Effect of Off-diagonal NSI Parameters on Entanglement Measurements in Neutrino Oscillations
Pith reviewed 2026-05-19 06:34 UTC · model grok-4.3
The pith
Off-diagonal NSI parameters alter neutrino entanglement measures most at low energies, with Negativity most sensitive to the CP phase.
A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.
Core claim
Expressing entanglement of formation, concurrence, and negativity directly in terms of oscillation probabilities shows that the off-diagonal NSI parameters ε_eμ, ε_eτ, and ε_μτ, together with their phases, modify these quantum correlations, with the largest changes appearing at low energies in DUNE while negativity continues to dominate at higher energies and exhibits clearer sensitivity to δ_CP than the other two measures.
What carries the argument
The rewriting of entanglement measures (EOF, concurrence, negativity) as functions of neutrino oscillation probabilities, followed by their evaluation under off-diagonal NSI parameters.
If this is right
- NSI effects would be most detectable in the low-energy region of long-baseline neutrino data.
- Negativity would continue to register quantum correlations after EOF and concurrence weaken at high energies.
- ε_eμ and ε_eτ would mainly modify entanglement through appearance-channel probabilities, while ε_μτ would act through disappearance channels.
- Negativity would display a visible dependence on δ_CP within specific low-energy intervals under off-diagonal NSI.
Where Pith is reading between the lines
- The same probability-based mapping could be applied to other long-baseline experiments to search for consistent NSI signatures.
- Entanglement observables might supplement conventional oscillation fits when placing bounds on NSI parameters.
- Low-energy runs could be prioritized to separate NSI contributions from standard oscillations using these measures.
Load-bearing premise
The entanglement measures can be extracted solely from oscillation probabilities without additional experimental or theoretical corrections that would alter the reported NSI dependence.
What would settle it
A DUNE measurement showing that the entanglement measures lack stronger NSI dependence at low energies or that negativity fails to remain dominant at high energies would falsify the central claim.
Figures
read the original abstract
In this work, we explore the influence of off-diagonal non-standard interaction (NSI) parameters on quantum entanglement within the three-flavor neutrino oscillation framework. By expressing three key entanglement measures: Entanglement of Formation (EOF), Concurrence, and Negativity in terms of oscillation probabilities, we analyze how these quantum correlations are affected by the NSI parameters $\epsilon_{e\mu}$, $\epsilon_{e\tau}$, and $\epsilon_{\mu\tau}$, including their complex phases. The quantum correlation measures considered in this work cannot be extracted directly from event rates, but solely in terms of oscillation probabilities. Using the DUNE experiment as a reference point, our analysis shows that NSI effects are most pronounced at lower energies, while Negativity continuing to dominate even at higher energies. It is observed that $\epsilon_{e \mu}$ and $\epsilon_{e \tau}$ affect entanglement measures mainly through the appearance channel, while the impact of $\epsilon_{\mu \tau}$ on EOF, Concurrence, and Negativity is predominantly linked to the disappearance channel. Further, our results show that Negativity is more sensitive than EOF and Concurrence in the [Energy ($E$) - $\delta_{CP}$] plane under the influence of off-diagonal NSI scenarios, displaying a clear dependence of the CP-violating phase, $\delta_{CP}$ on specific energy ranges, particularly in the lower energy regime.
Editorial analysis
A structured set of objections, weighed in public.
Referee Report
Summary. The paper explores the effects of off-diagonal NSI parameters (ε_eμ, ε_eτ, ε_μτ and their phases) on quantum entanglement in three-flavor neutrino oscillations. It expresses Entanglement of Formation (EOF), Concurrence, and Negativity in terms of oscillation probabilities, analyzes their behavior with DUNE as reference, and reports that NSI effects are strongest at low energies, Negativity dominates at higher energies, ε_eμ and ε_eτ primarily affect the appearance channel while ε_μτ affects disappearance, and Negativity shows greater sensitivity to δ_CP in the [E – δ_CP] plane under off-diagonal NSI.
