Defying eternal inflation in warm inflation with a negative running
From MaRDI portal
Publication:6497821
DOI10.1088/1475-7516/2024/02/006WikidataQ128813985 ScholiaQ128813985MaRDI QIDQ6497821
Katherine Freese, Gabriele Montefalcone, Gustavo S. Vicente, Rudnei O. Ramos
Publication date: 6 May 2024
Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)
Cites Work
- The importance of being warm (during inflation)
- Strengthening the De Sitter swampland conjecture in warm inflation
- Towards a reliable effective field theory of inflation
- A new type of isotropic cosmological models without singularity
- WARM INFLATION MODEL BUILDING
- THE GLOBAL STRUCTURE OF THE INFLATIONARY UNIVERSE
- Minimal warm inflation
- Inflationary universe: A possible solution to the horizon and flatness problems
This page was built for publication: Defying eternal inflation in warm inflation with a negative running