http://arxiv.org/abs/1506.06777
We simulate structure formation in the matter-dominated universe using a quasi-newtonian, one-dimensional model. In addition to dark matter, luminous matter is introduced to examine the potential bias in the distributions. We use multifractal analysis techniques to identify structures, including clusters and voids. Both dark matter and luminous matter exhibit fractal geometry as the universe evolves. We present the results on the generalized dimensions computed at various scales for each matter distribution.
Y. Shiozawa and B. Miller
Wed, 24 Jun 15
34/54
Comments: 6 pages, 4 figures
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