Warm Inflation with Barrow Holographic Dark Energy
arXiv:2406.02639 · doi:10.1016/j.nuclphysb.2025.116933
Abstract
In this work, we study the warm inflation mechanism in the presence of the Barrow holographic dark energy model. Warm inflation differs from other forms of inflation primarily in that it assumes that radiation and inflaton fields exist and interact throughout the inflationary process. After the warming process, energy moves from the inflaton to the radiation as a result of the interaction, keeping the cosmos warm. Here we have set up the warm inflationary mechanism using Barrow holographic dark energy as the driving agent. Warm inflation has been explored in a highly dissipative regime, and interesting results have been obtained. It is seen that the Barrow holographic dark energy can successfully drive a warm inflationary scenario in the early universe. Finally, the model was compared with the observational data, and compliance was found.
21 pages, 10 figures, 6 tables. This version matches the published version in Nucl. Phys. B
References in corpus (18)
- On the Geometry of the String Landscape and the Swampland
- The Area of a Rough Black Hole
- Infrared cut-off proposal for the Holographic density
- Barrow holographic dark energy
- Recent developments in warm inflation
- The warm inflationary universe
- Barrow holographic dark energy with Granda-Oliveros cut-off
- The warm inflation story
- Statefinder hierarchy model for the Barrow holographic dark energy
- Pleasant behavior of swampland conjectures in the face of specific inflationary models
- Quantum phase transitions in two-dimensional superconductors: a review on recent experimental progress
- Intermediate inflation driven by DBI scalar field
- Swampland Conjecture and Inflation Model from Brane Perspective
- Generalized interacting Barrow Holographic Dark Energy: cosmological predictions and thermodynamic considerations
- de Sitter Swampland Conjecture in String Field Inflation
- Running and running of the running of the scalar spectral index in warm inflation
- Cosmic evolution of the logarithmic f(R) model and the dS swampland conjecture
- A new class of holographic dark energy models in LRS Bianchi Type-I