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Inflation and The Minimal Supersymmetric Standard Model
High Energy Physics - Phenomenology · Submitted 18 Dec 2008
abstract compiled · 2026-09-23 · no language-model review
The authors' main claim We show how inflation can be realized within the Minimal Supersymmetric Standard Model (MSSM).
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The paper's own sentences, arranged. 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.
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The abstract, sentence by sentence
There is strong evidence from cosmological data that the universe underwent an epoch of superluminal expansion called inflation. A satisfactory embedding of inflation in fundamental physics has been an outstanding problem at the interface of cosmology and high energy physics. We show how inflation can be realized within the Minimal Supersymmetric Standard Model (MSSM). The inflaton candidates are two specific combinations of supersymmetric partners of quarks and leptons. MSSM inflation occurs at a low scale and generates perturbations in the range experimentally allowed by the latest data from Wilkinson Microwave Anisotropy Probe (WMAP). The parameter space for inflation is compatible with supersymmetric dark matter, and the Large Hadron Collider (LHC) is capable of discovering the inflaton candidates in the allowed regions of parameter space.
background contribution method result interpretation main claim
| # | sentence | role | the authors' own work | states the main conclusion | strength |
|---|---|---|---|---|---|
| s0 | There is strong evidence from cosmological data that the universe underwent an epoch of superluminal expansion called inflation. | background 1.00 | 0.05 | 0.02 | asserted 0.97 |
| s1 | A satisfactory embedding of inflation in fundamental physics has been an outstanding problem at the interface of cosmology and high energy physics. | gap 0.82 | 0.04 | 0.02 | asserted 1.00 |
| s2 | We show how inflation can be realized within the Minimal Supersymmetric Standard Model (MSSM). | contribution 1.00 | 0.94 | 0.73 | asserted 1.00 |
| s3 | The inflaton candidates are two specific combinations of supersymmetric partners of quarks and leptons. | contribution 0.79 | 0.80 | 0.12 | asserted 1.00 |
| s4 | MSSM inflation occurs at a low scale and generates perturbations in the range experimentally allowed by the latest data from Wilkinson Microwave Anisotropy Probe (WMAP). | result 1.00 | 0.85 | 0.21 | asserted 1.00 |
| s5 | The parameter space for inflation is compatible with supersymmetric dark matter, and the Large Hadron Collider (LHC) is capable of discovering the inflaton candidates in the allowed regions of parameter space. | result 0.54 | 0.80 | 0.30 | asserted 0.78 |
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The paper
Original abstract
There is strong evidence from cosmological data that the universe underwent an epoch of superluminal expansion called inflation. A satisfactory embedding of inflation in fundamental physics has been an outstanding problem at the interface of cosmology and high energy physics. We show how inflation can be realized within the Minimal Supersymmetric Standard Model (MSSM). The inflaton candidates are two specific combinations of supersymmetric partners of quarks and leptons. MSSM inflation occurs at a low scale and generates perturbations in the range experimentally allowed by the latest data from Wilkinson Microwave Anisotropy Probe (WMAP). The parameter space for inflation is compatible with supersymmetric dark matter, and the Large Hadron Collider (LHC) is capable of discovering the inflaton candidates in the allowed regions of parameter space.
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How the literature uses it
5 arXiv papers cite this in 5 sentences
Papers citing it · 4 sentences without a confident label
Cites it as background 1 paper
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In this model inflation occurs along a flat direction consisting of the supersymmetric partners of the right-handed (RH) neutrinos and left-handed (LH) leptons, and the Higgs field (for reviews on flat direction inflation, see [ref] ).
Unifying inflation and dark matter · Introduction · 0.93
What it cites · 4 sentences without a confident label
Uses data or values from 1 paper
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Eqs. ([ref],[ref],[ref]), combined with the $2 σ$ allowed region for the spectral index from 5-year WMAP data $0.934 ≤n_s ≤0.988$ [ref] , result in
Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation · Properties of MSSM inflation · 0.99
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