NuFit-6.0: Updated global analysis of three-flavor neutrino oscillations
Pith reviewed 2026-05-14 18:42 UTC · model grok-4.3
The pith
The updated global analysis of neutrino oscillations shows nearly equal fits for both normal and inverted mass orderings, with Super-Kamiokande data providing the only notable preference for normal ordering.
A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.
Core claim
The global fit including long-baseline, reactor and IceCube atmospheric data results into an almost equally good fit for both orderings. Only when the χ² table for atmospheric neutrino data from Super-Kamiokande is added to our χ², the global fit prefers normal ordering with Δχ² = 6.1. The parameters θ12, θ13, Δm²21, and |Δm²3ℓ| (ℓ=1,2) are well-determined with relative precision at 3σ of about 13%, 8%, 15%, and 6%, respectively. The third mixing angle θ23 still suffers from the octant ambiguity. For normal ordering the global fit is consistent with CP conservation within 1σ, whereas for inverted ordering CP-violating values of δCP around 270° are favored at more than 3.6σ. Updated ranges on
What carries the argument
Global χ² minimization that combines disappearance and appearance data from long-baseline, reactor, atmospheric, and solar neutrino experiments to extract best-fit parameters and ordering preference.
If this is right
- T2K and NOvA appearance data individually favor normal ordering but are more consistent with each other for inverted ordering.
- The joint determination of |Δm²3ℓ| from global disappearance data prefers normal ordering.
- For inverted ordering, CP-violating values of δCP around 270° are favored against CP conservation at more than 3.6σ.
- Updated ranges and correlations are given for effective neutrino mass parameters relevant to β-decay, neutrinoless double-beta decay, and cosmology.
Where Pith is reading between the lines
- The reduced discrimination power between orderings stems from opposing tendencies across different classes of datasets.
- Resolving the ordering will require dedicated next-generation long-baseline experiments to break the current near-degeneracy.
- These results provide tighter inputs for model-building that links neutrino mass generation to other beyond-Standard-Model phenomena.
Load-bearing premise
The analysis assumes that all included experimental datasets are free of unaccounted systematic uncertainties and that the three-flavor oscillation framework remains valid without additional physics.
What would settle it
A high-statistics result from a next-generation experiment such as DUNE or Hyper-Kamiokande that shows a strong preference for one ordering at several sigma would test whether the current near-degeneracy between orderings persists.
read the original abstract
We present an updated global analysis of neutrino oscillation data as of September 2024. The parameters $\theta_{12}$, $\theta_{13}$, $\Delta m^2_{21}$, and $|\Delta m^2_{3\ell}|$ ($\ell = 1,2$) are well-determined with relative precision at $3\sigma$ of about 13\%, 8\%, 15\%, and 6\%, respectively. The third mixing angle $\theta_{23}$ still suffers from the octant ambiguity, with no clear indication of whether it is larger or smaller than $45^\circ$. The determination of the leptonic CP phase $\delta_{CP}$ depends on the neutrino mass ordering: for normal ordering the global fit is consistent with CP conservation within $1\sigma$, whereas for inverted ordering CP-violating values of $\delta_{CP}$ around $270^\circ$ are favored against CP conservation at more than $3.6\sigma$. While the present data has in principle $2.5$--$3\sigma$ sensitivity to the neutrino mass ordering, there are different tendencies in the global data that reduce the discrimination power: T2K and NOvA appearance data individually favor normal ordering, but they are more consistent with each other for inverted ordering. Conversely, the joint determination of $|\Delta m^2_{3\ell}|$ from global disappearance data prefers normal ordering. Altogether, the global fit including long-baseline, reactor and IceCube atmospheric data results into an almost equally good fit for both orderings. Only when the $\chi^2$ table for atmospheric neutrino data from Super-Kamiokande is added to our $\chi^2$, the global fit prefers normal ordering with $\Delta\chi^2 = 6.1$. We provide also updated ranges and correlations for the effective parameters sensitive to the absolute neutrino mass from $\beta$-decay, neutrinoless double-beta decay, and cosmology.