Significance. If the expressions for the entanglement measures are shown to correctly incorporate all relevant phase information from the evolution operator, the work could provide a quantum-information-based approach to probing NSI in long-baseline experiments, with the reported differential sensitivities offering potential guidance for analysis strategies at DUNE and similar facilities.
major comments (1)
- [Section on quantum correlation measures] Section on quantum correlation measures (abstract and the section deriving entanglement measures from probabilities): The entanglement measures are expressed solely as functions of the oscillation probabilities P_αβ. For the pure state |ψ⟩ = ∑_β A_β |ν_β⟩ the density matrix has off-diagonal coherences √(P_α P_β) exp(i Δϕ_αβ), where the relative phases Δϕ_αβ are fixed by the full evolution operator containing both δ_CP and the complex phases of ε_eμ, ε_eτ, ε_μτ. Formulas discarding explicit phase information therefore cannot capture the full dependence on δ_CP and NSI phases reported in the [E – δ_CP] plane, especially at low energies where matter and NSI effects are stated to be largest. This is load-bearing for the central sensitivity claims.
minor comments (2)
- [Abstract and methods] The abstract and methods sections provide no error propagation for the entanglement measures derived from probabilities and no explicit baseline comparison to the standard oscillation case without NSI.
- [Numerical results] The numerical results lack a clear statement of how the NSI parameter magnitudes and phases are chosen or marginalized, which affects reproducibility of the reported [E – δ_CP] sensitivities.
Simulated Author's Rebuttal
We thank the referee for the careful reading of our manuscript and for identifying an important technical point regarding the treatment of phases in the entanglement measures. We address this comment below and will revise the manuscript to strengthen the presentation and accuracy of our results.
read point-by-point responses
-
Referee: Section on quantum correlation measures (abstract and the section deriving entanglement measures from probabilities): The entanglement measures are expressed solely as functions of the oscillation probabilities P_αβ. For the pure state |ψ⟩ = ∑_β A_β |ν_β⟩ the density matrix has off-diagonal coherences √(P_α P_β) exp(i Δϕ_αβ), where the relative phases Δϕ_αβ are fixed by the full evolution operator containing both δ_CP and the complex phases of ε_eμ, ε_eτ, ε_μτ. Formulas discarding explicit phase information therefore cannot capture the full dependence on δ_CP and NSI phases reported in the [E – δ_CP] plane, especially at low energies where matter and NSI effects are stated to be largest. This is load-bearing for the central sensitivity claims.
Authors: We thank the referee for this insightful comment. We agree that the off-diagonal elements of the density matrix for the pure neutrino state contain relative phases Δϕ_αβ that are determined by the full evolution operator and therefore depend on both δ_CP and the complex NSI phases. Our analytic expressions for EOF, Concurrence, and Negativity were written in a form that depends only on the probabilities P_αβ; this presentation omits explicit phase dependence and is therefore incomplete for capturing the full sensitivity structure. In the numerical DUNE analysis we did evolve the complete Hamiltonian (including all phases) to obtain the state amplitudes before computing the measures, but the manuscript does not make this distinction clear and the formulas as written do not retain the phases. We will revise the relevant section to express the measures directly from the full density-matrix elements ρ_αβ = A_α A_β^*, thereby incorporating both probabilities and phases. The abstract will also be updated to reflect the corrected derivation. These changes will ensure that the reported δ_CP and NSI-phase sensitivities in the [E – δ_CP] plane are rigorously justified. revision: yes
Circularity Check
No significant circularity; derivation substitutes NSI probabilities into independent entanglement formulas
full rationale
The paper computes oscillation probabilities modified by off-diagonal NSI parameters (including phases) using the standard three-flavor evolution Hamiltonian, then inserts those probabilities into the standard expressions for EOF, concurrence, and negativity. No step reduces by construction to a fitted parameter, self-defined quantity, or self-citation chain. The entanglement formulas are taken from external quantum-information literature and applied directly; DUNE baseline and energy ranges are external inputs, not derived inside the work. The chain is therefore self-contained against external benchmarks and does not exhibit any of the enumerated circularity patterns.
