On Exclusion of Positive Cosmological Constant
arXiv:1806.10877 · doi:10.1002/prop.201800092
Abstract
Some time ago we have suggested that positive vacuum energy exhibits a finite quantum break time, which can be a signal that a positive cosmological constant is inconsistent. From the requirement that Universe never undergoes through quantum breaking, we have derived an absolute lower bound on the speed of variation of positive vacuum energy. The same suggestion about exclusion of positive cosmological constant was made recently. We show that the new bound represents a particular string theoretic version of the old bound, which is more general. In this light, we show that the existing window still provides a large room for the inflationary and dark energy model building. In particular, the inflationary models with gravitational strength interactions, are protected against fast quantum breaking.
2 pages
Cited by in corpus (85)
- The Swampland: Introduction and Review
- Trans-Planckian Censorship and the Swampland
- The dS swampland conjecture and the Higgs potential
- Warm inflation as a way out of the swampland
- The zoo plot meets the swampland: mutual (in)consistency of single-field inflation, string conjectures, and cosmological data
- Cosmological window onto the string axiverse and the supersymmetry breaking scale
- Quintessential interpretation of the evolving dark energy in light of DESI
- A note on Inflation and the Swampland
- Swampland Variations on a Theme by KKLT
- Bounds on Slow Roll at the Boundary of the Landscape
- Quintessence Saves Higgs Instability
- The Swampland, Quintessence and the Vacuum Energy
- F-theory and Dark Energy
- The Gravitino and the Swampland
- The quantum swampland
- Pixelated Dark Energy
- Modular Symmetries and the Swampland Conjectures
- Weakly Coupled de Sitter Vacua with Fluxes and the Swampland
- Quantum Log-Corrections to Swampland Conjectures
- A Strong Scalar Weak Gravity Conjecture and Some Implications
- de Sitter in non-supersymmetric string theories: no-go theorems and brane-worlds
- de Sitter Vacua in the String Landscape
- Scaling limits of dS vacua and the swampland
- Phenomenological Consequences of the Refined Swampland Conjecture
- The trans-Planckian censorship conjecture from the swampland distance conjecture
- Draining the Swampland
- Warm dark energy
- Infinite Black Hole Entropies at Infinite Distances and Tower of States
- Do supernovae indicate an accelerating universe?
- Hyperbolic field space and swampland conjecture for DBI scalar
- The Dark Dimension in a Warped Throat
- Universe's Primordial Quantum Memories
- On the weak gravity conjecture in string theory with broken supersymmetry
- Multi-field Inflation in High-Slope Potentials
- Swampland, Gradient Flow and Infinite Distance
- Scale-invariant alternatives to general relativity. III. The inflation--dark-energy connection
- de Sitter Space as a Glauber-Sudarshan State: II
- Trans-Planckian censorship and single-field inflaton potential
- Eternal Inflation, Entropy Bounds and the Swampland
- Strongly Coupled Quintessence
- Revisiting the Scalar Weak Gravity Conjecture
- de Sitter Space as a Glauber-Sudarshan State
- Four-dimensional de Sitter space is a Glauber-Sudarshan state in string theory
- Reheating Constraints on Inflaton, Dark Matter: Swampland Conjecture
- Role of trans-Planckian modes in cosmology
- Combining cosmological and local bounds on bimetric theory
- Racetrack Potentials and the de Sitter Swampland Conjectures
- A refined trans-Planckian censorship conjecture
- Crisis on Infinite Earths: Short-lived de Sitter Vacua in the String Theory Landscape
- Fundamental Forces and Scalar Field Dynamics in the Early Universe
- Constraints on dark energy models from the Horndeski theory
- Is Trans-Planckian Censorship a Swampland Conjecture?
- Thermodynamics and decay of de Sitter vacuum
- The Black Hole Entropy Distance Conjecture and Black Hole Evaporation
- Wyman's "other" scalar field solution, Sultana's generalization, and their Brans-Dicke and relatives
- Inflection-Point Inflation with Axion Dark Matter in light of Trans-Planckian Censorship Conjecture
- Resurgence of a de Sitter Glauber-Sudarshan State: Nodal Diagrams and Borel Resummation
- High-quality axions in a class of chiral gauge theories
- Contracting Cosmologies and the Swampland
- Dark Energy, Dark Matter and Baryogenesis from a Model of a Complex Axion Field
- Thermal, Trapped and Chromo-Natural Inflation in light of the Swampland Criteria and the Trans-Planckian Censorship Conjecture
- De Sitter Quantum Breaking, Swampland Conjectures and Thermal Strings
- Unitarity Problems for an Effective Field Theory Description of Early Universe Cosmology
- On Sphaleron Heating in the Presence of Fermions
- Swampland Constraints on No-Boundary Quantum Cosmology
- Consistency of Cubic Galileon Cosmology: Model-Independent Bounds from Background Expansion and Perturbative Analyses
- Holographic Naturalness
- Notes on the Quantum Corrections of Swampland and Trans-Planckian Censorship Conjecture
- Swampland Conjectures for an Almost Topological Gravity Theory
- Limitations of an Effective Field Theory Treatment of Early Universe Cosmology
- dS Spaces and Brane Worlds in Exotic String Theories
- Is de Sitter space always excluded in semiclassical f(R) gravity?
- A Note on the Swampland Distance Conjecture
- Hidden Sectors in String Theory: Kinetic Mixings, Fifth Forces and Quintessence
- What if string theory has a de Sitter excited state?
- Bulk/boundary Modular Quintessence and DESI
- Quantum cosmology, eternal inflation, and swampland conjectures
- Breathing Comoving Hubble: Initial Condition and Eternity in view of the trans-Planckian Censorship Conjecture
- Hitchhiker's Guide to the Swampland: The Cosmologist's Handbook to the string-theoretical Swampland Programme
- Model of the quintessence axion
- Runaway potentials and a massive goldstino
- On the F-term problem and quintessence supersymmetry breaking
- Gravitational Wave Signatures from Warm Dark Energy
- Higgs potential near-criticality from a de Sitter swampland-like condition
- Breaking Free from the Swampland of Impossible Universes through the DESI Portal