English

Light Axion-Like Particles at Future Lepton Colliders

High Energy Physics - Phenomenology 2025-10-22 v2 High Energy Physics - Experiment

Abstract

Axion-like particles (ALPs) are well-motivated extensions of the Standard Model (SM) that appear in many new physics scenarios, with masses spanning a broad range. In this work, we systematically study the production and detection prospects of light ALPs at future lepton colliders, including electron-positron and multi-TeV muon colliders. At lepton colliders, light ALPs can be produced in association with a photon or a ZZ boson. For very light ALPs (ma<1m_a < 1 MeV), the ALPs are typically long-lived and escape detection, leading to a mono-VV (V=γ,ZV = \gamma, Z) signature. In the long-lived limit, we find that the mono-photon channel at the Tera-ZZ stage of future electron-positron colliders provides the strongest constraints on ALP couplings to SM gauge bosons, gaVVg_{aVV}, thanks to the high luminosity, low background, and resonant enhancement from on-shell ZZ bosons. At higher energies, the mono-photon cross section becomes nearly energy-independent, and the sensitivity is governed by luminosity and background. At multi-TeV muon colliders, the mono-ZZ channel can yield complementary constraints. For heavier ALPs (ma>100m_a > 100 MeV) that decay promptly, mono-VV signatures are no longer valid. In this case, ALPs can be probed via non-resonant vector boson scattering (VBS) processes, where the ALP is exchanged off-shell, leading to kinematic deviations from SM expectations. We analyze constraints from both light-by-light scattering and electroweak VBS, the latter only accessible at TeV-scale colliders. While generally weaker, these constraints are robust and model-independent. Our combined analysis shows that mono-VV and non-resonant VBS channels provide powerful and complementary probes of ALP-gauge boson interactions.

Keywords

Cite

@article{arxiv.2505.10023,
  title  = {Light Axion-Like Particles at Future Lepton Colliders},
  author = {Shou-shan Bao and Yang Ma and Yongcheng Wu and Keping Xie and Hong Zhang},
  journal= {arXiv preprint arXiv:2505.10023},
  year   = {2025}
}

Comments

Published on JHEP

R2 v1 2026-06-28T23:34:03.060Z