REVIEW 3 major objections 5 minor 1 cited by
This paper proposes that the neutrino mass-squared differences obey the exact ratio (√Δm²31 + √Δm²21)/(√Δm²31 − √Δm²21) = √2, which would fix the absolute neutrino masses if the lightest neutrino is massless.
Reviewed by Pith at T0; open to challenge. T0 means a machine referee read the full paper against a public rubric. the ladder, T0–T4 →
T0 review · deepseek-v4-flash
2026-08-03 07:52 UTC pith:YDT7UJMO
load-bearing objection A genuinely new numerical coincidence in neutrino mass-squared differences, honestly presented, but the paper promotes an assumption to a relation without quantifying how unlikely the coincidence is. the 3 major comments →
Another relation among the neutrino mass-squared differences?
The pith
A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.
Core claim
The author's central claim is that the ratio λ = (√Δm²31 + √Δm²21)/(√Δm²31 − √Δm²21) is exactly √2, not merely close to it. Assuming λ = √2, the paper derives that one mass-squared difference fixes the other two, that (Δm²21 + Δm²31)/(√Δm²21 + √Δm²31)² = 3/4, and that (Δm²32)²/(Δm²21 Δm²31) = 32. The author reads the last identity as evidence that ν1 is massless, which gives the mass ratio √(m2/m3) = tan(π/8) and the absolute predictions m2 ≈ 0.00866 eV, m3 ≈ 0.05029 eV, mνe ≈ 0.00892 eV, Σmi ≈ 0.05895 eV, and an effective Majorana mass between 0.00141 and 0.00383 eV depending on the unknown phases.
What carries the argument
The load-bearing object is the dimensionless ratio λ(Δm²21, Δm²31) defined in Eq. (1), built from the square roots of the two measured mass-squared differences. The entire paper is the algebra that follows from setting this ratio exactly to √2: the relation is rearranged into a sum-to-square ratio of 3/4, a product identity (Δm²32)² = 32 Δm²21 Δm²31, and, once m1 = 0 is assumed, into m3/m2 = (√2+1)/(√2−1), equivalently √(m2/m3) = tan(π/8). Because √2 is a fixed irrational number, the relation constrains the two independent splittings to a one-parameter family and ties absolute masses to a single input.
Load-bearing premise
The results stand or fall on the premise that the observed ratio's proximity to √2 — about 0.3% at best-fit values — is an exact physical equality rather than a numerical coincidence, together with the assumed normal mass ordering.
What would settle it
Measure Δm²21 and Δm²31 with sub-0.1% precision and form λ = (√Δm²31 + √Δm²21)/(√Δm²31 − √Δm²21); if the central value differs from √2 by more than the combined uncertainty — for instance a measured λ of 1.419 or 1.409 with errors near 10⁻⁴ — the exact relation is ruled out. Such a measurement is within the stated reach of upcoming reactor-neutrino experiments.
If this is right
- A single measured mass-squared difference determines the other two, so future precision on either Δm²21 or Δm²31 directly predicts the third.
- If m1 = 0, the absolute neutrino masses are predicted: m2 ≈ 0.00866 eV, m3 ≈ 0.05029 eV, and Σmi ≈ 0.05895 eV, a value near the lower limit allowed by cosmology.
- The predicted effective electron-neutrino mass mνe ≈ 0.00892 eV is within range of proposed quantum-technology beta-decay experiments aiming at ~0.01 eV sensitivity.
- The predicted effective Majorana mass lies between about 0.0014 and 0.0038 eV, a target for next-generation neutrinoless double-beta decay searches once their sensitivity crosses this band.
- The same algebraic structure that yields λ = √2 also produces a charged-lepton-mass-like relation with value 3/4, offering a possible link between neutrino and charged-lepton mass generation.
Where Pith is reading between the lines
- The 0.27% agreement across fits is not a calibrated test: a scan over many simple algebraic functions of the two splittings would show how many combinations land within 0.3% of a simple constant, which would calibrate how surprising this particular coincidence is.
