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On cosmological perturbations in FRW model with scalar field and false vacuum decay

General Relativity and Quantum Cosmology · Submitted 15 Jan 2000

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

The authors' main claim In this representation, the existence of a negative mode justifying the false vacuum decay picture turns out to be manifest.

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arXiv IDgr-qc/0001041 (version 3)
Pith IDEJBRT6OS, Pith's permanent record of this paper and its review
CitationArsen Khvedelidze, George Lavrelashvili, Takahiro Tanaka. "On cosmological perturbations in FRW model with scalar field and false vacuum decay." arXiv:gr-qc/0001041 (2000). https://pith.science/paper/EJBRT6OS
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What the abstract itself states, as probabilities: claims first 0.04 · states limitation 0.28 · human participants 0.01 · controlled comparison 0.02 · randomized assignment 0.01 · states quantitative result 0.04 · compares with prior results 0.94 · mentions code or data availability 0.01.

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arXiv listing abstract v3. Results and the main claim are underlined; .

The unconstrained reduced action corresponding to the dynamics of scalar fluctuations about the Friedmann-Robertson-Walker (FRW) background is derived using Dirac's method of description of singular Lagrangian systems. The results are applied to so-called negative mode problem in description of tunneling transitions with gravity. With our special choice of physical variable, the kinetic term of the reduced action has a conventional signature for a wide class of models. In this representation, the existence of a negative mode justifying the false vacuum decay picture turns out to be manifest. We also explain how the present result becomes consistent with the previously proved ``no negative mode (supercritical supercurvature mode) theorem''.

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#sentencerolethe authors' own workstates the main conclusionstrength
s0 The unconstrained reduced action corresponding to the dynamics of scalar fluctuations about the Friedmann-Robertson-Walker (FRW) background is derived using Dirac's method of description of singular Lagrangian systems. method 0.68 0.94 0.08 asserted 1.00
s1 The results are applied to so-called negative mode problem in description of tunneling transitions with gravity. contribution 0.75 0.80 0.08 asserted 0.99
s2 With our special choice of physical variable, the kinetic term of the reduced action has a conventional signature for a wide class of models. result 0.68 0.93 0.11 asserted 1.00
s3 In this representation, the existence of a negative mode justifying the false vacuum decay picture turns out to be manifest. result 0.75 0.91 0.53 asserted 1.00
s4 We also explain how the present result becomes consistent with the previously proved ``no negative mode (supercritical supercurvature mode) theorem''. interpretation 0.83 0.76 0.15 asserted 0.67

What kind of paper the classifier reports this is: theoretical result 0.99 · 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

The unconstrained reduced action corresponding to the dynamics of scalar fluctuations about the Friedmann-Robertson-Walker (FRW) background is derived using Dirac's method of description of singular Lagrangian systems. The results are applied to so-called negative mode problem in description of tunneling transitions with gravity. With our special choice of physical variable, the kinetic term of the reduced action has a conventional signature for a wide class of models. In this representation, the existence of a negative mode justifying the false vacuum decay picture turns out to be manifest. We also explain how the present result becomes consistent with the previously proved ``no negative mode (supercritical supercurvature mode) theorem''.

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References
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17 arXiv papers cite this in 34 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 · 18 sentences without a confident label

Contests it 1 paper
Uses its method or tool 2 papers
  • Using a Hamiltonian approach following Dirac the quadratic action has the form [ref] S^(2)_H= π^2 ∫dηΦ[-d/dη (ρ^3(η)/Q_Hd/dη ) + ρ^3(η) U[φ(η),ρ(η)] ] Φ

    Aspects of the negative mode problem in quantum tunneling with gravity · A short summary of the negative mode problem · 0.92

  • In order to derive the Hamiltonian in Eq. (17) in Ref. [ref] , we have to utilize four constraints; $Π_Ψ= 0$, $A-Ψ=0$, $Π_A = 0$, and $φ' Π_Φ- H Π_Ψ+ a^2 √(γ) [ (a^2 (∂V/∂φ) + 3φ' H )Φ- (6K/κ)Ψ] = 0$.

    Negative Mode Problem of False Vacuum Decay Revisited · An example in which elimination works · 0.83

Compares with it 1 paper
Cites it as background 11 papers
  • The negative modes of the Coleman-de Luccia instanton that represents vacuum decay in de Sitter space have been studied by several authors [ref] , and there is now compelling evidence that the bounce solutions can have either one or infinitely many negative modes, depending on the potential.

    Negative modes of Coleman-de Luccia and black hole bubbles · Introduction · 0.82

  • For a real saddle in a Euclidean path integral, one can probe this by investigating whether small real perturbations of the saddle increase or decrease the action.[ One should also take proper care of issues [ref] related to the so-called conformal factor problem which makes the action for Euclidean gravity unbounded below.

    The double cone geometry is stable to brane nucleation · Brane nucleation on complex saddles · 0.87

  • Despite quite a few studies [ref] , there is no conclusive answer to this problem yet.

    Negative Mode Problem of False Vacuum Decay Revisited · Introduction · 0.91

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