pith. sign in

arxiv: 2607.02026 · v1 · pith:VUQ2H466new · submitted 2026-07-02 · ✦ hep-ph

One-loop proton decay from Peccei-Quinn symmetry

Pith reviewed 2026-07-03 10:54 UTC · model grok-4.3

classification ✦ hep-ph
keywords Peccei-Quinn symmetryproton decayvector-like quarksaxionstrong CP problemZ2 symmetryone-loop processesKSVZ axion
0
0 comments X

The pith

Promoting the Standard Model B+L symmetry to Peccei-Quinn symmetry with vector-like quarks induces one-loop proton decay while a residual Z2 forbids tree-level decay.

A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.

The paper establishes that vector-like quarks can generate the QCD anomaly for a Kim-Shifman-Vainshtein-Zakharov axion while a residual Z2 symmetry after Peccei-Quinn breaking blocks tree-level proton decay. The same quarks plus Z2-odd scalar mediators produce the effective operator u_R u_R d_R e_R at one loop, allowing radiative proton decay. Different choices of representations yield distinct axion-photon couplings that can be tested in helioscope and haloscope searches. The setup also predicts an extra decay channel containing an axion, suppressed by the Peccei-Quinn scale, and allows axion dark matter in both pre- and post-inflationary cosmologies. A sympathetic reader would care because the construction ties the solution to the strong CP problem directly to a controlled, loop-level proton decay signal.

Core claim

We promote the accidental B+L symmetry of the Standard Model to a Peccei-Quinn symmetry while realizing spontaneous proton decay radiatively. The PQ anomaly sector consists of vector-like quarks providing a KSVZ-type axion solution to the strong CP problem. After spontaneous PQ breaking a residual Z2 symmetry remains which forbids tree-level proton decay. The VLQs required to generate the QCD anomaly, together with scalar mediators odd under the residual Z2, induce one-loop proton decay through the effective operator u_R u_R d_R e_R. The resulting models lead to distinct predictions for the axion-to-photon coupling.

What carries the argument

The residual Z2 symmetry after PQ breaking, together with vector-like quarks and Z2-odd scalars that generate the one-loop effective operator u_R u_R d_R e_R.

If this is right

  • Different ultraviolet completions with distinct vector-like fermion and scalar representations produce different values of the axion-photon coupling testable in helioscope and haloscope experiments.
  • The model predicts the additional decay channel p to e+ pi0 a, suppressed by the PQ-breaking scale.
  • Axion dark matter can be realized consistently in both pre-inflationary and post-inflationary cosmological scenarios.

Where Pith is reading between the lines

These are editorial extensions of the paper, not claims the author makes directly.

  • Searches for the axion-accompanied proton decay mode could serve as a distinctive signature that separates this mechanism from conventional GUT-induced decays.
  • The same Z2-odd scalars that mediate the loop may open new channels for axion production in astrophysical environments.
  • The construction suggests that other accidental global symmetries of the Standard Model could be promoted to Peccei-Quinn-like symmetries with similar radiative decay implications.

Load-bearing premise

Vector-like fermion and scalar representations exist that satisfy the PQ anomaly condition, carry the required Z2 charges, and generate a viable one-loop diagram for the u_R u_R d_R e_R operator without introducing other unwanted effects.

What would settle it

Observation of proton decay in the e+ pi0 channel at a rate far above the loop-suppressed expectation, or failure to find the predicted axion-photon coupling in the range fixed by the same representations, would rule out the construction.

Figures

Figures reproduced from arXiv: 2607.02026 by H. B. C\^amara.

Figure 1
Figure 1. Figure 1: FIG. 1: One-loop box diagram generating the proton decay operator [PITH_FULL_IMAGE:figures/full_fig_p005_1.png] view at source ↗
Figure 2
Figure 2. Figure 2: FIG. 2: One-loop proton (top) and neutron (bottom) two-body decays mediated by Ψ [PITH_FULL_IMAGE:figures/full_fig_p006_2.png] view at source ↗
Figure 3
Figure 3. Figure 3: FIG. 3: Axion-to-photon coupling [PITH_FULL_IMAGE:figures/full_fig_p011_3.png] view at source ↗
read the original abstract

