HOME

TheInfoList



OR:

In
differential geometry Differential geometry is a Mathematics, mathematical discipline that studies the geometry of smooth shapes and smooth spaces, otherwise known as smooth manifolds. It uses the techniques of Calculus, single variable calculus, vector calculus, lin ...
, Santaló's formula describes how to integrate a function on the unit
sphere bundle In the mathematical field of topology, a sphere bundle is a fiber bundle in which the fibers are spheres S^n of some dimension ''n''. Similarly, in a disk bundle, the fibers are disks D^n. From a topological perspective, there is no difference betw ...
of a
Riemannian manifold In differential geometry, a Riemannian manifold is a geometric space on which many geometric notions such as distance, angles, length, volume, and curvature are defined. Euclidean space, the N-sphere, n-sphere, hyperbolic space, and smooth surf ...
by first integrating along every
geodesic In geometry, a geodesic () is a curve representing in some sense the locally shortest path ( arc) between two points in a surface, or more generally in a Riemannian manifold. The term also has meaning in any differentiable manifold with a conn ...
separately and then over the space of all geodesics. It is a standard tool in
integral geometry In mathematics, integral geometry is the theory of measures on a geometrical space invariant under the symmetry group of that space. In more recent times, the meaning has been broadened to include a view of invariant (or equivariant) transformati ...
and has applications in isoperimetric and rigidity results. The formula is named after
Luis Santaló Luís Antoni Santaló Sors (October 9, 1911 – November 22, 2001) was a Spanish mathematician. He graduated from the University of Madrid and he studied at the University of Hamburg, where he received his Ph.D. in 1936. His advisor was Wilhe ...
, who first proved the result in 1952.


Formulation

Let (M,\partial M,g) be a compact, oriented Riemannian manifold with boundary. Then for a function f: SM \rightarrow \mathbb , Santaló's formula takes the form : \int_ f(x,v) \, d\mu(x,v) = \int_ \left \int_0^ f(\varphi_t(x,v)) \, dt \right\langle v, \nu(x) \rangle \, d \sigma(x,v), where * (\varphi_t)_t is the
geodesic flow In geometry, a geodesic () is a curve representing in some sense the locally shortest path ( arc) between two points in a surface, or more generally in a Riemannian manifold. The term also has meaning in any differentiable manifold with a conne ...
and \tau(x,v) = \sup\ is the exit time of the geodesic with initial conditions (x,v)\in SM , * \mu and \sigma are the
Riemannian volume form In mathematics, a volume form or top-dimensional form is a differential form of degree equal to the differentiable manifold dimension. Thus on a manifold M of dimension n, a volume form is an n-form. It is an element of the space of sections of th ...
s with respect to the Sasaki metric on SM and \partial S M respectively ( \mu is also called
Liouville measure In differential geometry, a subject of mathematics, a symplectic manifold is a smooth manifold, M , equipped with a closed nondegenerate differential 2-form \omega , called the symplectic form. The study of symplectic manifolds is called sym ...
), * \nu is the inward-pointing
unit normal In geometry, a normal is an object (e.g. a line, ray, or vector) that is perpendicular to a given object. For example, the normal line to a plane curve at a given point is the infinite straight line perpendicular to the tangent line to the cur ...
to \partial M and \partial_+ SM := \ the ''influx-boundary'', which should be thought of as parametrization of the space of geodesics.


Validity

Under the assumptions that # M is ''non-trapping'' (i.e. \tau(x,v) <\infty for all (x,v)\in SM ) and # \partial M is ''strictly convex'' (i.e. the
second fundamental form In differential geometry, the second fundamental form (or shape tensor) is a quadratic form on the tangent plane of a smooth surface in the three-dimensional Euclidean space, usually denoted by \mathrm (read "two"). Together with the first fundamen ...
II_(x) is positive definite for every x \in \partial M ), Santaló's formula is valid for all f\in C^\infty(M). In this case it is equivalent to the following identity of measures: : \Phi^*d \mu (x,v,t) = \langle \nu(x),x\rangle d \sigma(x,v) d t, where \Omega=\ and \Phi:\Omega \rightarrow SM is defined by \Phi(x,v,t)=\varphi_t(x,v). In particular this implies that the ''geodesic X-ray transform'' I f(x,v) = \int_0^ f(\varphi_t(x,v)) \, dt extends to a bounded linear map I: L^1(SM, \mu) \rightarrow L^1(\partial_+ SM, \sigma_\nu), where d\sigma_\nu(x,v) = \langle v, \nu(x) \rangle \, d \sigma(x,v) and thus there is the following, L^1-version of Santaló's formula: : \int_ f \, d \mu = \int_ If ~ d \sigma_\nu \quad \text f \in L^1(SM,\mu). If the non-trapping or the convexity condition from above fail, then there is a set E\subset SM of positive measure, such that the geodesics emerging from E either fail to hit the boundary of M or hit it non-transversely. In this case Santaló's formula only remains true for functions with support disjoint from this exceptional set E.


Proof

The following proof is taken from Lemma 3.3">ref>Guillarmou, Colin, Marco Mazzucchelli, and Leo Tzou. "Boundary and lens rigidity for non-convex manifolds." American Journal of Mathematics 143 (2021), no. 2, 533-575. Lemma 3.3 adapted to the (simpler) setting when conditions 1) and 2) from above are true. Santaló's formula follows from the following two ingredients, noting that \partial_0SM=\ has measure zero. * An integration by parts formula for the geodesic vector field X : : \int_ Xu ~ d \mu = - \int_ u ~ d \sigma_\nu \quad \text u \in C^\infty(SM) * The construction of a resolvent for the transport equation X u = - f: : \exists R: C_c^\infty( SM\smallsetminus\partial_0 SM) \rightarrow C^\infty(SM): XRf = - f \text Rf\vert_ = If \quad \text f\in C_c^\infty( SM\smallsetminus\partial_0 SM) For the integration by parts formula, recall that X leaves the Liouville-measure \mu invariant and hence Xu = \operatorname_G (uX) , the divergence with respect to the Sasaki-metric G . The result thus follows from the
divergence theorem In vector calculus, the divergence theorem, also known as Gauss's theorem or Ostrogradsky's theorem, reprinted in is a theorem relating the '' flux'' of a vector field through a closed surface to the ''divergence'' of the field in the volume ...
and the observation that \langle X(x,v), N(x,v)\rangle_G = \langle v, \nu(x)\rangle_g , where N is the inward-pointing unit-normal to \partial SM. The resolvent is explicitly given by Rf(x,v) = \int_0^ f(\varphi_t(x,v)) \, dt and the mapping property C_c^\infty( SM\smallsetminus\partial_0 SM) \rightarrow C^\infty(SM) follows from the smoothness of \tau: SM\smallsetminus\partial_0 SM \rightarrow [0,\infty), which is a consequence of the non-trapping and the convexity assumption.


References

*{{cite book, author=Isaac Chavel, url=https://books.google.com/books?id=Wg-gQcvS25sC&q=Santalo%27s+formula, title=Riemannian Geometry: A Modern Introduction, publisher=Cambridge University Press, year=1995, series=Cambridge Tracts in Mathematics, volume=108, chapter=5.2 Santalo's formula, isbn=0-521-48578-9 Differential geometry Integrals Riemannian geometry