Shapefinders: A new shape diagnostic for large-scale structure

被引:140
作者
Sahni, V
Sathyaprakash, BS
Shandarin, SF
机构
[1] Inter Univ Ctr Astron & Astrophys, Pune 411007, Maharashtra, India
[2] Univ Wales Coll Cardiff, Dept Phys & Astron, Cardiff CF2 3YB, S Glam, Wales
[3] Univ Kansas, Dept Phys & Astron, Lawrence, KS 66045 USA
基金
美国国家航空航天局;
关键词
cosmology; theory; galaxies; clusters; general; large-scale structure of universe; methods; analytical; numerical;
D O I
10.1086/311214
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We construct a set of shapefinders used to determine the shapes of compact surfaces (isodensity surfaces in galaxy surveys or N-body simulations) without fitting them to ellipsoidal configurations, as has been done earlier. The new indicators, based on the Minkowski functionals, arise from simple, geometrical considerations and are derived from the fundamental properties of a surface such as its volume, surface area, integrated mean curvature, and connectivity characterized by the genus. These "shapefinders" could be used to diagnose the presence of filaments, pancakes, and ribbons in large-scale structure. Their lower dimensional generalization may be useful for the study of two-dimensional distributions such as temperature maps of the cosmic microwave background.
引用
收藏
页码:L5 / L8
页数:4
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