Two-Field Quintessential Higgs model and the Swampland
arXiv:2406.15790 · doi:10.1007/s40995-025-01777-2
Abstract
We study a two-field model where a quintessence field with an exponential potential is coupled to the Higgs field. It is claimed that this model is consistent with the proposed Swampland conjecture. We check this claim by calculating its inflationary observables. Although, these observables are in good agreement with the latest CMB data, but we find an upper bound that strongly disfavors the Swampland conjecture.
10 pages, 2 figures, Received: 9 November 2024 / Accepted: 6 January 2025
References in corpus (12)
- Observation of a new particle in the search for the Standard Model Higgs boson with the ATLAS detector at the LHC
- Observation of a new boson at a mass of 125 GeV with the CMS experiment at the LHC
- The Standard Model Higgs boson as the inflaton
- On the Geometry of the String Landscape and the Swampland
- BICEP / Keck XIII: Improved Constraints on Primordial Gravitational Waves using Planck, WMAP, and BICEP/Keck Observations through the 2018 Observing Season
- The Swampland: Introduction and Review
- The Unity of Cosmological Attractors
- Non-Gaussianities in two-field inflation
- Conformal Transformations with Multiple Scalar Fields
- Palatini Quintessential Inflation
- Multi-field dark energy: cosmic acceleration on a steep potential
- Quintessential inflation and cosmological seesaw Mechanism: reheating and observational constraints