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arXiv 2602.18501math.DSgr-qc
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从渐近组成部分获得动力学不变量

Dynamical Invariants from Asymptotic Composants

Universität Bielefeld(比勒费尔德大学)

Franz Gähler

AI总结:

本文提出了一种简单算法,用于确定一维原始膨胀镶嵌空间的渐近组成部分,以区分不同的MLD类镶嵌,并展示了其与轨道分离维度结合的区分能力。

摘要:

渐近组成部分及其 incidence 关系是1维膨胀镶嵌空间的强大不变量,可以区分许多MLD类的镶嵌。特别是,与大多数其他不变量不同,它们可以经常提供阻碍一个镶嵌空间与其反射MLD的障碍。我们提出一个简单的算法来确定这些渐近组成部分,用于一维原始膨胀镶嵌空间,并说明如何利用它们来区分不同的MLD类的镶嵌。在附录中,我们则展示渐近组成部分的结构,结合轨道分离维度(OSD),可以区分所有具有纯点谱的膨胀镶嵌的MLD类,对于一系列小的膨胀因子,这展示了这些不变量的威力。

英文摘要:

Asymptotic composants and their incidence relations are powerful invariants of 1-dimensional inflation tilings spaces, which can distinguish many MLD classes of tilings. In particular, and unlike most other invariants, they can often provide obstructions to a tiling space being MLD to its reflection. We present a simple algorithm to determine these asymptotic composants for primitive inflation tiling spaces in one dimension, and illustrate how they can be used to tell different MLD classes of tilings apart. In an Appendix, we then show that the structure of asymptotic composants, together with the orbit separation dimension (OSD), can distinguish all MLD classes of inflations tilings with pure-point spectrum for a bunch of small inflation factors, which illustrates the power of these invariants.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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