The correlation structure of dark matter halo properties

被引:46
作者
Jeeson-Daniel, Akila [1 ,2 ]
Dalla Vecchia, Claudio [2 ,3 ]
Haas, Marcel R. [2 ,4 ]
Schaye, Joop [2 ]
机构
[1] Max Planck Inst Astrophys, D-85741 Garching, Germany
[2] Leiden Univ, Leiden Observ, NL-2300 RA Leiden, Netherlands
[3] Max Planck Inst Extraterr Phys, D-85748 Garching, Germany
[4] Space Telescope Sci Inst, Baltimore, MD 21218 USA
关键词
gravitation; methods: numerical; methods: statistical; dark matter; FORMATION TIMES; ASSEMBLY BIAS; DEPENDENCE; SIMULATION; PROFILE; SHAPE; SPIN; MASS;
D O I
10.1111/j.1745-3933.2011.01081.x
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We investigate the correlation between nine different dark matter halo properties using a rank correlation analysis and a Principal Component Analysis for a sample of haloes spanning five orders of magnitude in mass. We consider mass and dimensionless measures of concentration, age, relaxedness, sphericity, triaxiality, substructure, spin and environment, where the latter is defined in a way that makes it insensitive to mass. We find that concentration is the most fundamental property. Except for environment, all parameters are strongly correlated with concentration. Concentration, age, substructure, mass, sphericity and relaxedness can be considered a single family of parameters, albeit with substantial scatter. In contrast, spin, environment and triaxiality are more independent, although spin does correlate strongly with substructure and both spin and triaxiality correlate substantially with concentration. Although mass sets the scale of a halo, all other properties are more sensitive to concentration.
引用
收藏
页码:L69 / L73
页数:5
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