A Field Range Bound for General Single-Field Inflation
arXiv:1111.3040 · doi:10.1088/1475-7516/2012/05/017
Abstract
We explore the consequences of a detection of primordial tensor fluctuations for general single-field models of inflation. Using the effective theory of inflation, we propose a generalization of the Lyth bound. Our bound applies to all single-field models with two-derivative kinetic terms for the scalar fluctuations and is always stronger than the corresponding bound for slow-roll models. This shows that non-trivial dynamics can't evade the Lyth bound. We also present a weaker, but completely universal bound that holds whenever the Null Energy Condition (NEC) is satisfied at horizon crossing.
16 pages
References in corpus (18)
- The Effective Field Theory of Inflation
- Causality, Analyticity and an IR Obstruction to UV Completion
- Observational Signatures and Non-Gaussianities of General Single Field Inflation
- Monodromy in the CMB: Gravity Waves and String Inflation
- Starting the Universe: Stable Violation of the Null Energy Condition and Non-standard Cosmologies
- Signatures of Supersymmetry from the Early Universe
- Particle production during inflation and gravitational waves detectable by ground-based interferometers
- CMBPol Mission Concept Study: Probing Inflation with CMB Polarization
- Galileon inflation
- A Microscopic Limit on Gravitational Waves from D-brane Inflation
- Trapped Inflation
- Dissipative effects in the Effective Field Theory of Inflation
- New Sources of Gravitational Waves during Inflation
- Observable gravitational waves from inflation with small field excursions
- Gravitational Wave Constraints on DBI Inflation
- Supergravity for Effective Theories
- Gravitational Wave Constraints on Multi-Brane Inflation
- Inflating with Baryons
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- String Inflation After Planck 2013
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- On Squeezed Limits in Single-Field Inflation - Part I
- An accurate bound on tensor-to-scalar ratio and the scale of inflation
- No-go for the formation of heavy mass Primordial Black Holes in Single Field Inflation
- Towards a measurement of the spectral runnings
- Effective field theory of weakly coupled inflationary models
- Primordial backgrounds of relic gravitons
- B-modes and the Nature of Inflation
- The Lyth Bound of Inflation with a Tilt
- Large-Field Inflation and the Cosmological Collider
- BICEP2 implications for single-field slow-roll inflation revisited
- The Effective Theory of Shift-Symmetric Cosmologies
- Evading Lyth bound in models of quintessential inflation
- Cosmic inflation in a landscape of heavy-fields
- Supersymmetric DBI inflation
- CMB from EFT
- Bounds on non-adiabatic evolution in single-field inflation
- Alleviating the tension at low multipole through Axion Monodromy
- Constraints on Primordial Magnetic Fields from Inflation
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- On the integration of fields and quanta in time dependent backgrounds
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- Effective Field Theory of Multi-Field Inflation a la Weinberg
- On degenerate models of cosmic inflation
- Testing Split Supersymmetry with Inflation
- Natural Inflation from Near Alignment in Heterotic String Theory
- Non-Canonical Inflation in Supergravity
- Quantum Gravity Effect in Torsion Driven Inflation and CP violation
- The Inflated Chern-Simons Number in Spectator Chromo-Natural Inflation
- Clearing the Brush: The Last Stand of Solo Small Field Inflation
- Large tensor mode, field range bound and consistency in generalized G-inflation
- Lyth Bound, eternal inflation and future cosmological missions
- Large Tensor-to-Scalar Ratio in Small-Field Inflation
- Generically large nongaussianity in small multifield inflation
- B-modes and the sound speed of primordial fluctuations
- Studying G-axion Inflation model in light of PLANCK
- Inflationary field excursion in broad classes of scalar field models
- The Upper Bound on the Tensor-to-Scalar Ratio Consistent with Quantum Gravity
- Inflation with vector fields revisited: heavy entropy perturbations and primordial black holes
- A Tail of Eternal Inflation