Swampland constraints on no-boundary quantum cosmology

DOI10.1007/JHEP10(2020)162zbMath1456.83121arXiv2006.03443MaRDI QIDQ2657803

Takahiro Terada, Hiroki Matsui

Publication date: 14 March 2021

Published in: Journal of High Energy Physics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/2006.03443

zbMATH Keywords

spacetime singularitiesmodels of quantum gravitysolitons monopoles and instantons

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Quantization of the gravitational field (83C45) Space-time singularities, cosmic censorship, etc. (83C75) Astrophysical cosmology (85A40)

Related Items (4)

Eternal inflation in light of Wheeler-DeWitt equation ⋮ Wave function of the universe in the presence of trans-Planckian censorship ⋮ Review of the no-boundary wave function ⋮ Slow-roll approximation in quantum cosmology

Cites Work

• Unnamed Item
• On the topology of the inflaton field in minimal supergravity models
• Cosmological attractor models and higher curvature supergravity
• Superconformal inflationary \(\alpha\)-attractors
• The entropic quasi-de Sitter instability time from the distance conjecture
• On the geometry of the string landscape and the swampland
• De Sitter space and eternity
• Backreacted axion field ranges in string theory
• Super-Planckian spatial field variations and quantum gravity
• The weak gravity conjecture and scalar fields
• On the problem of initial conditions for inflation
• Generalized pole inflation: hilltop, natural, and chaotic inflationary attractors
• Quantum gravity slows inflation
• On the de Sitter swampland criterion
• Trans-Planckian censorship and the swampland
• The web of swampland conjectures and the TCC bound
• Strengthening the De Sitter swampland conjecture in warm inflation
• A strong scalar weak gravity conjecture and some implications
• Non-singular bouncing cosmology with positive spatial curvature and flat scalar potential
• Repulsive forces and the weak gravity conjecture
• Stochastic eternal inflation is in the swampland
• \(\alpha\)-attractors: Planck, LHC and dark energy
• Cosmological \(\alpha\)-attractors and de Sitter landscape
• Pole inflation -- shift symmetry and universal corrections
• On the gauged Kähler isometry in minimal supergravity models of inflation
• The no-boundary measure in scalar–tensor gravity
• No-boundary wave function for two-field inflation
• No-Boundary Measure of the Universe
• The no-boundary measure in string theory: applications to moduli stabilization, flux compactification and cosmic landscape
• Black holes and large N species solution to the hierarchy problem
• Quantum break-time of de Sitter
• Conditions for (no) eternal inflation
• Trans-Planckian Censorship and single-field inflaton potential
• Eternal inflation in swampy landscapes
• Quantum Theory of Gravity. I. The Canonical Theory
• The string swampland constraints require multi-field inflation
• The Landscape, the Swampland and the Era of Precision Cosmology
• On Exclusion of Positive Cosmological Constant
• Quantum Breaking Bound on de Sitter and Swampland
• Further Refining the de Sitter Swampland Conjecture
• The Swampland: Introduction and Review

This page was built for publication: Swampland constraints on no-boundary quantum cosmology