Axiom & Free-Parameter Ledger
free parameters (1)
- ε_eμ, ε_eτ, ε_μτ magnitudes and phases
axioms (1)
- domain assumption Three-flavor neutrino oscillation framework with standard matter effects remains valid when off-diagonal NSI are added
Lean theorems connected to this paper
-
IndisputableMonolith/Cost/FunctionalEquation.leanwashburn_uniqueness_aczel unclear?
unclearRelation between the paper passage and the cited Recognition theorem.
By expressing three key entanglement measures: Entanglement of Formation (EOF), Concurrence, and Negativity in terms of oscillation probabilities... NSI effects are most pronounced at lower energies
-
IndisputableMonolith/Foundation/RealityFromDistinction.leanreality_from_one_distinction unclear?
unclearRelation between the paper passage and the cited Recognition theorem.
The quantum correlation measures considered in this work cannot be extracted directly from event rates, but solely in terms of oscillation probabilities
What do these tags mean?
- matches
- The paper's claim is directly supported by a theorem in the formal canon.
- supports
- The theorem supports part of the paper's argument, but the paper may add assumptions or extra steps.
- extends
- The paper goes beyond the formal theorem; the theorem is a base layer rather than the whole result.
- uses
- The paper appears to rely on the theorem as machinery.
- contradicts
- The paper's claim conflicts with a theorem or certificate in the canon.
- unclear
- Pith found a possible connection, but the passage is too broad, indirect, or ambiguous to say the theorem truly supports the claim.
Reference graph
Works this paper leans on
-
[1]
From this analysis, it becomes clear that the impact of ϵeµ on the EOF is predominantly driven by its effect on the appearance channel. Next, we turn our attention to understanding how ϵeµ influences the other two entangle- ment measures: Concurrence and Negativity. The simplified form of Concurrence (Eq. 12) in terms of electron neutrino appearance and m...
-
[2]
Y. Fukuda et al. [Super-Kamiokande Collaboration], Phys. Rev. Lett. 81, 1562–1567 (1998)
work page 1998
-
[4]
K. Abe et al. [T2K Collaboration], Eur. Phys. J. C 83 (2023), 10.1140/epjc/s10052-023-11819- x
-
[6]
Abiet al.(DUNE), JINST15(08), T08008, arXiv:2002.02967 [physics.ins-det]
B. Abi et al. [DUNE Collaboration], JINST 15, T08008 (2020), arXiv:2002.02967 [physics.ins- det]
-
[7]
J. collaboration et al. , Prog. Part. Nucl. Phys. 123, 103927 (2022)
work page 2022
-
[8]
B. Abi et al. , Eur. Phys. J. C 81 (2021), 10.1140/epjc/s10052-021-09007-w
-
[10]
Mohanta, in Particle Physics and Cosmology in the Himalayas (2025) arXiv:2503.12985 [hep-ph]
R. Mohanta, in Particle Physics and Cosmology in the Himalayas (2025) arXiv:2503.12985 [hep-ph]
- [11]
- [12]
- [13]
- [14]
- [15]
-
[16]
Status of non-standard neutrino interactions
