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F-term uplifted racetrack inflation
High Energy Physics - Theory · Submitted 30 May 2010
abstract compiled · 2026-09-23 · no language-model review
The authors' main claim It is shown that two classes of racetrack inflation models, saddle point and inflection point ones, can be constructed in a fully supersymmetric framework with the matter field F-term as a source of supersymmetry (SUSY) breaking and uplifting.
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The abstract, sentence by sentence
It is shown that two classes of racetrack inflation models, saddle point and inflection point ones, can be constructed in a fully supersymmetric framework with the matter field F-term as a source of supersymmetry (SUSY) breaking and uplifting. Two models of F-term SUSY breaking are considered: the Polonyi model and the quantum corrected O'Raifeartaigh model. In the former case, both classes of racetrack inflation models differ significantly from the corresponding models with non-SUSY uplifting. The main difference is a quite strong dominance of the inflaton by the matter field. In addition, fine-tuning of the parameters is relaxed as compared to the original racetrack models. In the case of the racetrack inflation models coupled to the O'Raifeartaigh model, the matter field is approximately decoupled from the inflationary dynamics.
background contribution method result interpretation main claim
| # | sentence | role | the authors' own work | states the main conclusion | strength |
|---|---|---|---|---|---|
| s0 | It is shown that two classes of racetrack inflation models, saddle point and inflection point ones, can be constructed in a fully supersymmetric framework with the matter field F-term as a source of supersymmetry (SUSY) breaking and uplifting. | contribution 0.75 | 0.89 | 0.74 | asserted 0.99 |
| s1 | Two models of F-term SUSY breaking are considered: the Polonyi model and the quantum corrected O'Raifeartaigh model. | method 0.84 | 0.61 | 0.05 | asserted 0.98 |
| s2 | In the former case, both classes of racetrack inflation models differ significantly from the corresponding models with non-SUSY uplifting. | result 0.98 | 0.79 | 0.15 | asserted 1.00 |
| s3 | The main difference is a quite strong dominance of the inflaton by the matter field. | result 0.97 | 0.80 | 0.22 | asserted 1.00 |
| s4 | In addition, fine-tuning of the parameters is relaxed as compared to the original racetrack models. | result 0.94 | 0.81 | 0.13 | asserted 1.00 |
| s5 | In the case of the racetrack inflation models coupled to the O'Raifeartaigh model, the matter field is approximately decoupled from the inflationary dynamics. | result 1.00 | 0.83 | 0.09 | asserted 0.99 |
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The paper
Original abstract
It is shown that two classes of racetrack inflation models, saddle point and inflection point ones, can be constructed in a fully supersymmetric framework with the matter field F-term as a source of supersymmetry (SUSY) breaking and uplifting. Two models of F-term SUSY breaking are considered: the Polonyi model and the quantum corrected O'Raifeartaigh model. In the former case, both classes of racetrack inflation models differ significantly from the corresponding models with non-SUSY uplifting. The main difference is a quite strong dominance of the inflaton by the matter field. In addition, fine-tuning of the parameters is relaxed as compared to the original racetrack models. In the case of the racetrack inflation models coupled to the O'Raifeartaigh model, the matter field is approximately decoupled from the inflationary dynamics.
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How the literature uses it
2 arXiv papers cite this in 2 sentences
Papers citing it · 1 sentence without a confident label
Cites it as background 1 paper
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Closed string moduli inflation models include [ref] while open string moduli inflationary models include [ref] .
Time-dependent Backgrounds in String Theory and Dualities · Time-dependent Backgrounds in String Theory · 0.85
What it cites · 11 sentences without a confident label
Compares with 2 papers
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Fine-tuning of parameters is of order $10^-3$ so it is slightly weaker than in the original model [ref] in which fine-tuning is at the level of $10^-4$.
Racetrack Inflation · Racetrack inflation with Polonyi uplifting · 0.87
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However, racetrack inflation with Polonyi uplifting is significantly different from original racetrack models [ref] with non-SUSY uplifting.
Accidental Inflation in String Theory · Racetrack inflation with Polonyi uplifting · 0.99
Cites as background 4 papers
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Recent progress in moduli stabilization, due to the proposal of the KKLT mechanism [ref] , allowed for constructing viable inflationary models within the string theory.
de Sitter Vacua in String Theory · Introduction · 0.95
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In the second scenario, the real part of the volume modulus $t$ is the inflaton and inflation takes place in the vicinity of an inflection point of the potential [ref] .
Accidental Inflation in String Theory · Introduction · 0.90
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In the first of them, inflation takes place in the vicinity of a saddle point of the potential with the axion $τ$, associated with the volume modulus, being the inflaton [ref] .
Racetrack Inflation · Introduction · 0.80
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