ON RADON TRANSFORMS AND THE KAPPA OPERATOR. François Rouvière (Université de Nice) Bruxelles, November 24, 2006

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ON RADON TRANSFORMS AND THE KAPPA OPERATOR François Rouvière (Université de Nice) Bruxelles, November 24, 2006 1. Introduction In 1917 Johann Radon solved the following problem : nd a function f on the Euclidean plane R 2 knowing its integrals Rf() = f along all lines in the plane. The operator R is now called the Radon transform. Apart from an important contribution by Fritz John (1938) the problem fell into oblivion for about four decades, until it was given a nice general di erential geometric framework on the one hand and applications in medicine or physics on the other hand. In a radiograph of the human body the brightness of each point is determined by the absorption of X-ray light by bones and tissues, integrated along each ray. More generally let X be a manifold and let Y be a family of submanifolds of X equipped with measures dm (e.g. induced by a Riemannian measure on X). The Radon transform of a function f on X is the function Rf on Y de ned by Rf() = f(x) dm (x), 2 Y, x2 if the integral converges. The study of R is part of integral geometry. Problem 1 (inversion formula) : Reconstruct f from Rf. A natural tool here is the dual Radon transform ' 7! R ', mapping functions ' on Y into functions on X, with R '(x) = '() dm x (), x 2 X. 3x Thus ' is integrated over all all submanifolds containing the point x, with respect to a suitably chosen measure dm x. The corresponding di erential geometric framework (Helgason, Gelfand, Guillemin,...) is a double bration X. & where is the submanifold of X Y consisting of all couples (x; ) such that x 2. Problem 2 (range theorem) : Characterize the image under R of various function spaces on X. Y 1

Problem 3 (support theorem) : Let K be a compact subset of X (e.g. a closed ball if X is a complete Riemannian manifold). Prove that supp f is contained in K if and only if Rf() = 0 for all submanifolds 2 Y disjoint from K. Only Problem 1 will be considered here. In section 2 we will obtain inversion formulas for homogeneous spaces X and Y by means of tools from Lie group theory (Helgason and others). Two methods are presented, using either convolutions or shifted dual transforms. A completely di erent approach is given in section 3 by means of a rather mysterious di erential form (the kappa operator) introduced by Gelfand and his school. 2. Radon transforms on homogeneous spaces a. Going back to J. Radon s original problem, it was a fundamental observation by S. Helgason (1966) that the set X of points and the set Y of lines in the Euclidean plane are both homogeneous spaces of a same group G, the isometry group of R 2. This led him to study the following general situation ([7] chap. II, [9] chap. I). Let X and Y be two manifolds with given origins x 0 2 X and 0 2 Y and assume a Lie group G acts transitively on both manifolds X and Y. The elements x 2 X and 2 Y are said to be incident if they have the same relative position as x 0 and 0, i.e. if there exists some g 2 G such that x = g x 0 and = g 0. In most examples the s are submanifolds of X, the origins are chosen so that x 0 2 0 and the incidence relation is simply x 2. Let K be the subgroup of G which stabilizes x 0. It is a closed Lie subgroup of G, a point x = g x 0 identi es with the left coset gk and the manifold X with the homogeneous space G=K. Likewise Y = G=H where H is the stabilizer of 0 in G. The incidence relation translates into group-theoretic terms : x = g 1 x 0 and = g 2 0 are incident if and only if there exists g 2 G such that g 1 x 0 = g x 0 and g 2 0 = g 0, i.e. i g 1 k = g and g 2 h = g for some k 2 K, h 2 H, i.e. i the left cosets g 1 K and g 2 H are not disjoint in G. The set of all incident couples (x; ) identi es with the homogeneous space G=K \ H. Let us assume that K is compact. Then the Radon transform of a function f on X can be de ned as Rf(g 0 ) = f(gh x 0 ) dh, g 2 G H where dh is a left invariant measure on H. It is easily checked that f is here integrated over all x incident to = g 0. Likewise the dual Radon transform of a function ' on Y is R '(g x 0 ) = '(gk 0 ) dk, an integral of ' over all incident to x = g x 0. K b. A detailed study of R has been be carried out by Helgason when X is a Riemannian symmetric space of the noncompact type and Y is a family of submanifolds of X. Let us start with the basic example of the two-dimensional hyperbolic space 2

