Nonminimally-coupled warm Higgs inflation: Metric vs. Palatini Formulations
arXiv:2303.00572 · doi:10.1016/j.nuclphysb.2023.116289
Abstract
In this work, we study the non-minimally-coupled Higgs model in the context of warm inflation scenario on both metric and Palatini approaches. We particularly consider a dissipation parameter of the form with being a coupling parameter and focus only on the strong regime of the interaction between inflaton and radiation fluid. We compute all relevant cosmological parameters and constrain the models using the observational Planck 2018 data. We discover that the and values are consistent with the observational bounds. Having used the observational data, we constrain a relation between and for the non-minimally-coupled warm Higgs inflation in both metric and Palatini cases. To produce and in agreement with observation, we find that their values are two orders of magnitude higher than those of the usual (cold) non-minimally-coupled Higgs inflation.
v2: 18 pages, many figures. version accepted for publication in Nuclear Physics Section B. arXiv admin note: text overlap with arXiv:1812.03107, arXiv:2110.03925 by other authors
References in corpus (4)
Cited by in corpus (5)
- Cosmological constraints of Palatini gravity
- First constraints on non-minimally coupled Natural and Coleman-Weinberg inflation and massive neutrino self-interactions with Planck+BICEP/Keck
- Inflation in Myrzakulov Gravity: A Comparative Study in Metric, Symmetric Teleparallel, and Weitzenböck Formalisms
- Primordial non-Gaussianity in noncanonical warm inflation with nonminimal derivative coupling
- Dynamics of potential-free warm -inflation with nonminimal derivative coupling