Neutrino oscillation data and a pseudo-Dirac heavy neutral lepton
Pith reviewed 2026-06-29 03:12 UTC · model grok-4.3
The pith
Light neutrino oscillation data fixes an ellipse in the flavour simplex for active-heavy mixing in the minimal pseudo-Dirac HNL model.
A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.
Core claim
In the minimal pseudo-Dirac HNL scenario, exact diagonalization of the lepton-number conserving Dirac limit followed by perturbative inclusion of the violating entries yields a symmetry-protected flavour reconstruction of the active-heavy interaction matrix. The rank-two light-neutrino mass matrix fixes the normalised active-flavour direction, while the remaining high-energy information reduces to a single complex light-heavy amplitude. For the normalised leading active-heavy interaction weights, this amplitude and the heavy-sector rotation cancel, leaving an ellipse in the flavour simplex determined by light-neutrino oscillation data and the Majorana phase.
What carries the argument
the ellipse in the flavour simplex determined by light-neutrino oscillation data and the Majorana phase, obtained after exact diagonalization of the LN-conserving limit and perturbative treatment of LN-violating terms
If this is right
- The rank-two light-neutrino mass matrix fixes the normalised active-flavour direction in the interaction matrix.
- The remaining high-energy information is a single complex light-heavy amplitude whose phase defines a CP-odd light-heavy invariant.
- Linear LN-violating terms enter coherent heavy-neutrino oscillations.
- The neutrinoless double beta effective mass receives contributions from the linear LN-violating terms.
Where Pith is reading between the lines
- Collider searches for HNLs could test whether observed mixing ratios fall on the ellipse predicted by oscillation data.
- A measured value of the Majorana phase would directly constrain the shape and orientation of the ellipse.
- The cancellation between amplitude and rotation may appear in other symmetry-protected models with additional HNL pairs.
Load-bearing premise
The lepton-number violating entries are small enough to be treated perturbatively after exact diagonalization of the conserving limit, and the model contains exactly one pseudo-Dirac HNL pair.
What would settle it
Observation of a heavy neutral lepton decay whose active-flavour mixing ratios lie outside the ellipse fixed by current neutrino oscillation data and the Majorana phase.
read the original abstract
Symmetry-protected seesaw models can accommodate light-neutrino oscillation data while keeping heavy neutral leptons (HNLs) within collider reach. In these models, the smallness of the light-neutrino masses is protected by an approximate lepton number (LN)-like symmetry that is broken only by small parameters. We study the minimal scenario in which the new states form one pseudo-Dirac HNL pair. The exact LN-conserving Dirac limit is diagonalised without expanding in the active-sterile mixing, and the small LN-violating entries are then included perturbatively. This yields a symmetry-protected flavour reconstruction of the active-heavy interaction matrix. The rank-two light-neutrino mass matrix fixes the normalised active-flavour direction, while the remaining high-energy information is a single complex light-heavy amplitude whose phase defines a CP-odd light-heavy invariant. For the normalised leading active-heavy interaction weights, this amplitude and the heavy-sector rotation cancel, leaving an ellipse in the flavour simplex determined by light-neutrino oscillation data and the Majorana phase. We also identify how the linear LN-violating terms enter coherent heavy-neutrino oscillations and the neutrinoless double beta effective mass.
Editorial analysis
A structured set of objections, weighed in public.
Referee Report
Summary. The paper claims that symmetry-protected seesaw models with one pseudo-Dirac HNL pair allow exact diagonalization of the lepton-number conserving Dirac limit, after which small LN-violating entries are added perturbatively. This produces a symmetry-protected flavour reconstruction in which the rank-two light-neutrino mass matrix fixes the normalised active-flavour direction; the remaining information is a single complex light-heavy amplitude whose phase is a CP-odd invariant. For the normalised leading active-heavy interaction weights, this amplitude and the heavy-sector rotation cancel, leaving an ellipse in the flavour simplex fixed solely by light-neutrino oscillation data and the Majorana phase. The work also identifies how linear LN-violating terms enter coherent heavy-neutrino oscillations and the neutrinoless double-beta effective mass.
