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Cosmological Perturbations in Brane-World Theories: Formalism
High Energy Physics - Theory · Submitted 3 May 2000
abstract compiled · 2026-09-23 · no language-model review
The authors' main claim Moreover, we show how the five-dimensional formalism can be matched to the known four-dimensional one in the limit where an effective four-dimensional description is appropriate.
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We develop a gauge-invariant formalism to describe metric perturbations in five-dimensional brane-world theories. In particular, this formalism applies to models originating from heterotic M-theory. We introduce a generalized longitudinal gauge for scalar perturbations. As an application, we discuss some aspects of the evolution of fluctuations on the brane. Moreover, we show how the five-dimensional formalism can be matched to the known four-dimensional one in the limit where an effective four-dimensional description is appropriate.
background contribution method result interpretation main claim
| # | sentence | role | the authors' own work | states the main conclusion | strength |
|---|---|---|---|---|---|
| s0 | We develop a gauge-invariant formalism to describe metric perturbations in five-dimensional brane-world theories. | contribution 0.97 | 0.96 | 0.20 | asserted 1.00 |
| s1 | In particular, this formalism applies to models originating from heterotic M-theory. | contribution 0.51 | 0.19 | 0.06 | asserted 0.98 |
| s2 | We introduce a generalized longitudinal gauge for scalar perturbations. | method 0.55 | 0.96 | 0.08 | asserted 1.00 |
| s3 | As an application, we discuss some aspects of the evolution of fluctuations on the brane. | contribution 0.96 | 0.88 | 0.09 | asserted 0.89 |
| s4 | Moreover, we show how the five-dimensional formalism can be matched to the known four-dimensional one in the limit where an effective four-dimensional description is appropriate. | contribution 0.57 | 0.93 | 0.21 | asserted 1.00 |
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The paper
Original abstract
We develop a gauge-invariant formalism to describe metric perturbations in five-dimensional brane-world theories. In particular, this formalism applies to models originating from heterotic M-theory. We introduce a generalized longitudinal gauge for scalar perturbations. As an application, we discuss some aspects of the evolution of fluctuations on the brane. Moreover, we show how the five-dimensional formalism can be matched to the known four-dimensional one in the limit where an effective four-dimensional description is appropriate.
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References
How the literature uses it
9 arXiv papers cite this in 13 sentences
Papers citing it · 5 sentences without a confident label
Uses its method or tool 3 papers
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Inspired by the similarities between perturbations in cosmological and warped backgrounds, in this section we will develop a similar formalism for warped perturbation theory, following [ref] .
A Breathing Mode for Warped Compactifications · Warped Perturbation Theory · 0.94
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In particular, we can apply the scalar-vector-tensor decomposition [ref] for the metric perturbations $δg_μν$ around the anisotropic background $g_μν= g_μν^(0)+δg_μν$: [equation] with $i$ accounting for the $x,y,$ and $z$ coordinates.
How to deal with conformal and pure scale-invariant theories of gravity in d dimensions? · The ghosts in five dimensions · 1.00
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Let us now consider the perturbations around the previous background, similarly to the formalism developed in [ref] : [equation] where [equation] Here, $i$ runs over $x,y,$ and $z$ coordinates.
Conformal and pure scale-invariant gravities in d dimensions · Perturbations · 0.98
Cites it as background 5 papers
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Cosmological perturbation theory in braneworld cosmology also has some distinct features [ref] .
Density perturbations in braneworld cosmology and primordial black holes · Introduction · 0.95
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The study of dynamics and fluctuations on warped compactifications is much more complicated than the standard Kaluza-Klein (KK) reduction on direct product spaces, and has been studied extensively by a number of authors [ref] .
A Breathing Mode for Warped Compactifications · Introduction · 0.99
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As mentioned in [ref] , the general formalism for the cosmological perturbations in brane world theories has been studied [ref] .
Analysis of inflationary models in higher-dimensional uniform inflation · Cosmological perturbation in $D+4$ dimensions · 0.84
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