REVIEW 4 major objections 4 minor 116 references
Axion framework with color-mediated Dirac neutrino masses
T0 review · 4 major / 4 minor · reviewed 2026-08-10 · deepseek-v4-flash
Pith's one-line read A single Peccei-Quinn symmetry is proposed to generate radiative Dirac neutrino masses, solve the strong CP problem, and supply the axion as dark matter.
desk verdict Table I's PQ charges forbid the charged-lepton Yukawa, the leading Dirac operator, and the Yη loop vertex, so the central model fails as written, despite a worthwhile framework direction and careful phenomenology. read the letter →
The pith
A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.
The reading
What carries the argument
The central object is the one-loop color-mediated neutrino mass formula, Eq. (9), together with the Peccei-Quinn charge assignments in Tables I and II. The formula sums over the five quark mass eigenstates (three standard quarks plus two vector-like quarks) and the two scalar mass eigenstates $\zeta_{1,2}$ that come from mixing the leptoquarks $\eta$ and $\chi$ through the $\kappa(\eta^\dagger\Phi)\chi$ term: $$(M_\nu)_{\$\alpha$\$\beta$} = \frac{N_c}{16\$pi^{2}$\sqrt{2}}\sum_{j,k=1}^{5}(\tilde Y_\eta)_{\$\alpha$ j}(\tilde Y_\chi)_{j\$\beta$}R_{1k}R_{2k}\frac{\tilde m_j}{m_{\zeta_k}^2 - \tilde $m_j^{2}$}\ln\left(\frac{\tilde $m_j^{2}$}{m_{\zeta_k}^2}\right).$$ This formula is what turns the axion's colored fermions into the origin of neutrino mass. The residual $\mathbb{Z}_3$ is the symmetry selector that allows only Dirac operators, while the anomaly factors $N$ and $E$ computed from the same charges feed the axion-to-photon coupling relation $g_{a\gamma\gamma} = \frac{\alpha_e}{2\pi f_a}\left(\frac{E}{N} - 1.92(4)\right)$, and the heavy-light mixing matrices $\Theta^q_X$ feed the flavor-violating axion couplings of Eq. (14).
What would settle it
Computing the Peccei-Quinn charge of the coupling term that connects the lepton doublet, the colored scalar, and the vector-like quark for each of the seven representations would settle the internal consistency: any nonzero charge would break the symmetry that the strong-CP solution, the Dirac nature of neutrinos, and the axion dark-matter picture all depend on. Experimentally, a haloscope search that covers the predicted $m_a \sim 1$–$200\,\mu$eV band without detecting axions in the predicted axion-to-photon coupling lines would rule out the framework's dark-matter claim.
Extended reading notes
Core claim
On the paper's own terms, the central discovery is that a global $U(1)_{\rm PQ}$ under which the vector-like quarks $\Psi$ are chirally charged does double duty: it is the symmetry whose spontaneous breaking yields the axion, and it forbids Majorana neutrino mass terms so neutrinos are forced to be Dirac. The charge assignments leave a residual $\mathbb{Z}_3$ under which leptons and scalar leptoquarks rotate by different powers, which selects the dimension-five Dirac operator $(\bar\ell_L \tilde\Phi \nu_R)\sigma^*$ while blocking all Majorana operators. The one-loop diagram with $\Psi$, $\eta$, and $\chi$ then gives the neutrino mass matrix of Eq. (9), and the paper shows that the anomaly factors $N=1,2,3$ and the electromagnetic anomaly ratio $E/N$ vary across the seven viable vector-like quark representations, producing distinct, experimentally distinguishable axion-to-photon couplings. In three of the models, heavy-light quark mixing is large enough to induce flavor-violating axion-quark couplings, which are constrained by rare decays, meson mixing, and top decays. The axion can also account for the dark-matter abundance, with the post-inflationary case selecting $f_a$ in the range preferred by string-network simulations for the $N_{\rm DW}=1$ models.
Load-bearing premise
The load-bearing premise is that the Peccei-Quinn symmetry is an exact symmetry of every interaction term in the model, in particular that the term coupling the lepton doublet, the colored scalar, and the vector-like quark carries zero Peccei-Quinn charge for all seven representations; the paper states this condition but does not verify it case by case.
Editorial extensions
If this is right
- The seven vector-like-quark representations give seven distinct $E/N$ values, so measuring $g_{a\gamma\gamma}$ at the level projected for next-generation haloscopes and helioscopes can discriminate which representation, if any, is realized.
- In the post-inflationary dark-matter picture, only the isosinglet models with $N_{\rm DW}=1$ avoid the domain-wall problem; the isodoublet and isotriplet models require a bias term or a pre-inflationary breaking history.
- With two vector-like quark families, the neutrino mass matrix has rank two, so the lightest neutrino is massless and no light-neutrino-exchange contribution to neutrinoless double beta decay is expected; a third family would make all three neutrinos massive.
- Three models develop sizable heavy-light mixing, leading to flavor-violating axion-quark couplings; the combined bounds from rare meson decays, $D^0$–$\bar{D}^0$ mixing, and top-quark decays restrict the heavy bare mass parameter to the range $M_B\in[10^8,10^{10}]$ GeV.
- Because the same PQ symmetry supplies an accidental baryon number, proton decay operators are forbidden, so the colored leptoquarks and vector-like quarks can be present at the PQ scale without destabilizing matter.
Reading between the lines
- Beyond the paper, the residual-$\mathbb{Z}_3$ selection rule is a portable trick: any symmetry that leaves the same unbroken $\mathbb{Z}_3$ could play the role of the global PQ symmetry, which would also address the 'PQ quality' problem the authors explicitly flag.
- Beyond the paper, the predicted $E/N$ ladder offers a sharp discrimination strategy: if a future axion search fixes $g_{a\gamma\gamma}$ while the dark-matter requirement fixes $f_a$, that single measurement would select one of the seven vector-like-quark representations and dictate the quantum numbers of the colored scalars for collider searches.
