K-minus Estimator Approach to Large Scale Structure
M. Martinis, M. Sosic

TL;DR
This paper introduces a K-minus estimator for analyzing large-scale self-similar cosmic structures, revealing a quasifractal dimension around 2 in galaxy distribution data, and emphasizes the role of visual inspection in spatial correlation analysis.
Contribution
It proposes a simplified local K-minus estimator for correlation analysis, validated on galaxy data, and highlights the importance of visual methods and critiques current cosmological simulations.
Findings
K-minus estimator reveals D≈2 in 2dfGRS data
Dimensions D between 1 and 1.7 are invalid for this method
Visual inspection is crucial for analyzing spatial distributions
Abstract
Self similar 3D distributions of point-particles, with a given quasifractal dimension D, were generated on a Menger sponge model and then compared with \textit{2dfGRS} and \textit{Virgo project} data \footnote{http://www.mso.anu.edu.au/2dFGRS/, http://www.mpa-garching.mpg.de/Virgo/}. Using the principle of local knowledge, it is argued that in a finite volume of space only the two-point minus estimator is acceptable in the correlation analysis of self similar spatial distributions. In this sense, we have simplified the Pietronero-Labini correlative analysis by defining a K-minus estimator, which when applied to 2dfGRS data revealed the quasifractal dimension as expected. In our approach the K-minus estimator is used only locally. Dimensions between D = 1 and D = 1.7, as suggested by the standard analysis, were found to be fallacy of the method. In order to…
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Taxonomy
TopicsSoil Geostatistics and Mapping · Spatial and Panel Data Analysis · Scientific Research and Discoveries
