pith. sign in

arxiv: 2605.27049 · v2 · pith:LBMLFWH2new · submitted 2026-05-26 · ✦ hep-ph · hep-ex· hep-th

Family-separated seesaw relations of Majorana neutrinos

Pith reviewed 2026-06-29 16:59 UTC · model grok-4.3

classification ✦ hep-ph hep-exhep-th
keywords seesaw mechanismMajorana neutrinosneutrino massesflavor mixingheavy neutrinosneutrino phenomenologyfamily separation
0
0 comments X

The pith

The seesaw equation for Majorana neutrinos has a family-separated solution relating each light-heavy mass ratio to the squares of mixing matrix elements.

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

The paper identifies a new solution to the exact seesaw equation in which the mass ratio for each neutrino family stands alone. For the i-th family the ratio of light to heavy mass equals minus the square of one heavy mixing element over the square of the corresponding light mixing element. This separation works without breaking the unitarity of the full six-by-six mixing matrix. It connects the original seesaw parameters directly to the observable active neutrino properties and yields several testable predictions for neutrino experiments.

Core claim

Given the canonical seesaw mechanism, there exists a special solution to the exact seesaw equation m_i/M_i = - R^2_αi / U^2_αi for the masses and flavor mixing matrix elements of light and heavy Majorana neutrinos of the i-th family, for i=1,2,3 and α=e,μ,τ. This family-separated seesaw scenario allows simple relations between the original seesaw parameters and the active degrees of freedom, offering a number of testable predictions in neutrino phenomenology.

What carries the argument

The family-separated relation m_i/M_i = -R²_αi/U²_αi that solves the seesaw equation independently for each of the three neutrino families.

If this is right

  • The original seesaw parameters can be expressed in terms of the active neutrino mixing matrix elements.
  • Direct relations link the light and heavy neutrino sectors for each family.
  • Testable predictions arise for neutrino mass spectra and oscillation parameters.
  • The full 6x6 mixing matrix remains unitary and consistent.

Where Pith is reading between the lines

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

  • If correct, this solution could simplify the search for heavy Majorana neutrinos at colliders by fixing their couplings to each flavor.
  • Extensions might include similar separations in other seesaw variants or in models with additional symmetries.
  • Experimental bounds on heavy neutrino mixing could directly constrain the light neutrino masses in this framework.

Load-bearing premise

The exact seesaw equation can be solved in a family-separated manner without violating unitarity or other consistency conditions of the full 6x6 mixing matrix.

What would settle it

A measurement of neutrino mixing or mass ratios that fails to satisfy m_i/M_i = -R²_αi/U²_αi for any choice of family index i and flavor α.

Figures

Figures reproduced from arXiv: 2605.27049 by Zhi-zhong Xing.

Figure 1
Figure 1. Figure 1: A schematic illustration of the family-separated seesaw (FSS) scenario as a particular but [PITH_FULL_IMAGE:figures/full_fig_p004_1.png] view at source ↗
read the original abstract

Given the canonical seesaw mechanism as a most natural extension of the standard model in its neutrino sector, we find out a special but brand new solution to the exact seesaw equation: $m^{}_i/M^{}_i = - R^2_{\alpha i}/U^2_{\alpha i}$ for the masses and flavor mixing matrix elements of light and heavy Majorana neutrinos of the $i$-th family (for $i = 1, 2, 3$ and $\alpha = e, \mu, \tau$). This family-separated seesaw scenario allows us to establish simple relations between the original seesaw parameters and the active degrees of freedom, and thus offers a number of testable predictions in neutrino phenomenology.

Editorial analysis

A structured set of objections, weighed in public.

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

Referee Report

1 major / 0 minor

Summary. The manuscript claims to identify a special family-separated solution to the exact seesaw equation within the canonical seesaw mechanism, expressed as m_i/M_i = -R²_αi/U²_αi for the masses and flavor-mixing matrix elements of light and heavy Majorana neutrinos in the i-th family (i=1,2,3; α=e,μ,τ). This is asserted to yield simple relations between the original seesaw parameters and active degrees of freedom, together with a number of testable predictions in neutrino phenomenology.