- Beyond the paper, the models with sizable down-quark flavor-violating axion couplings are natural candidates for an axion-based explanation of the $B^+\to K^+ + E_{\rm miss}$ anomaly, an avenue the paper mentions but does not develop.
- Beyond the paper, a numerical fit of Eq. (9) to current neutrino oscillation data has not been shown; doing so would test whether the minimal two-family realization can reproduce the measured splittings and mixing angles, or whether a third family is needed.
Editorial analysis
A structured set of objections, weighed in public.
Referee Report
Summary. This paper proposes a KSVZ-type axion framework in which vector-like quarks and two scalar leptoquarks generate radiative Dirac neutrino masses at one loop, while an anomalous U(1)_PQ symmetry (with the exotic fermions charged) solves the strong CP problem and provides axion dark matter. Seven representations of vector-like quarks are surveyed, leading to distinct predictions for the axion-to-photon coupling and, in three cases, sizable flavor-violating axion-quark couplings. The one-loop neutrino mass formula, the anomaly coefficients, and the heavy-light mixing appendix are standard and clearly presented. However, the charge assignments in Tables I and II do not render the Yukawa and effective operators invariant under the SM hypercharge and PQ symmetries, so the central model as written is not internally consistent.
Significance. If the symmetry assignments were corrected, the framework would be a notable unification of radiative Dirac neutrino masses with the QCD axion, with falsifiable predictions: distinct E/N ratios for each vector-like quark representation, a restricted fa range for dark matter, and flavor-violating axion couplings that can be probed in haloscopes, helioscopes, and flavor experiments. The paper's strengths are the systematic listing of the seven representations, the explicit one-loop formula in Eq. (9), the detailed heavy-light mixing appendix, and the honest acknowledgment of the PQ quality problem. Nevertheless, the hypercharge and PQ charge inconsistencies mean that the phenomenological predictions in Figs. 2 and 3 and the neutrino mass formula are not yet attached to a valid model; the present version cannot be accepted as it stands.
major comments (4)
- [II B, Eq. (6), Tables I/II] The Yukawa vertices in Eq. (6) are not invariant under U(1)_Y for any of the listed representations. Taking \tilde η = iτ2 η* as the standard SU(2)-conjugate notation (the same convention used for \tilde Φ), the Yη vertex has hypercharge -1/2 - (yΨ + 1/2) + yΨ = -1, while the Yχ vertex has hypercharge yΨ + yΨ + 0 = 2yΨ, which is non-zero for every yΨ appearing in Table II. Hence the one-loop diagram in Fig. 1 is not a gauge-invariant amplitude under the stated field content. The authors must correct the hypercharges of η and χ (or the definition of \tilde η) and re-derive the allowed couplings.
- [II, Table I and the first bullet] The charged-lepton Yukawa ℓL Φ eR carries PQ charge 1/6 + 0 + 1/6 = 1/3 under the charges printed in Table I, so it is forbidden by the exact PQ symmetry and the model cannot generate charged-lepton masses. The claimed leading Dirac operator (ℓL \tilde Φ νR) σ* of Eq. (2) has PQ charge 1/6 + 4/6 - 1/2 = 1/3 and is likewise forbidden. A complete, term-by-term PQ charge-conservation check should be provided for the entire Lagrangian, including the SM Yukawa sector.
- [II B, Eq. (6)] The PQ charge sum of the Yη ℓL \tilde η ΨR term is 1/3 for \tilde η = iτ2 η* (independent of QPQ), so this vertex is never PQ-invariant under Table I. If instead \tilde η = η, the PQ charge is 2 QPQ - 1, which vanishes only for QPQ = 1/2, but then the Yχ ΨL χ νR and YΨ ΨL ΨR σ terms have PQ charge 2 QPQ = 1 and are forbidden. Thus, for every representation in Table II, at least one term of Eq. (6) explicitly breaks U(1)_PQ, invalidating the claimed Diracness of neutrinos and the strong-CP solution.
- [II, first bullet] The residual Z3 symmetry is not realized by the stated charges. For a Z3 to survive the σ VEV, the PQ charge of σ must be a multiple of 3 in a normalization where the Z3 phase is 2π/3; with qσ = 1/2, σ transforms nontrivially under every phase, so no such discrete subgroup remains. Moreover, the statement that ℓL, eR, and νR all transform as ω under a residual Z3 is incompatible with the gauge-invariant charged-lepton Yukawa, which requires qℓ + qe = 0. The authors should specify the discrete charges explicitly and verify that they forbid every Majorana operator in Eq. (1) while allowing the Dirac operator in Eq. (2).
minor comments (4)
- [III B, near Eq. (15)] The text refers to 'Ψ ∼ (3, 1, 1/6)' as one of the two models with sizable up-quark flavor-violating couplings; this should read 'Ψ ∼ (3, 2, 1/6)', the isodoublet model with sizable Θu_L in Table III.
- [Eq. (6) and Table I] The symbol \tilde η is never defined; since the hypercharge and PQ invariance checks depend on whether it denotes η or iτ2 η*, please define it explicitly in the text.
- [Table I caption] The PQ charges of the SM quark fields are not listed, although the text later assumes they vanish; please state this assumption in the table caption or in the main text.
- [Eq. (14)] The index structure in Eq. (14) is unclear: the last equality mixes qαX and qβX without specifying the Hermitian contraction, and the relation (cqV)αβ = (cqA)αβ = cq_αβ should be stated with explicit indices and a definition of the flavor matrices involved.