Editorial analysis
A structured set of objections, weighed in public.
Referee Report
Summary. The manuscript presents NuFit-6.0, an updated global analysis of three-flavor neutrino oscillation data as of September 2024. It reports 3σ relative precisions of ~13%, 8%, 15%, and 6% on θ12, θ13, Δm²21, and |Δm²3ℓ|, respectively, notes the persistent octant ambiguity in θ23, and finds that δCP is consistent with CP conservation within 1σ for normal ordering but favors CP-violating values near 270° at >3.6σ for inverted ordering. The global fit to long-baseline, reactor, and IceCube atmospheric data yields nearly equal χ² for both orderings, while adding the Super-Kamiokande atmospheric χ² table produces a Δχ²=6.1 preference for normal ordering; updated ranges for effective mass parameters from β-decay, 0νββ, and cosmology are also given.
Significance. This is a timely and valuable update to the global neutrino oscillation fit. The transparent reporting of dataset tensions (e.g., T2K/NOvA appearance vs. disappearance constraints on |Δm²3ℓ|), explicit Δχ² values, and inclusion of IceCube data strengthen the result. Such global fits are central to the field and directly inform experimental planning and theoretical interpretations.
minor comments (3)
- [Abstract and § on mass ordering] In the abstract and results section, the quoted 2.5–3σ sensitivity to mass ordering should be accompanied by a brief statement of the exact test statistic and degrees of freedom used to derive it.
- [Figures showing Δχ² vs. ordering] Figure captions for the Δχ² profiles versus ordering should explicitly note whether the profiles are minimized over all other parameters or profiled in a specific way.
- [Section on effective mass parameters] The correlation matrices or tables for the effective mass parameters (mβ, mββ, Σ) should include the numerical values of the off-diagonal correlations for completeness.
Simulated Author's Rebuttal
We thank the referee for the careful review and the recommendation to accept the manuscript. The provided summary accurately captures the main results and the transparent discussion of dataset tensions in our NuFit-6.0 global analysis.
Circularity Check
No significant circularity; direct global fit to external data
full rationale
The manuscript performs a standard χ² minimization over neutrino oscillation parameters using independent experimental datasets (long-baseline accelerators, reactors, atmospheric neutrinos from IceCube and Super-Kamiokande). All reported results, including the Δχ² = 6.1 preference for normal ordering upon inclusion of the Super-Kamiokande table, are obtained by direct comparison of the global χ² surfaces for the two mass orderings; no parameter is defined in terms of the target observable, no fitted input is relabeled as a prediction, and no load-bearing step reduces to a self-citation or prior ansatz. The three-flavor framework and dataset independence assumptions are stated explicitly and are standard external inputs, leaving the derivation self-contained against the supplied data.
Axiom & Free-Parameter Ledger
free parameters (1)
- oscillation parameters
axioms (1)
- domain assumption Three-flavor neutrino mixing is complete and valid
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Reference graph
Works this paper leans on
-
[1]
I. Esteban, M.C. Gonzalez-Garcia, M. Maltoni, T. Schwetz and A. Zhou,The fate of hints: updated global analysis of three-flavor neutrino oscillations,JHEP09(2020) 178 [2007.14792]
-
[2]
2020 Global reassessment of the neutrino oscillation picture
P. de Salas, D. Forero, S. Gariazzo, P. Martinez-Mirave, O. Mena, C. Ternes et al.,2020 Global Reassessment of the Neutrino Oscillation Picture,2006.11237
work page internal anchor Pith review arXiv 2020
-
[3]
Current unknowns in the three neutrino framework
F. Capozzi, E. Lisi, A. Marrone and A. Palazzo,Current Unknowns in the Three Neutrino Framework,Prog. Part. Nucl. Phys.102(2018) 48 [1804.09678]. [7]JUNOcollaboration,Potential to Identify the Neutrino Mass Ordering with Reactor Antineutrinos in JUNO,2405.18008. [8]DUNEcollaboration,Long-baseline neutrino oscillation physics potential of the DUNE experime...
work page internal anchor Pith review Pith/arXiv arXiv 2018
-
[4]
Standard Solar Models B23/SF-III,
Y. Herrera and A. Serenelli,Standard Solar Models B23 / SF-III, 2023. ZENODO, https://doi.org/10.5281/zenodo.10174170. [11]Super-Kamiokandecollaboration,Solar neutrino measurements using the full data period of Super-Kamiokande-IV,2312.12907. [12]Borexinocollaboration,First Simultaneous Precision Spectroscopy ofpp, 7Be, andpep Solar Neutrinos with Borexin...