X = H 2 (R). This Riemannian manifold can be realized as the open unit disc jzj < 1 in C equipped with the metric ds 2 jdzj 2 = 4 (1 jzj 2 ) 2, jdzj2 = dx 2 + dy 2. a b Here G = SU(1; 1), the group of matrices g = with a; b 2 C and det g = 1, b a acting on C by g z = az + b bz + a. The origin x 0 = 0 is stabilized by the subgroup K de ned by b = 0 whence X = G=K. Now the Euclidean lines of R 2 in Radon s original problem admit two analogues : geodesics of X, i.e. circles (or lines) meeting orthogonally the circle at in nity jzj = 1 horocycles of X, i.e. curves orthogonal to a family of "parallel" geodesics (geodesics having a common point at in nity), i.e. circles contained in jzj < 1 and tangent to jzj = 1. Which is best? The former may seem more natural from a geometric point of view, but the latter turns out to be closely related to harmonic analysis on X. Indeed its Laplace operator admits a family of eigenfunctions which are constant on each horocycle. The horocycle Radon transform is thus linked to the analogue of the Fourier transform on X. All this extends to the n-dimensional hyperbolic space X = H n (R), with (n 1)- dimensional horospheres instead of horocycles, and even to all Riemannian symmetric spaces of the noncompact type. c. The following proposition ([12] p. 215) gives a rst clue towards an inversion formula of R. Proposition 1 In the general setting of a above assume that Y = G=H has a G-invariant measure. Then R R is a convolution operator on X = G=K. Convolution on X is deduced from convolution on the Lie group G by means of the natural projection G! G=K. Idea of proof. From the de nitions of R and R it is clear that R R commutes with the action of G on X and the proposition easily follows. To invert R it is therefore su cient to nd an inverse of this convolution and harmonic analysis on X provides natural tools for that. In the next theorem C denotes various nonzero constant factors, r is the (Riemannian) distance from the origin in X, is the Laplace operator of X and f is an arbitrary function in Cc 1 (X). Theorem 2 (i) For the Radon transform on lines in R n one has R Rf = C f r 1 f = SR Rf = C ( n ) 1=2 R Rf 3

where S is the convolution operator by C r 1 n. (ii) For the Radon transform on geodesics in H n (R) one has R Rf = C f (sinh r) 1 f = ( + n 2)SR Rf where S is the convolution operator by C (sinh r) 1 n cosh r. (iii) For the Radon transform on horospheres of H n (R) one has n R Rf = C f (sinh r) 1 cosh r 2 3 n where P is a polynomial of degree k. f = P ()R Rf if n = 2k + 1, In R n the symbol denotes the usual convolution whereas if g(r) is a radial function on H n (R) (f g) (x) = f(y)g(d(x; y)) dm(y), H n (R) where d(:; :) is the Riemannian distance and dm is the Riemannian measure. See [7] p. 29 for (i), [1] p. for (ii) and [12] p. 218 and 229 for (iii). d. A di erent method, initiated by Radon himself in his 1917 paper, makes use of the shifted dual Radon transform de ned (in the group-theoretic setting of a) by R'(g x 0 ) = '(gk 0 ) dk, K with g; 2 G. The origin 0 in Y is now replaced by the shifted origin 0. Roughly speaking, instead of integrating ' over all containing x = g x 0 as was done by R (in most examples at least), we now integrate over all at a given distance from x. The shifted transform turns out to be a convenient tool to prove inversion formulas. In Theorems 3 and 4 below the origins are chosen so that x 0 2 0 and f is an arbitrary function in Cc 1 (X). Theorem 3 (i) For the Radon transform on lines in R n one has f(x) = 1 1 0 dt R(t) t Rf(x) t where (t) is a translation of length t orthogonally to the line 0. (ii) Let X = G=K be a Riemannian symmetric space of the noncompact type. The Radon transform on geodesics of X is inverted by f(x) = C 1 0 dt R(t) t Rf(x) sinh t with (t) = exp tv 2 G, V being a suitably chosen vector orthogonal to 0 in the tangent space to X at x 0. 4