Circularity Check
No significant circularity: the Dirac neutrino loop formula, E/N anomaly ratios, and flavor-violating axion couplings are computed from the stated field content and symmetries rather than fitted to the quantities they predict. Self-citations to the prior color-mediated framework are not load-bearing for the Dirac-specific derivation.
full rationale
The paper's central derivation chain is not circular. The one-loop Dirac neutrino mass formula (Eq. 9) follows from the Yukawa interactions in Eq. (6), the scalar-potential term in Eq. (7), and the eta-chi mixing in Eq. (A3); Eq. (10) is an order-of-magnitude benchmark, not a fit of neutrino data used to define the model. The axion-to-photon coupling predictions (Eqs. 12 and 13, Fig. 2) are anomaly coefficients computed from the Table I PQ charges and are not extracted from haloscope or helioscope data. The flavor-violating axion-quark couplings in Eq. (14) are derived from the heavy-light mixing matrices computed in Appendix B, with external bounds from Refs. [98, 99] applied afterward. The statement that the PQ symmetry ensures Diracness is a model-building assignment, not a hidden prediction: the lepton PQ charges were chosen to leave a residual Z3 that forbids Majorana operators, and the testable content lies in the E/N values and flavor couplings. The self-citations to Refs. [49] and [115] supply the earlier color-mediated framework and flavor-anomaly applications, but the Dirac loop calculation and axion predictions are presented self-contained and are not reductions to those citations; hence they do not raise the circularity score. The paper also explicitly acknowledges the PQ quality problem and the unresolved topological-defect contribution to axion DM, which are limitations rather than circular steps. Separately, and as a correctness matter rather than a circularity: using the printed Table I charges, the charged-lepton Yukawa ell_L Phi e_R has PQ charge 1/6+0+1/6 = 1/3, and the claimed leading Dirac operator (ell_L Phi-tilde nu_R) sigma* has PQ charge 1/6+4/6-1/2 = 1/3; both are thus forbidden by the stated U(1)_PQ. The authors should supply a corrected charge table or an explicit term-by-term invariance check for Eqs. (2) and (6). This is a load-bearing consistency issue, but it is not an input-output circularity.
Assumptions & free parameters
free parameters (7)
- Number of VLQ species NΨ =
2
- PQ charge assignment QPQ per VLQ representation =
0 or 1/2 depending on model
- Yukawa matrices Yη, Yχ, YΨ =
benchmark ~10^-2 in Eq. (10)
- Scalar cubic coupling κ =
10^2 GeV benchmark in Eq. (10)
- Bare heavy-light mass MB =
benchmarks 10^6 to 10^11 GeV, constrained to 10^8 to 10^10 GeV
- Axion decay constant fa =
around 5 x 10^11 GeV for theta0 of order one; post-inflationary band 5 x 10^9 to 3 x 10^11 GeV
- Initial misalignment angle theta0 =
free in pre-inflationary case; averaged to sqrt(2.152) in post-inflationary case
assumptions (6)
- standard math The one-loop neutrino mass formula of Eq. (9), taken from Ref. [30], applies to this color-mediated Dirac setup with the R matrix of Eq. (A3).
- domain assumption The PQ charge assignments in Table I leave a residual Z3 symmetry that forbids all Majorana operators of Eq. (1) while allowing the Dirac operator of Eq. (2).
- domain assumption Heavy-light quark mixing is in the seesaw regime Md much less than MΨd and MΨ, so the block diagonalization in Appendix B is valid.
- standard math The QCD axion mass and axion-photon coupling relations from Ref. [79] are model independent at NLO.
- domain assumption Post-inflationary axion string simulations restrict fa to the range 5 x 10^9 to 3 x 10^11 GeV for NDW=1.
- ad hoc to paper A global U(1)PQ symmetry survives Planck-scale corrections, the so-called PQ quality problem.
invented entities (4)
-
Right-handed neutrinos νR
-
Vector-like quarks Ψ
-
Scalar leptoquarks η and χ
-
PQ scalar σ and its axion
independent evidence
Cite this review
Pith. "Pith review of Axion framework with color-mediated Dirac neutrino masses." pith.science (2026). https://pith.science/paper/UAUIB6H6
@misc{pith2026250113156,
author = {Pith},
title = {Pith review of: Axion framework with color-mediated Dirac neutrino masses},
year = {2026},
howpublished = {\url{https://pith.science/paper/UAUIB6H6}},
note = {Machine review of arXiv:2501.13156}
}
read the original abstract
We propose a KSVZ-type axion framework in which vector-like quarks (VLQ) and colored scalars generate Dirac neutrino masses radiatively. The global Peccei-Quinn symmetry (under which the exotic fermions are charged) addresses the strong CP problem and ensures the Dirac nature of neutrinos. The axion also accounts for the observed cosmological dark matter. We systematically explore all viable VLQ representations. Depending on the specific scenario, the framework predicts distinct axion-to-photon couplings, testable through haloscope and helioscope experiments, as well as potentially significant flavor-violating quark-axion interactions.
Figures
Reference graph
Works this paper leans on
-
[1]
Nobel Lecture: Discovery of atmospheric neutrino oscillations,
T. Kajita, “Nobel Lecture: Discovery of atmospheric neutrino oscillations,” Rev. Mod. Phys. 88 no. 3, (2016) 030501
2016
-
[2]
As we will see in Sec. II C, fa ∼ O(1012) GeV is the typical scale required for the axion particle to account for the observed DM abundance. Notice that the parameter κ can be naturally small in the t’ Hooft sense [80], as in the limit κ → 0, the theory exhibits a larger symmetry. It follows that the smallness of Dirac neutrino masses is naturally control...