We promote the accidental $B+L$ symmetry of the Standard Model to a Peccei-Quinn (PQ) symmetry while realizing spontaneous proton decay radiatively. The PQ anomaly sector consists of vector-like quarks (VLQs), providing a Kim-Shifman-Vainshtein-Zakharov-type axion solution to the strong CP problem. After spontaneous PQ breaking, a residual $\mathcal{Z}_2$ symmetry remains, which forbids tree-level proton decay. The VLQs required to generate the QCD anomaly, together with scalar mediators, odd under the residual $\mathcal{Z}_2$, induce one-loop proton decay through the effective operator $u_R u_R d_R e_R$. We study its ultraviolet completions, featuring distinct vector-like fermion and scalar representations, and show that the resulting models lead to distinct predictions for the axion-to-photon coupling, testable in helioscope and haloscope experiments. In addition to the proton decay channel $p \rightarrow e^+ \pi^0$, this framework predicts proton decay with an axion in the final state, $p \rightarrow e^+ \pi^0 a$, suppressed by the PQ-breaking scale. We also discuss axion dark matter in pre- and post-inflationary cosmology.

Editorial analysis

A structured set of objections, weighed in public.

Desk editor's note, referee report, simulated authors' rebuttal, and a circularity audit. Tearing a paper down is the easy half of reading it; the pith above is the substance, this is the friction.

Referee Report

1 major / 2 minor

Summary. The paper promotes the SM's accidental B+L symmetry to a global PQ symmetry solved by vector-like quarks (VLQs) in a KSVZ-like setup. Spontaneous PQ breaking leaves a residual Z2 that forbids all tree-level ΔB=1 operators. The same VLQs, together with additional Z2-odd scalar mediators, generate a one-loop diagram for the effective operator u_R u_R d_R e_R, inducing proton decay. Explicit UV completions with different fermion and scalar representations are constructed; these yield distinct values of the axion-photon coupling g_aγγ and predict an additional channel p → e⁺ π⁰ a suppressed by the PQ scale. Axion dark-matter cosmology in pre- and post-inflationary scenarios is also discussed.

Significance. If the charge assignments and loop diagrams are viable, the work supplies a concrete mechanism that simultaneously addresses the strong-CP problem and renders proton decay radiative while protecting against tree-level violation. The explicit construction of multiple UV completions that produce distinguishable g_aγγ predictions (testable in helioscopes and haloscopes) and the additional axion-accompanied decay mode constitute clear strengths. The framework is falsifiable and links two otherwise separate phenomenological sectors.

major comments (1)
  1. [UV completions] UV-completion sections: the manuscript states that the chosen VLQ and scalar representations simultaneously satisfy the QCD anomaly condition, carry the required Z2 charges, and permit a one-loop diagram for u_R u_R d_R e_R without generating tree-level ΔB=1 operators. An explicit listing or table of all allowed operators generated by the new fields at dimension 6 and below would make this claim directly verifiable; without it the protection argument remains schematic.
minor comments (2)
  1. [Abstract / Introduction] The abstract and introduction refer to 'distinct predictions for the axion-to-photon coupling' but do not quote the numerical ranges or the functional dependence on the PQ scale; adding a short table or explicit expressions would improve clarity.
  2. [Model setup] Notation for the residual Z2 charges on the scalar mediators is introduced without a dedicated charge table; a compact table listing all new fields, their SM quantum numbers, PQ charges, and Z2 parities would aid the reader.

Simulated Author's Rebuttal

1 responses · 0 unresolved

We thank the referee for the careful reading and positive assessment of our work. The single major comment is constructive and we address it directly below. We will incorporate the requested addition in the revised manuscript.

read point-by-point responses
  1. Referee: [UV completions] UV-completion sections: the manuscript states that the chosen VLQ and scalar representations simultaneously satisfy the QCD anomaly condition, carry the required Z2 charges, and permit a one-loop diagram for u_R u_R d_R e_R without generating tree-level ΔB=1 operators. An explicit listing or table of all allowed operators generated by the new fields at dimension 6 and below would make this claim directly verifiable; without it the protection argument remains schematic.

