平面最小星团的Steiner性质。各向异性的情况

Valentina Franceschi, A. Pratelli, Giorgio Stefani
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引用次数: 4

摘要

本文讨论了各向异性双密度平面上最小簇的Steiner性质。这意味着我们考虑的是星系团的经典等周问题,但体积和周长是通过使用两个密度来定义的。特别地,周长密度也可能取决于法向量的方向。经典的欧几里得情形的“斯坦纳性质”(对应于两个密度都等于$1$)说,最小的星团是由有限多个${\rm C}^{1,\gamma}$弧线组成的,在有限多个“三点”中会合。我们可以证明,在密度的非常弱的假设下,这个性质是成立的。在平行论文《关于平面最小化簇的Steiner性质》中。“我们考虑的是各向同性的情况,即当周长密度不依赖于方向时,这使得大多数构造变得简单得多。特别地,在本例中,三点处的三条弧线不一定以120^ circ$的三个角度相交,而在各向同性的情况下则相反。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
On the Steiner property for planar minimizing clusters. The anisotropic case
In this paper we discuss the Steiner property for minimal clusters in the plane with an anisotropic double density. This means that we consider the classical isoperimetric problem for clusters, but volume and perimeter are defined by using two densities. In particular, the perimeter density may also depend on the direction of the normal vector. The classical"Steiner property"for the Euclidean case (which corresponds to both densities being equal to $1$) says that minimal clusters are made by finitely many ${\rm C}^{1,\gamma}$ arcs, meeting in finitely many"triple points". We can show that this property holds under very weak assumptions on the densities. In the parallel paper"On the Steiner property for planar minimizing clusters. The isotropic case"we consider the isotropic case, i.e., when the perimeter density does not depend on the direction, which makes most of the construction much simpler. In particular, in the present case the three arcs at triple points do not necessarily meet with three angles of $120^\circ$, which is instead what happens in the isotropic case.
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