-
[5]
I. Esteban, M.C. Gonzalez-Garcia, A. Hernandez-Cabezudo, M. Maltoni and T. Schwetz, Global analysis of three-flavour neutrino oscillations: synergies and tensions in the determination ofθ 23,δ CP, and the mass ordering,JHEP01(2019) 106 [1811.05487]
work page internal anchor Pith review Pith/arXiv arXiv 2019
-
[6]
Z. Maki, M. Nakagawa and S. Sakata,Remarks on the unified model of elementary particles, Prog. Theor. Phys.28(1962) 870
work page 1962
-
[7]
M. Kobayashi and T. Maskawa,CP Violation in the Renormalizable Theory of Weak Interaction,Prog. Theor. Phys.49(1973) 652
work page 1973
-
[8]
Cabibbo,Time Reversal Violation in Neutrino Oscillation,Phys
N. Cabibbo,Time Reversal Violation in Neutrino Oscillation,Phys. Lett.72B(1978) 333
work page 1978
-
[9]
S.M. Bilenky, J. Hosek and S.T. Petcov,On Oscillations of Neutrinos with Dirac and Majorana Masses,Phys. Lett.B94(1980) 495
work page 1980
- [10]
-
[11]
P. Langacker, S.T. Petcov, G. Steigman and S. Toshev,On the Mikheev-Smirnov-Wolfenstein (MSW) Mechanism of Amplification of Neutrino Oscillations in Matter,Nucl. Phys.B282 (1987) 589
work page 1987
- [12]
-
[13]
Three-Neutrino Mixing after the First Results from K2K and KamLAND
M.C. Gonzalez-Garcia and C. Pena-Garay,Three neutrino mixing after the first results from K2K and KamLAND,Phys. Rev.D68(2003) 093003 [hep-ph/0306001]. – 29 –
work page internal anchor Pith review Pith/arXiv arXiv 2003
-
[14]
P.I. Krastev and S.T. Petcov,Resonance Amplification and t Violation Effects in Three Neutrino Oscillations in the Earth,Phys. Lett.B205(1988) 84
work page 1988
-
[15]
C. Jarlskog,Commutator of the Quark Mass Matrices in the Standard Electroweak Model and a Measure of Maximal CP Violation,Phys.Rev.Lett.55(1985) 1039. [36]Particle Data Groupcollaboration,Review of particle physics,Phys. Rev. D110(2024) 030001
work page 1985
-
[16]
On the determination of the leptonic CP phase
J. Elevant and T. Schwetz,On the determination of the leptonic CP phase,JHEP09(2015) 016 [1506.07685]
work page internal anchor Pith review Pith/arXiv arXiv 2015
-
[17]
Wolfenstein,Neutrino oscillations in matter,Phys
L. Wolfenstein,Neutrino oscillations in matter,Phys. Rev.D17(1978) 2369
work page 1978
-
[18]
Testing the statistical compatibility of independent data sets
M. Maltoni and T. Schwetz,Testing the Statistical Compatibility of Independent Data Sets, Phys. Rev.D68(2003) 033020 [hep-ph/0304176]
work page internal anchor Pith review Pith/arXiv arXiv 2003
-
[19]
Another possible way to determine the Neutrino Mass Hierarchy
H. Nunokawa, S.J. Parke and R. Zukanovich Funchal,Another Possible Way to Determine the Neutrino Mass Hierarchy,Phys. Rev.D72(2005) 013009 [hep-ph/0503283]
work page internal anchor Pith review Pith/arXiv arXiv 2005
-
[20]
H. Minakata, H. Nunokawa, S.J. Parke and R. Zukanovich Funchal,Determining Neutrino Mass Hierarchy by Precision Measurements in Electron and Muon Neutrino Disappearance Experiments,Phys. Rev.D74(2006) 053008 [hep-ph/0607284]
work page internal anchor Pith review Pith/arXiv arXiv 2006
