REVIEW 3 major objections 4 minor 93 references
Archimedean Seesaw: Small Neutrino Masses and Large Lepton-number Violation
T0 review · 3 major / 4 minor · reviewed 2026-08-14 · deepseek-v4-flash
Pith's one-line read A texture-zero seesaw can cancel the active neutrino mass exactly while lepton-number violation in the heavy sector stays large, and small perturbations make the neutrino mass naturally small without reinstating the usual suppression.
desk verdict The tree-level cancelation is real and the paper is worth refereeing, but the 'arbitrarily large LNV' claim is only established at tree level because the accidental symmetry is not a symmetry of the Lagrangian. 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 mechanism is the texture-zero Archimedean seesaw: a $3\times3$ neutrino mass matrix whose first two rows are linearly dependent, so that one active eigenstate is exactly massless. The load-bearing object is the accidental $U(1)_{\rm acc}$ symmetry generated by the projector $T=|\nu\rangle\langle\nu|$; it leaves the renormalizable mass matrix invariant for all heavy-sector parameters and makes the zero mode exact rather than fine-tuned. Higher-dimensional operators that respect the underlying $U(1)_X$ symmetry but break $U(1)_{\rm acc}$ provide the leading perturbation $\Delta M$, and the active neutrino mass is simply $\langle\nu|\Delta M|\nu\rangle=\mathrm{Tr}(T\Delta M)$, naturally small and independent of $M_{22}$. The paper also gives a lever-arm picture: the relation $m_\nu V_{\ell\nu}^2+M_1 V_{\ell N_1}^2+M_2 V_{\ell N_2}^2=0$ is an Archimedean balance condition, with the heavy masses acting as counterweights that allow large active-sterile mixing without a large neutrino mass.
What would settle it
Compute the three-flavor generalization: if any light neutrino mass acquires a term proportional to $M_{22}$, or if the exact massless mode cannot be maintained while fitting oscillation data, the central decoupling claim collapses. An experimental falsifier would be a precise measurement of same-sign dilepton production that returns $|V_{\ell N}|^2 M_N \simeq m_\nu$ in a parameter region where the Archimedean model predicts a much larger value.
Extended reading notes
Core claim
The central claim is that the light neutrino mass in a seesaw can be made independent of the heavy Majorana mass that controls lepton-number violation. With the texture-zero choice $m_1=0$ and $M_{11}=0$ for $Y=(0,y_2)$ and $M=(M_{ij})$, the $3\times3$ neutrino mass matrix has an exact zero eigenvalue for arbitrarily large $M_{12}$ and $M_{22}$; the eigenvector $|\nu\rangle=(M_{12},-m_2,0)/\rho$ with $\rho^2=m_2^2+M_{12}^2$ defines a projector $T=|\nu\rangle\langle\nu|$, and $U(\alpha)=e^{i\alpha T}$ is an accidental $U(1)$ symmetry of the renormalizable mass matrix. Lifting the texture zeros by small perturbations $\mu_1,\mu_2$ gives $m_\nu=-2\mu_1 m_2 M_{12}/\rho^2+\mu_2 m_2^2/\rho^2=\mathrm{Tr}(T\Delta M)$, an expression in which $M_{22}$ does not appear. The induced mass is naturally small because the breaking first appears through higher-dimensional operators suppressed by $\langle\phi\rangle/\Lambda$, and the two heavy eigenstates need not form a Dirac pair, so heavy-sector lepton-number violation remains unsuppressed.
Load-bearing premise
The load-bearing premise is that the realistic three-generation version needed to fit neutrino oscillations keeps the same protective structure, so the heavy mass that controls lepton-number violation stays out of the light neutrino mass formula; the paper shows this only for one active flavor.
Editorial extensions
If this is right
- If the central claim is right, $|V_{\ell N}|^2 M_N=m_\nu$ is not a universal seesaw constraint, and heavy neutral lepton searches no longer need to be pre-scaled by the tiny neutrino mass.
- The model maps the observable $(M_N,|V_{\mu N}|^2)$ plane directly onto the heavy-sector scale $M_2$, so current and future exclusions become bounds on $M_2$.
- Same-sign dilepton signatures, both vector-boson fusion and resonant Drell-Yan $q\bar q\to W\to \ell N_i$, become viable discovery channels at the LHC and future colliders for HNL masses from MeV to TeV.
- In the limit $M_{22}\to0$ the two heavy states form an approximate Dirac pair and lepton-number violation is partially cancelled, recovering the inverse seesaw; the new physics is the asymmetric regime where this cancellation is absent.
Reading between the lines
- The paper proves the decoupling for a single active flavor; a natural next test is whether a three-flavor texture can protect all three light neutrinos while fitting solar and atmospheric oscillations, a check not carried out here.
- Because the neutrino mass is proportional to $\mu_1,\mu_2$, generating these parameters radiatively at one loop would make their smallness fully natural without needing a very large $\Lambda$; the paper does not explore this origin.
