1990
DOI: 10.1007/3-540-52846-6_94
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Star unfolding of a polytope with applications

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Cited by 39 publications
(119 citation statements)
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“…To the best of our knowledge no complete solution to this problem has been published so far. It had been announced in [1,21] that methods applied to special cases, such as planar polygonal domain [21] and surface of convex polytopes [1], extend to the general case. These potential solutions represent a theoretical interest only, due to their high time and space complexities.…”
Section: Overview Of Previous Workmentioning
confidence: 99%
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“…To the best of our knowledge no complete solution to this problem has been published so far. It had been announced in [1,21] that methods applied to special cases, such as planar polygonal domain [21] and surface of convex polytopes [1], extend to the general case. These potential solutions represent a theoretical interest only, due to their high time and space complexities.…”
Section: Overview Of Previous Workmentioning
confidence: 99%
“…For a polytope of size n it takes O(n log n) preprocessing time and distance queries to the source are answered in O(log n) time. The exact APQ problem on the surface of a convex polytope has been studied by Agarwal et al in [1]. They proposed a scheme that, for a convex polytope of size n and an input parameter m, 1 ≤ m ≤ n 2 , takes O(n 6 m 1+δ ) (δ > 0) preprocessing time and space to construct a data structure that serves distance queries between arbitrary pairs of points in O( √ n log n/m 1/4 ) time.…”
Section: Overview Of Previous Workmentioning
confidence: 99%
“…Our main result improves the edge sequence and diameter algorithms of [1] by a linear factor. We achieve this improvement by combining the star unfolding technique of [1] with the kinetic Voronoi diagram structure of Albers et al [3]. A kinetic Voronoi diagram allows its defining point sites to move.…”
mentioning
confidence: 99%
“…The shortest path π(s, t) can always be represented by a two-dimensional shortest path in the star unfolding that originates from one of the source images s 1 , ..., s M and terminates at the image of t. If the image of t lies in the anti-core region containing s i , then the two-dimensional shortest path in the star unfolding from s i to the image of t is optimal. By contrast, if the image of 1 The core has also been referred to as the kernel or the antarctic in [1,15]. Note that neither the star unfolding nor its core are necessarily star-shaped [1].…”
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confidence: 99%
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