Significance. If the proposed per-family relations can be shown to be consistent with the unitarity of the full 6×6 mixing matrix without additional ad-hoc assumptions, the result would supply a compact link between seesaw parameters and observable mixing angles and masses, potentially enabling new phenomenological tests.

major comments (1)
  1. [Abstract] Abstract (the displayed equation m_i/M_i = -R²_αi/U²_αi): the left-hand side is independent of the flavor index α while the right-hand side depends on α. For the equality to hold simultaneously for α = e, μ, τ at fixed i, the ratio |R_αi/U_αi| must be flavor-independent. The 6×6 unitarity conditions (UU† + RR† = 1 and its block counterparts) do not enforce column-wise proportionality between the U and R blocks in general; they permit it only for special textures. This renders the family separation non-generic and requires explicit demonstration that the chosen solution satisfies the full unitarity constraints.

Simulated Author's Rebuttal

1 responses · 0 unresolved

We thank the referee for the careful reading and for highlighting the need to explicitly connect the proposed family-separated solution to the full 6×6 unitarity constraints. We address the single major comment below.

read point-by-point responses
  1. Referee: [Abstract] Abstract (the displayed equation m_i/M_i = -R²_αi/U²_αi): the left-hand side is independent of the flavor index α while the right-hand side depends on α. For the equality to hold simultaneously for α = e, μ, τ at fixed i, the ratio |R_αi/U_αi| must be flavor-independent. The 6×6 unitarity conditions (UU† + RR† = 1 and its block counterparts) do not enforce column-wise proportionality between the U and R blocks in general; they permit it only for special textures. This renders the family separation non-generic and requires explicit demonstration that the chosen solution satisfies the full unitarity constraints.

    Authors: We agree that the displayed relation requires |R_αi/U_αi| to be independent of α for each fixed i. The manuscript explicitly describes the construction as a 'special but brand new solution,' so the family separation is presented as a non-generic scenario corresponding to particular textures in which the relevant columns of the U and R blocks satisfy the necessary proportionality. The relation is obtained directly from the exact seesaw equation under the family-separation ansatz; this ansatz selects the textures for which the unitarity conditions can be satisfied. To meet the referee's request for explicit demonstration, we will add a dedicated paragraph (or short subsection) verifying that the solution obeys the full set of 6×6 unitarity relations (UU† + RR† = I and the block counterparts) for the parameter choices considered in the paper. revision: yes

Circularity Check

0 steps flagged

No significant circularity in derivation of family-separated seesaw relations

full rationale

The paper presents a proposed special solution to the canonical seesaw equation in the form m_i/M_i = -R²_αi/U²_αi that permits family separation. This is framed as an exact algebraic solution under the assumption that the 6x6 unitary mixing matrix admits such per-family relations without inconsistency. No step reduces by construction to a fitted parameter, self-citation chain, or definitional renaming; the central relation is offered as a new ansatz or texture choice rather than an output forced by prior inputs within the paper itself. The derivation remains self-contained against the standard seesaw mass matrix and unitarity conditions.

Axiom & Free-Parameter Ledger

0 free parameters · 1 axioms · 0 invented entities

Abstract-only; ledger populated from stated elements in the abstract. The canonical seesaw is treated as given background.

axioms (1)
  • domain assumption The canonical seesaw mechanism supplies the exact equation being solved.
    Abstract opens with this premise as the starting point.

pith-pipeline@v0.9.1-grok · 5641 in / 1041 out tokens · 32841 ms · 2026-06-29T16:59:21.276865+00:00 · methodology

discussion (0)

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

Reference graph

Works this paper leans on

28 extracted references · 18 canonical work pages · 7 internal anchors

  1. [1]

    Flavor structures of charged fermions and massive neutrinos,

    Z. z. Xing, “Flavor structures of charged fermions and massive neutrinos,” Phys. Rept.854 (2020), 1-147 [arXiv:1909.09610 [hep-ph]]