- The demonstrated 0.03σ shift of Δm²21 that reproduces √2 to seven digits is a reminder that the relation is an ansatz rather than a fit; future tests should compare the predicted ratio against the full correlated uncertainties of both splittings, not against each best-fit point separately.
- If m1 is not exactly zero but small, the relation still holds while the absolute masses scale differently; a cosmological measurement of Σmi near 0.059 eV would support m1 = 0, while a value noticeably above that would favor a lighter-but-nonzero m1 within the relation.
- A derivation of the values 3/4 and √2 from a single mass-generation mechanism would unify this relation with the charged-lepton mass formula; searching for such a mechanism is a natural theoretical next step.
Editorial analysis
A structured set of objections, weighed in public.
Referee Report
Summary. The manuscript proposes an exact relation, Eq. (2), between the solar and atmospheric neutrino mass-squared differences: (sqrt(Δm²31)+sqrt(Δm²21))/(sqrt(Δm²31)-sqrt(Δm²21)) = sqrt(2). It reports that this ratio evaluated at best-fit points from several global fits lies within 0.27% of sqrt(2), and that a 0.03σ shift of Δm²21 produces a seven-decimal match. The paper derives algebraic consequences, including a Koide-like relation, Eq. (4), and interprets the relation as pointing toward m1 = 0. For m1 = 0 it obtains m2 ≈ 0.00866 eV, m3 ≈ 0.05029 eV, Σmi ≈ 0.05895 eV, mνe ≈ 0.00892 eV, and a range for mββ. The normal mass ordering is assumed throughout.
Significance. If Eq. (2) were exact and m1 = 0, the neutrino mass spectrum would be fixed by a single mass-squared difference, and the predicted absolute mass scale would sit near the lower edge of cosmological bounds. The algebra from Eq. (2) to Eq. (8) is simple and correct, and the paper is transparent in stating that Eq. (2) is an assumption rather than a derived law. The relation is falsifiable with future JUNO and other oscillation data. However, the quantitative evidence presented is only a numerical coincidence: no statistical test is performed, no null hypothesis is defined, and no account is taken of the post hoc choice of the ratio and the target value sqrt(2). Consequently, the paper's central claim is not yet quantitatively supported, and the 'predictions' in Section IV mostly restate the input data plus the ansatz rather than providing independent checks.
major comments (3)
- [Section II, Eq. (2), Table I] The only evidence for Eq. (2) is that λ evaluated at several best-fit points lies in [1.4140, 1.4181], a 0.27% spread. This is not a statistical test. The paper does not compute the probability that two measured quantities would yield a ratio this close to sqrt(2) under a plausible null hypothesis, nor does it account for the look-elsewhere effect of selecting this particular functional form and target constant after inspecting the data. I request a quantitative evaluation: a chi-square or posterior probability for λ = sqrt(2) using the full (correlated) covariance matrix of Δm²21 and Δm²31, and an estimate of the trials factor involved in choosing this ratio. This is load-bearing, since Eq. (2) is the basis for all subsequent results.
- [Section III, Eqs. (6)-(7)] The inference that Eq. (7) implies m1 = 0 is not justified. Equations (6) and (7) are algebraic rewritings of Eq. (2); the left-hand side Δm²21 Δm²31 depends on m1 in general, and expressing it as (1/32)(m3² - m2²)² follows from the assumed ratio, not from vanishing m1. The statement 'we attribute this observation to the masslessness of ν1' is an interpretation, not a derivation. To support m1 ≈ 0, the author should solve Eq. (2) for m1 using the measured values of Δm²21 and Δm²31 (including uncertainties) or otherwise demonstrate that the data favor m1 = 0. As written, the 'solutions' in Section IV impose m1 = 0 by hand.