arXiv 2020
-
[3]
Nobel Lecture: The Sudbury Neutrino Observatory: Observation of flavor change for solar neutrinos,
A. B. McDonald, “Nobel Lecture: The Sudbury Neutrino Observatory: Observation of flavor change for solar neutrinos,” Rev. Mod. Phys. 88 no. 3, (2016) 030502
2016
-
[4]
Teoria simmetrica dell’elettrone e del positrone,
E. Majorana, “Teoria simmetrica dell’elettrone e del positrone,” Nuovo Cim. 14 (1937) 171– 184
1937
-
[5]
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. D 22 (1980) 2227
1980
-
[6]
µ → eγ at a Rate of One Out of 109 Muon Decays?,
P. Minkowski, “ µ → eγ at a Rate of One Out of 109 Muon Decays?,” Phys. Lett. B 67 (1977) 421–428
1977
-
[7]
Complex Spinors and Unified Theories,
M. Gell-Mann, P. Ramond, and R. Slansky, “Complex Spinors and Unified Theories,” Conf. Proc. C 790927 (1979) 315–321, arXiv:1306.4669 [hep-th]
arXiv 1979
-
[8]
Horizontal gauge symmetry and masses of neutrinos,
T. Yanagida, “Horizontal gauge symmetry and masses of neutrinos,” Conf. Proc. C 7902131 (1979) 95–99
1979
Show all 116 references
-
[9]
The Future of Elementary Particle Physics,
S. L. Glashow, “The Future of Elementary Particle Physics,” NATO Sci. Ser. B 61 (1980) 687
1980
-
[10]
Neutrino Mass and Spontaneous Parity Nonconserva- tion,
R. N. Mohapatra and G. Senjanovic, “Neutrino Mass and Spontaneous Parity Nonconserva- tion,” Phys. Rev. Lett. 44 (1980) 912. 23
1980
-
[11]
Quantum Numbers of Majorana Neutrino Masses,
A. Zee, “Quantum Numbers of Majorana Neutrino Masses,” Nucl. Phys. B 264 (1986) 99– 110
1986
-
[12]
Model of ’Calculable’ Majorana Neutrino Masses,
K. S. Babu, “Model of ’Calculable’ Majorana Neutrino Masses,” Phys. Lett. B 203 (1988) 132–136
1988
-
[13]
Radiative seesaw mechanism at weak scale,
Z.-j. Tao, “Radiative seesaw mechanism at weak scale,” Phys.Rev.D 54 (1996) 5693–5697, arXiv:hep-ph/9603309 [hep-ph]
1996 arXiv
-
[14]
Verifiable radiative seesaw mechanism of neutrino mass and dark matter,
E. Ma, “Verifiable radiative seesaw mechanism of neutrino mass and dark matter,” Phys. Rev. D 73 (2006) 077301, arXiv:hep-ph/0601225
2006 arXiv
-
[15]
Effective Gauge Theories,
S. Weinberg, “Effective Gauge Theories,” Phys. Lett. B 91 (1980) 51–55
1980
-
[16]
Neutrinoless Double beta Decay in SU(2) x U(1) Theories,
J. Schechter and J. W. F. Valle, “Neutrinoless Double beta Decay in SU(2) x U(1) Theories,” Phys. Rev. D 25 (1982) 2951
1982
-
[17]
The Physics of Neutrinoless Double Beta Decay: A Primer,
B. J. P. Jones, “The Physics of Neutrinoless Double Beta Decay: A Primer,” in Theoretical Advanced Study Institute in Elementary Particle Physics: The Obscure Universe: Neutrinos and Other Dark Matters . 8, 2021. arXiv:2108.09364 [nucl-ex]
2021 arXiv
-
[18]
Neutrinoless Double-Beta Decay: A Roadmap for Matching Theory to Experiment,
V. Cirigliano et al. , “Neutrinoless Double-Beta Decay: A Roadmap for Matching Theory to Experiment,” arXiv:2203.12169 [hep-ph]
-
[19]
Neutrinoless Double-Beta Decay: Status and Prospects,
M. J. Dolinski, A. W. P. Poon, and W. Rodejohann, “Neutrinoless Double-Beta Decay: Status and Prospects,” Ann. Rev. Nucl. Part. Sci. 69 (2019) 219–251, arXiv:1902.04097 [nucl-ex]
2019 arXiv
-
[20]
Dirac neutrinos from flavor symmetry,
A. Aranda et al. , “Dirac neutrinos from flavor symmetry,” Phys. Rev. D 89 no. 3, (2014) 033001, arXiv:1307.3553 [hep-ph]
2014 arXiv
-
[21]
Dirac or inverse seesaw neutrino masses with B − L gauge symmetry and S3 flavor symmetry,
E. Ma and R. Srivastava, “Dirac or inverse seesaw neutrino masses with B − L gauge symmetry and S3 flavor symmetry,” Phys. Lett. B 741 (2015) 217–222, arXiv:1411.5042 [hep-ph]
2015 arXiv
-
[22]
String completion of an SU(3) c ⊗ SU(3)L ⊗ U(1)X electroweak model,
A. Addazi, J. W. F. Valle, and C. A. Vaquera-Araujo, “String completion of an SU(3) c ⊗ SU(3)L ⊗ U(1)X electroweak model,” Phys. Lett. B 759 (2016) 471–478, arXiv:1604.02117 [hep-ph]
2016 arXiv
-
[23]
Flavour-symmetric type-II Dirac neutrino seesaw mechanism,
C. Bonilla, J. M. Lamprea, E. Peinado, and J. W. F. Valle, “Flavour-symmetric type-II Dirac neutrino seesaw mechanism,” Phys. Lett. B 779 (2018) 257–261, arXiv:1710.06498 [hep-ph]
2018 arXiv
-
[24]
Dynamical seesaw mechanism for Dirac neutri- nos,
J. W. F. Valle and C. A. Vaquera-Araujo, “Dynamical seesaw mechanism for Dirac neutri- nos,” Phys. Lett. B 755 (2016) 363–366, arXiv:1601.05237 [hep-ph]
2016 arXiv
-
[25]
Realistic SU(3) c ⊗ SU(3)L ⊗ U(1)X model with a type II Dirac neutrino seesaw mechanism,
M. Reig, J. W. F. Valle, and C. A. Vaquera-Araujo, “Realistic SU(3) c ⊗ SU(3)L ⊗ U(1)X model with a type II Dirac neutrino seesaw mechanism,” Phys. Rev. D 94 no. 3, (2016) 033012, arXiv:1606.08499 [hep-ph]