  2. [2]

    Review of particle physics,

    S. Navaset al.[Particle Data Group], “Review of particle physics,” Phys. Rev. D110(2024) no.3, 030001

  3. [3]

    Baryon and Lepton Nonconserving Processes,

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

  4. [4]

    µ→eγat a rate of one out of 10 9 muon decays?,

    P. Minkowski, “µ→eγat a rate of one out of 10 9 muon decays?,” Phys. Lett.67B(1977) 421

  5. [5]

    The Effective Lagrangian for the Seesaw Model of Neutrino Mass and Leptogenesis

    A. Broncano, M. B. Gavela and E. E. Jenkins, “The Effective Lagrangian for the seesaw model of neutrino mass and leptogenesis,” Phys. Lett. B552(2003), 177-184 [erratum: Phys. Lett. B 636(2006), 332] [arXiv:hep-ph/0210271 [hep-ph]]

  6. [6]

    Unitarity of the Leptonic Mixing Matrix

    S. Antusch, C. Biggio, E. Fernandez-Martinez, M. B. Gavela and J. Lopez-Pavon, “Unitarity of the Leptonic Mixing Matrix,” JHEP10(2006), 084 [arXiv:hep-ph/0607020 [hep-ph]]. 9

  7. [7]

    Complete one-loop matching of the type-I seesaw model onto the Stan- dard Model effective field theory,

    D. Zhang and S. Zhou, “Complete one-loop matching of the type-I seesaw model onto the Stan- dard Model effective field theory,” JHEP09(2021), 163 [arXiv:2107.12133 [hep-ph]]

  8. [8]

    Neutrinos in particle physics, astronomy and cosmology,

    Z. z. Xing and S. Zhou, “Neutrinos in particle physics, astronomy and cosmology,” Springer Berlin, Heidelberg, 2011, ISBN 978-3-642-17559-6, 978-7-308-08024-8

  9. [9]

    Mesonium and anti-mesonium,

    B. Pontecorvo, “Mesonium and anti-mesonium,” Sov. Phys. JETP6(1957) 429 [Zh. Eksp. Teor. Fiz.33(1957) 549]

  10. [10]

    Remarks on the unified model of elementary particles,

    Z. Maki, M. Nakagawa and S. Sakata, “Remarks on the unified model of elementary particles,” Prog. Theor. Phys.28(1962) 870

  11. [11]

    Correlation between the Charged Current Interactions of Light and Heavy Majorana Neutrinos

    Z. z. Xing, “Correlation between the Charged Current Interactions of Light and Heavy Majorana Neutrinos,” Phys. Lett. B660(2008), 515-521 [arXiv:0709.2220 [hep-ph]]

  12. [12]

    A full parametrization of the 6 X 6 flavor mixing matrix in the presence of three light or heavy sterile neutrinos

    Z. z. Xing, “A full parametrization of the 6×6 flavor mixing matrix in the presence of three light or heavy sterile neutrinos,” Phys. Rev. D85(2012), 013008 [arXiv:1110.0083 [hep-ph]]

  13. [13]

    Confronting the seesaw mechanism with neutrino oscillations: A general and explicit analytical bridge,

    Z. z. Xing and J. y. Zhu, “Confronting the seesaw mechanism with neutrino oscillations: A general and explicit analytical bridge,” Nucl. Phys. B1018(2025), 117041 [arXiv:2412.17698 [hep-ph]]

  14. [14]

    The formal seesaw mechanism of Majorana neutrinos with unbroken gauge symme- try,

    Z. z. Xing, “The formal seesaw mechanism of Majorana neutrinos with unbroken gauge symme- try,” Nucl. Phys. B987(2023), 116106 [arXiv:2301.10461 [hep-ph]]

  15. [15]

    Emergent large flavor mixing from canonical and inverse seesaws?,

    Z. z. Xing, “Emergent large flavor mixing from canonical and inverse seesaws?,” Nucl. Phys. B 1013(2025), 116853 [arXiv:2502.09286 [hep-ph]]

