New evidence and analysis of cosmological-scale asymmetry in galaxy spin directions

TL;DR

This paper investigates the potential existence of a cosmological-scale axis by analyzing the distribution of galaxy spin directions across multiple datasets, providing evidence for large-scale anisotropy in the universe.

Contribution

It introduces a new analysis of galaxy spin directions from four telescopes, supporting the hypothesis of a universe with a major axis.

Findings

Nearly identical axis profiles across different datasets

Evidence of large-scale anisotropy in galaxy spin directions

Supports theories proposing a cosmological-scale axis

Abstract

In the past several decades, multiple cosmological theories that are based on the contention that the Universe has a major axis have been proposed. Such theories can be based on the geometry of the Universe, or multiverse theories such as black hole cosmology. The contention of a cosmological-scale axis is supported by certain evidence such as the dipole axis formed by the CMB distribution. Here I study another form of cosmological-scale axis, based on the distribution of the spin direction of spiral galaxies. Data from four different telescopes is analyzed, showing nearly identical axis profiles when the distribution of the redshifts of the galaxies is similar.