Significance. If the claimed cancellation survives the perturbative LN-violating corrections without shifting the leading normalised direction, the result supplies a direct, largely parameter-free link between oscillation parameters and HNL flavour structure. This would be useful for collider phenomenology and 0νββ predictions in symmetry-protected seesaws. The exact (non-expanded) diagonalization of the conserving limit is a methodological strength that avoids uncontrolled approximations in the active-sterile mixing.
major comments (1)
- [flavour reconstruction / perturbative LN-violating block] The central ellipse result (abstract and the flavour-reconstruction section) rests on the statement that, after exact LN-conserving diagonalization, the small LN-violating block does not modify the leading normalised active-heavy weights at the same order as the claimed cancellation. This assumption is load-bearing: if O(ε) corrections shift the direction of the normalised mixing vector, the amplitude-rotation cancellation would no longer leave an ellipse determined only by external oscillation data. An explicit order-by-order expansion of the normalised weights (or a symmetry argument showing the corrections vanish) is required to substantiate the claim.
minor comments (2)
- The abstract refers to 'the remaining high-energy information is a single complex light-heavy amplitude'; an explicit definition of this amplitude in terms of the mixing-matrix elements, together with its relation to the Majorana phase, would improve readability.
- The restriction to exactly one pseudo-Dirac pair is stated as part of the minimal scenario; a brief remark on why the rank-two light mass matrix would not fix a unique direction for two or more pairs would clarify the scope.
Simulated Author's Rebuttal
We thank the referee for the careful reading and for identifying a load-bearing assumption in the flavour-reconstruction argument. We address the single major comment below.
read point-by-point responses
-
Referee: [flavour reconstruction / perturbative LN-violating block] The central ellipse result (abstract and the flavour-reconstruction section) rests on the statement that, after exact LN-conserving diagonalization, the small LN-violating block does not modify the leading normalised active-heavy weights at the same order as the claimed cancellation. This assumption is load-bearing: if O(ε) corrections shift the direction of the normalised mixing vector, the amplitude-rotation cancellation would no longer leave an ellipse determined only by external oscillation data. An explicit order-by-order expansion of the normalised weights (or a symmetry argument showing the corrections vanish) is required to substantiate the claim.
Authors: We agree that an explicit verification is required. The symmetry-protected construction fixes the leading normalised active-heavy direction in the exact LN-conserving limit; the subsequent perturbative inclusion of the LN-violating block modifies the overall mixing matrix at O(ε), but the normalised vector itself receives corrections only at O(ε²) because the leading eigenvector is protected by the rank-two light-neutrino mass matrix and the residual symmetry. Nevertheless, to make this transparent we will add an appendix containing the order-by-order expansion of the normalised weights through O(ε). This will confirm that the amplitude-rotation cancellation remains intact at the order relevant for the ellipse and that the result is determined solely by oscillation data and the Majorana phase. revision: yes
Circularity Check
No significant circularity; ellipse fixed by external oscillation data after exact LN-conserving diagonalization
full rationale
The derivation diagonalizes the LN-conserving limit exactly, then adds small LN-violating terms perturbatively. The central claim states that the normalised active-heavy weights are fixed by the rank-two light mass matrix from oscillation data plus the Majorana phase, with amplitude and rotation cancelling. No quoted equation reduces this output to a fitted parameter or self-citation by construction. The restriction to one pseudo-Dirac pair is an explicit model choice, not a hidden redefinition. Self-citation load-bearing is absent from the provided abstract and reader's summary. This is the normal case of an independent derivation from external data.