- An anomaly-free gauging of $U(1)_X$ would introduce a $Z'$ coupled to the singlet sector, giving an additional search channel through heavy neutral lepton pair production that is not discussed in the paper.
Editorial analysis
A structured set of objections, weighed in public.
Referee Report
Summary. The paper proposes a seesaw variant, the "Archimedean seesaw," in which a texture-zero mass matrix for one active and two sterile neutrinos has an exact massless eigenstate even when the heavy Majorana sector violates lepton number by a large amount. Small neutrino masses are then generated by small texture-lifting parameters (mu1, mu2), and the paper claims that the heavy Majorana mass M22 that controls LNV does not enter the light-neutrino mass, thereby evading the conventional seesaw relation U^2 M_N ~ m_nu. The authors present a U(1)_X extension intended to justify the texture zeros, give tree-level formulas for the masses and mixings, and map the model onto experimental HNL searches. The tree-level matrix algebra in Eqs. (8)-(13) is correct, but the paper's broader claims of a natural, symmetry-protected mechanism are not established.
Significance. If the core claim were correct, it would open a qualitatively new avenue for low-scale seesaw phenomenology: heavy neutral leptons with sizeable active-sterile mixing and observable LNV could coexist with sub-eV neutrino masses, in contrast to the standard Type-I seesaw relation. The paper also gives a clear EFT interpretation of the texture-lifting, and the phenomenological projections are concrete and useful. However, the significance is currently conditional: the explicit U(1)_X realization is internally inconsistent, the accidental symmetry used for technical naturalness is not a symmetry of the full Lagrangian, and the three-generation extension is not provided. The tree-level one-flavor result is a valid mathematical observation, but it does not by itself support the advertised class of realistic models.
major comments (3)
- [TEXTURE ZEROS FROM AN EXTRA U(1)_X SYMMETRY (Eqs. (15)-(16) and charge table)] The U(1)_X assignments are internally inconsistent under the standard convention that the charge conjugate N_i^c has charge -q_i. With the stated charges q(L)=0, q(N1)=1, q(N2)=0, q(H)=0, q(phi)=-1, the term lambda phi N_1^c N_2 has total charge -2 and the term beta phi^2 N_1^c N_1 has total charge -2, so neither is invariant; only the alpha term is allowed. This invalidates the claim that Eqs. (15)-(16) are the complete set of U(1)_X-invariant operators. More generally, invariance of the beta operator forces q(phi)=0, which together with invariance of the lambda operator forces q1=q2, and then the renormalizable M11 term is allowed, destroying the texture zero. The advertised symmetry protection of the texture-zero structure is therefore not realized by the explicit model.
- [End Matter, Eqs. (21)-(25) and main text after Eq. (13)] The accidental symmetry U(1)_acc is only a symmetry of the tree-level mass matrix M0, not of the full Lagrangian. The transformation U(alpha)=exp(i alpha T) mixes nu_L, an SU(2) doublet with U(1)_X charge 0, with N_1, an SU(2) singlet with U(1)_X charge 1, so it does not commute with the gauge-covariant kinetic terms. Consequently, the statement that this symmetry 'assures the zero neutrino mass technically natural' is unsupported. Since the Weinberg operator (LH)(LH) is neutral under U(1)_X, radiative corrections will generically generate the (1,1) entry of the neutrino mass matrix even when mu1=mu2=0, re-introducing M22 into m_nu. The paper does not compute any loop correction, so Eq. (13) and the central conclusion that 'arbitrarily large LNV can coexist with sub-eV neutrino masses' are established only at tree level.
- [Footnote 1 and the phenomenology section] The proof of the mechanism is carried out for a single active flavor, and the realistic extension to three generations is deferred to a forthcoming paper. The observed neutrino spectrum requires at least two non-zero masses and a specific flavor mixing pattern, and it is not demonstrated that the texture-zero protection survives the required flavor structure. The Supplemental Material's assertion that the mechanism is 'flavor independent' is not backed by a construction. Without an explicit three-generation model, the abstract's claim of a 'class of seesaw models' that realizes sub-eV neutrino masses with sizeable LNV is not supported.
minor comments (4)
- [Section 'ACCIDENTALLY VANISHING NEUTRINO MASSES', after Eq. (6)] The phrase 'without loss of generality' is misleading: the choice m1=0, M11=0 is one particular solution of Eq. (6), not the general solution. The paper is free to adopt this ansatz, but the wording overstates its generality.
- [Eq. (13) and the discussion following it] The sign of m_nu is not fixed; a Majorana mass eigenvalue can be negative, but the paper should refer to |m_nu| when comparing to sub-eV bounds and to experimental constraints.
- [Charge table in 'TEXTURE ZEROS FROM AN EXTRA U(1)_X SYMMETRY'] The charges of the conjugate fields N_i^c are not listed in the table. Given that the mass terms involve N_i^c, this omission contributes to the inconsistency discussed above and should be clarified.