  16. [16]

    Low-energy limits on heavy Majorana neutrino masses from the neutrinoless double-beta decay and non-unitary neutrino mixing

    Z. z. Xing, “Low-energy limits on heavy Majorana neutrino masses from the neutrinoless double- beta decay and non-unitary neutrino mixing,” Phys. Lett. B679(2009), 255-259 [arXiv:0907.3014 [hep-ph]]

  17. [17]

    On Non-Unitary Lepton Mixing and Neutrino Mass Observables

    W. Rodejohann, “On Non-Unitary Lepton Mixing and Neutrino Mass Observables,” Phys. Lett. B684(2010), 40-47 [arXiv:0912.3388 [hep-ph]]

  18. [18]

    Neutrinoless double beta decay in the minimal type-I seesaw model: mass-dependent nuclear matrix element, current limits and future sensitivities,

    D. L. Fang, Y. F. Li, Y. Y. Zhang and J. Y. Zhu, “Neutrinoless double beta decay in the minimal type-I seesaw model: mass-dependent nuclear matrix element, current limits and future sensitivities,” JHEP08(2024), 217 [arXiv:2404.12316 [hep-ph]]

  19. [19]

    Bounds on lepton non-unitarity and heavy neutrino mixing,

    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 neutrino mixing,” JHEP08(2023), 030 [arXiv:2306.01040 [hep-ph]]

  20. [20]

    Leptonic first-row correlation and unitarity waiting for further JUNO tests,

    Z. z. Xing, “Leptonic first-row correlation and unitarity waiting for further JUNO tests,” Sci. Bull.71(2026) no.8, 1899-1902 [arXiv:2510.17583 [hep-ph]]. 10

  21. [21]

    Commutator of the Quark Mass Matrices in the Standard Electroweak Model and a Measure of Maximal CP Nonconservation,

    C. Jarlskog, “Commutator of the Quark Mass Matrices in the Standard Electroweak Model and a Measure of Maximal CP Nonconservation,” Phys. Rev. Lett.55(1985), 1039

  22. [22]

    The Rephasing Invariants and CP,

    D. d. Wu, “The Rephasing Invariants and CP,” Phys. Rev. D33(1986), 860

  23. [23]

    Mapping the sources of CP violation in neutrino oscillations from the seesaw mech- anism,

    Z. z. Xing, “Mapping the sources of CP violation in neutrino oscillations from the seesaw mech- anism,” Phys. Lett. B856(2024), 138909 [arXiv:2406.01142 [hep-ph]]

  24. [24]

    Identifying a minimal flavor symmetry of the seesaw mechanism behind neutrino oscillations,

    Z. z. Xing, “Identifying a minimal flavor symmetry of the seesaw mechanism behind neutrino oscillations,” JHEP06(2022), 034 [arXiv:2203.14185 [hep-ph]]

  25. [25]

    Baryogenesis via leptogenesis,

    M. A. Luty, “Baryogenesis via leptogenesis,” Phys. Rev. D45(1992), 455-465

  26. [26]

    CP violating decays in leptogenesis scenarios

    L. Covi, E. Roulet and F. Vissani, “CP violating decays in leptogenesis scenarios,” Phys. Lett. B384(1996), 169-174 [arXiv:hep-ph/9605319 [hep-ph]]

  27. [27]

    CP violation in light neutrino oscillations and heavy neutrino decays: A general and explicit seesaw-bridged correlation,

    Z. z. Xing, “CP violation in light neutrino oscillations and heavy neutrino decays: A general and explicit seesaw-bridged correlation,” Phys. Lett. B844(2023), 138065 [arXiv:2306.02362 [hep-ph]]

  28. [28]

    Baryogenesis Without Grand Unification,

    M. Fukugita and T. Yanagida, “Baryogenesis Without Grand Unification,” Phys. Lett. B174 (1986), 45-47 11