Anomalies, the Dark Universe and Matter-Antimatter asymmetry
Nick E. Mavromatos (Natl. Tech. U. Athens, King's Coll. London)

TL;DR
This paper presents a string-inspired cosmological model with gravitational anomalies and torsion that explains inflation, matter-antimatter asymmetry, and dark matter through axion-like particles and primordial black holes, with potential observable signatures.
Contribution
It introduces a novel anomaly-driven inflationary model with gravitational axions, linking dark matter, black hole formation, and leptogenesis within a unified framework.
Findings
Inflation driven by gravitational anomaly condensates without external inflatons.
Generation of chiral matter and residual gauge anomalies affecting post-inflation physics.
Potential observable effects on gravitational wave profiles and primordial black hole production.
Abstract
I review a (3+1)-dimensional, string-inspired cosmological model with gravitational anomalies (of Chern-Simons (CS) type) at early epochs, and a totally-antisymmetric torsion, dual to a massless axion-like field ("gravitational axion"), which couples to the CS term. Under appropriate conditions, primordial gravitational waves can condense, leading to a condensate of the CS anomaly term. As a consequence, one obtains inflation in this theory, of running-vacuum-model (RVM) type, without the need for external inflatons. At the end of the inflationary era, chiral fermionic matter is generated, whose gravitational anomalies cancel the primordial ones. On the other hand, chiral anomalies of gauge type, which are also generated by the chiral matter, remain present during the post-inflationary epochs and become responsible for the generation of a non-perturbative mass for the torsion-related…
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Taxonomy
TopicsCosmology and Gravitation Theories · Dark Matter and Cosmic Phenomena · Computational Physics and Python Applications
