Topological constraints for Stein fillings of tight structures on lens spaces

Pub Date : 2019-06-21 DOI:10.4310/JSG.2020.V18.N6.A1
Edoardo Fossati
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引用次数: 6

Abstract

In this article we give a sharp upper bound on the possible values of the Euler characteristic for a minimal symplectic filling of a tight contact structure on a lens space. This estimate is obtained by looking at the topology of the spaces involved, extending this way what we already knew from the universally tight case to the virtually overtwisted one. As a lower bound, we prove that virtually overtwisted structures on lens spaces never bound Stein rational homology balls. Then we turn our attention to covering maps: since an overtwisted disk lifts to an overtwisted disk, all the coverings of a universally tight structure are themselves tight. The situation is less clear when we consider virtually overtwisted structures. By starting with such a structure on a lens space, we know that this lifts to an overtwisted structure on $S^3$, but what happens to all the other intermediate coverings? We give necessary conditions for these lifts to still be tight, and deduce some information about the fundamental groups of the possible Stein fillings of certain virtually overtwisted structures.
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透镜空间上紧密结构Stein填充的拓扑约束
本文给出了透镜空间上紧接触结构的极小辛填充的欧拉特性可能值的一个明显的上界。这个估计是通过观察所涉及的空间的拓扑得到的,通过这种方式将我们已经知道的从普遍紧密的情况扩展到几乎过度扭曲的情况。作为下界,我们证明了透镜空间上的虚超扭结构不约束Stein理性同调球。然后我们将注意力转向覆盖映射:由于一个超扭的磁盘提升为一个超扭的磁盘,一个普遍紧结构的所有覆盖本身都是紧的。当我们考虑过度扭曲的结构时,情况就不那么清楚了。从透镜空间上的这种结构开始,我们知道它在$S^3$上上升到一个超扭曲结构,但是其他中间覆盖层会发生什么呢?我们给出了这些提升仍然是紧的必要条件,并推导了一些关于某些虚超扭结构可能的Stein填充的基本群的信息。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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