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dc.contributor.authorElor, G.-
dc.contributor.authorEscudero Abenza, Miguel-
dc.contributor.authorNelson, A.E.-
dc.identifierdoi: 10.1103/PhysRevD.99.035031-
dc.identifierissn: 2470-0029-
dc.identifier.citationPhysical Review D 99 (3): 035031 (2019)-
dc.description.abstractWe 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 B meson oscillations and subsequent decays. This setup is testable at hadron colliders and B factories. In the early universe, decays of a long lived particle produce B mesons and antimesons out of thermal equilibrium. These mesons/antimesons then undergo CP violating oscillations before quickly decaying into visible and dark sector particles. Dark matter will be charged under the 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 B decays: an experimental observable. Dark matter is stabilized by an unbroken discrete symmetry, and proton decay is simply evaded by kinematics. We will illustrate this mechanism with a model that is unconstrained by dinucleon decay, does not require a high reheat temperature, and would have unique experimental signals - a positive leptonic asymmetry in B meson decays, a new decay of B mesons into a baryon and missing energy, and a new decay of b-flavored baryons into mesons and missing energy. These three observables are testable at current and upcoming collider experiments, allowing for a distinct probe of this mechanism.-
dc.publisherAmerican Physical Society-
dc.relation.isversionofPublisher's version-
dc.titleBaryogenesis and dark matter from B mesons-
dc.description.versionPeer Reviewed-
dc.contributor.funderEuropean Commission-
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