- [Figure captions (Figs. 3 and 4)] The captions refer to 'colored diagonal lines' and shaded regions, but the actual figures are not included in the manuscript text. The captions should be self-contained enough for a reader to interpret the constraints independently.
Circularity Check
Tree-level mass derivation is self-contained, but the claimed U(1)_acc protection of the zero neutrino mass is self-definitional: the symmetry is constructed from the zero-mode projector it is invoked to protect.
-
self definitional
[Supplemental Material, 'Accidental symmetry of the texture-zero solution', Eqs. (21)-(25); main text Section 'Texture zeros from an extra U(1)_X symmetry'.]
"The renormalizable neutrino mass matrix in Eq. (8) possesses an exact massless eigenstate satisfying M0|ν⟩=0, with normalized eigenvector |ν⟩=1/ρ(M12,−m2,0)... We define the projector onto the exact zero mode, T≡|ν⟩⟨ν|... The transformation U(α)≡e^{iαT}=1+(e^{iα}−1)T leaves the neutrino mass matrix invariant for all α... Therefore, the renormalizable neutrino mass matrix possesses an accidental global U(1) symmetry acting on the exact massless eigenstate, U(1)_acc: |ν⟩ → e^{iα}|ν⟩."
The 'accidental' U(1)_acc is not an independently motivated symmetry of the Lagrangian; it is defined by T=|ν⟩⟨ν|, the projector onto the very massless eigenstate it is invoked to protect, and its invariance property U^T M0 U = M0 is algebraically equivalent to M0|ν⟩=0 (using T M0 = M0 T = 0). Saying that this symmetry 'assures the zero neutrino mass technically natural' is therefore a restatement of the zero-mode condition, not evidence that radiative corrections vanish. The paper never verifies that U(α) preserves the gauge-covariant kinetic terms or commutes with U(1)_X; since ν_L and N_1 carry different quantum numbers, U mixes fields in a way that is not a symmetry of the full renormalizable action. The tree-level result Eq.
full rationale
The central mass formula Eq. (13) is a straightforward consequence of the explicitly assumed texture-zero structure and the small perturbation matrix ΔM; no parameters are fitted to neutrino data, and the decoupling of M22 from mν is a designed feature of the operator content, not a fitted result. The phenomenology sections recast existing experimental limits rather than deriving predictions from fitted quantities. The paper's self-citations (e.g., refs. [22], [40], [81]) are background references and are not load-bearing for the central mechanism. The one genuine circular element is the technical-naturalness claim: the U(1)_acc symmetry is built entirely from the massless eigenvector it is said to protect, and its invariance of the mass matrix is a tautological consequence of M0|ν⟩=0. Because the paper uses this symmetry to argue that the zero mode is protected against radiative corrections, without demonstrating that U(1)_acc is a symmetry of the full renormalizable Lagrangian (including kinetic and gauge terms), that explanatory step is self-definitional. This does not invalidate the tree-level 'Archimedean seesaw' decoupling, so the overall circularity is mild.
Assumptions & free parameters
free parameters (5)
- y2 =
benchmark 0.1, also 1e-2 and 1e-5
- M22 =
benchmark 1e4 to 1e12 GeV in Fig. 4
- M12
- mu1, mu2 =
not numerically fit
- epsilon = <phi>/Lambda
assumptions (4)
- domain assumption Type-I seesaw with two right-handed neutrinos and SM gauge content
- domain assumption One-lepton-generation simplification
- ad hoc to paper U(1)_X charge assignments and the operator selection in Eqs. (15)-(16)
- ad hoc to paper Higher-dimensional operators are the leading breaking of U(1)_acc and are controlled by one scale Lambda
invented entities (3)
-
Global U(1)_X symmetry
-
Singlet scalar phi
-
Accidental U(1)_acc symmetry
Cite this review
Pith. "Pith review of Archimedean Seesaw: Small Neutrino Masses and Large Lepton-number Violation." pith.science (2026). https://pith.science/paper/HBVYYEW3
@misc{pith2026260810062,
author = {Pith},
title = {Pith review of: Archimedean Seesaw: Small Neutrino Masses and Large Lepton-number Violation},
year = {2026},
howpublished = {\url{https://pith.science/paper/HBVYYEW3}},
note = {Machine review of arXiv:2608.10062}
}
read the original abstract
Contrary to the common lore that observable lepton-number violation (LNV) is inevitably suppressed by tiny neutrino masses, we identify a class of seesaw models in which arbitrarily large LNV can naturally coexist with sub-eV neutrino masses. We construct a symmetry-protected texture-zero structure in the neutrino Yukawa couplings and heavy Majorana mass matrix that gives rise to the required accidental symmetry, thereby protecting the light neutrinos from acquiring mass even in the presence of arbitrarily large LNV in the heavy sector. Small neutrino masses arise naturally from lifting the texture-zero structure while preserving the underlying symmetry. The resulting framework offers a rich and experimentally accessible phenomenology, predicting Heavy Neutral Leptons with sizeable active-sterile mixing over a broad range of experimentally accessible masses, giving rise to observable LNV signatures at collider and intensity-frontier experiments.
