REVIEW
An Alternative to Compactification
High Energy Physics - Theory · Submitted 8 Jun 1999 · 13 references
Pith's verdict: The graviton zero mode on a single positive-tension brane in infinite AdS5 is real, the 1/(r²k²) correction checks out, and the paper's own caveats are the honest ones.
T0 · AI review
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Referee report
The paper
The paper claims
An infinite fifth dimension can still reproduce four-dimensional Newtonian and general relativistic gravity, provided the bulk is curved and a single 3-brane traps the graviton.
The reading
What carries the argument
The load-bearing object is the analogue quantum-mechanical potential $V(z) = 15k^2/[8(k|z|+1)^2] - (3k/2)$ obtained from the linearized graviton equation after the substitution $z = (e^{k|y|}-1)/k$ and a wavefunction rescaling. Its delta-function term binds a single normalizable zero mode, $k^{-1}(k|z|+1)^{-3/2}$, which is identified with the four-dimensional graviton; its long tail falls to zero at large $|z|$, so the rest of the spectrum is a continuum with no gap, and the small-argument Bessel behaviour $J_2, Y_2$ forces those continuum wavefunctions to vanish like $m^2 z^2$ at the brane. That vanishing is the mechanism that suppresses both the static force correction, giving $1/(r^2 k^2)$, and the production rate of continuum gravitons from brane processes, giving $(p/k)^2$.
Extended reading notes
Core claim
The central claim is that a 3-brane of positive tension embedded in an infinite slice of AdS$_5$, with brane tension and bulk cosmological constant tuned against each other, reproduces four-dimensional gravity to well within experimental precision despite a gapless Kaluza-Klein continuum. The argument runs through the linearized tensor fluctuation equation, which after a change of variable becomes an analogue non-relativistic Schrödinger problem with potential $V(z) = 15k^2/[8(k|z|+1)^2] - (3k/2),$ where the delta function at the brane supports exactly one normalizable bound state. That bound state is the massless four-dimensional graviton; the remaining continuum modes have wavefunctions suppressed near the brane by $m/k$, so exchange of the whole tower yields $V(r) = G_N m_1 m_2 (1 + 1/(r^2 k^2))/r$. The leading term is ordinary Newtonian gravity and the correction is negligible for $k$ of order the fundamental Planck scale, which is what the authors mean by reproducing four-dimensional gravity without a gap.
Load-bearing premise
The whole construction rests on tuning the brane tension and the bulk cosmological constant against each other so that the four-dimensional cosmological constant vanishes; the authors impose this by hand and say only that they accept the necessary fine tuning without further explanation.
Editorial extensions
If this is right
- An infinite extra dimension is compatible with all existing gravitational tests, so compactification is not required in order to hide extra dimensions from experiment.
- The four-dimensional Planck mass is fixed by the bulk curvature through $M_{Pl}^2 = M^3/k$, so the fundamental and four-dimensional gravitational scales can be comparable without any large extra-dimensional volume.
- The modulus problem for the brane separation dissolves in the infinite-radius limit: the would-be modulus is not coupled to brane matter, so no modulus mass is needed to stabilise it.
- Low-energy processes on the brane lose energy into the continuum at a rate suppressed by $(p/k)^2$, so missing-energy signals from the extra dimension are far below gravitational strength at accessible energies.
- The authors speculate that a dual description may exist in terms of a four-dimensional conformal field theory with a cutoff, in the spirit of the AdS/CFT correspondence.
Reading between the lines
- The trapping mechanism looks generic rather than tied to this exact background: any geometry whose linearized fluctuation operator has a normalizable zero mode and a potential that rises away from the brane should localise gravity the same way, which suggests a family of alternatives to compactification worth cataloguing.
- Read through an AdS/CFT lens, the $1/(r^2 k^2)$ correction to Newton's law is plausibly the leading large-$N$ correction of a dual strongly coupled theory, which would make short-distance gravity a direct probe of the dual central charge rather than merely a test of extra dimensions.
- The tuning that sets the four-dimensional cosmological constant to zero is the weakest link; if it holds only approximately, the residual cosmological constant becomes the leading observable consequence, so cosmological measurements become an indirect test of the brane-tension relation.
- The authors' own observation that five-dimensional couplings grow as $z^{3/2}/M_{Pl}$ implies an energy-dependent cutoff set by how far into the bulk a process can reach; a natural extension is to ask whether that same blue-shift argument bounds the maximum energy of any process describable without a ultraviolet completion.
Original abstract
Conventional wisdom states that Newton's force law implies only four non-compact dimensions. We demonstrate that this is not necessarily true in the presence of a non-factorizable background geometry. The specific example we study is a single 3-brane embedded in five dimensions. We show that even without a gap in the Kaluza-Klein spectrum, four-dimensional Newtonian and general relativistic gravity is reproduced to more than adequate precision.
