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Homogeneous magnetic fields in fully anisotropic string cosmological backgrounds

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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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Massimo Giovannini (Institute for Theoretical Physics, Lausanne University)

General Relativity and Quantum Cosmology · Submitted 30 Mar 2000

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

The authors' main claim We present new solutions of the string cosmological effective action in the presence of a homogeneous Maxwell field with pure magnetic component.

how it is stated · asserted 1.00 read the record →

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arXiv IDgr-qc/0003112 (version 1)
Pith IDDO7LCOLP, Pith's permanent record of this paper and its review
CitationLausanne University), Massimo Giovannini (Institute for Theoretical Physics. "Homogeneous magnetic fields in fully anisotropic string cosmological backgrounds." arXiv:gr-qc/0003112 (2000). https://pith.science/paper/DO7LCOLP
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, 2,878 input tokens, $0.0001 reported.

What the abstract itself states, as probabilities: claims first 0.06 · states limitation 0.46 · human participants 0.01 · controlled comparison 0.01 · 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; .

We present new solutions of the string cosmological effective action in the presence of a homogeneous Maxwell field with pure magnetic component. Exact solutions are derived in the case of space-independent dilaton and vanishing torsion background. In our examples the four dimensional metric is either of Bianchi-type III and VI$_{-1}$ or Kantowski-Sachs.

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 We present new solutions of the string cosmological effective action in the presence of a homogeneous Maxwell field with pure magnetic component. contribution 0.99 0.95 0.40 asserted 1.00
s1 Exact solutions are derived in the case of space-independent dilaton and vanishing torsion background. contribution 0.33 0.95 0.13 asserted 1.00
s2 In our examples the four dimensional metric is either of Bianchi-type III and VI$_{-1}$ or Kantowski-Sachs. result 0.96 0.88 0.14 asserted 0.99

What kind of paper the classifier reports this is: theoretical result 1.00 · evidence from proof or derivation 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
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

We present new solutions of the string cosmological effective action in the presence of a homogeneous Maxwell field with pure magnetic component. Exact solutions are derived in the case of space-independent dilaton and vanishing torsion background. In our examples the four dimensional metric is either of Bianchi-type III and VI$_{-1}$ or Kantowski-Sachs.

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