    Authors: We agree that an explicit operator table would make the Z2 protection argument immediately verifiable. In the revised version we will add a new table (or subsection) that enumerates all gauge- and Z2-invariant operators involving the VLQs and Z2-odd scalars up to dimension 6. The table will explicitly show (i) the absence of any tree-level ΔB=1 operators, (ii) the presence of the required one-loop diagram for u_R u_R d_R e_R, and (iii) consistency with the QCD anomaly condition. This addition will be placed in the UV-completion sections and will not alter any numerical results or conclusions. revision: yes

Circularity Check

0 steps flagged

No significant circularity identified

full rationale

The paper constructs explicit UV completions by choosing vector-like fermion and scalar representations that simultaneously satisfy the PQ anomaly condition, residual Z2 charge assignments, and permit a one-loop diagram for the u_R u_R d_R e_R operator. The resulting axion-photon coupling predictions follow directly from the anomaly coefficients of those chosen representations rather than from any fitted parameter or self-citation chain. No load-bearing step reduces by construction to an input; the central claims remain independent of the target observables once the representations are fixed.

Axiom & Free-Parameter Ledger

1 free parameters · 1 axioms · 1 invented entities

The construction rests on the existence of suitable VLQ representations for the anomaly and Z2-odd scalars for the loop; these are postulated without independent evidence beyond satisfying the stated conditions.

free parameters (1)
  • PQ breaking scale
    Suppresses the p -> e+ pi0 a channel; value not fixed by the abstract.
axioms (1)
  • domain assumption Vector-like quarks can be chosen to generate the required QCD anomaly while preserving a residual Z2 after PQ breaking.
    Invoked to enable both the axion and the one-loop decay.
invented entities (1)
  • Z2-odd scalar mediators no independent evidence
    purpose: To mediate the one-loop proton decay diagram together with VLQs.
    Introduced to realize the effective operator while respecting the residual symmetry.

pith-pipeline@v0.9.1-grok · 5742 in / 1368 out tokens · 40661 ms · 2026-07-03T10:54:26.340251+00:00 · methodology

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.

Reference graph

Works this paper leans on

83 extracted references · 55 canonical work pages · 32 internal anchors

  1. [1]

    Baryon and Lepton Nonconserving Processes,

    S. Weinberg, “Baryon and Lepton Nonconserving Processes,”Phys. Rev. Lett.43(1979) 1566–1570

  2. [2]

    Operator Analysis of Nucleon Decay,

    F. Wilczek and A. Zee, “Operator Analysis of Nucleon Decay,”Phys. Rev. Lett.43(1979) 1571–1573

  3. [3]

    The Effective Hamiltonian for Nucleon Decay,

    L. F. Abbott and M. B. Wise, “The Effective Hamiltonian for Nucleon Decay,”Phys. Rev. D22(1980) 2208

  4. [4]

    Baryon Number, Lepton Number, and Operator Dimension in the Standard Model

    A. Kobach, “Baryon Number, Lepton Number, and Operator Dimension in the Standard Model,”Phys. Lett. B758(2016) 455–457,arXiv:1604.05726 [hep-ph]

  5. [5]

    Dimension-Six Terms in the Standard Model Lagrangian

    B. Grzadkowski, M. Iskrzynski, M. Misiak, and J. Rosiek, “Dimension-Six Terms in the Standard Model Lagrangian,” JHEP10(2010) 085,arXiv:1008.4884 [hep-ph]

  6. [6]

    Unified Lepton-Hadron Symmetry and a Gauge Theory of the Basic Interactions,

    J. C. Pati and A. Salam, “Unified Lepton-Hadron Symmetry and a Gauge Theory of the Basic Interactions,”Phys. Rev. D8(1973) 1240–1251

  7. [7]

    Unity of All Elementary Particle Forces,

    H. Georgi and S. L. Glashow, “Unity of All Elementary Particle Forces,”Phys. Rev. Lett.32(1974) 438–441

  8. [8]

    Unified Interactions of Leptons and Hadrons,

    H. Fritzsch and P. Minkowski, “Unified Interactions of Leptons and Hadrons,”Annals Phys.93(1975) 193–266

  9. [9]

    Experimental Tests of Baryon and Lepton Number Conservation,

    V. Takhistov, “Experimental Tests of Baryon and Lepton Number Conservation,”arXiv:2602.09097 [hep-ph]. [10]Super-KamiokandeCollaboration, A. Takenakaet al., “Search for proton decay viap→e +π0 andp→µ +π0 with an enlarged fiducial volume in Super-Kamiokande I-IV,”Phys. Rev. D102no. 11, (2020) 112011,arXiv:2010.16098 [hep-ex]. [11]Hyper-KamiokandeCollaborat...

