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High energy extension of the FLUKA atmospheric neutrino flux

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G.Battistoni, A.Ferrari, T.Montaruli, P.R.Sala

High Energy Physics - Phenomenology · Submitted 19 May 2003

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

The authors' main claim We point out that the primary flux model above 100 GeV/nucleon still contributes with an important systematic error to the neutrino flux.

how it is stated · asserted 0.98 read the record →

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arXiv IDhep-ph/0305208 (version 1)
Pith IDQGMDYI4S, Pith's permanent record of this paper and its review
CitationA.Ferrari, G.Battistoni, P.R.Sala, T.Montaruli. "High energy extension of the FLUKA atmospheric neutrino flux." arXiv:hep-ph/0305208 (2003). https://pith.science/paper/QGMDYI4S
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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, 3,053 input tokens, $0.0001 reported.

What the abstract itself states, as probabilities: claims first 0.06 · states limitation 0.95 · human participants 0.02 · controlled comparison 0.04 · randomized assignment 0.01 · states quantitative result 0.84 · compares with prior results 0.48 · mentions code or data availability 0.15.

The abstract, sentence by sentence

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

The atmospheric neutrino flux calculated with FLUKA was originally limited to 100-200 GeV for statistical reasons. In order to make it available for the analysis of high energy events, like upward through-going muons detected by neutrino telescopes, we have extended the calculation so to provide a reliable neutrino yield per primary nucleon up to about 10**6 GeV/nucleon, as far as the interaction model is concerned. We point out that the primary flux model above 100 GeV/nucleon still contributes with an important systematic error to the neutrino flux.

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 The atmospheric neutrino flux calculated with FLUKA was originally limited to 100-200 GeV for statistical reasons. background 0.75 0.37 0.04 asserted 1.00
s1 In order to make it available for the analysis of high energy events, like upward through-going muons detected by neutrino telescopes, we have extended the calculation so to provide a reliable neutrino yield per primary nucleon up to about 10**6 GeV/nucleon, as far as the interaction model is concerned. contribution 0.98 0.95 0.36 asserted 0.99
s2 We point out that the primary flux model above 100 GeV/nucleon still contributes with an important systematic error to the neutrino flux. limitation 0.98 0.55 0.30 asserted 0.98

What kind of paper the classifier reports this is: simulation study 0.92 · evidence from simulation or computation 1.00.

What was examined, and what was not

sources read
  • arXiv listing abstract v1
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

The atmospheric neutrino flux calculated with FLUKA was originally limited to 100-200 GeV for statistical reasons. In order to make it available for the analysis of high energy events, like upward through-going muons detected by neutrino telescopes, we have extended the calculation so to provide a reliable neutrino yield per primary nucleon up to about 10**6 GeV/nucleon, as far as the interaction model is concerned. We point out that the primary flux model above 100 GeV/nucleon still contributes with an important systematic error to the neutrino flux.

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References
How the literature uses it

6 arXiv papers cite this in 7 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 · 4 sentences without a confident label

Uses its data or values 2 papers
Cites it as background 1 paper

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