Figures
Reference graph
Works this paper leans on
-
[24]
S. Antusch and O. Fischer, Testing sterile neutrino ex- tensions of the Standard Model at future lepton colliders, JHEP05, 053, arXiv:1502.05915 [hep-ph]
-
[1]
Weinberg, Baryon and Lepton Nonconserving Pro- cesses, Phys
S. Weinberg, Baryon and Lepton Nonconserving Pro- cesses, Phys. Rev. Lett.43, 1566 (1979)
1979
-
[2]
counterweight
In the limitM≫m, the effective light neutrino mass is mν ≃ −m M−1 mT .(5) The requirement that the neutrino mass matrix Eq. (5) vanishes implies: m2 1M22 −2m 1m2M12 +m 2 2M11 = 0.(6) Notably, the choicem 1 = 0,M 11 = 0 solves this equation. Thus, without loss of generality, we take the matrices as Y= 0y 2 , M= 0M 12 M12 M22 ,(7) that leads to vanishing ne...
-
[3]
Minkowski,µ→eγat a Rate of One Out of 10 9 Muon Decays?, Phys
P. Minkowski,µ→eγat a Rate of One Out of 10 9 Muon Decays?, Phys. Lett. B67, 421 (1977)
1977
-
[4]
M. Gell-Mann, P. Ramond, and R. Slansky, Complex Spinors and Unified Theories, Conf. Proc. C790927, 315 (1979), arXiv:1306.4669 [hep-th]
arXiv 1979
-
[5]
Yanagida, Horizontal gauge symmetry and masses of neutrinos, Conf
T. Yanagida, Horizontal gauge symmetry and masses of neutrinos, Conf. Proc. C7902131, 95 (1979)
1979
-
[6]
R. N. Mohapatra and G. Senjanovic, Neutrino Mass and Spontaneous Parity Nonconservation, Phys. Rev. Lett. 44, 912 (1980)
1980
-
[7]
R. N. Mohapatra, Mechanism for Understanding Small Neutrino Mass in Superstring Theories, Phys. Rev. Lett. 56, 561 (1986)
1986
Show all 93 references
-
[8]
R. N. Mohapatra and J. W. F. Valle, Neutrino Mass and Baryon Number Nonconservation in Superstring Models, Phys. Rev. D34, 1642 (1986)
1986
-
[9]
E. K. Akhmedov, M. Lindner, E. Schnapka, and J. W. F. Valle, Left-right symmetry breaking in NJL approach, Phys. Lett. B368, 270 (1996), arXiv:hep-ph/9507275
1996 arXiv
-
[10]
Malinsky, J
M. Malinsky, J. C. Romao, and J. W. F. Valle, Novel supersymmetric SO(10) seesaw mechanism, Phys. Rev. Lett.95, 161801 (2005), arXiv:hep-ph/0506296
2005 arXiv
-
[11]
S. L. Glashow, The Future of Elementary Particle Physics, NATO Sci. Ser. B61, 687 (1980)
1980
-
[12]
Konetschny and W
W. Konetschny and W. Kummer, Nonconservation of To- tal Lepton Number with Scalar Bosons, Phys. Lett. B70, 433 (1977)
1977
-
[13]
Magg and C
M. Magg and C. Wetterich, Neutrino Mass Problem and Gauge Hierarchy, Phys. Lett. B94, 61 (1980)
1980
-
[14]
Lazarides, Q
G. Lazarides, Q. Shafi, and C. Wetterich, Proton Lifetime and Fermion Masses in an SO(10) Model, Nucl. Phys. B 181, 287 (1981)
1981
-
[15]
Schechter and J
J. Schechter and J. W. F. Valle, Neutrino Masses in SU(2) x U(1) Theories, Phys. Rev. D22, 2227 (1980)
1980
-
[16]
T. P. Cheng and L.-F. Li, Neutrino Masses, Mixings and Oscillations in SU(2) x U(1) Models of Electroweak In- teractions, Phys. Rev. D22, 2860 (1980)
1980
-
[17]
S. M. Bilenky, J. Hosek, and S. T. Petcov, On Oscil- lations of Neutrinos with Dirac and Majorana Masses, Phys. Lett. B94, 495 (1980)
1980
-
[18]
Wyler and L
D. Wyler and L. Wolfenstein, Massless Neutrinos in Left- Right Symmetric Models, Nucl. Phys. B218, 205 (1983)
1983
-
[19]
R. N. Mohapatra et al., Theory of Neutrinos: A White Paper, Rept. Prog. Phys.70, 1757 (2007), arXiv:hep- ph/0510213
2007
-
[20]
Shaposhnikov, A Possible symmetry of the nuMSM, Nucl
M. Shaposhnikov, A Possible symmetry of the nuMSM, Nucl. Phys. B763, 49 (2007), arXiv:hep-ph/0605047
2007 arXiv
-
[21]
