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 (56)
- Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
- Measurements of Omega and Lambda from 42 High-Redshift Supernovae
- Planck 2018 results. X. Constraints on inflation
- A Model of Holographic Dark Energy
- Lectures on holographic methods for condensed matter physics
- Effective Field Theory, Black Holes, and the Cosmological Constant
- The dS/CFT Correspondence
- On the Geometry of the String Landscape and the Swampland
- Pre-Big-Bang in String Cosmology
- Interpretation of the nonextensitivity parameter in some applications of Tsallis statistics and Lévy distributions
- Logarithmic correction to the Bekenstein-Hawking entropy
- Black hole thermodynamical entropy
- Chaotic inflation on the brane
- Logarithmic Corrections to Black Hole Entropy from the Cardy Formula
- The Area of a Rough Black Hole
- Holographic Dark Energy
- Infrared cut-off proposal for the Holographic density
- Thermally Induced Density Perturbations in the Inflation Era
- Scalar perturbation spectra from warm inflation
- Wilson loops in heavy ion collisions and their calculation in AdS/CFT
- Inflation from a Tachyon Fluid?
- Barrow holographic dark energy
- Warm Inflation in the Adiabatic Regime- a Model, an Existence Proof for Inflationary Dynamics in Quantum Field Theory
- Strong Dissipative Behavior in Quantum Field Theory
- Interpolating the Stage of Exponential Expansion in the Early Universe: a possible alternative with no reheating
- Warm Little Inflaton
- Entanglement Entropy from a Holographic Viewpoint
- Perturbation Spectra in the Warm Inflationary Scenario
- Warm inflation model building
- The importance of being warm (during inflation)
- Is Warm Inflation Possible?
- Recent developments in warm inflation
- The warm inflationary universe
- Barrow holographic dark energy with Granda-Oliveros cut-off
- Interacting Entropy-Corrected Holographic Dark Energy and IR Cut-Off Length
- The warm inflation story
- Warm natural inflation
- Warming up brane-antibrane inflation
- Extended Warm Inflation
- Statefinder hierarchy model for the Barrow holographic dark energy
- Logarithmic corrected Polynomial inflation mimicking a cosmological constant
- Circumventing the eta problem in building an inflationary model in string theory
- 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
- Holographic Dark Energy from Fluid/Gravity Duality Constraint by Cosmological Observations
- Slow roll in simple non-canonical inflation
- Intermediate inflation driven by DBI scalar field
- The Interaction Structure and Cosmological Relevance of Mass Scales in String Motivated Supersymmetric Theories
- Swampland Conjecture and Inflation Model from Brane Perspective
- de Sitter Swampland Conjecture in String Field Inflation
- Generalized interacting Barrow Holographic Dark Energy: cosmological predictions and thermodynamic considerations
- 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
- 1/N Resolution to Inflationary eta-Problem
- A new class of holographic dark energy models in LRS Bianchi Type-I
- Particle production and dissipation caused by the Kaluza-Klein tower