T. Ohlsson, Rept. Prog. Phys. 76, 044201 (2013), arXiv:1209.2710 [hep-ph]
work page internal anchor Pith review Pith/arXiv arXiv 2013
-
[17]
O. G. Miranda and H. Nunokawa, New J. Phys. 17, 095002 (2015), arXiv:1505.06254 [hep-ph]
work page internal anchor Pith review Pith/arXiv arXiv 2015
-
[18]
Neutrino oscillations and Non-Standard Interactions
Y. Farzan and M. Tortola, Front. in Phys. 6, 10 (2018), arXiv:1710.09360 [hep-ph]
work page internal anchor Pith review Pith/arXiv arXiv 2018
- [19]
-
[20]
K. N. Deepthi, S. C, and R. Mohanta, New J. Phys. 17, 023035 (2015), arXiv:1409.2343 [hep-ph]
work page internal anchor Pith review Pith/arXiv arXiv 2015
-
[21]
Complementarity Between Hyperkamiokande and DUNE in Determining Neutrino Oscillation Parameters
S. Fukasawa, M. Ghosh, and O. Yasuda, Nucl. Phys. B 918, 337 (2017), arXiv:1607.03758 [hep-ph]
work page internal anchor Pith review Pith/arXiv arXiv 2017
-
[22]
Probing CP violation signal at DUNE in presence of non-standard neutrino interactions
M. Masud, A. Chatterjee, and P. Mehta, J. Phys. G 43, 095005 (2016), arXiv:1510.08261 [hep-ph]
work page internal anchor Pith review Pith/arXiv arXiv 2016
-
[23]
Non-standard Neutrino Interactions at DUNE
A. de Gouvˆ ea and K. J. Kelly, Nucl. Phys. B 908, 318 (2016), arXiv:1511.05562 [hep-ph]
work page internal anchor Pith review Pith/arXiv arXiv 2016
- [24]
-
[25]
M. Blennow, P. Coloma, E. Fernandez-Martinez, J. Hernandez-Garcia, and J. Lopez-Pavon, JHEP 2017 (2017), 10.1007/jhep04(2017)153
-
[26]
S. K. Agarwalla, S. S. Chatterjee, and A. Palazzo, Phys. Lett. B 762, 64–71 (2016)
work page 2016
-
[27]
M. Masud and P. Mehta, Phys. Rev. D 94 (2016), 10.1103/physrevd.94.053007
-
[28]
P. Coloma and T. Schwetz, Phys. Rev. D 95 (2017), 10.1103/physrevd.95.079903
-
[29]
J. Liao, D. Marfatia, and K. Whisnant, Phys. Rev. D 93 (2016), 10.1103/physrevd.93.093016
-
[30]
Coloma, JHEP 2016 (2016), 10.1007/jhep03(2016)016
P. Coloma, JHEP 2016 (2016), 10.1007/jhep03(2016)016
-
[31]
A. K. Alok, S. Banerjee, and S. Uma Sankar, Nucl. Phys. B 909, 65–72 (2016)
work page 2016
-
[32]
S. Banerjee, A. K. Alok, R. Srikanth, and B. C. Hiesmayr, Eur. Phys. J. C 75, 1 (2015)
work page 2015
-
[33]
J. Formaggio, D. Kaiser, M. Murskyj, and T. Weiss, Phys. Rev. Lett. 117 (2016), 10.1103/physrevlett.117.050402
-
[34]
Q. Fu and X. Chen, Eur. Phys. J. C 77 (2017), 10.1140/epjc/s10052-017-5371-y
-
[35]
J. Naikoo, A. K. Alok, S. Banerjee, and S. U. Sankar, Phys. Rev. D 99 (2019), 10.1103/phys- revd.99.095001
- [36]
- [37]
-
[38]
T. Sarkar and K. Dixit, Eur. Phys. J. C 81 (2021), 10.1140/epjc/s10052-021-08874-7
-
[39]
M. Blasone, F. Illuminati, L. Petruzziello, and L. Smaldone, Phys. Rev. A 108, 032210 (2023), arXiv:2111.09979 [quant-ph]
- [40]
-
[42]
K. Dixit, S. S. Haque, and S. Razzaque, Eur. Phys. J. C 84 (2024), 10.1140/epjc/s10052-024- 12620-0
- [43]
-
[44]
