Manifestation of central symmetry of the celestial sphere in the mutual disposition and luminosity of the Quasars

TL;DR

This study investigates the central symmetry of the celestial sphere by analyzing pairs of quasars with opposite positions, finding significant correlations in their luminosity profiles that support the symmetry hypothesis.

Contribution

It provides empirical evidence for the manifestation of central symmetry through pairs of quasars with similar luminosity profiles, interpreted as potential images of the same object.

Findings

High correlation coefficients (Rxy>0.98) in opposite quasar pairs.

Symmetry effects diminish with symmetry breaking over 0.05 degrees.

Supports the possibility of modeling these dependencies in a closed Universe model.

Abstract

We performed the check of supposition about the possibility of manifestation of the previously observed phenomenon of central symmetry of the celestial sphere through existence of the opposite quasars. We discovered the existence of some pairs of quasars located opposite each other with close by form profiles magnitudes of luminosity in the ranges u, g, r, i, z, when correlation coefficient close to 1. We discovered that the percentage of the pairs with correlation coefficients Rxy>0.98 for the opposite located quasars is significantly higher than that for the random pairs. The analysis of the dependence of this exceedance from the artificial breaking of the central symmetry has shown, that it practically disappears with symmetry breaking by more than 0.05 degrees. Thus we can confirmed the manifestation of the central symmetry of celestial sphere through existence of the central symmetrical pairs of quasars, which can be interpreted as the pairs of images of the same object. We shown the possibility of a theoretical modeling of the observed dependencies in the closed Universe model. It can be supposed, that a relatively small amount of the discovered pairs of the opposite quasars is conditioned by the fact, that the opposite objects for most of the quasars are galaxies, which are not included to the chosen as initial source of data quasar catalog SDSS-DR5.