Light vector dark matter via a magnetic dipole portal: bridging direct detection and fixed-target searches
Artikel i vetenskaplig tidskrift, 2026

We present a model featuring sub-GeV vector dark matter by augmenting the Standard Model with a new non-Abelian dark SU(2)D, spontaneously broken by the vacuum expectation values of a scalar doublet and a triplet. Interactions between the dark and visible sectors arise through a dimension-5 non-Abelian avatar of kinetic mixing portal, inducing effective magnetic dipole couplings of the dark matter, with the photon and Z boson. The resulting spectrum of the dark gauge bosons naturally exhibits an inverse mass hierarchy between the dark matter and the Z′, leading to interesting phenomenology at fixed-target experiments such as LDMX through dark off-shell bremsstrahlung, dark Higgs-strahlung, invisible vector meson decay, and visible decays. We compute the thermal relic abundance across sub-GeV dark matter masses, with regions of freeze-out proceeding via annihilation into dark sector states or direct annihilation into Standard Model states. Bounds from a broad set of laboratory probes, along with cosmological and astrophysical observations, are incorporated in our analysis. Among them, the most restrictive bounds originate from direct detection experiments, Big Bang Nucleosynthesis, collider searches, and the CMB. Our results demonstrate that a sizeable region of parameter space remains consistent with the observed relic abundance and current experimental constraints, and that fixed-target searches should be considered in tandem with direct detection and cosmological probes for an effective and comprehensive search strategy, especially in the off-shell regime.

Dark Matter at Colliders

New Gauge Interactions

New Light Particles

Models for Dark Matter

Författare

Avik Banerjee

Tata Institute of Fundamental Research

Riccardo Catena

Chalmers, Fysik, Subatomär, högenergi- och plasmafysik

Taylor Gray

Chalmers, Fysik, Subatomär, högenergi- och plasmafysik

Journal of High Energy Physics

1126-6708 (ISSN) 1029-8479 (eISSN)

Vol. 2026 8 211

Susceptibilitet och materialeffeker i mörk materias spridning mot elektroner

Vetenskapsrådet (VR) (2022-04299), 2023-01-01 -- 2026-12-31.

Ämneskategorier (SSIF 2025)

Astronomi, astrofysik och kosmologi

Subatomär fysik

DOI

10.1007/JHEP08(2026)211

Mer information

Senast uppdaterat

2026-09-08