-
[21]
Determination of the neutrino mass ordering by combining PINGU and Daya Bay II
M. Blennow and T. Schwetz,Determination of the Neutrino Mass Ordering by Combining Pingu and Daya Bay II,JHEP09(2013) 089 [1306.3988]
work page internal anchor Pith review Pith/arXiv arXiv 2013
-
[22]
Quantifying the sensitivity of oscillation experiments to the neutrino mass ordering
M. Blennow, P. Coloma, P. Huber and T. Schwetz,Quantifying the sensitivity of oscillation experiments to the neutrino mass ordering,JHEP03(2014) 028 [1311.1822]
work page internal anchor Pith review Pith/arXiv arXiv 2014
-
[23]
X. Qian, A. Tan, W. Wang, J.J. Ling, R.D. McKeown and C. Zhang,Statistical Evaluation of Experimental Determinations of Neutrino Mass Hierarchy,Phys. Rev. D86(2012) 113011 [1210.3651]. [45]Super-Kamiokandecollaboration,Solar neutrino measurements in Super-Kamiokande-II, Phys. Rev.D78(2008) 032002 [0803.4312]
work page internal anchor Pith review Pith/arXiv arXiv 2012
-
[24]
N. Grevesse and A.J. Sauval,Standard Solar Composition,Space Sci. Rev.85(1998) 161
work page 1998
-
[25]
The chemical composition of the Sun
M. Asplund, N. Grevesse, A.J. Sauval and P. Scott,The Chemical Composition of the Sun, ARA&A47(2009) 481 [0909.0948]
work page internal anchor Pith review Pith/arXiv arXiv 2009
-
[26]
New Solar Composition: The Problem With Solar Models Revisited
A. Serenelli, S. Basu, J.W. Ferguson and M. Asplund,New Solar Composition: The Problem With Solar Models Revisited,Astrophys. J.705(2009) L123 [0909.2668]
work page internal anchor Pith review Pith/arXiv arXiv 2009
-
[27]
Solar models with accretion. I. Application to the solar abundance problem
A.M. Serenelli, W.C. Haxton and C. Pena-Garay,Solar models with accretion. I. Application to the solar abundance problem,Astrophys. J.743(2011) 24 [1104.1639]
work page internal anchor Pith review Pith/arXiv arXiv 2011
-
[28]
A new Generation of Standard Solar Models
N. Vinyoles, A.M. Serenelli, F.L. Villante, S. Basu, J. Bergström, M.C. Gonzalez-Garcia et al.,A new Generation of Standard Solar Models,Astrophys. J.835(2017) 202 [1611.09867]
work page internal anchor Pith review Pith/arXiv arXiv 2017
-
[29]
The chemical make-up of the Sun: A 2020 vision
M. Asplund, A.M. Amarsi and N. Grevesse,The chemical make-up of the Sun: A 2020 vision,arXiv e-prints(2021) arXiv:2105.01661 [2105.01661]
work page internal anchor Pith review arXiv 2020
-
[30]
Magg et al.,Observational constraints on the origin of the elements - IV
E. Magg et al.,Observational constraints on the origin of the elements - IV. Standard composition of the Sun,Astron. Astrophys.661(2023) A140 [2203.02255]
-
[31]
M.C. Gonzalez-Garcia, M. Maltoni, J.a.P. Pinheiro and A.M. Serenelli,Status of direct determination of solar neutrino fluxes after Borexino,JHEP02(2024) 064 [2311.16226]. – 30 – [54]Katrincollaboration,Direct neutrino-mass measurement based on 259 days of KATRIN data,2406.13516. [55]GERDAcollaboration,Final Results of GERDA on the Search for Neutrinoless ...
