 6

  29. TRA VELTIME TOMOGRAPHY (Transmission) Motivation:Determine inner structure of Earth by measuring travel times of seismic waves Herglotz, Wiechert-Zoeppritz (1905) Sound speed c ( r ), r = | x | � � d r > 0 dr c ( r ) Reconstruction method of c ( r ) from lengths of geodesics 7

  30. ds 2 = 1 c 2 ( r ) dx 2 More generally ds 2 = c 2 ( x ) dx 2 1 Velocity v ( x, ξ ) = c ( x ) , | ξ | = 1 (isotropic) Anisotropic case n X g = ( g ij ) is a positive defi- ds 2 = g ij ( x ) dx i dx j nite symmetric matrix i,j =1 qP n i,j =1 g ij ( x ) ξ i ξ j , Velocity v ( x, ξ ) = | ξ | = 1 g ij = ( g ij ) − 1 The information is encoded in the boundary distance function 8

  31. More general set-up ( M, g ) a Riemannian manifold with boundary (compact) g = ( g ij ) x, y 2 @ M d g ( x, y ) = inf L ( σ ) σ (0)= x σ (1)= y L ( σ ) = length of curve σ r R 1 P n d σ j i,j =1 g ij ( σ ( t )) d σ i L ( σ ) = dt dt 0 dt Inverse problem Determine g knowing d g ( x, y ) x, y 2 @ M 9

  32. dg ) g ? (Boundary rigidity problem) Answer NO ψ : M ! M di ff eomorphism � � � @ M = Identity ψ d ψ ∗ g = d g � D ψ ◦ g ◦ ( D ψ ) T � ψ ∗ g = ◦ ψ r R 1 P n d σ j i,j =1 g ij ( σ ( t )) d σ i L g ( σ ) = dt dt 0 dt σ = ψ ◦ σ L ψ ∗ g ( e σ ) = L g ( σ ) e 10

  33. d ψ ∗ g = d g Only obstruction to determining g from d g ? No d g ( x 0 , @ M ) > sup x,y 2 @ M d g ( x, y ) Can change metric near SP 11

  34. Def ( M, g ) is boundary rigid if ( M, e g ) satisfies d e g = d g . � � Then 9 ψ : M ! M di ff eomorphism, ψ � @ M = Identity, so that g = ψ ∗ g e Need an a-priori condition for ( M, g ) to be boundary rigid. One such condition is that ( M, g ) is simple 12

  35. DEF ( M, g ) is simple if given two points x, y 2 @ M , 9 ! geodesic joining x and y and @ M is strictly convex CONJECTURE ( M, g ) is simple then ( M, g ) is boundary rigid ,that is d g determines g up to the natural obstruction. ( d ψ ∗ g = d g ) ( Conjecture posed by R. Michel, 1981 ) 13

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