Baryogenesis and Dark Matter from $B$ Mesons
Gilly Elor, Miguel Escudero, Ann E. Nelson

TL;DR
This paper proposes a novel mechanism linking B meson oscillations to baryogenesis and dark matter production, which can be tested through specific collider and B-factory experiments, offering new insights into the matter-antimatter asymmetry.
Contribution
It introduces a new, testable model where B meson oscillations generate baryon asymmetry and dark matter, avoiding high reheat temperatures and proton decay constraints.
Findings
Dark matter relic abundance linked to B meson oscillations
Observable leptonic asymmetry in B decays predicted
Unique collider signatures including B decays into baryons and missing energy
Abstract
We present a new mechanism of Baryogenesis and dark matter production in which both the dark matter relic abundance and the baryon asymmetry arise from neutral meson oscillations and subsequent decays. This set-up is testable at hadron colliders and -factories. In the early Universe, decays of a long lived particle produce mesons and anti-mesons out of thermal equilibrium. These mesons/anti-mesons then undergo CP violating oscillations before quickly decaying into visible and dark sector particles. Dark matter will be charged under Baryon number so that the visible sector baryon asymmetry is produced without violating the total baryon number of the Universe. The produced baryon asymmetry will be directly related to the leptonic charge asymmetry in neutral decays; an experimental observable. Dark matter is stabilized by an unbroken discrete symmetry, and proton decay is…
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