- [Section II, seven-decimal agreement] The demonstration that shifting Δm²21 to 7.5065×10⁻⁵ eV², within 0.03σ of the reference best fit, yields λ = 1.41421359 does not add evidential weight: for any continuous observable and any target value, one can normally find a point inside a confidence interval that satisfies the target exactly. The sentence 'the accuracy can be made arbitrarily high' is therefore misleading. In addition, Table I reports λ without uncertainties, and the various global fits are not independent; their scatter cannot be interpreted as a distribution of λ. I recommend propagating the errors of a single reference fit (including correlations) and de-emphasizing the tuned seven-decimal match.
minor comments (5)
- [Eq. (3)] Please state how the uncertainty 0.0045 is obtained and whether the uncertainties in Δm²21 from JUNO and Δm²31 from NuFIT are treated as uncorrelated. Also clarify that these two inputs come from different datasets.
- [Section II, near Eq. (2)] The phrase 'the relatively small error' should refer to a specific quantity, ideally the propagated uncertainty in λ or the deviation of the ratio from sqrt(2).
- [Section IV] Typographical: 'Zpole' should be 'Z pole'.
- [Table I] The two rows for NuFIT-6.0 [49] and the two rows for NuFIT-6.1 [17] should be labeled to indicate which dataset or ordering they correspond to, since they currently appear as duplicate entries.
- [General] The paper uses 'best fit' inconsistently: sometimes it means global-fit central values, sometimes a value shifted within 1σ. A uniform terminology with explicit error bars would improve readability.
Circularity Check
The central 'predictions' for neutrino masses are the fitted mass-squared differences renamed under the assumption m1 = 0; the ansatz (2) is adopted because the same data already satisfy it, making its 'consistency' checks algebraic tautologies.
specific steps
-
fitted input called prediction
[Section IV, after Eq. (9); numerical solutions]
"Our interpretation implies the solutions m1 ≃0, m2 = sqrt(Δm2_21), m3 = sqrt(Δm2_31), Σ_i m_i = sqrt(Δm2_21)+sqrt(Δm2_31) ... By adopting the first JUNO results [20] for Δm2_21 ... and taking Δm2_31 ... from the NuFIT-6.1 global analysis [17], we numerically find m1 ≃0, m2 = 0.00866±0.00007 eV, m3 = 0.05029±0.00021 eV ... Σ_i m_i = 0.05895±0.00022 eV"
With m1 = 0, the identities Δm2_21 = m2^2 and Δm2_31 = m3^2 make m2, m3, and Σm_i literally the square roots and sum of the very same fitted inputs used to motivate and calibrate relation (2). The numbers quoted as 'predictions' are therefore not new results but a relabeling of the input global-fit values; any agreement with external constraints is inherited automatically from the choice of inputs.
-
self definitional
[Section II, Eq. (2) and following 'consistency' checks; Section III, Eqs. (4), (6), (8)]
"Inspired by these observations, we assume that (sqrt(Δm2_31)+sqrt(Δm2_21))/(sqrt(Δm2_31)-sqrt(Δm2_21)) = sqrt(2) ... From (2), we also find [Eq. (4)] ... which is consistent with the global fits as well. For example, with the data from [50], the left-hand side is 0.7501, in excellent agreement with the predicted value of 3/4."
Equation (2) is adopted because the global-fit best-fit points already make the left-hand side close to √2; then Eq. (4) is algebraically equivalent to Eq. (2), and Eq. (8) is a rearranged form of the same relation. Checking these equations against the same fitted values is therefore a check of the ansatz against the data that generated the ansatz, not an independent test. The 'excellent agreement' is built into the choice of (2).
-
fitted input called prediction
[Section II, seven-figure agreement; footnote 2]
"For example, a minor shift in just Δm2_21 to 7.5065×10^-5 eV^2 – a value within 0.03σ of the best fit [50] – leads to the result λ(7.5065×10^-5 eV^2, 2.55×10^-3 eV^2) = 1.41421359, which approximates √2 to seven (!) decimal places."
