Non-linear gravitational clustering of cold matter in an expanding universe: indications from 1D toy models
Michael Joyce, Fran\c{c}ois Sicard

TL;DR
This paper uses 1D toy models to explore non-linear gravitational clustering, revealing scale-invariant, virialized fractal structures that support the stable clustering hypothesis and challenge assumptions about dark matter halo profiles.
Contribution
It demonstrates that non-linear clustering in 1D models aligns with stable clustering predictions and suggests implications for 3D dark matter halo modeling.
Findings
Scale-invariant clustering exponents match stable clustering predictions.
Selected structures are statistically virialized across scales.
Results imply dark matter halos may be fractal and not smooth.
Abstract
Studies of a class of infinite one dimensional self-gravitating systems have highlighted that, on the one hand, the spatial clustering which develops may have scale invariant (fractal) properties, and, on the other, that they display "self-similar" properties in their temporal evolution. The relevance of these results to three dimensional cosmological simulations has remained unclear. We show here that the measured exponents characterizing the scale-invariant non-linear clustering are in excellent agreement with those derived from an appropriately generalized "stable-clustering" hypothesis. Further an analysis in terms of "halos" selected with a friend-of-friend algorithm reveals that such structures are, statistically, virialized across the range of scales corresponding to scale-invariance. Thus the strongly non-linear clustering in these models is accurately described as a virialized…
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