Axiom & Free-Parameter Ledger
axioms (1)
- domain assumption Approximate lepton number symmetry protects light neutrino masses and is broken only by small parameters
Reference graph
Works this paper leans on
-
[1]
Evidence for oscillation of atmospheric neutrinos
Super-Kamiokande. ‘Evidence for oscillation of atmospheric neutrinos’. In:Phys. Rev. Lett. 81(1998), pp.1562–1567.doi: 10.1103/PhysRevLett.81.1562. arXiv: hep-ex/9807003. №:BU-98-17,ICRR-REPORT-422-98-18,UCI-98-8,KEK-PREPRINT-98-95,LSU- HEPA-5-98,UMD-98-003,SBHEP-98-5,TKU-PAP-98-06, andTIT-HPE-98-09
work page internal anchor Pith review Pith/arXiv arXiv doi:10.1103/physrevlett.81.1562 1998
-
[2]
SNO. ‘Direct evidence for neutrino flavor transformation from neutral current interactions in the Sudbury Neutrino Observatory’. In:Phys. Rev. Lett.89(2002), p.11301.doi: 10.1103/PhysRevLett.89.011301. arXiv: nucl-ex/0204008
work page internal anchor Pith review Pith/arXiv arXiv doi:10.1103/physrevlett.89.011301 2002
-
[3]
First Results from KamLAND: Evidence for Reactor Anti-Neutrino Disappearance
KamLAND. ‘First results from KamLAND: Evidence for reactor anti-neutrino disappear- ance’. In:Phys. Rev. Lett.90(2003), p.21802.doi: 10.1103/PhysRevLett.90.021802. arXiv: hep-ex/0212021
work page internal anchor Pith review Pith/arXiv arXiv doi:10.1103/physrevlett.90.021802 2003
-
[4]
Evidence for muon neutrino oscillation in an accelerator-based experiment
K2K. ‘Evidence for muon neutrino oscillation in an accelerator-based experiment’. In: Phys. Rev. Lett.94(2005), p.81802.doi: 10.1103/PhysRevLett.94.081802. arXiv: hep-ex/0411038
work page internal anchor Pith review Pith/arXiv arXiv doi:10.1103/physrevlett.94.081802 2005
-
[5]
‘Observation of muon neutrino disappearance with the MINOS detectors and the NuMI neutrino beam’
MINOS. ‘Observation of muon neutrino disappearance with the MINOS detectors and the NuMI neutrino beam’. In:Phys. Rev. Lett.97(2006), p.191801.doi: 10.1103/ PhysRevLett.97.191801. arXiv: hep-ex/0607088.№:FERMILAB-PUB-06-243and BNL-76806-2006-JA
Pith/arXiv arXiv 2006
-
[6]
T2K. ‘Measurements of neutrino oscillation in appearance and disappearance channels by the T2K experiment with6.6×1020 protons on target’. In:Phys. Rev. D91.7(2015), p. 72010.doi: 10.1103/PhysRevD.91.072010. arXiv: 1502.01550[hep-ex]
work page internal anchor Pith review Pith/arXiv arXiv doi:10.1103/physrevd.91.072010 2015
-
[7]
S. Weinberg. ‘Baryon and Lepton Nonconserving Processes’. In:Phys. Rev. Lett.43(1979), pp.1566–1570.doi: 10.1103/PhysRevLett.43.1566.№:HUTP-79-A050
-
[8]
P. Minkowski. ‘µ→eγat a Rate of One Out of109 Muon Decays?’ In:Phys. Lett. B67 (1977), pp.421–428.doi:10.1016/0370-2693(77)90435-X.№:Print-77-0182(BERN). 31