  10. [10]

    Proton decay at 1-loop

    J. C. Helo, M. Hirsch, and T. Ota, “Proton decay at one loop,”Phys. Rev. D99no. 9, (2019) 095021,arXiv:1904.00036 [hep-ph]

  11. [11]

    Radiative Seesaw Mechanism at Weak Scale

    Z.-j. Tao, “Radiative seesaw mechanism at weak scale,”Phys.Rev.D54(1996) 5693–5697,arXiv:hep-ph/9603309 [hep-ph]

  12. [12]

    Verifiable Radiative Seesaw Mechanism of Neutrino Mass and Dark Matter

    E. Ma, “Verifiable radiative seesaw mechanism of neutrino mass and dark matter,”Phys. Rev. D73(2006) 077301, arXiv:hep-ph/0601225

  13. [13]

    Extended scotogenic model of neutrino mass and proton decay,

    T. Nomura and O. Popov, “Extended scotogenic model of neutrino mass and proton decay,”Phys. Rev. D110no. 7, (2024) 075035,arXiv:2406.00651 [hep-ph]

  14. [14]

    Pathways to proton’s stability via naturally small neutrino masses,

    S. K. Kang and O. Popov, “Pathways to proton’s stability via naturally small neutrino masses,”arXiv:2412.20723 [hep-ph]

  15. [15]

    Dark Matter Induced Proton Decays

    R. Kumar and R. Srivastava, “Dark matter induced proton decays,”JHEP04(2026) 024,arXiv:2506.04370 [hep-ph]

  16. [16]

    A Revised Experimental Upper Limit on the Electric Dipole Moment of the Neutron

    J. M. Pendleburyet al., “Revised experimental upper limit on the electric dipole moment of the neutron,”Phys. Rev. D 92no. 9, (2015) 092003,arXiv:1509.04411 [hep-ex]

  17. [17]

    An Improved Experimental Limit on the Electric Dipole Moment of the Neutron

    C. A. Bakeret al., “An Improved experimental limit on the electric dipole moment of the neutron,”Phys. Rev. Lett.97 (2006) 131801,arXiv:hep-ex/0602020

  18. [18]

    CP Conservation in the Presence of Instantons,

    R. D. Peccei and H. R. Quinn, “CP Conservation in the Presence of Instantons,”Phys. Rev. Lett.38(1977) 1440–1443

  19. [19]

    Constraints Imposed by CP Conservation in the Presence of Instantons,

    R. D. Peccei and H. R. Quinn, “Constraints Imposed by CP Conservation in the Presence of Instantons,”Phys. Rev. D 16(1977) 1791–1797

  20. [20]

    A New Light Boson?,

    S. Weinberg, “A New Light Boson?,”Phys. Rev. Lett.40(1978) 223–226

  21. [21]

    Problem of StrongPandTInvariance in the Presence of Instantons,

    F. Wilczek, “Problem of StrongPandTInvariance in the Presence of Instantons,”Phys. Rev. Lett.40(1978) 279–282

  22. [22]

    On Possible Suppression of the Axion Hadron Interactions. (In Russian),

    A. R. Zhitnitsky, “On Possible Suppression of the Axion Hadron Interactions. (In Russian),”Sov. J. Nucl. Phys.31(1980) 14 260

  23. [23]

    A Simple Solution to the Strong CP Problem with a Harmless Axion,

    M. Dine, W. Fischler, and M. Srednicki, “A Simple Solution to the Strong CP Problem with a Harmless Axion,”Phys. Lett. B104(1981) 199–202

  24. [24]

    Weak Interaction Singlet and Strong CP Invariance,

    J. E. Kim, “Weak Interaction Singlet and Strong CP Invariance,”Phys. Rev. Lett.43(1979) 103

  25. [25]

    Can Confinement Ensure Natural CP Invariance of Strong Interac- tions?,

    M. A. Shifman, A. I. Vainshtein, and V. I. Zakharov, “Can Confinement Ensure Natural CP Invariance of Strong Interac- tions?,”Nucl. Phys. B166(1980) 493–506

  26. [26]

    The landscape of QCD axion models

    L. Di Luzio, M. Giannotti, E. Nardi, and L. Visinelli, “The landscape of QCD axion models,”Phys. Rept.870(2020) 1–117,arXiv:2003.01100 [hep-ph]

  27. [27]

    Cosmology of the Invisible Axion,

    J. Preskill, M. B. Wise, and F. Wilczek, “Cosmology of the Invisible Axion,”Phys. Lett. B120(1983) 127–132

  28. [28]

