The paper studies convex radiant sets (i.e. containing the origin) of a linear normed space X and their representation by means of a gauge. By gauge of a convex radiant set C we mean a sublinear function p such that C=[p< 1]. We characterize the class of convex radiant sets which admit a gauge different from the Minkowski gauge in two different ways: they are contained in a translate of their recession cone or, equivalently, they are costarshaped, that is complement of a starshaped set. We prove that the family of all sublinear gauges of a convex radiant set admits a least element and characterize its support set in terms of polar sets. The key concept for this study is the outer kernel of C, that is the kernel (in the sense of Starshaped Analysis) of the complement of C. We also devote some attention to the relation between costarshaped and hyperbolic convex sets.
Convex Radiant Costarshaped Sets and the Least Sublinear Gauge / Zaffaroni, Alberto. - In: JOURNAL OF CONVEX ANALYSIS. - ISSN 0944-6532. - STAMPA. - 20:(2013), pp. 307-328.
Convex Radiant Costarshaped Sets and the Least Sublinear Gauge
ZAFFARONI, Alberto
2013
Abstract
The paper studies convex radiant sets (i.e. containing the origin) of a linear normed space X and their representation by means of a gauge. By gauge of a convex radiant set C we mean a sublinear function p such that C=[p< 1]. We characterize the class of convex radiant sets which admit a gauge different from the Minkowski gauge in two different ways: they are contained in a translate of their recession cone or, equivalently, they are costarshaped, that is complement of a starshaped set. We prove that the family of all sublinear gauges of a convex radiant set admits a least element and characterize its support set in terms of polar sets. The key concept for this study is the outer kernel of C, that is the kernel (in the sense of Starshaped Analysis) of the complement of C. We also devote some attention to the relation between costarshaped and hyperbolic convex sets.Pubblicazioni consigliate
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