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Spin light of relativistic electrons in neutrino fluxes

High Energy Physics - Phenomenology · Submitted 8 Nov 2014

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

The authors' main claim It is shown that a reasonable portion of energy of the neutrino flux can be transferred by the $SLe_\nu$ to gamma-rays .

how it is stated · asserted 0.93 read the record →

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arXiv ID1502.05346 (version 1)
Pith IDT6MQFQKM, Pith's permanent record of this paper and its review
CitationAlexander I. Studenikin, Ilya A. Balantsev. "Spin light of relativistic electrons in neutrino fluxes." arXiv:1502.05346 (2014). https://pith.science/paper/T6MQFQKM
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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, 3,673 input tokens, $0.0002 reported.

What the abstract itself states, as probabilities: claims first 0.16 · states limitation 0.10 · human participants 0.01 · controlled comparison 0.04 · randomized assignment 0.01 · states quantitative result 0.08 · compares with prior results 0.07 · mentions code or data availability 0.01.

The abstract, sentence by sentence

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

A new mechanism of electromagnetic radiation by electrons under the influence of a dense neutrino flux, termed "the spin light of electron" in neutrino flux ($SLe_\nu$), is considered. It is shown that in the case when electrons are moving against the neutrino flux with relativistic energy there is a reasonable increase of the efficiency of the energy transfer from the neutrino flux to the electromagnetic radiation by the $SLe_\nu$ mechanism. The proposed radiation process is applied to an astrophysical environment with characteristics peculiar to supernovae. It is shown that a reasonable portion of energy of the neutrino flux can be transferred by the $SLe_\nu$ to gamma-rays .

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 A new mechanism of electromagnetic radiation by electrons under the influence of a dense neutrino flux, termed "the spin light of electron" in neutrino flux ($SLe_\nu$), is considered. contribution 1.00 0.72 0.10 asserted 0.94
s1 It is shown that in the case when electrons are moving against the neutrino flux with relativistic energy there is a reasonable increase of the efficiency of the energy transfer from the neutrino flux to the electromagnetic radiation by the $SLe_\nu$ mechanism. result 1.00 0.89 0.37 asserted 0.96
s2 The proposed radiation process is applied to an astrophysical environment with characteristics peculiar to supernovae. contribution 0.87 0.74 0.06 asserted 0.95
s3 It is shown that a reasonable portion of energy of the neutrino flux can be transferred by the $SLe_\nu$ to gamma-rays . result 0.97 0.87 0.52 asserted 0.93

What kind of paper the classifier reports this is: theoretical result 0.99 · evidence from proof or derivation 0.96.

What was examined, and what was not

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  • 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
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  • T body sentences
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  • 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

A new mechanism of electromagnetic radiation by electrons under the influence of a dense neutrino flux, termed "the spin light of electron" in neutrino flux ($SLe_\nu$), is considered. It is shown that in the case when electrons are moving against the neutrino flux with relativistic energy there is a reasonable increase of the efficiency of the energy transfer from the neutrino flux to the electromagnetic radiation by the $SLe_\nu$ mechanism. The proposed radiation process is applied to an astrophysical environment with characteristics peculiar to supernovae. It is shown that a reasonable portion of energy of the neutrino flux can be transferred by the $SLe_\nu$ to gamma-rays .

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