    A Cosmological Bound on the Invisible Axion,

    L. F. Abbott and P. Sikivie, “A Cosmological Bound on the Invisible Axion,”Phys. Lett. B120(1983) 133–136

  29. [29]

    The Not So Harmless Axion,

    M. Dine and W. Fischler, “The Not So Harmless Axion,”Phys. Lett. B120(1983) 137–141

  30. [30]

    µ→eγat a Rate of One Out of 10 9 Muon Decays?,

    P. Minkowski, “µ→eγat a Rate of One Out of 10 9 Muon Decays?,”Phys. Lett. B67(1977) 421–428

  31. [31]

    Complex Spinors and Unified Theories

    M. Gell-Mann, P. Ramond, and R. Slansky, “Complex Spinors and Unified Theories,”Conf. Proc. C790927(1979) 315–321,arXiv:1306.4669 [hep-th]

  32. [32]

    Horizontal gauge symmetry and masses of neutrinos,

    T. Yanagida, “Horizontal gauge symmetry and masses of neutrinos,”Conf. Proc. C7902131(1979) 95–99

  33. [33]

    Neutrino Masses in SU(2) x U(1) Theories,

    J. Schechter and J. W. F. Valle, “Neutrino Masses in SU(2) x U(1) Theories,”Phys. Rev. D22(1980) 2227

  34. [34]

    The Future of Elementary Particle Physics,

    S. L. Glashow, “The Future of Elementary Particle Physics,”NATO Sci. Ser. B61(1980) 687

  35. [35]

    Neutrino Mass and Spontaneous Parity Nonconservation,

    R. N. Mohapatra and G. Senjanovic, “Neutrino Mass and Spontaneous Parity Nonconservation,”Phys. Rev. Lett.44 (1980) 912

  36. [36]

    NATURALNESS OF THE INVISIBLE AXION MODEL,

    R. R. Volkas, A. J. Davies, and G. C. Joshi, “NATURALNESS OF THE INVISIBLE AXION MODEL,”Phys. Lett. B 215(1988) 133–138

  37. [37]

    $\nu$DFSZ: a technically natural non-supersymmetric model of neutrino masses, baryogenesis, the strong CP problem, and dark matter

    J. D. Clarke and R. R. Volkas, “Technically natural nonsupersymmetric model of neutrino masses, baryogenesis, the strong CP problem, and dark matter,”Phys. Rev. D93no. 3, (2016) 035001,arXiv:1509.07243 [hep-ph]

  38. [38]

    VISHν: a unified solution to five SM shortcomings with a protected electroweak scale,

    A. H. Sopov and R. R. Volkas, “VISHν: a unified solution to five SM shortcomings with a protected electroweak scale,” arXiv:2206.11598 [hep-ph]

  39. [39]

    VISHν: Flavour-Variant DFSZ Axion Model for Inflation, Neutrino Masses, Dark Matter, and Baryogene- sis,

    R. R. Volkas, “VISHν: Flavour-Variant DFSZ Axion Model for Inflation, Neutrino Masses, Dark Matter, and Baryogene- sis,”LHEP2023(2023) 358

  40. [40]

    Inflation and Higgs phenomenology in a model unifying the DFSZ axion with the majoron,

    M. Matlis, J. Dutta, G. Moortgat-Pick, and A. Ringwald, “Inflation and Higgs phenomenology in a model unifying the DFSZ axion with the majoron,”JCAP07(2024) 007,arXiv:2309.10857 [hep-ph]

  41. [41]

    A Simple Motivated Completion of the Standard Model below the Planck Scale: Axions and Right-Handed Neutrinos

    A. Salvio, “A Simple Motivated Completion of the Standard Model below the Planck Scale: Axions and Right-Handed Neutrinos,”Phys. Lett. B743(2015) 428–434,arXiv:1501.03781 [hep-ph]

  42. [42]

    Unifying inflation with the axion, dark matter, baryogenesis and the seesaw mechanism

    G. Ballesteros, J. Redondo, A. Ringwald, and C. Tamarit, “Unifying inflation with the axion, dark matter, baryogenesis and the seesaw mechanism,”Phys. Rev. Lett.118no. 7, (2017) 071802,arXiv:1608.05414 [hep-ph]

  43. [43]

