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Gravitationally Induced Neutrino-Oscillation Phases

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D. V. Ahluwalia, C. Burgard

General Relativity and Quantum Cosmology · Submitted 8 Mar 1996

abstract compiled · 2026-09-23 · no language-model review

The authors' main claim When this information is coupled with the mass square differences implied by the existing neutrino-oscillation data we find that the new effect may have profound consequences for type-II supernova evolution.

how it is stated · hedged possibility 0.96 read the record →

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arXiv IDgr-qc/9603008 (version 6)
Pith IDIY72U4AW, Pith's permanent record of this paper and its review
CitationC. Burgard, D. V. Ahluwalia. "Gravitationally Induced Neutrino-Oscillation Phases." arXiv:gr-qc/9603008 (1996). https://pith.science/paper/IY72U4AW
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The compiled record

The paper's own sentences, arranged. 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.

Open the compiled record

Compiled by classifier-1.13-20260917 via OpenRouter, question bank abstract-p1-20260923, 2026-09-23: 1 request, 3,636 input tokens, $0.0002 reported.

What the abstract itself states, as probabilities: claims first 0.47 · states limitation 0.10 · human participants 0.01 · controlled comparison 0.16 · randomized assignment 0.01 · states quantitative result 0.96 · compares with prior results 0.70 · mentions code or data availability 0.02.

The abstract, sentence by sentence

arXiv listing abstract v6. Results and the main claim are underlined; .

In this essay, we introduce a new effect of gravitationally induced quantum mechanical phases in neutrino oscillations. These phases arise from an hitherto unexplored interplay of gravitation and the principle of the linear superposition of quantum mechanics. In the neighborhood of a 1.4 solar-mass neutron star, gravitationally induced quantum mechanical phases are roughly 20% of their kinematical counterparts. When this information is coupled with the mass square differences implied by the existing neutrino-oscillation data we find that the new effect may have profound consequences for type-II supernova evolution.

background contribution method result interpretation main claim

What the classifier reports for each sentence. The number is the probability it gave the label.
#sentencerolethe authors' own workstates the main conclusionstrength
s0 In this essay, we introduce a new effect of gravitationally induced quantum mechanical phases in neutrino oscillations. contribution 1.00 0.84 0.12 asserted 0.97
s1 These phases arise from an hitherto unexplored interplay of gravitation and the principle of the linear superposition of quantum mechanics. contribution 0.72 0.38 0.07 asserted 1.00
s2 In the neighborhood of a 1.4 solar-mass neutron star, gravitationally induced quantum mechanical phases are roughly 20% of their kinematical counterparts. result 1.00 0.78 0.14 asserted 0.93
s3 When this information is coupled with the mass square differences implied by the existing neutrino-oscillation data we find that the new effect may have profound consequences for type-II supernova evolution. interpretation 0.99 0.86 0.70 hedged possibility 0.96

What kind of paper the classifier reports this is: theoretical result 0.99 · evidence from proof or derivation 0.72.

What was examined, and what was not

sources read
  • arXiv listing abstract v6
not examined
  • full text
  • figures and tables
  • references and citing sentences
  • relations to other papers
levels run
  • P abstract
not run
  • S sections
  • T body sentences
  • C citations
  • R cross-paper relations

Every quoted sentence on this record is the authors'. Every label is from Pith's closed vocabulary, with the probability shown beside it. Every number in the measurements table is the authors', checked by code. Record as JSON

The paper
Original abstract

In this essay, we introduce a new effect of gravitationally induced quantum mechanical phases in neutrino oscillations. These phases arise from an hitherto unexplored interplay of gravitation and the principle of the linear superposition of quantum mechanics. In the neighborhood of a 1.4 solar-mass neutron star, gravitationally induced quantum mechanical phases are roughly 20% of their kinematical counterparts. When this information is coupled with the mass square differences implied by the existing neutrino-oscillation data we find that the new effect may have profound consequences for type-II supernova evolution.

Human review

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References
How the literature uses it

19 arXiv papers cite this in 23 sentences

Each citing sentence is taken from the citing paper's LaTeX source and typed by Pith's classifier. A label appears at probability 0.8 or more (0.95 for support), a contest at 0.7 or more; the quoted words are the citing authors'. How each label was checked · JSON

Papers whose main result relates to this one's

Found among the papers closest to this one by title and main claim. Pith's classifier compared each pair's main results and a second model family confirmed the relation; checked against two further families, shown conflicts agreed 118 times in 120 and shown same results 218 times in 239. The quoted sentence is the other paper's main claim.

States a conflicting result 1 paper
  • A straightforward exercise in the Schwarzschild coordinates appropriate to a spherically symmetric non-rotating star shows that, although there is a general relativistic effect of the star's gravity on neutrino oscillations, it is not of the form claimed, and is too small to be measured.

    Comment on "Gravitationally Induced Neutrino-Oscillation Phases" · 0.99

Papers citing it · 10 sentences without a confident label

Cites it as background 11 papers
  • Neutrino oscillation was first formulated in flat spacetime which was subsequently generalized to curved spacetime [ref] and the formalism can also be used to test the equivalence principle [ref] .

    Aspects of Neutrino Oscillation in Alternative Gravity Theories · Introduction · 0.85

  • As discussed in Refs. [ref] [ref] [ref] [ref] , when discussing neutrino oscillation we might distinguish at least three different scenarios where neutrino oscillate in I) a flat spacetime, II) a curved spacetime in a non-rotating frame and III) a curved spacetime in a rotating frame.

    Neutrino flavor oscillations in a curved space-time · Probability of oscillation · 0.89

  • Neutrino oscillations, in curved spacetime has gained attention in recent times [ref] , for the reason that such analysis is not only sensitive to the background geometry and hence the gravity theory at work [ref] but they also reveal some salient features of the neutrino sector which are not present in flat spacetime [ref] .

    Aspects of gravitational decoherence in neutrino lensing · Introduction · 0.91

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