2016 arXiv
-
[26]
Naturally light neutrinos in Diracon model,
C. Bonilla and J. W. F. Valle, “Naturally light neutrinos in Diracon model,” Phys. Lett. B 762 (2016) 162–165, arXiv:1605.08362 [hep-ph]
2016 arXiv
-
[27]
Two-loop Dirac neutrino mass and 24 WIMP dark matter,
C. Bonilla, E. Ma, E. Peinado, and J. W. F. Valle, “Two-loop Dirac neutrino mass and 24 WIMP dark matter,” Phys. Lett. B 762 (2016) 214–218, arXiv:1607.03931 [hep-ph]
2016 arXiv
-
[28]
Dark matter stability and Dirac neutrinos using only Standard Model symmetries,
C. Bonilla, S. Centelles-Chuli´ a, R. Cepedello, E. Peinado, and R. Srivastava, “Dark matter stability and Dirac neutrinos using only Standard Model symmetries,” Phys. Rev. D 101 no. 3, (2020) 033011, arXiv:1812.01599 [hep-ph]
2020 arXiv
-
[29]
Dark matter stability from Dirac neutrinos in scotogenic 3-3-1-1 theory,
J. Leite, A. Morales, J. W. F. Valle, and C. A. Vaquera-Araujo, “Dark matter stability from Dirac neutrinos in scotogenic 3-3-1-1 theory,” Phys. Rev. D 102 no. 1, (2020) 015022, arXiv:2005.03600 [hep-ph]
2020 arXiv
-
[30]
Scotogenic dark matter and Dirac neutrinos from unbroken gauged B −L symmetry,
J. Leite, A. Morales, J. W. F. Valle, and C. A. Vaquera-Araujo, “Scotogenic dark matter and Dirac neutrinos from unbroken gauged B −L symmetry,” Phys. Lett. B 807 (2020) 135537, arXiv:2003.02950 [hep-ph]
2020 arXiv
-
[31]
Comprehensive Phenomenology of the Dirac Scotogenic Model: Novel Low Mass Dark Matter,
S. Centelles Chuli´ a, R. Srivastava, and S. Yadav, “Comprehensive Phenomenology of the Dirac Scotogenic Model: Novel Low Mass Dark Matter,” arXiv:2409.18513 [hep-ph]
-
[32]
Revised experimental upper limit on the electric dipole moment of the neutron,
J. M. Pendlebury and et al, “Revised experimental upper limit on the electric dipole moment of the neutron,” Phys. Rev. D 92 (2015) 092003. https://link.aps.org/doi/10.1103/ PhysRevD.92.092003
2015
-
[33]
Improved experimental limit on the electric dipole moment of the neutron,
C. A. Baker and et al , “Improved experimental limit on the electric dipole moment of the neutron,” Phys. Rev. Lett. 97 (2006) 131801. https://link.aps.org/doi/10.1103/ PhysRevLett.97.131801
2006
-
[34]
CP conservation in the presence of pseudoparticles,
R. Peccei and H. Quinn, “CP conservation in the presence of pseudoparticles,” Phys. Rev. Lett. 38 (Jun, 1977) 1440–1443. https://link.aps.org/doi/10.1103/PhysRevLett.38. 1440
1977 doi
-
[35]
Constraints imposed by CP conservation in the presence of pseu- doparticles,
R. Peccei and H. Quinn, “Constraints imposed by CP conservation in the presence of pseu- doparticles,” Phys. Rev. D 16 (Sep, 1977) 1791–1797. https://link.aps.org/doi/10. 1103/PhysRevD.16.1791
1977
-
[36]
A new light boson?,
S. Weinberg, “A new light boson?,” Phys. Rev. Lett. 40 (1978) 223–226. https://link.aps. org/doi/10.1103/PhysRevLett.40.223
1978 doi
-
[37]
Problem of strong p and t invariance in the presence of instantons,
F. Wilczek, “Problem of strong p and t invariance in the presence of instantons,” Phys. Rev. Lett. 40 (1978) 279–282. https://link.aps.org/doi/10.1103/PhysRevLett.40.279
1978 doi
-
[38]
Weak Interaction Singlet and Strong CP Invariance,
J. E. Kim, “Weak Interaction Singlet and Strong CP Invariance,” Phys. Rev. Lett. 43 (1979) 103
1979
-
[39]
Can Confinement Ensure Natural CP Invariance of Strong Interactions?,
M. A. Shifman, A. I. Vainshtein, and V. I. Zakharov, “Can Confinement Ensure Natural CP Invariance of Strong Interactions?,” Nucl. Phys. B 166 (1980) 493–506
1980
-
[40]
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) 260
1980
-
[41]
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. B 104 (1981) 199–202
1981
-
[42]
Cosmology of the Invisible Axion,
J. Preskill, M. B. Wise, and F. Wilczek, “Cosmology of the Invisible Axion,” Phys. Lett. B 120 (1983) 127–132. 25
1983
-
[43]
A Cosmological Bound on the Invisible Axion,
L. F. Abbott and P. Sikivie, “A Cosmological Bound on the Invisible Axion,” Phys. Lett. B 120 (1983) 133–136
1983
-
[44]
The Not So Harmless Axion,
M. Dine and W. Fischler, “The Not So Harmless Axion,” Phys. Lett. B 120 (1983) 137–141
1983
-
[45]
Peccei-Quinn symmetry for Dirac seesaw and leptogenesis,
P.-H. Gu, “Peccei-Quinn symmetry for Dirac seesaw and leptogenesis,” JCAP 07 (2016) 004, arXiv:1603.05070 [hep-ph]
2016 arXiv
-
[46]
Dirac neutrinos from Peccei-Quinn symmetry: A fresh look at the axion,
E. Peinado, M. Reig, R. Srivastava, and J. W. F. Valle, “Dirac neutrinos from Peccei-Quinn symmetry: A fresh look at the axion,” Mod. Phys. Lett. A 35 no. 21, (2020) 2050176, arXiv:1910.02961 [hep-ph]
2020 arXiv
-
[47]
