DW-genesis: baryon number from domain wall network collapse
Alberto Mariotti, Xander Nagels, A\"aron Rase, Miguel Vanvlasselaer

TL;DR
This paper investigates how collapsing axionic domain walls in the early universe can generate the observed baryon asymmetry through spontaneous baryogenesis, analyzing different models and phenomenological signals like gravitational waves.
Contribution
It systematically studies baryon asymmetry production via domain wall collapse across various models, highlighting conditions for maximized asymmetry and addressing cancellation effects.
Findings
Baryon asymmetry peaks when domain walls collapse near interaction decoupling.
Gravitational wave signals from domain wall annihilation are potentially detectable.
Cancellation effects can suppress asymmetry, but methods to mitigate this are discussed.
Abstract
Axionic domain walls, as they move through the early universe plasma during their collapse, can generate a net baryon and lepton number through the mechanism of spontaneous baryogenesis, provided that there is a coupling between the axion and the lepton or baryon current. In this paper, we study systematically the baryon asymmetry produced by these domain walls (DWs) at annihilation, within different realisations of the - or -violating sector, and refer to this process as DW-genesis. We find that the baryon number is maximised when the DW network collapses approximately at the moment when the - or -violating interaction decouples. We study a model of minimal leptogenesis, a model of cogenesis, a model of baryogenesis and finally the possibility that the baryon asymmetry is produced by electroweak sphalerons. As phenomenological consequences of DW-genesis, we discuss the…
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Taxonomy
TopicsMechanical stress and fatigue analysis · Adhesion, Friction, and Surface Interactions · Urologic and reproductive health conditions
