{"title":"Stratifications of the ray space of a tropical quadratic form by Cauchy-Schwartz functions","authors":"Z. Izhakian, Manfred Knebusch","doi":"10.13001/ela.2022.6493","DOIUrl":null,"url":null,"abstract":"Classes of an equivalence relation on a module $V$ over a supertropical semiring, called rays, carry the underlying structure of 'supertropical trigonometry' and thereby a version of convex geometry which is compatible with quasilinearity. In this theory, the traditional Cauchy-Schwarz inequality is replaced by the CS-ratio, which gives rise to special characteristic functions, called CS-functions. These functions partite the ray space $\\mathrm{Ray}(V)$ into convex sets and establish the main tool for analyzing varieties of quasilinear stars in $\\mathrm{Ray}(V)$. They provide stratifications of $\\mathrm{Ray}(V)$ and, therefore, a finer convex analysis that helps better understand geometric properties.","PeriodicalId":50540,"journal":{"name":"Electronic Journal of Linear Algebra","volume":" ","pages":""},"PeriodicalIF":0.7000,"publicationDate":"2022-05-30","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Electronic Journal of Linear Algebra","FirstCategoryId":"100","ListUrlMain":"https://doi.org/10.13001/ela.2022.6493","RegionNum":4,"RegionCategory":"数学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q2","JCRName":"Mathematics","Score":null,"Total":0}
引用次数: 0
Abstract
Classes of an equivalence relation on a module $V$ over a supertropical semiring, called rays, carry the underlying structure of 'supertropical trigonometry' and thereby a version of convex geometry which is compatible with quasilinearity. In this theory, the traditional Cauchy-Schwarz inequality is replaced by the CS-ratio, which gives rise to special characteristic functions, called CS-functions. These functions partite the ray space $\mathrm{Ray}(V)$ into convex sets and establish the main tool for analyzing varieties of quasilinear stars in $\mathrm{Ray}(V)$. They provide stratifications of $\mathrm{Ray}(V)$ and, therefore, a finer convex analysis that helps better understand geometric properties.
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