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