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Color Unifed Dynamical Axion

Canonical reference. 83% of citing Pith papers cite this work as background.

9 Pith papers citing it
Background 83% of classified citations
abstract

We consider an enlarged color sector which solves the strong CP problem via new massless fermions. The spontaneous breaking of a unified color group into QCD and another confining group provides a source of naturally large axion mass $m_a$ due to small size instantons. This extra source of axion mass respects automatically the alignment of the vacuum, ensuring a low-energy CP-conserving vacuum. The mechanism does not appeal to a $Z_2$ 'mirror' copy of the SM, nor does it require any fine-tuning of the axion-related couplings at the unification scale. There is no light axion and uncharacteristically the lighter spectrum contains instead sterile fermions. The axion scale $f_a$ can be naturally brought down to a few TeV, with an exotic spectrum of colored pseudoscalars lighter than this scale, observable at colliders exclusively via strong interactions. The $\{m_a, f_a\}$ parameter space which allows a solution of the strong CP problem is thus enlarged well beyond that of invisible axion models.

citation-role summary

background 6

citation-polarity summary

years

2026 6 2025 3

verdicts

UNVERDICTED 9

roles

background 6

polarities

background 5 unclear 1

representative citing papers

Heavy Axion from a Confining Mirror GUT

hep-ph · 2026-05-27 · unverdicted · novelty 6.0

A mirror GUT model confines dynamically to produce a heavy axion solving the strong CP problem while allowing observable EDMs and a rich hidden sector.

The structure of multi-axion solutions to the strong CP problem

hep-ph · 2026-05-07 · unverdicted · novelty 6.0 · 2 refs

Multi-axion solutions to the strong CP problem produce varied mass-coupling patterns set by PQ symmetry breaking structure and QCD-EM anomaly alignment, summarized by a general sum rule for N-axion systems.

Accidental Peccei-Quinn Symmetry from Chiral Gauge Symmetry and Mirror QCD

hep-ph · 2026-04-27 · unverdicted · novelty 6.0

A chiral U(1) gauge symmetry generates an accidental Peccei-Quinn symmetry broken by mirror QCD, solving the strong CP problem without a light axion while supplying WIMP dark matter, stochastic gravitational waves, and LHC-testable colored pNGBs.

A Closer Look at Constrained Instantons

hep-th · 2026-04-03 · unverdicted · novelty 6.0

Constrained instantons satisfy all boundary conditions consistently in massive φ⁴ and broken Yang-Mills theories when asymptotic behaviors are tracked properly, resolving a prior claimed inconsistency.

Oscillating Imprints of Dark Matter in Mesons Decays

hep-ph · 2026-05-22 · unverdicted · novelty 5.0

Ultralight dark matter induces oscillating CKM elements that can be probed at NA62 through direct counting of meson decay events, which avoids sensitivity loss from unknown particle flux.

High-Quality Axion Dark Matter at Gravitational Wave Interferometers

hep-ph · 2025-09-17 · unverdicted · novelty 5.0

In gauged U(1) completions enabling high-quality axion dark matter, cosmic string loops generate a stochastic gravitational wave background with an infrared break frequency that exceeds foregrounds above 10^14 GeV breaking scales and offers a probe at interferometers.

citing papers explorer

Showing 9 of 9 citing papers.

  • A covariant description of the interactions of axion-like particles and hadrons hep-ph · 2025-06-18 · unverdicted · none · ref 17 · internal anchor

    A covariant framework identifies redefinition-invariant ALP couplings to gluons and quarks and computes physical decay rates for mixed scenarios.

  • Heavy Axion from a Confining Mirror GUT hep-ph · 2026-05-27 · unverdicted · none · ref 15 · internal anchor

    A mirror GUT model confines dynamically to produce a heavy axion solving the strong CP problem while allowing observable EDMs and a rich hidden sector.

  • The structure of multi-axion solutions to the strong CP problem hep-ph · 2026-05-07 · unverdicted · none · ref 60 · 2 links · internal anchor

    Multi-axion solutions to the strong CP problem produce varied mass-coupling patterns set by PQ symmetry breaking structure and QCD-EM anomaly alignment, summarized by a general sum rule for N-axion systems.

  • Braking protons at the EIC: from invisible meson decay to new physics searches hep-ph · 2025-12-31 · unverdicted · none · ref 80 · internal anchor

    The EIC can probe invisible pseudoscalar meson decays down to branching ratios of 10^{-8} and invisibly decaying ALPs with couplings up to 10^5 GeV for masses 0.1-2 GeV.

  • Accidental Peccei-Quinn Symmetry from Chiral Gauge Symmetry and Mirror QCD hep-ph · 2026-04-27 · unverdicted · none · ref 41

    A chiral U(1) gauge symmetry generates an accidental Peccei-Quinn symmetry broken by mirror QCD, solving the strong CP problem without a light axion while supplying WIMP dark matter, stochastic gravitational waves, and LHC-testable colored pNGBs.

  • On Exclusive Coherent Production of Bosons in Electron-Proton Collisions hep-ph · 2026-04-09 · unverdicted · none · ref 54

    A phenomenological 2-to-3 framework is constructed for exclusive boson electroproduction that matches flux-factorized predictions near Q^{2}=0 while capturing finite-Q^{2} effects at larger virtualities.

  • A Closer Look at Constrained Instantons hep-th · 2026-04-03 · unverdicted · none · ref 21

    Constrained instantons satisfy all boundary conditions consistently in massive φ⁴ and broken Yang-Mills theories when asymptotic behaviors are tracked properly, resolving a prior claimed inconsistency.

  • Oscillating Imprints of Dark Matter in Mesons Decays hep-ph · 2026-05-22 · unverdicted · none · ref 32 · internal anchor

    Ultralight dark matter induces oscillating CKM elements that can be probed at NA62 through direct counting of meson decay events, which avoids sensitivity loss from unknown particle flux.

  • High-Quality Axion Dark Matter at Gravitational Wave Interferometers hep-ph · 2025-09-17 · unverdicted · none · ref 41 · internal anchor

    In gauged U(1) completions enabling high-quality axion dark matter, cosmic string loops generate a stochastic gravitational wave background with an infrared break frequency that exceeds foregrounds above 10^14 GeV breaking scales and offers a probe at interferometers.