R. Banerjee, P. Panda, R. Mohanta, and S. Patra, (2024), arXiv:2410.05727 [hep-ph]
-
[45]
L. Konwar and B. Yadav, J. Phys. G 52, 045001 (2025), arXiv:2411.14234 [hep-ph]
-
[46]
Konwar, Journal of Subatomic Particles and Cosmology , 100065 (2025)
L. Konwar, Journal of Subatomic Particles and Cosmology , 100065 (2025)
work page 2025
-
[47]
M. Blasone, F. Dell’Anno, S. De Siena, and F. Illuminati, EPL 85, 50002 (2009)
work page 2009
-
[48]
M. Blasone, F. Dell’Anno, S. D. Siena, and F. Illuminati, Journal of Physics: Conference Series 237, 012007 (2010)
work page 2010
-
[49]
M. Blasone, S. De Siena, and C. Matrella, Eur. Phys. J. C 81 (2021), 10.1140/epjc/s10052- 021-09471-4
-
[50]
A. Kumar Jha, S. Mukherjee, and B. A. Bambah, Mod. Phys. Lett. A 36, 2150056 (2021), arXiv:2004.14853 [hep-ph]
- [51]
-
[52]
R. Horodecki, P. Horodecki, M. Horodecki, and K. Horodecki, Rev. Mod. Phys. 81, 865–942 (2009)
work page 2009
-
[53]
M. Blasone, F. Dell’Anno, S. De Siena, M. Di Mauro, and F. Illuminati, Phys. Rev. D 77 (2008), 10.1103/physrevd.77.096002
-
[54]
C. H. Bennett, D. P. DiVincenzo, J. A. Smolin, and W. K. Wootters, Phys. Rev. A 54, 3824 (1996), arXiv:quant-ph/9604024
work page internal anchor Pith review Pith/arXiv arXiv 1996
- [55]
-
[56]
Entanglement of a Pair of Quantum Bits
S. Hill and W. K. Wootters, Phys. Rev. Lett. 78, 5022 (1997), arXiv:quant-ph/9703041
work page internal anchor Pith review Pith/arXiv arXiv 1997
-
[57]
W. K. Wootters, Phys. Rev. Lett. 80, 2245 (1998), arXiv:quant-ph/9709029
work page internal anchor Pith review Pith/arXiv arXiv 1998
- [58]
-
[59]
Separability Criterion for Density Matrices
A. Peres, Phys. Rev. Lett. 77, 1413 (1996), arXiv:quant-ph/9604005
work page internal anchor Pith review Pith/arXiv arXiv 1996
-
[60]
A computable measure of entanglement
G. Vidal and R. F. Werner, Phys. Rev. A 65, 032314 (2002), arXiv:quant-ph/0102117
work page internal anchor Pith review Pith/arXiv arXiv 2002
- [61]
-
[62]
J. Liao, D. Marfatia, and K. Whisnant, JHEP 01, 071 (2017), arXiv:1612.01443 [hep-ph]
work page internal anchor Pith review Pith/arXiv arXiv 2017
-
[63]
L.-J. Li, F. Ming, X.-K. Song, L. Ye, and D. Wang, Eur. Phys. J. C 81, 728 (2021)
work page 2021
- [64]
- [65]
-
[66]
New features in the simulation of neutrino oscillation experiments with GLoBES 3.0
P. Huber, J. Kopp, M. Lindner, M. Rolinec, and W. Winter, Comput. Phys. Commun. 177, 432 (2007), arXiv:hep-ph/0701187
work page internal anchor Pith review Pith/arXiv arXiv 2007
-
[67]
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, JHEP 2024 (2024), 10.1007/jhep12(2024)216. 24
- [68]
- [69]
-
[70]
The fate of hints: updated global analysis of three-flavor neutrino oscillations,
I. Esteban, M. C. Gonzalez-Garcia, M. Maltoni, T. Schwetz, and A. Zhou, JHEP 09, 178 (2020), arXiv:2007.14792 [hep-ph]. 25
discussion (0)
Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.