REVIEW
Building a Better Racetrack
High Energy Physics - Theory · Submitted 30 Apr 2004 · 94 references
Pith's verdict: The durable contribution is the geometry — explicit fourfolds, the h^{1,1}=1 no-go, and the Fano classification — not the headline stabilization claim, which rests on a W0 the paper's own flux count doesn't deliver in a controlled regime.
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Referee report
The paper
The paper claims
Explicit Calabi-Yau orientifold compactifications are exhibited in which D3-instanton and gaugino-condensation effects stabilize every Kähler modulus, together with a no-go argument that rules out the one-modulus case.
The reading
Extended reading notes
Core claim
There exist type IIB orientifold compactifications on Calabi-Yau threefolds in which nonperturbative D3-instanton and gaugino-condensation contributions to the superpotential stabilize every Kähler modulus at positive radius. The paper exhibits explicit examples on the Fano bases F11 and F18 and on the elliptic fibration over IP^2, gives their toric data and triple intersection numbers, and solves D_i W = 0 numerically to find tachyon-free minima (sections 5 and 6).
Load-bearing premise
That flux vacua with the exponentially small W0 the Kähler stabilization requires actually exist in these same models. Section 6.1 sets W0 = 10^-30 by hand for F18 and F11, while the paper's own flux counting in section 5.1 (eq. 5.17) gives N_vac ~ 10^-100 in the controlled large complex structure region; the authors write that only by lowering the cutoff to y_i > 0.075 does the expected number become of order 1. The two halves of the construction are therefore demonstrated in disjoint regimes.
Original abstract
We find IIb compactifications on Calabi-Yau orientifolds in which all Kahler moduli are stabilized, along lines suggested by Kachru, Kallosh, Linde and Trivedi.
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
We find IIb compactifications on Calabi-Yau orientifolds in which all Kahler moduli are stabilized, along lines suggested by Kachru, Kallosh, Linde and Trivedi.
background contribution method result interpretation main claim
| # | sentence | role | the authors' own work | states the main conclusion | strength |
|---|---|---|---|---|---|
| s0 | We find IIb compactifications on Calabi-Yau orientifolds in which all Kahler moduli are stabilized, along lines suggested by Kachru, Kallosh, Linde and Trivedi. | result 0.72 | 0.91 | 0.78 | asserted 1.00 |
What was examined, and what was not
- arXiv listing abstract v3
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Figures
Figures reproduced from arXiv:hep-th/0404257 by the authors.
References
How later papers used it
113 later papers cite it
3 later papers by other authors are listed below: 2 used its method or tool and 1 used its data or values.
Uses its method or tool 2 of 8 papers with this label
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Used the same algorithms as this paper to generate as small as possible values for the entries of f and h, aiming for a D3 tadpole below a chosen maximum.
Finding all flux vacua in an explicit example (2012) · 0.99 · paraphrased: the licence does not allow quoting
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Applied the strategy suggested in this paper to find stationary points.
Building an explicit de Sitter (2012) · 0.99 · paraphrased: the licence does not allow quoting
Uses its data or values 1 of 5 papers with this label
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Used this paper's value of about O(10^506) vacua for IIB on CP_1,1,1,6,9.
Exacerbating the cosmological constant problem with interacting dark energy (2016) · 0.97 · paraphrased: the licence does not allow quoting
How the literature uses it
113 arXiv papers cite this in 178 sentences
Papers citing it · 112 sentences without a confident label
Uses its method or tool 8 papers
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A mechanism to achieve this was suggested and applied in [ref] .
Explicit de Sitter Flux Vacua for Global String Models with Chiral Matter · Reducing the complex structure moduli by discrete symmetries · 0.90
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The basic idea is to fix points in moduli space together with a subset of flux quanta, and fix the remaining fluxes through the ISD condition [ref] or alternatively [ref] [ref] .
Deep observations of the Type IIB flux landscape · Bounding the flux landscape · 0.85
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To find stationary points we apply the strategy suggested in [ref] :[A detailed analysis of the flux solution space will be presented in [ref] .
Building an explicit de Sitter · Complex structure moduli · 0.99
Uses its data or values 5 papers
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For example, the two-Kähler model with the orientifold of $P^4_[1,1,1,6,9]$ studied in [ref] has $n=2$, $α= 1/9√(2)$ and $λ_2=1$.
Preheating After Modular Inflation · Large Volume Compactification · 0.95
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N_vac ≈{[ O(10^506) IIB on ℂℙ_1,1,1,6,9 [ref] ,; O(10^272,000) F-theory on M_max [ref] . ] .
Exacerbating the cosmological constant problem with interacting dark energy · Introduction · 0.97
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[ref] was estimated in [ref] to be be $1/1296$, using the $Γ$ symmetry of the moduli space such that [equation] Since paramotopy allows us to find all solutions for a given flux configuration we can not only check the $L$ dependence of eq.
Finding all flux vacua in an explicit example · Distribution of parameters · 0.90
Compares with it 2 papers
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First of all, in [ref] the methods for finding flux vacua with $W_0 ≪1$ were less powerful, and the smallest value obtained was $𝒪(10^-2)$, whereas we have found examples with $W_0$ as small as[ See [ref] for a comparison of our findings to the statistical predictions of [ref] .] $10^-95$.
Small Cosmological Constants in String Theory · Introduction · 0.99
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A similar conclusion was drawn in [ref] for the $ℱ_18$-example with $b_3=190$ and $L_*=552$.
D7-Brane Moduli Space in Axion Monodromy and Fluxbrane Inflation · Statistics of Flux Vacua at Large Complex Structure · 0.89
Cites it as support 3 papers
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[ref] generically provides a stable minimum of all 272 complex structure moduli [ref] .
Finding all flux vacua in an explicit example · Effective reduction of the moduli space · 0.96
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This is because the Kähler cone condition restricts the range of moduli space, prohibiting large decay constants [ref] ; moreover, with many cycles the cone becomes very narrow, yielding large cycle volumes $τ_i ∼(h^1,1)^p$ [ref] .
Aligned Natural Inflation in the Large Volume Scenario · Choice of internal manifold · 0.96
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However, the analysis of [ref] implies that with higher values of $h^1,2_-$ the vacua in the large complex structure limit give a lower contribution to the statistics.
On the Search for Low $W_0$ · Conclusion and discussion · 0.96
Cites it as background 40 papers
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In particular, as a simple example to the latter category, an inflation model was developed using a racetrack potential inspired by KKLT construction [ref] within the context of type IIB string theory [ref] , and later refined by an explicit construction [ref] of specific orbifolded Calabi-Yau manifold with two Kähler moduli [ref] .
Inflation in a refined racetrack · Introduction and summary · 0.83
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More specifically, what can we say about the set from the point of view of the statistical approach to string phenomenology [ref] (see [ref] for studies in various settings in this context)?
On the Search for Low $W_0$ · Introduction · 0.93
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Here the complex structure moduli and the dilaton are stabilised by three-form fluxes and the Kähler moduli by non-perturbative terms arising from D3-brane instantons and/or gaugino condensation on D7-branes (for a systematic analysis see for instance [ref] ).[In the remainder of this paper we will mainly consider D3-brane instantons.
Moduli Stabilisation versus Chirality for MSSM like Type IIB Orientifolds · Introduction · 0.90
Discussion
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