The 'seven-decimal' match is manufactured by selecting a point inside the 1σ interval of the fitted Δm2_21 specifically to make λ equal √2. Since any continuous function can be matched to any target value by moving within a confidence interval, this is not evidence for (2); it is an explicit tuning of the input to the claimed output.
full rationale
The paper is honest that Eq. (2) is an ansatz ('we assume'), not a derived law, so the choice of the relation itself is not presented as a prediction. However, the subsequent 'physical predictions' — m2, m3, Σm_i — are obtained by setting m1 = 0 and then taking square roots of the exact same Δm2_21 and Δm2_31 inputs that were used to select Eq. (2). This is a textbook case of fitted input renamed as prediction: the numerical outputs are identities once m1 = 0. The consistency checks in Eqs. (4), (6), and (8) are algebraic rearrangements of Eq. (2), and Eq. (2) was itself chosen because the best-fit values already satisfy it to ~0.3%; the seven-figure agreement is produced by a deliberate 0.03σ shift of Δm2_21. There is no self-citation load-bearing chain and no uniqueness theorem imported from the authors; the circularity is in the reduction of the quantitative predictions to the fitted inputs. Score 7 reflects that the core number-output of the paper reduces by construction, while the paper's one genuinely new content — the specific algebraic form with √2 as a phenomenological hypothesis — remains an unproven ansatz rather than a tested prediction. The external comparisons (KATRIN, DESI, Koide extensions) are only consistency comments and do not rescue the predictions from being restatements of the inputs.
Axiom & Free-Parameter Ledger
free parameters (2)
- Δm²21 = 7.5065×10⁻⁵ eV² (shifted best-fit) =
7.5065e-5 eV²
- m1 (lightest neutrino mass) =
0 eV (assumed)
axioms (5)
- domain assumption Standard three-flavor neutrino oscillation framework with unitary PMNS mixing.
- domain assumption Normal mass ordering (m1 < m2 < m3) with Δm²31 > 0.
- domain assumption The measured best-fit values for Δm²21 and Δm²31 from global fits are correct and can be used as exact inputs.
- ad hoc to paper The ratio λ is exactly √2 (Eq. 2).
- ad hoc to paper m1 = 0 (lightest neutrino mass vanishes).
read the original abstract
Determining the absolute neutrino mass scale remains a compelling challenge in particle physics. Establishing precise mathematical connections among the neutrino masses could significantly facilitate this task and shed additional light on the underlying mass-generation mechanism. We highlight the possible existence of a simple algebraic relation between the mass-squared differences, $(\sqrt{\Delta m^2_{31}}+\sqrt{\Delta m^2_{21}})/(\sqrt{\Delta m^2_{31}}-\sqrt{\Delta m^2_{21}})=\sqrt{2}$, which exhibits excellent agreement with the central values of recent global fits of neutrino oscillation data. We investigate the implications of adopting this ansatz and how it reduces the number of independent parameters in the neutrino sector. Notably, for a vanishing $\nu_1$ mass, this expression directly simplifies to the elegant Fritzsch relation: $\sqrt{m_2/m_3}=\tan{(\pi/8)}$.
Forward citations
Cited by 1 Pith paper
-
Integral representation of the neutrino mass-squared differences
The claimed m1 < 0.0023 eV bound is an artifact of assuming the trapezoid error is small enough to force the result; the integral representation gives no independent constraint.
Reference graph
Works this paper leans on
-
[1]
Navaset al.(Particle Data Group), Review of particle physics, Phys
S. Navaset al.(Particle Data Group), Review of particle physics, Phys. Rev. D110, 030001 (2024)
2024
-
[2]
The results (reported to five significant digits) approximate √ 2 with a maximum relative error of 0.27%. [Ref.] ∆m2 21 10−5 eV2 ∆m2 31 10−3 eV2 λ(∆m2 21,∆m 2 31) Best fit Best fit [This work] Capozziet al.[47]7.34 2.485 1.4151 Capozziet al.[48]7.37 2.495 1.4151 NuFIT-6.0 [49]7.49 2.513 1.4173 NuFIT-6.0 [49]7.49 2.534 1.4152 de Salaset al.[50]7.50 2.550 1...