Reloading the axion in a 3-3-1 setup,
A. G. Dias, J. Leite, J. W. F. Valle, and C. A. Vaquera-Araujo, “Reloading the axion in a 3-3-1 setup,” Phys. Lett. B 810 (2020) 135829, arXiv:2008.10650 [hep-ph]
2020 arXiv
-
[48]
Dirac neutrinos from Peccei-Quinn symmetry: two examples,
L. M. G. de la Vega, N. Nath, and E. Peinado, “Dirac neutrinos from Peccei-Quinn symmetry: two examples,” Nucl. Phys. B 957 (2020) 115099, arXiv:2001.01846 [hep-ph]
2020 arXiv
-
[49]
S.M.A.S.H.E.D.: Standard Model Axion Seesaw Higgs inflation Extended for Dirac neutrinos,
M. Berbig, “S.M.A.S.H.E.D.: Standard Model Axion Seesaw Higgs inflation Extended for Dirac neutrinos,” JCAP 11 (2022) 042, arXiv:2207.08142 [hep-ph]
2022 arXiv
-
[50]
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. 132 no. 5, (2024) 051801, arXiv:2309.06473 [hep-ph]
2024 arXiv
-
[51]
Im- proved axion emissivity from a supernova via nucleon-nucleon bremsstrahlung,
P. Carenza, T. Fischer, M. Giannotti, G. Guo, G. Mart ´ ınez-Pinedo, and A. Mirizzi, “Im- proved axion emissivity from a supernova via nucleon-nucleon bremsstrahlung,” JCAP 10 no. 10, (2019) 016, arXiv:1906.11844 [hep-ph]. [Erratum: JCAP 05, E01 (2020)]
2019 arXiv
-
[52]
Effective description of quark mixing,
F. del Aguila, M. Perez-Victoria, and J. Santiago, “Effective description of quark mixing,” Phys. Lett. B 492 (2000) 98–106, arXiv:hep-ph/0007160
2000 arXiv
-
[53]
Observable contributions of new exotic quarks to quark mixing,
F. del Aguila, M. Perez-Victoria, and J. Santiago, “Observable contributions of new exotic quarks to quark mixing,” JHEP 09 (2000) 011, arXiv:hep-ph/0007316
2000 arXiv
-
[54]
Handbook of vectorlike quarks: Mixing and single production,
J. A. Aguilar-Saavedra, R. Benbrik, S. Heinemeyer, and M. P´ erez-Victoria, “Handbook of vectorlike quarks: Mixing and single production,” Phys. Rev. D 88 no. 9, (2013) 094010, arXiv:1306.0572 [hep-ph]
2013 arXiv
-
[55]
Redefining the Axion Window,
L. Di Luzio, F. Mescia, and E. Nardi, “Redefining the Axion Window,” Phys. Rev. Lett. 118 no. 3, (2017) 031801, arXiv:1610.07593 [hep-ph]
2017 arXiv
-
[56]
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. A 16 (2001) 2137–2164, arXiv:hep-ex/0102033
2001 arXiv
-
[57]
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
2009
-
[58]
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 massive particles,”Phys. Rept. 582 (2015) 1–52, arXiv:1410.1374 [hep-ph]
2015 arXiv
-
[59]
Astrophysical Constraints on Singlet Scalars at LHC,
M. P. Hertzberg and A. Masoumi, “Astrophysical Constraints on Singlet Scalars at LHC,” 26 JCAP 04 (2017) 028, arXiv:1607.06445 [hep-ph]
2017 arXiv
-
[60]
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. D 76 (2007) 043523, arXiv:0705.4298 [astro-ph]
2007 arXiv
-
[61]
Grand Unified Models With an Automatic Peccei-Quinn Symmetry,
H. M. Georgi, L. J. Hall, and M. B. Wise, “Grand Unified Models With an Automatic Peccei-Quinn Symmetry,” Nucl. Phys. B 192 (1981) 409–416
1981
-
[62]
String Theory and the Strong CP Problem,
M. Dine and N. Seiberg, “String Theory and the Strong CP Problem,” Nucl. Phys. B 273 (1986) 109–124
1986
-
[63]
Planck scale corrections to axion models,
S. M. Barr and D. Seckel, “Planck scale corrections to axion models,” Phys. Rev. D 46 (1992) 539–549
1992
-
[64]
Planck scale physics and the Peccei-Quinn mech- anism,
M. Kamionkowski and J. March-Russell, “Planck scale physics and the Peccei-Quinn mech- anism,” Phys. Lett. B 282 (1992) 137–141, arXiv:hep-th/9202003
1992 arXiv
-
[65]
Solutions to the strong CP problem in a world with gravity,
R. Holman, S. D. H. Hsu, T. W. Kephart, E. W. Kolb, R. Watkins, and L. M. Widrow, “Solutions to the strong CP problem in a world with gravity,” Phys. Lett. B 282 (1992) 132–136, arXiv:hep-ph/9203206
1992 arXiv
-
[66]
Instability of the invisible axion,
S. Ghigna, M. Lusignoli, and M. Roncadelli, “Instability of the invisible axion,” Phys. Lett. B 283 (1992) 278–281
1992
-
[67]
The KeV majoron as a dark matter particle,
V. Berezinsky and J. W. F. Valle, “The KeV majoron as a dark matter particle,” Phys. Lett. B 318 (1993) 360–366, arXiv:hep-ph/9309214
1993 arXiv
-
[68]
Discrete gauge symmetries in axionic extensions of the SSM,
E. J. Chun and A. Lukas, “Discrete gauge symmetries in axionic extensions of the SSM,” Phys. Lett. B 297 (1992) 298–304, arXiv:hep-ph/9209208
1992 arXiv
-
[69]
A Next-to-minimal supersymmetric model of hybrid infla- tion,
M. Bastero-Gil and S. F. King, “A Next-to-minimal supersymmetric model of hybrid infla- tion,” Phys. Lett. B 423 (1998) 27–34, arXiv:hep-ph/9709502
1998 arXiv
-
[70]
Stabilizing the axion by discrete gauge symmetries,
