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Simulating Glueball Production in $N_f = 0$ QCD

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arxiv 2202.12899 v2 pith:EG4SGOVU submitted 2022-02-25 hep-ph hep-ex

classification hep-phhep-ex
keywords glueballdarkconfinementgluehadronizationhiddenhierarchyphenomenology
verification ladder T0 review T1 audit T2 compute T3 formal
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abstract

In an $SU(N_c)$ gauge theory with zero light quark flavours $N_f = 0$, the only hadronic states that form below the confinement scale are composite gluon states called glueballs. These minimal confining sectors arise in many Hidden Valley extensions of the Standard Model, including scenarios that could hold the solution to the dark matter question and the hierarchy problem. Quantitative study of dark glueball phenomenology requires an understanding of pure glue hadronization, which to date is severely lacking. In this work we show that significant progress can be made by combining a perturbative pure glue parton shower with a self-consistent and physically motivated parameterization of the unknown non-perturbative physics, thanks to the modest hierarchy between the glueball mass and the confinement scale. We make our simulation code available as the public GlueShower package, the first glueball generator for Hidden Valley theories, and perform preliminary studies of several glueball production observables, with theoretical uncertainties that take the full range of possible hadronization scenarios into account. We hope this will enable new studies of dark sector phenomenology that were previously inaccessible.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Glueball Axion-Like Particles

    hep-ph 2024-11 conditional novelty 4.0 of 10

    A pseudoscalar glueball from a dark Yang-Mills sector, called a GALP, is shown to behave like an axion-like particle and to be a viable dark matter candidate with a predicted mass-coupling relation.

  2. Populating dark sectors with relativistic bubble walls

    hep-ph 2024-12 conditional novelty 3.0 of 10

    Relativistic bubble walls can pair-produce dark matter much heavier than the phase transition scale, which then free-streams as warm dark matter.

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