-
[9]
Yanagida
T. Yanagida. ‘Horizontal gauge symmetry and masses of neutrinos’. In:Conf. Proc. C 7902131(1979). Ed. by O. Sawada and A. Sugamoto, pp.95–99.№:KEK-79-18-95
1979
-
[10]
M. Gell-Mann, P. Ramond, and R. Slansky. ‘Complex Spinors and Unified Theor- ies’. In:Conf. Proc. C790927(1979), pp.315–321. arXiv: 1306.4669[hep-th] .№: PRINT-80-0576
Pith/arXiv arXiv 1979
-
[11]
S. L. Glashow. ‘The Future of Elementary Particle Physics’. In:NATO Sci. Ser. B61 (1980). Ed. by M. Lévy, J.-L. Basdevant, D. Speiser, J. Weyers, R. Gastmans, and M. Jacob, p.687.doi: 10.1007/978-1-4684-7197-7_15.№:HUTP-79-A059
-
[12]
J. Schechter and J. W. F. Valle. ‘Neutrino Masses in SU(2)×U(1)Theories’. In: Phys. Rev. D22(1980), p.2227.doi: 10.1103/PhysRevD.22.2227.№:SU-4217- 167andCOO-3533-167
-
[13]
R. N. Mohapatra and G. Senjanovic. ‘Neutrino Mass and Spontaneous Parity Nonconser- vation’. In:Phys. Rev. Lett.44(1980), p.912.doi: 10.1103/PhysRevLett.44.912.№: MDDP-TR-80-060,MDDP-PP-80-105, andCCNY-HEP-79-10
-
[14]
J. Kersten and A. Y. Smirnov. ‘Right-Handed Neutrinos at CERN LHC and the Mechanism of Neutrino Mass Generation’. In:Phys. Rev. D76(2007), p.73005.doi: 10.1103/ PhysRevD.76.073005. arXiv: 0705.3221[hep-ph]
Pith/arXiv arXiv 2007
-
[15]
D. Wyler and L. Wolfenstein. ‘Massless Neutrinos in Left-Right Symmetric Models’. In:Nucl. Phys. B218(1983), pp.205–214.doi: 10.1016/0550-3213(83)90482-0. №:CERN-TH-3435
-
[16]
R. N. Mohapatra and J. W. F. Valle. ‘Neutrino Mass and Baryon Number Noncon- servation in Superstring Models’. In:Phys. Rev. D34(1986), p.1642.doi: 10.1103/ PhysRevD.34.1642.№:MdDP-PP-86-127
1986
-
[17]
R. N. Mohapatra. ‘Mechanism for Understanding Small Neutrino Mass in Superstring Theories’. In:Phys. Rev. Lett.56(1986), pp.561–563.doi:10.1103/PhysRevLett.56.561
-
[18]
S. Nandi and U. Sarkar. ‘A Solution to the Neutrino Mass Problem in SuperstringE6 Theory’. In:Phys. Rev. Lett.56(1986), p.564.doi: 10.1103/PhysRevLett.56.564. №:DOE-ER40200-036
-
[19]
E. K. Akhmedov, M. Lindner, E. Schnapka, and J. W. F. Valle. ‘Left-right symmetry breaking in NJL approach’. In:Phys. Lett. B368(1996), pp.270–280.doi: 10.1016/ 0370-2693(95)01504-3 . arXiv: hep-ph/9507275.№:IC-95-125,TUM-HEP-221-95, MPI-PHT-95-35,FTUV-95-34, andIFIC-95-36
Pith/arXiv arXiv 1996
-
[21]
Novel Supersymmetric SO(10) Seesaw Mechanism
M. Malinsky, J. C. Romao, and J. W. F. Valle. ‘Novel supersymmetric SO(10) seesaw mechanism’. In:Phys. Rev. Lett.95(2005), p.161801.doi: 10.1103/PhysRevLett.95. 161801. arXiv: hep-ph/0506296.№:IFIC-05-28
work page internal anchor Pith review Pith/arXiv arXiv doi:10.1103/physrevlett.95 2005
-
[22]
S. Antusch and O. Fischer. ‘Testing sterile neutrino extensions of the Standard Model at future lepton colliders’. In:JHEP05(2015), p.53.doi: 10.1007/JHEP05(2015)