Formula (i) extends Radon s result to the n-dimensional Euclidean space, (ii) is proved in [13] and independently in [10]. Idea of proof. It su ces to work at x = x 0 and, taking averages over K, with K- invariant (radial) functions f. Then (i) is proved by solving an integral equation of Abel type. For (ii) Lie bracket computations show that V and the tangent to 0 at x 0 generate a two-dimensional hyperbolic subspace of X. In this H 2 (R) the integrals can be written down explicitly and the problem boils down again to an Abel integral equation. Theorem 4 Let X = G=K be a Riemannian symmetric space of the noncompact type. The Radon transform on horospheres of X is inverted by f(x) = < T (a); R arf(x) > where the variable a runs over A, the Abelian subgroup in an Iwasawa decomposition G = KAN, and T (a) is a distribution on A. See [12] p. 236 for a proof. Here shifted dual transforms provide a simpler proof of an inversion formula due to Helgason (1964, see [9] p.116). Up to a factor T is the Fourier transform of jc()j 2 where c is Harish-Chandra s famous function. If X = H 2k+1 (R) (more generally if all Cartan subalgebras are conjugate in the Lie algebra of G) jc()j 2 is a polynomial and T, supported at the origin of A, is a di erential operator : the inversion formula from Theorem 2 (iii) can then be deduced from Theorem 4. 3. The Kappa operator Introduced by Gelfand, Graev and Shapiro (1967) to study the Radon transform on k-dimensional planes in C n the "kappa operator" has been developed in several papers by the Russian school (Gelfand, Gindikin, Graev - and Goncharov who related it to the language of D-modules). But apart from Grinberg s paper [6] it has never been used by others (to the best of my knowledge), though this di erential form seems to provide an e cient tool to invert Radon transforms in various situations. Here we introduce it in the context of the n-dimensional hyperbolic space X = H n (R), following [3] chapter 5 and several papers by Gindikin [4] [5]. a. Preliminaries. Let M be a n-dimensional manifold,! a volume form on M and S the hypersurface de ned by '(x) = 0 where ' : M! R is a C 1 function with d'(x) 6= 0 for x 2 S. Let V be a vector eld on M which is transversal to S, i.e. V '(x) 6= 0 for any x 2 S. Then the (n 1)-form = 1 V ' i V! (restricted to S) (1) is a volume form on S such that d' ^ =!. Here i V denotes the interior product de ned by (i V!) (V 1 ; :::; V n 1 ) =!(V; V 1 ; :::; V n 1 ) for any tangent vectors V 1 ; :::; V n 1. 5

Integration over S with respect to de nes a distribution (') supported in S : < ('); f >= f, f 2 Cc 1 (M), (2) and it is easily checked that S '(') = 0, (') = 1 (') (3) if is any strictly positive C 1 function on M. In the framework of microlocal analysis (') can also be de ned as the pullback (') = ' of the Dirac measure on R, which is given by the oscillatory integral (see [11] Theorem 8.2.4) < ('); f >= dt f(x)e it'(x)!(x). (4) R M b. Radon transform on a quadric. Let " 0 = 1; " i = 1 for i 1 and Q(x) = nx " i x 2 i = x 2 0 x 2 1 x 2 n. i=0 From now on we consider the upper sheet of the hyperboloid X = fx 2 R n+1 jq(x) = 1 and x 0 > 0g and the Radon transform obtained by integrating over sections of X by all hyperplanes x 0 x 0 + + n x n + n+1 = 0 that is, for f 2 C 1 c (X), 2 R n+2 n0, Rf() = < ( x); f(x) >. (5) In view of (1) above we may take the Euler vector eld V = P n j=0 x j(=x j ) as a transversal eld to X R n+1 and! = 1 V Q i V (dx 0 ^ ^ dx n ) = 1 nx ( 1) j x j dx 0 ^ ^ 2 ddx j ^ ^ dx n (6) j=0 (with dx j removed) as a volume form on X. As such we get an overdetermined problem of integral geometry : reconstruct a function f of n variables (the dimension of X) from a function of (n + 1) (dimension of the space of s, up to a factor). It is therefore to be expected that Rf satis es additional conditions (Proposition 5 below) and that knowing its restriction to some n-dimensional submanifold should su ce to reconstruct f. 6

