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Deflection of Highly Relativistic Particles in a Gravitational Field

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Paper breakdownThe authors' claims, conditions and measurements, as JSON Signed receiptProof this review has not been altered
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C. Barrabes, P. A. Hogan

General Relativity and Quantum Cosmology · Submitted 4 Nov 2003

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

The authors' main claim A novel approach to the calculation of the deflection of highly relativistic test particles in gravitational fields is described.

how it is stated · asserted 0.96 read the record →

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arXiv IDgr-qc/0311010 (version 2)
Pith IDBY6FBVGM, Pith's permanent record of this paper and its review
CitationC. Barrabes, P. A. Hogan. "Deflection of Highly Relativistic Particles in a Gravitational Field." arXiv:gr-qc/0311010 (2003). https://pith.science/paper/BY6FBVGM
Claim paper

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, 3,536 input tokens, $0.0001 reported.

What the abstract itself states, as probabilities: claims first 0.16 · states limitation 0.05 · human participants 0.01 · controlled comparison 0.02 · randomized assignment 0.01 · states quantitative result 0.04 · compares with prior results 0.09 · mentions code or data availability 0.02.

The abstract, sentence by sentence

arXiv listing abstract v2. Results and the main claim are underlined; .

A novel approach to the calculation of the deflection of highly relativistic test particles in gravitational fields is described. We make use of the light-like boosts of the gravitational fields of the sources. Examples are given of the deflection of highly relativistic particles in the Schwarzschild and Kerr gravitational fields, in the field of a static, axially symmetric, multipole source and in the field of a cosmic string. The deflection of spinning particles is also discussed.

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 novel approach to the calculation of the deflection of highly relativistic test particles in gravitational fields is described. contribution 1.00 0.77 0.11 asserted 0.96
s1 We make use of the light-like boosts of the gravitational fields of the sources. method 0.99 0.89 0.07 asserted 0.98
s2 Examples are given of the deflection of highly relativistic particles in the Schwarzschild and Kerr gravitational fields, in the field of a static, axially symmetric, multipole source and in the field of a cosmic string. contribution 0.85 0.81 0.11 asserted 0.98
s3 The deflection of spinning particles is also discussed. contribution 1.00 0.70 0.07 asserted 0.92

What kind of paper the classifier reports this is: method or tool 0.98 · evidence from proof or derivation 1.00.

What was examined, and what was not

sources read
  • arXiv listing abstract v2
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

A novel approach to the calculation of the deflection of highly relativistic test particles in gravitational fields is described. We make use of the light-like boosts of the gravitational fields of the sources. Examples are given of the deflection of highly relativistic particles in the Schwarzschild and Kerr gravitational fields, in the field of a static, axially symmetric, multipole source and in the field of a cosmic string. The deflection of spinning particles is also discussed.

Human review

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How the literature uses it

3 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

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