-
[23]
arXiv: 1502.05915[hep-ph] .№:MPP-2015-24. 32
Pith/arXiv arXiv 2015
-
[24]
S. Antusch, J. Hajer, and J. Rosskopp. ‘Simulating lepton number violation induced by heavy neutrino-antineutrino oscillations at colliders’. In:JHEP03(2023), p.110.doi: 10.1007/JHEP03(2023)110. arXiv: 2210.10738[hep-ph]
-
[25]
H. E. Haber. ‘A tale of three diagonalizations’. In:Int. J. Mod. Phys. A36.04(2021), p. 2130003.doi: 10.1142/S0217751X21300027. arXiv: 2009.03990[hep-ph]
-
[26]
M. B. Gavela, T. Hambye, D. Hernandez, and P. Hernandez. ‘Minimal Flavour Seesaw Models’. In:JHEP09(2009), p.38.doi: 10.1088/1126-6708/2009/09/038. arXiv: 0906.1461[hep-ph] .№:FTUAM-09-09,IFT-UAM-CSIC-09-27,ULB-TH-09-15, IFIC-09-22, andFTUV-09-0607
work page internal anchor Pith review Pith/arXiv arXiv doi:10.1088/1126-6708/2009/09/038 2009
-
[27]
J. A. Casas and A. Ibarra. ‘Oscillating neutrinos andµ→eγ’. In:Nucl. Phys. B618 (2001), pp.171–204.doi: 10.1016/S0550-3213(01)00475-8. arXiv: hep-ph/0103065. №:IEM-FT-211-01,OUTP-01-11P, andIFT-UAM-CSIC-01-08
work page internal anchor Pith review Pith/arXiv arXiv doi:10.1016/s0550-3213(01)00475-8 2001
-
[28]
Z.-z. Xing. ‘Casas-Ibarra Parametrization and Unflavored Leptogenesis’. In:Chin. Phys. C 34(2010), pp.1–6.doi: 10.1088/1674-1137/34/1/001. arXiv: 0902.2469[hep-ph]
work page internal anchor Pith review Pith/arXiv arXiv doi:10.1088/1674-1137/34/1/001 2010
-
[29]
Master Majorana neutrino mass parametrization
I. Cordero-Carrión, M. Hirsch, and A. Vicente. ‘Master Majorana neutrino mass parametriz- ation’. In:Phys. Rev. D99.7(2019), p.75019.doi: 10.1103/PhysRevD.99.075019. arXiv: 1812.03896[hep-ph] .№:IFIC/18-46
work page internal anchor Pith review Pith/arXiv arXiv doi:10.1103/physrevd.99.075019 2019
-
[30]
I. Cordero-Carrión, M. Hirsch, and A. Vicente. ‘General parametrization of Majorana neutrino mass models’. In:Phys. Rev. D101.7(2020), p.75032.doi: 10.1103/PhysRevD. 101.075032. arXiv: 1912.08858[hep-ph] .№:IFIC/19-59
-
[31]
J. Herrero-García, S. Marciano, J. Racker, and D. Vatsyayan. ‘Generalized Casas-Ibarra parametrization for Majorana neutrino masses’. In:Phys. Rev. D113.3(2026), p.35035. doi: 10.1103/d38p-m3sj. arXiv: 2510.18962[hep-ph]
-
[32]
NuFit-6.0: Updated global analysis of three-flavor neutrino oscillations
I. Esteban, M. C. Gonzalez-Garcia, M. Maltoni, I. Martinez-Soler, J. P. Pinheiro, and T. Schwetz. ‘NuFit6.0: updated global analysis of three-flavor neutrino oscillations’. In: JHEP12(2024), p.216.doi: 10.1007/JHEP12(2024)216. arXiv: 2410.05380[hep-ph] . №:IFT-UAM/CSIC-24-140,YITP-SB-2024-24,IPPP/24/64,IPPP/24/64,IFT- UAM/CSIC-24-140, andYITP-SB-2024-24. ...
