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Inflating baby-Skyrme branes in six dimensions

High Energy Physics - Theory · Submitted 5 Jul 2010

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

The authors' main claim Our results indicate that the perturbation equations do not admit localized solutions for certain type of perturbation.

how it is stated · hedged possibility 0.88 read the record →

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arXiv ID1007.0736 (version 1)
Pith IDSQLDYRPA, Pith's permanent record of this paper and its review
CitationNobuyuki Sawado, T\'erence Delsate, Yuta Kodama, Yves Brihaye. "Inflating baby-Skyrme branes in six dimensions." arXiv:1007.0736 (2010). https://pith.science/paper/SQLDYRPA
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Compiled by classifier-1.13-20260917 via OpenRouter, question bank abstract-p1-20260923, 2026-09-23: 1 request, 4,944 input tokens, $0.0002 reported.

What the abstract itself states, as probabilities: claims first 0.03 · states limitation 0.86 · human participants 0.01 · controlled comparison 0.02 · randomized assignment 0.01 · states quantitative result 0.15 · compares with prior results 0.06 · mentions code or data availability 0.02.

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

We consider a six dimensional brane world model, where the brane is described by a localized solution to the baby-Skyrme model extending in the extradimensions. The branes have a cosmological constant modeled by inflating four dimensional slices and we further consider a bulk cosmological constant. We construct solutions numerically and present evidences that the solutions cease to exist for large values of the brane cosmological constant in some particular case. Then we study the stability of the model by considering perturbation of the gravitational part (resp. baby skyrmion) with fixed matter fields (resp. gravitational background). Our results indicate that the perturbation equations do not admit localized solutions for certain type of perturbation. The stability analysis can be alternatively seen as leading to a particle spectrum; we give mass estimations for the baby-Skyrme perturbation and for the graviton.

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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 We consider a six dimensional brane world model, where the brane is described by a localized solution to the baby-Skyrme model extending in the extradimensions. contribution 0.59 0.42 0.03 asserted 0.97
s1 The branes have a cosmological constant modeled by inflating four dimensional slices and we further consider a bulk cosmological constant. method 0.64 0.54 0.04 asserted 0.99
s2 We construct solutions numerically and present evidences that the solutions cease to exist for large values of the brane cosmological constant in some particular case. result 0.97 0.96 0.34 hedged possibility 0.66
s3 Then we study the stability of the model by considering perturbation of the gravitational part (resp. baby skyrmion) with fixed matter fields (resp. gravitational background). method 0.80 0.92 0.06 asserted 0.89
s4 Our results indicate that the perturbation equations do not admit localized solutions for certain type of perturbation. result 1.00 0.94 0.24 hedged possibility 0.88
s5 The stability analysis can be alternatively seen as leading to a particle spectrum; we give mass estimations for the baby-Skyrme perturbation and for the graviton. interpretation 0.54 0.93 0.19 asserted 0.80

What kind of paper the classifier reports this is: simulation study 0.53 · evidence from simulation or computation 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

We consider a six dimensional brane world model, where the brane is described by a localized solution to the baby-Skyrme model extending in the extradimensions. The branes have a cosmological constant modeled by inflating four dimensional slices and we further consider a bulk cosmological constant. We construct solutions numerically and present evidences that the solutions cease to exist for large values of the brane cosmological constant in some particular case. Then we study the stability of the model by considering perturbation of the gravitational part (resp. baby skyrmion) with fixed matter fields (resp. gravitational background). Our results indicate that the perturbation equations do not admit localized solutions for certain type of perturbation. The stability analysis can be alternatively seen as leading to a particle spectrum; we give mass estimations for the baby-Skyrme perturbation and for the graviton.

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How the literature uses it

6 arXiv papers cite this in 12 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 · 7 sentences without a confident label

Cites it as background 5 papers

What it cites · 16 sentences without a confident label

Uses the method or tool of 2 papers
  • Eq.([ref]) can be rewritten in the form of a zero-eigenvalue mode Schrödinger equation for the function [equation] namely [equation] where the potential is [equation] Eq.([ref]) can be understood in the context of so called the supersymmetric quantum mechanics [ref] where the function $W(r)$ is identified as the superpotential in the SUSY QM.

    Supersymmetry and Quantum Mechanics · Stability of the Baby-skyrmions with fixed gravitational background · 0.80

  • We follow a scheme employed for the analysis of the six-dimensional Abelian vortex [ref] .

    Stability of six-dimensional hyperstring braneworlds · Stability of the Baby-skyrmions with fixed gravitational background · 1.00

Cites as background 21 papers

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