Kersten and A
J. Kersten and A. Y. Smirnov, Right-Handed Neutrinos at CERN LHC and the Mechanism of Neutrino Mass Gen- eration, Phys. Rev. D76, 073005 (2007), arXiv:0705.3221 [hep-ph]
2007 arXiv
-
[22]
M. B. Gavela, T. Hambye, D. Hernandez, and P. Her- nandez, Minimal Flavour Seesaw Models, JHEP09, 038, arXiv:0906.1461 [hep-ph]
-
[23]
Ibarra, E
A. Ibarra, E. Molinaro, and S. T. Petcov, TeV Scale See- Saw Mechanisms of Neutrino Mass Generation, the Majo- rana Nature of the Heavy Singlet Neutrinos and (ββ) 0ν - Decay, JHEP09, 108, arXiv:1007.2378 [hep-ph]
-
[25]
Moffat, S
K. Moffat, S. Pascoli, and C. Weiland, Equivalence be- tween massless neutrinos and lepton number conserva- tion in fermionic singlet extensions of the Standard Model 7 (2017), arXiv:1712.07611 [hep-ph]
2017 arXiv
-
[26]
Blennow, E
M. Blennow, E. Fernandez-Martinez, J. Lopez-Pavon, and J. Menendez, Neutrinoless double beta decay in see- saw models, JHEP07, 096, arXiv:1005.3240 [hep-ph]
-
[27]
Mitra, G
M. Mitra, G. Senjanovic, and F. Vissani, Neutrinoless Double Beta Decay and Heavy Sterile Neutrinos, Nucl. Phys. B856, 26 (2012), arXiv:1108.0004 [hep-ph]
2012 arXiv
-
[28]
A. Atre, T. Han, S. Pascoli, and B. Zhang, The Search for Heavy Majorana Neutrinos, JHEP05, 030, arXiv:0901.3589 [hep-ph]
-
[29]
Aad et al
G. Aad et al. (ATLAS), Search for Majorana neutri- nos in same-sign WW scattering events from pp colli- sions at √s= 13 TeV, Eur. Phys. J. C83, 824 (2023), arXiv:2305.14931 [hep-ex]
2023 arXiv
-
[30]
Aad et al
G. Aad et al. (ATLAS), Search for heavy Majorana neu- trinos in e±e±and e±µ±final states via WW scattering in pp collisions at s=13 TeV with the ATLAS detector, Phys. Lett. B856, 138865 (2024), arXiv:2403.15016 [hep- ex]
2024 arXiv
-
[31]
Aad et al
G. Aad et al. (ATLAS), Search for heavy neutral leptons in decays of W bosons produced in 13 TeVppcollisions us- ing prompt signatures in the ATLAS detector, Eur. Phys. J. C86, 153 (2026), arXiv:2508.20929 [hep-ex]
2026 arXiv
-
[32]
del Aguila, J
F. del Aguila, J. de Blas, and M. Perez-Victoria, Effects of new leptons in Electroweak Precision Data, Phys. Rev. D78, 013010 (2008), arXiv:0803.4008 [hep-ph]
2008 arXiv
-
[33]
Akhmedov, A
E. Akhmedov, A. Kartavtsev, M. Lindner, L. Michaels, and J. Smirnov, Improving Electro-Weak Fits with TeV- scale Sterile Neutrinos, JHEP05, 081, arXiv:1302.1872 [hep-ph]
-
[34]
de Blas, Electroweak limits on physics beyond the Standard Model, EPJ Web Conf.60, 19008 (2013), arXiv:1307.6173 [hep-ph]
J. de Blas, Electroweak limits on physics beyond the Standard Model, EPJ Web Conf.60, 19008 (2013), arXiv:1307.6173 [hep-ph]
2013 arXiv
-
[35]
Basso, O
L. Basso, O. Fischer, and J. J. van der Bij, Precision tests of unitarity in leptonic mixing, EPL105, 11001 (2014), arXiv:1310.2057 [hep-ph]
2014 arXiv
-
[36]
Antusch and O
S. Antusch and O. Fischer, Non-unitarity of the leptonic mixing matrix: Present bounds and future sensitivities, JHEP10, 094, arXiv:1407.6607 [hep-ph]
-
[37]
Chrzaszcz, M
M. Chrzaszcz, M. Drewes, T. E. Gonzalo, J. Harz, S. Kr- ishnamurthy, and C. Weniger, A frequentist analysis of three right-handed neutrinos with GAMBIT, Eur. Phys. J. C80, 569 (2020), arXiv:1908.02302 [hep-ph]
2020 arXiv
-
[38]
Bryman, V
D. Bryman, V. Cirigliano, A. Crivellin, and G. Inguglia, Testing Lepton Flavor Universality with Pion, Kaon, Tau, and Beta Decays, Ann. Rev. Nucl. Part. Sci.72, 69 (2022), arXiv:2111.05338 [hep-ph]
