Math 2.0

Convex and discrete geometry Definition

Intersection body

Builds on Convex bodyn-sphere

Definition

Let n≥2n \ge 2, and let K⊆ℝnK \subseteq \R^n be a convex body with the origin in its interior. Let Sn−1S^{n-1} be the unit sphere of ℝn\R^n, and for u∈Sn−1u \in S^{n-1} let u⊥={x:x⋅u=0}u^\perp = \set{x : x \cdot u = 0}. Write voln−1\mathrm{vol}_{n-1} for the (n−1)(n-1)-dimensional volume in the hyperplane u⊥u^\perp. The intersection body of KK is the set IK={ru:u∈Sn−1, 0≤r≤voln−1(K∩u⊥)}.IK = \set{r u : u \in S^{n-1}, \ 0 \le r \le \mathrm{vol}_{n-1}(K \cap u^\perp)}. So IKIK is star-shaped about the origin, and its radial function is ρIK(u)=voln−1(K∩u⊥)\rho_{IK}(u) = \mathrm{vol}_{n-1}(K \cap u^\perp).

Remarks

Example: let BB be the closed unit ball of ℝn\R^n and ωn−1\omega_{n-1} the volume of the unit ball of ℝn−1\R^{n-1}. Every section B∩u⊥B \cap u^\perp is a unit ball of dimension n−1n - 1, so ρIB=ωn−1\rho_{IB} = \omega_{n-1} and IB=ωn−1BIB = \omega_{n-1} B. Non-example: let the origin lie outside KK. Then some hyperplane u⊥u^\perp misses KK, and the radial function vanishes in the direction uu. So the construction no longer gives a body with the origin in its interior, which is why the definition requires the origin to be an interior point of KK. Busemann's theorem says that IKIK is convex when KK is convex and symmetric about the origin. The definition is often stated more generally for star bodies, with the same formula for the radial function.

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  1. Convex body concept
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Further reading

  1. Web https://en.wikipedia.org/wiki/Busemann%E2%80%93Petty_problem
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DefinesIntersection body
UsesConvex body, n-sphere

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