Topological eternal hilltop inflation and the swampland criteria
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Publication:5069156
DOI10.1088/1475-7516/2020/06/015zbMath1492.83100arXiv1912.00749OpenAlexW3104631747MaRDI QIDQ5069156
Publication date: 8 April 2022
Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1912.00749
inflationmonopolesdomain wallscosmic stringscosmology with extra dimensionsstring theory and cosmology
Black holes (83C57) String and superstring theories in gravitational theory (83E30) Geometrodynamics and the holographic principle (83E05) Kaluza-Klein and other higher-dimensional theories (83E15) Surgery obstructions, Wall groups (57R67) Mono-, di- and multipole moments (EM and other), gyromagnetic relations (81V60)
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Cites Work
- Unnamed Item
- Quantum corrections and the de Sitter swampland conjecture
- On the geometry of the string landscape and the swampland
- Non-conventional cosmology from a brane universe
- Cardassian expansion: a model in which the universe is flat, matter dominated, and accelerating
- Non-supersymmetric AdS and the swampland
- On the de Sitter swampland criterion
- Trans-Planckian censorship and the swampland
- The web of swampland conjectures and the TCC bound
- Stochastic eternal inflation is in the swampland
- A new type of isotropic cosmological models without singularity
- dS vacua and the swampland
- The quantum swampland
- de Sitter vacua in string theory
- Flux compactification
- Inflationary Cosmology with Quantum Gravitational Effects and Swampland Conjectures*
- Topology of cosmic domains and strings
- Large Mass Hierarchy from a Small Extra Dimension
- An Alternative to Compactification
- Cosmological Expansion in the Presence of an Extra Dimension
- Conditions for (no) eternal inflation
- Eternal inflation in swampy landscapes
- Helical phase inflation and its observational constraints
- Inflationary universe: A possible solution to the horizon and flatness problems
- The string swampland constraints require multi-field inflation
- Minimal gauge inflation and the refined Swampland conjecture
- Quantization of four-form fluxes and dynamical neutralization of the cosmological constant
- Cosmology of one extra dimension with localized gravity
- The Landscape, the Swampland and the Era of Precision Cosmology
- de Sitter Extrema and the Swampland
- Quantum Breaking Bound on de Sitter and Swampland
- New Constraints on Classical de Sitter: Flirting with the Swampland
- The Swampland: Introduction and Review
- Pixelated Dark Energy
- A Note on Inflation and the Swampland
- F‐theory and Dark Energy