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Broad axion resonances: Clockwork ALPs at hadron colliders

Srimoy Bhattacharya*

Debajyoti Choudhury†

Suvam Maharana‡

Tripurari Srivastava§

  • *Contact author: bhattacharyasrimoy@gmail.com
  • †Contact author: debchou.physics@gmail.com
  • ‡Contact author: suvam.maharana_528@tifr.res.in
  • §Contact author: tripurarisri022@gmail.com
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Phys. Rev. D 112, 055030 – Published 19 September, 2025

DOI: https://doi.org/10.1103/dsmk-v7n8

Abstract

Scenarios with multiple pseudoscalars are interesting as they usually tend to provide a framework to naturally realize a light axion with a large decay constant which has rich applications in cosmology, especially in the context of inflation and light dark matter physics. On the other hand, from a particle physics perspective, this facilitates a solution to the strong CP problem with a low Peccei-Quinn symmetry breaking scale. One such realization is afforded within the framework of the clockwork mechanism where the axion can have suppressed couplings with the gluons or photons while its companion axionlike particles (ALPs) have relatively unsuppressed couplings, thereby facilitating detectability. We study a minimal clockwork model for the QCD axion invoking a Kim–Shifman–Vainshtein–Zakharov (KSVZ)-like setup and examine the visibility of its unique multi-ALP (an) signature at the LHC, the most sensitive channel being pp→an(+additional  jets) followed by an→γγ. In congruence with the astrophysical and cosmological bounds for the axion, a striking feature emerges for the case of light ALPs (m∼O(10  GeV)) wherein the mass splittings among the former are so small that the signal profile mimics that of a single broad resonance, or an axion iceberg. The scenario is found to be imminently testable by the end of LHC’s Run 3 phase for an integrated luminosity of ∼300  fb−1. A larger average ALP mass, on the other hand, results in multiple closely spaced peaks with a characteristic signal profile, and would be expected to be seen at the forthcoming HL-LHC. Possible additional signals are also listed.

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Phys. Rev. D 112, 055030– Published 19 September, 2025
  • Received 12 December 2024
  • Accepted 8 August 2025
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