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.
arXiv comment10 pages, 2 figures, Received: 9 November 2024 / Accepted: 6 January 2025
References in corpus (42)
- Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
- Measurements of Omega and Lambda from 42 High-Redshift Supernovae
- 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
- Quintessence, Cosmic Coincidence, and the Cosmological Constant
- The Standard Model Higgs boson as the inflaton
- Towards the Theory of Reheating After Inflation
- Exponential potentials and cosmological scaling solutions
- 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
- Distance and de Sitter Conjectures on the Swampland
- Quintessence: A Review
- Quintessential inflation
- How long before the end of inflation were observable perturbations produced?
- On the Cosmological Implications of the String Swampland
- The Unity of Cosmological Attractors
- First CMB Constraints on the Inflationary Reheating Temperature
- A universal attractor for inflation at strong coupling
- Primordial Spectral Indices from Generalized Einstein Theories
- Non-Gaussianities in two-field inflation
- The landscape, the swampland and the era of precision cosmology
- The string swampland constraints require multi-field inflation
- Conformal Transformations with Multiple Scalar Fields
- Cosmological perturbations from multi-field inflation in generalized Einstein theories
- De Sitter vs Quintessence in String Theory
- Dark Energy in the Swampland
- The dS swampland conjecture and the Higgs potential
- Dark energy, -attractors, and large-scale structure surveys
- Quintessential Inflation with -attractors
- Calculations of Inflaton Decays and Reheating: with Applications to No-Scale Inflation Models
- Spectral Running and Non-Gaussianity from Slow-Roll Inflation in Generalised Two--Field Models
- Do We Live in the Swampland?
- Quintessence Saves Higgs Instability
- CMB and reheating constraints to α-attractor inflationary models
- Slow-roll Inflation for Generalized Two-Field Lagrangians
- Dark Energy and the Fate of the Universe
- Palatini Quintessential Inflation
- Multi-field dark energy: cosmic acceleration on a steep potential
- Quintessential inflation and cosmological seesaw Mechanism: reheating and observational constraints
- A Non-minimally Coupled Potential for Inflation and Dark Energy after Planck 2015: A Comprehensive Study
- Two-field inflation with non-minimal coupling