Nonminimally-coupled warm Higgs inflation: metric vs. Palatini formulations
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Publication:6095223
DOI10.1016/J.NUCLPHYSB.2023.116289arXiv2303.00572OpenAlexW4384206996MaRDI QIDQ6095223
Davood Momeni, Punsiri Dam-O, Thammarong Eadkhong, Phongpichit Channuie
Publication date: 7 September 2023
Published in: Nuclear Physics. B (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/2303.00572
Relativistic cosmology (83F05) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05)
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Implications of Palatini gravity for inflation and beyond ⋮ Cosmological constraints of Palatini \(f(\mathcal{R})\) gravity
Cites Work
- The importance of being warm (during inflation)
- Tracing the high energy theory of gravity: an introduction to Palatini inflation
- A new type of isotropic cosmological models without singularity
- WARM INFLATION MODEL BUILDING
- Minimal warm inflation with complete medium response
- Reheating in models with non-minimal coupling in metric and Palatini formalisms
- On UV-completion of Palatini-Higgs inflation
- Inflationary universe: A possible solution to the horizon and flatness problems
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