Abstract |
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A celebrated theorem of P. Funk, 1916, states
that an origin-centered star body in R3
is determined by the areas of its central hyperplane
cross-sections. In particular, if all these concurrent sections
have the same area then the body must be a ball (its boundary is
a sphere). It is natural to try to strengthen the theorem by
using a smaller class of planes. It is evident that a
lower-dimensional class of hyperplanes, e.g., planes passing through an axis, does not
sufice, but a proper open subset of planes appears
plausible. The class of planes at a small angle relative to an
axis has been considered in the literature. We show that this
class does not characterize the body. We then show that if a body
is known to osculate a ball centered at the origin to
infinite order along one hyperplane through the axis, then
the proper open class of planes above does determine whether the
body is a ball. We generalize our theorem to arbitrary origin
centered star bodies and to any open connected collection of
planes that fills out Rn.
We have counterexamples to the theorem for every finite
order of osculation. We have similar theorems for the cosine
transform and projection areas.
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Authors
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