Let us point out two interesting such submanifolds. For n+1 = 0 we obtain all planes through the origin and their intersections with X are the (n 1)-dimensional totally geodesic hypersurfaces of the hyperbolic space X. For Q( 0 ; :::; n ) = 0 we obtain the horospheres of X. This can be checked for instance by projecting X onto the plane x 0 = 0 in R n+1 from the point ( 1; 0; :::; 0). The image of X is the open unit ball of R n (the Poincaré model of hyperbolic geometry), geodesics hypersurfaces become (n 1)-spheres orthogonal to the unit sphere and horospheres become (n 1)-spheres tangent to the unit sphere (cf. 2.b above). Proposition 5 Let P ( ) = P n+1 j=0 " j(= j ) 2. For f 2 C 1 c (X) the function Rf on R n+2 n0 satis es Rf() = 1 Rf(), > 0, P ( )Rf() = 0. Proof. The homogeneity follows from (3). The di erential equation is best seen from (4) : Rf() = dt f(x)e itx!(x) R X implies P ( )Rf() = t 2 dt f(x)(q(x) 1)e itx!(x) = 0 R X since Q(x) = 1 on X. c. The kappa operator at last. It will act on functions of 2 R n+2 n0. Let d = d 0 ^ ^ d n+1 n+1 X E = j=0 j be the volume form and Euler vector eld respectively. For ' 2 C 1 (R n+2 n0) we consider the di erential n-form on R n+2 n0 j ' = i E i (d) (7) where is a vector eld on R n+2 n0 to be chosen shortly and depending on '. The goal is to obtain a closed form when ' = Rf so that R Rf will only depend on the homology class of the n-cycle. First, using the Lie derivatives L E = d i E + i E d, L = d i + i d, and the divergence de ned by L (d) = (div )d we have d' = L E (i d) (div )i E d. (8) Lemma 6 For any linear di erential operator P with C 1 coe cients on R n+2 n0 and any '; u 2 C 1 (R n+2 n0) there exists a vector eld = (P; '; u) on R n+2 n0 such that div = u P ' ' t P u, where t P is the transpose of P with respect to d. In other words d (i d) = up ' 7 ' t P u d.

Proof. (i) If P is a vector eld we may take (P; '; u) = 'up. Indeed for any vector eld V and any smooth function f div(fv ) = V f + f div V. This classical formula is easily checked from together with div(fv )d = L fv d = d(i fv d) = d(f i V d) = df ^ i V d + f d(i V d) = df ^ i V d + f (div V ) d 0 = i V (df ^ d) = (i V df) ^ d df ^ i V d = (V f) d df ^ i V d. Taking now V = 'up and for f an arbitrary compactly supported function it follows that ('up f + f div('up )) d = div(f'up )d = 0 by Stokes formula. But 'up f d = = (up (f') fup ') d f ' t P u up ' d, whence div('up ) = u P ' ' t P u as claimed. (ii) If P = P 1 P 2 is a product of two operators we may take (P 1 P 2 ; '; u) = (P 1 ; P 2 '; u) + (P 2 ; '; t P 1 u). The lemma follows by linearity and induction on the order of P. If is chosen according to the lemma with i d homogeneous of degree 0 and t P u = 0, (8) becomes d' = (up ') i E d so that ' is a closed form if (and only if) P ' = 0. Going back to our problem with P = P ( ) = P n+1 j=0 " j(= j ) 2 = t P, " 0 = 1; " j = 1 for j 1, we may take, according to Lemma 6, n+1 X ' (P; '; u) = " j u j j=0 ' u (9) j j and, for xed x 2 X, u() = u x () = ( x) 1 n. (10) Indeed t P ( )u x = n(n 1)(Q(x) 1)( x) 1 n = 0 and i d will have the required homogeneity if ' is homogeneous of degree 1. Summarizing we obtain 8

