Mass Hierarchies and Dynamical Field Range
arXiv:1806.01874 · doi:10.1103/PhysRevD.98.066012
Abstract
Several swampland conjectures suggest that there is a critical field range beyond which the effective field theory (EFT) description breaks down in quantum gravity. In applications of these conjectures, however, the field range of interest is the field space distance traced by the physical trajectory that solves the equations of motion. We refer to this field space distance as the dynamical field range. We show that in the absence of a mass hierarchy between the light and heavy fields, the trajectory of the light field does not, in general, follow a geodesic in field space. Then, stabilizing the heavy fields at the minimum of their potential does not accurately describe the dynamics of the light field in general. A mass hierarchy can delay the breakdown of the EFT, and extend the effective field range. We illustrate these subtleties of multi-field dynamics with axions in Type II string compactifications.
arXiv comment8 pages, 3 figures
References in corpus (37)
- de Sitter Vacua in String Theory
- The String Landscape, Black Holes and Gravity as the Weakest Force
- On the Geometry of the String Landscape and the Swampland
- Systematics of Moduli Stabilisation in Calabi-Yau Flux Compactifications
- Monodromy in the CMB: Gravity Waves and String Inflation
- Gravity Waves and Linear Inflation from Axion Monodromy
- What would we learn by detecting a gravitational wave signal in the cosmic microwave background anisotropy?
- Infinite Distances in Field Space and Massless Towers of States
- Scalar perturbations during multiple-field slow-roll inflation
- Cosmology with Nilpotent Superfields
- Super-Planckian Spatial Field Variations and Quantum Gravity
- The Gelaton Scenario: Equilateral non-Gaussianity from multi-field dynamics
- Emergence and the Swampland Conjectures
- F-term Axion Monodromy Inflation
- Simple exercises to flatten your potential
- Backreacted Axion Field Ranges in String Theory
- Mass hierarchies and non-decoupling in multi-scalar field dynamics
- D7-Brane Chaotic Inflation
- Heavy fields, reduced speeds of sound and decoupling during inflation
- Towards Universal Axion Inflation and Reheating in String Theory
- The Swampland Conjecture and F-term Axion Monodromy Inflation
- Effective Field Theory and Decoupling in Multi-field Inflation: An Illustrative Case Study
- The Refined Swampland Distance Conjecture in Calabi-Yau Moduli Spaces
- Influence of heavy modes on perturbations in multiple field inflation
- On Axionic Field Ranges, Loopholes and the Weak Gravity Conjecture
- A Flux-Scaling Scenario for High-Scale Moduli Stabilization in String Theory
- Backreaction Issues in Axion Monodromy and Minkowski 4-forms
- A Geometrical Upper Bound on the Inflaton Range
- Challenges for Large-Field Inflation and Moduli Stabilization
- The Challenge of Realizing F-term Axion Monodromy Inflation in String Theory
- Higgs-otic Inflation and String Theory
- N-flation with Hierarchically Light Axions in String Compactifications
- Higgs-otic Inflation and Moduli Stabilization
- Flux Flattening in Axion Monodromy Inflation
- Large field inflation from D-branes
- Challenges for D-brane large-field inflation with stabilizer fields
- Effect of massive fields on inflation
Cited by in corpus (33)
- Distance and de Sitter Conjectures on the Swampland
- The string swampland constraints require multi-field inflation
- Infinite Distance Networks in Field Space and Charge Orbits
- A note on Inflation and the Swampland
- Instantons and infinite distances
- The Swampland Distance Conjecture and Towers of Tensionless Branes
- A Holographic Derivation of the Weak Gravity Conjecture
- Rescuing Single Field Inflation from the Swampland
- Instanton Corrections and Emergent Strings
- Clockwork Axions in Cosmology: Is Chromonatural Inflation Chrononatural?
- Tackling the SDC in AdS with CFTs
- Modular Symmetries and the Swampland Conjectures
- Weakly Coupled de Sitter Vacua with Fluxes and the Swampland
- A Strong Scalar Weak Gravity Conjecture and Some Implications
- The trans-Planckian censorship conjecture from the swampland distance conjecture
- Infinite Distances and the Axion Weak Gravity Conjecture
- The Fundamental Need for a SM Higgs and the Weak Gravity Conjecture
- A Tip for Landscape Riders: Multi-Field Inflation Can Fulfill the Swampland Distance Conjecture
- Relating the scalar weak gravity conjecture and the swampland distance conjecture for an accelerating universe
- Large Field Ranges from Aligned and Misaligned Winding
- de Sitter Space as a Glauber-Sudarshan State
- de Sitter swampland bound in the Dirac-Born-Infeld inflation model
- Role of trans-Planckian modes in cosmology
- Rigid nongeometric orientifolds and the swampland
- -dualizing the de-Sitter no-go scenarios
- A stringy perspective on the coincidence problem
- On stable type IIA de-Sitter vacua with geometric flux
- Seeking de-Sitter Vacua in the String Landscape
- The Swampland Spectrum Conjecture in Inflation
- Helical phase inflation and its observational constraints
- Hitchhiker's Guide to the Swampland: The Cosmologist's Handbook to the string-theoretical Swampland Programme
- Enhancement of axion decay constants in type IIA theory?
- Systematic exploration of the non-geometric flux landscape