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Neutrino Flight Times in Cosmology

Astrophysics · Submitted 10 Nov 1999

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

The authors' main claim If neutrinos have a small but non-zero mass, time-of-flight effects for neutrino bursts from distant sources can yield information on the large-scale geometry of the universe, the effects being proportional to the integral over time of the cosmological expansion parameter.

how it is stated · hedged possibility 0.91 read the record →

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arXiv IDastro-ph/9911167 (version 1)
Pith IDKGAVZJET, Pith's permanent record of this paper and its review
CitationLeo Stodolsky. "Neutrino Flight Times in Cosmology." arXiv:astro-ph/9911167 (1999). https://pith.science/paper/KGAVZJET
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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.

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Compiled by classifier-1.13-20260917 via OpenRouter, question bank abstract-p1-20260923, 2026-09-23: 1 request, 2,954 input tokens, $0.0001 reported.

What the abstract itself states, as probabilities: claims first 0.03 · states limitation 0.66 · human participants 0.02 · controlled comparison 0.02 · randomized assignment 0.01 · states quantitative result 0.04 · compares with prior results 0.04 · mentions code or data availability 0.02.

The abstract, sentence by sentence

arXiv listing abstract v1. Results and the main claim are underlined; .

If neutrinos have a small but non-zero mass, time-of-flight effects for neutrino bursts from distant sources can yield information on the large-scale geometry of the universe, the effects being proportional to the integral over time of the cosmological expansion parameter. In principle absolute physical determinations of the Hubble constant and the acceleration parameter are possible. Practical realization of these possibilities would depend on neutrino masses being in a favorable range and the future development of very large detectors.

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 If neutrinos have a small but non-zero mass, time-of-flight effects for neutrino bursts from distant sources can yield information on the large-scale geometry of the universe, the effects being proportional to the integral over time of the cosmological expansion parameter. background 0.60 0.09 0.51 hedged possibility 0.91
s1 In principle absolute physical determinations of the Hubble constant and the acceleration parameter are possible. interpretation 0.77 0.06 0.31 hedged possibility 0.93
s2 Practical realization of these possibilities would depend on neutrino masses being in a favorable range and the future development of very large detectors. limitation 0.79 0.04 0.13 hedged possibility 0.85

What kind of paper the classifier reports this is: theoretical result 0.78 · evidence from argument 0.74.

What was examined, and what was not

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not examined
  • full text
  • figures and tables
  • references and citing sentences
  • relations to other papers
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  • 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

If neutrinos have a small but non-zero mass, time-of-flight effects for neutrino bursts from distant sources can yield information on the large-scale geometry of the universe, the effects being proportional to the integral over time of the cosmological expansion parameter. In principle absolute physical determinations of the Hubble constant and the acceleration parameter are possible. Practical realization of these possibilities would depend on neutrino masses being in a favorable range and the future development of very large detectors.

Human review
References
How the literature uses it

4 arXiv papers cite this in 5 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 citing it · 2 sentences without a confident label

Uses its method or tool 1 paper
  • The time delay of a neutrino emitted at the moment of neutron star coalescence at redshift $z$, relative to the gravitational wave signal of coalescence, is given by [ref] [equation] where $m_ν$ is the mass of the neutrino mass eigenstate under consideration and $E_ν(z')=(1+z') E_ν$, with $E_ν$ being the neutrino energy at Earth.

    Prospects for Neutrino Observation and Mass Measurement from Binary Neutron Star Mergers · Background mitigation · 0.86

Cites it as background 2 papers
  • Despite the fact that some proposals of new distance indicators with ultra-relativistic particles emitted from the source have been recently investigated from the theoretical point of view [ref] , most of the cosmological distance tools involve massless particles which travel from the source to the observer's laboratory.

    Relations between physical observables: what is better? · Introduction · 0.92

  • The idea of using time delays between UR particles as a cosmological probe is more recent [ref] (see also the short review [ref] ).

    On the time delay between ultra-relativistic particles · Introduction · 0.98

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