2022 arXiv
-
[39]
Blennow, E
M. Blennow, E. Fern´ andez-Mart ´ ınez, J. Hern´ andez- Garc ´ ıa, J. L´ opez-Pav´ on, X. Marcano, and D. Naredo- Tuero, Bounds on lepton non-unitarity and heavy neu- trino mixing, JHEP08, 030, arXiv:2306.01040 [hep-ph]
-
[40]
Keung and G
W.-Y. Keung and G. Senjanovic, Majorana Neutrinos and the Production of the Right-handed Charged Gauge Bo- son, Phys. Rev. Lett.50, 1427 (1983)
1983
-
[41]
Ilakovac and A
A. Ilakovac and A. Pilaftsis, Flavor violating charged lep- ton decays in seesaw-type models, Nucl. Phys. B437, 491 (1995), arXiv:hep-ph/9403398
1995 arXiv
-
[42]
Alonso, M
R. Alonso, M. Dhen, M. B. Gavela, and T. Hambye, Muon conversion to electron in nuclei in type-I seesaw models, JHEP01, 118, arXiv:1209.2679 [hep-ph]
-
[43]
M. Daum, B. Jost, R. M. Marshall, R. C. Minehart, W. A. Stephens, and K. O. H. Ziock, Search for Admixtures of Massive Neutrinos in the Decayπ+ →µ + Neutrino, Phys. Rev. D36, 2624 (1987)
1987
-
[44]
Aguilar-Arevalo et al
A. Aguilar-Arevalo et al. (PIENU), Search for heavy neu- trinos inπ→µνdecay, Phys. Lett. B798, 134980 (2019), arXiv:1904.03269 [hep-ex]
2019 arXiv
-
[45]
Bernardi et al., Search for Neutrino Decay, Phys
G. Bernardi et al., Search for Neutrino Decay, Phys. Lett. B166, 479 (1986)
1986
-
[46]
Bernardi et al., FURTHER LIMITS ON HEA VY NEUTRINO COUPLINGS, Phys
G. Bernardi et al., FURTHER LIMITS ON HEA VY NEUTRINO COUPLINGS, Phys. Lett. B203, 332 (1988)
1988
-
[47]
Abe et al
K. Abe et al. (T2K), Search for heavy neutrinos with the T2K near detector ND280, Phys. Rev. D100, 052006 (2019), arXiv:1902.07598 [hep-ex]
2019 arXiv
-
[48]
K. J. Kelly and P. A. N. Machado, MicroBooNE experi- ment, NuMI absorber, and heavy neutral leptons, Phys. Rev. D104, 055015 (2021), arXiv:2106.06548 [hep-ph]
2021 arXiv
-
[49]
C. A. Arg¨ uelles, N. Foppiani, and M. Hostert, Heavy neutral leptons below the kaon mass at hodoscopic neutrino detectors, Phys. Rev. D105, 095006 (2022), arXiv:2109.03831 [hep-ph]
2022 arXiv
-
[50]
R. S. Hayano et al., HEA VY NEUTRINO SEARCH US- ING K(mu2) DECAY, Phys. Rev. Lett.49, 1305 (1982)
1982
-
[51]
Yamazaki et al., Search for Heavy Neutrinos in Kaon Decay, Conf
T. Yamazaki et al., Search for Heavy Neutrinos in Kaon Decay, Conf. Proc. C840719, 262 (1984)
1984
-
[52]
A. V. Artamonov et al. (BNL-E949), Study of the decay K + →π +ν¯νin the momentum region 140< P π <199 MeV/c, Phys. Rev. D79, 092004 (2009), arXiv:0903.0030 [hep-ex]
2009 arXiv
-
[53]
Cortina Gil et al
E. Cortina Gil et al. (NA62), Search forK + decays to a muon and invisible particles, Phys. Lett. B816, 136259 (2021), arXiv:2101.12304 [hep-ex]
2021 arXiv
-
[54]
A. M. Cooper-Sarkar et al. (W A66), Search for Heavy Neutrino Decays in the BEBC Beam Dump Experiment, Phys. Lett. B160, 207 (1985)
1985
-
[55]
Vaitaitis et al
A. Vaitaitis et al. (NuTeV, E815), Search for neutral heavy leptons in a high-energy neutrino beam, Phys. Rev. Lett.83, 4943 (1999), arXiv:hep-ex/9908011
1999 arXiv
-
[56]
Bergsma et al
F. Bergsma et al. (CHARM), A Search for Decays of Heavy Neutrinos in the Mass Range 0.5-GeV to 2.8-GeV, Phys. Lett. B166, 473 (1986)
1986
-
[57]
Aad et al
G. Aad et al. (ATLAS), Search for heavy neutral leptons in decays ofWbosons produced in 13 TeVppcollisions using prompt and displaced signatures with the ATLAS detector, JHEP10, 265, arXiv:1905.09787 [hep-ex]
1905 arXiv
-
[58]
Aad et al
