Axions of Evil
arXiv:1703.00453 · doi:10.1103/PhysRevD.98.061301
Abstract
We provide a systematic framework for theories of multiple axions. We discover a novel type of "alignment" that renders even very complex theories analytically tractable. Theories with about 100 axions and random parameters have an exponential number of meta-stable vacua and accommodate a diverse range of inflationary observables. Very light fields can serve as dark matter with the correct abundance. Tunneling from a minimum with large vacuum energy can occur via a thin-wall instanton and be followed by a sufficient period of slow-roll inflation that ends in a vacuum containing axion dark matter and a cosmological constant with a value consistent with observation. Hence, this model can reproduce many macroscopic features of our universe without tuned parameters.
arXiv comment5 pages, 2 figures
References in corpus (49)
- Axion Cosmology
- String Axiverse
- Cold and Fuzzy Dark Matter
- Ultralight scalars as cosmological dark matter
- Axions In String Theory
- The String Landscape, Black Holes and Gravity as the Weakest Force
- Quantization of Four-form Fluxes and Dynamical Neutralization of the Cosmological Constant
- A new approach to the evolution of cosmological perturbations on large scales
- Gravity Waves and Linear Inflation from Axion Monodromy
- Quasi-Single Field Inflation and Non-Gaussianities
- Completing Natural Inflation
- N-flation
- Assisted inflation
- A Natural Framework for Chaotic Inflation
- Observational Consequences of a Landscape
- Scalar perturbations during multiple-field slow-roll inflation
- Naturalness and the Weak Gravity Conjecture
- An Ignoble Approach to Large Field Inflation
- Transplanckian axions !?
- Sharpening the Weak Gravity Conjecture with Dimensional Reduction
- Euclidean Wormholes in String Theory
- Planckian Axions and the Weak Gravity Conjecture
- Is There A String Theory Landscape
- Trapped Inflation
- Weak Gravity Strongly Constrains Large-Field Axion Inflation
- Quantum Creation of an Open Inflationary Universe
- Productive Interactions: heavy particles and non-Gaussianity
- A Toy Model for Open Inflation
- On Axionic Field Ranges, Loopholes and the Weak Gravity Conjecture
- The Weak Gravity Conjecture and Effective Field Theory
- Natural and Multi-Natural Inflation in Axion Landscape
- Multi-Natural Inflation in Supergravity and BICEP2
- Multi-Natural Inflation in Supergravity
- A New Angle on Chaotic Inflation
- Planck-Suppressed Operators
- Planckian Axions in String Theory
- Universality and the circular law for sparse random matrices
- Unwinding Inflation
- Axion Landscape and Natural Inflation
- MultiModeCode: An efficient numerical solver for multifield inflation
- What is the Magnetic Weak Gravity Conjecture for Axions?
- On Gaussian Random Supergravity
- Systematics of Axion Inflation in Calabi-Yau Hypersurfaces
- Systematics of Aligned Axions
- Vacuum statistics and stability in axionic landscapes
- A Tale of Two Timescales: Mixing, Mass Generation, and Phase Transitions in the Early Universe
- Inflation Expels Runaways
- Kaluza-Klein Towers in the Early Universe: Phase Transitions, Relic Abundances, and Applications to Axion Cosmology
- Axionic Band Structure of the Cosmological Constant
Cited by in corpus (12)
- Euclidean wormholes, baby universes, and their impact on particle physics and cosmology
- Superradiance in String Theory
- A Systematic Approach to Kähler Moduli Stabilisation
- An Ultralight Axion in Supersymmetry and Strings and Cosmology at Small Scales
- Friendship in the Axiverse: Late-time direct and astrophysical signatures of early-time nonlinear axion dynamics
- Crunching Away the Cosmological Constant Problem: Dynamical Selection of a Small
- Axion Landscape Cosmology
- Axion Hilltops, Kahler Modulus Quintessence and the Swampland Criteria
- Constraining Ultralight Axions with Galaxy Surveys
- Improved Halo Model Calibrations for Mixed Dark Matter Models of Ultralight Axions
- A Quantal Theory of Restoration of Strong CP Symmetry
- Axion scales and couplings with Stückelberg mixing