Flux-Induced Baryon Asymmetry
L.E. Ibanez

TL;DR
This paper proposes a novel mechanism for the universe's baryon asymmetry, induced by a non-zero antisymmetric field background in string-inspired models, avoiding Sakharov conditions.
Contribution
It introduces a new baryogenesis scenario based on antisymmetric field backgrounds in D-brane models, bypassing traditional Sakharov conditions.
Findings
Baryon asymmetry can be generated without Sakharov conditions.
Antisymmetric field backgrounds induce (B-L) number density.
D-brane models naturally incorporate the necessary ingredients.
Abstract
I propose that the primordial baryon asymmetry of the universe was induced by the presence of a non-vanishing antisymmetric field background H_ijk across the three space dimensions. This background creates a dilute (B-L)-number density in the universe cancelling the contribution from baryons and leptons. This situation naturally appears if the U(1)_{B-L} symmetry is gauged and the corresponding gauge boson gets a Stuckelberg mass by combining with an antisymmetric field B_ij. All these ingredients are present in D-brane models of particle physics. None of the Sakharov conditions are required.
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Taxonomy
TopicsBlack Holes and Theoretical Physics · Cosmology and Gravitation Theories · Particle physics theoretical and experimental studies