- [32]
-
[33]
D. Naredo-Tuero, M. Escudero, E. Fernández-Martínez, X. Marcano and V. Poulin,Living at the Edge: A Critical Look at the Cosmological Neutrino Mass Bound,2407.13831. [59]DESIcollaboration,DESI 2024 VI: Cosmological Constraints from the Measurements of Baryon Acoustic Oscillations,2404.03002
-
[34]
G.L. Fogli, E. Lisi, A. Marrone, A. Melchiorri, A. Palazzo, P. Serra et al.,Observables sensitive to absolute neutrino masses: Constraints and correlations from world neutrino data, Phys. Rev.D70(2004) 113003 [hep-ph/0408045]
work page internal anchor Pith review Pith/arXiv arXiv 2004
-
[35]
S. Pascoli, S.T. Petcov and T. Schwetz,The Absolute Neutrino Mass Scale, Neutrino Mass Spectrum, Majorana Cp-Violation and Neutrinoless Double-Beta Decay,Nucl. Phys.B734 (2006) 24 [hep-ph/0505226]
work page internal anchor Pith review Pith/arXiv arXiv 2006
-
[36]
S. Gariazzo et al.,Neutrino mass and mass ordering: no conclusive evidence for normal ordering,JCAP10(2022) 010 [2205.02195]
-
[37]
B.T. Cleveland et al.,Measurement of the solar electron neutrino flux with the Homestake chlorine detector,Astrophys. J.496(1998) 505
work page 1998
-
[38]
Reanalysis of the GALLEX solar neutrino flux and source experiments
F. Kaether, W. Hampel, G. Heusser, J. Kiko and T. Kirsten,Reanalysis of the GALLEX solar neutrino flux and source experiments,Phys. Lett.B685(2010) 47 [1001.2731]. [65]SAGEcollaboration,Measurement of the solar neutrino capture rate with gallium metal. III: Results for the 2002–2007 data-taking period,Phys. Rev.C80(2009) 015807 [0901.2200]. [66]Super-Kami...
work page internal anchor Pith review Pith/arXiv arXiv 2010
-
[39]
Atmospheric neutrino flux calculation using the NRLMSISE00 atmospheric model
M. Honda, M. Sajjad Athar, T. Kajita, K. Kasahara and S. Midorikawa,Atmospheric Neutrino Flux Calculation Using the Nrlmsise-00 Atmospheric Model,Phys. Rev.D92 (2015) 023004 [1502.03916]. – 31 – [72]KamLANDcollaboration,Reactor On-Off Antineutrino Measurement with Kamland,Phys. Rev.D88(2013) 033001 [1303.4667]
work page internal anchor Pith review Pith/arXiv arXiv 2015
-
[40]
New Results from the Double Chooz Experiment
T. Bezerra, “New Results from the Double Chooz Experiment.” Talk given at theXXIX International Conference on Neutrino Physics and Astrophysics, Chicago, USA, June 22–July 2, 2020 (online conference) doi.org/10.5281/zenodo.3959542
-
[41]
J. Yoo, “RENO.” Talk given at theXXIX International Conference on Neutrino Physics and Astrophysics, Chicago, USA, June 22–July 2, 2020 (online conference) doi.org/10.5281/zenodo.3959698. [75]MINOScollaboration,Measurement of Neutrino and Antineutrino Oscillations Using Beam and Atmospheric Data in MINOS,Phys. Rev. Lett.110(2013) 251801 [1304.6335]. [76]M...
work page internal anchor Pith review Pith/arXiv arXiv doi:10.5281/zenodo.3959698 2020
-
[42]
New Oscillation Results from the NOvA Experiment,
A. Himmel, “New Oscillation Results from the NOvA Experiment.” Talk given at theXXIX International Conference on Neutrino Physics and Astrophysics, Chicago, USA, June 22–July 2, 2020 (online conference) doi.org/10.5281/zenodo.3959581. [80]IceCubecollaboration,IceCube 3 year high statistics neutrino oscillation samples, 2019. 10.21234/AC23-RA43. – 32 –
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