Proposition 7 Let x 2 X and ' 2 C 1 (R n+2 n0), homogeneous of degree 1. The di erential n-form x ' = i E i (d) (where E is the Euler vector eld and is given by (9) and (10)) is closed if and only if P ( )' = 0. This holds in particular if ' = Rf. A technical di culty arises here : our u x is singular when x = 0, i.e. when the hyperplane de ned by contains the given point x. It can be circumvented by replacing ( x) 1 n with the distribution i.e. the pullback of u x () = ( x i0) 1 n = lim "!0 +( x i")1 n, (t i0) 1 n = t 1 n + i( 1)n (n 2)! (n 2) (t) (11) under the map 7! x. Then x ' becomes a n-form with distribution valued coe cients and Proposition 7 remains valid. Explicitly where n+1 X = j=0 j, j = " j j ' j u x ' u x j n+1 X, x ' = j! j, (12) n+1 X! 0 = i E (d 1 ^ ^ d n+1 ) = ( 1) k 1 k d 1 ^ ^ cd k ^ ^ d n+1 (13) k=1 and the subsequent! j are obtained from! 0 by cyclic permutation of 0 ; :::; n+1 and multiplication by ( 1) (n 1)j. Remark. The above construction of x ' extends to all nondegenerate quadratic form P on R n+2 (see [4]). d. Inversion formula. Theorem 8 (Gindikin) Let f 2 Cc 1 (X) where X is the upper sheet of the n- dimensional hyperboloid. Let be any n-dimensional submanifold of R n+2 n0 homologous to the cycle 0 de ned in the proof below. The Radon transform on X is then inverted by x Rf = C f(x), x 2 X, where C = (2i) n =(n 2)!. Proof. Let us take j=0 0 = 2 R n+2 0 = 1 and 2 1 + + 2 n = 1. Any homologous n-cycle in R n+2 n0 will give the same integral since x Rf is a closed n-form by Proposition 7. For instance as a more natural but equivalent choice 9

might be de ned by 0 = 1 and 2 0 + 2 1 + + 2 n = 1. The rst condition means that we consider hyperplanes containing (1; 1; 0; :::; 0) 2 X. We now show the claim boils down to the classical inversion formula for the Radon transform on hyperplanes of R n. (i) Restricting Rf() to 0 = 1 we obtain the function ( 1 ; :::; n+1 ) Rf( 1 ; 1 ; :::; n+1 ) = < ( 1 (x 0 + x 1 ) + 2 x 2 + + n x n + n+1 ); f(x) >. The brackets are here computed by means of the volume form! on X (see (6) above). The map x = (x 0 ; :::; x n ) 7! y = (y 1 ; y 2 ; :::; y n ) with y 1 = x 0 + x 1, y 2 = x 2,..., y n = x n induces a di eomorphism of X onto the half space y 1 > 0 in R n. In view of Q(x) = x 2 0 x 2 1 x 2 n = 1 x 0 dx 0 = x 1 dx 1 + + x n dx n y 1 dx 1 ^ ^ dx n = x 0 dy 1 ^ ^ dy n it is readily checked that the volume form!(x) on X becomes e!(y) = 1 2y 1 dy 1 ^ ^ dy n. To f corresponds the function e f(y) = f(x), compactly supported in y 1 > 0. Then ( 1 ; :::; n+1 ) = < ( 1 y 1 + + n y n + n+1 ); e f(y) >, where the brackets are now computed by means of e!. In other words is the Radon tranform of the function e f(y 1 ; :::; y n )=2y 1 over hyperplanes of R n. Let c = (2i) n =(n 1)!. From a classical inversion formula (see e.g. [3] p. 11) it follows that = 2y 1 S n 1 R c f(x) = c e f(y) = ( 1 ; :::; n+1 ) ( 1 y 1 + + n y n + n+1 i0) n ^ d n+1 (14) an integral taken over all n+1 2 R and all ( 1 ; :::; n ) in the unit sphere S n volume form nx = ( 1) j 1 j d 1 ^ ^ cd j ^ ^ d n. j=1 1 with (ii) Let us now consider the restriction to of x ' with ' 2 C 1 (R n+2 n0), homogeneous of degree 1. From the de nition of we have d 0 = d 1, d 1 ^ ^ d n = 0, and! 0 =! 1 = ^ d n+1,! j = 0 for j 2 by (13). On (12) thus reduces to = 0 + 1 x ' = ( 0 1 )! 0 ': + 0 1 ':u x u x ^ d n+1. 10

