Do we live in the swampland?

DOI10.1007/JHEP12(2018)032zbMath1405.83014arXiv1809.00478OpenAlexW3101753449WikidataQ128747264 ScholiaQ128747264MaRDI QIDQ1712303

Masahito Yamazaki, Tsutomu T. Yanagida, Hitoshi Murayama

Publication date: 21 January 2019

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

Full work available at URL: https://arxiv.org/abs/1809.00478

zbMATH Keywords

superstring vacuacompactification and string models

Mathematics Subject Classification ID

String and superstring theories in gravitational theory (83E30) Supersymmetric field theories in quantum mechanics (81T60) Quantization of the gravitational field (83C45) Symmetry breaking in quantum theory (81R40)

Related Items

Multi-field inflation in high-slope potentials ⋮ Eternal inflation in swampy landscapes ⋮ Finite temperature effects in modular cosmology ⋮ On the weak gravity conjecture in string theory with broken supersymmetry ⋮ Heterotic de Sitter beyond modular symmetry ⋮ The Asymptotic dS Swampland Conjecture ‐ a Simplified Derivation and a Potential Loophole ⋮ Further Refining the de Sitter Swampland Conjecture ⋮ Pixelated Dark Energy ⋮ Hidden sectors in string theory: kinetic mixings, fifth forces and quintessence ⋮ Scaling limits of ds vacua and the swampland ⋮ Weakly coupled de Sitter vacua with fluxes and the swampland ⋮ A holographic derivation of the weak gravity conjecture ⋮ Two-field cosmological $\alpha$-attractors with Noether symmetry ⋮ F‐theory and Dark Energy ⋮ On the occurrence of finite-time singularities in swampland-related quintessence dark energy models ⋮ On inflation scenarios and dark energy in a scaled gravity ⋮ Reconstruction of quintessence field for the THDE with swampland correspondence in f(R,T) gravity ⋮ Racetrack potentials and the de Sitter swampland conjectures ⋮ Compact objects and the swampland ⋮ Cosmology of linear Higgs-sigma models with conformal invariance ⋮ A strong scalar weak gravity conjecture and some implications ⋮ Dark energy beyond quintessence: constraints from the swampland ⋮ Dark energy and the refined De Sitter conjecture ⋮ Modular symmetries and the swampland conjectures ⋮ Leaving the Swampland: non-geometric fluxes and the distance conjecture ⋮ Hyperbolic field space and swampland conjecture for DBI scalar ⋮ Conditions for (no) eternal inflation ⋮ On primordial black holes from rapid turns in two-field models

Cites Work

• Unnamed Item
• Monodromy inflation in SUSY QCD
• Dynamical breaking of supersymmetry
• Inflationary constraints on type IIA string theory
• Quantum corrections and the de Sitter swampland conjecture
• On the geometry of the string landscape and the swampland
• Ising model and \(N=2\) supersymmetric theories
• Proof of the weak gravity conjecture from black hole entropy
• Supersymmetry breaking by fluxes
• Tensionless strings and the weak gravity conjecture
• The weak gravity conjecture in three dimensions
• Wormholes, emergent gauge fields, and the weak gravity conjecture
• Sharpening the weak gravity conjecture with dimensional reduction
• From 4d Yang-Mills to 2d \(\mathbb{C} {\mathbb{P}}^{N-1}\) model: IR problem and confinement at weak coupling
• Evidence for a sublattice weak gravity conjecture
• Non-supersymmetric AdS and the swampland
• Spontaneous \(CP\) breaking in QCD and the axion potential: an effective Lagrangian approach
• Infinite distances in field space and massless towers of states
• M-theory and type IIA flux compactifications
• Vacuum structure of Yang-Mills theory as a function of \(\theta\)
• Dynamical supersymmetry breaking on quantum moduli spaces
• On the de Sitter swampland criterion
• Model independent analysis of supernova data, dark energy, trans-Planckian censorship and the swampland
• Axion monodromy in a model of holographic gluodynamics
• Transplanckian axions!?
• Fencing in the swampland: quantum gravity constraints on large field inflation
• Weak gravity strongly constrains large-field axion inflation
• Quintessence: a review
• Theta Dependence in the Large<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi mathvariant="italic">N</mml:mi></mml:math>Limit of Four-Dimensional Gauge Theories
• What if string theory has no de Sitter vacua?
• Inflation and conformal invariance: the perspective from radial quantization
• The string swampland constraints require multi-field inflation
• f(R) and Brans-Dicke theories and the Swampland
• The Landscape, the Swampland and the Era of Precision Cosmology
• De Sitter vs Quintessence in String Theory