    Standard Model-Axion-Seesaw-Higgs Portal Inflation. Five problems of particle physics and cosmology solved in one stroke

    G. Ballesteros, J. Redondo, A. Ringwald, and C. Tamarit, “Standard Model—axion—seesaw—Higgs portal inflation. Five problems of particle physics and cosmology solved in one stroke,”JCAP08(2017) 001,arXiv:1610.01639 [hep-ph]

  44. [44]

    Flavored Peccei-Quinn symmetries in the minimalνDFSZ model,

    J. R. Rocha, H. B. Cˆ amara, and F. R. Joaquim, “Flavored Peccei-Quinn symmetries in the minimalνDFSZ model,”Phys. Rev. D112no. 7, (2025) 075053,arXiv:2504.00088 [hep-ph]

  45. [45]

    Axion Paradigm with Color-Mediated Neutrino Masses,

    A. Batra, H. B. Cˆ amara, F. R. Joaquim, R. Srivastava, and J. W. F. Valle, “Axion Paradigm with Color-Mediated Neutrino Masses,”Phys. Rev. Lett.132no. 5, (2024) 051801,arXiv:2309.06473 [hep-ph]

  46. [46]

    Axion framework with color-mediated Dirac neutrino masses,

    A. Batra, H. B. Cˆ amara, F. R. Joaquim, N. Nath, R. Srivastava, and J. W. F. Valle, “Axion framework with color-mediated Dirac neutrino masses,”Phys. Lett. B868(2025) 139629,arXiv:2501.13156 [hep-ph]

  47. [47]

    Spontaneous proton decay and the origin of Peccei-Quinn symmetry

    M. Reig and R. Srivastava, “Spontaneous proton decay and the origin of Peccei–Quinn symmetry,”Phys. Lett. B790 (2019) 134–139,arXiv:1809.02093 [hep-ph]

  48. [48]

    $\Delta L = 3$ processes: Proton decay and LHC

    R. M. Fonseca, M. Hirsch, and R. Srivastava, “∆L= 3 processes: Proton decay and the LHC,”Phys. Rev. D97no. 7, (2018) 075026,arXiv:1802.04814 [hep-ph]

  49. [49]

    The QCD axion, precisely

    G. Grilli di Cortona, E. Hardy, J. Pardo Vega, and G. Villadoro, “The QCD axion, precisely,”JHEP01(2016) 034, arXiv:1511.02867 [hep-ph]. [54]Super-KamiokandeCollaboration, N. Taniuchiet al., “Search for proton decay via p→e+ηand p→µ+ηwith a 0.37 Mton- year exposure of Super-Kamiokande,”Phys. Rev. D110no. 11, (2024) 112011,arXiv:2409.19633 [hep-ex]. [55]Su...

  50. [50]

    Improved lattice computation of proton decay matrix elements

    Y. Aoki, T. Izubuchi, E. Shintani, and A. Soni, “Improved lattice computation of proton decay matrix elements,”Phys. Rev. D96no. 1, (2017) 014506,arXiv:1705.01338 [hep-lat]

  51. [51]

    Baryon-number-violating nucleon decays in ALP effective field theories,

    T. Li, M. A. Schmidt, and C.-Y. Yao, “Baryon-number-violating nucleon decays in ALP effective field theories,”JHEP08 (2024) 221,arXiv:2406.11382 [hep-ph]

  52. [52]

    Comprehensive investigation on baryon number violating nucleon decays involving an axion-like particle*,

    W.-Q. Fan, Y. Liao, X.-D. Ma, and H.-L. Wang, “Comprehensive investigation on baryon number violating nucleon decays involving an axion-like particle*,”Chin. Phys. C50no. 3, (2026) 033103,arXiv:2507.11844 [hep-ph]. [61]PlanckCollaboration, N. Aghanimet al., “Planck 2018 results. VI. Cosmological parameters,”Astron. Astrophys.641 (2020) A6,arXiv:1807.06209...

