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Spontaneous Current Generation in Cosmic Strings

High Energy Physics - Phenomenology · Submitted 14 Dec 1993

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

The authors' main claim It is shown that in models including the standard electroweak theory and for some particular values of the underlying parameters, electric currents can be spontaneously generated in cosmic strings, without the need of any external field (e.g., electric or magnetic) as is required in most models.

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arXiv IDhep-ph/9312280 (version 1)
Pith IDMBJTVVFV, Pith's permanent record of this paper and its review
CitationPatrick Peter. "Spontaneous Current Generation in Cosmic Strings." arXiv:hep-ph/9312280 (1993). https://pith.science/paper/MBJTVVFV
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What the abstract itself states, as probabilities: claims first 0.07 · states limitation 0.52 · human participants 0.01 · controlled comparison 0.07 · randomized assignment 0.01 · states quantitative result 0.17 · compares with prior results 0.86 · mentions code or data availability 0.01.

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

It is shown that in models including the standard electroweak theory and for some particular values of the underlying parameters, electric currents can be spontaneously generated in cosmic strings, without the need of any external field (e.g., electric or magnetic) as is required in most models. This mechanism is then shown to break spontaneously the Lorentz invariance along the initially Goto-Nambu string. The characteristic time needed for the current to build up is estimated and found to lowest order to depend only on the mass of the intermediate $W$ vector boson and the fine structure constant.

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What the classifier reports for each sentence. The number is the probability it gave the label.
#sentencerolethe authors' own workstates the main conclusionstrength
s0 It is shown that in models including the standard electroweak theory and for some particular values of the underlying parameters, electric currents can be spontaneously generated in cosmic strings, without the need of any external field (e.g., electric or magnetic) as is required in most models. result 0.92 0.89 0.86 asserted 0.98
s1 This mechanism is then shown to break spontaneously the Lorentz invariance along the initially Goto-Nambu string. result 0.91 0.90 0.20 asserted 1.00
s2 The characteristic time needed for the current to build up is estimated and found to lowest order to depend only on the mass of the intermediate $W$ vector boson and the fine structure constant. result 1.00 0.94 0.09 asserted 1.00

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

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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

It is shown that in models including the standard electroweak theory and for some particular values of the underlying parameters, electric currents can be spontaneously generated in cosmic strings, without the need of any external field (e.g., electric or magnetic) as is required in most models. This mechanism is then shown to break spontaneously the Lorentz invariance along the initially Goto-Nambu string. The characteristic time needed for the current to build up is estimated and found to lowest order to depend only on the mass of the intermediate $W$ vector boson and the fine structure constant.

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7 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 · 3 sentences without a confident label

Cites it as background 4 papers
  • Of particular interest are superconducting cosmic strings, which initially were suggested in Ref. [ref] , since they are the expected outcome of various high energy scenarios [ref] ; it was even argued that when the low-energy limit of the string-forming model contains the standard SU(3)$×$SU(2)$×$U(1) model, currents must be produced, at least at the electroweak scale, but also at any intermediate scale structured in a similar way [ref] .

    Charge-velocity-dependent one-scale linear model · Introduction · 0.87

  • In particular, this requires a comprehensive understanding of all possible additional degrees of freedom and structures, such as long-lasting currents [ref] , often dubbed superconducting—a nomenclature we prefer not to use here as it often refers to long-range electromagnetic effects—and Y-junctions [ref] , each of which can introduce deviations from the conventional cosmic string evolution paradigm [ref] .

    Cosmic Microwave Background Signatures from Current-carrying Cosmic Strings · Introduction · 0.97

  • This mechanism is closely analogous to that underlying the Ginzburg–Landau description of superconductivity [ref] , which is the origin of the name “superconducting cosmic strings.” Superconducting strings and their physical properties have been studied extensively in the literature [ref] .

    Gravitational Waves from Superconducting Cosmic Strings · Introduction · 0.92

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