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Top partners and scalar dark matter -- a non-minimal reappraisal

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arxiv 2209.13093 v2 pith:WZHWUMYB submitted 2022-09-27 hep-ph

classification hep-ph
keywords darkmattermodelvector-likeinteractionsstandardcompositemodels
verification ladder T0 review T1 audit T2 compute T3 formal
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A large set of models beyond the Standard Model of particle physics suggest that the top quark plays a special role in fundamental interactions. At the same time some of these models predict that a particle responsible for dark matter is present in the physical spectrum of the theory, and in particular cases dark matter may be specially linked to the top sector. Such a new physics configuration occurs, for instance, in composite frameworks that additionally feature vector-like quarks as mediators of the interactions of the dark matter with the Standard Model. We investigate the interplay of top-philic dark matter and the presence of several vector-like top partners. Such a non-minimal setup with several vector-like fermions is typical of composite scenarios, and we make use of an effective model to study to which extent such non-minimality modifies the collider and cosmological phenomenology of the minimal model, the latter only including one vector-like mediator of the dark matter interactions with the Standard Model.

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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. Dark matter in composite Higgs models with a scotogenic EFT

    hep-ph 2026-07 conditional novelty 5.0 of 10

    In the SU(6)/Sp(6) composite Higgs model with a scotogenic Z2, three of four neutral pseudo-Goldstone dark matter candidates can reproduce the observed relic density, while the SU(2)L triplet candidate fails; spin-1 r...

  2. Revisiting the Inert Scalar Dark Matter with Vector-like Quarks

    hep-ph 2024-12 conditional novelty 4.0 of 10

    A Z2-odd vector-like quark added to the inert doublet model restores the correct dark matter relic abundance for DM masses above about 550 GeV in compressed spectra.

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