G. Aad et al. (ATLAS), Search for Heavy Neutral Leptons in Decays of W Bosons Using a Dilepton Displaced Ver- tex in s=13 TeV pp Collisions with the ATLAS Detector, Phys. Rev. Lett.131, 061803 (2023), arXiv:2204.11988 [hep-ex]
2023 arXiv
-
[59]
Tumasyan et al
A. Tumasyan et al. (CMS), Search for long-lived heavy neutral leptons with displaced vertices in proton- proton collisions at √s =13 TeV, JHEP07, 081, arXiv:2201.05578 [hep-ex]
-
[60]
Abreu et al
P. Abreu et al. (DELPHI), Search for neutral heavy lep- tons produced in Z decays, Z. Phys. C74, 57 (1997), [Erratum: Z.Phys.C 75, 580 (1997)]
1997
-
[61]
Fernandez-Martinez, J
E. Fernandez-Martinez, J. Hernandez-Garcia, and J. Lopez-Pavon, Global constraints on heavy neutrino mixing, JHEP08, 033, arXiv:1605.08774 [hep-ph]
-
[62]
A. M. Abdullahi et al., The present and future status of heavy neutral leptons, J. Phys. G50, 020501 (2023), arXiv:2203.08039 [hep-ph]
2023 arXiv
-
[63]
Krasnov, DUNE prospects in the search for ster- ile neutrinos, Phys
I. Krasnov, DUNE prospects in the search for ster- ile neutrinos, Phys. Rev. D100, 075023 (2019), arXiv:1902.06099 [hep-ph]
2019 arXiv
-
[64]
Ballett, T
P. Ballett, T. Boschi, and S. Pascoli, Heavy Neutral Lep- tons from low-scale seesaws at the DUNE Near Detector, JHEP03, 111, arXiv:1905.00284 [hep-ph]
1905 arXiv
-
[65]
Carbajal and A
S. Carbajal and A. M. Gago, Indirect search of heavy neutral leptons using the DUNE near detector, Front. in 8 Phys.12, 1398070 (2024), arXiv:2202.09217 [hep-ph]
2024 arXiv
-
[66]
J. L. Feng, I. Galon, F. Kling, and S. Trojanowski, For- wArd Search ExpeRiment at the LHC, Phys. Rev. D97, 035001 (2018), arXiv:1708.09389 [hep-ph]
2018 arXiv
-
[67]
Ahdida et al
C. Ahdida et al. (SHiP), Sensitivity of the SHiP ex- periment to Heavy Neutral Leptons, JHEP04, 077, arXiv:1811.00930 [hep-ph]
-
[68]
J. P. Chou, D. Curtin, and H. J. Lubatti, New Detectors to Explore the Lifetime Frontier, Phys. Lett. B767, 29 (2017), arXiv:1606.06298 [hep-ph]
2017 arXiv
-
[69]
Aielli et al
G. Aielli et al. (CODEX-b), Expression of interest for the CODEX-b detector, Eur. Phys. J. C80, 1177 (2020), arXiv:1911.00481 [hep-ex]
2020 arXiv
-
[70]
Hirsch and Z
M. Hirsch and Z. S. Wang, Heavy neutral leptons at ANU- BIS, Phys. Rev. D101, 055034 (2020), arXiv:2001.04750 [hep-ph]
2020 arXiv
-
[71]
E. J. Chun, A. Das, S. Mandal, M. Mitra, and N. Sinha, Sensitivity of Lepton Number Violating Meson Decays in Different Experiments, Phys. Rev. D100, 095022 (2019), arXiv:1908.09562 [hep-ph]
2019 arXiv
-
[72]
Antusch, E
S. Antusch, E. Cazzato, and O. Fischer, Sterile neutrino searches via displaced vertices at LHCb, Phys. Lett. B 774, 114 (2017), arXiv:1706.05990 [hep-ph]
2017 arXiv
-
[73]
Drewes and J
M. Drewes and J. Hajer, Heavy Neutrinos in displaced vertex searches at the LHC and HL-LHC, JHEP02, 070, arXiv:1903.06100 [hep-ph]
1903 arXiv
-
[74]
Blondel et al., Searches for long-lived particles at the future FCC-ee, Front
A. Blondel et al., Searches for long-lived particles at the future FCC-ee, Front. in Phys.10, 967881 (2022), arXiv:2203.05502 [hep-ex]
2022 arXiv
-
[75]
Blondel, E
A. Blondel, E. Graverini, N. Serra, and M. Shaposhnikov (FCC-ee study Team), Search for Heavy Right Handed Neutrinos at the FCC-ee, Nucl. Part. Phys. Proc.273- 275, 1883 (2016), arXiv:1411.5230 [hep-ex]
2016 arXiv
-
[76]
Antusch, O
S. Antusch, O. Fischer, and A. Hammad, Lepton-Trijet and Displaced Vertex Searches for Heavy Neutrinos at Future Electron-Proton Colliders, JHEP03, 110, arXiv:1908.02852 [hep-ph]
