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Inflationary attractor property of phantoms

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Xin-He Meng, Peng Wang (Nankai U.)

High Energy Physics - Phenomenology · Submitted 6 Nov 2003

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

The authors' main claim In this paper we will show that the inflationary attractor property still holds for canonical and Born-Infeld phantom fields in the standard Friedmann-Robertson-Walker cosmology, however, it does not hold for canonical and Born-Infeld phantom fields in the Randall -Sundrum II cosmology.

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arXiv IDhep-ph/0311070 (version 1)
Pith IDVRZJTR3Z, Pith's permanent record of this paper and its review
CitationPeng Wang (Nankai U.), Xin-he Meng. "Inflationary attractor property of phantoms." arXiv:hep-ph/0311070 (2003). https://pith.science/paper/VRZJTR3Z
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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, 3,592 input tokens, $0.0002 reported.

What the abstract itself states, as probabilities: claims first 0.04 · states limitation 0.71 · human participants 0.01 · controlled comparison 0.21 · randomized assignment 0.01 · states quantitative result 0.03 · compares with prior results 0.35 · mentions code or data availability 0.02.

The abstract, sentence by sentence

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

There are some motivations to consider inflation driven by a phantom field. Before entering into some specific models and perform data fitting, it is important first investigating some general features that any viable inflation model should hold. The inflationary attractor property is an important one of those features. In this paper we will show that the inflationary attractor property still holds for canonical and Born-Infeld phantom fields in the standard Friedmann-Robertson-Walker cosmology, however, it does not hold for canonical and Born-Infeld phantom fields in the Randall -Sundrum II cosmology.

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 There are some motivations to consider inflation driven by a phantom field. background 1.00 0.05 0.02 hedged possibility 0.54
s1 Before entering into some specific models and perform data fitting, it is important first investigating some general features that any viable inflation model should hold. background 0.91 0.10 0.02 asserted 0.92
s2 The inflationary attractor property is an important one of those features. background 1.00 0.06 0.03 asserted 1.00
s3 In this paper we will show that the inflationary attractor property still holds for canonical and Born-Infeld phantom fields in the standard Friedmann-Robertson-Walker cosmology, however, it does not hold for canonical and Born-Infeld phantom fields in the Randall -Sundrum II cosmology. result 0.97 0.93 0.96 asserted 1.00

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

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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

There are some motivations to consider inflation driven by a phantom field. Before entering into some specific models and perform data fitting, it is important first investigating some general features that any viable inflation model should hold. The inflationary attractor property is an important one of those features. In this paper we will show that the inflationary attractor property still holds for canonical and Born-Infeld phantom fields in the standard Friedmann-Robertson-Walker cosmology, however, it does not hold for canonical and Born-Infeld phantom fields in the Randall -Sundrum II cosmology.

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References
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2 arXiv papers cite this in 2 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

Cites it as background 2 papers
  • Attracting many attentions, the interesting fluid has been widely discussed recent years [ref] , and Ref. [ref] investigated the thermodynamics on phantom dark energy dominant universe.

    Thermodynamics of Spinor Quintom · GSL in a System Filled with Spinor Quintom Matter · 0.92

  • In spite of the fact that the theory of phantom fields encounter the problem of stability, which one could try to bypass by assuming them to be effective fields [ref] ,gib, it is nevertheless interesting to study their cosmological implications and there are many relevant studies recently on phantom energy [ref] .

    Quintom Cosmology with General Potentials · Introduction · 0.81

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