K. S. Babu, I. Gogoladze, and K. Wang, “Stabilizing the axion by discrete gauge symmetries,” Phys. Lett. B 560 (2003) 214–222, arXiv:hep-ph/0212339
2003 arXiv
-
[71]
Naturally light invisible axion and local Z(13) x Z(3) symmetries,
A. G. Dias, V. Pleitez, and M. D. Tonasse, “Naturally light invisible axion and local Z(13) x Z(3) symmetries,” Phys. Rev. D 69 (2004) 015007, arXiv:hep-ph/0210172
2004 arXiv
-
[72]
Peccei-Quinn symmetry from a gauged discrete R symmetry,
K. Harigaya, M. Ibe, K. Schmitz, and T. T. Yanagida, “Peccei-Quinn symmetry from a gauged discrete R symmetry,” Phys. Rev. D 88 no. 7, (2013) 075022, arXiv:1308.1227 [hep-ph]
2013 arXiv
-
[73]
A ”gauged
H. Fukuda, M. Ibe, M. Suzuki, and T. T. Yanagida, “A ”gauged” U (1) Peccei–Quinn sym- metry,” Phys. Lett. B 771 (2017) 327–331, arXiv:1703.01112 [hep-ph]
2017 arXiv
-
[74]
Protecting the Axion with Local Baryon Number,
M. Duerr, K. Schmidt-Hoberg, and J. Unwin, “Protecting the Axion with Local Baryon Number,” Phys. Lett. B 780 (2018) 553–556, arXiv:1712.01841 [hep-ph]
2018 arXiv
-
[75]
Axions in a highly protected gauge symmetry model,
Q. Bonnefoy, E. Dudas, and S. Pokorski, “Axions in a highly protected gauge symmetry model,” Eur. Phys. J. C 79 no. 1, (2019) 31, arXiv:1804.01112 [hep-ph]
2019 arXiv
-
[76]
Composite axion models and Planck scale physics,
L. Randall, “Composite axion models and Planck scale physics,” Phys. Lett. B 284 (1992) 77–80. 27
1992
-
[77]
Accidental Peccei-Quinn symmetry protected to arbitrary order,
L. Di Luzio, E. Nardi, and L. Ubaldi, “Accidental Peccei-Quinn symmetry protected to arbitrary order,” Phys. Rev. Lett. 119 no. 1, (2017) 011801, arXiv:1704.01122 [hep-ph]
2017 arXiv
-
[78]
A High Quality Composite Axion,
B. Lillard and T. M. P. Tait, “A High Quality Composite Axion,” JHEP 11 (2018) 199, arXiv:1811.03089 [hep-ph]
2018 arXiv
-
[79]
Peccei-Quinn symmetry from a hidden gauge group structure,
H.-S. Lee and W. Yin, “Peccei-Quinn symmetry from a hidden gauge group structure,” Phys. Rev. D 99 no. 1, (2019) 015041, arXiv:1811.04039 [hep-ph]
2019 arXiv
-
[80]
The QCD axion, precisely,
G. Grilli di Cortona, E. Hardy, J. Pardo Vega, and G. Villadoro, “The QCD axion, precisely,” JHEP 01 (2016) 034, arXiv:1511.02867 [hep-ph]
2016 arXiv
-
[81]
Naturalness, chiral symmetry, and spontaneous chiral symmetry breaking,
G. ’t Hooft, “Naturalness, chiral symmetry, and spontaneous chiral symmetry breaking,” NATO Sci. Ser. B 59 (1980) 135–157
1980
-
[82]
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]
2020 arXiv
-
[83]
Planck 2018 results. VI. Cosmological param- eters,
Planck Collaboration, N. Aghanim et al. , “Planck 2018 results. VI. Cosmological param- eters,” Astron. Astrophys. 641 (2020) A6, arXiv:1807.06209 [astro-ph.CO]. [Erratum: Astron.Astrophys. 652, C4 (2021)]
2020 arXiv
-
[84]
Evidence for a Scaling Solution in Cosmic String Evolu- tion,
D. P. Bennett and F. R. Bouchet, “Evidence for a Scaling Solution in Cosmic String Evolu- tion,” Phys. Rev. Lett. 60 (1988) 257
1988
-
[85]
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. 121 no. 15, (2018) 151301, arXiv:1804.05857 [astro-ph.CO]
2018 arXiv
-
[86]
Axions from Strings: the Attractive Solution,
M. Gorghetto, E. Hardy, and G. Villadoro, “Axions from Strings: the Attractive Solution,” JHEP 07 (2018) 151, arXiv:1806.04677 [hep-ph]
2018 arXiv
-
[87]
Early-Universe Simulations of the Cosmologi- cal Axion,
M. Buschmann, J. W. Foster, and B. R. Safdi, “Early-Universe Simulations of the Cosmologi- cal Axion,” Phys. Rev. Lett. 124 no. 16, (2020) 161103, arXiv:1906.00967 [astro-ph.CO]
2020 arXiv
-
[88]
Spontaneous Breaking of Lepton Number and the 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. 122 no. 15, (2019) 151301, arXiv:1806.11198 [hep-ph]
2019 arXiv
-
[89]
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. 13 no. 1, (2022) 1049, arXiv:2108.05368 [hep-ph]
2022 arXiv
-
[90]
More axions from strings,
M. Gorghetto, E. Hardy, and G. Villadoro, “More axions from strings,” SciPost Phys. 10 no. 2, (2021) 050, arXiv:2007.04990 [hep-ph]
2021 arXiv
-
[91]
The dark-matter axion mass,
V. B. . Klaer and G. D. Moore, “The dark-matter axion mass,” JCAP 11 (2017) 049, arXiv:1708.07521 [hep-ph]
2017 arXiv
-
[92]
Axion dark matter from topological defects,
M. Kawasaki, K. Saikawa, and T. Sekiguchi, “Axion dark matter from topological defects,” Phys. Rev. D 91 no. 6, (2015) 065014, arXiv:1412.0789 [hep-ph]
2015 arXiv
-
[93]
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. 28
1982
-
[94]
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. 97 no. 1, (2025) 015001, arXiv:2401.04388 [hep-ph]
2025 arXiv
-
[95]
Constraining postinflationary axions with pulsar timing arrays,