1908 arXiv
-
[77]
Pascoli, R
S. Pascoli, R. Ruiz, and C. Weiland, Heavy neutrinos with dynamic jet vetoes: multilepton searches at √s= 14 , 27, and 100 TeV, JHEP06, 049, arXiv:1812.08750 [hep-ph]
-
[78]
The International Linear Collider Technical Design Report - Volume 1: Executive Summary (2013), arXiv:1306.6327 [physics.acc-ph]
2013 arXiv
-
[79]
Antusch, E
S. Antusch, E. Cazzato, and O. Fischer, Sterile neutrino searches at futuree −e+,pp, ande −pcolliders, Int. J. Mod. Phys. A32, 1750078 (2017), arXiv:1612.02728 [hep- ph]
2017 arXiv
-
[80]
Boyarsky, O
A. Boyarsky, O. Mikulenko, M. Ovchynnikov, and L. Shchutska, Exploring the potential of FCC-hh to search for particles from B mesons, JHEP01, 042, arXiv:2204.01622 [hep-ph]
-
[81]
P. Li, Z. Liu, and K.-F. Lyu, Heavy neutral leptons at muon colliders, JHEP03, 231, arXiv:2301.07117 [hep-ph]
-
[82]
Kitano, I
R. Kitano, I. Low, R. Matsudo, S. Okawa, and S. Roy, Heavy Neutral Lepton at Same-Sign Muon Collider (2025), arXiv:2510.18390 [hep-ph]
2025
-
[83]
P. D. Bolton, F. F. Deppisch, and P. S. Bhupal Dev, Neu- trinoless double beta decay versus other probes of heavy sterile neutrinos, JHEP03, 170, arXiv:1912.03058 [hep- ph]
1912 arXiv
-
[84]
Fern´ andez-Mart ´ ınez, M
E. Fern´ andez-Mart ´ ınez, M. Gonz´ alez-L´ opez, J. Hern´ andez-Garc ´ ıa, M. Hostert, and J. L´ opez-Pav´ on, Effective portals to heavy neutral leptons, JHEP09, 001, arXiv:2304.06772 [hep-ph]
-
[85]
A. C. Vincent, E. F. Martinez, P. Hern´ andez, M. Lat- tanzi, and O. Mena, Revisiting cosmological bounds on sterile neutrinos, JCAP04, 006, arXiv:1408.1956 [astro- ph.CO]
1956 arXiv
-
[86]
Langhoff, N
K. Langhoff, N. J. Outmezguine, and N. L. Rodd, Irre- ducible Axion Background, Phys. Rev. Lett.129, 241101 (2022), arXiv:2209.06216 [hep-ph]
2022 arXiv
-
[87]
Hernandez, M
P. Hernandez, M. Kekic, and J. Lopez-Pavon,N eff in low- scale seesaw models versus the lightest neutrino mass, Phys. Rev. D90, 065033 (2014), arXiv:1406.2961 [hep- ph]
2014 arXiv
-
[88]
A. D. Dolgov, S. H. Hansen, G. Raffelt, and D. V. Semikoz, Cosmological and astrophysical bounds on a heavy sterile neutrino and the KARMEN anomaly, Nucl. Phys. B580, 331 (2000), arXiv:hep-ph/0002223
2000 arXiv
-
[89]
Boyarsky, O
A. Boyarsky, O. Ruchayskiy, and M. Shaposhnikov, The Role of sterile neutrinos in cosmology and astro- physics, Ann. Rev. Nucl. Part. Sci.59, 191 (2009), arXiv:0901.0011 [hep-ph]
2009 arXiv
-
[90]
Ruchayskiy and A
O. Ruchayskiy and A. Ivashko, Restrictions on the life- time of sterile neutrinos from primordial nucleosynthesis, JCAP10, 014, arXiv:1202.2841 [hep-ph]
-
[91]
G. B. Gelmini, M. Kawasaki, A. Kusenko, K. Murai, and V. Takhistov, Big Bang Nucleosynthesis constraints on sterile neutrino and lepton asymmetry of the Universe, JCAP09, 051, arXiv:2005.06721 [hep-ph]
2005 arXiv
-
[92]
Sabti, A
N. Sabti, A. Magalich, and A. Filimonova, An Extended Analysis of Heavy Neutral Leptons during Big Bang Nu- cleosynthesis, JCAP11, 056, arXiv:2006.07387 [hep-ph]
2006 arXiv
-
[93]
Boyarsky, M
A. Boyarsky, M. Ovchynnikov, O. Ruchayskiy, and V. Syvolap, Improved big bang nucleosynthesis con- straints on heavy neutral leptons, Phys. Rev. D104, 023517 (2021), arXiv:2008.00749 [hep-ph]. END MA TTER Accidental symmetry of the texture-zero solution The texture-zero soluti...
2021 arXiv
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