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Genericity of Cosmic Strings Formation in SUSY GUTs

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J. Rocher, R. Jeannerot, M. Sakellariadou

High Energy Physics - Phenomenology · Submitted 15 Jun 2004

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

The authors' main claim We conclude that all acceptable symmetry breaking schemes produce cosmic strings after the last inflationary phase.

how it is stated · asserted 1.00 read the record →

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arXiv IDhep-ph/0406161 (version 1)
Pith ID7JSYFMKS, Pith's permanent record of this paper and its review
CitationJ. Rocher, M. Sakellariadou, R. Jeannerot. "Genericity of Cosmic Strings Formation in SUSY GUTs." arXiv:hep-ph/0406161 (2004). https://pith.science/paper/7JSYFMKS
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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, 4,146 input tokens, $0.0002 reported.

What the abstract itself states, as probabilities: claims first 0.03 · states limitation 0.15 · human participants 0.01 · controlled comparison 0.02 · randomized assignment 0.01 · states quantitative result 0.20 · 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; .

The idea of GUT implies that the universe went through a series of phase transitions during which topological defects are expected to form. We investigate here the genericity of cosmic strings formation in realistic SUSY GUTs models. We conclude that all acceptable symmetry breaking schemes produce cosmic strings after the last inflationary phase. Generically, as they form at the end of inflation, they have a mass of order of the GUT scale. Since cosmological data coming from CMB measurements do not show evidence for such strings, they constrain GUT scale physics.

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 idea of GUT implies that the universe went through a series of phase transitions during which topological defects are expected to form. background 1.00 0.04 0.02 hedged possibility 0.67
s1 We investigate here the genericity of cosmic strings formation in realistic SUSY GUTs models. contribution 1.00 0.84 0.03 unclear 0.82
s2 We conclude that all acceptable symmetry breaking schemes produce cosmic strings after the last inflationary phase. result 1.00 0.89 0.93 asserted 1.00
s3 Generically, as they form at the end of inflation, they have a mass of order of the GUT scale. result 0.94 0.68 0.08 asserted 0.96
s4 Since cosmological data coming from CMB measurements do not show evidence for such strings, they constrain GUT scale physics. interpretation 0.98 0.12 0.10 asserted 0.98

What kind of paper the classifier reports this is: theoretical result 1.00 · evidence from argument 0.60.

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

The idea of GUT implies that the universe went through a series of phase transitions during which topological defects are expected to form. We investigate here the genericity of cosmic strings formation in realistic SUSY GUTs models. We conclude that all acceptable symmetry breaking schemes produce cosmic strings after the last inflationary phase. Generically, as they form at the end of inflation, they have a mass of order of the GUT scale. Since cosmological data coming from CMB measurements do not show evidence for such strings, they constrain GUT scale physics.

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Found among the papers closest to this one by title and main claim. Pith's classifier compared each pair's main results and a second model family confirmed the relation; checked against two further families, shown conflicts agreed 118 times in 120 and shown same results 218 times in 239. The quoted sentence is the other paper's main claim.

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