But, for ' = Rf and as above, + ' ( 1 ; 1 ; :::; n+1 ) = ( 1 ; :::; n+1 ) 0 1 1 and, for u x = ( x i0) 1 n, + u x = (1 n)(x 0 + x 1 )( x i0) n. 0 1 Therefore on x Rf = ( x i0) 1 n + (n 1)y 1 ( x i0) n ^ d n+1. 1 Integrating the rst term by parts we obtain x Rf = 2(n 1)y 1 ( x i0) n ^ d n+1, where the latter integral is taken over all n+1 2 R and all ( 1 ; :::; n ) 2 S n 1. Comparing with (14) we are done. e. Examples. Geodesic hypersurfaces of X. As noted above geodesics hypersurfaces of the hyperbolic space are the sections of X by hyperplanes through the origin of R n+1, i.e. x = 0 with n+1 = 0. Now Theorem 8 applies with the cycle replaced by 1 = 2 R n+2 n+1 = 0 and 2 1 + + 2 n = 1. Indeed one can nd in the group SL(n + 2; R) a continuous curve g t, 0 t 1, from the identity to the matrix 0 0 0::::0 1 1 g 1 = 0 Id n 0 A. 1 10:::0 0 Applying it to we obtain a continuous deformation of to 1 and R 1 x Rf = C f(x). The result can be made explicit by means of (12) and (13). In! j, 0 j n, each term contains n+1 or d n+1 hence! j = 0 on 1 and x ' = ' u x n+1 ' u x! n+1. n+1 The corresponding inversion formula eventually simpli es to ([3] p. 154) 2 Rf()( x i0) n! n+1 () = C f(x). 1 11

Horospheres of X. We need here all hyperplanes x = 0 such that Q() = 2 0 2 1 2 n = 0. Adding as before the condition 2 1 + + 2 n = 1 we consider the cycle 2 = 2 R n+2 0 = 1 and 2 1 + + 2 n = 1. By continuous deformation the condition 0 = 1 can be changed into 0 = 0, then to 0 = 1 by a continuous path in SL(n + 2; R) as above. Thus Theorem 8 applies with replaced by 2 and leads to the inversion formula ([3] p.156) 2 Rf()( x i0) n! 0 () = C f(x). References [1] Berenstein, C. and Casadio Tarabusi, E., Inversion formulas for the k-dimensional Radon transform in real hyperbolic space, Duke Math. J. 62 (1991), p. 613-631. [2] Gelfand, I.M., Gindikin, S.G. and Graev, M.I., Integral geometry in a ne and projective spaces, J. Sov. Math. 18 (1980), p. 39-167 ; also in Gelfand, Collected papers, vol. III, Springer-Verlag 1989, p. 99-227. [3] Gelfand, I.M., Gindikin, S.G. and Graev, M.I., Selected topics in integral geometry, Transl. Math. Monographs 220, Amer. Math. Soc. 2003. [4] Gindikin, S.G., Integral geometry on real quadrics, Amer. Math. Soc. Transl. (2) 169 (1995), p. 23-31 [5] Gindikin, S.G., Real integral geometry and complex analysis, in Lecture Notes in Math. 1684, p. 70-98, Springer 1998 [6] Grinberg, E., That kappa operator, in Lectures in Applied Math. 30, Amer. Math. Soc. 1994, p. 93-104. [7] Helgason, S., The Radon transform, Second Edition, Progress in Math., Birkhäuser 1999. [8] Helgason, S., Groups and geometric analysis, Academic Press 1984. [9] Helgason, S., Geometric analysis on symmetric spaces, Math. Surveys and Monographs 39, Amer. Math. Soc. 1994. [10] Helgason, S., The inversion of the X-ray transform on a compact symmetric space, preprint, September 2006. [11] Hörmander, L., The analysis of linear partial di erential operators I, Springer- Verlag 1983. [12] Rouvière, F., Inverting Radon transforms : the group-theoretic approach, L Ens. Math. 47 (2001), p. 205-252. [13] Rouvière, F., Transformation aux rayons X sur un espace symétrique, C.R. Acad. Sci. Paris, Ser. I, 342 (2006), p. 1-6. 12