Strengthening the De Sitter swampland conjecture in warm inflation
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Publication:2225767
DOI10.1007/JHEP08(2020)127zbMath1454.83164arXiv2002.04925WikidataQ123359511 ScholiaQ123359511MaRDI QIDQ2225767
Vahid Kamali, Rudnei O. Ramos, Robert H. Brandenberger
Publication date: 10 February 2021
Published in: Journal of High Energy Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/2002.04925
Relativistic cosmology (83F05) String and superstring theories in gravitational theory (83E30) Space-time singularities, cosmic censorship, etc. (83C75) Astrophysical cosmology (85A40) Effective quantum field theories (81T12)
Related Items (7)
Gravity waves and primordial black holes in scalar warm little inflation ⋮ Swampland constraints on no-boundary quantum cosmology ⋮ Multi-field cold and warm inflation and the de Sitter swampland conjectures ⋮ Seeding the vacuum with entropy: the Chaplygin-like vacuum hypothesis ⋮ On the occurrence of finite-time singularities in swampland-related quintessence dark energy models ⋮ Towards a reliable effective field theory of inflation ⋮ Defying eternal inflation in warm inflation with a negative running
Cites Work
- The importance of being warm (during inflation)
- Chaos and complementarity in de Sitter space
- On the geometry of the string landscape and the swampland
- A covariant entropy conjecture
- Inflation in the warm and cold regimes
- WARM INFLATION MODEL BUILDING
- Identifying universality in warm inflation
- Minimal warm inflation
- String gases and the swampland
- The Swampland: Introduction and Review
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