Cosmological constraints on string scale and coupling arising from tachyonic instability
arXiv:hep-th/0502185 · doi:10.1088/1126-6708/2005/08/084
Abstract
We demonstrate that string motivated inflation ending via tachyonic instability leaves a detectable imprint on the cosmic microwave background (CMB) radiation by virtue of the excitation of non-Gaussian gravitational fluctuations. The present WMAP bound on non-Gaussianity is shown to constrain the string scale by for string coupling , hence improving the existing bounds. If tachyon fluctuations during inflation are not negligible, we find the stringent constraint for . This case may soon be ruled out by the forthcoming CMB non-Gaussinianity bounds.
12 pages, 2 figures, typo corrected, discussion and references added
References in corpus (33)
- de Sitter Vacua in String Theory
- Towards Inflation in String Theory
- Non-Gaussianity from Inflation: Theory and Observations
- Brane Inflation
- First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Tests of Gaussianity
- Second-Order Cosmological Perturbations from Inflation
- Cosmic String Production Towards the End of Brane Inflation
- Field Theory of Tachyon Matter
- The Inflationary Brane-Antibrane Universe
- Dynamics of Symmetry Breaking and Tachyonic Preheating
- Assisted inflation via tachyon condensation
- Racetrack Inflation
- D3/D7 Inflationary Model and M-theory
- On Exact Tachyon Potential in Open String Field Theory
- Inflation from D-\bar{D} brane annihilation
- Brane Interaction as the Origin of Inflation
- Inflationary Scenarios from Branes at Angles
- Observational Constraints on Cosmic String Production During Brane Inflation
- Remarks on Tachyon Condensation in Superstring Field Theory
- String Theory and Hybrid Inflation/Acceleration
- Non-Gaussianity from Preheating
- An Inflationary Model in String Theory
- Non-Gaussianity from Instant and Tachyonic Preheating
- Multiple Inflation, Cosmic String Networks and the String Landscape
- Recombination of Intersecting D-Branes and Cosmological Inflation
- Non-Gaussian perturbations in hybrid inflation
- Search for Cosmic Strings in CMB Anisotropies
- Overproduction of cosmic superstrings
- Inflation in warped geometries
- Accelerated expansion and the Goldstone ghost
- Braneworld inflation
- Long time scales and eternal black holes
- Non-Gaussianity in braneworld and tachyon inflation
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- Very Large Primordial Non-Gaussianity from multi-field: Application to Massless Preheating
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- Supersymmetric Thermalization and Quasi-Thermal Universe: Consequences for Gravitinos and Leptogenesis
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- Combined local and equilateral non-Gaussianities from multifield DBI inflation
- On the evolution of tachyonic perturbations at super-Hubble scales
- Reheating in supersymmetric high scale inflation
- Contribution of the hybrid inflation waterfall to the primordial curvature perturbation
- Exciting gauge field and gravitons in a brane-anti-brane annihilation
- Brane Annihilations during Inflation
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- The Origin of the Large-Scale Structure in the Universe: Theoretical and Statistical Aspects
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