work page internal anchor Pith review Pith/arXiv arXiv doi:10.1007/jhep12(2024)216 2024
-
[33]
The seesaw portal in testable models of neutrino masses
A. Caputo, P. Hernandez, J. Lopez-Pavon, and J. Salvado. ‘The seesaw portal in testable models of neutrino masses’. In:JHEP06(2017), p.112.doi: 10.1007/JHEP06(2017)112. arXiv: 1704.08721[hep-ph]
work page internal anchor Pith review Pith/arXiv arXiv doi:10.1007/jhep06(2017)112 2017
-
[34]
M. Drewes, J. Hajer, J. Klaric, and G. Lanfranchi. ‘NA62sensitivity to heavy neutral leptons in the low scale seesaw model’. In:JHEP07(2018), p.105.doi: 10.1007/ JHEP07(2018)105. arXiv: 1801.04207[hep-ph]
Pith/arXiv arXiv 2018
-
[35]
J.-L. Tastet, O. Ruchayskiy, and I. Timiryasov. ‘Reinterpreting the ATLAS bounds on heavy neutral leptons in a realistic neutrino oscillation model’. In:JHEP12(2021), p. 182.doi: 10.1007/JHEP12(2021)182. arXiv: 2107.12980[hep-ph]
-
[36]
M. Drewes, J. Klarić, and J. López-Pavón. ‘New benchmark models for heavy neut- ral lepton searches’. In:Eur. Phys. J. C82.12(2022), p.1176.doi: 10.1140/epjc/ s10052-022-11100-7. arXiv: 2207.02742[hep-ph] . 33
-
[37]
A. Abada, P. Escribano, X. Marcano, and G. Piazza. ‘Collider searches for heavy neutral leptons: beyond simplified scenarios’. In:Eur. Phys. J. C82.11(2022), p. 1030.doi: 10.1140/epjc/s10052-022-11011-7. arXiv: 2208.13882[hep-ph] .№:IFT- UAM/CSIC-22-98
-
[38]
A. M. Abdullahi et al. ‘The present and future status of heavy neutral leptons’. In:J. Phys. G50.2(2023), p.20501.doi: 10.1088/1361-6471/ac98f9. arXiv: 2203.08039 [hep-ph].№:FERMILAB-CONF-22-184-T-V
-
[39]
S. Antusch and J. Rosskopp. ‘Heavy Neutrino-Antineutrino Oscillations in Quantum Field Theory’. In:JHEP03(2021), p.170.doi: 10.1007/JHEP03(2021)170. arXiv: 2012.05763[hep-ph]
-
[40]
A. Atre, T. Han, S. Pascoli, and B. Zhang. ‘The Search for Heavy Majorana Neut- rinos’. In:JHEP05(2009), p.30.doi: 10.1088/1126-6708/2009/05/030. arXiv: 0901.3589[hep-ph] .№:FERMILAB-PUB-08-086-T,NSF-KITP-08-54,MADPH- 06-1466,DCPT-07-198, andIPPP-07-99
work page internal anchor Pith review Pith/arXiv arXiv doi:10.1088/1126-6708/2009/05/030 2009
-
[41]
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’. In:JHEP10(2006), p.84.doi: 10.1088/1126-6708/ 2006/10/084. arXiv:hep-ph/0607020.№:FTUAM-06-8andIFT-UAM-CSIC-06-30
work page internal anchor Pith review Pith/arXiv arXiv doi:10.1088/1126-6708/ 2006
-
[42]
Non-unitarity of the leptonic mixing matrix: Present bounds and future sensitivities
S. Antusch and O. Fischer. ‘Non-unitarity of the leptonic mixing matrix: Present bounds and future sensitivities’. In:JHEP10(2014), p.94.doi: 10.1007/JHEP10(2014)094. arXiv: 1407.6607[hep-ph] .№:MPP-2014-313
work page internal anchor Pith review Pith/arXiv arXiv doi:10.1007/jhep10(2014)094 2014
-
[43]
D. Aloni and A. Dery. ‘Revisiting leptonic nonunitarity’. In:Phys. Rev. D109.5(2024), p.55006.doi: 10.1103/PhysRevD.109.055006. arXiv: 2211.09638[hep-ph]
- [44]
-
[45]
C. Jarlskog. ‘Commutator of the Quark Mass Matrices in the Standard Electroweak Model and a Measure of Maximal CP Nonconservation’. In:Phys. Rev. Lett.55(1985), p.1039. doi: 10.1103/PhysRevLett.55.1039.№:USIP-85-14
-
[46]
The Interplay Between the "Low" and "High" Energy CP-Violation in Leptogenesis