  53. [53]

    Isocurvature bounds on axions revisited

    M. Beltran, J. Garcia-Bellido, and J. Lesgourgues, “Isocurvature bounds on axions revisited,”Phys. Rev. D75(2007) 103507,arXiv:hep-ph/0606107

  54. [54]

    Redefining the Axion Window

    L. Di Luzio, F. Mescia, and E. Nardi, “Redefining the Axion Window,”Phys. Rev. Lett.118no. 3, (2017) 031801, arXiv:1610.07593 [hep-ph]

  55. [55]

    Revisiting isocurvature bounds on the minimal QCD axion,

    P. W. Graham and D. Racco, “Revisiting isocurvature bounds on the minimal QCD axion,”JHEP12(2025) 028, arXiv:2506.03348 [hep-ph]

  56. [56]

    Evidence for a Scaling Solution in Cosmic String Evolution,

    D. P. Bennett and F. R. Bouchet, “Evidence for a Scaling Solution in Cosmic String Evolution,”Phys. Rev. Lett.60(1988) 257

  57. [57]

    Gravitational Bose-Einstein condensation in the kinetic regime

    D. G. Levkov, A. G. Panin, and I. I. Tkachev, “Gravitational Bose-Einstein condensation in the kinetic regime,”Phys. Rev. Lett.121no. 15, (2018) 151301,arXiv:1804.05857 [astro-ph.CO]

  58. [58]

    Axions from Strings: the Attractive Solution

    M. Gorghetto, E. Hardy, and G. Villadoro, “Axions from Strings: the Attractive Solution,”JHEP07(2018) 151, arXiv:1806.04677 [hep-ph]

  59. [59]

    Early-Universe Simulations of the Cosmological Axion,

    M. Buschmann, J. W. Foster, and B. R. Safdi, “Early-Universe Simulations of the Cosmological Axion,”Phys. Rev. Lett. 124no. 16, (2020) 161103,arXiv:1906.00967 [astro-ph.CO]

  60. [60]

    Spontaneous Breaking of Lepton Number and Cosmological Domain Wall Problem

    G. Lazarides, M. Reig, Q. Shafi, R. Srivastava, and J. W. F. Valle, “Spontaneous Breaking of Lepton Number and the Cosmological Domain Wall Problem,”Phys. Rev. Lett.122no. 15, (2019) 151301,arXiv:1806.11198 [hep-ph]

  61. [61]

    Axion dark matter from topological defects

    M. Kawasaki, K. Saikawa, and T. Sekiguchi, “Axion dark matter from topological defects,”Phys. Rev. D91no. 6, (2015) 065014,arXiv:1412.0789 [hep-ph]

  62. [62]

    The dark-matter axion mass

    V. B. . Klaer and G. D. Moore, “The dark-matter axion mass,”JCAP11(2017) 049,arXiv:1708.07521 [hep-ph]

  63. [63]

    More axions from strings,

    M. Gorghetto, E. Hardy, and G. Villadoro, “More axions from strings,”SciPost Phys.10no. 2, (2021) 050, arXiv:2007.04990 [hep-ph]

  64. [64]

    Dark matter from axion strings with adaptive mesh refinement,

    M. Buschmann, J. W. Foster, A. Hook, A. Peterson, D. E. Willcox, W. Zhang, and B. R. Safdi, “Dark matter from axion strings with adaptive mesh refinement,”Nature Commun.13no. 1, (2022) 1049,arXiv:2108.05368 [hep-ph]

  65. [65]

    Axion Mass Prediction from Adaptive Mesh Refinement Cosmological Lattice Simulations,

    J. N. Benabou, M. Buschmann, J. W. Foster, and B. R. Safdi, “Axion Mass Prediction from Adaptive Mesh Refinement Cosmological Lattice Simulations,”Phys. Rev. Lett.134no. 24, (2025) 241003,arXiv:2412.08699 [hep-ph]

  66. [66]

    Of Axions, Domain Walls and the Early Universe,

    P. Sikivie, “Of Axions, Domain Walls and the Early Universe,”Phys. Rev. Lett.48(1982) 1156–1159

  67. [67]

    Using gravitational waves to see the first second of the Universe,

    R. Roshan and G. White, “Using gravitational waves to see the first second of the Universe,”Rev. Mod. Phys.97no. 1, (2025) 015001,arXiv:2401.04388 [hep-ph]

  68. [68]

    Constraining postinflationary axions with pulsar timing arrays,

    G. Servant and P. Simakachorn, “Constraining postinflationary axions with pulsar timing arrays,”Phys. Rev. D108no. 12, (2023) 123516,arXiv:2307.03121 [hep-ph]

  69. [69]

    Exploring the viability of a pseudo-Nambu-Goldstone boson as ultralight dark matter in a mass range relevant for strong gravity applications,

