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Fixed and Periodic Points of the Intersection Body Operator
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abstract
The intersection body $IK$ of a star-body $K$ in $\mathbb{R}^n$ was introduced by E. Lutwak following the work of H. Busemann, and plays a central role in the dual Brunn-Minkowski theory. We show that when $n \geq 3$, $I^2 K = c K$ iff $K$ is a centered ellipsoid, and hence $I K = c K$ iff $K$ is a centered Euclidean ball, answering long-standing questions by Lutwak, Gardner, and Fish-Nazarov-Ryabogin-Zvavitch. To this end, we recast the iterated intersection body equation as an Euler-Lagrange equation for a certain volume functional under radial perturbations, derive new formulas for the volume of $I K$, and introduce a continuous version of Steiner symmetrization for Lipschitz star-bodies, which (surprisingly) yields a useful radial perturbation exactly when $n\geq 3$.
Forward citations
Cited by 2 Pith papers
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On the homothety conjecture for the body of flotation and the body of buoyancy on a plane
Under the assumption that the body of flotation and the body of buoyancy are homothetic and every flotation chord cuts off one third of the total affine arc length, the body must be an ellipse.
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Quantitative stability of the intersection body operator near the ball, and the dynamical origin of the two--dimensional degeneracy
Near the ball in dimension n≥3 the operator IB^{2} has neutral ellipsoidal modes and a sharp spectral gap (n-2)(n+4)/(n+1)^{2} that yields an explicit local stability rate for the characterization of ellipsoids.
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