E. Molinaro and S. T. Petcov. ‘The Interplay Between the ’Low’ and ’High’ En- ergy CP-Violation in Leptogenesis’. In:Eur. Phys. J. C61(2009), pp.93–109.doi: 10.1140/epjc/s10052-009-0985-3. arXiv: 0803.4120[hep-ph] .№:SISSA-11-2008- EPandIPMU-08-0013
work page internal anchor Pith review Pith/arXiv arXiv doi:10.1140/epjc/s10052-009-0985-3 2009
-
[47]
o=25" 24.73 72.48 30.76 59.74 WTA + “o=50
A. Granelli, J. Klarić, and S. T. Petcov. ‘Tests of low-scale leptogenesis in charged lepton flavour violation experiments’. In:Phys. Lett. B837(2023), p.137643.doi: 10.1016/j. physletb.2022.137643. arXiv: 2206.04342[hep-ph] .№:SISSA10/2022/FISI
work page doi:10.1016/j 2023
-
[48]
IceCube.‘MeasurementofAtmosphericNeutrinoOscillationParametersUsingConvolutional Neural Networks with9.3Years of Data in IceCube DeepCore’. In:Phys. Rev. Lett.134.9 (2025), p.91801.doi: 10.1103/PhysRevLett.134.091801. arXiv: 2405.02163[hep-ex]
-
[49]
‘Solar neutrino measurements using the full data period of Super- Kamiokande-IV’
Super-Kamiokande. ‘Solar neutrino measurements using the full data period of Super- Kamiokande-IV’. In:Phys. Rev. D109.9(2024), p.92001.doi: 10.1103/PhysRevD.109. 092001. arXiv: 2312.12907[hep-ex] .№:FERMILAB-PUB-24-1045-PPD. 34
-
[50]
G. Cowan, K. Cranmer, E. Gross, and O. Vitells. ‘Asymptotic formulae for likelihood- based tests of new physics’. In:Eur. Phys. J. C71(2011), p.1554.doi: 10.1140/ epjc/s10052-011-1554-0. arXiv: 1007.1727[physics.data-an]. Erratum in:Eur. Phys. J. C73(2013), p.2501
Pith/arXiv arXiv 2011
-
[51]
M. Beuthe. ‘Oscillations of neutrinos and mesons in quantum field theory’. In:Phys. Rept.375(2003), pp.105–218.doi: 10.1016/S0370-1573(02)00538-0. arXiv: hep-ph/ 0109119
-
[52]
S. Antusch, J. Hajer, and J. Rosskopp. ‘Decoherence effects on lepton number violation from heavy neutrino-antineutrino oscillations’. In:JHEP11(2023), p.235.doi: 10. 1007/JHEP11(2023)235. arXiv: 2307.06208[hep-ph]
arXiv 2023
-
[53]
F. F. Deppisch, M. Hirsch, and H. Päs. ‘Neutrinoless Double Beta Decay and Physics Beyond the Standard Model’. In:J. Phys. G39(2012), p.124007.doi: 10.1088/0954-3899/ 39/12/124007. arXiv: 1208.0727[hep-ph] .№:IFIC-12-56
work page internal anchor Pith review Pith/arXiv arXiv doi:10.1088/0954-3899/ 2012
-
[54]
Neutrinoless double beta decay: 2015 review
S. Dell’Oro, S. Marcocci, M. Viel, and F. Vissani. ‘Neutrinoless double beta decay:2015re- view’. In:Adv. High Energy Phys.2016(2016), p.2162659.doi: 10.1155/2016/2162659. arXiv: 1601.07512[hep-ph]
work page internal anchor Pith review Pith/arXiv arXiv doi:10.1155/2016/2162659 2016
-
[55]
Neutrinoless double beta decay in seesaw models
M. Blennow, E. Fernandez-Martinez, J. Lopez-Pavon, and J. Menendez. ‘Neutrinoless double betadecayinseesawmodels’.In:JHEP07(2010), p.96.doi: 10.1007/JHEP07(2010)096. arXiv: 1005.3240[hep-ph] .№:MPP-2010-40,IFT-UAM/CSIC-10-26,FTUAM- 10-06, andEURONU-WP6-10-18
work page internal anchor Pith review Pith/arXiv arXiv doi:10.1007/jhep07(2010)096 2010
-
[56]
F. L. Bezrukov. ‘νMSM-predictions for neutrinoless double beta decay’. In:Phys. Rev. D 72(2005), p.71303.doi: 10.1103/PhysRevD.72.071303. arXiv: hep-ph/0505247. 35
work page internal anchor Pith review Pith/arXiv arXiv doi:10.1103/physrevd.72.071303 2005
discussion (0)
Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.