Contracting Cosmologies and the Swampland
arXiv:2104.00630 · doi:10.1007/JHEP07(2021)206
Abstract
We consider the cosmology obtained using scalar fields with a negative potential energy, such as employed to obtain an Ekpyrotic phase of contraction. Applying the covariant entropy bound to the tower of states dictated by the distance conjecture, we find that the relative slope of the potential is bounded from below by a constant of the order one in Planck units. This is consistent with the requirement to obtain slow Ekpyrotic contraction. We also derive a refined condition on the potential which holds near local minima of a negative potential.
arXiv comment8 pages, 2 figures; v2: 14 pages, 2 figures; references and comments on conformal diagrams added; matches published version
References in corpus (55)
- de Sitter Vacua in String Theory
- The holographic principle
- The Ekpyrotic Universe: Colliding Branes and the Origin of the Hot Big Bang
- Exponential potentials and cosmological scaling solutions
- On the Geometry of the String Landscape and the Swampland
- The Swampland: Introduction and Review
- A Covariant Entropy Conjecture
- Distance and de Sitter Conjectures on the Swampland
- From Big Crunch to Big Bang
- On the Cosmological Implications of the String Swampland
- Large-Volume Flux Compactifications: Moduli Spectrum and D3/D7 Soft Supersymmetry Breaking
- Bounds on Slow Roll and the de Sitter Swampland
- De Sitter Space and the Swampland
- What if string theory has no de Sitter vacua?
- On the Back Reaction Problem for Gravitational Perturbations
- De Sitter Space and Eternity
- Trans-Planckian Censorship and the Swampland
- Quantum Gravity Slows Inflation
- Kasner and Mixmaster behavior in universes with equation of state w \ge 1
- Trans-Planckian Censorship and Inflationary Cosmology
- Inflationary Constraints on Type IIA String Theory
- Cosmology with positive and negative exponential potentials
- Quantum Break-Time of de Sitter
- Dark Energy in the Swampland
- Towards de Sitter from 10D
- On Exclusion of Positive Cosmological Constant
- Supersymmetry Breaking by Fluxes
- Constraining de Sitter Space in String Theory
- Duality Invariant Cosmology to all Orders in
- Quantum Breaking Bound on de Sitter and Swampland
- The String Landscape, the Swampland, and the Missing Corner
- Quantum Corrections and the de Sitter Swampland Conjecture
- Supersmoothing through Slow Contraction
- O covariant String Cosmology to all orders in
- Back Reaction of Cosmological Perturbations and the Cosmological Constant Problem
- Visible Branes with Negative Tension in Heterotic M-Theory
- de Sitter Vacua in the String Landscape
- On de Sitter String Vacua from Anti-D3-Branes in the Large Volume Scenario
- Nonsingular Ekpyrotic Cosmology with a Nearly Scale-Invariant Spectrum of Cosmological Perturbations and Gravitational Waves
- Small-Field and Scale-Free: Inflation and Ekpyrosis at their Extremes
- Ekpyrotic Cosmology with a Zero-Shear S-Brane
- Back-Reaction of Super-Hubble Cosmological Perturbations Beyond Perturbation Theory
- Reheating after S-Brane Ekpyrosis
- -Cosmology: solutions and stability analysis
- New non-perturbative de Sitter vacua in -complete cosmology
- de Sitter Space as a Glauber-Sudarshan State
- New solutions with accelerated expansion in string theory
- de Sitter, -Corrections & Duality Invariant Cosmology
- Crisis on Infinite Earths: Short-lived de Sitter Vacua in the String Theory Landscape
- Effective Theories as Truncated Trans-Series and Scale Separated Compactifications
- No-Go theorems for ekpyrosis from ten-dimensional supergravity
- Causal structures in cosmology
- String Gases and the Swampland
- de Sitter duality and logarithmic decay of dark energy
- Note on Shape Moduli Stabilization, String Gas Cosmology and the Swampland Criteria
Cited by in corpus (7)
- Swampland Constraints on Neutrino Masses
- Negative scalar potentials and the swampland: an Anti-Trans-Planckian Censorship Conjecture
- Fingerprints of a Non-Inflationary Universe from Massive Fields
- The robustness of slow contraction and the shape of the scalar field potential
- Cuscuton Bounce Beyond the Linear Regime: Bispectrum and Strong Coupling Constraints
- Limitations of an Effective Field Theory Treatment of Early Universe Cosmology
- Hitchhiker's Guide to the Swampland: The Cosmologist's Handbook to the string-theoretical Swampland Programme