G. Servant and P. Simakachorn, “Constraining postinflationary axions with pulsar timing arrays,” Phys. Rev. D 108 no. 12, (2023) 123516, arXiv:2307.03121 [hep-ph]
2023 arXiv
-
[96]
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. D 110 no. 3, (2024) 035008, arXiv:2305.03776 [hep-ph]
2024 arXiv
-
[97]
Axion Dark Matter,
C. B. Adams et al. , “Axion Dark Matter,” in Snowmass 2021 . 3, 2022. arXiv:2203.14923 [hep-ex]
2021 arXiv
-
[98]
cajohare/axionlimits: Axionlimits
C. O’Hare, “cajohare/axionlimits: Axionlimits.” https://cajohare.github.io/ AxionLimits/, July, 2020
2020
-
[99]
Quark Flavor Phenomenology of the QCD Axion,
J. Martin Camalich, M. Pospelov, P. N. H. Vuong, R. Ziegler, and J. Zupan, “Quark Flavor Phenomenology of the QCD Axion,” Phys. Rev. D 102 no. 1, (2020) 015023, arXiv:2002.04623 [hep-ph]
2020 arXiv
-
[100]
The flavor of QCD axion dark matter,
G. Alonso- ´Alvarez, J. M. Cline, and T. Xiao, “The flavor of QCD axion dark matter,” JHEP 07 (2023) 187, arXiv:2305.00018 [hep-ph]
2023 arXiv
-
[101]
New CAST Limit on the Axion-Photon Interaction,
CAST Collaboration, V. Anastassopoulos et al. , “New CAST Limit on the Axion-Photon Interaction,” Nature Phys. 13 (2017) 584–590, arXiv:1705.02290 [hep-ex]
2017 arXiv
-
[102]
A Search for Invisible Axion Dark Matter with the Axion Dark Matter Experiment,
ADMX Collaboration, N. Du et al. , “A Search for Invisible Axion Dark Matter with the Axion Dark Matter Experiment,” Phys. Rev. Lett. 120 no. 15, (2018) 151301, arXiv:1804.05750 [hep-ex]
2018 arXiv
-
[103]
Extended Search for the Invisible Axion with the Axion Dark Matter Experiment,
ADMX Collaboration, T. Braine et al. , “Extended Search for the Invisible Axion with the Axion Dark Matter Experiment,” Phys. Rev. Lett. 124 no. 10, (2020) 101303, arXiv:1910.08638 [hep-ex]
2020 arXiv
-
[104]
Search for Invisible Axion Dark Matter in the 3.3–4.2 µeV Mass Range,
ADMX Collaboration, C. Bartram et al. , “Search for Invisible Axion Dark Matter in the 3.3–4.2 µeV Mass Range,” Phys. Rev. Lett. 127 no. 26, (2021) 261803, arXiv:2110.06096 [hep-ex]
2021 arXiv
-
[105]
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. Wuen- sch, 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
1987
-
[106]
First Results from an Axion Haloscope at CAPP around 10.7 µeV,
CAPP Collaboration, O. Kwon et al. , “First Results from an Axion Haloscope at CAPP around 10.7 µeV,” Phys. Rev. Lett. 126 no. 19, (2021) 191802, arXiv:2012.10764 [hep-ex]
2021 arXiv
-
[107]
A quantum-enhanced search for dark matter axions,
HA YST ACCollaboration, K. M. Backes et al. , “A quantum-enhanced search for dark matter axions,” Nature 590 no. 7845, (2021) 238–242, arXiv:2008.01853 [quant-ph]
2021 arXiv
-
[108]
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 Trans- 29 actions on Applied Superconductivity 23 no. 3, (2013) 4500604–4500604. https://doi.org/ 10.1109%2...
2013
-
[109]
ADMX Status,
I. Stern, “ADMX Status,” PoS ICHEP2016 (2016) 198, arXiv:1612.08296 [physics.ins-det]
2016 arXiv
-
[110]
MADMAX Status Report,
S. Beurthey et al. , “MADMAX Status Report,” arXiv:2003.10894 [physics.ins-det]
2003 arXiv
-
[111]
First Results from ABRACADABRA-10 cm: A Search for Sub- µeV Ax- ion Dark Matter,
J. L. Ouellet et al., “First Results from ABRACADABRA-10 cm: A Search for Sub- µeV Ax- ion Dark Matter,” Phys. Rev. Lett. 122 no. 12, (2019) 121802, arXiv:1810.12257 [hep-ex]
2019 arXiv
-
[112]
Searching for dark matter with plasma halo- scopes,
ALPHA Collaboration, A. J. Millar et al. , “Searching for dark matter with plasma halo- scopes,” Phys. Rev. D 107 no. 5, (2023) 055013, arXiv:2210.00017 [hep-ph]
2023 arXiv
-
[113]
Tunable axion plasma haloscopes,
M. Lawson, A. J. Millar, M. Pancaldi, E. Vitagliano, and F. Wilczek, “Tunable axion plasma haloscopes,” Phys. Rev. Lett. 123 no. 14, (2019) 141802, arXiv:1904.11872 [hep-ph]
2019 arXiv
-
[114]
Exploration of Wire Array Metamaterials for the Plasma Axion Haloscope,
M. Wooten, A. Droster, A. Kenany, D. Sun, S. M. Lewis, and K. van Bibber, “Exploration of Wire Array Metamaterials for the Plasma Axion Haloscope,” Annalen Phys. 536 no. 1, (2024) 2200479, arXiv:2203.13945 [hep-ex]
2024 arXiv
-
[115]
Neutrino Decay and Spontaneous Violation of Lepton Number,
J. Schechter and J. W. F. Valle, “Neutrino Decay and Spontaneous Violation of Lepton Number,” Phys. Rev. D 25 (1982) 774
1982
-
[116]
The QCD axion, colour-mediated neutrino masses, and B+ → K+ + Emiss anomaly,
C. Hati et al. , “The QCD axion, colour-mediated neutrino masses, and B+ → K+ + Emiss anomaly,” arXiv:2408.00060 [hep-ph]
Reviewed August 10, 2026 · model on record in the stance chip above.
Discussion (0). Continue with ORCID to comment.