-
[3]
Then, we have investigated the implications of this ratio and proposed an interpreta- tion of the results obtained
This provides an algebraic framework for the manipulation of the mass-squared differences. Then, we have investigated the implications of this ratio and proposed an interpreta- tion of the results obtained. In particular, it follows that specifying just two neutrino masses allows for the recon- struction of the entire mass-squared difference spectrum. Thi...
-
[4]
In these non-ideal scenarios, such a deviation can be treated as perturbation, justifying the use of (2) as an unperturbed equation
Based on Table I (right- most column) as well as on (3), the ratio is expected to be stable to at least two decimal places (being ap- proximately 1.41). In these non-ideal scenarios, such a deviation can be treated as perturbation, justifying the use of (2) as an unperturbed equation. Notably, the val- ues in Table I approximate √ 2 with a maximum relativ...
-
[5]
M. G. Aartsenet al.(IceCube), Determining neutrino oscillation parameters from atmospheric muon neutrino disappearance with three years of IceCube DeepCore data, Phys. Rev. D91, 072004 (2015), arXiv:1410.7227 [hep-ex]
Pith/arXiv arXiv 2015
-
[6]
Q. R. Ahmadet al.(SNO), Direct evidence for neutrino flavor transformation from neutral current interactions in the Sudbury Neutrino Observatory, Phys. Rev. Lett.89, 011301 (2002), arXiv:nucl-ex/0204008
Pith/arXiv arXiv 2002
-
[7]
S. Fukudaet al.(Super-Kamiokande), Solar B-8 and hep neutrino measurements from 1258 days of Super- Kamiokande data, Phys. Rev. Lett.86, 5651 (2001), arXiv:hep-ex/0103032
Pith/arXiv arXiv 2001
-
[8]
Fukudaet al.(Super-Kamiokande), Evidence for os- cillation of atmospheric neutrinos, Phys
Y. Fukudaet al.(Super-Kamiokande), Evidence for os- cillation of atmospheric neutrinos, Phys. Rev. Lett.81, 1562 (1998), arXiv:hep-ex/9807003
Pith/arXiv arXiv 1998
-
[9]
N. Agafonovaet al.(OPERA), Discovery ofτNeu- trino Appearance in the CNGS Neutrino Beam with the OPERA Experiment, Phys. Rev. Lett.115, 121802 (2015), arXiv:1507.01417 [hep-ex]
Pith/arXiv arXiv 2015
-
[10]
Aliuet al.(K2K), Evidence for muon neutrino oscilla- tion in an accelerator-based experiment, Phys
E. Aliuet al.(K2K), Evidence for muon neutrino oscilla- tion in an accelerator-based experiment, Phys. Rev. Lett. 94, 081802 (2005), arXiv:hep-ex/0411038
Pith/arXiv arXiv 2005
-
[11]
P. Adamsonet al.(MINOS), Measurement of Neu- trino Oscillations with the MINOS Detectors in the NuMI Beam, Phys. Rev. Lett.101, 131802 (2008), arXiv:0806.2237 [hep-ex]
Pith/arXiv arXiv 2008
-
[12]
K. Abeet al.(T2K), Indication of Electron Neutrino Ap- pearance from an Accelerator-produced Off-axis Muon Neutrino Beam, Phys. Rev. Lett.107, 041801 (2011), arXiv:1106.2822 [hep-ex]
Pith/arXiv arXiv 2011
-
[13]
J. K. Ahnet al.(RENO), Observation of Reactor Electron Antineutrino Disappearance in the RENO Experiment, Phys. Rev. Lett.108, 191802 (2012), arXiv:1204.0626 [hep-ex]
Pith/arXiv arXiv 2012
-
[14]
K. Eguchiet al.(KamLAND), First results from Kam- LAND: Evidence for reactor anti-neutrino disappear- ance, Phys. Rev. Lett.90, 021802 (2003), arXiv:hep- ex/0212021
