Warm Little Inflaton becomes dark energy
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Publication:2187219
DOI10.1016/j.physletb.2019.134984zbMath1434.83174arXiv1906.11835OpenAlexW2955349610WikidataQ127217154 ScholiaQ127217154MaRDI QIDQ2187219
Publication date: 2 June 2020
Published in: Physics Letters. B (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1906.11835
Related Items (6)
Cosmological viability of a double field unified model from warm inflation ⋮ Hubble-induced phase transitions: Walls are not forever ⋮ Warm dark energy ⋮ Towards a reliable effective field theory of inflation ⋮ Warm inflation, neutrinos and dark matter: a minimal extension of the standard model ⋮ Hidden inflaton dark matter
Cites Work
- The importance of being warm (during inflation)
- Quintessential inflation from a variable cosmological constant in a 5D vacuum
- Isocurvature fluctuations in tracker quintessence models
- Asymptotic behavior of homogeneous cosmological models in the presence of a positive cosmological constant
- Quintessence: a review
- WARM INFLATION MODEL BUILDING
- A SIMPLE QUINTESSENTIAL INFLATION MODEL
- Reconstructing a model of quintessential inflation
- Reheating after quintessential inflation and gravitational waves
- Bulk viscous quintessential inflation
- Unification of inflation and dark energyà laquintessential inflation
- Electroweak symmetry breaking from dimensional deconstruction
- Inflation, braneworlds and quintessence
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