COSMOLOGICAL DARK TURBULENCE AND SCALING RELATIONS IN SELF-GRAVITATING SYSTEMS

被引:0
|
作者
Nakamichi, A. [1 ]
Morikawa, M. [2 ]
机构
[1] Gunma Astron Observ, 6860-86 Nakayama, Gunma 3770702, Japan
[2] Ochanomizu Univ, Dept Phys, Tokyo 1128610, Japan
关键词
D O I
10.1051/eas/0936019
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Many scaling relations have been observed for self-gravitating systems (SOS) in the universe. We explore a consistent understanding of them from a simple principle based oil the proposal that the collision-less dark matter (DM) fluid terns into a turbulent state, i.e. dark turbulence, after crossing the caustic surface in the non-linear stage. After deriving Kolmogorov scaling laws from Navier-Stokes and Jeans equations by the method used in solving the Smoluchowski coagulation equation, we apply this to several observations such as the scale-dependent velocity dispersion, mass-luminosity ratio, and mass-angular momentum relation. They all point the concordant value for the constant energy flow per mass: 0.3 cm(2)/s(3) which may be understood as the speed of the hierarchical coalescence process in the cosmic structure formation.
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收藏
页码:141 / +
页数:2
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