arXiv 2003
-
[15]
Y. Abeet al.(Double Chooz), Indication of Reactor ¯ν e Disappearance in the Double Chooz Experiment, Phys. Rev. Lett.108, 131801 (2012), arXiv:1112.6353 [hep-ex]
Pith/arXiv arXiv 2012
-
[16]
F. P. Anet al.(Daya Bay), Observation of electron- antineutrino disappearance at Daya Bay, Phys. Rev. Lett.108, 171803 (2012), arXiv:1203.1669 [hep-ex]
Pith/arXiv arXiv 2012
-
[17]
I. Esteban, M. C. Gonzalez-Garcia, M. Maltoni, I. Martinez-Soler, J. P. Pinheiro, and T. Schwetz, Lessons from the first JUNO results, (2026), arXiv:2601.09791 [hep-ph]
Pith/arXiv arXiv 2026
-
[18]
K. Abeet al.(T2K), Measurements of neutrino oscilla- 5 tion parameters from the T2K experiment using 3.6×1021 protons on target, Eur. Phys. J. C83, 782 (2023), arXiv:2303.03222 [hep-ex]
arXiv 2023
-
[19]
K. Abeet al.(T2K), Results from the T2K Experi- ment on Neutrino Mixing Including a New Far Detec- torµ-like Sample, Phys. Rev. Lett.135, 261801 (2025), arXiv:2506.05889 [hep-ex]
arXiv 2025
-
[20]
S. Abubakaret al.(NOvA), Precision Measurement of Neutrino Oscillation Parameters with 10 Years of Data from the NOvA Experiment, Phys. Rev. Lett.136, 011802 (2026), arXiv:2509.04361 [hep-ex]
arXiv 2026
-
[21]
B. Abiet al.(DUNE), Deep Underground Neutrino Ex- periment (DUNE), Far Detector Technical Design Re- port, Volume I Introduction to DUNE, JINST15(08), T08008 (2020), arXiv:2002.02967 [physics.ins-det]
arXiv 2020
-
[22]
S. Abubakaret al.(T2K, NOvA), Joint neutrino oscil- lation analysis from the T2K and NOvA experiments, Nature646, 818 (2025), arXiv:2510.19888 [hep-ex]
arXiv 2025
-
[23]
A. Abuslemeet al.(JUNO), Sub-percent precision mea- surement of neutrino oscillation parameters with JUNO, Chin. Phys. C46, 123001 (2022), arXiv:2204.13249 [hep- ex]
arXiv 2022
-
[24]
A. Abuslemeet al.(JUNO), First measurement of reactor neutrino oscillations at JUNO, (2025), arXiv:2511.14593 [hep-ex]
arXiv 2025
-
[25]
A. D. Dolgov, Neutrinos in cosmology, Phys. Rept.370, 333 (2002), arXiv:hep-ph/0202122
Pith/arXiv arXiv 2002
-
[26]
K. Abeet al.(Hyper-Kamiokande), Hyper-Kamiokande Design Report, (2018), arXiv:1805.04163 [physics.ins- det]
Pith/arXiv arXiv 2018
-
[27]
P. B. Denton, Neutrino Oscillations in the Three Flavor Paradigm, (2025), arXiv:2501.08374 [hep-ph]
arXiv 2025
-
[28]
G. Drexlin and C. Weinheimer, KATRIN experiment, (2026), arXiv:2601.00248 [nucl-ex]
arXiv 2026
-
[29]
S. Dell’Oro, S. Marcocci, M. Viel, and F. Vissani, Neutri- noless double beta decay: 2015 review, Adv. High Energy Phys.2016, 2162659 (2016), arXiv:1601.07512 [hep-ph]
Pith/arXiv arXiv 2015
-
[30]
M. Akeret al.(KATRIN), Direct neutrino-mass measure- ment based on 259 days of KATRIN data, Science388, adq9592 (2025), arXiv:2406.13516 [nucl-ex]
arXiv 2025
-
[31]
It provides a framework to analytically manipulate these parameters and admits specific physical interpretations. In particular, the results may point toward a vanishingν 1 mass. I. INTRODUCTION The standard three-neutrino paradigm is based on the principle that three neutrino flavor eigenstates (νe,ν µ,ν τ ) are mixed with three neutrino mass eigen- stat...
