REVIEW
Interpreting quantum coherence of neutrinos in asymptotically flat spacetimes via effective distances: Solution to the paradoxes of the Leggett-Garg inequality and quantum information quantities
High Energy Physics - Phenomenology · Submitted 16 Sep 2026 · 64 references
Pith's verdict: A clean resolution to the measure-dependence paradox in neutrino coherence via effective distances, though the claim about metric discrimination relies on limited parameter scans.
T0 · AI review
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Referee report
The paper
The paper claims
By mapping neutrino oscillation phases in curved spacetimes onto flat spacetime via effective distances, the paper proves that the maximum of the Leggett-Garg parameter is universal and independent of the gravitational background.
The reading
Extended reading notes
Core claim
One can always map neutrino-oscillation phases in asymptotically flat spacetimes onto the phases in flat spacetime (Eq. 10), and as a result the maximal amount of quantum coherence quantified by the Leggett-Garg parameter is independent from background spacetimes (Section III.B).
Load-bearing premise
The derivation assumes that the neutrino mass eigenstates satisfy the WKB approximation and that the propagation phase can be computed via the Hamilton-Jacobi equation using a null reference trajectory (Appendix A). This requires the relativistic limit m^2/E^2 << 1 and that the affine parameter from the null geodesic is valid for massive particles at leading order.
Original abstract
In this work, we propose a notion called effective distance to characterize the essential gravitational effects on quantum coherence of neutrinos. Employing effective distances, we prove that one can always map neutrino-oscillation phases in asymptotically flat spacetimes onto the phases in flat spacetime, which is considered as a nontrivial realization of equivalence principle. Hence, the maximal amount of quantum coherence, quantified by the Leggett-Garg (LG) parameter is independent from background spacetimes, namely, the paradox that the gravitational effects on quantum coherence of neutrinos are measure-dependent (Ettefaghi et al.[1]) does not arise. Following the same route, we preclude the gravitational amplifying or damping of amplitudes of the quantum information quantities for special masses of black holes (Wang et al. [2]). To demonstrate furthermore the independence of quantum coherence from background spacetimes, we examine the proposal using the LG parameter to identify quantum-corrected models of spacetimes. For different emission positions of neutrinos and various quantum parameters, we find no consistent patterns in oscillating LG curves to discriminate a quantum metric from the classical one.
The compiled record
The paper's own sentences, arranged, kept beside the review and separate from it. Each label is drawn from a closed vocabulary; the number beside it is the probability the classifier gave that label. Numbers in the tables are the authors', checked by code. No sentence in this record was written by a model.
The abstract, sentence by sentence
In this work, we propose a notion called effective distance to characterize the essential gravitational effects on quantum coherence of neutrinos. Employing effective distances, we prove that one can always map neutrino-oscillation phases in asymptotically flat spacetimes onto the phases in flat spacetime, which is considered as a nontrivial realization of equivalence principle. Hence, the maximal amount of quantum coherence, quantified by the Leggett-Garg (LG) parameter is independent from background spacetimes, namely, the paradox that the gravitational effects on quantum coherence of neutrinos are measure-dependent (Ettefaghi et al.[1]) does not arise. Following the same route, we preclude the gravitational amplifying or damping of amplitudes of the quantum information quantities for special masses of black holes (Wang et al. [2]). To demonstrate furthermore the independence of quantum coherence from background spacetimes, we examine the proposal using the LG parameter to identify quantum-corrected models of spacetimes. For different emission positions of neutrinos and various quantum parameters, we find no consistent patterns in oscillating LG curves to discriminate a quantum metric from the classical one.
background contribution method result interpretation main claim
| # | sentence | role | the authors' own work | states the main conclusion | strength |
|---|---|---|---|---|---|
| s0 | In this work, we propose a notion called effective distance to characterize the essential gravitational effects on quantum coherence of neutrinos. | contribution 0.94 | 0.90 | 0.07 | asserted 0.78 |
| s1 | Employing effective distances, we prove that one can always map neutrino-oscillation phases in asymptotically flat spacetimes onto the phases in flat spacetime, which is considered as a nontrivial realization of equivalence principle. | result 0.68 | 0.94 | 0.19 | asserted 0.99 |
| s2 | Hence, the maximal amount of quantum coherence, quantified by the Leggett-Garg (LG) parameter is independent from background spacetimes, namely, the paradox that the gravitational effects on quantum coherence of neutrinos are measure-dependent (Ettefaghi et al.[1]) does not arise. | result 0.79 | 0.80 | 0.66 | asserted 1.00 |
| s3 | Following the same route, we preclude the gravitational amplifying or damping of amplitudes of the quantum information quantities for special masses of black holes (Wang et al. [2]). | result 0.96 | 0.81 | 0.10 | asserted 1.00 |
| s4 | To demonstrate furthermore the independence of quantum coherence from background spacetimes, we examine the proposal using the LG parameter to identify quantum-corrected models of spacetimes. | contribution 0.67 | 0.85 | 0.06 | asserted 0.90 |
| s5 | For different emission positions of neutrinos and various quantum parameters, we find no consistent patterns in oscillating LG curves to discriminate a quantum metric from the classical one. | result 1.00 | 0.95 | 0.14 | asserted 1.00 |
What was examined, and what was not
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Figures
Figures reproduced from arXiv:2609.19198 by the authors.
References
Discussion
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