The compiled record
The paper's own sentences, arranged, kept beside the review and separate from it. 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.
The abstract, sentence by sentence
Conventional wisdom states that Newton's force law implies only four non-compact dimensions. We demonstrate that this is not necessarily true in the presence of a non-factorizable background geometry. The specific example we study is a single 3-brane embedded in five dimensions. We show that even without a gap in the Kaluza-Klein spectrum, four-dimensional Newtonian and general relativistic gravity is reproduced to more than adequate precision.
background contribution method result interpretation main claim
| # | sentence | role | the authors' own work | states the main conclusion | strength |
|---|---|---|---|---|---|
| s0 | Conventional wisdom states that Newton's force law implies only four non-compact dimensions. | background 1.00 | 0.03 | 0.03 | asserted 0.96 |
| s1 | We demonstrate that this is not necessarily true in the presence of a non-factorizable background geometry. | contribution 0.55 | 0.90 | 0.65 | asserted 0.91 |
| s2 | The specific example we study is a single 3-brane embedded in five dimensions. | contribution 0.64 | 0.50 | 0.05 | asserted 0.96 |
| s3 | We show that even without a gap in the Kaluza-Klein spectrum, four-dimensional Newtonian and general relativistic gravity is reproduced to more than adequate precision. | result 1.00 | 0.94 | 0.70 | asserted 1.00 |
What was examined, and what was not
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References
How later papers used it
1,185 later papers cite it
7 later papers by other authors are listed below: 1 built on it, 4 used its method or tool and 2 compared their own results with it.
Builds on it 1 of 11 papers with this label
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Generalized this paper's Randall-Sundrum solution with one brane to the case of broken Poincare invariance and bulk anisotropic perfect fluid.
Brane world models with bulk perfect fluid and broken 4D Poincare invariance (2017) · 1.00 · paraphrased: the licence does not allow quoting
Uses its method or tool 4 of 16 papers with this label
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Brought its equations of motion into the form of a 1d Schrodinger equation as in this paper, following another work explicitly.
Towards Axion Monodromy Inflation with Warped KK-Modes (2015) · 0.86 · paraphrased: the licence does not allow quoting
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Followed this paper to introduce regulator (negative tension) branes at ±z_r and take the limit z_r→∞ at the end.
Breaking the $Z_2$ symmetry of the Randall-Sundrum scenario and the fate of the massive modes (2010) · 0.94 · paraphrased: the licence does not allow quoting
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Applied a cutting and pasting procedure analogous to that used in this paper's Randall-Sundrum scenario to yield new brane world models from the solitons.
New AdS solitons and brane worlds with compact extra-dimensions (2010) · 0.80 · paraphrased: the licence does not allow quoting
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Used this paper's Randall-Sundrum construction to couple mSYM to dynamical gravity.
The holographic dual of a Hawking pair has a wormhole (2014) · 0.92 · paraphrased: the licence does not allow quoting
Compares with it 2 of 55 papers with this label
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Concluded that with the addition of the source brane at t=0 its five-dimensional space has become very similar to this paper's Randall-Sundrum one.
Scale-dependent Planck mass and Higgs VEV from holography and functional renormalization (2011) · 0.98 · paraphrased: the licence does not allow quoting
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Mentioned that the ETW brane it found in this way is similar to those of the Randall-Sundrum model discussed in this paper.
Quotient-AdS/BCFT: Holographic Boundary CFT$_2$ on AdS$_3$ Quotients (2020) · 0.98 · paraphrased: the licence does not allow quoting
How the literature uses it
1,103 arXiv papers cite this in 1,723 sentences
Papers citing it · 692 sentences without a confident label
Contests it 1 paper
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The attempt [ref] to explain the difference between the Planck scale and the electroweak scale is interesting but suffers the same shortage as was shown in [ref] .
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Builds on it 11 papers
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In this paper we extend our previous analysis [ref] to a wider class of warped backgrounds including Randall–Sundrum model [ref] and Karch–Randall model [ref] .
Emergent Supersymmetry in Warped Backgrounds · Introduction · 1.00
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In this section, we will redo and expand the works of Randall, Sundrum, and Karch [ref] , simplifying the computations and generalizing them to any number of spacetime dimensions, while dealing simultaneously with all three maximally symmetric brane geometries.
Gravity in Enhanced Brane-World Models · Gravity on KRS Brane-Worlds · 1.00
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The absolute value sign around $r$ gives a $δ$-function source/brane at $r=0$ exactly like the one brane models of [ref] .
