H0 Tensions in Cosmology and Axion Pseudocycles in the Stringy Universe

The tension between early and late H-0 is revised in the context of axion dark matter arising naturally from string theoretical integrations of antisymmetric tensor fields over non-trivial cycles. Certain early universe cycles may appear non-trivial from the perspective of a homology analysis focused on the early universe, while they may become trivial when analysed from the perspective of a homology theory reaching out to lower energies and later times. Such phenomena can introduce variations in the axion potential that would explain the observed H-0 tension. The decay of such pseudo-axions when the pseudo-cycles dissipate trigger axion-two-photon (otherwise having an extremely long lifetime) and axion-gravitational processes mediated by Chern-Simons couplings with observable electromagnetic or gravitational wave signals originating in the early universe.

Automated summary

This article revises the tension between early and late universe in the context of axion dark matter arising naturally from string theoretical integrations. The analysis from different perspectives explains the observed H-0 tension and proposes that electromagnetic or gravitational wave signals from the early universe may originate from the decay process of axions.