Disentangling the cosmic web. I. Morphology of isodensity contours

被引:87
作者
Schmalzing, J
Buchert, T
Melott, AL
Sahni, V
Sathyaprakash, BS
Shandarin, SF
机构
[1] Univ Munich, D-80333 Munich, Germany
[2] Max Planck Inst Astrophys, D-85740 Garching, Germany
[3] CERN, Div Theory, CH-1211 Geneva, Switzerland
[4] Univ Kansas, Dept Phys & Astron, Lawrence, KS 66045 USA
[5] Inter Univ Ctr Astron & Astrophys, Poona 411007, Maharashtra, India
[6] Univ Wales Coll Cardiff, Dept Phys & Astron, Cardiff CF2 3YB, S Glam, Wales
[7] Theoret Astrophys Ctr, DK-2100 Copenhagen O, Denmark
关键词
large-scale structure of universe; methods : numerical; methods : statistical;
D O I
10.1086/308039
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We apply Minkowski functionals and various derived measures to decipher the morphological properties of large-scale structure seen in simulations of gravitational evolution. Minkowski functionals of isodensity contours serve as tools to test global properties of the density field. Furthermore, we identify coherent objects at various threshold levels and calculate their partial Minkowski functionals. We propose a set of two derived dimensionless quantities, planarity and filamentarity, which reduce the morphological information in a simple and intuitive way. Several simulations of the gravitational evolution of initial power-law spectra provide a framework for systematic tests of our method.
引用
收藏
页码:568 / 578
页数:11
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