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Collider and Dark Matter Searches in the Inert Doublet Model from Peccei-Quinn Symmetry

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arxiv 1606.07086 v1 pith:XII3BTPP submitted 2016-06-22 hep-ph

classification hep-ph
keywords darkmattermodelsymmetrycomponentdoubletinertpeccei-quinn
verification ladder T0 review T1 audit T2 compute T3 formal
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abstract

Weakly Interacting Massive Particles (WIMPs) and axions are arguably the most compelling dark matter candidates in the literature. Could they coexist as dark matter particles? More importantly, can they be incorporated in a well motivated framework in agreement with experimental data? In this work, we show that this two component dark matter can be realized in the Inert Doublet Model in an elegant and natural manner by virtue of the spontaneous breaking of a Peccei-Quinn $U(1)_{PQ}$ symmetry into a residual $Z_2$ symmetry. The WIMP stability is guaranteed by the $Z_{2}$ symmetry and a new dark matter component, the axion, arises. There are two interesting outcomes: (i) vector-like quarks needed to implement the Peccei-Quinn symmetry in the model act as a portal between the dark sector and the SM fields with a supersymmetry-type phenomenology at colliders; (ii) two-component Inert Doublet Model re-opens the phenomenologically interesting 100-500 GeV mass region. We show that the model can plausibly have two component dark matter and at the same time avoid low and high energy physics constraints such as monojet and dijet plus missing energy, as well as indirect and direct dark matter detection bounds.

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  1. Synchronization Induced by Ultralight Dark Matter

    hep-ph 2025-07 reject novelty 3.0 of 10

    Ultralight dark matter is claimed to lock oscillator phases together once the coupling gω exceeds a mass-dependent threshold, with sensitivity projected for masses from 10^-14 eV to 1 eV.

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