Pith/arXiv arXiv 2026
-
[32]
A. G. Adameet al.(DESI), DESI 2024 VI: cosmologi- cal constraints from the measurements of baryon acous- tic oscillations, JCAP02, 021 (2025), arXiv:2404.03002 [astro-ph.CO]
Pith/arXiv arXiv 2024
-
[33]
D. Naredo-Tuero, M. Escudero, E. Fern´ andez-Mart ´ ınez, X. Marcano, and V. Poulin, Critical look at the cosmo- logical neutrino mass bound, Phys. Rev. D110, 123537 (2024), arXiv:2407.13831 [astro-ph.CO]
Pith/arXiv arXiv 2024
-
[34]
J. J. G´ omez-Cadenas, J. Mart ´ ın-Albo, J. Men´ endez, M. Mezzetto, F. Monrabal, and M. Sorel, The search for neutrinoless double-beta decay, Riv. Nuovo Cim.46, 619 (2023)
2023
-
[35]
Abeet al.(KamLAND-Zen), Search for Majorana Neutrinos with the Complete KamLAND-Zen Dataset, Phys
S. Abeet al.(KamLAND-Zen), Search for Majorana Neutrinos with the Complete KamLAND-Zen Dataset, Phys. Rev. Lett.135, 262501 (2025), arXiv:2406.11438 [hep-ex]. [32]Neutrino 2024,XXXI International Conference on Neu- trino Physics and Astrophysics (Milan, Italy) held in 16–22 June 2024. Website:https://agenda.infn.it/ event/37867/
arXiv 2025
-
[36]
Gatto, G
R. Gatto, G. Sartori, and M. Tonin, Weak Selfmasses, Cabibbo Angle, and Broken SU(2) x SU(2), Phys. Lett. B28, 128 (1968)
1968
-
[37]
Koide, Fermion - Boson Two-body Model of Quarks and Leptons and Cabibbo Mixing, Lett
Y. Koide, Fermion - Boson Two-body Model of Quarks and Leptons and Cabibbo Mixing, Lett. Nuovo Cim.34, 201 (1982)
1982
-
[38]
Koide, A Fermion - Boson Composite Model of Quarks and Leptons, Phys
Y. Koide, A Fermion - Boson Composite Model of Quarks and Leptons, Phys. Lett. B120, 161 (1983)
1983
-
[39]
Koide, A New View of Quark and Lepton Mass Hier- archy, Phys
Y. Koide, A New View of Quark and Lepton Mass Hier- archy, Phys. Rev. D28, 252 (1983)
1983
-
[40]
Z.-z. Xing and H. Zhang, On the Koide-like relations for the running masses of charged leptons, neutrinos and quarks, Phys. Lett. B635, 107 (2006), arXiv:hep- ph/0602134
arXiv 2006
-
[41]
Y. Koide, Tribimaximal Neutrino Mixing and a Relation Between Neutrino- and Charged Lepton-Mass Spectra, J. Phys. G34, 1653 (2007), arXiv:hep-ph/0605074
Pith/arXiv arXiv 2007
-
[42]
N. Li and B.-Q. Ma, Estimate of neutrino masses from Koide’s relation, Phys. Lett. B609, 309 (2005), arXiv:hep-ph/0505028
Pith/arXiv arXiv 2005
-
[43]
Cao, Neutrino masses from lepton and quark mass relations and neutrino oscillations, Phys
F.-G. Cao, Neutrino masses from lepton and quark mass relations and neutrino oscillations, Phys. Rev. D85, 113003 (2012), arXiv:1205.4068 [hep-ph]