    A. P. Morais, V. Oliveira, A. Onofre, R. Pasechnik, and R. Santos, “Exploring the viability of a pseudo-Nambu-Goldstone boson as ultralight dark matter in a mass range relevant for strong gravity applications,”Phys. Rev. D110no. 3, (2024) 035008,arXiv:2305.03776 [hep-ph]

  70. [70]

    Are exotic stable quarks cosmologically allowed?,

    E. Nardi and E. Roulet, “Are exotic stable quarks cosmologically allowed?,”Phys. Lett. B245(1990) 105–110

  71. [71]

    The Search for Stable, Massive, Elementary Particles

    M. L. Perl, P. C. Kim, V. Halyo, E. R. Lee, I. T. Lee, D. Loomba, and K. S. Lackner, “The Search for stable, massive, elementary particles,”Int. J. Mod. Phys. A16(2001) 2137–2164,arXiv:hep-ex/0102033

  72. [72]

    Searches for fractionally charged particles,

    M. L. Perl, E. R. Lee, and D. Loomba, “Searches for fractionally charged particles,”Ann. Rev. Nucl. Part. Sci.59(2009) 47–65

  73. [73]

    Non-collider searches for stable massive particles

    S. Burdin, M. Fairbairn, P. Mermod, D. Milstead, J. Pinfold, T. Sloan, and W. Taylor, “Non-collider searches for stable 16 massive particles,”Phys. Rept.582(2015) 1–52,arXiv:1410.1374 [hep-ph]

  74. [74]

    Astrophysical Constraints on Singlet Scalars at LHC

    M. P. Hertzberg and A. Masoumi, “Astrophysical Constraints on Singlet Scalars at LHC,”JCAP04(2017) 028, arXiv:1607.06445 [hep-ph]

  75. [75]

    Towards Closing the Window on Strongly Interacting Dark Matter: Far-Reaching Constraints from Earth's Heat Flow

    G. D. Mack, J. F. Beacom, and G. Bertone, “Towards Closing the Window on Strongly Interacting Dark Matter: Far- Reaching Constraints from Earth’s Heat Flow,”Phys. Rev. D76(2007) 043523,arXiv:0705.4298 [astro-ph]

  76. [76]

    Window for preferred axion models

    L. Di Luzio, F. Mescia, and E. Nardi, “Window for preferred axion models,”Phys. Rev. D96no. 7, (2017) 075003, arXiv:1705.05370 [hep-ph]. [86]CASTCollaboration, V. Anastassopouloset al., “New CAST Limit on the Axion-Photon Interaction,”Nature Phys.13 (2017) 584–590,arXiv:1705.02290 [hep-ex]. [87]ADMXCollaboration, N. Duet al., “A Search for Invisible Axion...

  77. [77]

    Limits on the Abundance and Coupling of Cosmic Axions at 4.5-Microev< m(a)<5.0-Microev,

    S. De Panfilis, A. C. Melissinos, B. E. Moskowitz, J. T. Rogers, Y. K. Semertzidis, W. Wuensch, H. J. Halama, A. G. Prodell, W. B. Fowler, and F. A. Nezrick, “Limits on the Abundance and Coupling of Cosmic Axions at 4.5-Microev< m(a)<5.0-Microev,”Phys. Rev. Lett.59(1987) 839. [91]CAPPCollaboration, O. Kwonet al., “First Results from an Axion Haloscope at ...

  78. [78]

    Conceptual design of a new large superconducting toroid for IAXO, the new international AXion observatory,

    I. Shilon, A. Dudarev, H. Silva, and H. H. J. ten Kate, “Conceptual design of a new large superconducting toroid for IAXO, the new international AXion observatory,”IEEE Transactions on Applied Superconductivity23no. 3, (2013) 4500604– 4500604.https://doi.org/10.1109%2Ftasc.2013.2251052

  79. [79]

    ADMX Status

    I. Stern, “ADMX Status,”PoSICHEP2016(2016) 198,arXiv:1612.08296 [physics.ins-det]

  80. [80]

    MADMAX Status Report,

    S. Beurtheyet al., “MADMAX Status Report,”arXiv:2003.10894 [physics.ins-det]. [96]ALPHACollaboration, A. J. Millaret al., “Searching for dark matter with plasma haloscopes,”Phys. Rev. D107no. 5, (2023) 055013,arXiv:2210.00017 [hep-ph]

Showing first 80 references.