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Composite heavy axion-like dark matter

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arxiv 2408.14245 v2 pith:HNQAG7ON submitted 2024-08-26 hep-ph astro-ph.COhep-th

classification hep-phastro-ph.COhep-th
keywords darkcompositeheavyaxion-likefermiongalpmatternovel
verification ladder T0 review T1 audit T2 compute T3 formal
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We propose a novel class of Dark Matter (DM) candidates in the form of a heavy composite Axion-Like Particle (ALP) with highly suppressed electromagnetic interactions populating vast yet unexplored domains in the ALP parameter space. This is achieved for the first time in the simplest dark confining gauge theory yielding a new composite glueball ALP (GALP) DM coupling-mass relation found in terms of two distinct fundamental scales -- the large dark fermion mass scale and the dynamical scale of dark confinement. The presence of a heavy fermion portal between the visible (photons) and dark (GALPs) sectors ensures a strong radiative suppression of the GALP-photon coupling naturally without any fine-tuning. The observable features of heavy GALP DM in a minimal realization are controlled by only three physical parameters. Our work paves the road for a novel research field exploring the theory and phenomenology of composite ALPs in multi-messenger astrophysics and cosmology.

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Cited by 1 Pith paper

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

  1. Analysis of axion-like particles in a top-quark pair production at the CLIC

    hep-ph 2025-01 conditional novelty 6.0 of 10

    A simulation shows the CLIC gamma-gamma mode could exclude ALP-top couplings down to about 0.11 TeV^-1 for ALP masses near 10 GeV.

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