The Local Dimension: a method to quantify the Cosmic Web
Prakash Sarkar, Somnath Bharadwaj

TL;DR
This paper introduces the Local Dimension method to quantify the shapes of structures in the Cosmic Web, using galaxy counts within spheres to distinguish filaments, sheets, and clusters locally.
Contribution
It proposes a novel local measure, the Local Dimension, to characterize the Cosmic Web's structures, and demonstrates its effectiveness using LCDM simulations.
Findings
Approximately 33% of galaxies have a well-defined Local Dimension.
The Local Dimension correlates with visual identification of filaments and sheets.
Global D distribution helps visualize the Cosmic Web's structure.
Abstract
It is now well accepted that the galaxies are distributed in filaments, sheets and clusters all of which form an interconnected network known as the Cosmic Web. It is a big challenge to quantify the shapes of the interconnected structural elements that form this network. Tools like the Minkowski functionals which use global properties, though well suited for an isolated object like a single sheet or filament, are not suited for an interconnected network of such objects. We consider the Local Dimension , defined through , where is the galaxy number count within a sphere of comoving radius centered on a particular galaxy, as a tool to locally quantify the shape in the neigbourhood of different galaxies along the Cosmic Web. We expect and 3 for a galaxy located in a filament, sheet and cluster respectively. Using LCDM N-body simulations we find that…
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