A Note on Inflation and the Swampland
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Publication:6084548
DOI10.1002/prop.201800052arXiv1807.05445OpenAlexW2884327748WikidataQ129388393 ScholiaQ129388393MaRDI QIDQ6084548
Publication date: 6 November 2023
Published in: Fortschritte der Physik (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1807.05445
Related Items (15)
Constraints on dark energy models from the Horndeski theory ⋮ Consistency of tachyacoustic cosmology with de Sitter swampland conjectures ⋮ Multi-field inflation in high-slope potentials ⋮ Eternal inflation in swampy landscapes ⋮ Topological eternal hilltop inflation and the swampland criteria ⋮ Multi-field cold and warm inflation and the de Sitter swampland conjectures ⋮ Hidden sectors in string theory: kinetic mixings, fifth forces and quintessence ⋮ Scaling limits of ds vacua and the swampland ⋮ (Super)universal attractors and the de Sitter vacua in string landscape ⋮ Compact objects and the swampland ⋮ Inflationary Cosmology with Quantum Gravitational Effects and Swampland Conjectures* ⋮ Dark energy beyond quintessence: constraints from the swampland ⋮ Dark energy and the refined De Sitter conjecture ⋮ Hyperbolic field space and swampland conjecture for DBI scalar ⋮ f(R) and Brans-Dicke theories and the Swampland
Cites Work
- On the geometry of the string landscape and the swampland
- Infinite distances in field space and massless towers of states
- On the de Sitter swampland criterion
- What if string theory has no de Sitter vacua?
- Inflationary universe: A possible solution to the horizon and flatness problems
- The string swampland constraints require multi-field inflation
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