Pith/arXiv arXiv 2012
-
[44]
W. Rodejohann and H. Zhang, Extension of an empirical charged lepton mass relation to the neutrino sector, Phys. Lett. B698, 152 (2011), arXiv:1101.5525 [hep-ph]
Pith/arXiv arXiv 2011
-
[45]
G.-H. Gao and N. Li, Explorations of two empirical for- mulas for fermion masses, Eur. Phys. J. C76, 140 (2016), arXiv:1512.06349 [hep-ph]
Pith/arXiv arXiv 2016
-
[46]
W. Rodejohann, M. Tanimoto, and A. Watanabe, Relat- ing largeU e3 to the ratio of neutrino mass-squared dif- ferences, Phys. Lett. B710, 636 (2012), arXiv:1201.4936 [hep-ph]
Pith/arXiv arXiv 2012
-
[47]
D. Hernandez and A. Y. Smirnov, Relating neutrino masses and mixings by discrete symmetries, Phys. Rev. D88, 093007 (2013), arXiv:1304.7738 [hep-ph]
Pith/arXiv arXiv 2013
-
[48]
S. Roy, K. Sashikanta Singh, and J. Borah, Revamped Bi- Large neutrino mixing with Gatto-Sartori-Tonin like rela- tion, Nucl. Phys. B960, 115204 (2020), arXiv:2001.07401 [hep-ph]
Pith/arXiv arXiv 2020
-
[49]
R. N. Mohapatra and A. Y. Smirnov, Neutrino Mass and New Physics, Ann. Rev. Nucl. Part. Sci.56, 569 (2006), arXiv:hep-ph/0603118
Pith/arXiv arXiv 2006
-
[50]
F. Capozzi, E. Di Valentino, E. Lisi, A. Marrone, A. Mel- chiorri, and A. Palazzo, Global constraints on absolute neutrino masses and their ordering, Phys. Rev. D95, 096014 (2017), [Addendum: Phys.Rev.D 101, 116013 (2020)], arXiv:1703.04471 [hep-ph]
Pith/arXiv arXiv 2017
-
[51]
F. Capozzi, W. Giar` e, E. Lisi, A. Marrone, A. Melchiorri, and A. Palazzo, Neutrino masses and mixing: Entering the era of subpercent precision, Phys. Rev. D111, 093006 (2025), arXiv:2503.07752 [hep-ph]
Pith/arXiv arXiv 2025
-
[52]
I. Esteban, M. C. Gonzalez-Garcia, M. Maltoni, I. Martinez-Soler, J. P. Pinheiro, and T. Schwetz, NuFit- 6.0: updated global analysis of three-flavor neutrino os- cillations, JHEP12, 216 (2024), arXiv:2410.05380 [hep- ph]
Pith/arXiv arXiv 2024
-
[53]
P. F. de Salas, D. V. Forero, S. Gariazzo, P. Mart ´ ınez- Mirav´ e, O. Mena, C. A. Ternes, M. T´ ortola, and J. W. F. Valle, 2020 Global reassessment of the neutrino oscil- lation picture, JHEP02, 071 (2021), arXiv:2006.11237 [hep-ph]
Pith/arXiv arXiv 2020
-
[54]
J. A. Formaggio, A. L. C. de Gouvˆ ea, and R. G. H. Robertson, Direct Measurements of Neutrino Mass, 6 Phys. Rept.914, 1 (2021), arXiv:2102.00594 [nucl-ex]
Pith/arXiv arXiv 2021
-
[55]
A. A. S. Amadet al., Determining absolute neutrino mass using quantum technologies, New J. Phys.27, 105006 (2025), arXiv:2412.06338 [hep-ex]
arXiv 2025
discussion (0)
Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.