Anti-de-Sitter Island-Universes from 5D Standing Waves · Metric and Einstein's equations · 0.81
Uses its method or tool 16 papers
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Inserting a $4d$ plane wave ansatz $ϕ(x,y)=e^ipx χ(y)$ with $p^2=-m^2$ the equations of motion take the form [equation] which can be brought into the form of a 1d Schrödinger equation [ref] (we follow explicitly [ref] ) [equation] with $z≡e^-ky$, $χ=z^3/2f$, $E=m^2/k^2$ and potential [equation] where $z_IR=1$ and $z_UV=e^-k L$.
Towards Axion Monodromy Inflation with Warped KK-Modes · KK-Reduction on the Effective 5d-Throat and the 4d Action · 0.86
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The lower dimensional effective semi-classical theory for the bulk configuration described above may be obtained through a combination of a partial Randall-Sundrum reduction [ref] and the usual AdS/BCFT duality [ref] .
Defect extremal surfaces for entanglement negativity · Effective description and boundary island formula · 0.85
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For the reduction region, we employ Randall-Sundrum reduction [ref] and obtain a gravity theory on the brane, coupled with CFT matter.
Partial Reduction and Cosmology at Defect Brane · Island formula for cosmology at the end of the world · 0.96
Uses its data or values 2 papers
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A lower bound on $ρ_RS^1/4 ≳1.3$ TeV, or equivalently, $M_5 ≳1.1 ×10^8$ GeV was obtained in Ref. [ref] from the precision measurements of the gravitational law in sub-millimeter range.
Braneworld Cosmological Effect on Freeze-in Dark Matter Density and Lifetime Frontier · RS cosmology · 0.82
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From particle physics, recent report by CMS collaboration suggests that the size for one “large" extra dimension based on the Randall-Sundrum scenario [ref] is of order $∼10^-4$ fm [ref] .
Bound orbits around charged black strings · Conclusion · 0.84
Compares with it 50 papers
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In the SW1 case for the parameter range $1>ν>2$ the spectrum is quite similar to the RS1 model [ref] , with some particularities.
Studies on Generalized Warped Five-Dimensional Models · Applications of soft-wall models · 0.95
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Firstly, the cosmological mass reduction formula (cMRF) [equation] is clearly different from that obtained in a static AdS$_5$ brane-world configuration [ref] , for which [equation] Secondly, and perhaps more importantly, no parameter of the action would have to be tuned to keep $Λ_4$ positive.
De Sitter brane-world, localization of gravity, and the cosmological constant · A spatially flat universe · 1.00
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For case VO, the relative correction term $ΔU∝1/(kr)^2$ is the same as the RS model [ref] .
Fundamental energy scale of the thick brane in mimetic gravity · Conclusion · 0.96
Cites it as support 6 papers
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Requiring that the integral of the cosmic energy density (with respect to the scalar field) has a constant Schwarzian derivative led naturally to a modified Friedmann equation that arises generically in the Randall-Sundrum and Shtanov-Sahni braneworld models [ref] and loop quantum cosmology scenarios [ref] .
Cosmology and the Korteweg-de Vries Equation · Discussion · 0.96
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As noticed in [ref] , a non-compact extra dimension can nevertheless lead to localized gravity.
Self-tuning of the cosmological constant in brane-worlds with $P(X,\phi)$ · Brane-world model with a bulk k-essence scalar · 0.96
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The reason is that we know that the gravitational force of attraction in the RS model is stronger than in GR on scales less than $ℓ$ [ref] .
Scalar perturbations in Randall-Sundrum braneworld cosmology · Introduction · 0.97
Cites it as background 754 papers
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The first simple, systematic and direct approach to decoupling gravitational sources in general relativity (GR) was recently developed [ref] from the so-called Minimal Geometric Deformation (MGD) approach (henceforth MGD-decoupling), an idea originally proposed [ref] in the context of the Randall-Sundrum brane-world [ref] and extended to investigate new black hole solutions [ref] (For some earlier works, see for instance Refs. [ref] , and for some recent applications Refs. [ref] ).
A simple method to generate exact physically acceptable anisotropic solutions in general relativity · Introduction · 0.80
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The $AdS$/CFT correspondence [ref] adapted to the Randall-Sundrum braneworld model RS2 [ref] predicts that classical bulk physics in $AdS_5$ is dual to a particular cut-off CFT (namely $N=4$ SU($N$) SYM in the planar limit) coupled to gravity living on the brane.
Quantum Effects in Black Holes from the Schwarzschild Black String? · Introduction · 0.84
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Randall and Sundrum [ref] proposed a five-dimension AdS space (AdS$_5$) brane-world model where the extra dimension has an infinite size and a negative bulk cosmological constant $$.
Brane-world extra dimensions in light of GW170817 · Introduction · 0.98
Discussion
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