Cosmology as Matter-Antimatter Phase Separation
Paul R. Gerber
Gerber Molecular Design, Forten 649, CH-8873 Amden, Switzerland
Within the bipolar-gravity picture
gravitation has no influence on the early development of the Universe
because radiation does not gravitate and matter and antimatter are fully
mixed such that their gravitation effects completely compensate.
This is what one would have expected in the first place, because
gravitation is by far the weakest elementary interaction.
Gravitation starts to play a role when modes that separate matter and
antimatter start to grow. The larger the wavelength of these modes,
the more important is the influence of gravity because ever larger
junks of either species develop with increasing tendency to contract.
Gravity Dominated Final Phase
The current picture is that a continued expansion takes place, due to the
interspersed arrangement of matter and antimatter. This yields an ever
lasting, though decreasing accelleration
of the expansion rate (see 'Accelerated cosmic expansion' in
Furthermore, it is expected, that continued merging of islands of the same matter
type takes place, such that ever larger superclusters develop.
This note is under development.