Filling radius

Filling radius

In Riemannian geometry, the filling radius of a Riemannian manifold "X" is a metric invariant of "X". It was originally introduced in 1983 by Mikhail Gromov, who used it to prove his systolic inequality for essential manifolds, vastly generalizing Loewner's torus inequality and Pu's inequality for the real projective plane, and creating Systolic geometry in its modern form.

The filling radius of a simple loop "C" in the plane is defined as the largest radius, "R>0", of a circle that fits inside "C":

:mathrm{FillRad}(Csubset mathbb{R}^2) = R.

Dual definition via neighborhoods

There is a kind of a dual point of view that allows one to generalize this notion in an extremely fruitful way, as shown by Gromov. Namely, we consider the epsilon-neighborhoods of the loop "C", denoted

:U_epsilon C subset mathbb{R}^2.

As epsilon>0 increases, the epsilon-neighborhood U_epsilon C swallows up more and more of the interior of the loop. The "last" point to be swallowed up is precisely the center of a largest inscribed circle. Therefore we can reformulate the above definition by defining mathrm{FillRad}(Csubset mathbb{R}^2) to be the infimum of epsilon > 0 such that the loop "C" contracts to a point in U_epsilon C.

Given a compact manifold "X" imbedded in, say, Euclidean space "E", we could define the filling radius "relative" to the imbedding, by minimizing the size of the neighborhood U_epsilon Xsubset E in which "X" could be homotoped to something smaller dimensional, e.g., to a lower dimensional polyhedron. Technically it is more convenient to work with a homological definition.

Homological definition

Denote by "A" the coefficient ring mathbb{Z} or mathbb{Z}_2, depending on whether or not "X" is orientable. Then the fundamental class, enoted " [X] ", of a compact "n"-dimensional manifold "X", is a generator of H_n(X;A)=A, and we set :mathrm{FillRad}(Xsubset E) = inf left{ epsilon > 0 left
;iota_epsilon( [X] )=0in H_n(U_epsilon X) ight. ight},

where iota_epsilon is the inclusion homomorphism.

To define an "absolute" filling radius in a situation where "X" is equipped with a Riemannian metric "g", Gromov proceeds as follows. One exploits an imbedding due to C. Kuratowski. One imbeds "X" in the Banach space L^infty(X) of bounded Borel functions on "X", equipped with the sup norm |;|. Namely, we map a point xin X to the function f_xin L^infty(X) defined by the formula f_x(y) = d(x,y)for all yin X, where "d" is the distance function defined by the metric. By the triangle inequality we have d(x,y) = | f_x - f_y |, and therefore the imbedding is strongly isometric, in the precise sense that internal distance and ambient distance coincide. Such a strongly isometric imbedding is impossible if the ambient space is a Hilbert space, even when "X" is the Riemannian circle (the distance between opposite points must be"π", not 2!). We then set E= L^infty(X) in the formula above, and define

:mathrm{FillRad}(X)=mathrm{FillRad} left( XsubsetL^{infty}(X) ight).

Example

The filling radius of the Riemannian circle of length 2π, i.e. the unit circle with the induced Riemannian distance function, equals π/3, i.e. a sixth of its length.

ee also

*Filling area conjecture
*Gromov's systolic inequality for essential manifolds

References

* Gromov, M.: Filling Riemannian manifolds, J. Diff. Geom. 18 (1983), 1-147.

*Citation | last1=Katz | first1=Mikhail G. | title=Systolic geometry and topology| publisher=American Mathematical Society | location=Providence, R.I. | series=Mathematical Surveys and Monographs | isbn=978-0-8218-4177-8 | year=2007 | volume=137


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